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  <front>
    <journal-meta><journal-id journal-id-type="publisher">NHESS</journal-id><journal-title-group>
    <journal-title>Natural Hazards and Earth System Sciences</journal-title>
    <abbrev-journal-title abbrev-type="publisher">NHESS</abbrev-journal-title><abbrev-journal-title abbrev-type="nlm-ta">Nat. Hazards Earth Syst. Sci.</abbrev-journal-title>
  </journal-title-group><issn pub-type="epub">1684-9981</issn><publisher>
    <publisher-name>Copernicus Publications</publisher-name>
    <publisher-loc>Göttingen, Germany</publisher-loc>
  </publisher></journal-meta>
    <article-meta>
      <article-id pub-id-type="doi">10.5194/nhess-22-481-2022</article-id><title-group><article-title>Automated determination of landslide locations after large trigger events: advantages and disadvantages compared to manual mapping</article-title><alt-title>Automated determination of landslide locations</alt-title>
      </title-group><?xmltex \runningtitle{Automated determination of landslide locations}?><?xmltex \runningauthor{D.~G. Milledge et al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes" rid="aff1">
          <name><surname>Milledge</surname><given-names>David G.</given-names></name>
          <email>david.milledge@newcastle.ac.uk</email>
        <ext-link>https://orcid.org/0000-0003-4077-4898</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Bellugi</surname><given-names>Dino G.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-6701-7507</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3 aff4">
          <name><surname>Watt</surname><given-names>Jack</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3 aff4">
          <name><surname>Densmore</surname><given-names>Alexander L.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0003-0629-6554</ext-link></contrib>
        <aff id="aff1"><label>1</label><institution>School of Engineering, Newcastle University, Newcastle upon Tyne, UK</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>Department of Geography, University of California, Berkeley, Berkeley, CA, USA</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>Institute of Hazard, Risk and Resilience, Durham University, Durham, UK</institution>
        </aff>
        <aff id="aff4"><label>4</label><institution>Department of Geography, Durham University, Durham, UK</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">David G. Milledge (david.milledge@newcastle.ac.uk)</corresp></author-notes><pub-date><day>16</day><month>February</month><year>2022</year></pub-date>
      
      <volume>22</volume>
      <issue>2</issue>
      <fpage>481</fpage><lpage>508</lpage>
      <history>
        <date date-type="received"><day>8</day><month>June</month><year>2021</year></date>
           <date date-type="rev-request"><day>8</day><month>July</month><year>2021</year></date>
           <date date-type="rev-recd"><day>19</day><month>October</month><year>2021</year></date>
           <date date-type="accepted"><day>23</day><month>December</month><year>2021</year></date>
      </history>
      <permissions>
        <copyright-statement>Copyright: © 2022 </copyright-statement>
        <copyright-year>2022</copyright-year>
      <license license-type="open-access"><license-p>This work is licensed under the Creative Commons Attribution 4.0 International License. To view a copy of this licence, visit <ext-link ext-link-type="uri" xlink:href="https://creativecommons.org/licenses/by/4.0/">https://creativecommons.org/licenses/by/4.0/</ext-link></license-p></license></permissions><self-uri xlink:href="https://nhess.copernicus.org/articles/.html">This article is available from https://nhess.copernicus.org/articles/.html</self-uri><self-uri xlink:href="https://nhess.copernicus.org/articles/.pdf">The full text article is available as a PDF file from https://nhess.copernicus.org/articles/.pdf</self-uri>
      <abstract><title>Abstract</title>

      <p id="d1e129">Earthquakes in mountainous areas can trigger thousands of
co-seismic landslides, causing significant damage, hampering relief efforts,
and rapidly redistributing sediment across the landscape. Efforts to
understand the controls on these landslides rely heavily on manually mapped
landslide inventories, but these are costly and time-consuming to collect,
and their reproducibility is not typically well constrained. Here we develop
a new automated landslide detection index (ALDI) algorithm based on pixel-wise
normalised difference vegetation index (NDVI) differencing of Landsat time series within Google Earth Engine
accounting for seasonality. We compare classified inventories to manually
mapped inventories from five recent earthquakes: Kashmir in 2005, Aysén in 2007,
Wenchuan in 2008, Haiti in 2010, and Gorkha in 2015. We test the ability of ALDI to
recover landslide locations (using receiver operating characteristic – ROC – curves) and landslide sizes (in terms
of landslide area–frequency statistics). We find that ALDI more skilfully
identifies landslide locations than published inventories in 10 of 14 cases
when ALDI is locally optimised and in 8 of 14 cases both when ALDI is
globally optimised and in holdback testing. These results reflect not only good
performance of the automated approach but also surprisingly poor performance
of manual mapping, which has implications both for how future
classifiers are tested and for the interpretations that are based on
these inventories. We find that manual mapping, which typically uses finer-resolution imagery, more skilfully captures the landslide area–frequency
statistics, likely due to reductions in both the censoring of individual small
landslides and amalgamation of landslide clusters relative to ALDI. We
conclude that ALDI is a viable alternative to manual mapping in terms of its
ability to identify landslide-affected locations but is less suitable for
detecting small isolated landslides or precise landslide geometry. Its fast
run time, cost-free image requirements, and near-global coverage suggest the
potential to significantly improve the coverage and quantity of landslide
inventories. Furthermore, its simplicity (pixel-wise analysis only) and
parsimony of inputs (optical imagery only) mean that considerable further
improvement should be possible.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <label>1</label><title>Introduction</title>
      <?pagebreak page482?><p id="d1e141">Landslides are important as both agents of erosion and as a dangerous hazard
(Marc et al., 2016; Froude and Petley, 2018). Large earthquakes or
rainstorms can trigger thousands of landslides, redistributing tonnes of
rock over distances of hundreds or thousands of metres within a few seconds
(Li et al., 2014; Roback et al., 2018). These landslides can cause
significant damage, hamper relief efforts, and rapidly redistribute sediment
across the landscape. Efforts to understand the drivers, behaviour, and
consequences of these landslides rely heavily on landslide inventories, in
which landslide locations are mapped either as points, pixels, or polygons,
usually associated with one or more assumed trigger events. Landslide
inventories are important because they document the extent and impact of
landslides in a region, informing disaster response and recovery (Williams
et al., 2018); they capture the distribution, properties, and (through
predictive models) drivers of landslides (Guzzetti et al., 2012; Tanyaş et
al., 2019); they can be used to train and evaluate models of landslide
susceptibility, hazard, and risk (Van Westen et al., 2006; Reichenbach et
al., 2018); and they enable geophysical flux calculations central to the
study of landscape evolution and the global carbon cycle (e.g. Hilton et
al., 2008; Marc et al., 2016; Dietrich et al., 2003).</p>
      <p id="d1e144">Polygon-based and pixel-based inventories both capture information on the
area affected by landslide movement. Polygon-based inventories have the
additional advantage that they can be analysed to yield distributions of
landslide geometry (such as area and shape), which is useful for
understanding fluxes of material (Larsen et al., 2010) or impact forces and
distinguishing scars from runout areas (Marc et al., 2018).</p>
      <p id="d1e147">Landslide inventories were traditionally generated from expensive and
time-consuming site visits (e.g. Warburton et al., 2008), severely limiting
the number of landslides that could be mapped and thus the scale of enquiry.
However, they are now increasingly collected remotely based on
interpretation of satellite or aerial imagery, which enables much larger datasets to be compiled (e.g. Li et al., 2014; Roback et al., 2018).</p>
      <p id="d1e150">Imagery provides an opportunity for rapid mapping over wide areas but is
subject to some important limitations. For optical imagery, which depends on
reflected solar energy reaching the sensor, clouds and shadows can obscure the
ground surface. Active sensors, such as radar, that operate at wavelengths
that are not reflected by cloud suffer from other issues (e.g. radar
layover and shadowing), and their images have only recently been incorporated
into operational landslide mapping approaches (e.g. Konishi and Suga, 2018;
Burrows et al., 2019; Aimaiti et al., 2019; Mondini et al., 2019). Images
may not be available for the study area over the time window of interest,
and – when they are available – they can be costly to acquire. In steep or
high-relief topography, images can suffer severe georectification errors
(Williams et al., 2018), which is particularly problematic for landslide
mapping because these are the areas of most interest. Imagery is becoming
increasingly available across a very wide range of spatial and spectral
resolutions, but there remains a trade-off between resolution and cost, with
10–30 m imagery freely available globally with a 14 d revisit time (e.g.
Sentinel-2, Landsat 8), while sub-metric resolution data (e.g. WorldView,
Pléiades) can be acquired on demand but at a cost of USD 10–10 000 per square kilometre.</p>
      <p id="d1e154">Landslides are typically identified in imagery either by automated
classification, manual mapping, or some hybrid of the two. Manual mapping,
although much faster than site visits, remains very time-consuming over
moderate to large areas (Galli et al., 2008), particularly for co-seismic
inventories, which can involve digitising 10<inline-formula><mml:math id="M1" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msup></mml:math></inline-formula> to 10<inline-formula><mml:math id="M2" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">5</mml:mn></mml:msup></mml:math></inline-formula> landslides
(e.g. Xu et al., 2014; Harp et al., 2016). It also requires a comparison of
pre- and post-event images to identify change and to avoid conflation of
landslides related to the trigger event with those occurring before or after
the event (e.g. Hovius et al., 2011; Marc et al., 2015). Automated
classification can considerably speed up this process but is complicated by
other factors, including the range of possible landslide sizes and
geometries; the non-unique signatures of landslides relative to roads,
buildings, or other features; and the difficulty of excluding pre-existing
landslides (Parker et al., 2011; Behling et al., 2014). Automated landslide
classification has been demonstrated predominantly using high-resolution
imagery and requires a high level of tuning; thus it is not necessarily
transferrable from one region or event to another. Imagery can be combined
with other sources of information (e.g. slope inclination from digital elevation models, DEMs) to
remove some false positives, where a location is incorrectly classified as a
landslide (Parker et al., 2011). This can improve classifier performance but
can also generate spurious correlation when interpreting the results (e.g.
landslide susceptibility with slope inclination). Some authors have adopted
hybrid approaches; for example, Li et al. (2014) applied manual checking to
the earlier automated mapping of Parker et al. (2011).</p>
      <p id="d1e175">As a result of these issues, our database of landslide inventories is
limited in number and biased towards the most spectacular trigger events.
This point is most easily illustrated by examining earthquake-triggered
landslide inventories, since in this case the trigger event is generally very
clearly identifiable in time, and its footprint is well defined in space. Of
the 326 earthquakes known to have triggered landslides between 1976 and
2016, only 46 have published landslide maps (Tanyaş et al., 2017). For 225
earthquakes the existence of co-seismic landslides was known from news
reports and witness testimony (Marano et al., 2010), but no reliable
quantitative or spatial landslide data are available (Tanyaş et al., 2017).
Many other earthquakes have likely triggered landslides, but these have gone
unreported because they occurred out of human view. Between 1976 and 2016
there were <inline-formula><mml:math id="M3" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">6500</mml:mn></mml:mrow></mml:math></inline-formula> earthquakes sufficiently large (<inline-formula><mml:math id="M4" display="inline"><mml:mi mathvariant="italic">&gt;</mml:mi></mml:math></inline-formula> <inline-formula><mml:math id="M5" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">w</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> 5), shallow (<inline-formula><mml:math id="M6" display="inline"><mml:mi mathvariant="italic">&lt;</mml:mi></mml:math></inline-formula> 25 km), and near to land (<inline-formula><mml:math id="M7" display="inline"><mml:mi mathvariant="italic">&lt;</mml:mi></mml:math></inline-formula> 25 km) to
trigger landslides (based on Marc et al., 2016). This suggests that the
existing set of co-seismic landslide inventories is a small subset
(<inline-formula><mml:math id="M8" display="inline"><mml:mi mathvariant="italic">&lt;</mml:mi></mml:math></inline-formula> 15 %) of those earthquakes known to have triggered landslides
and a tiny subset (<inline-formula><mml:math id="M9" display="inline"><mml:mi mathvariant="italic">&lt;</mml:mi></mml:math></inline-formula> 1 %) of those likely to have triggered
landslides.</p>
      <p id="d1e235">Extending the number of landslide inventories requires a reduction in the
cost of inventory collection, both in terms of imagery expense and mapping
time. We hypothesise that recent improvements in satellite data management
(e.g. data cubes) and computing capabilities (e.g. cloud computing) have
made it possible to collect automated landslide inventories of comparable
quality to manual mapping, at a fraction of the cost, due to reductions
in both imagery cost and mapping time. Imagery cost could be reduced by
using cheaper, lower-resolution imagery, while mapping time could be reduced
by using automated detection rather than manual mapping. However, these
savings will only represent value for<?pagebreak page483?> money if they can deliver inventories
of comparable or superior quality to manual mapping.</p>
      <p id="d1e238">Large amounts of freely available optical imagery with near-global coverage
have been generated by the Landsat and Sentinel programmes. Landsat has been
running for more than 30 years (since the Landsat 4 launch in 1982), imaging
the majority of Earth's surface at a return time of ca. 14 d and at 30 m spatial resolution through the visible and infrared bands. Landsat
received early attention as a source of imagery for manual landslide mapping
(e.g. Sauchyn and Trench, 1978; Greenbaum et al., 1995) but has since been
largely superseded by imagery with higher spatial resolution, which is often
assumed to result in more precise inventories (e.g. Parker et al., 2011; Li
et al., 2014; Roback et al., 2018). The recent HazMapper application of
Scheip and Wegmann (2021) is a notable exception and seeks to leverage the
large volume of freely available coarser-resolution imagery to provide
information on vegetation change that can be used to map a range of hazards
including landslides. It is not clear, however, whether the long time series
of coarser-resolution imagery that is now available contains as much usable
information as individual images of finer resolution.</p>
      <p id="d1e241">There have been some attempts at automated landslide detection from Landsat
(e.g. Barlow et al., 2003; Martin and Franklin, 2005). However, manual
mapping remains the most common approach to map landslides despite the time
costs associated with it. Automated or hybrid approaches still need visual
interpretation for calibration, sometimes over large areas (e.g. Ðurić
et al., 2017), and are typically compared to a manual map of landslides that
is considered to represent the “ground truth” (Van Westen et al., 2006;
Guzzetti et al., 2012; Pawłuszek et al., 2017; Bernard et al., 2021).
There remains a perception in the landslide community that automated methods
are neither necessarily more accurate (Guzzetti et al., 2012; Pawłuszek et
al., 2017) nor less time-consuming (Santangelo et al., 2015; Fan et al.,
2019) than manual interpretation. Given the considerable investment of time
and money involved in compiling an inventory, many researchers continue to
generate inventories through manual mapping. It is therefore timely and
useful to evaluate both automated classification and manual mapping against
a common measure of performance.</p>
      <p id="d1e244">Establishing the performance of an automated classifier against manual
mapping requires both establishing the landslide characteristics that should
be reproduced and establishing the quality of manual mapping with respect to
these characteristics. This is typically done by comparing similarity
between at least two independently collected landslide inventories in terms
of their overlap or the similarity in their area–frequency distributions.
Uncertainty in area–frequency distributions from manually mapped landslide
inventories has received considerable attention (e.g. Galli et al., 2008;
Fan et al., 2019; Tanyaş et al., 2019), but uncertainty in landslide spatial
properties has received relatively little attention. However, the limited
number of studies that do quantify landslide inventory error all suggest
very weak spatial agreement between different manually mapped landslide
inventories. Ardizzone et al. (2002) found 34 %–42 % overlap between three
inventories for the same study area (i.e. 34 %–42 % of the area classified
as a landslide in one inventory was classified as a landslide in another).
Galli et al. (2008) found 19 %–34 % overlap for three different inventories,
and Fan et al. (2019) found 33 %–44 % overlap for three inventories
associated with the Wenchuan earthquake. Fan et al. (2019) also compared
their own inventory to the three published inventories and found overlaps of
a similar magnitude (32 %–47 %) with two inventories but a much closer
agreement (82 % overlap) with the third; however, they did not suggest a
reason for this closer agreement. These low-similarity figures suggest that
caution is needed in assuming that any one inventory represents a ground
truth.</p>
      <p id="d1e248">This research seeks to test our hypothesis that an automated detection
algorithm applied to a time series of lower-resolution imagery can deliver
inventories of comparable quality to those generated from the manual mapping of
higher-resolution imagery. We introduce a new approach to automated
landslide detection using Landsat time series in Google Earth Engine (GEE).
Our approach uses similar data and architecture to HazMapper but is focused
on landslides in particular and uses an expectation of long- and short-term
change rather than a straight comparison of pre- and post-event composite
images (Scheip and Wegmann, 2021). To account for uncertainty in the quality
of manually mapped inventories, we apply this approach to case studies where
there are at least two pre-existing inventories. This allows for the direct
comparison of the inventories that we create (in terms of both landslide
location and size) with multiple uncertain manually mapped inventories. The
key question is as follows: can landslide location and size be reproduced more skilfully
by our automated approach than by a second manual inventory?</p>
</sec>
<sec id="Ch1.S2">
  <label>2</label><title>Case study sites</title>
      <p id="d1e259">We choose earthquake-triggered landslide detection to test our hypothesis
because (1) this type of trigger is well constrained in time and its
footprint is well defined in space and (2) there are several earthquake case
studies for which at least two landslide inventories are available in order
to assess the quality of manual mapping. We choose five earthquake case
studies in which at least two landslide inventories have been published and
where the authors attributed the landslides to the same trigger event (i.e.
earthquake timing and epicentral location). The mapping times given below
are each team's estimates of the total number of person-days taken to map
the landslides in their inventory; this is reported in the metadata
associated with that team's submissions to the USGS ScienceBase catalogue
of landslide inventories (Schmitt et al., 2017).</p>
      <?pagebreak page484?><p id="d1e262"><?xmltex \hack{\newpage}?>The 2005 Kashmir, Pakistan, earthquake triggered <inline-formula><mml:math id="M10" display="inline"><mml:mi mathvariant="italic">&gt;</mml:mi></mml:math></inline-formula> 2900
landslides with a combined area of <inline-formula><mml:math id="M11" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 110 km<inline-formula><mml:math id="M12" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula> across an
area of 4000 km<inline-formula><mml:math id="M13" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula> (Basharat et al., 2016). The study area is primarily
underlain by sedimentary rock, with a summer monsoon climate and seasonal
snow on the highest peaks (note that the climate is drier than the 2015
Gorkha study site). Landslides associated with the earthquake were mapped by
Sato et al. (2007, 2017), who estimated that they spent 60 d mapping the
landslides using 2.5 m resolution SPOT 5 (Satellite pour l'Observation de la Terre) optical satellite imagery and by
Basharat et al. (2016, 2017) over 90 d using 2.5 m resolution SPOT 5
imagery and field reconnaissance. The inventories of Sato et al. (2007,
2017) and Basharat et al. (2016, 2017), hereafter referred to as Sato and
Basharat, respectively, contain 2424 and 2930 landslides, respectively.</p>
      <p id="d1e298">The 2007 Aysén Fjord, Chile, earthquake triggered <inline-formula><mml:math id="M14" display="inline"><mml:mi mathvariant="italic">&gt;</mml:mi></mml:math></inline-formula> 500
landslides with a combined area of <inline-formula><mml:math id="M15" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 17 km<inline-formula><mml:math id="M16" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula> across an
area of 1500 km<inline-formula><mml:math id="M17" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula> (Sepulveda et al., 2010b). The study area is glacially
carved valleys in volcanic rock and has a temperate climate with seasonal
snow throughout and perennial snow at altitude. The associated co-seismic
landslides were mapped by Sepulveda et al. (2010a, b) over 120 d
using Landsat images and field mapping and by Gorum et al. (2014, 2017b)
over 5 d using 5 m resolution SPOT 5 imagery. The inventories of
Sepulveda et al. (2010a, b) and Gorum et al. (2014, 2017b), hereafter referred
to as Sepulveda and Gorum, respectively, contain 538 and 517 landslides,
respectively.</p>
      <p id="d1e333">The 2008 Wenchuan, China, earthquake triggered <inline-formula><mml:math id="M18" display="inline"><mml:mi mathvariant="italic">&gt;</mml:mi></mml:math></inline-formula> 190 000
landslides with a combined area of <inline-formula><mml:math id="M19" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 1000 km<inline-formula><mml:math id="M20" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula> across an
area of 75 000 km<inline-formula><mml:math id="M21" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula> (Xu et al., 2014). The study area is primarily
underlain by meta-igneous and sedimentary rock with a humid temperate
climate and snow cover limited to the highest peaks. The associated
co-seismic landslides were mapped by Li et al. (2014, 2017) over 300 d
using high-resolution (3–10 m) optical satellite images and by Xu et al. (2014, 2017) over 1200 d using high-resolution (1–20 m) satellite images.
The inventories of Li et al. (2014, 2017) and Xu et al. (2014, 2017),
hereafter referred to as Li and Xu, respectively, contain 69 606 and 197 481
landslides, respectively.</p>
      <p id="d1e369">The 2010 Haiti earthquake triggered <inline-formula><mml:math id="M22" display="inline"><mml:mi mathvariant="italic">&gt;</mml:mi></mml:math></inline-formula> 20 000 landslides with a
combined area of <inline-formula><mml:math id="M23" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 25 km<inline-formula><mml:math id="M24" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula> (Harp et al., 2016) across an
area of <inline-formula><mml:math id="M25" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 4000 km<inline-formula><mml:math id="M26" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula>. The study area is characterised by
steep but low-relief valleys cut through sedimentary rock with a humid
temperate climate in which snow is extremely rare and a land-use regime in
which the vegetation is rapidly changing. The associated co-seismic
landslides were mapped by Gorum et al. (2013, 2017a) over 40 d using
GeoEye-2 and WorldView-2 (0.6–1 m resolution) satellite images and by Harp
et al. (2016, 2017) using 0.6 m resolution aerial photographs and field
mapping. The inventories of Gorum et al. (2013, 2017a) and Harp et al. (2016, 2017), hereafter referred to as Gorum and Harp, respectively, contain
4490 and 23 567 landslides, respectively.</p>
      <p id="d1e411">The 2015 Gorkha, Nepal, earthquake triggered <inline-formula><mml:math id="M27" display="inline"><mml:mi mathvariant="italic">&gt;</mml:mi></mml:math></inline-formula> 24 000 landslides
with a combined area of <inline-formula><mml:math id="M28" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 87 km<inline-formula><mml:math id="M29" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula> across an area of 20 000 km<inline-formula><mml:math id="M30" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula> (Roback et al., 2018). The study area is primarily sedimentary and
metamorphic rock with seasonal snow at higher elevations and perennial snow
and ice at the highest elevations. The climate ranges from humid temperate to
alpine with a strong summer monsoon. The associated co-seismic landslides
were mapped by Zhang et al. (2016, 2017) over 20 d using Gaofen 1 and Gaofen 2
(1–5.8 m resolution) and Landsat satellite images, by Roback et al. (2017,
2018) using WorldView satellite images (0.5–2 m resolution), and by Watt (2016) using Landsat satellite images. The inventories of Roback et al. (2017, 2018), Zhang et al. (2016, 2017), and Watt (2016), hereafter referred to as
Roback, Zhang, and Watt, respectively, contain 24 915, 2643, and 4924
landslides, respectively. The Watt (2016) mapping reported here was
undertaken for a period of 60 d and involved comparing pan-sharpened
false-colour composites (red, green, and near infrared) derived from Landsat 8 images before and after the earthquake. Mapping was undertaken from
multiple images to minimise occlusion by clouds, but all images were acquired
within 1 year before and after the earthquake. The majority of the study
area was mapped by a single person based on comparison of one pre- and two
post-event images (from 13 March 2015, 1 June 2015, and 7 October 2015). This mapping
was checked and supplemented by a second mapper using the same procedure to
capture previously occluded areas using seven more Landsat 8 images.   The
registration errors in the Watt (2016) inventory were estimated from those
associated with the underlying imagery from which the landslides were
mapped. These Landsat 7 and Landsat 8 images were all georeferenced to Level 1TP
resulting in a radial root mean square error of <inline-formula><mml:math id="M31" display="inline"><mml:mi mathvariant="italic">&lt;</mml:mi></mml:math></inline-formula> 12 m (USGS, 2019),
which is less than the pan-sharpened pixel resolution (15 m). We were unable
to find registration error estimates for the other landslide inventories
examined here.</p>
</sec>
<sec id="Ch1.S3">
  <label>3</label><title>Methods</title>
<sec id="Ch1.S3.SS1">
  <label>3.1</label><title>ALDI classifier: theory</title>
      <p id="d1e468">The automated landslide detection index (ALDI) leverages the change in vegetation cover (and the associated
spectral signature of reflected light) caused by the removal of vegetation
by landslides. The change in spectral signature is typically characterised
by a change in the normalised difference vegetation index (NDVI; Tucker,
1979), defined as
            <disp-formula id="Ch1.E1" content-type="numbered"><label>1</label><mml:math id="M32" display="block"><mml:mrow><mml:mi mathvariant="normal">NDVI</mml:mi><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">n</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">r</mml:mi></mml:msub></mml:mrow><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">n</mml:mi></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">r</mml:mi></mml:msub></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
          where <inline-formula><mml:math id="M33" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">n</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is spectral reflectance in the near-infrared band and
<inline-formula><mml:math id="M34" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">r</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is spectral reflectance in the red band (wavelengths in Table 1). The
light reflected from landslide-affected pixels, whether they are within the
scar or runout area, has a spectral<?pagebreak page485?> signature associated with rock or
sediment. This differs considerably from vegetation in terms of <inline-formula><mml:math id="M35" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">n</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and
<inline-formula><mml:math id="M36" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">r</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, resulting in extremely low NDVI values. We call the difference in
NDVI before and after the trigger event d<inline-formula><mml:math id="M37" display="inline"><mml:mi>V</mml:mi></mml:math></inline-formula>, which is bounded by [<inline-formula><mml:math id="M38" display="inline"><mml:mo lspace="0mm">-</mml:mo></mml:math></inline-formula>1, 1] and
should be negative for landslide pixels associated with the event. This is
not in itself a novel approach and is similar to other NDVI differencing
approaches (e.g. Behling et al., 2014, 2016; Marc et al., 2019; Scheip and
Wegmann, 2021).</p>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T1" specific-use="star"><?xmltex \currentcnt{1}?><label>Table 1</label><caption><p id="d1e573">Landsat and Sentinel image characteristics (Barsi et al., 2014; ESA, 2022).</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="4">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="left"/>
     <oasis:colspec colnum="3" colname="col3" align="left"/>
     <oasis:colspec colnum="4" colname="col4" align="left"/>
     <oasis:thead>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2">Landsat 5 and Landsat 7</oasis:entry>
         <oasis:entry colname="col3">Landsat 8</oasis:entry>
         <oasis:entry colname="col4">Sentinel-2</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>
         <oasis:entry colname="col1">Green (<inline-formula><mml:math id="M39" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>m)</oasis:entry>
         <oasis:entry colname="col2">Band 2: 0.52–0.60</oasis:entry>
         <oasis:entry colname="col3">Band 3: 0.53–0.59</oasis:entry>
         <oasis:entry colname="col4">Band 3: 0.52–0.60</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Red (<inline-formula><mml:math id="M40" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>m)</oasis:entry>
         <oasis:entry colname="col2">Band 3: 0.63–0.69</oasis:entry>
         <oasis:entry colname="col3">Band 4: 0.64–0.67</oasis:entry>
         <oasis:entry colname="col4">Band 4: 0.65–0.69</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Near infrared (<inline-formula><mml:math id="M41" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>m)</oasis:entry>
         <oasis:entry colname="col2">Band 4: 0.77–0.90</oasis:entry>
         <oasis:entry colname="col3">Band 5: 0.85–0.88</oasis:entry>
         <oasis:entry colname="col4">Band 8: 0.76–0.91</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Short-wave infrared (<inline-formula><mml:math id="M42" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>m)</oasis:entry>
         <oasis:entry colname="col2">Band 5: 1.55–1.75</oasis:entry>
         <oasis:entry colname="col3">Band 6: 1.57–1.65</oasis:entry>
         <oasis:entry colname="col4">Band 11: 1.51–1.70</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Spatial resolution (m)</oasis:entry>
         <oasis:entry colname="col2">30</oasis:entry>
         <oasis:entry colname="col3">30</oasis:entry>
         <oasis:entry colname="col4">10</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Revisit time (days)</oasis:entry>
         <oasis:entry colname="col2">16</oasis:entry>
         <oasis:entry colname="col3">16</oasis:entry>
         <oasis:entry colname="col4">5</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Operational life</oasis:entry>
         <oasis:entry colname="col2">1984–2013 (L5)</oasis:entry>
         <oasis:entry colname="col3">2013–present</oasis:entry>
         <oasis:entry colname="col4">June 2015–present (S2a)</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2">1999–present (L7)</oasis:entry>
         <oasis:entry colname="col3"/>
         <oasis:entry colname="col4">March 2017–present (S2b)</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table></table-wrap>

