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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-19-2385-2019</article-id><title-group><article-title>Simulation of fragmental rockfalls detected using terrestrial laser scans from rock slopes in south-central <?xmltex \hack{\break}?> British Columbia, Canada</article-title><alt-title>Simulation of fragmental rockfalls detected using terrestrial laser scans</alt-title>
      </title-group><?xmltex \runningtitle{Simulation of fragmental rockfalls detected using terrestrial laser scans}?><?xmltex \runningauthor{Z.~Sala et al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes" rid="aff1 aff2">
          <name><surname>Sala</surname><given-names>Zac</given-names></name>
          <email>zac.sala@queensu.ca</email>
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Hutchinson</surname><given-names>D. Jean</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Harrap</surname><given-names>Rob</given-names></name>
          
        </contrib>
        <aff id="aff1"><label>1</label><institution>Department of Geological Sciences and Geological Engineering, Queen's
University, <?xmltex \hack{\break}?> Kingston, K7L 3N6, Canada</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>BGC Engineering Inc., Vancouver, V6Z 0C8, Canada</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Zac Sala (zac.sala@queensu.ca)</corresp></author-notes><pub-date><day>30</day><month>October</month><year>2019</year></pub-date>
      
      <volume>19</volume>
      <issue>11</issue>
      <fpage>2385</fpage><lpage>2404</lpage>
      <history>
        <date date-type="received"><day>29</day><month>October</month><year>2018</year></date>
           <date date-type="rev-request"><day>24</day><month>January</month><year>2019</year></date>
           <date date-type="rev-recd"><day>18</day><month>July</month><year>2019</year></date>
           <date date-type="accepted"><day>25</day><month>July</month><year>2019</year></date>
      </history>
      <permissions>
        <copyright-statement>Copyright: © 2019 </copyright-statement>
        <copyright-year>2019</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="d1e108">Rockfall presents an ongoing challenge to the safe
operation of transportation infrastructure, creating hazardous conditions
which can result in damage to roads and railways, as well as loss of life.
Rockfall risk assessment frameworks often involve the determination of
rockfall runout in an attempt to understand the likelihood that rockfall
debris will reach an element at risk. Rockfall modelling programs which
simulate the trajectory of rockfall material are one method commonly used to
assess potential runout. This study aims to demonstrate the effectiveness of
a rockfall simulation prototype which uses the Unity 3D game engine. The
technique is capable of simulating rockfall events comprised of many mobile
fragments, a limitation of many industry standard rockfall modelling
programs. Five fragmental rockfalls were simulated using the technique, with
slope and rockfall geometries constructed from high-resolution terrestrial
laser scans. Simulated change detection was produced for each of the events
and compared to the actual change detection results for each rockfall as a
basis for testing model performance. In each case the simulated change
detection results aligned well with the actual observed change in terms of
location and magnitude. An example of how the technique could be used to
support the design of rockfall catchment ditches is shown. Suggestions are
made for future development of the simulation technique with a focus on
better informing simulated rockfall fragment size and the timing of
fragmentation.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <label>1</label><title>Introduction</title>
      <p id="d1e120">Rockfall is a mass-movement hazard often found in mountainous environments,
posing risk to human lives and the safe operation of infrastructure. In
Canada, rockfall hazard is particularly problematic for transportation
infrastructure, where traffic corridors have been constructed in steep river
valleys, adjacent to natural and cut slopes. In many of these valleys,
right-of-way space is limited, forcing operators to construct highways and
railways with minimal clearance to potentially unstable rock masses. The
proximity and extensive presence of fractured and weathered rock slopes,
combined with the seemingly unpredictable nature of rockfall events, makes
it difficult for operators to manage this hazard.</p>
      <p id="d1e123">Like any geohazard, we are interested in knowing how frequently we can
expect events to occur, where they are most likely to come from, and whether
or not they will reach and cause harm to our elements at risk. For rockfall
this could involve identifying lithologies which are more susceptible to
rockfall (e.g. Rosser et al., 2005; van Veen, 2016) or correlating rockfall
frequency to triggering events like severe rain storms (e.g. D'Amato et al.,
2016; Pratt et al., 2018). In order to build these relationships, we first
need knowledge of previous rockfall in the area. This is one of the main
challenges in the study of rockfall. Due to challenging terrain in
mountainous areas, and safety concerns where rockfall activity is high, site
access to the slopes of interest is often limited, prohibiting direct
measurement.</p>
      <p id="d1e126">In order to circumvent these obstacles, modern remote sensing techniques,
such as lidar, have seen widespread use<?pagebreak page2386?> in the study of landslide hazards
like rockfall (Jaboyedoff et al., 2012). Terrestrial laser scanning (TLS) in
particular has been increasingly applied in recent years to the study of
rock slope instabilities (Abellán et al., 2014; e.g. Lato et al., 2009, 2015; Kromer et al., 2017). TLS provides a detailed 3-D model of
the slope geometry, supporting a range of geotechnical and geomechanical
analyses. From a single scan we can extract slope angle measurements, map
rock mass structure and look for evidence of past rockfall (Telling et al.,
2017). Using multiple successive scans of the same slope, progressive
changes to the slope surface can be measured. Multi-temporal scanning
enables researchers to detect rockfall events over time and build detailed
magnitude–frequency relationships for slopes, supporting the study of
processes such as coastal cliff erosion (e.g. Rosser et al., 2007; Williams
et al., 2018), as well as hazard and risk assessments for linear
infrastructure such as railways (e.g. van Veen et al., 2017). The
identification of rockfall events using sequential scans also permits the
back analysis of rockfall-triggering factors and failure mechanisms. A study
by Kromer et al. (2015) used TLS change detection to investigate the
occurrence of a 2600 m<inline-formula><mml:math id="M1" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:math></inline-formula> failure above a section of the Canadian National (CN) Railway in
western Canada, including an analysis of structural constraints, pre-failure
deformation, and precursor rockfall leading up to failure.</p>
      <p id="d1e138">While the application of TLS to rock slope monitoring is often focused on
determining how likely future rockfall is or where the rockfall may come
from, it is also important to determine how likely it is that the rockfall
material will reach an element at risk should a fall occur. In order to
answer that question, rockfall modelling programs can be used to simulate
the runout of falling rock material using numerical models (Turner and
Duffy, 2012). A rockfall simulation requires a representation of the slope
surface and rockfall mass being modelled in 2-D, 2.5-D, or 3-D. TLS can support
rockfall simulation by providing a high-resolution 3-D model of the slope
surface and, in cases where a rockfall event has been identified using
change detection between multiple scans, the volume and location of the
rockfall mass. In order to make use of the quality and quantity of 3-D point
cloud data being collected as part of a rock slope monitoring program in
western Canada, a 3-D rockfall simulation technique using game-engine
technology has been developed (Ondercin, 2016; Sala, 2018). The technique
uses the video game development platform Unity 3D (Unity Technologies, 2018)
and is capable of simulating rockfall runout using fully 3-D meshes built
from TLS point cloud data.</p>
      <p id="d1e142">One of the strengths of this simulation technique is its ability to simulate
rockfall runout using numerous interacting bodies. This capability allows us
to produce simulations of fragmental rockfall events, which are defined by
the presence of multiple mobile fragments of rock during runout (Hungr and
Evans, 1988). Conventional rockfall modelling programs (e.g. RocFall,
Rocscience Technologies, 2016; Rockyfor3D,  Dorren, 2015; RAMMS:ROCKFALL,
Bartelt et al., 2016) simulate single boulder trajectories at a time and
therefore are unable to model fragmental rockfall runout. Efforts to model
fragmental rockfall processes, including the disaggregation of falling rock
masses along pre-existing discontinuities, or the breakage of intact blocks
during impact, have been demonstrated by previous authors. Cuervo et al. (2015) utilized a discrete element technique to model the disaggregation of
a 1000 m<inline-formula><mml:math id="M2" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:math></inline-formula> rockfall event in southern France comprised of numerous
mobile fragments. Wang and Tonon (2011) developed a discrete element code
which models the fragmentation of a falling rock at impact, taking into
consideration the effect of impact velocity, ground condition, energy loss,
and fracture properties such as persistence. The GIS-based tool RockGIS,
presented in Matas et al. (2017), incorporates both breakage along
pre-existing discontinuities and the generation of new fragments
during impact into a 3-D runout modelling program and has been utilized to
model a 10 000 m<inline-formula><mml:math id="M3" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:math></inline-formula> fragmental rockfall in the eastern Pyrenees
mountains. The goal of the work presented in this paper is to demonstrate
the capability of our novel game-engine-hosted simulation technique to model
a series of rockfall events detected using TLS change detection at two rock
slopes in south-central British Columbia. Emphasis is placed on the ability
of the technique to be used for fragmental rockfall runout simulation,
including a discussion of how these types of simulation could support
mitigation design.</p>
</sec>
<sec id="Ch1.S2">
  <label>2</label><title>Study sites</title>
      <p id="d1e171">The rock slopes of focus for this paper are part of the Ashcroft subdivision
of the CN Railway. The subdivision follows sections of the Thompson and
Fraser River valleys, located between the towns of Ashcroft and Lytton,
British Columbia. This region serves as an important transportation corridor
for Canada, with the presence of the CN Rail mainline, as well as sections
of the Canadian Pacific Railway, and the Trans-Canada Highway. A previous
study by Piteau (1977) identified that rock cuts in this region are subject
to slope instability issues due to a combination of lateral erosion from
river activity, over-steepening from blasting during the construction of the
railways, and a lack of adequate rockfall catchment areas.</p>
      <p id="d1e174">Two sites in the Ashcroft subdivision will form the basis for this research,
White Canyon and Goldpan. The location of these sites along the
Thompson River and proximity to the town of Lytton, BC, can be seen in Fig. 1. The monitoring of these slopes is part of the Railway Ground
Hazard Research Program, a collaborative research initiative focused on the
characterization and assessment of mass movement hazards affecting Canadian
railways.</p>
      <p id="d1e177">Data collection in the Ashcroft subdivision first took place in 2012, and
regular monitoring at both sites has been ongoing since 2014, with data
collection taking place on a seasonal basis, approximately every 3 months.
Point cloud data<?pagebreak page2387?> collection consists of TLS scans acquired using an Optech
ILRIS 3D-ER (2012–2017) or Riegl VZ-400i (2018) lidar system. Additionally,
aerial laser scan (ALS) data coverage for both sites, with an average point spacing of 0.3 m,
was acquired in 2014 and 2015. Site photos are collected using a Nikon D700
or similar camera with a 135 mm prime lens. A series of photos of the slope
are taken using a GigaPan EPIC Pro robotic camera mount and stitched
together into a single high-resolution site panorama using GigaPan Stitch
(GigaPan Systems, 2013).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1"><?xmltex \currentcnt{1}?><label>Figure 1</label><caption><p id="d1e183">Aerial imagery showing the location of the White Canyon and
Goldpan field sites situated along the Thompson River, near the town of
Lytton in south-central British Columbia. This region is approximately 160
km northeast of the city of Vancouver. (Image source: © Google
Earth; Digital Globe 2018.)</p></caption>
        <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/19/2385/2019/nhess-19-2385-2019-f01.jpg"/>