      <p id="d1e761">In addition, vegetation that is disturbed by landslides regrows slowly –
over timescales of months to years (Restrepo et al., 2009). Thus, for
landslide-affected pixels NDVI should not only reduce after the trigger
event but also stay low for an extended period (at least 1 year, depending
on climate and seasonality as well as the timing of the earthquake).
Therefore, we examine a time series of post-event images to calculate a
time-averaged post-event NDVI, which we call <inline-formula><mml:math id="M43" display="inline"><mml:mrow><mml:msub><mml:mi>V</mml:mi><mml:mi mathvariant="normal">post</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, which is bounded by
[0, 1] and which should be low for landslide pixels associated with the
trigger event.</p>
      <p id="d1e776">Averaging over a time series of images has the additional advantage that it
enables robust estimates of both  d<inline-formula><mml:math id="M44" display="inline"><mml:mi>V</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M45" display="inline"><mml:mrow><mml:msub><mml:mi>V</mml:mi><mml:mi mathvariant="normal">post</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> even for NDVI time series
that are both patchy and noisy. The time series are patchy because cloud
cover occludes the ground for some pixels on some days; this cloud can be
removed using filtering algorithms (e.g. Irish, 2000; Goodwin et al., 2013),
but this leaves a gap in the series. The timing and number of these gaps
vary from pixel to pixel, making a comparison of NDVI for particular dates or
images problematic. The time series are noisy because atmospheric conditions
alter both incoming radiation (e.g. cloud shadow) and that received by the
sensor and because ground surface (and especially vegetation) properties
will vary over time both periodically (e.g. due to seasonal vegetation
growth and harvesting) and randomly (e.g. due to leaf orientation).</p>
      <p id="d1e797">Since we expect NDVI to be noisy, we seek a third metric to identify whether
there is a shift in NDVI in the presence of broadly consistent seasonal
variations and random noise in NDVI. For this we take the difference in NDVI
across monthly bins to account for the seasonal component, then quantify the
shift in NDVI since the trigger event. For the shift to be indicative of
real change it should be considerably larger than the noise present in the
NDVI signal. Thus, we express the NDVI shift relative to the noise for each
pixel as
            <disp-formula id="Ch1.E2" content-type="numbered"><label>2</label><mml:math id="M46" display="block"><mml:mrow><mml:mi>t</mml:mi><mml:mo>=</mml:mo><mml:msqrt><mml:mi>n</mml:mi></mml:msqrt><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mi mathvariant="normal">d</mml:mi><mml:mi>V</mml:mi></mml:mrow><mml:mrow><mml:msub><mml:mi>S</mml:mi><mml:mi mathvariant="normal">v</mml:mi></mml:msub></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
          where <inline-formula><mml:math id="M47" display="inline"><mml:mi>n</mml:mi></mml:math></inline-formula> is the sample size (12 for monthly bins), d<inline-formula><mml:math id="M48" display="inline"><mml:mi>V</mml:mi></mml:math></inline-formula> is the mean of the monthly
NDVI differences, and <inline-formula><mml:math id="M49" display="inline"><mml:mrow><mml:msub><mml:mi>S</mml:mi><mml:mi mathvariant="normal">v</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the standard deviation of the monthly NDVI
differences. We then normalise this by mapping <inline-formula><mml:math id="M50" display="inline"><mml:mi>t</mml:mi></mml:math></inline-formula> onto the cumulative Student's <inline-formula><mml:math id="M51" display="inline"><mml:mi>t</mml:mi></mml:math></inline-formula> distribution to generate <inline-formula><mml:math id="M52" display="inline"><mml:mrow><mml:msub><mml:mi>P</mml:mi><mml:mi mathvariant="normal">t</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, the likelihood that the pre- and post-event
NDVIs are drawn from different distributions:
            <disp-formula id="Ch1.E3" content-type="numbered"><label>3</label><mml:math id="M53" display="block"><mml:mrow><mml:msub><mml:mi>P</mml:mi><mml:mi mathvariant="normal">t</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:msub><mml:mi>I</mml:mi><mml:mstyle scriptlevel="+1"><mml:mfrac><mml:mrow><mml:mo>(</mml:mo><mml:mi>n</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>)</mml:mo></mml:mrow><mml:mrow><mml:mi>n</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>+</mml:mo><mml:msup><mml:mi>t</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:mfrac></mml:mstyle></mml:msub><mml:mfenced close=")" open="("><mml:mrow><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mi>n</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow><mml:mn mathvariant="normal">2</mml:mn></mml:mfrac></mml:mstyle><mml:mo>,</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mn mathvariant="normal">1</mml:mn><mml:mn mathvariant="normal">2</mml:mn></mml:mfrac></mml:mstyle></mml:mrow></mml:mfenced><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
          where <inline-formula><mml:math id="M54" display="inline"><mml:mrow><mml:msub><mml:mi>I</mml:mi><mml:mi>x</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>a</mml:mi><mml:mo>,</mml:mo><mml:mi>b</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> is the regularised incomplete beta function. While this is
equivalent to a paired <inline-formula><mml:math id="M55" display="inline"><mml:mi>t</mml:mi></mml:math></inline-formula> test, the results cannot be interpreted as formal
probabilities, as the distribution of d<inline-formula><mml:math id="M56" display="inline"><mml:mi>V</mml:mi></mml:math></inline-formula> may not be Gaussian. Rather they
represent an index of change relative to expected variability which is
bounded by [0, 1]. <inline-formula><mml:math id="M57" display="inline"><mml:mrow><mml:msub><mml:mi>P</mml:mi><mml:mi mathvariant="normal">t</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> should be high for landslide pixels associated
with the trigger event. High <inline-formula><mml:math id="M58" display="inline"><mml:mrow><mml:msub><mml:mi>P</mml:mi><mml:mi mathvariant="normal">t</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> could also result from other events that
reduce the coverage or vigour of vegetation, particularly if this involves
complete removal (e.g. fire or logging). However, seasonal vegetation
changes should be accounted for by examining monthly differences, while
episodic events should only be noticeable when (1) their timing is
coincident with the earthquake and (2) their effect persists over more than
1 year.</p>
      <?pagebreak page486?><p id="d1e1003">Although low NDVI is effective for identifying the absence of vegetation, it
does not uniquely identify landslides, since a range of other surfaces
generate similar signatures, particularly snow and cloud. Cloud cover varies
from one image to another, and we thus seek to remove cloud-affected pixels
from both the pre- and post-event time series. Clouds can be identified based
on their spectral signature, with different types resulting in different
signatures. The “Landsat simple cloud score” function within Google Earth
Engine returns the minimum of a set of five cloudiness indices using
Eqs. (4a)–(4f) and parameters in Table 2 (Earth Engine, 2021). Each index
reflects an expectation about cloud reflectance and temperature: they should
be reasonably bright in the blue band (CI<inline-formula><mml:math id="M59" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">b</mml:mi></mml:msub></mml:math></inline-formula>), in all visible bands
(CI<inline-formula><mml:math id="M60" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mi mathvariant="normal">v</mml:mi></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>, and in all infrared bands (CI<inline-formula><mml:math id="M61" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mrow><mml:mi>i</mml:mi><mml:mi>r</mml:mi></mml:mrow></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>; they should be
reasonably cool in the thermal infrared band (CI<inline-formula><mml:math id="M62" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mrow><mml:mi>T</mml:mi><mml:mi>e</mml:mi><mml:mi>m</mml:mi><mml:mi>p</mml:mi></mml:mrow></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>; but they should
not be snow (CI<inline-formula><mml:math id="M63" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mrow><mml:mi>N</mml:mi><mml:mi>D</mml:mi><mml:mi>S</mml:mi><mml:mi>I</mml:mi></mml:mrow></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>:<?xmltex \setcounter{equation}{3}?>

                <disp-formula id="Ch1.E4" specific-use="gather" content-type="subnumberedsingle"><mml:math id="M64" display="block"><mml:mtable displaystyle="true"><mml:mlabeledtr id="Ch1.E4.5"><mml:mtd><mml:mtext>4a</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:msub><mml:mi mathvariant="normal">CI</mml:mi><mml:mi mathvariant="normal">b</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">b</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">bmin</mml:mi></mml:msub></mml:mrow><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">bmax</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi>R</mml:mi><mml:mrow><mml:mi>b</mml:mi><mml:mi>m</mml:mi><mml:mi>i</mml:mi><mml:mi>n</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E4.6"><mml:mtd><mml:mtext>4b</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:msub><mml:mi mathvariant="normal">CI</mml:mi><mml:mi mathvariant="normal">v</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mfenced open="(" close=")"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">r</mml:mi></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">g</mml:mi></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">b</mml:mi></mml:msub></mml:mrow></mml:mfenced><mml:mo>-</mml:mo><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">vmin</mml:mi></mml:msub></mml:mrow><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">vmax</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">vmin</mml:mi></mml:msub></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E4.7"><mml:mtd><mml:mtext>4c</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:msub><mml:mi mathvariant="normal">CI</mml:mi><mml:mrow><mml:mi>i</mml:mi><mml:mi>r</mml:mi></mml:mrow></mml:msub><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mfenced close=")" open="("><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">n</mml:mi></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi>R</mml:mi><mml:mrow><mml:mi mathvariant="normal">s</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi>R</mml:mi><mml:mrow><mml:mi mathvariant="normal">s</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msub></mml:mrow></mml:mfenced><mml:mo>-</mml:mo><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">irmin</mml:mi></mml:msub></mml:mrow><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">irmax</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">irmin</mml:mi></mml:msub></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E4.8"><mml:mtd><mml:mtext>4d</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:msub><mml:mi mathvariant="normal">CI</mml:mi><mml:mi mathvariant="normal">Temp</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>-</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">t</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">tmin</mml:mi></mml:msub></mml:mrow><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">tmax</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">tmin</mml:mi></mml:msub></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E4.9"><mml:mtd><mml:mtext>4e</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:msub><mml:mi mathvariant="normal">CI</mml:mi><mml:mi mathvariant="normal">NDSI</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>-</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mi mathvariant="normal">NDSI</mml:mi><mml:mo>-</mml:mo><mml:msub><mml:mi mathvariant="normal">NDSI</mml:mi><mml:mi mathvariant="normal">min</mml:mi></mml:msub></mml:mrow><mml:mrow><mml:msub><mml:mi mathvariant="normal">NDSI</mml:mi><mml:mi mathvariant="normal">max</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi mathvariant="normal">NDSI</mml:mi><mml:mi mathvariant="normal">min</mml:mi></mml:msub></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E4.10"><mml:mtd><mml:mtext>4f</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:mi mathvariant="normal">CI</mml:mi><mml:mo>=</mml:mo><mml:mi mathvariant="normal">min</mml:mi><mml:mfenced close=")" open="("><mml:mrow><mml:msub><mml:mi mathvariant="normal">CI</mml:mi><mml:mi mathvariant="normal">b</mml:mi></mml:msub><mml:mo>,</mml:mo><mml:msub><mml:mi mathvariant="normal">CI</mml:mi><mml:mi mathvariant="normal">v</mml:mi></mml:msub><mml:mo>,</mml:mo><mml:msub><mml:mi mathvariant="normal">CI</mml:mi><mml:mi mathvariant="normal">ir</mml:mi></mml:msub><mml:mo>,</mml:mo><mml:msub><mml:mi mathvariant="normal">CI</mml:mi><mml:mi mathvariant="normal">Temp</mml:mi></mml:msub><mml:mo>,</mml:mo><mml:msub><mml:mi mathvariant="normal">CI</mml:mi><mml:mi mathvariant="normal">NDSI</mml:mi></mml:msub></mml:mrow></mml:mfenced><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr></mml:mtable></mml:math></disp-formula>

            where <inline-formula><mml:math id="M65" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">g</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M66" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">b</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> are the spectral reflectances from the red and
blue bands, <inline-formula><mml:math id="M67" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mrow><mml:mi mathvariant="normal">s</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M68" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mrow><mml:mi mathvariant="normal">s</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> are those from the first and second
short-wave infrared bands, and <inline-formula><mml:math id="M69" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">t</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is that from the thermal infrared
band (the only band used here with a coarser 60 m resolution). The
parameters with min and max subscripts (e.g. <inline-formula><mml:math id="M70" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">bmin</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M71" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">bmax</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> for the
red band) in Eq. (4) are minimum and maximum values used to normalise
pixel reflectances; their values are given in Table 2. NDSI is the
normalised difference snow index:
            <disp-formula id="Ch1.E11" content-type="numbered"><label>5</label><mml:math id="M72" display="block"><mml:mrow><mml:mi mathvariant="normal">NDSI</mml:mi><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">g</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub></mml:mrow><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">g</mml:mi></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula></p>
      <p id="d1e1535">This index is also used within ALDI outside the Landsat simple cloud score
function to identify pixels where persistent snow cover could result in
misleading statistics. Where pixels remain snow-covered for periods of
several weeks or months, we cannot retain sufficient observations to
calculate stable statistics from these pixels. Instead, we identify pixels
with persistent snow cover based on time-averaged NDSI and censor them from
the analysis.</p>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T2"><?xmltex \currentcnt{2}?><label>Table 2</label><caption><p id="d1e1541">Parameters for Landsat simple cloud score, Eqs. (4a)–(4f).</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="3">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="left"/>
     <oasis:colspec colnum="3" colname="col3" align="left"/>
     <oasis:thead>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">Threshold</oasis:entry>
         <oasis:entry colname="col2">Minimum</oasis:entry>
         <oasis:entry colname="col3">Maximum</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>
         <oasis:entry colname="col1">Blue (Eq. 4a)</oasis:entry>
         <oasis:entry colname="col2"><inline-formula><mml:math id="M73" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">bmin</mml:mi></mml:msub><mml:mo>=</mml:mo></mml:mrow></mml:math></inline-formula> 0.1</oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M74" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">bmax</mml:mi></mml:msub><mml:mo>=</mml:mo></mml:mrow></mml:math></inline-formula> 0.3</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Visible (Eq. 4b)</oasis:entry>
         <oasis:entry colname="col2"><inline-formula><mml:math id="M75" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">vmin</mml:mi></mml:msub><mml:mo>=</mml:mo></mml:mrow></mml:math></inline-formula> 0.2</oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M76" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">vmax</mml:mi></mml:msub><mml:mo>=</mml:mo></mml:mrow></mml:math></inline-formula> 0.8</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Infrared (Eq. 4c)</oasis:entry>
         <oasis:entry colname="col2"><inline-formula><mml:math id="M77" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">irmin</mml:mi></mml:msub><mml:mo>=</mml:mo></mml:mrow></mml:math></inline-formula> 0.3</oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M78" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">irmax</mml:mi></mml:msub><mml:mo>=</mml:mo></mml:mrow></mml:math></inline-formula> 0.8</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Temperature (Eq. 4d)</oasis:entry>
         <oasis:entry colname="col2"><inline-formula><mml:math id="M79" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">tmin</mml:mi></mml:msub><mml:mo>=</mml:mo></mml:mrow></mml:math></inline-formula> 290</oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M80" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">tmax</mml:mi></mml:msub><mml:mo>=</mml:mo></mml:mrow></mml:math></inline-formula> 300</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">NDSI (Eq. 4e)</oasis:entry>
         <oasis:entry colname="col2">NDSI<inline-formula><mml:math id="M81" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mi mathvariant="normal">min</mml:mi></mml:msub><mml:mo>=</mml:mo></mml:mrow></mml:math></inline-formula> 0.6</oasis:entry>
         <oasis:entry colname="col3">NDSI<inline-formula><mml:math id="M82" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mi mathvariant="normal">max</mml:mi></mml:msub><mml:mo>=</mml:mo></mml:mrow></mml:math></inline-formula> 0.8</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table></table-wrap>

      <p id="d1e1754">We define the automated landslide detection index (ALDI) as the product of
the three parameters defined above. While this formulation is entirely
arbitrary, it has the advantage of allowing the index to take a minimum
value of zero (indicating negligible probability that the images reflect a
landslide at that location) if any of the individual terms is zero. Because
we have no a priori knowledge of the relative importance of each parameter in
determining the landslide signature, we assume a power-functional form with
empirical exponents <inline-formula><mml:math id="M83" display="inline"><mml:mi mathvariant="italic">α</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math id="M84" display="inline"><mml:mi mathvariant="italic">β</mml:mi></mml:math></inline-formula>, and <inline-formula><mml:math id="M85" display="inline"><mml:mi mathvariant="italic">λ</mml:mi></mml:math></inline-formula>:
            <disp-formula id="Ch1.E12" content-type="numbered"><label>6</label><mml:math id="M86" display="block"><mml:mrow><?xmltex \hack{\hbox\bgroup\fontsize{8.4}{8.4}\selectfont$\displaystyle}?><mml:mi mathvariant="normal">ALDI</mml:mi><mml:mo>=</mml:mo><mml:mfenced close="" open="{"><mml:mtable class="array" columnalign="left"><mml:mtr><mml:mtd><mml:mrow><mml:msup><mml:mfenced open="(" close=")"><mml:mrow><mml:mo>-</mml:mo><mml:mi mathvariant="normal">d</mml:mi><mml:mi>V</mml:mi></mml:mrow></mml:mfenced><mml:mi mathvariant="italic">α</mml:mi></mml:msup><mml:msup><mml:mfenced close=")" open="("><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>-</mml:mo><mml:msub><mml:mi>V</mml:mi><mml:mi mathvariant="normal">post</mml:mi></mml:msub></mml:mrow></mml:mfenced><mml:mi mathvariant="italic">β</mml:mi></mml:msup><mml:msubsup><mml:mi>P</mml:mi><mml:mi mathvariant="normal">t</mml:mi><mml:mi mathvariant="italic">λ</mml:mi></mml:msubsup><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mrow><mml:mn mathvariant="normal">0</mml:mn><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:mfenced><mml:mtable class="array" columnalign="left"><mml:mtr><mml:mtd><mml:mrow><mml:mi mathvariant="normal">if</mml:mi><mml:mspace linebreak="nobreak" width="0.25em"/><mml:msub><mml:mi>S</mml:mi><mml:mi mathvariant="normal">post</mml:mi></mml:msub><mml:mo>&gt;</mml:mo><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">snow</mml:mi></mml:msub><mml:mi mathvariant="normal">|</mml:mi><mml:mi mathvariant="normal">d</mml:mi><mml:mi>V</mml:mi><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mi mathvariant="normal">otherwise</mml:mi></mml:mtd></mml:mtr></mml:mtable><mml:mo>,</mml:mo><?xmltex \hack{$\egroup}?></mml:mrow></mml:math></disp-formula>
          where <inline-formula><mml:math id="M87" display="inline"><mml:mrow><mml:msub><mml:mi>S</mml:mi><mml:mi mathvariant="normal">post</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the mean post-earthquake NDSI and <inline-formula><mml:math id="M88" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">snow</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is a threshold
value for NDSI, chosen to identify persistent snow cover. The likelihood
that a pixel is landslide-affected increases monotonically with the ALDI
output value, which has upper and lower bounds of 0 and 1, respectively.
Landslide pixels should be characterised by negative  d<inline-formula><mml:math id="M89" display="inline"><mml:mi>V</mml:mi></mml:math></inline-formula>, indicating vegetation
removal; low <inline-formula><mml:math id="M90" display="inline"><mml:mrow><mml:msub><mml:mi>V</mml:mi><mml:mi mathvariant="normal">post</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, indicating a lack of vegetation after the
earthquake; and high <inline-formula><mml:math id="M91" display="inline"><mml:mrow><mml:msub><mml:mi>P</mml:mi><mml:mi mathvariant="normal">t</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, due to a distinguishable shift in post-event
NDVI distributions relative to the pre-event distributions. The likelihood
that a pixel contains a landslide should increase with <inline-formula><mml:math id="M92" display="inline"><mml:mrow><mml:msub><mml:mi>P</mml:mi><mml:mi mathvariant="normal">t</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and decrease
with  d<inline-formula><mml:math id="M93" display="inline"><mml:mi>V</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M94" display="inline"><mml:mrow><mml:msub><mml:mi>V</mml:mi><mml:mi mathvariant="normal">post</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>. We exclude snow-dominated pixels where <inline-formula><mml:math id="M95" display="inline"><mml:mrow><mml:msub><mml:mi>S</mml:mi><mml:mi mathvariant="normal">post</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> exceeds
threshold <inline-formula><mml:math id="M96" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">snow</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, as well as pixels where median post-earthquake
exceeds pre-earthquake NDVI (i.e. positive d<inline-formula><mml:math id="M97" display="inline"><mml:mi>V</mml:mi></mml:math></inline-formula>).</p>
      <p id="d1e1982">The empirical exponents <inline-formula><mml:math id="M98" display="inline"><mml:mi mathvariant="italic">α</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math id="M99" display="inline"><mml:mi mathvariant="italic">β</mml:mi></mml:math></inline-formula>, and <inline-formula><mml:math id="M100" display="inline"><mml:mi mathvariant="italic">λ</mml:mi></mml:math></inline-formula> can be expressed
in terms of one parameter (<inline-formula><mml:math id="M101" display="inline"><mml:mi mathvariant="italic">α</mml:mi></mml:math></inline-formula>) and two ratios (<inline-formula><mml:math id="M102" display="inline"><mml:mi mathvariant="italic">α</mml:mi></mml:math></inline-formula> : <inline-formula><mml:math id="M103" display="inline"><mml:mi mathvariant="italic">β</mml:mi></mml:math></inline-formula> and
<inline-formula><mml:math id="M104" display="inline"><mml:mi mathvariant="italic">α</mml:mi></mml:math></inline-formula> : <inline-formula><mml:math id="M105" display="inline"><mml:mi mathvariant="italic">λ</mml:mi></mml:math></inline-formula>) because
            <disp-formula id="Ch1.E13" content-type="numbered"><label>7</label><mml:math id="M106" display="block"><mml:mrow><mml:mi mathvariant="italic">β</mml:mi><mml:mo>=</mml:mo><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="italic">α</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mn mathvariant="normal">1</mml:mn><mml:mrow><mml:mi mathvariant="italic">α</mml:mi><mml:mo>:</mml:mo><mml:mi mathvariant="italic">β</mml:mi></mml:mrow></mml:mfrac></mml:mstyle><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="normal">and</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="italic">λ</mml:mi><mml:mo>=</mml:mo><mml:mi mathvariant="italic">α</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mn mathvariant="normal">1</mml:mn><mml:mrow><mml:mi mathvariant="italic">α</mml:mi><mml:mo>:</mml:mo><mml:mi mathvariant="italic">λ</mml:mi></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>,</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mspace linebreak="nobreak" width="0.125em"/></mml:mrow></mml:math></disp-formula>
          substituting the following terms into Eq. (6),
            <disp-formula id="Ch1.E14" content-type="numbered"><label>8</label><mml:math id="M107" display="block"><mml:mrow><?xmltex \hack{\hbox\bgroup\fontsize{7.5}{7.5}\selectfont$\displaystyle}?><mml:mi mathvariant="normal">ALDI</mml:mi><mml:mo>=</mml:mo><mml:mfenced close="" open="{"><mml:mtable class="array" columnalign="left"><mml:mtr><mml:mtd><mml:mrow><mml:msup><mml:mfenced open="(" close=")"><mml:mrow><mml:mo>-</mml:mo><mml:mi mathvariant="normal">d</mml:mi><mml:mi>V</mml:mi></mml:mrow></mml:mfenced><mml:mi mathvariant="italic">α</mml:mi></mml:msup><mml:msup><mml:mfenced open="(" close=")"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>-</mml:mo><mml:msub><mml:mi>V</mml:mi><mml:mi mathvariant="normal">post</mml:mi></mml:msub></mml:mrow></mml:mfenced><mml:mrow><mml:mi mathvariant="italic">α</mml:mi><mml:mstyle scriptlevel="+1"><mml:mfrac><mml:mn mathvariant="normal">1</mml:mn><mml:mrow><mml:mi mathvariant="italic">α</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mo>:</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="italic">β</mml:mi></mml:mrow></mml:mfrac></mml:mstyle></mml:mrow></mml:msup><mml:msubsup><mml:mi>P</mml:mi><mml:mi mathvariant="normal">t</mml:mi><mml:mrow><mml:mi mathvariant="italic">α</mml:mi><mml:mstyle scriptlevel="+1"><mml:mfrac><mml:mn mathvariant="normal">1</mml:mn><mml:mrow><mml:mi mathvariant="italic">α</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mo>:</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="italic">λ</mml:mi></mml:mrow></mml:mfrac></mml:mstyle></mml:mrow></mml:msubsup><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mrow><mml:mn mathvariant="normal">0</mml:mn><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:mfenced><mml:mtable class="array" columnalign="left"><mml:mtr><mml:mtd><mml:mrow><mml:mi mathvariant="normal">if</mml:mi><mml:mspace linebreak="nobreak" width="0.25em"/><mml:msub><mml:mi>S</mml:mi><mml:mi mathvariant="normal">post</mml:mi></mml:msub><mml:mo>&gt;</mml:mo><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">snow</mml:mi></mml:msub><mml:mi mathvariant="normal">|</mml:mi><mml:mi mathvariant="normal">d</mml:mi><mml:mi>V</mml:mi><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mi mathvariant="normal">otherwise</mml:mi></mml:mtd></mml:mtr></mml:mtable><mml:mo>,</mml:mo><?xmltex \hack{$\egroup}?></mml:mrow></mml:math></disp-formula>
          then taking logarithms of both sides clarifies the role of the ratio
parameters. This yields
            <disp-formula id="Ch1.E15" content-type="numbered"><label>9</label><mml:math id="M108" display="block"><mml:mtable rowspacing="0.2ex" class="split" displaystyle="true" columnalign="right left"><mml:mtr><mml:mtd><mml:mrow><mml:mi mathvariant="normal">log</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="normal">ALDI</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mo>=</mml:mo><mml:mi mathvariant="italic">α</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mo mathsize="1.1em">(</mml:mo><mml:mi>log⁡</mml:mi><mml:mfenced close=")" open="("><mml:mrow><mml:mo>-</mml:mo><mml:mi mathvariant="normal">d</mml:mi><mml:mi>V</mml:mi></mml:mrow></mml:mfenced><mml:mo>+</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mn mathvariant="normal">1</mml:mn><mml:mrow><mml:mi mathvariant="italic">α</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mo>:</mml:mo><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="italic">β</mml:mi></mml:mrow></mml:mfrac></mml:mstyle><mml:mi>log⁡</mml:mi><mml:mfenced close=")" open="("><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>-</mml:mo><mml:msub><mml:mi>V</mml:mi><mml:mi mathvariant="normal">post</mml:mi></mml:msub></mml:mrow></mml:mfenced></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mo>+</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mn mathvariant="normal">1</mml:mn><mml:mrow><mml:mi mathvariant="italic">α</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mo>:</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="italic">λ</mml:mi></mml:mrow></mml:mfrac></mml:mstyle><mml:mi mathvariant="normal">log</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi>P</mml:mi><mml:mi mathvariant="normal">t</mml:mi></mml:msub><mml:mo>)</mml:mo><mml:mo mathsize="1.1em">)</mml:mo><mml:mo>.</mml:mo></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:math></disp-formula></p>
      <p id="d1e2316">The values of d<inline-formula><mml:math id="M109" display="inline"><mml:mi>V</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math id="M110" display="inline"><mml:mrow><mml:msub><mml:mi>V</mml:mi><mml:mi mathvariant="normal">post</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, and <inline-formula><mml:math id="M111" display="inline"><mml:mrow><mml:msub><mml:mi>P</mml:mi><mml:mi mathvariant="normal">t</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> are all <inline-formula><mml:math id="M112" display="inline"><mml:mo>≤</mml:mo></mml:math></inline-formula> 1 (thus their logarithms are
negative), and larger values of the ratio parameters (<inline-formula><mml:math id="M113" display="inline"><mml:mi mathvariant="italic">α</mml:mi></mml:math></inline-formula> : <inline-formula><mml:math id="M114" display="inline"><mml:mi mathvariant="italic">β</mml:mi></mml:math></inline-formula> and
<inline-formula><mml:math id="M115" display="inline"><mml:mi mathvariant="italic">α</mml:mi></mml:math></inline-formula> : <inline-formula><mml:math id="M116" display="inline"><mml:mi mathvariant="italic">λ</mml:mi></mml:math></inline-formula>) result in smaller powers for their respective layers
(<inline-formula><mml:math id="M117" display="inline"><mml:mrow><mml:msub><mml:mi>V</mml:mi><mml:mi mathvariant="normal">post</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M118" display="inline"><mml:mrow><mml:msub><mml:mi>P</mml:mi><mml:mi mathvariant="normal">t</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>). Therefore, large <inline-formula><mml:math id="M119" display="inline"><mml:mi mathvariant="italic">α</mml:mi></mml:math></inline-formula> : <inline-formula><mml:math id="M120" display="inline"><mml:mi mathvariant="italic">β</mml:mi></mml:math></inline-formula> ratios result in
a stronger influence of <inline-formula><mml:math id="M121" display="inline"><mml:mrow><mml:msub><mml:mi>V</mml:mi><mml:mi mathvariant="normal">post</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> on ALDI; large <inline-formula><mml:math id="M122" display="inline"><mml:mi mathvariant="italic">α</mml:mi></mml:math></inline-formula> : <inline-formula><mml:math id="M123" display="inline"><mml:mi mathvariant="italic">λ</mml:mi></mml:math></inline-formula> ratios
result in the same for <inline-formula><mml:math id="M124" display="inline"><mml:mrow><mml:msub><mml:mi>P</mml:mi><mml:mi mathvariant="normal">t</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>; and when both <inline-formula><mml:math id="M125" display="inline"><mml:mi mathvariant="italic">α</mml:mi></mml:math></inline-formula> : <inline-formula><mml:math id="M126" display="inline"><mml:mi mathvariant="italic">β</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M127" display="inline"><mml:mi mathvariant="italic">α</mml:mi></mml:math></inline-formula> : <inline-formula><mml:math id="M128" display="inline"><mml:mi mathvariant="italic">λ</mml:mi></mml:math></inline-formula> are small, d<inline-formula><mml:math id="M129" display="inline"><mml:mi>V</mml:mi></mml:math></inline-formula> dominates. These ratios are more informative than
the raw parameters because it is the relationship between exponents rather
than the exponents themselves which defines the relative role of the
different ALDI components (i.e. equal but high values of <inline-formula><mml:math id="M130" display="inline"><mml:mi mathvariant="italic">α</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math id="M131" display="inline"><mml:mi mathvariant="italic">β</mml:mi></mml:math></inline-formula>, and <inline-formula><mml:math id="M132" display="inline"><mml:mi mathvariant="italic">λ</mml:mi></mml:math></inline-formula> result in the same ALDI classification pattern as equal but
low values).</p>
</sec>
<?pagebreak page487?><sec id="Ch1.S3.SS2">
  <label>3.2</label><title>ALDI classifier implementation and data pre-processing</title>
      <p id="d1e2523">We implement ALDI and perform all pre-processing steps within Google Earth
Engine (GEE; Gorelick et al., 2017) because (1) it hosts an extensive
Landsat archive and provides efficient access to large volumes of
freely available satellite data; (2) it provides both a toolkit of
pre-compiled algorithms for image processing and cloud computing resources
to run these algorithms; and (3) it is an open-access platform so that both
the data and the algorithms used here are widely accessible and reproducible
(see Milledge, 2021, for source code).</p>
      <p id="d1e2526">The objective of pre-processing is to generate four layers: d<inline-formula><mml:math id="M133" display="inline"><mml:mi>V</mml:mi></mml:math></inline-formula>, the change in
NDVI before and after the trigger event; <inline-formula><mml:math id="M134" display="inline"><mml:mrow><mml:msub><mml:mi>V</mml:mi><mml:mi mathvariant="normal">post</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, the time-averaged
post-event NDVI; <inline-formula><mml:math id="M135" display="inline"><mml:mrow><mml:msub><mml:mi>S</mml:mi><mml:mi mathvariant="normal">post</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, the post-event NDSI; and <inline-formula><mml:math id="M136" display="inline"><mml:mrow><mml:msub><mml:mi>P</mml:mi><mml:mi mathvariant="normal">t</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, the likelihood
that pre- and post-event NDVIs are drawn from different distributions. These
layers should synthesise the time series of available imagery from multiple
sensors minimising bias due to the sensor, the influence of clouds, and
seasonal vegetation changes.</p>
      <p id="d1e2569">We use time series of NDVI calculated from Landsat 5, Landsat 7, and Landsat 8 imagery
following “top-of-atmosphere” correction (Chander et al., 2009) to adjust
for radiometric variations due to solar illumination geometry (angle and
distance to Sun) and sensor-specific gains and offsets. Sentinel-2 data
would offer additional gains in terms of both spatial and temporal
resolution of data but are not available for any of our case study events
and thus cannot yet be evaluated within the same framework. Landsat 8
sensors aggregate red and near-infrared reflectance over slightly different
frequency bands to Landsat 5 and Landsat 7, but their central frequencies vary by <inline-formula><mml:math id="M137" display="inline"><mml:mi mathvariant="italic">&lt;</mml:mi></mml:math></inline-formula> 4 % between sensors and by <inline-formula><mml:math id="M138" display="inline"><mml:mi mathvariant="italic">&gt;</mml:mi></mml:math></inline-formula> 20 % between bands
(Table 1). To ensure satisfactory image-to-image registration for time
series analysis, we use only images which have been both georeferenced to
ground control points and terrain-corrected (i.e. Level 1TP) and thus have
<inline-formula><mml:math id="M139" display="inline"><mml:mo>≤</mml:mo></mml:math></inline-formula> 12 m radial root mean square error (RMSE) in <inline-formula><mml:math id="M140" display="inline"><mml:mi mathvariant="italic">&gt;</mml:mi></mml:math></inline-formula> 90 % of
cases (USGS, 2019).</p>
      <p id="d1e2600">The time series is split into two “stacks” of images, those before the
trigger event and those after it (Fig. 1b). The duration of these time
series (and thus length of stacks) reflects a trade-off between shorter
durations, which limit the sample size, and longer durations, which include
landscape changes unrelated to the earthquake. We remove “cloudy” pixels
from each stack using the GEE simple cloud score exceeding a tuneable
threshold (<inline-formula><mml:math id="M141" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">cloud</mml:mi></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>, where stricter thresholds not only remove more cloudy pixels
but also incorrectly remove more cloud-free false positives (Earth Engine,
2018). The number of images in each stack is controlled by the stack lengths
and cloud threshold, introducing three tuneable parameters to be calibrated.
These parameters are found using the calibration process described in
Sect. 3.4 rather than by considering the physical processes that
characterise the possible evolution of the time series.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1" specific-use="star"><?xmltex \currentcnt{1}?><?xmltex \def\figurename{Figure}?><label>Figure 1</label><caption><p id="d1e2619">ALDI pre-processing steps. <bold>(a)</bold> Time series of NDVI values for a
single landslide-affected pixel (circled in panels <bold>b</bold> and <bold>d</bold>) before and after
the trigger event, with cloud-free values shown as solid symbols. This time
series is derived from a stack of NDVI images <bold>(b)</bold> and is used to calculate
monthly median NDVI before and after the earthquake and their difference
<bold>(c)</bold>, which can be used to calculate d<inline-formula><mml:math id="M142" display="inline"><mml:mi>V</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math id="M143" display="inline"><mml:mrow><mml:msub><mml:mi>P</mml:mi><mml:mi mathvariant="normal">t</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, and <inline-formula><mml:math id="M144" display="inline"><mml:mrow><mml:msub><mml:mi>V</mml:mi><mml:mi mathvariant="normal">post</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> for every
pixel in the study area <bold>(d)</bold>. Please note that the date format in this figure is month/year.</p></caption>
          <?xmltex \igopts{width=398.338583pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/22/481/2022/nhess-22-481-2022-f01.png"/>