      </fig>

      <p id="d1e192">Goldpan is located on the north side of the Thompson River, approximately 26 km upstream from the town of Lytton. Present at the base of the slope is a
section of the CN Rail main line. The rock slope spans 800 m, rising up to
65 m vertically above track level. The average slope angle at the site is
55–60<inline-formula><mml:math id="M4" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>. TLS data are collected from scanning vantage points across the
river from the slope, accessed via Goldpan Provincial Park. Scan distances
range between 170 and 230 m, producing an average point spacing of
approximately 6 cm.</p>
      <p id="d1e204">White Canyon is located on the north side of the Thompson River,
approximately 5 km upstream from the town of Lytton. Present at the base of
the slope is a section of the CN Rail main line. The rock slope spans 2.4 km, rising up to 375 m vertically above track level. The average slope angle
at the site is 40–45<inline-formula><mml:math id="M5" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>. TLS data are collected from scanning vantage
points across the river from the slope. Scan distances range between 400 and 600 m, producing an average point spacing of approximately 10 cm.</p>
      <p id="d1e216">Goldpan and White Canyon are located in the Intermontane belt of the
Canadian Cordillera. Both sites belong to the Quesnellia volcanic arc
terrane, which is composed of Carboniferous to mid-Jurassic volcanic,
sedimentary, and plutonic rocks (Struik, 1987; Monger and Nokelberg, 1996).
The rock mass at Goldpan is largely massive and is predominantly composed of
volcanics of the mid-Cretaceous Kingsvale–Spences Bridge Group. The main
rock types of this group are basaltic to andesitic flows interspersed with
volcaniclastic sandstones, shales, and conglomerates (Brown, 1981). The
comparatively large rock slope of White Canyon belongs to the Mt Lytton
plutonic complex (Greig, 1989). Locally, the dominant rock type is an
amphibolite grade quartzofeldspathic gneiss. Amphibolite banding is also
present and gneissic layering is crosscut throughout the canyon by
intrusive phases of gabbro, tonalite, and granodiorite (Brown, 1981).
Preferential weathering around these intrusions often results in the
formation of vertical rock spires which act as source zones for rockfall.</p>
      <p id="d1e219">Mitigative measures at both sites have been installed in response to
frequent rockfall activity impacting railway operations. At Goldpan this
includes rockfall wire mesh draped over parts of the slope, extensive
sections of shotcrete, and four concrete rock sheds. In the eastern half of
White Canyon there are two timber rock sheds and one concrete shed, as
well as wire mesh rockfall nets and concrete lock blocks adjacent to the
track. The western half of White Canyon also has wire mesh rockfall nets
and lock block retaining walls, as well as an additional three concrete rock
sheds and one timber rock shed. Slide detector fences are present at both
sites, comprised of horizontal wires strung between upright telephone poles,
and provide warning by switching the track signal to stop when broken.</p>
</sec>
<sec id="Ch1.S3">
  <label>3</label><title>Rockfall events</title>
      <p id="d1e230">Five rockfall events were selected from a database of rockfalls which have
been identified using change detection at White Canyon West, White Canyon
East, and Goldpan since 2012 (Kromer et al., 2015). These events have masses
ranging from 2  to 170 m<inline-formula><mml:math id="M6" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:math></inline-formula>, exhibiting a combination of
structurally controlled failure modes including wedge sliding, planar
sliding, toppling, and overhanging blocks. Images of the five slope sections
where the rockfall events of interest took place can be seen in Fig. 2.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2"><?xmltex \currentcnt{2}?><label>Figure 2</label><caption><p id="d1e244">Photos of five rock slope sections, prior to failure, from the Goldpan <bold>(a)</bold> and White Canyon <bold>(b–e)</bold> sites adjacent to the CN Railway. The red
regions indicate the source zone for the rockfall events discussed in this
paper.</p></caption>
        <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/19/2385/2019/nhess-19-2385-2019-f02.jpg"/>

      </fig>

      <p id="d1e259">Each event showed material accumulation below the source zone in the change
detection results. This is essential information for comparison with our
simulation results. Each event is also close to track level, with the
highest fall occurring 46 m vertically above the track. These events were
selected because the shorter distance from source to a notable accumulation
of material presents a simpler trajectory for back analysis and reduces
potential confusion in interpreting whether the material gain is due to the
selected rockfall or another mass-movement nearby. In each case, change was
detected using the Multiscale Model to Model Cloud Comparison (M3C2)
point–point distance calculation (Lague et al., 2013) in CloudCompare (2018), between the pre- and<?pagebreak page2388?> post-fall TLS scans. A summary of each of the
rockfall events including change detection results, and site photos before
and after the event, is provided in Figs. 3–7. Discontinuity and slope
angle measurements used for the stereonet failure mode analysis shown in
each figure were completed using the Compass tool in CloudCompare.</p>