        </fig>

      <p id="d1e2676"><?xmltex \hack{\newpage}?>To account for seasonal vegetation change, NDVI values for each pixel in the
pre- and post-earthquake stacks are extracted as a time series (Fig. 1a)
and binned based on the month in which the image was acquired. Monthly bins
are used since they are generally long enough to contain data in every bin
(even after removal of cloudy pixels) but short enough to capture annual
seasonality (e.g. Fig. 1a). Monthly bins result in four images per bin
per year on average, and thus empty bins are very unlikely except for
month–location pairs that are characterised by extreme cloudiness (such as
Nepal in July; see Wilson and Jetz, 2016). Monthly bins that are empty in
either the pre- or post-earthquake period are not used in the subsequent
analysis, with calculations for that pixel performed using the remaining
monthly bins. We calculate median NDVI for each monthly bin, choosing median
rather than mean, since it is less sensitive to skew and to extreme values
(Fig. 1c). We difference the monthly median values prior to and after the
trigger event, generating a distribution of differences (Fig. 1c). From
that distribution, we calculate the mean monthly NDVI difference (d<inline-formula><mml:math id="M145" display="inline"><mml:mi>V</mml:mi></mml:math></inline-formula>) and
evaluate the likelihood that the mean monthly NDVI difference differs
significantly from zero using a pairwise <inline-formula><mml:math id="M146" display="inline"><mml:mi>t</mml:mi></mml:math></inline-formula> test to calculate <inline-formula><mml:math id="M147" display="inline"><mml:mrow><mml:msub><mml:mi>P</mml:mi><mml:mi mathvariant="normal">t</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>. We take
the mean of the post-event monthly NDVI values to generate <inline-formula><mml:math id="M148" display="inline"><mml:mrow><mml:msub><mml:mi>V</mml:mi><mml:mi mathvariant="normal">post</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, then
apply a similar procedure to the pixel-wise NDSI values to calculate the
mean of the post-event monthly NDSI, <inline-formula><mml:math id="M149" display="inline"><mml:mrow><mml:msub><mml:mi>S</mml:mi><mml:mi mathvariant="normal">post</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>. This allows us to construct
maps of the pixel-wise values of d<inline-formula><mml:math id="M150" display="inline"><mml:mi>V</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math id="M151" display="inline"><mml:mrow><mml:msub><mml:mi>V</mml:mi><mml:mi mathvariant="normal">post</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M152" display="inline"><mml:mrow><mml:msub><mml:mi>S</mml:mi><mml:mi mathvariant="normal">post</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, and <inline-formula><mml:math id="M153" display="inline"><mml:mrow><mml:msub><mml:mi>P</mml:mi><mml:mi mathvariant="normal">t</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>
(Fig. 1d) and thus to evaluate Eq. (6). The full routine runs in GEE in
less than 30 min for an area of <inline-formula><mml:math id="M154" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 10<inline-formula><mml:math id="M155" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msup></mml:math></inline-formula> km<inline-formula><mml:math id="M156" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula> (ca.
10<inline-formula><mml:math id="M157" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">7</mml:mn></mml:msup></mml:math></inline-formula> pixels).</p>
</sec>
<sec id="Ch1.S3.SS3">
  <label>3.3</label><title>Performance testing</title>
      <p id="d1e2811">We evaluate ALDI performance in terms of its ability to reproduce the
location and size of manually mapped landslides. For each earthquake
inventory we define a study area based either on the area defined by the
manual mappers (e.g. excluding areas where cloud or snow cover hampered
manual mapping) or, where this is not available, on a convex hull that
bounds the landslide inventory.</p>
      <p id="d1e2814">ALDI returns a continuous relative measure of the certainty with which a
pixel is classified as a landslide. To evaluate this measure against a
manually mapped landslide inventory it must be converted into a binary
classification by thresholding the classification surface. The manual map is
then rasterised to the same resolution as the classification surface – in
this case, 30 m – using a “majority area” rule, whereby landslide pixels are
those with the majority of their area overlapped by landslide polygons. The
benefit of a given classification can then be quantified in terms of success
in identifying positive (landslide) and negative (non-landslide) outcomes on
a pixel-by-pixel basis. Thresholding the classification surface is a
difficult exercise involving a trade-off between sensitivity, the fraction
of the landslides that should be captured (also known as the true-positive
rate, TPR – the number of true positives normalised by all<?pagebreak page488?> positive
observations), and specificity, the number of false positives that should be
allowed in doing so (also known as the false-positive rate, FPR – the number
of false positives normalised by all negative observations). In practice,
this threshold is often set by external requirements in terms of a desired
sensitivity or specificity, but these requirements can vary considerably
between users and applications.</p>
      <p id="d1e2817">Receiver operating characteristic (ROC) curves provide a more complete
quantification of the performance of the classifier (e.g. Frattini et al.,
2010). The ROC curve is constructed by incrementally thresholding the
classifier and evaluating true- and false-positive rates at different
threshold values to generate a curve where the 1 : 1 line reflects the
naïve (i.e. random) case. The true- and false-positive rates are
insensitive to imbalanced data and thus are well suited to the evaluation of
landslide classification, which typically has many more non-landslide than
landslide pixels (García et al., 2010). The area under the curve (AUC)
tends to 1 as the skill of the classifier improves towards perfect
classification and to 0.5 as the classifier worsens towards the naïve
(random) case. The strength of AUC is that it avoids the need to threshold
the classifier and is widely used, enabling comparison with other landslide
detection methods; its main weakness is that it is difficult to interpret in
absolute terms. What AUC value constitutes “good” performance?</p>
      <p id="d1e2820">In our case, we seek to establish whether automated detection performance is
such that it can be used as an alternative to manual mapping. However, it is
difficult to compare the ALDI output against manual mapping because manual
mapping is itself being used as the ground truth in the absence of a
better alternative. To address this, we first test the agreement between
manual inventories in terms of true- and false-positive rates. TPR<inline-formula><mml:math id="M158" display="inline"><mml:msub><mml:mi/><mml:mtext>I1-2</mml:mtext></mml:msub></mml:math></inline-formula>
indicates the fraction of landslides in inventory I1 that are also predicted
by I2, and FPR<inline-formula><mml:math id="M159" display="inline"><mml:msub><mml:mi/><mml:mtext>I1-2</mml:mtext></mml:msub></mml:math></inline-formula> indicates the fraction of non-landslide pixels in I1
that are “incorrectly” identified as landslide pixels by I2.</p>
      <p id="d1e2842">ALDI performance in identifying landslide location on a pixel-by-pixel basis
can then be compared against one of the manual maps as a competitor with the
other manual map used as the check dataset. To enable the comparison, we
first threshold the ALDI output to generate a binary classifier with the
same FPR as the competitor inventory with respect to the check inventory.
The ability of ALDI to successfully identify more landslide pixels than the
competitor inventory can then be calculated from the difference in their
true-positive rates as TPR<inline-formula><mml:math id="M160" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">diff</mml:mi></mml:msub></mml:math></inline-formula>:
            <disp-formula id="Ch1.E16" content-type="numbered"><label>10</label><mml:math id="M161" display="block"><mml:mrow><mml:msub><mml:mi mathvariant="normal">TPR</mml:mi><mml:mi mathvariant="normal">diff</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:msub><mml:mi mathvariant="normal">TPR</mml:mi><mml:mi mathvariant="normal">ALDI</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi mathvariant="normal">TPR</mml:mi><mml:mi mathvariant="normal">Comp</mml:mi></mml:msub><mml:mo>,</mml:mo><mml:msub><mml:mi mathvariant="normal">FPR</mml:mi><mml:mi mathvariant="normal">ALDI</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:msub><mml:mi mathvariant="normal">FPR</mml:mi><mml:mi mathvariant="normal">Comp</mml:mi></mml:msub><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
          where TPR<inline-formula><mml:math id="M162" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">ALDI</mml:mi></mml:msub></mml:math></inline-formula> and FPR<inline-formula><mml:math id="M163" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">ALDI</mml:mi></mml:msub></mml:math></inline-formula> are the ALDI true- and false-positive
rates, respectively, both calculated from the check inventory, and
TPR<inline-formula><mml:math id="M164" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">Comp</mml:mi></mml:msub></mml:math></inline-formula> and FPR<inline-formula><mml:math id="M165" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">Comp</mml:mi></mml:msub></mml:math></inline-formula> are the true- and false-positive rates for
the competitor inventory, also calculated from the check inventory. The
magnitude of TPR<inline-formula><mml:math id="M166" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">diff</mml:mi></mml:msub></mml:math></inline-formula> indicates the similarity in performance, while the
sign indicates the<?pagebreak page489?> best performer (positive values indicate that ALDI
outperforms manual mapping and vice versa). This approach allows for direct
comparison between ALDI and manual mapping for the same classification
threshold. Other metrics could be derived from the confusion matrix (e.g.
Tharwat, 2020; Prakash et al., 2020), but these typically require assumptions
about the relative weight assigned to true and false positives and
negatives. Our approach avoids these assumptions because the ALDI output is
thresholded to ensure that FPRs are equal to those of the competitor
inventory.</p>
      <p id="d1e2941">In addition, we express spatial mapping error between manual inventories as
the ratio of the intersection of the two maps to their union. This is
equivalent to the “degree of matching” (Carrara et al., 1992; Galli et al.,
2008) and can be interpreted as the percentage of total mapped landslide
area that the inventories have in common.</p>
      <p id="d1e2944">To examine the ability of ALDI to recover landslide size information we
compare the area–frequency distributions of landslides from each manual map
with those for landslides detected by ALDI. For manually mapped inventories
this information is generally captured automatically, since landslides are
mapped as discrete objects rather than on a pixel-by-pixel basis. However,
automated classifiers like ALDI require additional steps to convert a
continuous pixel-based classification surface to a set of landslide objects.
First, we generate a binary prediction of landslide presence or absence by
thresholding the ALDI classification surface to match the manually mapped
FPR, as described above. The manual inventories examined here typically have
very low FPRs (<inline-formula><mml:math id="M167" display="inline"><mml:mi mathvariant="italic">&lt;</mml:mi></mml:math></inline-formula> 2 % of TPR on average and <inline-formula><mml:math id="M168" display="inline"><mml:mi mathvariant="italic">&lt;</mml:mi></mml:math></inline-formula> 7 % at
most, Table 3). Second, we convert the binary landslide map to a set of
landslide objects by identifying connected components at the 30 m resolution
of the Landsat imagery (Haralick and Shapiro, 1992). This connected-component clustering is one of the simplest of many possible clustering
algorithms. Finally, we calculate the area of individual landslide objects
from the number of pixels in each object (cluster) and generate an
area–frequency distribution.</p>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T3" specific-use="star"><?xmltex \currentcnt{3}?><label>Table 3</label><caption><p id="d1e2964">Performance metrics for ALDI applied with the different parameter sets to identify landslide-affected areas from each of the 14 inventory pairs. Abbreviated names for the inventory pairs indicate the case study with subscripts denoting first check and then competitor inventories (e.g. <inline-formula><mml:math id="M169" display="inline"><mml:mrow><mml:msub><mml:mi>K</mml:mi><mml:mi mathvariant="normal">SB</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> denotes the Kashmir earthquake with Sato as the check inventory and Basharat as the competitor inventory). The true-positive rate (TPR) and false-positive rate (FPR) are reported for both object-based analysis (in brackets) and pixel-based analysis at 30 m resolution. Overlap indicates the percentage overlap between pairs of landslide inventories. Shading in right-hand columns indicates performance of ALDI relative to each competitor and for each metric and calibration, with a linear colour scale from blue where ALDI outperforms the manual competitor to red where the manual competitor outperforms ALDI. Vertical blocks reflect different performance metrics: TPR<inline-formula><mml:math id="M170" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">diff</mml:mi></mml:msub></mml:math></inline-formula>  and AUC (see text). Columns within each block reflect different ALDI calibration strategies: local calibration optimised to both site and check inventory, global calibration using a compilation of the best parameter sets from all sites, and holdback calibration where parameter sets from the test site are excluded. Note that positive values of TPR<inline-formula><mml:math id="M171" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">diff</mml:mi></mml:msub></mml:math></inline-formula> reflect cases where ALDI outperforms manual mapping, while negative values reflect cases where manual mapping is better.</p></caption>
  <?xmltex \igopts{width=398.338583pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/22/481/2022/nhess-22-481-2022-t03.png"/>
</table-wrap>

</sec>
<sec id="Ch1.S3.SS4">
  <label>3.4</label><title>Parameter calibration and uncertainty estimation</title>
      <p id="d1e3009">The ALDI landslide classifier has seven tuneable parameters: cloud threshold
(<inline-formula><mml:math id="M172" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">cloud</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>), pre-event stack length (<inline-formula><mml:math id="M173" display="inline"><mml:mrow><mml:msub><mml:mi>L</mml:mi><mml:mi mathvariant="normal">pre</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>), post-event stack length
(<inline-formula><mml:math id="M174" display="inline"><mml:mrow><mml:msub><mml:mi>L</mml:mi><mml:mi mathvariant="normal">post</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>), snow threshold (<inline-formula><mml:math id="M175" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">snow</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>), and the three exponents (<inline-formula><mml:math id="M176" display="inline"><mml:mi mathvariant="italic">α</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math id="M177" display="inline"><mml:mi mathvariant="italic">β</mml:mi></mml:math></inline-formula>, and <inline-formula><mml:math id="M178" display="inline"><mml:mi mathvariant="italic">λ</mml:mi></mml:math></inline-formula>) that control the weighting assigned to the
<inline-formula><mml:math id="M179" display="inline"><mml:mrow><mml:msub><mml:mi>V</mml:mi><mml:mi mathvariant="normal">post</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, d<inline-formula><mml:math id="M180" display="inline"><mml:mi>V</mml:mi></mml:math></inline-formula>, and <inline-formula><mml:math id="M181" display="inline"><mml:mrow><mml:msub><mml:mi>P</mml:mi><mml:mi mathvariant="normal">t</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> layers, respectively. Calibrating the parameters and
estimating the associated uncertainty is important because the parameters
are difficult or impossible to set a priori and because we seek to develop a general
model that can be applied to new landslide events not examined here. Our
calibration seeks to optimise classifier performance evaluated by comparing
the classifier to 11 manually mapped landslide inventories using the
performance metrics described in Sect. 3.3.</p>
      <p id="d1e3107"><?xmltex \hack{\newpage}?>We calibrate ALDI parameters using one-at-a-time calibration for parameters
that are internal to the GEE routine (<inline-formula><mml:math id="M182" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">cloud</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M183" display="inline"><mml:mrow><mml:msub><mml:mi>L</mml:mi><mml:mi mathvariant="normal">pre</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M184" display="inline"><mml:mrow><mml:msub><mml:mi>L</mml:mi><mml:mi mathvariant="normal">post</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>),
since these parameters are well constrained (in the case of <inline-formula><mml:math id="M185" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">cloud</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and
<inline-formula><mml:math id="M186" display="inline"><mml:mrow><mml:msub><mml:mi>L</mml:mi><mml:mi mathvariant="normal">post</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) or have a limited number of possible values (in the case of
<inline-formula><mml:math id="M187" display="inline"><mml:mrow><mml:msub><mml:mi>L</mml:mi><mml:mi mathvariant="normal">pre</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M188" display="inline"><mml:mrow><mml:msub><mml:mi>L</mml:mi><mml:mi mathvariant="normal">post</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>). We use an informal Bayesian calibration procedure
(e.g. Beven and Binley, 1992) for parameters in Eq. (6) (<inline-formula><mml:math id="M189" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">snow</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>
<inline-formula><mml:math id="M190" display="inline"><mml:mi mathvariant="italic">α</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math id="M191" display="inline"><mml:mi mathvariant="italic">β</mml:mi></mml:math></inline-formula>, and <inline-formula><mml:math id="M192" display="inline"><mml:mi mathvariant="italic">λ</mml:mi></mml:math></inline-formula>), since these parameters are less well
constrained, but evaluation of Eq. (6) is computationally cheap. We
calibrate <inline-formula><mml:math id="M193" display="inline"><mml:mrow><mml:msub><mml:mi>L</mml:mi><mml:mi mathvariant="normal">post</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M194" display="inline"><mml:mrow><mml:msub><mml:mi>L</mml:mi><mml:mi mathvariant="normal">pre</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, and <inline-formula><mml:math id="M195" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">cloud</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> one-at-a-time (in that order)
for each earthquake event then test alternative near-optimum parameter
combinations to minimise the effect of the calibration order. These
combinations are obtained by varying <inline-formula><mml:math id="M196" display="inline"><mml:mrow><mml:msub><mml:mi>L</mml:mi><mml:mi mathvariant="normal">post</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> by <inline-formula><mml:math id="M197" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 1 year for optimum
values of <inline-formula><mml:math id="M198" display="inline"><mml:mrow><mml:msub><mml:mi>L</mml:mi><mml:mi mathvariant="normal">pre</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M199" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">cloud</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and doing the same for <inline-formula><mml:math id="M200" display="inline"><mml:mrow><mml:msub><mml:mi>L</mml:mi><mml:mi mathvariant="normal">pre</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> at
optimum values of <inline-formula><mml:math id="M201" display="inline"><mml:mrow><mml:msub><mml:mi>L</mml:mi><mml:mi mathvariant="normal">post</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M202" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">cloud</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>. For each GEE run in the
one-at-a-time process we run 500 simulations of Eq. (6) with <inline-formula><mml:math id="M203" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">snow</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>
and <inline-formula><mml:math id="M204" display="inline"><mml:mi mathvariant="italic">α</mml:mi></mml:math></inline-formula> randomly sampled from uniform probability distributions and
the ratio parameters sampled from uniform distributions of log<inline-formula><mml:math id="M205" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">10</mml:mn></mml:msub></mml:math></inline-formula>(<inline-formula><mml:math id="M206" display="inline"><mml:mi mathvariant="italic">α</mml:mi></mml:math></inline-formula> : <inline-formula><mml:math id="M207" display="inline"><mml:mi mathvariant="italic">β</mml:mi></mml:math></inline-formula>) and log<inline-formula><mml:math id="M208" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">10</mml:mn></mml:msub></mml:math></inline-formula>(<inline-formula><mml:math id="M209" display="inline"><mml:mi mathvariant="italic">α</mml:mi></mml:math></inline-formula> : <inline-formula><mml:math id="M210" display="inline"><mml:mi mathvariant="italic">λ</mml:mi></mml:math></inline-formula>). We sample the ratio parameters
in logarithmic space to maintain symmetric sampling density with distance
from a ratio of unity (e.g. <inline-formula><mml:math id="M211" display="inline"><mml:mi mathvariant="italic">α</mml:mi></mml:math></inline-formula> : <inline-formula><mml:math id="M212" display="inline"><mml:mrow><mml:mi mathvariant="italic">β</mml:mi><mml:mo>=</mml:mo></mml:mrow></mml:math></inline-formula> 0.1, where <inline-formula><mml:math id="M213" display="inline"><mml:mrow><mml:mi mathvariant="italic">β</mml:mi><mml:mo>=</mml:mo></mml:mrow></mml:math></inline-formula> 10<inline-formula><mml:math id="M214" display="inline"><mml:mi mathvariant="italic">α</mml:mi></mml:math></inline-formula> should be sampled as densely as <inline-formula><mml:math id="M215" display="inline"><mml:mi mathvariant="italic">α</mml:mi></mml:math></inline-formula> : <inline-formula><mml:math id="M216" display="inline"><mml:mrow><mml:mi mathvariant="italic">β</mml:mi><mml:mo>=</mml:mo></mml:mrow></mml:math></inline-formula>10,
where <inline-formula><mml:math id="M217" display="inline"><mml:mrow><mml:mi mathvariant="italic">α</mml:mi><mml:mo>=</mml:mo></mml:mrow></mml:math></inline-formula> 10<inline-formula><mml:math id="M218" display="inline"><mml:mi mathvariant="italic">β</mml:mi></mml:math></inline-formula>).</p>
      <p id="d1e3464">We examine <inline-formula><mml:math id="M219" display="inline"><mml:mrow><mml:msub><mml:mi>L</mml:mi><mml:mi mathvariant="normal">post</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> of up to 5 years because vegetation typically begins
to regrow over this timescale (Restrepo et al., 2009) and <inline-formula><mml:math id="M220" display="inline"><mml:mrow><mml:msub><mml:mi>L</mml:mi><mml:mi mathvariant="normal">pre</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> of up
to 10 years because we expect that other landscape changes (e.g. fire,
drought, and landslides caused by other triggers) will begin to disrupt the
pre-event signal at longer timescales. In both cases we examine only integer
year values to ensure consistent sampling within the monthly bins. We use
the full range of NDSI values for <inline-formula><mml:math id="M221" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">snow</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> ([0, 1]) and cloud score values
for <inline-formula><mml:math id="M222" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">cloud</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> ([0, 1]). For the three exponents, we use zero for the lower
bound and iteratively refine the upper bound to ensure that optimum
performance at any site is found to be within the range.</p>
      <p id="d1e3511">We perform the calibration for individual earthquakes to estimate the
optimum classification skill that could be obtained when calibrating on all
the check data. We then retain the best 20 parameter sets (measured in terms
of AUC) from each earthquake to generate a global set of 100 parameter sets.
To account for parameter interaction (particularly between the three
exponents <inline-formula><mml:math id="M223" display="inline"><mml:mi mathvariant="italic">α</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math id="M224" display="inline"><mml:mi mathvariant="italic">β</mml:mi></mml:math></inline-formula>, and <inline-formula><mml:math id="M225" display="inline"><mml:mi mathvariant="italic">λ</mml:mi></mml:math></inline-formula>) within a set we retain
parameter sets as seven-element vectors. To ensure that each manually mapped
landslide inventory is given equal weight as a check dataset we calibrate to
each in turn taking 7 parameter sets from calibration to each of the 3 Gorkha inventories and 10 from each of the 2 inventories at the other
sites. Finally, we run ALDI with each of these 100 parameter sets to
generate 100 ALDI classification surfaces then take the mean for each cell.</p>
      <p id="d1e3536">To simulate the “blind” application of ALDI to future events, we perform a
holdback test in which we run ALDI using the global-parameter set but
hold back the 20 parameter sets that were derived from the site at which
testing is<?pagebreak page490?> being performed. In this test the parameters used to run ALDI are
uninfluenced by the specific behaviour of the test site.</p>
</sec>
</sec>
<sec id="Ch1.S4">
  <label>4</label><title>Results</title>
<sec id="Ch1.S4.SS1">
  <label>4.1</label><title>Spatial agreement: Gorkha case study</title>
      <p id="d1e3555">We first illustrate our approach using the 2015 Gorkha earthquake, where
three manual inventories are available, and then consider the other four
earthquakes introduced in Sect. 2. All three manual inventories for the
Gorkha earthquake show an elongated cluster of landslides extending from
northwest to southeast (Fig. 2a) that coincides with the area of steep
slopes that experienced the most intense shaking. However, when the maps are
compared at a finer scale they differ considerably (Fig. 2c, e). In some
cases, one mapper has identified a landslide, but one or both of the others
have not (e.g. location A in Fig. 2e). Some, but not all, of these missed
landslides can be attributed to areas where imagery was unavailable or where
the ground was obscured by clouds (shown as grey areas in Fig. 2c). In
other cases, mapped landslides overlap, but their size and/or shape differ,
due either to differences in the interpretation of landslide boundaries (e.g.
location B in Fig. 2e) or to the georeferencing of the underlying imagery
from which the landslides were mapped. Georeferencing differences seem
particularly likely to explain mapped landslides of very similar size and
shape that are offset by<?pagebreak page491?> small distances (e.g. location C in Fig. 2e) or
appear distorted relative to one another so that their outlines only
partially overlap (e.g. location D in Fig. 2e).</p>

      <?xmltex \floatpos{p}?><fig id="Ch1.F2" specific-use="star"><?xmltex \currentcnt{2}?><?xmltex \def\figurename{Figure}?><label>Figure 2</label><caption><p id="d1e3560">Mapped landslides and the ALDI classifier for the Gorkha study
site. <bold>(a)</bold> Mapped landslides at the scale of the full study area with AOIs (areas of interest; the mapped area) shown in grey. Zhang, Roback, and Watt refer to the
inventories of Zhang et al. (2016), Roback et al. (2018), and Watt (2016).
<bold>(b)</bold> ALDI values for the full study area, using locally optimised parameters.
<bold>(c)</bold> Mapped landslides from the three inventories for a subset of the study
area, with areas that were unmapped in one or more inventory shaded grey. <bold>(d)</bold> ALDI values using locally optimised parameters for the same subset of the
study area shown in <bold>(c)</bold>. <bold>(e)</bold> Detailed view of mapped landslides from the
three inventories and ALDI values. Yellow boxes in each panel show the
locations of nested panels (e.g. <bold>c</bold> in <bold>a</bold> and <bold>d</bold> in <bold>b</bold>). Green labels in <bold>(e)</bold> indicate examples of (A) missed landslides, (B) agreement between
inventories, (C) offset landslide outlines, (D) distorted landslide outlines,
and (F) landslides identified by ALDI but missed by manual mapping.</p></caption>
          <?xmltex \igopts{width=426.791339pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/22/481/2022/nhess-22-481-2022-f02.png"/>

        </fig>

      <p id="d1e3603">The ALDI classifier applied to the Gorkha earthquake captures the broad
spatial pattern of mapped co-seismic landslides with large patches of high
ALDI values, and thus high classification likelihood, corresponding to
clusters of mapped landslides (Fig. 2b). Examining a subsection of the
study area (Fig. 2d) shows that ALDI identifies the same broad zones of
more intense landsliding as identified in the manual mapping. However, the ALDI
output also contains a series of stripes <inline-formula><mml:math id="M226" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 1 km apart and
<inline-formula><mml:math id="M227" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 150 m wide trending west-northwest to east-southeast most clearly visible across the centre of the map. These are
the result of data gaps in Landsat 7 images since 2003 due to Scan Line
Corrector (SLC) failure on the Landsat 7 sensor. Although both pre- and
post-event image stacks include Landsat 5 and Landsat 8 images in addition to
Landsat 7, these data gaps clearly influence the ALDI output, with high
values more likely for pixels where Landsat 7 data are not available.</p>
      <p id="d1e3621">Zooming in to a smaller subsection of the study area suggests that most of
the landslides that are included in both inventories overlap areas of high
ALDI values (Fig. 2e). In addition, areas of high ALDI values overlap many
of those landslides identified by one inventory but not the other, although
there are mapped landslides that do not overlap areas with high ALDI values
(Fig. 2e). In many cases, the patches of high ALDI values have shapes that
closely follow those of the mapped landslides (Fig. 2e). In other cases,
patches of high ALDI values have typical landslide morphology but are not in
either inventory (e.g. location E in Fig. 2e), raising the question of
whether these should be considered genuine classifier false positives or are
in fact landslides missed in all three manual maps. Given that each
inventory misses landslides identified by another, this possibility cannot
be excluded. In other cases, the patches of high ALDI values have a size
and/or shape that suggest that they are misclassifications. These may be
due to clouds, shadows, snow, or other landscape changes not associated with
landslides (e.g. crop harvesting, river channel change, building
construction).</p>
</sec>
<sec id="Ch1.S4.SS2">
  <label>4.2</label><title>ALDI calibration: Gorkha case study</title>
      <p id="d1e3632">In this section, we seek to establish the best possible ALDI performance
when parameters can be optimised to a single study site and identify the
influence of parameters on that performance, both in terms of sensitivity to
the parameter and preferred range for the parameter. We illustrate this
using the Gorkha earthquake, calibrating ALDI's seven tuneable parameters
(columns a–g in Fig. 3) to optimise agreement with two of the manually
mapped landslide inventories measured using our two performance metrics
(rows in Fig. 3). The results are visualised in Fig. 3 using dotty plots
(after Beven and Binley, 1992): a matrix of scatter plots where each subplot
shows model performance (<inline-formula><mml:math id="M228" display="inline"><mml:mi>y</mml:mi></mml:math></inline-formula> axis) against a parameter value (<inline-formula><mml:math id="M229" display="inline"><mml:mi>x</mml:mi></mml:math></inline-formula> axis). The
histogram above each scatter plot shows the frequency distribution of
parameter values for the best 50 model runs for that metric and check
dataset.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3" specific-use="star"><?xmltex \currentcnt{3}?><?xmltex \def\figurename{Figure}?><label>Figure 3</label><caption><p id="d1e3651">Dotty plots and posterior parameter distributions for the Gorkha
case study for the seven tuneable parameters associated with ALDI (columns)
evaluated using two of the test datasets (Watt and Roback) and two
performance metrics (rows): (1) TPR<inline-formula><mml:math id="M230" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">diff</mml:mi></mml:msub></mml:math></inline-formula>, the difference in TPR between ALDI
and the competitor inventory at the FPR defined by the competitor inventory,
and (2) AUC, the area under the ROC curve, a more general indicator of
classifier performance over the full range of FPRs. “Roback/Watt” refers to
using Roback as the check dataset and Watt as the competitor in row 1;
“Watt/Roback” refers to the converse in row 2. Roback is used as the check
dataset in row 3, and Watt is the check dataset in row 4. Points plotting
above the yellow line are results for the best 100 parameter values. In each
case the parameter distributions are for the best 100 parameter sets
evaluated using the same metric and datasets as the dotty plot below it.
Dotty plots for the other Gorkha inventories and for all other sites are
given in the Supplement. EQ: earthquake.</p></caption>
          <?xmltex \igopts{width=426.791339pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/22/481/2022/nhess-22-481-2022-f03.png"/>

        </fig>

      <p id="d1e3669">All the scatter plots in Fig. 3 show wide scatter in performance for a
single value of any given parameter, indicating that the model is sensitive
to multiple parameters. However, the key feature of each plot is the upper
bound on ALDI performance for a given parameter value and the sensitivity of this upper bound
to change in that parameter. This upper bound can be interpreted as the best
possible ALDI performance at value <inline-formula><mml:math id="M231" display="inline"><mml:mi>x</mml:mi></mml:math></inline-formula> of parameter A when all other
parameters are given flexibility to optimise. Plots where this upper bound
is near horizontal suggest limited influence of a particular parameter and
are accompanied by broad histograms. Narrow peaks in a plot's upper bound
indicate that good model performance requires that parameter to be set
within a narrow range, with performance degrading rapidly as values depart
from this range independent of other parameter values. In the following
paragraphs we examine the influence of each parameter in turn (Fig. 3).</p>
      <p id="d1e3680">Setting the pre- and post-earthquake stack lengths (<inline-formula><mml:math id="M232" display="inline"><mml:mrow><mml:msub><mml:mi>L</mml:mi><mml:mi mathvariant="normal">pre</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and
<inline-formula><mml:math id="M233" display="inline"><mml:mrow><mml:msub><mml:mi>L</mml:mi><mml:mi mathvariant="normal">post</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, respectively) involves a trade-off between errors caused by
landslides (or other landscape changes) not associated with the earthquake,
if the stack is too long, and errors caused by cloud cover, if the stack is
too short. For the Gorkha earthquake, ALDI performance is most sensitive to
<inline-formula><mml:math id="M234" display="inline"><mml:mrow><mml:msub><mml:mi>L</mml:mi><mml:mi mathvariant="normal">post</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, indicated by the steep gradient in upper-bound performance across
both metrics and for all check datasets (Fig. 3, column g). For all
metrics and datasets, a post-earthquake stack length of only 1 year
produces the best performance. This may be because longer stacks are more
likely to include other landscape changes after the earthquake that disrupt
the signal, such as post-seismic landslides or re-vegetation of co-seismic
landslides.</p>
      <p id="d1e3716">ALDI allows landslides to be identified only in pixels where NDSI is lower
than the snow threshold (<inline-formula><mml:math id="M235" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">snow</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>). ALDI performs well (i.e. <inline-formula><mml:math id="M236" display="inline"><mml:mi mathvariant="italic">&lt;</mml:mi></mml:math></inline-formula> 20 % from optimum) for <inline-formula><mml:math id="M237" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">snow</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> values ranging from 0.1 to 0.9 (Fig. 4,
column d). For TPR<inline-formula><mml:math id="M238" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">diff</mml:mi></mml:msub></mml:math></inline-formula> the best values of <inline-formula><mml:math id="M239" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">snow</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> are 0.2–0.4 with a
rapid decline in performance as <inline-formula><mml:math id="M240" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">snow</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is reduced and a slow decline as
it is increased (Fig. 4, rows 1–2 of column d). This suggests that snow
rarely causes false positives even when little effort is made to remove it
but that an overly conservative snow threshold results in landslides being
misclassified as snow. The AUC metric behaves similarly to TPR<inline-formula><mml:math id="M241" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">diff</mml:mi></mml:msub></mml:math></inline-formula> with
a larger performance reduction at low <inline-formula><mml:math id="M242" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">snow</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> values and reduced
performance reduction at high <inline-formula><mml:math id="M243" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">snow</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> values (Fig. 4, rows 3–4 of column d).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4" specific-use="star"><?xmltex \currentcnt{4}?><?xmltex \def\figurename{Figure}?><label>Figure 4</label><caption><p id="d1e3813">Dotty plots and posterior parameter distributions for the seven
tuneable parameters associated with ALDI (columns <bold>a</bold>–<bold>g</bold>) for the five study
earthquakes (rows 1–5). Dotty plots show classifier performance evaluated
using AUC, the area under the ROC curve. Blue or red colours indicate the
inventory used as the check dataset, as shown to the right. Parameter
distributions are for the best 100 parameter sets evaluated using the same
metric. EQ: earthquake.</p></caption>
          <?xmltex \igopts{width=426.791339pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/22/481/2022/nhess-22-481-2022-f04.png"/>