      <?xmltex \floatpos{p}?><fig id="Ch1.F3" specific-use="star"><?xmltex \currentcnt{3}?><label>Figure 3</label><caption><p id="d1e265">Site A. Visual overview of the 170 m<inline-formula><mml:math id="M7" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:math></inline-formula>  wedge sliding
rockfall event detected at the Goldpan site between July and October 2016.
The event involved a large triangular slab of weathered and jointed rock mass
which failed approximately 35 m above a rock shed which is protecting the
track at Goldpan. Site photos <bold>(a, b)</bold> of the source zone pre- and
post-failure are shown. Change detection results of the event are shown
<bold>(c)</bold> with cool colours indicating material loss and warm colours
indicating material accumulation. Material from the rockfall accumulated on
the bench of the mid-slope gully, as well as on top of the rock shed, with
the majority of the material running out over the shed and leaving the
slope. The rockfall hull of the event extracted from the pre- and
post-failure meshes is shown <bold>(d)</bold>, as well as a stereonet
representation of the wedge sliding failure mode.</p></caption>
        <?xmltex \igopts{width=441.017717pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/19/2385/2019/nhess-19-2385-2019-f03.png"/>

      </fig>

      <?xmltex \floatpos{p}?><fig id="Ch1.F4" specific-use="star"><?xmltex \currentcnt{4}?><label>Figure 4</label><caption><p id="d1e294">Site B. Visual overview of the 24 m<inline-formula><mml:math id="M8" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:math></inline-formula> wedge sliding rockfall event
detected at the White Canyon East site between May and July 2016. The event
involved a large pseudo-cubic block of weathered and jointed rock mass which
failed approximately 46 m above track level. Site photos <bold>(a, b)</bold> of the
source zone pre- and post-failure are shown. Change detection results of the
event are shown <bold>(c)</bold> with cool colours indicating material loss and warm
colours indicating material accumulation. A small portion of the rockfall
volume was retained in the gully leading down to track level, with the
majority of the accumulation taking place in the track-side ditch. The rockfall
hull of the event extracted from the pre- and post-failure meshes is shown <bold>(d)</bold>, as well as a stereonet representation of the wedge sliding
failure mode. It should be noted that parts of the source rock mass also
exhibited overhanging sections.</p></caption>
        <?xmltex \igopts{width=441.017717pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/19/2385/2019/nhess-19-2385-2019-f04.png"/>

      </fig>

<sec id="Ch1.S3.SS1">
  <label>3.1</label><title>Event fragmentation</title>
      <p id="d1e328">While the selected rockfall events were not observed directly, each rockfall
is believed to have been comprised of multiple mobile fragments. This
interpretation is based on observations of the fractured state of the source
zones pre- and post-fall, as well as the size and distribution of visible
rock fragments in the post-fall areas of accumulation, below the source zone
and adjacent to the track. An example of this can be seen in Fig. 8 for
White Canyon overhanging wedge event. In these photos it is clear that
the source rock mass is heavily jointed and that the accumulation of
material generated from the event is not a few large blocks but rather a
deposit of coarse granular material.</p>

      <?xmltex \floatpos{p}?><fig id="Ch1.F5" specific-use="star"><?xmltex \currentcnt{5}?><label>Figure 5</label><caption><p id="d1e333">Site C. Visual overview of the 32 m<inline-formula><mml:math id="M9" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:math></inline-formula>  flexural toppling
event detected at the White Canyon East site between June and August 2016.
The event involved a large slab of weathered and heavily jointed rock mass
which failed approximately 14 m above track level. Site photos <bold>(a, b)</bold> of the
source zone pre- and post-failure are shown. Change detection results of the
event are shown <bold>(c)</bold> with cool colours indicating material loss and warm
colours indicating material accumulation. Change detection results indicate
the bulk of material from the rockfall event was retained in the track-side
ditch. The rockfall hull of the event extracted from the pre- and
post-failure meshes is shown <bold>(d)</bold>, as well as a stereonet
representation of the flexural toppling failure mode. It should be noted
that parts of the source rock mass also exhibited overhanging sections.</p></caption>
          <?xmltex \igopts{width=441.017717pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/19/2385/2019/nhess-19-2385-2019-f05.png"/>

        </fig>

      <?xmltex \floatpos{p}?><fig id="Ch1.F6" specific-use="star"><?xmltex \currentcnt{6}?><label>Figure 6</label><caption><p id="d1e362">Site D. Schematic overview of the 15 m<inline-formula><mml:math id="M10" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:math></inline-formula> planar sliding rockfall
event detected at the White Canyon West site between October 2015 and
February 2016. The event involved an irregularly shaped slab of weathered
and heavily jointed rock mass which failed approximately 9.5 m above track
level. Site photos <bold>(a, b)</bold> of the source zone pre- and post-failure are
shown. Change detection results of the event are shown <bold>(c)</bold> with cool
colours indicating material loss and warm colours indicating material
accumulation. Change detection results indicate that the bulk of the
material from the event was retained by the track-side ditch. The rockfall
hull of the event extracted from the pre- and post-failure meshes is shown <bold>(d)</bold>, as well as a stereonet representation of the planar sliding
failure mode.</p></caption>
          <?xmltex \igopts{width=441.017717pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/19/2385/2019/nhess-19-2385-2019-f06.png"/>

        </fig>

      <p id="d1e390">The presence of multiple mobile fragments means that these events may be
classified as fragmental rockfalls (Hungr and Evans, 1988; Hungr et al.,
2014). Hungr and Evans (1988) originally proposed that for the case of
fragmental falls, the movements of the most mobile fragments in the fall are
independent of each other. This suggests that the modelling of these events
as a volume of fractured material is unnecessary, and instead single design
blocks with a specified average or maximum fragment volume could be used.
This is in contrast to the idea that larger volume rock slope failures
such as rock avalanches should be modelled as granular flows rather than
independent ballistic trajectories (Bourrier et al., 2013). The distinction
between these two types of motion is often discussed in relation to the
volume of material mobilized as part of the event, with larger volumes
(<inline-formula><mml:math id="M11" display="inline"><mml:mrow><mml:mi mathvariant="italic">&gt;</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>–10<inline-formula><mml:math id="M12" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msup></mml:math></inline-formula> m<inline-formula><mml:math id="M13" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:math></inline-formula>) suggested to show stronger
interaction between individual fragments. A discussion of the various
volumes and classifications of rock slope failure relevant to the transition
between these two styles of motion is presented by Corominas et al. (2017)
and suggests that volume thresholds and terminology for these types of
events is not yet consistent in the literature.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F7" specific-use="star"><?xmltex \currentcnt{7}?><label>Figure 7</label><caption><p id="d1e427">Site E. Schematic overview of the 8 m<inline-formula><mml:math id="M14" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:math></inline-formula> planar sliding event
detected at the White Canyon West site between July and October 2016. The
event involved the failure of two distinct sections of the jointed source
rock mass, with the upper (6 m<inline-formula><mml:math id="M15" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:math></inline-formula>) and lower (2 m<inline-formula><mml:math id="M16" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:math></inline-formula>) failures releasing from 10 and 6 m above track level respectively. Site photos <bold>(a, b)</bold> of the source
zone pre- and post-failure are shown. Change detection results of the event
are shown <bold>(c)</bold> with cool colours indicating material loss and warm
colours indicating material accumulation. Interpretation of the post-fall
imagery indicates that the lower failure was inside the slide path of the
upper rockfall event. It is our interpretation that these events likely
occurred simultaneously, with the lower failure occurring as a result of
impact from the upper failure. Change detection results indicate that the
bulk of the material from the two events was retained by the track-side
ditch. The rockfall hull of the events, extracted from the pre- and
post-failure meshes is shown <bold>(d)</bold>, as well as a stereonet
representation of the planar sliding failure mode for the upper, larger
event.</p></caption>
          <?xmltex \igopts{width=441.017717pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/19/2385/2019/nhess-19-2385-2019-f07.png"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F8" specific-use="star"><?xmltex \currentcnt{8}?><label>Figure 8</label><caption><p id="d1e475">Before and after photos of the 24 m<inline-formula><mml:math id="M17" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:math></inline-formula> wedge sliding event from
White Canyon East, Site B. The top row of photos shows the pre-fall debris
present in the track-side ditch <bold>(a)</bold>, as well as the pre-fall source zone <bold>(b)</bold>. The bottom row shows the post-fall accumulation in the track-side ditch <bold>(c)</bold>, as well as the post-fall source zone <bold>(d)</bold>. From these images we can see
the heavily jointed state of the rockfall mass pre-fall and the rockfall
back scarp post-fall. A notable increase in the quantity and size of debris
fragments in the track-side ditch is visible post-fall.</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/19/2385/2019/nhess-19-2385-2019-f08.jpg"/>

        </fig>

      <p id="d1e505">While rockfall events <inline-formula><mml:math id="M18" display="inline"><mml:mrow><mml:mi mathvariant="italic">&lt;</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mn mathvariant="normal">1000</mml:mn></mml:mrow></mml:math></inline-formula> m<inline-formula><mml:math id="M19" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:math></inline-formula>, such as those considered in
this study, may be described as having limited interaction between mobile
fragments, the use of a single design block is not effective in cases where
sufficiently large fragmental falls might overwhelm ditches at the base of a
slope. A schematic overview of this process can be seen in Fig. 9.
Material which builds up in the ditch or other retaining structures may
allow trailing rockfall debris to roll out over the newly formed surface.
Additionally, a trailing fragment of rock may impact the accumulated pile of
debris with enough force to push some fragments out onto the track.
Simulation of the entire fragmental rockfall volume at once, as a moving
mass of many fragments, allows for important slope-stopping features such as
benches, gullies, and ditches to be filled, impacting the runout of trailing
rockfall material. Snapshots from a video of a recorded fragmental rockfall,
which filled a ditch and impacted a section of railway in western Canada,
can be seen in Fig. 10. In this case, the leading portion of the rockfall
event was pushed forward by trailing material before it fully came to rest
in the ditch. Additionally, subsequent individual rock fragments were able
to run out into the track region as a result of the catchment ditch being
full.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F9"><?xmltex \currentcnt{9}?><label>Figure 9</label><caption><p id="d1e531">Schematic of potential fragmental rockfall runout behaviour. Here
leading material from the event has filled up a catchment ditch. Trailing
rockfall material impacting the back of the deposit has the potential to
push the leading material forward and out of the ditch (black arrows)
reaching the track area. Additionally, the initial material has created a
surface over which trailing rock fragments can move (grey trajectory),
reducing the effectiveness of the ditch.</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/19/2385/2019/nhess-19-2385-2019-f09.png"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F10" specific-use="star"><?xmltex \currentcnt{10}?><label>Figure 10</label><caption><p id="d1e542">Snapshots from a video of a fragmental rockfall event occurring
above a section of railway in western Canada. Elapsed time between frame (1)
and frame (6) is approximately 2 s.</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/19/2385/2019/nhess-19-2385-2019-f10.jpg"/>

        </fig>

      <?pagebreak page2391?><p id="d1e551">The simulation of these events as single block falls would produce
unrealistic runout due to interaction with retaining structures like
ditches. In addition, the mobility of larger falls is much different than
smaller fragments, with significantly higher potential energies at release,
as well as larger moments of inertia affecting rotation during runout. At
track level the impact energy of a single coherent block would be larger,
resulting in an overestimate of the potential for damage to the track.
Additionally, a single block simulation may underestimate the spatial extent
of track interaction, as individual fragments from a multi-block fall are
free to disperse from each other laterally, impacting multiple points on the
track at once. From a design perspective, this would influence the type of
mitigation selected for the site. The isolated high-energy impacts of a
large single block may require a fixed, high-strength system like a
mechanically stabilized earth wall or rock shed. In the case of the
numerous, small impacts from a fragmented source volume, wire mesh draping
to divert the fragments into the ditch may suffice.</p>
</sec>
</sec>
<sec id="Ch1.S4">
  <label>4</label><title>Runout simulations</title>
      <p id="d1e563">For each of the selected rockfall events from our field sites, we can set up
a simulation in the Unity game engine. The main input parameters for
simulation setup are
<list list-type="bullet"><list-item>
      <p id="d1e568">coefficient of friction,</p></list-item><list-item>
      <p id="d1e572">coefficient of restitution,</p></list-item><list-item>
      <p id="d1e576">coefficient of viscoplastic ground drag,</p></list-item><list-item>
      <p id="d1e580">slope geometry,</p></list-item><list-item>
      <p id="d1e584">rockfall geometry, and</p></list-item><list-item>
      <p id="d1e588">rockfall release position and orientation.</p></list-item></list>
Collision detection, contact resolution, and the application of material-specific impact coefficients are handled by the built-in physics system in
the Unity game engine. The resolution of linear and angular velocity
per contact along a 3-D fragment surface is dependent on the simple friction
and restitution equations shown below. The friction coefficient (<inline-formula><mml:math id="M20" display="inline"><mml:mi mathvariant="italic">μ</mml:mi></mml:math></inline-formula>) is
used during collision to determine the proportion of the normal force (<inline-formula><mml:math id="M21" display="inline"><mml:mi>N</mml:mi></mml:math></inline-formula>)
between the simulated rockfall and slope surfaces which is to be used for
frictional resistance to movement. The friction force (<inline-formula><mml:math id="M22" display="inline"><mml:mrow><mml:msub><mml:mi>F</mml:mi><mml:mi mathvariant="normal">f</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) acts in the
opposite direction of the downslope component of the incoming velocity
vector. The force calculated per contact is applied over the simulation time
step (as an impulse) and used in the solution of the new translational and
rotational velocities which occur as a result of collision. In the Unity
environment, surface collisions are resolved into two contact anchor points,
resulting in the frictional force applied being twice as strong. Therefore,
the effective friction angle (<inline-formula><mml:math id="M23" display="inline"><mml:mi mathvariant="italic">ϕ</mml:mi></mml:math></inline-formula>) is equal to the arctangent of double
the Unity friction coefficient. The equation for the frictional force
applied per contact anchor point, as well as the conversion between the
coefficient of friction and friction angle, is shown below. Unlike the
coefficient of dynamic friction, which is applied to the tangential
component of velocity, the coefficient of restitution operates only in the
normal direction. The coefficient is equal to the ratio of the per-contact
relative velocity between the two colliding objects before and after the
collision. The third parameter, viscoplastic ground (vpg) drag, is assigned
to regions of the slope which are expected to have deformable surface
materials. The equation used here to model the force applied due to vpg drag
is based on the ground drag equation from the RAMMS::ROCKFALL model and is
given below (Bartelt et al. 2016). The drag force (<inline-formula><mml:math id="M24" display="inline"><mml:mrow><mml:msub><mml:mi>F</mml:mi><mml:mi mathvariant="normal">v</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) is proportional
to the mass of the rock block and the square of the block velocity at impact
(<inline-formula><mml:math id="M25" display="inline"><mml:mrow><mml:msubsup><mml:mi>V</mml:mi><mml:mi mathvariant="normal">s</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msubsup></mml:mrow></mml:math></inline-formula>). Essentially, impacts with higher kinetic energy (heavier,
faster moving blocks) are expected to result in a larger amount of dampening
as they cause more surface deformation of the slope material, resulting in
an increased dragging effect on the rockfall block.