        </fig>

      <?pagebreak page493?><p id="d1e3828">The <inline-formula><mml:math id="M244" display="inline"><mml:mi mathvariant="italic">α</mml:mi></mml:math></inline-formula> : <inline-formula><mml:math id="M245" display="inline"><mml:mi mathvariant="italic">β</mml:mi></mml:math></inline-formula> ratio controls the influence of change in NDVI (d<inline-formula><mml:math id="M246" display="inline"><mml:mi>V</mml:mi></mml:math></inline-formula>)
relative to mean post-earthquake NDVI (<inline-formula><mml:math id="M247" display="inline"><mml:mrow><mml:msub><mml:mi>V</mml:mi><mml:mi mathvariant="normal">post</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>). Noting that d<inline-formula><mml:math id="M248" display="inline"><mml:mi>V</mml:mi></mml:math></inline-formula> and
<inline-formula><mml:math id="M249" display="inline"><mml:mrow><mml:msub><mml:mi>V</mml:mi><mml:mi mathvariant="normal">post</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> are bounded to be <inline-formula><mml:math id="M250" display="inline"><mml:mi mathvariant="italic">&lt;</mml:mi></mml:math></inline-formula> 1 and that by definition <inline-formula><mml:math id="M251" display="inline"><mml:mrow><mml:mi mathvariant="italic">β</mml:mi><mml:mo>=</mml:mo><mml:mi mathvariant="italic">α</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="italic">α</mml:mi></mml:mrow></mml:math></inline-formula> : <inline-formula><mml:math id="M252" display="inline"><mml:mrow><mml:mi mathvariant="italic">β</mml:mi><mml:msup><mml:mo>)</mml:mo><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>, larger values of <inline-formula><mml:math id="M253" display="inline"><mml:mi mathvariant="italic">α</mml:mi></mml:math></inline-formula> : <inline-formula><mml:math id="M254" display="inline"><mml:mi mathvariant="italic">β</mml:mi></mml:math></inline-formula> result in smaller exponents on <inline-formula><mml:math id="M255" display="inline"><mml:mrow><mml:msub><mml:mi>V</mml:mi><mml:mi mathvariant="normal">post</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and larger values of the term.
ALDI is thus dominated by <inline-formula><mml:math id="M256" display="inline"><mml:mrow><mml:msub><mml:mi>V</mml:mi><mml:mi mathvariant="normal">post</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> at higher <inline-formula><mml:math id="M257" display="inline"><mml:mi mathvariant="italic">α</mml:mi></mml:math></inline-formula> : <inline-formula><mml:math id="M258" display="inline"><mml:mi mathvariant="italic">β</mml:mi></mml:math></inline-formula> ratios and
by d<inline-formula><mml:math id="M259" display="inline"><mml:mi>V</mml:mi></mml:math></inline-formula> at lower ratios. There is a clear optimum within the parameter space and
a large reduction in performance away from this optimum indicating that both
layers (d<inline-formula><mml:math id="M260" display="inline"><mml:mi>V</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M261" display="inline"><mml:mrow><mml:msub><mml:mi>V</mml:mi><mml:mi mathvariant="normal">post</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) are important components of the classifier (Fig. 3, column b). Best performances are found in the range <inline-formula><mml:math id="M262" display="inline"><mml:mi mathvariant="italic">α</mml:mi></mml:math></inline-formula> : <inline-formula><mml:math id="M263" display="inline"><mml:mi mathvariant="italic">β</mml:mi></mml:math></inline-formula> <inline-formula><mml:math id="M264" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 3–4 for TPR<inline-formula><mml:math id="M265" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">diff</mml:mi></mml:msub></mml:math></inline-formula> and in the range <inline-formula><mml:math id="M266" display="inline"><mml:mi mathvariant="italic">α</mml:mi></mml:math></inline-formula> : <inline-formula><mml:math id="M267" display="inline"><mml:mrow><mml:mi mathvariant="italic">β</mml:mi><mml:mo>=</mml:mo></mml:mrow></mml:math></inline-formula> 10–20 for
AUC, suggesting that more weight needs to be given to <inline-formula><mml:math id="M268" display="inline"><mml:mrow><mml:msub><mml:mi>V</mml:mi><mml:mi mathvariant="normal">post</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> to
successfully identify landslides, particularly when bulk performance over
the full ROC curve is of primary concern.</p>
      <p id="d1e4057">The <inline-formula><mml:math id="M269" display="inline"><mml:mi mathvariant="italic">α</mml:mi></mml:math></inline-formula> : <inline-formula><mml:math id="M270" display="inline"><mml:mi mathvariant="italic">λ</mml:mi></mml:math></inline-formula> ratio controls the influence of change in NDVI
(d<inline-formula><mml:math id="M271" display="inline"><mml:mi>V</mml:mi></mml:math></inline-formula>) relative to the likelihood that the d<inline-formula><mml:math id="M272" display="inline"><mml:mi>V</mml:mi></mml:math></inline-formula> values in the post-event stack are
significantly different from those in the pre-event stack (<inline-formula><mml:math id="M273" display="inline"><mml:mrow><mml:msub><mml:mi>P</mml:mi><mml:mi mathvariant="normal">t</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>). As explained
above, ALDI is dominated by <inline-formula><mml:math id="M274" display="inline"><mml:mrow><mml:msub><mml:mi>P</mml:mi><mml:mi mathvariant="normal">t</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> at higher <inline-formula><mml:math id="M275" display="inline"><mml:mi mathvariant="italic">α</mml:mi></mml:math></inline-formula> : <inline-formula><mml:math id="M276" display="inline"><mml:mi mathvariant="italic">λ</mml:mi></mml:math></inline-formula> ratios and
by d<inline-formula><mml:math id="M277" display="inline"><mml:mi>V</mml:mi></mml:math></inline-formula> at lower ratios. ALDI performance is somewhat sensitive to this parameter
for both TPR<inline-formula><mml:math id="M278" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">diff</mml:mi></mml:msub></mml:math></inline-formula> and AUC, with gentle but consistent slopes to the
upper-bound performances (Fig. 3, column c). Best performances are found
for <inline-formula><mml:math id="M279" display="inline"><mml:mi mathvariant="italic">α</mml:mi></mml:math></inline-formula> : <inline-formula><mml:math id="M280" display="inline"><mml:mi mathvariant="italic">λ</mml:mi></mml:math></inline-formula> in the range 0.01–1 for TPR<inline-formula><mml:math id="M281" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">diff</mml:mi></mml:msub></mml:math></inline-formula> and 0.1–5 for
AUC, suggesting that, although both layers contribute important information,
d<inline-formula><mml:math id="M282" display="inline"><mml:mi>V</mml:mi></mml:math></inline-formula> is a stronger predictor than <inline-formula><mml:math id="M283" display="inline"><mml:mrow><mml:msub><mml:mi>P</mml:mi><mml:mi mathvariant="normal">t</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> for the Gorkha case study.</p>
      <?pagebreak page494?><p id="d1e4184">Optimum parameters for the Gorkha study site differ slightly between
performance metrics (compare histograms down columns in Fig. 3). This
reflects the different focus of the metrics, where TPR<inline-formula><mml:math id="M284" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">diff</mml:mi></mml:msub></mml:math></inline-formula> gives the
strongest weight to very conservative (i.e. low FPR) classification
thresholds (Fig. 3, rows 1–2), and AUC weights all classification
thresholds equally (Fig. 3, rows 3–4). In general, the parameters to which
ALDI performance is most sensitive are also those for which optimum values
are most robust to changes in check dataset or performance metric. For
example, there is negligible change in optimum values for <inline-formula><mml:math id="M285" display="inline"><mml:mrow><mml:msub><mml:mi>L</mml:mi><mml:mi mathvariant="normal">post</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and
<inline-formula><mml:math id="M286" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">snow</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> across the range of metrics and datasets. <inline-formula><mml:math id="M287" display="inline"><mml:mi mathvariant="italic">α</mml:mi></mml:math></inline-formula> : <inline-formula><mml:math id="M288" display="inline"><mml:mi mathvariant="italic">β</mml:mi></mml:math></inline-formula> and
<inline-formula><mml:math id="M289" display="inline"><mml:mi mathvariant="italic">α</mml:mi></mml:math></inline-formula> : <inline-formula><mml:math id="M290" display="inline"><mml:mi mathvariant="italic">λ</mml:mi></mml:math></inline-formula> are both broadly comparable between metrics, although in
both cases there is a shift towards higher optimum values for AUC,
indicating that for this metric NDVI difference is less important than it
was for TPR<inline-formula><mml:math id="M291" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">diff</mml:mi></mml:msub></mml:math></inline-formula> (noting that the improvement is always <inline-formula><mml:math id="M292" display="inline"><mml:mi mathvariant="italic">&lt;</mml:mi></mml:math></inline-formula> 3%). <inline-formula><mml:math id="M293" display="inline"><mml:mi mathvariant="italic">α</mml:mi></mml:math></inline-formula> : <inline-formula><mml:math id="M294" display="inline"><mml:mi mathvariant="italic">β</mml:mi></mml:math></inline-formula> has a progressively less clear optimum as metrics
become more generalised (from TPR<inline-formula><mml:math id="M295" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">diff</mml:mi></mml:msub></mml:math></inline-formula> to AUC) indicating reduced
parameter sensitivity for AUC. <inline-formula><mml:math id="M296" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">cloud</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M297" display="inline"><mml:mrow><mml:msub><mml:mi>L</mml:mi><mml:mrow><mml:mi>p</mml:mi><mml:mi>r</mml:mi><mml:mi>e</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> have larger changes
in optimised parameters between the metrics, although the sensitivity to
these changes is small in performance terms (Fig. 3, columns e–f). Optimum
<inline-formula><mml:math id="M298" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">cloud</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is 0.7 for TPR<inline-formula><mml:math id="M299" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">diff</mml:mi></mml:msub></mml:math></inline-formula> but 0.5 for AUC; optimum <inline-formula><mml:math id="M300" display="inline"><mml:mrow><mml:msub><mml:mi>L</mml:mi><mml:mi mathvariant="normal">pre</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is in
the range 2–5 for TPR<inline-formula><mml:math id="M301" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">diff</mml:mi></mml:msub></mml:math></inline-formula> and 5–10 for AUC. ALDI performance is
insensitive to <inline-formula><mml:math id="M302" display="inline"><mml:mi mathvariant="italic">α</mml:mi></mml:math></inline-formula>, varying by <inline-formula><mml:math id="M303" display="inline"><mml:mi mathvariant="italic">&lt;</mml:mi></mml:math></inline-formula> 10 % across the parameter
range for all metrics, generating a broad histogram of best-performing
parameter values and showing large shifts in the optimum value depending on both
the metric and the dataset used to assess performance (Fig. 3, column a).</p>
</sec>
<sec id="Ch1.S4.SS3">
  <label>4.3</label><title>ALDI calibration: global comparison</title>
      <p id="d1e4377">We focus our global comparison on the AUC performance metric. Results for
TPR<inline-formula><mml:math id="M304" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">diff</mml:mi></mml:msub></mml:math></inline-formula> are very similar and can be found in the Supplement (Figs. S1–S6). Figure 4 shows that optimum values for a given
parameter differ between sites; that sensitive parameters at one site are
usually sensitive at others; and that absolute performance differences
between different inventories at a site can be large, although the trends
are generally similar.</p>
      <p id="d1e4389">ALDI is sensitive to <inline-formula><mml:math id="M305" display="inline"><mml:mrow><mml:msub><mml:mi>L</mml:mi><mml:mi mathvariant="normal">post</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> for all sites but with trends that differ
between sites: for Haiti and Gorkha a value of 1 year is best, 2 years is
reasonable, and 3 years is poor. For Kashmir and Wenchuan a value of 1 year is
best, but a value of 2 years also gives reasonable results. For Aysén a value of 5 years is best, and
a value of 1 year is particularly poor (Fig. 4, column g). An <inline-formula><mml:math id="M306" display="inline"><mml:mrow><mml:msub><mml:mi>L</mml:mi><mml:mi mathvariant="normal">post</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> of 2 years
generally results in fairly good performances for all five sites. These
site-by-site differences suggest a connection between the optimum time
series length <inline-formula><mml:math id="M307" display="inline"><mml:mrow><mml:msub><mml:mi>L</mml:mi><mml:mi mathvariant="normal">post</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, the frequency of Landsat image acquisition during
the study period, and the processes that cause NDVI change at different
sites (e.g. vegetation growth rates, fire, drought, or post-seismic
landsliding). While this does not preclude good performance of ALDI using a
global-parameter set, it does imply that performance with this global-parameter set will almost always be sub-optimal relative to a
locally calibrated set. However, such local calibration requires independent
landslide mapping over at least part of the study area. Further work might
seek to connect optimum parameters at a site with its image and landscape
characteristics, enabling a refinement of the parameters without the need for
additional mapping.</p>
      <?pagebreak page495?><p id="d1e4425">ALDI is sensitive to <inline-formula><mml:math id="M308" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">snow</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> in three of the five sites and particularly
for Aysén, but in all cases <inline-formula><mml:math id="M309" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">snow</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> of 0.5–0.8 results in performances
that are at least close to optimum (Fig. 4, column d). ALDI is only weakly
sensitive to <inline-formula><mml:math id="M310" display="inline"><mml:mrow><mml:msub><mml:mi>L</mml:mi><mml:mi mathvariant="normal">pre</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> for all sites and with subtly differing trends: for
Kashmir a value of 3 years is best; for Wenchuan and Haiti a value of 10 years is best; and for
Aysén and Gorkha best performances are in the range of 5 to 10 years
(Fig. 4, column f). However, the trends are not linear, and an <inline-formula><mml:math id="M311" display="inline"><mml:mrow><mml:msub><mml:mi>L</mml:mi><mml:mi mathvariant="normal">pre</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> of 5 years generally results in fairly good performances for all five sites.
ALDI is generally insensitive to <inline-formula><mml:math id="M312" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">cloud</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> across the range 0.3–0.7 with
best performances consistently found at 0.5, although these are at most
10 % better than those for other values in the range (Fig. 4, column e).
ALDI is insensitive to <inline-formula><mml:math id="M313" display="inline"><mml:mi mathvariant="italic">α</mml:mi></mml:math></inline-formula> alone but is strongly sensitive to <inline-formula><mml:math id="M314" display="inline"><mml:mi mathvariant="italic">α</mml:mi></mml:math></inline-formula> : <inline-formula><mml:math id="M315" display="inline"><mml:mi mathvariant="italic">β</mml:mi></mml:math></inline-formula> and weakly sensitive to <inline-formula><mml:math id="M316" display="inline"><mml:mi mathvariant="italic">α</mml:mi></mml:math></inline-formula> : <inline-formula><mml:math id="M317" display="inline"><mml:mi mathvariant="italic">λ</mml:mi></mml:math></inline-formula> at all sites (Fig. 4, columns a–c) with best performances found for <inline-formula><mml:math id="M318" display="inline"><mml:mi mathvariant="italic">α</mml:mi></mml:math></inline-formula> : <inline-formula><mml:math id="M319" display="inline"><mml:mi mathvariant="italic">β</mml:mi></mml:math></inline-formula> in the
range 1–100.</p>
      <p id="d1e4534">ALDI application would be both faster and simpler if single optimum values
could be used for the three pre-processing parameters within Google Earth
Engine (<inline-formula><mml:math id="M320" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">cloud</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M321" display="inline"><mml:mrow><mml:msub><mml:mi>L</mml:mi><mml:mi mathvariant="normal">pre</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M322" display="inline"><mml:mrow><mml:msub><mml:mi>L</mml:mi><mml:mi mathvariant="normal">post</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>). In particular, the shorter
post-event window <inline-formula><mml:math id="M323" display="inline"><mml:mrow><mml:msub><mml:mi>L</mml:mi><mml:mi mathvariant="normal">post</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is, the sooner an inventory following an earthquake can be compiled. Our site-by-site calibration suggests that it is
possible to find single values for these parameters that result in good
performance for all study sites (Fig. 4). This is the case when cloud
threshold <inline-formula><mml:math id="M324" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">cloud</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is 0.5, pre-earthquake stack length <inline-formula><mml:math id="M325" display="inline"><mml:mrow><mml:msub><mml:mi>L</mml:mi><mml:mi mathvariant="normal">pre</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is 5 years, and post-earthquake stack length <inline-formula><mml:math id="M326" display="inline"><mml:mrow><mml:msub><mml:mi>L</mml:mi><mml:mi mathvariant="normal">post</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is 2 years (thus it is
reasonable to expect that an ALDI-derived inventory can be generated after 2 years). We also examined performance when these parameters were allowed to
vary but found that the performance improvement for the global-parameter set
was negligible.</p>
      <p id="d1e4616">To examine similarity between locally optimised parameters and compare them
to a global set of parameter sets, we first identified the best 100 parameter sets for each study site, using AUC as the performance metric
(Fig. 5). To generate the global-parameter sets we held <inline-formula><mml:math id="M327" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">cloud</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>,
<inline-formula><mml:math id="M328" display="inline"><mml:mrow><mml:msub><mml:mi>L</mml:mi><mml:mi mathvariant="normal">pre</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, and <inline-formula><mml:math id="M329" display="inline"><mml:mrow><mml:msub><mml:mi>L</mml:mi><mml:mi mathvariant="normal">post</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> constant at 0.5, 5, and 2 years, respectively;
then, treating the remaining parameter sets as four-element vectors, we sampled
the best 20 parameters from each site; finally, we generated a holdback
parameter set for each site by removing that site's parameters from the
global set. Locally optimised parameter sets (grey histograms in Fig. 5)
are broadly consistent with the global set (blue histograms) with a small
number of exceptions: <inline-formula><mml:math id="M330" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">snow</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> should be set lower for Kashmir and higher
for Aysén; <inline-formula><mml:math id="M331" display="inline"><mml:mi mathvariant="italic">α</mml:mi></mml:math></inline-formula> : <inline-formula><mml:math id="M332" display="inline"><mml:mi mathvariant="italic">β</mml:mi></mml:math></inline-formula> should be set higher for Kashmir; and <inline-formula><mml:math id="M333" display="inline"><mml:mi mathvariant="italic">α</mml:mi></mml:math></inline-formula> : <inline-formula><mml:math id="M334" display="inline"><mml:mi mathvariant="italic">λ</mml:mi></mml:math></inline-formula> should be set lower for Gorkha. These differences are accentuated in the
holdback distributions (the black outlined histograms) because the divergent
local parameter values are stripped from the set, pulling the distributions
away from their local optima. We would expect larger performance degradation
from local to global to holdback parameter sets at sites where these
distributions are more different.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F5" specific-use="star"><?xmltex \currentcnt{5}?><?xmltex \def\figurename{Figure}?><label>Figure 5</label><caption><p id="d1e4694">Posterior parameter distributions for the four parameters external
to Google Earth Engine after global optimisation (top row) and local
optimisation for each earthquake. Rows 2–6 show posterior frequency
distributions for each ALDI parameter following local optimisation (grey
bars) and the holdback parameter set derived from the global set excluding
locally optimised parameters (hollow bars).</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/22/481/2022/nhess-22-481-2022-f05.png"/>