              <disp-formula specific-use="gather" content-type="numbered"><mml:math id="M26" display="block"><mml:mtable displaystyle="true"><mml:mlabeledtr id="Ch1.E1"><mml:mtd><mml:mtext>1</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:msub><mml:mi>F</mml:mi><mml:mi mathvariant="normal">f</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mi mathvariant="italic">μ</mml:mi><mml:mo>∗</mml:mo><mml:mi>N</mml:mi></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E2"><mml:mtd><mml:mtext>2</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:mi mathvariant="italic">ϕ</mml:mi><mml:mo>=</mml:mo><mml:mi mathvariant="normal">arctan</mml:mi><mml:mo>(</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="italic">μ</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E3"><mml:mtd><mml:mtext>3</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:msub><mml:mi>R</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:msub><mml:mi>v</mml:mi><mml:mi mathvariant="normal">incident</mml:mi></mml:msub></mml:mrow><mml:mrow><mml:msub><mml:mi>v</mml:mi><mml:mi mathvariant="normal">rebound</mml:mi></mml:msub></mml:mrow></mml:mfrac></mml:mstyle></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E4"><mml:mtd><mml:mtext>4</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:msub><mml:mi>F</mml:mi><mml:mi mathvariant="normal">v</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mo>-</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mi>m</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:mfrac></mml:mstyle><mml:msub><mml:mi>C</mml:mi><mml:mi mathvariant="normal">v</mml:mi></mml:msub><mml:msubsup><mml:mi>V</mml:mi><mml:mi mathvariant="normal">s</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msubsup></mml:mrow></mml:mtd></mml:mlabeledtr></mml:mtable></mml:math></disp-formula></p>
      <?pagebreak page2393?><p id="d1e757"><?xmltex \hack{\newpage}?>A more detailed description of the material coefficients and their influence
on the rotational and translational velocity of simulated rock fragments,
along with a parametric investigation into the effects of simulated block
shape and release orientation, can be found in Sala (2018).</p>
      <p id="d1e761">The geometry used to build simulations is comprised of slope and rockfall
elements. The slope geometry is a 3-D mesh produced from the pre-fall TLS
scan of the slope, generated using Poisson reconstruction in CloudCompare.
The rockfall geometry is a 3-D mesh produced from the pre- and post-fall TLS
scans of the source region, generated using Poisson reconstruction and
connected into a single hull in Blender (Blender Foundation, 2017). By
extracting the rockfall source volume directly from the same TLS data used
to generate the slope geometry, the release position and orientation of the
source volume relative to the slope surface is well defined. This 3-D hull is
then segmented into a collection of convex hull fragments, using Voronoi
fracturing in Blender. This method subdivides the source rockfall volume
into a specified number of fragments selected by the user, with control over
the size and shape of fragments produced. An example of various Voronoi
fracturing results, including recursive fracturing, and fracturing with
preferential shape constraints can be seen in Fig. 11. The end result is a
simulated rockfall source volume which reflects the shape and fractured
nature of the rockfall event detected from the field.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F11"><?xmltex \currentcnt{11}?><label>Figure 11</label><caption><p id="d1e767">Showing the results of different Voronoi fracturing methods.
Recursive fracturing in <bold>(b)</bold> results in the additional fracturing of the
initial convex polyhedra in <bold>(a)</bold>. Shape constraints in <bold>(c)</bold> result in the
elongation of the convex polyhedra, creating a more sheet-like fracture
network.</p></caption>
        <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/19/2385/2019/nhess-19-2385-2019-f11.png"/>

      </fig>

      <p id="d1e785">A detailed explanation of the steps necessary to move from field remote
sensing data to a functioning simulation in Unity, including the workflow
from CloudCompare to Blender to Unity, can be found in Sala (2018). One of
the key strengths of this modelling technique is its ability to simulate the
collision between multiple moving rigid bodies at once. Support for
multi-body collisions allows us to simulate the disaggregation of heavily
jointed source rockfall volumes. This enables us to study the types of
rockfall runout expected to occur at our field sites, taking into
consideration the implications of fragmental runout discussed<?pagebreak page2394?> above.
Snapshots of an example fragmental rockfall simulation for the 170 m<inline-formula><mml:math id="M27" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:math></inline-formula>
Goldpan event (Site A) can be seen in Fig. 12.</p>
      <p id="d1e797">When developing or attempting to calibrate any new simulation technique, it
is necessary to compare simulation outputs to real observations of the
phenomena you are modelling in order to test how well the simulation
performs. Where direct observation of rockfall events is possible, such as
in rockfall drop tests, (e.g. Ushiro et al., 2006; Vick et al., 2015;
Volkwein et al., 2018), this information could include translational and
rotational velocity, mapped runout trajectories, or pass height above the
slope. For the five rockfall cases selected from our field sites, this
information is not available as the events were not observed directly.
Instead the location and magnitude of change present in the change detection
results for each event serve as the basis for simulation comparison.</p>
      <p id="d1e800">Simulations of each of the five selected rockfall events were run and change
maps of the simulation results were produced. In order to generate change
detection maps for the simulations, the positions of the post-simulation
fragments were merged with the slope geometry to create a post-simulation 3-D
mesh. Similarly, the fragmented rockfall geometry, pre-simulation, was
merged with the slope geometry to create a pre-simulation 3-D mesh. Each mesh
was then converted into a point cloud in Blender. The conversion of the mesh
data to a point cloud allows us to use the M3C2 point–point distance
calculation for both the actual and simulated rockfall events. The
transition from simulation mesh to point cloud is done by selecting only
visible vertices in the mesh, using a similar vantage point to the direction
of the original TLS scan. The selection of only visible vertices in the mesh
is necessary as the 3-D rockfall fragments, pre- and post-simulation, have
vertices across their entire surfaces, both front and back facing. This
results in multiple layers of points in the pre-fall source zone and
post-fall accumulation zone, adversely affecting point cloud normal
calculations and producing errors in the distance measurements between what
should be distinct pre- and post-fall surfaces. The extraction of visible
vertices from the mesh geometry, using a specified vantage point, ensures
that only a single layer of points is present in the simulated point cloud.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F12"><?xmltex \currentcnt{12}?><label>Figure 12</label><caption><p id="d1e805">Screenshots of a fragmental rockfall simulation (1000 fragments)
for the 170 m<inline-formula><mml:math id="M28" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:math></inline-formula> rockfall event at Goldpan.</p></caption>
        <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/19/2385/2019/nhess-19-2385-2019-f12.png"/>

      </fig>

      <?xmltex \floatpos{p}?><fig id="Ch1.F13" specific-use="star"><?xmltex \currentcnt{13}?><label>Figure 13</label><caption><p id="d1e826">A comparison of the actual and simulated change detection results
from the 170 m<inline-formula><mml:math id="M29" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:math></inline-formula> wedge sliding event at Goldpan, Site A. The simulation
produced a good comparison with the actual change results, yielding a
similar spatial distribution, and magnitude of change. In both cases
accumulation takes place on the mid-slope bench and on top of the rock shed,
with the majority of the material running out over the shed and off the slope.
The percentage of initial source volume retained at various locations on the
actual and simulated slope is displayed and shows a strong agreement. Areas
of additional loss in the actual change detection, on top of the rock shed
and at the mid-slope bench, are not captured in the simulation results. The
simulation technique uses a fixed, rigid slope surface and is not able to
capture smaller slope failures which may have occurred as a result of talus
impacts during the initial 170 m<inline-formula><mml:math id="M30" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:math></inline-formula> event.</p></caption>
        <?xmltex \igopts{width=384.112205pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/19/2385/2019/nhess-19-2385-2019-f13.png"/>

      </fig>

      <?xmltex \floatpos{p}?><fig id="Ch1.F14" specific-use="star"><?xmltex \currentcnt{14}?><label>Figure 14</label><caption><p id="d1e855">A comparison of the actual and simulated change detection results
from the 24 m<inline-formula><mml:math id="M31" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:math></inline-formula> wedge sliding event from White Canyon East, Site B. The
simulation produced a good comparison with the actual change results,
yielding a similar spatial distribution, and magnitude of change. The
percentage of initial source volume retained at various locations on the
actual and simulated slope is shown. In this case the majority of the material
in both the actual and simulated analysis ends up in the track-side ditch,
with a smaller component of the volume stopped inside the gully. In the
simulated change a small number of fragments do reach track level,
representing approximately 2 % of the simulated volume.</p></caption>
        <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/19/2385/2019/nhess-19-2385-2019-f14.png"/>

      </fig>

      <p id="d1e873">The results of the change detection analysis for each simulated rockfall
event are shown in Figs. 13–17. In each case the game-engine-based
simulation prototype was able to produce rockfall runout which compared well
in terms of the location and magnitude of the measured actual change. The
percentages of source rockfall volume retained at different locations on the
slope is shown. Volume measurements using the actual event point cloud data
were completed using the 2.5-D Volume tool in CloudCompare. Simulated volume
percentages were determined using the 3-D mesh data for each of the convex
hull fragments simulated in Unity 3D. For each event, the simulated volume
percentages for each of the slope locations was within 5 % of the actual
percentage, with the majority of the rockfall material ending up in the
track-side ditches for every rockfall event except the Goldpan wedge slide.
In the Goldpan case, Site A, we see two distinct areas of accumulation, on
the mid-slope bench and on top of the rock shed. In this case the simulation
results produced similar accumulations in both locations, with the majority
of the material leaving the slope over the edge of the rock shed.</p>

      <?xmltex \floatpos{p}?><fig id="Ch1.F15" specific-use="star"><?xmltex \currentcnt{15}?><label>Figure 15</label><caption><p id="d1e878">A comparison of the actual and simulated change detection results
from the 32 m<inline-formula><mml:math id="M32" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:math></inline-formula> flexural toppling event from White Canyon East, Site
C. The simulation produced a good comparison with the actual change
detection results, yielding a similar spatial distribution, and magnitude of
change. The percentage of initial source volume retained at various
locations on the actual and simulated slope is shown. The majority of
the material in both cases is retained in the track-side ditch. In the simulated
case a small amount of the simulated volume comes to rest on the slope
(0.5 %) and runs out into the track area (1.5 %).</p></caption>
        <?xmltex \igopts{width=355.659449pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/19/2385/2019/nhess-19-2385-2019-f15.png"/>

      </fig>

      <?xmltex \floatpos{p}?><fig id="Ch1.F16" specific-use="star"><?xmltex \currentcnt{16}?><label>Figure 16</label><caption><p id="d1e899">A comparison of the actual and simulated change detection results
from the 15 m<inline-formula><mml:math id="M33" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:math></inline-formula> planar sliding event from White Canyon West, Site D.
The simulation produced a good comparison with the actual change detection
results, yielding a similar spatial distribution, and magnitude of change.
The percentage of initial source volume retained at various locations on the
actual and simulated slope is shown. The majority of the material in both cases
is retained in the track-side ditch. In the simulated case, 1 % of the
volume reaches the track area.</p></caption>
        <?xmltex \igopts{width=384.112205pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/19/2385/2019/nhess-19-2385-2019-f16.png"/>

      </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F17" specific-use="star"><?xmltex \currentcnt{17}?><label>Figure 17</label><caption><p id="d1e919">A comparison of the actual and simulated change detection results
from the 8 m<inline-formula><mml:math id="M34" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:math></inline-formula> planar sliding event from White Canyon West, Site E.
The simulation produced a good comparison with the actual change detection
results, yielding a similar spatial distribution and magnitude of change.
The percentage of initial source volume retained at various locations on the
actual and simulated slope is shown. The majority of the material in both cases
is retained in the track-side ditch. In the simulated case a small amount of
the simulated volume comes to rest on the slope (1.5 %) and runs out into
the track area (1.5 %).</p></caption>
        <?xmltex \igopts{width=369.885827pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/19/2385/2019/nhess-19-2385-2019-f17.png"/>

      </fig>

<sec id="Ch1.S4.SS1">
  <label>4.1</label><title>Simulation with multiple parameterizations</title>
      <?pagebreak page2397?><p id="d1e944">In each of the above change-based simulation comparisons, a single model
iteration which produced a positive comparison to the observed change was
shown. The input parameters used to produce each comparison are not
identical, with variation between the five sites. For a single simulation, a
parameter set consisting of coefficients of dynamic friction, restitution,
and viscoplastic ground drag that best simulated the actual results was
chosen. The parameter sets used for each of the five site comparisons are
shown in Table 1.</p>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T1"><?xmltex \currentcnt{1}?><label>Table 1</label><caption><p id="d1e950">The material coefficients used for each of the five rockfall event
simulations. The fragmentation levels selected for the 15 simulation
iterations run for the White Canyon East wedge sliding event are also
included. Fric indicates Friction and Rest indicates Restitution.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="5">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="left"/>
     <oasis:colspec colnum="3" colname="col3" align="right"/>
     <oasis:colspec colnum="4" colname="col4" align="right"/>
     <oasis:colspec colnum="5" colname="col5" align="right"/>
     <oasis:thead>
       <oasis:row>
         <oasis:entry colname="col1"/>
         <oasis:entry rowsep="1" colname="col2">Coarse</oasis:entry>
         <oasis:entry rowsep="1" colname="col3">Medium</oasis:entry>
         <oasis:entry rowsep="1" colname="col4">Fine</oasis:entry>
         <oasis:entry colname="col5"/>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">Fragment no.</oasis:entry>
         <oasis:entry colname="col2">250</oasis:entry>
         <oasis:entry colname="col3">500</oasis:entry>
         <oasis:entry colname="col4">1000</oasis:entry>
         <oasis:entry colname="col5"/>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">Site</oasis:entry>
         <oasis:entry colname="col2">Material</oasis:entry>
         <oasis:entry colname="col3">Fric</oasis:entry>
         <oasis:entry colname="col4">Rest</oasis:entry>
         <oasis:entry colname="col5">Vpg</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Goldpan wedge slide</oasis:entry>
         <oasis:entry colname="col2">rock</oasis:entry>
         <oasis:entry colname="col3">0.5</oasis:entry>
         <oasis:entry colname="col4">0.4</oasis:entry>
         <oasis:entry colname="col5">0</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2">talus</oasis:entry>
         <oasis:entry colname="col3">0.35</oasis:entry>
         <oasis:entry colname="col4">0.3</oasis:entry>
         <oasis:entry colname="col5">0.15</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">White Canyon East</oasis:entry>
         <oasis:entry colname="col2">rock</oasis:entry>
         <oasis:entry colname="col3">0.45</oasis:entry>
         <oasis:entry colname="col4">0.25</oasis:entry>
         <oasis:entry colname="col5">0</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">wedge slide</oasis:entry>
         <oasis:entry colname="col2">talus</oasis:entry>
         <oasis:entry colname="col3">0.3</oasis:entry>
         <oasis:entry colname="col4">0.2</oasis:entry>
         <oasis:entry colname="col5">0.3</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">White Canyon East</oasis:entry>
         <oasis:entry colname="col2">rock</oasis:entry>
         <oasis:entry colname="col3">0.55</oasis:entry>
         <oasis:entry colname="col4">0.25</oasis:entry>
         <oasis:entry colname="col5">0</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">flexural topple</oasis:entry>
         <oasis:entry colname="col2">talus</oasis:entry>
         <oasis:entry colname="col3">0.45</oasis:entry>
         <oasis:entry colname="col4">0.2</oasis:entry>
         <oasis:entry colname="col5">0.3</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">White Canyon West</oasis:entry>
         <oasis:entry colname="col2">rock</oasis:entry>
         <oasis:entry colname="col3">0.5</oasis:entry>
         <oasis:entry colname="col4">0.3</oasis:entry>
         <oasis:entry colname="col5">0</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">planar slide 1</oasis:entry>
         <oasis:entry colname="col2">talus</oasis:entry>
         <oasis:entry colname="col3">0.4</oasis:entry>
         <oasis:entry colname="col4">0.2</oasis:entry>
         <oasis:entry colname="col5">0.3</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">White Canyon West</oasis:entry>
         <oasis:entry colname="col2">rock</oasis:entry>
         <oasis:entry colname="col3">0.45</oasis:entry>
         <oasis:entry colname="col4">0.3</oasis:entry>
         <oasis:entry colname="col5">0</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">planar slide 2</oasis:entry>
         <oasis:entry colname="col2">talus</oasis:entry>
         <oasis:entry colname="col3">0.35</oasis:entry>
         <oasis:entry colname="col4">0.25</oasis:entry>
         <oasis:entry colname="col5">0.3</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table></table-wrap>