        </fig>

      <p id="d1e4703">ALDI with locally optimised parameters always outperforms the global
parameters, and the global parameters always outperform the holdback
parameters (Table 3). The difference between local and global parameters is
generally larger than between global and holdback parameters. In fact,
performance reduction from global to holdback parameters is always <inline-formula><mml:math id="M335" display="inline"><mml:mi mathvariant="italic">&lt;</mml:mi></mml:math></inline-formula> 1 % for AUC. This indicates that the five study sites provide an
adequately varied calibration set to enable the generation of a general
parameter set that is not overly influenced by any one site. This is
encouraging for future blind ALDI application. However, the difference in
performance between local and global parameters shows that local
optimisation can improve ALDI performance in terms of AUC by up to 9 %
(and by 2 % on average). In three cases, one for Kashmir and two for
Gorkha, local optimisation improves ALDI to the point where it is no longer
outperformed by the manually mapped competitor inventory but instead
outperforms it in terms of identifying landslide locations in the check
inventory. This is somewhat consistent with the observed divergence of
locally optimised parameter distributions from the global distribution at
these sites (Fig. 5). However, it likely also reflects the broadly similar
performance (i.e. skill) of ALDI and manual mapping at the sites (Table 3).</p>
</sec>
<sec id="Ch1.S4.SS4">
  <label>4.4</label><title>Spatial agreement: global comparison to manual mapping</title>
      <p id="d1e4721">Spatial agreement between manual landslide inventories is surprisingly low
not only for the Gorkha study site shown in Fig. 2 but across all sites.
TPRs range from 0.08 to 0.8 indicating that at best 80 % and at worst 8 %
of the landslide area mapped by one inventory is also identified as a
landslide by a second test inventory (Fig. 6a and Table 3). FPRs range
from 0.0003 to 0.03, indicating that at best 0.03 % and at worst 3 % of the
area that is identified as a non-landslide area in one inventory is instead
identified as a landslide by a second test inventory. There are two possible
reasons why FPRs are so much lower than TPRs: (1) landslide density is low,
so there are few positives (TP<inline-formula><mml:math id="M336" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>FN) and many negatives (TN <inline-formula><mml:math id="M337" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> FP) – these are
the denominators of TPR and FPR, respectively, amplifying TPR and damping
FPR – and (2) landslide mappers may be inherently conservative, mapping only
features that they are confident are landslides. TPRs and FPRs are
positively correlated but with considerable scatter (Fig. 6a). In some
cases manual maps agree quite closely: for example, the inventories of Gorum
et al. (2013) and Harp et al. (2016) for Haiti (<inline-formula><mml:math id="M338" display="inline"><mml:mrow><mml:msub><mml:mi>H</mml:mi><mml:mi mathvariant="normal">GH</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M339" display="inline"><mml:mrow><mml:msub><mml:mi>H</mml:mi><mml:mi mathvariant="normal">HG</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) or those
of Zhang et al. (2016) and Watt (2016) for Gorkha (<inline-formula><mml:math id="M340" display="inline"><mml:mrow><mml:msub><mml:mi>G</mml:mi><mml:mi mathvariant="normal">ZW</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M341" display="inline"><mml:mrow><mml:msub><mml:mi>G</mml:mi><mml:mi mathvariant="normal">WZ</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>).
These cases have a relatively high TPR given their FPR and plot towards the
top left of the point cloud in ROC space (Fig. 6a). In other cases the
agreement is weaker, such as between the inventories of Li et al. (2014) and
Xu et al. (2014) for Wenchuan (<inline-formula><mml:math id="M342" display="inline"><mml:mrow><mml:msub><mml:mi>W</mml:mi><mml:mi mathvariant="normal">LX</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M343" display="inline"><mml:mrow><mml:msub><mml:mi>W</mml:mi><mml:mi mathvariant="normal">XL</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>), or those of Sato et al. (2007) and Basharat et al. (2016) for Kashmir (<inline-formula><mml:math id="M344" display="inline"><mml:mrow><mml:msub><mml:mi>K</mml:mi><mml:mi mathvariant="normal">SB</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M345" display="inline"><mml:mrow><mml:msub><mml:mi>K</mml:mi><mml:mi mathvariant="normal">BS</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>). There is
a symmetry to the inventory comparison because each inventory takes a turn
as the competitor dataset (to which ALDI is being compared) and as the<?pagebreak page496?> check
dataset (against which both are evaluated). As a result, a single pairwise
comparison results in two points in Fig. 6a reflecting the switching of
roles. The three-way comparison for the Gorkha earthquake results in three
pairwise comparisons and six points. When one inventory is considerably more
complete and less conservative, then the separation between pairs of points
will be large (e.g. Watt and Zhang for Gorkha). Zhang et al. (2017)
reported, in their metadata, that their inventory is incomplete and focuses
on the largest landslides, while that of Watt (2016) was more complete and
less conservative. As a result Zhang et al. (2016) successfully identified
only 10 % of the landslide pixels identified by Watt (2016) but identified
only a tiny fraction (<inline-formula><mml:math id="M346" display="inline"><mml:mi mathvariant="italic">&lt;</mml:mi></mml:math></inline-formula> 0.1 %) of the study area as landslides
when Watt (2016) considered that they were not (<inline-formula><mml:math id="M347" display="inline"><mml:mrow><mml:msub><mml:mi>G</mml:mi><mml:mi mathvariant="normal">ZW</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> in Fig. 6a).
Conversely, Watt (2016) successfully identified 80 % of the landslides
identified by Zhang et al. (2016) but identified a further 1 % of
the study area as landslides that were not identified as such by Zhang et
al. (2016) (<inline-formula><mml:math id="M348" display="inline"><mml:mrow><mml:msub><mml:mi>G</mml:mi><mml:mi mathvariant="normal">WZ</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> in Fig. 6a).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F6" specific-use="star"><?xmltex \currentcnt{6}?><?xmltex \def\figurename{Figure}?><label>Figure 6</label><caption><p id="d1e4859"><bold>(a)</bold> TPR and FPR pairs for the 14 inventory cross comparisons. Open
symbols are calculated from a pixel-based analysis at 30 m resolution; solid
symbols are calculated from an object-based analysis using mapped polygons.
The grey line shows the naïve (random) 1 : 1 relationship. Note the
difference in <inline-formula><mml:math id="M349" display="inline"><mml:mi>x</mml:mi></mml:math></inline-formula>- and <inline-formula><mml:math id="M350" display="inline"><mml:mi>y</mml:mi></mml:math></inline-formula>-axis scales for this and all other panels. <bold>(b)</bold>–<bold>(f)</bold> ROC
curves for ALDI for each case study. There are three ROC curves for ALDI
evaluated against each check inventory (e.g. <inline-formula><mml:math id="M351" display="inline"><mml:mrow><mml:msub><mml:mi>K</mml:mi><mml:mi mathvariant="normal">SB</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) all with the same
line style (solid or dashed). In every case the upper curve is from ALDI
with locally optimised parameters; the middle curve (indicated with an
arrowed end) is from ALDI with global parameters; and the lower curve is from
ALDI with holdback parameters. The global and holdback curves are
indistinguishable in almost all cases. Red lines indicate the value of
TPR<inline-formula><mml:math id="M352" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">diff</mml:mi></mml:msub></mml:math></inline-formula>, the difference in TPR between ALDI and the competitor
inventory when both are evaluated using the same check inventory. Legend
acronyms indicate the study site (e.g. <inline-formula><mml:math id="M353" display="inline"><mml:mi>K</mml:mi></mml:math></inline-formula>) with the check and then
competitor inventory labels as subscripts; see Table 3.</p></caption>
          <?xmltex \igopts{width=426.791339pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/22/481/2022/nhess-22-481-2022-f06.png"/>

        </fig>

      <?pagebreak page497?><p id="d1e4918"><?xmltex \hack{\newpage}?>To evaluate ALDI performance relative to manual mapping, we compare the
ability of ALDI to successfully identify more landslide pixels in one
(check) inventory than another (competitor) inventory when ALDI output is
thresholded to reproduce the FPR of the competitor inventory. This TPR
difference (TPR<inline-formula><mml:math id="M354" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">diff</mml:mi></mml:msub></mml:math></inline-formula>) is shown as a red line in Fig. 6b–f; positive
differences indicate that ALDI outperforms manual mapping and vice versa.
ALDI outperforms manual mapping in the majority of cases when parameters
are locally optimised (10 of 14 cases, Fig. 6 and Table 3) and is
comparable to manual mapping when a single global-parameter set is applied
to all study sites (8 of 14 cases). Performance is only slightly reduced
when the test site is held back from the global optimisation, and ALDI
continues to outperform manual mapping in 8 of 14 cases.</p>
      <p id="d1e4932">ALDI performs better at some sites than others, with performances for Aysén
and Gorkha particularly good (Table 3). Performance is poor for Haiti, both
in absolute terms and relative to the manual mapping. For AUC, an indicator
of absolute performance, ALDI performance for the Haiti case is ranked
10th–11th of 14 (where the range results from combining local, global, or holdback tests). Relative to manual mapping, ALDI correctly
identifies 51 %–74 % fewer landslide pixels for the same FPR. Explanations
for these performance differences are discussed in Sect. 5.4. ALDI in
Wenchuan performs only moderately in absolute terms, with ranked
performances in the range 9th to 12th out of 14 for AUC, but
outperforms manual mapping (1st and 4th for TPR<inline-formula><mml:math id="M355" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">diff</mml:mi></mml:msub></mml:math></inline-formula>) as a
result of the relatively poor agreement between manual maps for the site.
Kashmir has very marked differences in ALDI performance depending on the
test dataset (all <inline-formula><mml:math id="M356" display="inline"><mml:mi mathvariant="italic">&lt;</mml:mi></mml:math></inline-formula> 4th of 14 for Sato et al., 2007; all <inline-formula><mml:math id="M357" display="inline"><mml:mi mathvariant="italic">&gt;</mml:mi></mml:math></inline-formula> 9th of 14 for Basharat et al., 2016), illustrating the
difficulty of interpreting performance relative to check data when the check
data themselves contain errors of similar magnitude to the data being
tested.</p>
</sec>
<?pagebreak page498?><sec id="Ch1.S4.SS5">
  <label>4.5</label><title>Area–frequency distributions</title>
      <p id="d1e4967">Probability density functions (PDFs) for manually mapped landslide areas (Fig. 7a–e) follow a consistent distribution with a roll-over and a heavy right
tail that is approximately linear in logarithmic space but that usually has
positive (convex up) curvature or a roll-off at very large areas. These
characteristics have already been widely reported both for the study
inventories in particular (e.g. Gorum et al., 2013; Li et al., 2014; Roback
et al., 2018) and for many other landslide inventories worldwide (e.g.
Tanyaş et al., 2019). Different inventories for the same study site show
broadly consistent scaling in their right tail but tend to differ markedly
in the location of the roll-over, modal size, degree of curvature in their
right tail, and the location (and presence) of a roll-off for very large
areas (e.g. Fig. 7a, d, and e). These differences, as well as their possible
explanations, have also been widely reported for these and other sites (see
review by Tanyaş et al., 2019).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F7" specific-use="star"><?xmltex \currentcnt{7}?><?xmltex \def\figurename{Figure}?><label>Figure 7</label><caption><p id="d1e4972">Empirical area–frequency distributions for manually mapped and
classified landslides for the five case studies. Manually mapped PDFs are
calculated from areas of mapped polygons; resampled PDFs are calculated from
patch areas generated from the mapped polygons resampled to a 30 m grid; and
classified PDFs are calculated from clustered pixel areas generated by
thresholding the ALDI classification values.</p></caption>
          <?xmltex \igopts{width=426.791339pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/22/481/2022/nhess-22-481-2022-f07.png"/>

        </fig>

      <p id="d1e4981">The area–frequency distributions derived from ALDI reflect the sizes of
clustered landslide-affected areas (rather than the areas of landslide
objects themselves). The ALDI-based distributions generally exhibit a
broadly similar right tail to those of the manually mapped distributions;
both have heavy right tails that closely approximate a power law and have
similar scaling (i.e. slope in logarithmic space) in that right tail.
However, the ALDI-based distributions are clearly different from those
derived from manual mapping, and they lack the following: (1) the roll-over at small areas (in
all cases, Fig. 7a–e), (2) the positive curvature to the right tail
(particularly clear for Haiti, Fig. 7d), and (3) the roll-off at very large
areas (resulting in oversampling of landslides <inline-formula><mml:math id="M358" display="inline"><mml:mi mathvariant="italic">&gt;</mml:mi></mml:math></inline-formula> 10<inline-formula><mml:math id="M359" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">5</mml:mn></mml:msup></mml:math></inline-formula> m<inline-formula><mml:math id="M360" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula>
for Wenchuan, Fig. 7c).</p>
      <p id="d1e5010">These differences can be explained in terms of amalgamation and censoring.
The amalgamation of multiple neighbouring landslides increases the frequency of
large landslides, fattening the right tail (Marc and Hovius, 2015) and in
some cases considerably increasing the size of the largest landslide (e.g.
Aysén and Wenchuan, Fig. 7b–c). Resampling to a 30 m grid makes it
impossible to record landslides smaller than a single pixel (i.e. 900 m<inline-formula><mml:math id="M361" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula>), censoring them from the area–frequency distribution.</p>
      <p id="d1e5022">To illustrate the role of amalgamation and censoring we convert the manual
landslide maps to binary grids at 30 m resolution, using a majority area
rule to identify landslide-affected pixels, and perform the same connected-component clustering used for ALDI. Resampling to 30 m should result in
strong censoring and some amalgamation as explained above. Re-clustering
with a connected-component algorithm likely results in further
amalgamation. Figure 7 shows that resampling and re-clustering
manually mapped landslides transforms their area–frequency distributions,
removing the roll-over and resulting in distributions that are very similar
to those for landslide pixels classified with ALDI. This supports our
interpretation that the misfit between ALDI and manual mapping is due to
censoring and amalgamation, although we are unable to determine their
relative roles. Misfits due to the resolution of Landsat and thus the
classification surface are difficult to overcome, whereas improvements in
clustering could be more easily implemented.</p>
</sec>
</sec>
<sec id="Ch1.S5">
  <label>5</label><title>Discussion</title>
<sec id="Ch1.S5.SS1">
  <label>5.1</label><title>The problem of testing landslide location against uncertain check data</title>
      <p id="d1e5042">The TPR<inline-formula><mml:math id="M362" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">diff</mml:mi></mml:msub></mml:math></inline-formula> results for the five study sites show that ALDI
outperforms manual mapping in 8 of 14 inventories in terms of its ability
to identify landslide-affected areas identified in a second check inventory.
This may indicate that ALDI is more skilful than each of these inventories
at identifying the locations of landslides. However, because the check
inventories are themselves known to contain error, this is not a secure
result; erroneous outperformance by ALDI would result if it identified the
same artefacts that had been (erroneously) mapped in the check dataset but
not in the competitor.</p>
      <p id="d1e5054">A more secure result can be obtained from the four (of seven) inventory
pairs where ALDI outperforms both inventories in the pair when the other is
used as check data. This indicates that the ALDI output is more similar to
each inventory than the inventories are to one another (Table 3) and
demonstrates that ALDI must be more skilful than at least one of the
inventories (either the check or competitor inventory) in identifying the
locations of landslides. However, we are still unable to conclude whether
ALDI is better than one or both inventories or identify which inventory is
better. This is because errors in a single inventory influence the result
both when it is used as the predictor (i.e. as a competitor against ALDI)
and the check dataset (against which both are evaluated).</p>
</sec>
<sec id="Ch1.S5.SS2">
  <label>5.2</label><title>Spatial disagreement in manually mapped inventories reflects processing
errors, not solely mapping errors</title>
      <p id="d1e5065">Our findings on the large locational mismatch between co-seismic landslide
inventories are initially surprising, given the widespread assumption that
such inventories represent a ground truth and the limited attempts to
propagate these errors into hazard maps, classification tests, process
inferences, or landslide rate estimates. However, the limited number of
other studies that do quantify landslide inventory error all suggest very
weak spatial agreement between landslide inventories (Ardizzone et al.,
2002; Galli et al., 2008; Fan et al., 2019).</p>
      <p id="d1e5068">The process of generating a landslide inventory from satellite imagery
involves choosing which images to map from and how to post-process and
georeference them before landslides can be identified and delineated by a
human mapper. Thus, the comparison of two inventories is not a<?pagebreak page499?> direct test
of the consistency with which human mappers detect and delineate landslides
but instead the consistency with which different research groups generate
landslide inventory maps. As an illustration of this distinction, Fan et al. (2019) found that landslide inventories had an overlap of 67 %–86 % (and
76 % on average) when comparing between mappers in the same team mapping
from the same imagery. This differs considerably from both our own results
(8 %–30 % overlap, Table 3) and other published cross-inventory comparisons
(19 %–44 % overlap, Ardizzone et al., 2002; Galli et al., 2008; Fan et al.,
2019). In these cases, the inventories being compared were published by
independent research groups and were not only collected by different mappers
without collaboration but were also generated from different sets of satellite
images. For example, Roback et al. (2018) used WorldView imagery with high
spatial resolution but which suffers from severe distortions in the Gorkha
study area due to the steep landscape and oblique look angles (Williams et
al., 2018). Even if landslides were correctly identified in both sets of
imagery, differences between inventories could be introduced during
georeferencing. Figure 8 shows evidence of the same problem for the Wenchuan
inventories, where two sets of mapped landslides with strikingly similar
patterns are offset by <inline-formula><mml:math id="M363" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 1 km. These georeferencing errors are
difficult to attribute to a single inventory and appear to vary in magnitude
and direction even over quite short length scales within an inventory
(Figs. 2 and 8). Thus, improved performance of ALDI relative to a
particular inventory reflects an improved overall workflow rather than
specifically the ability to identify landslides in images.</p>

      <?xmltex \floatpos{p}?><fig id="Ch1.F8" specific-use="star"><?xmltex \currentcnt{8}?><?xmltex \def\figurename{Figure}?><label>Figure 8</label><caption><p id="d1e5080">Manually mapped landslides and ALDI classifier results for the
Wenchuan study site. <bold>(a)</bold> Mapped landslides at the scale of the full study
area with AOIs shown in grey; Xu and Li refer to the inventories of Xu et
al. (2014) and Li et al. (2014), respectively. <bold>(b)</bold> ALDI values for the full
study area. <bold>(c)</bold> Mapped landslides and <bold>(d)</bold> ALDI values for a subset of the
study area. <bold>(e)</bold> Detailed view of mapped landslides overlain on ALDI values.
Yellow boxes in each panel show the locations of nested panels (e.g. <bold>c</bold> in
<bold>a</bold> and <bold>d</bold> in <bold>b</bold>). Thicker outlines in panel <bold>(e)</bold> indicate landslides of very
similar geometry that are offset by <inline-formula><mml:math id="M364" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 1 km in the different
inventories; the ALDI pattern suggests that the map by Xu et al. (2014) is
more likely to be correctly georeferenced in this case.</p></caption>
          <?xmltex \igopts{width=398.338583pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/22/481/2022/nhess-22-481-2022-f08.png"/>