      <p id="d1e1206">While a single parameter set can be selected, producing results which align
with the material accumulations seen in the change detection, we cannot be
certain that this parameter set will best reflect conditions at any given
site in the area. The friction, restitution, and damping coefficients used
are a simplification of a suite of interconnected and complex processes
which govern the loss of energy during collision between the rockfall and
slope. For example, variations in moisture content for a section of soil
affect slope deformation and therefore the transfer of energy which takes
place during collision (e.g. Vick, 2015). From a forward-modelling
perspective, while advances in rock slope monitoring have shown that we are
now able to detect pre-failure deformation for unstable sections of slopes
(e.g. Royan et al., 2013; Kromer et al., 2015, 2017), in some
cases providing time-to-failure estimates, we are not able to predict the
exact time at which a failure will occur. Therefore, in terms of material
parameters, we cannot know the exact state of the slope when runout will
take place. For this reason, it makes sense that a range of potential
material coefficients be used to capture the variability in these
parameters.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F18" specific-use="star"><?xmltex \currentcnt{18}?><label>Figure 18</label><caption><p id="d1e1212">Results of the 15 simulations run for the 24 m<inline-formula><mml:math id="M35" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:math></inline-formula> wedge
sliding event at White Canyon East, Site B. Each point represents the end
point of a simulated fragment in one of the 15 simulations. The envelope of
red points indicates the runout of 95 % of the simulated volume, with the
purple and blue portions representing envelopes containing the additional
4 % and 1 % of the material, respectively.</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/19/2385/2019/nhess-19-2385-2019-f18.png"/>

        </fig>

      <p id="d1e1230">Similarly, for forward modelling of events based on pre-failure deformation
or precursor rockfall, the exact volume of a failure would not be known
prior to the event. While volume estimates based on structure in the source
rock mass are possible (e.g. Lambert et al., 2012; e.g. Salvini et al.,
2013), they require assumptions about joint persistence and shape. As a
result, it would be advisable to estimate a range of potential volumes using
the least and most conservative<?pagebreak page2398?> persistence estimates. Additionally, while
we may be able to identify potential failure events, and even estimate block
volume from visible structure, we won't know the degree of fracturing
expected as part of the disaggregation of the source volume. With this in
mind, it is important that we also use a range of fragmentation values as
well, in this case termed coarse, medium, and fine. The use of a suite of
material coefficients, volumes, and levels of fragmentation allows us to
produce an envelope of potential rockfall runout rather than a single
deterministic result.</p>
      <p id="d1e1233">An example suite of simulations has been produced for the 24 m<inline-formula><mml:math id="M36" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:math></inline-formula>
overhanging wedge failure at White Canyon East, Site B. Varying source
volumes were not used in this case as the rockfall has already occurred, and
the source volume is therefore known. The material coefficients used were
based on the five parameter sets from Table 1, each of which produced a
positive comparison at one of the five sites. These five material
parameterizations were each run for three levels of fragmentation (250
fragments, 500 fragments, 1000 fragments) produced using Voronoi fracturing
in Blender. The distribution of potential rockfall runout for the event was
produced for each of these 15 simulations. Each point shown on the slope
surface in Fig. 18 is the end position of a fragment from one of the 15 simulations. The red points represent the runout of 95 % of the simulated
volume. This boundary illustrates that the majority of the material from the
event, based on 15 different simulation parameterizations, is retained by
the track-side ditch. This result compares well with the actual change
detection from the event, in which all of the rockfall material appears to
have come to rest in the gully above track or in the track-side ditch. The
99 % (purple) and 100 % (blue) runout boundaries are also shown,
illustrating that a portion of the additional 5 % of simulated material
does come to rest in the track area.</p>
</sec>
<sec id="Ch1.S4.SS2">
  <label>4.2</label><title>Volume comparisons and ditch design</title>
      <p id="d1e1253">From an engineering design perspective, one application of this simulation
technique is the assessment of mitigation performance. The simulation of a
fragmental rockfall event as a single large block overestimates potential
impact energies and underestimates the spatial distribution of impacts
possible when rockfall volumes run out as hundreds or thousands of
individual, interacting fragments. The simulation of<?pagebreak page2399?> rockfall volumes as a
collection of free-moving fragments allows us to produce more realistic
material accumulations in retaining ditches adjacent to the track.</p>
      <p id="d1e1256">Using the 15 simulations run for the 24 m<inline-formula><mml:math id="M37" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:math></inline-formula> White Canyon East wedge
sliding event, Site B, we can analyze the distribution of accumulated
material along the slope surface. Figure 19 shows the same end point
locations as in Fig. 18 but in section view. Also included is a plot
displaying the volume of material accumulated along the slope surface. From
this distribution we observe a notable peak in volume occurring at the
location of the track-side ditch. This style of volume accumulation curve
allows us to visualize the effectiveness of countermeasures at retaining
material. In preparation for an expected rockfall event, or during the
construction of new ditches along a section of railway or highway, this
analysis could be used to evaluate the effectiveness of different ditch
shapes or the use of simple retaining structures like lock blocks.
Additionally, the retention capacity and the effectiveness of
countermeasures, as material progressively accumulates, could be tested.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F19"><?xmltex \currentcnt{19}?><label>Figure 19</label><caption><p id="d1e1270">A section view of the 15 simulation
iterations run for the 24 m<inline-formula><mml:math id="M38" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:math></inline-formula> wedge sliding event at White Canyon East, Site B. <bold>(a)</bold> shows
the accumulation of simulated fragments across the section. The notable peak
visible at 270 m is in alignment with the location of the track-side
catchment ditch, as shown in <bold>(b)</bold>.</p></caption>
          <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/19/2385/2019/nhess-19-2385-2019-f19.png"/>

        </fig>

      <p id="d1e1295">In the initial 15 simulations run for the White Canyon East wedge sliding
event, the pre-failure slope surface was used in order to examine the match
between the simulated and actual conditions on the slope during runout. We
can also re-run these 15 simulations using the post-failure slope surface.
In this case, the ditch area is full of debris and large rockfall fragments
from the 24 m<inline-formula><mml:math id="M39" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:math></inline-formula> event, representing a ditch near full retention
capacity. The simulation results using the post-failure surface conditions
can be seen in Fig. 20, compared to the initial pre-failure analysis. From
this we can see that the 95 % volume-runout boundary has moved closer to
the track for the full ditch scenario, with some end points now touching the
track boundary. A comparison of the two volume accumulation profiles for
these different ditch scenarios can be seen in Fig. 21. Two vertical lines
indicate the location of the 95 % volume-runout boundary for the two
curves, with the red line indicating the start of the track area. The use of
the post-failure, full ditch slope model resulted in the 95 % boundary
moving forward 1.2 m, illustrating a decrease in the effectiveness of the
ditch at stopping material when full. From a back-analysis perspective this
effect on runout illustrates the importance of using the true pre-failure
slope conditions for our simulation comparisons. From a forward analysis
perspective, it may not be possible to know the state of the ditch during
the runout event, and therefore different ditch conditions should be
simulated in order to assess the range of possible outcomes when evaluating
countermeasure options.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F20" specific-use="star"><?xmltex \currentcnt{20}?><label>Figure 20</label><caption><p id="d1e1309">Comparison of the 15 simulation iterations of the 24 m<inline-formula><mml:math id="M40" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:math></inline-formula> wedge sliding event at Site B using the pre-fall (empty) and post-fall
(full) ditch geometries. In the full ditch scenario the 95 % and 99 %
runout boundaries have shifted further forward into the track area,
indicating a decreased effectiveness in the ditch at stopping material from
reaching the track.</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/19/2385/2019/nhess-19-2385-2019-f20.png"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F21"><?xmltex \currentcnt{21}?><label>Figure 21</label><caption><p id="d1e1329">The distribution of simulated volume for the pre-fall and
post-fall ditch geometries is shown. The vertical grey and black lines
indicate the 95 % volume-runout boundaries for the two cases. Simulation
using the post-fall (full) ditch geometry results in the 95 %
volume-runout boundary shifting 1.2 m closer to the inside rail.</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/19/2385/2019/nhess-19-2385-2019-f21.png"/>