        </fig>

</sec>
<sec id="Ch1.S5.SS3">
  <label>5.3</label><title>Limitations to ALDI performance</title>
      <?pagebreak page501?><p id="d1e5135">ALDI performance varies from site to site, with particularly good
performances for Aysén and Gorkha but particularly poor ones for Haiti. The
overall poor performance for Haiti may reflect the drier conditions in the
study area, which lead to vegetation that is more difficult to differentiate
from landslide scars, or the higher degree of human influence on land cover
relative to other sites, which may result in more vegetation changes not
related to landslides. ALDI can identify landslides only in areas where they
result in a change in NDVI and will perform better in areas where this
change is more pronounced (all else being equal). This will occur where
pre-event NDVI is higher due to denser and/or more vigorous vegetation
coverage, both of which result in a larger share of reflectance from leaves,
with their more pronounced “red edge” (the red–near-infrared reflectance
change). Conversely, ALDI will perform poorly in areas with sparse
vegetation such as the epicentral area of the 2010 Sierra Cucapah earthquake
(Barlow et al., 2015).</p>
      <p id="d1e5138">Poor performance for Haiti in comparison with the manual mapping may also be
due to ALDI's coarse 30 m resolution relative to the dimensions of the
landslides in the study area. ALDI will identify a pixel as landslide-affected only if the landslide occupies enough of the pixel to alter its
spectral response and will perform better when landslides are large enough
to occupy large fractions of one or many pixels. Given their typically
elongate shape (Taylor et al., 2018), landslides with widths <inline-formula><mml:math id="M365" display="inline"><mml:mi mathvariant="italic">&lt;</mml:mi></mml:math></inline-formula> 30 m
and thus areas <inline-formula><mml:math id="M366" display="inline"><mml:mi mathvariant="italic">&lt;</mml:mi></mml:math></inline-formula> 2700 m<inline-formula><mml:math id="M367" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula> (assuming <inline-formula><mml:math id="M368" display="inline"><mml:mrow><mml:mi>L</mml:mi><mml:mo>/</mml:mo><mml:mi>W</mml:mi><mml:mo>=</mml:mo></mml:mrow></mml:math></inline-formula> 3, 75th
percentile from Taylor et al., 2018) will be partially censored, with the
degree of censoring increasing as width declines. Median landslide area in
the inventories examined here ranges from 250 m<inline-formula><mml:math id="M369" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula> for Haiti (Harp et
al., 2016) to 19 000 m<inline-formula><mml:math id="M370" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula> for Kashmir (Basharat et al., 2016), with
medians less than 2700 m<inline-formula><mml:math id="M371" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula> in 4 of 14 inventories. Therefore, this
censoring will strongly affect ALDI-derived inventories, particularly in
areas with lower relief (such as Haiti) where smaller landslides are
expected to be more common (Jeandet et al., 2019).</p>
      <p id="d1e5206">Finally, poor performance for Haiti is also likely to reflect the limited
number and quality of Landsat images acquired over the study area. ALDI used
imagery from 2005–2012 to identify landslides triggered by the Haiti
earthquake and thus relies exclusively on Landsat 5 and Landsat 7 data (Landsat 8
launched in 2013). Both Landsat 5 and Landsat 7 are problematic for this study site
and period. All of the Landsat 7 data contain data gaps due to Scan Line
Corrector (SLC) failure from June 2003 onwards, and only small amounts of
Landsat 5 data for areas outside the USA were retained during this period,
limiting archival imagery in some areas (see Fig. S5 in Pekel et al.,
2016). For Haiti the pre-earthquake stack is composed of 6 Landsat 5 images
and 205 Landsat 7 images and the post-earthquake stack of 16 and 91 images,
respectively. Limited availability of Landsat 5 data at this site means that
in some areas the classifier relies exclusively on Landsat 7 and is thus
unable to calculate an ALDI value for pixels within the data gaps (these are
visible as white stripes in the eastern half of Fig. 9b). While some areas
of high ALDI values show good agreement with mapped landslides, there are
also large patches of high ALDI values with complex shapes that are
uncharacteristic of landslides and that manual mapping shows as likely false
positives (Fig. 9c).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F9" specific-use="star"><?xmltex \currentcnt{9}?><?xmltex \def\figurename{Figure}?><label>Figure 9</label><caption><p id="d1e5212">Mapped landslides and the ALDI classifier for the Haiti (left) and
Hokkaido (right) study sites. <bold>(a)</bold> Mapped landslides from Harp et al. (2016)
in Haiti at the scale of the full study area with the associated AOI shown
in grey. <bold>(b)</bold> ALDI values for the full study area; the yellow box shows the
location of panel <bold>(c)</bold>. <bold>(c)</bold> ALDI values overlain by mapped landslides from Harp
et al. (2016) for a subset of the study area. <bold>(d)</bold> Mapped landslides from Wang
et al. (2019) in Hokkaido at the scale of the full study area with the
associated AOI shown in grey. <bold>(e)</bold> ALDI values for the full study area. The
yellow box shows the location of panel <bold>(f)</bold>. <bold>(f)</bold> ALDI values overlain by mapped
landslides from Wang et al. (2019) for a subset of the study area. ALDI uses
Landsat 5 and Landsat 7 for Haiti and Sentinel-2 for Hokkaido, both gridded
at 30 m resolution.</p></caption>
          <?xmltex \igopts{width=497.923228pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/22/481/2022/nhess-22-481-2022-f09.png"/>

        </fig>

      <p id="d1e5246">Given these limitations to Landsat 5 and Landsat 7 imagery, it is perhaps surprising
that ALDI performs so well in the Aysén case (where the stack extends from
2002–2009). This is likely due to the larger number of Landsat 5 images
available for the study site (140 in the pre-earthquake stack and 46 in the
post-earthquake stack) and to the location of the area of densest
landsliding near the centre of a Landsat 7 image where data gaps related to
SLC failure are minimised. The 2015 Gorkha earthquake is the only case study
for which Landsat 8 data were available, perhaps explaining the relatively
good performance at this site and offering hope for application to more
recent events.</p>
      <p id="d1e5249">Sparse image data (associated with incomplete archiving of Landsat 5) and
sensor problems (primarily SLC failure on Landsat 7) from 2003–2014 suggest
ALDI-based mapping in this period should be handled with care. However, the
majority of our test earthquakes come from this period, and we have
demonstrated that even with these constraints, ALDI performs well in
determining landslide locations for four of the five case studies, both in
absolute terms and relative to manual mapping. Potential checks on ALDI
applications during this time period could entail careful checking of the
numbers of images in the pre- and post-earthquake stacks, the extent of
Landsat 7-derived striping in the ALDI map, and the size and shape of the
landslides in the ALDI-derived inventory. Small image stacks (particularly
for Landsat 5), extensive striping, and large complex landslide shapes
should all be treated as indicators of potentially poor ALDI performance.
However, even when large image stacks are available for an
earthquake-affected area, cloud cover can limit the number of usable
observations per pixel within the pre- and post-earthquake stacks.</p>
      <p id="d1e5252">ALDI can identify landslide-affected pixels with a high degree of skill
(comparable to manual mapping) but is considerably less skilful in
identifying discrete landslides, as demonstrated by the difference in ALDI
and manually mapped area–frequency distributions. As with Parker et al. (2011), additional steps are required to identify separate landslides (e.g.
Marc et al., 2016). Calibration based on a small subset of manually mapped
landslides followed by subsequent manual editing to remove false positives
could result in a very good inventory in a fraction of the time associated
with full manual mapping.</p>
</sec>
<sec id="Ch1.S5.SS4">
  <label>5.4</label><title>Strengths and weaknesses of ALDI relative to manual mapping</title>
      <p id="d1e5263">The most widely used properties of landslide inventories are landslide
location and geometry (Guzzetti et al., 2012). In terms of location, ALDI
performs comparably to manual mapping in identifying whether the majority of
each pixel in a 30 m grid is landslide-affected. However, it performs worse
in capturing landslide area–frequency distributions, primarily because it
cannot identify small isolated landslides (i.e. with areas <inline-formula><mml:math id="M372" display="inline"><mml:mi mathvariant="italic">&lt;</mml:mi></mml:math></inline-formula> 900 m<inline-formula><mml:math id="M373" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula> separated by more than 30 m), and separating the output from ALDI (or
any other pixel-based classifier) into discrete landslide objects is not
straightforward.</p>
      <p id="d1e5282">Current approaches to train and test landslide prediction models (including
hazard and susceptibility models) almost exclusively use pixel-based
information on landslide presence or absence rather than information about
the size or shape of a landslide at a particular location (see Bellugi et
al., 2015, for an exception). For such applications, skilful identification
of landslide-affected pixels is the sole requirement. Our results suggest
that the ALDI landslide inventory would<?pagebreak page502?> be an appropriate product to use in
these cases, as it is better than at least one of the manual inventories in
four of the five case studies (Table 3).</p>
      <p id="d1e5285">Landslide geometry is required to construct landslide area–frequency
distributions and is useful to distinguish landslide initiation and runout
zones (Marc et al., 2018). Manual mapping provides landslide geometry with a
high level of accuracy, although disagreements in landslide area–frequency
distributions for manually mapped inventories have already been reported,
with the most pronounced differences being in roll-over location, usually due to
differences in image resolution (Galli et al., 2008; Fan et al., 2019;
Tanyaş et al., 2019). The accuracy of landslide geometry derived from ALDI
depends strongly on the extent to which landslide pixels can be clustered to
identify separate landslides (e.g. Marc et al., 2016) and on the pixel
resolution. The first<?pagebreak page503?> of these is common to all pixel-based classifiers.
Given the relatively coarse resolution of the underlying Landsat data, we
expect ALDI-derived geometries to be accurate only for large landslides, as
shown in Fig. 7.</p>
      <p id="d1e5288">All in all, we expect ALDI to be useful in identifying areas for further
(more detailed) mapping at multiple scales: (1) globally, as a supplement to
the existing archive of co-seismic landslide inventories by examining
historic events for which a landslide inventory has never previously been
generated but where landslides are known or expected to have been triggered;
(2) at a site, to identify areas of interest or to extend the study area
beyond that which can be feasibly mapped by hand; and (3) at the finest scale, to
identify individual candidate landslides to be manually checked and
re-digitised if necessary. We also expect ALDI to be a useful check on
manual mapping, enabling increased homogeneity in areas where there is only
patchy coverage of high-resolution imagery and perhaps for identifying
georeferencing errors.</p>
      <p id="d1e5292">We do not expect ALDI in its current form to be as useful as manual mapping:
(1) as a source of rapid landslide information to inform emergency response
(because ALDI performs better with 2 years of post-event images); (2) for
size or shape distributions (because of censoring and amalgamation inherent
in 30 m pixel-based output); (3) for analysis where landslide initiation
zones must be differentiated from runout; (4) in landscapes where vegetation
is sparse (because NDVI changes in landslide pixels are unlikely to be
detectable relative to natural variability); and (5) in landscapes where
small landslides are widely distributed across the landscape (because the
pixel-averaged NDVI change will be small if only a fraction of a pixel is
disrupted).</p>
</sec>
<sec id="Ch1.S5.SS5">
  <label>5.5</label><title>Comparison to other automated detection methods</title>
      <p id="d1e5304">Automated detection of landslides typically relies on vegetation change
detection and involves either generating indices of surface disturbance from
which landslides can be manually identified (e.g. Scheip and Wegmann, 2021)
or performing a supervised classification (e.g. Barlow et al., 2003; Behling
et al., 2014, 2016; Prakash et al., 2020).</p>
      <p id="d1e5307">A recent example of automated surface disturbance detection, HazMapper
(Scheip and Wegmann, 2021), uses similar image data (Landsat) and the same
platform (Google Earth Engine) as ALDI but for a different purpose and
using different functions to combine and transform the imagery. HazMapper is
designed to generate a qualitative metric for surface change rather than a
landslide-specific mapping tool. As a result, the approach does not mask
snow-covered areas in case these are of interest for a user's particular
application. The approach is simpler than that of ALDI in that HazMapper
calculates the NDVI difference only, rather than accounting for post-event
NDVI, seasonal variability, and noise in the NDVI signal for each pixel. It
is currently only applied to Landsat 7 onwards and only for individual
sensors, rather than combining images from multiple Landsat sensors. This
limits the events that can be examined to those occurring after 1999.
However, results from HazMapper for the same study periods examined here
show a good qualitative agreement with the ALDI results. The similarity in
approach, using stacks of Landsat imagery before and after a suspected
trigger event, means that the two approaches will likely have many of the
same strengths (e.g. the accurate georeferencing of Landsat imagery) and
limitations (e.g. the coarse resolution of Landsat imagery and long wait
times required to generate the post-event stack).</p>
      <p id="d1e5310">Alternative approaches to landslide detection that involve supervised
classification typically rely on machine learning (e.g. Prakash et al.,
2020) or clustering methods (e.g. Barlow et al., 2003; Behling et al., 2014;
2016). These more complex approaches are compatible with the data and
platforms that we use here. Although we have taken a simpler approach, the
classification surfaces generated by ALDI could be coupled with modern
machine learning approaches to improve ALDI's landslide detection skill.
However, our results also highlight an important potential limitation to the
use of supervised learning for landslide detection in general. Given the
very severe disagreement between manually mapped landslide inventories, any
supervised learning method will have a very high risk of propagating gross
errors into the classifier unless the training inventory is precisely
co-located with the imagery used by the classifier. ALDI could help improve
existing supervised classification efforts by providing additional
well-referenced landslide inventories or by correcting existing ones.</p>
</sec>
<sec id="Ch1.S5.SS6">
  <label>5.6</label><title>Application to future earthquakes</title>
      <p id="d1e5321">The increased frequency and quality of optical imagery suggest that ALDI should
perform well for future earthquakes. In particular, Sentinel-2 imagery can
generate NDVI at 10 m spatial resolution (Table 1). The two Sentinel-2
satellites were launched between June 2015 and March 2017, and thus there is
a limited stack of pre- or post-earthquake images available to date. The
2018 Hokkaido earthquake offers the best trade-off to date between pre- and
post-event data. As a test of the wider applicability of ALDI to future
events, we ran ALDI using the global-parameter set identified above and
evaluated its results against landslides mapped from aerial imagery by Wang
et al. (2019). The results are extremely promising both at the scale of the
entire epicentral area (Fig. 9d and e), as well as of individual landslides, with
few false positives, a large area under the ROC curve (0.94), and many
landslides clearly delineated by a sharp break from high to low ALDI values
(Fig. 9f).</p><?xmltex \hack{\newpage}?>
</sec>
</sec>
<?pagebreak page504?><sec id="Ch1.S6" sec-type="conclusions">
  <label>6</label><title>Conclusion</title>
      <p id="d1e5334">Rapid derivation of landslide inventories after large triggering events
remains a key research challenge. We have developed a parsimonious automatic
landslide classifier, ALDI, that uses pre- and post-event stacks of
freely available medium-resolution satellite imagery and relies on
landslide-induced changes to vegetation cover and thus to NDVI values. We
test the classifier against multiple independent manually mapped inventories
from five recent earthquakes. Considering that manually mapped inventories
are typically assumed to be the ground truth against which automatic
classifiers are evaluated, we find that agreement between different manual
inventories is surprisingly low (8 %–30 % of landslide area in common). ALDI
often identifies landslides in one inventory missed in the other and even
identifies some candidate landslides not in either inventory but that have
location and morphometric characteristics that strongly suggest they are
true positives.</p>
      <p id="d1e5337">We further find that ALDI can identify landslide locations with a level of
skill that is comparable to manual mapping on a pixel-by-pixel basis. ALDI
calibrated to mapped landslides at a site outperforms manual mapping in 10 of 14 cases (i.e. 71 %). The only cases where manual mapping performs
better are the two inventories for the 2010 Haiti earthquake, where the
stack of available Landsat images is extremely limited, and the cross
comparison of inventories for the 2015 Gorkha earthquake, where strong
agreement between inventories is the result of mapping from very similar
satellite imagery.</p>
      <p id="d1e5340">Even when using a global-parameter set, ALDI outperforms manual mapping in 8 of 14 cases (57 %) with 10 of 14 cases (71 %) performing either better
than manual mapping or within the uncertainty in manual mapping performance
estimates. These results suggest that ALDI can be applied with considerable
confidence to map the areas affected by co-seismic landslides in future
earthquakes without the need for additional calibration. Holdback tests do
not change either of these statistics and affect our chosen performance
metrics by only a few percent, suggesting that the set of earthquakes that
we have used is large enough to develop a robust global-parameter set.</p>
      <p id="d1e5343">The area–frequency distributions for clusters of pixels that are classified
as landslides both from manual and automated landslide classification are
broadly similar, particularly in their heavy right tail. However, the
classifier-derived inventories are fundamentally limited by the resolution
of the imagery and their inability to disaggregate amalgamated landslides so that an object-based approach is required to recover realistic
area–frequency information.</p>
      <p id="d1e5347">ALDI is fast to run, uses free imagery with near-global coverage, and
generates landslide information that is of comparable quality to that of
costly and time-consuming manual mapping, depending on its intended use.
Thus, even in its current form it has the potential to significantly improve
the coverage and quantity of landslide inventories. However, its simplicity
(performing only pixel-wise analysis) and parsimony of inputs (using only
optical imagery) suggest that considerable further improvement should be
possible.</p>
</sec>

      
      </body>
    <back><notes notes-type="codeavailability"><title>Code availability</title>

      <p id="d1e5354">The Google Earth Engine code to run ALDI is available on GitHub at <uri>https://github.com/DavidMilledge/ALDI</uri> (last access: 9 February 2022; Milledge, 2021) and as a GEE App at <uri>https://dgmilledge.users.earthengine.app/view/aldi-landslide-detection</uri> (ALDI-landslide-detection, 2022).</p>
  </notes><notes notes-type="dataavailability"><title>Data availability</title>

      <p id="d1e5366">All data used in this research are openly available. The satellite imagery
is provided by USGS and archived by Google within Google Earth Engine. The
Watt landslide inventory will be deposited in the open USGS Global Earthquake-Triggered Ground-Failure Inventory Database on publication. All other
landslide inventories used in this research are already in this repository.</p>
  </notes><app-group>
        <supplementary-material position="anchor"><p id="d1e5369">The supplement related to this article is available online at: <inline-supplementary-material xlink:href="https://doi.org/10.5194/nhess-22-481-2022-supplement" xlink:title="pdf">https://doi.org/10.5194/nhess-22-481-2022-supplement</inline-supplementary-material>.</p></supplementary-material>
        </app-group><notes notes-type="authorcontribution"><title>Author contributions</title>

      <p id="d1e5378">JW and DGM collected one of the landslide inventories and made it ready
for use. DGM designed and implemented the ALDI classifier with input from
DGB and analysed data with input from ALD. DGM, DGB and ALD
wrote the paper. ALD organised funds.</p>
  </notes><notes notes-type="competinginterests"><title>Competing interests</title>

      <p id="d1e5384">The contact author has declared that neither they nor their co-authors have any competing interests.</p>
  </notes><notes notes-type="disclaimer"><title>Disclaimer</title>

      <p id="d1e5390">Publisher’s note: Copernicus Publications remains neutral with regard to jurisdictional claims in published maps and institutional affiliations.</p>
  </notes><ack><title>Acknowledgements</title><p id="d1e5396">Some of this work was undertaken while David G. Milledge was supported by the Natural
Environment Research Council (grant nos. NE/J01995X/1 and NE/N012216/1). Dino G. Bellugi
was supported by a grant from the National Science Foundation (NSF, no. EAR-1945431) and by a Gordon and Betty Moore Foundation Data-Driven
Discovery Initiative award (no. GMBF-4555). We are extremely grateful to
Google and the Google Earth Engine team for sharing their software, to the
USGS for access to the Landsat data, and to all the research teams involved
in the USGS ScienceBase Landslide Inventory project for sharing their
landslide inventories. Comments from Odin Marc and Ali P. Yunus and one anonymous referee
were very useful in helping us to refine our approach and arguments.</p></ack><?xmltex \hack{\newpage}?><?xmltex \hack{\newpage}?><notes notes-type="financialsupport"><title>Financial support</title>

      <p id="d1e5403">This research has been supported by the Natural Environment Research Council (grant nos. NE/N012216/1 and NE/J01995X/1), the National Science Foundation (NSF, grant no. EAR-1945431), and the Betty Moore Foundation Data-Driven Discovery Initiative (award no. GMBF-4555).</p>
  </notes><notes notes-type="reviewstatement"><title>Review statement</title>

      <p id="d1e5409">This paper was edited by Filippo Catani and reviewed by Ali P. Yunus and one anonymous referee.</p>
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