        </fig>

      <p id="d1e1338">A comparison of the percentage of rockfall volume retained in different
areas of the model for the empty and full ditch scenarios is shown in Fig. 22. Simulation using the post-fall ditch geometry results in almost twice as
much material reaching track level. Additionally, we can look at the size
distribution of the fragments which end up in the track area, as shown in
Fig. 22 for the full ditch scenario. The use of volume-based runout
envelopes takes into consideration both the size and number of fragments
which reach the track. Different-sized fragments have different implications
from a hazard management perspective. For example, in the CN Rockfall Hazard
Risk Assessment framework (Abbot et al., 1998a, b), rockfall fragments
with maximum dimensions of 0.3–1 m are noted as the sizes most likely to
cause derailments due to their potential to get wedged underneath a train
car. Of the 11 % of simulated fragments which reach the track in the 15 simulations of the full ditch scenario, approximately 57 % of them fall
within the 0.3–1 m size range.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F22" specific-use="star"><?xmltex \currentcnt{22}?><label>Figure 22</label><caption><p id="d1e1344">A schematic overview of the volume percentages stopping at
different locations for the 15 simulation iterations using the empty and
full ditch geometries. Simulation using the full ditch geometry resulted in
nearly twice as much material reaching track level. The distribution of the
grain sizes which reached track level in the full ditch scenario is also
shown.</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/19/2385/2019/nhess-19-2385-2019-f22.png"/>

        </fig>

</sec>
</sec>
<sec id="Ch1.S5">
  <label>5</label><title>Limitations</title>
      <p id="d1e1363">The objective of this work was to demonstrate the ability of our rockfall
simulation workflow to model complex rockfall source geometries comprised of
many moving fragments. While this process is a step forward in the
simulation of fragmental rockfall events, a discussion of current
limitations is important. The two main limitations of this work are
fragmentation timing and the distribution and size of rockfall fragments
used.</p><?xmltex \hack{\newpage}?>
<?pagebreak page2400?><sec id="Ch1.S5.SS1">
  <label>5.1</label><title>Fragmentation timing</title>
      <p id="d1e1374">The events modelled in this paper were not observed directly, and therefore
it is not possible, using the available TLS data and site photographs, to
understand at what point fragmentation took place during the event. While
the post-fall accumulations visible in the photos and change detection
indicate that the final state of the source volumes were deposits of coarse
rock fragments, the transition from coherent rock mass to thousands of
fragments could have occurred immediately at the time of detachment, or as a
result of impact during the first or subsequent collisions between the
source volume and slope surfaces.</p>
      <p id="d1e1377">The current methodology simulates the release of rock from the source zone
as a gravity-induced, rapid unravelling of highly jointed material (Fig. 23a). It is possible that this unravelling of jointed rock mass could have
instead occurred slowly over time as small isolated events (Fig. 23b).
Alternatively, the separation of the source mass into individual blocks
could have occurred as a result of loading during impact (Fig. 23c). At
the same time, the decision to model the events as a rapid disaggregation of
jointed rock was not arbitrary. This style of fragmentation is akin to the
disaggregation-without-breakage rockfall mechanism described by Ruiz-Carulla
et al. (2016a), in which the rockfall body separates along discontinuities
present in the source rock mass, with no breakage of individual,
discontinuity-bounded blocks. This appears to be the dominant behaviour in
the railway rock slope video shown in Fig. 10. This type of rock mass
behaviour is also observed in low-stress underground excavations, in which
structurally controlled failures of highly jointed or crushed rock will
unravel from<?pagebreak page2401?> excavation ceilings under the influence of gravity (Palmström,
1995).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F23"><?xmltex \currentcnt{23}?><label>Figure 23</label><caption><p id="d1e1382">Comparison of potential timing of rock mass fragmentation, which could
have taken place for the events discussed. Red blocks indicate material
which breaks away from the initial source volume at a given time.</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/19/2385/2019/nhess-19-2385-2019-f23.png"/>

        </fig>

      <p id="d1e1392">The choice to model the events as a rapid unravelling of the entire source
volume (Fig. 22a) was also inherently influenced by the current capabilities
of the modelling technique. In Sala (2018), the possibility to connect
simulated fragments in the source mass using strength-based object-to-object
connections was briefly discussed. Each simulated connection between objects
can be assigned a strength value, with the connection broken when this
threshold is exceeded. The use of these connections could facilitate future
simulations in which the source mass does not disaggregate immediately but
instead as a result of force from impact. While this is one potential method
for simulating break-up of the source volume during runout, field data to
support the calibration of these connections are not currently available.</p>
</sec>
<sec id="Ch1.S5.SS2">
  <label>5.2</label><title>Fragment size distribution</title>
      <p id="d1e1403">One of the goals of modelling rockfall source volumes as a collection of
rock fragments was to better capture the size of mobile fragments involved
in the rockfall events rather than using a single large block. While this
effect was achieved using our modelling workflow, it should be noted that an
evaluation of actual versus simulated grain size distribution has not been
completed.</p>
      <p id="d1e1406">At this time, Voronoi fracturing is used for source volume fragmentation. In
3-D this method partitions the source mesh into disjointed convex polyhedra,
based on seed points distributed in the mesh volume (Ledoux, 2007). Several
parameters can be set in the fracturing algorithm including the recursive
partitioning of larger fragments and control over fragment shape. While the
use of this method is capable of rapidly creating fragmented 3-D volumes,
ready for use inside the Unity game engine, the fracture network produced is
not based on actual discontinuities in the rock mass. For rock masses which
are less jointed, discontinuity planes can be used in Blender to separate
the source volume into blocks based on discrete joints mapped from available
imagery or 3-D models of the slope. In the case of the White Canyon and
Goldpan events, where hundreds to thousands of fragments were visible in the
post fall accumulations, the mapping of discrete joint planes was not
practical. For these cases the use of Voronoi fracture networks, instead of
discrete joint planes,<?pagebreak page2402?> permitted us to model the sheer number of fragments
present in the rockfall deposits.</p>
      <p id="d1e1409">The size of the fragments deposited during the five rockfall events is
clearly not unimodal, with a variety of grain sizes present. Grain size
distributions for these events were not created due to a lack of adequate
data. Point spacing in the TLS data is too sparse to be able to isolate
individual grains. Additionally, vantage points from our scan sites often
result in notable occlusions at the track level, resulting in missing data
in the post-fall debris piles. Photos of the events do capture the post-fall
debris, but due to the oblique angle of the images, and homogenous colour of
the material, accurate image-based grain segmentation is challenging.</p>
      <p id="d1e1412">A select few fragments measured for the White Canyon East 24 m<inline-formula><mml:math id="M41" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:math></inline-formula> case,
Site B, show approximate sizes ranging from 1.6 to <inline-formula><mml:math id="M42" display="inline"><mml:mrow><mml:mi mathvariant="italic">&lt;</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mn mathvariant="normal">0.05</mml:mn></mml:mrow></mml:math></inline-formula> m.
Particles smaller than 5 cm are clearly present but cannot be measured as
the images are too noisy at this scale due to resolution limitations. Size
ranges for the coarsest models (250 fragments) and finest models (1000 fragments) of the 24 m<inline-formula><mml:math id="M43" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:math></inline-formula> event were 0.09–0.8 m and 0.02–0.6 m
respectively. While we do not have a full grain size distribution for the
actual event, we can see from these measurements that the grain sizes
produced using the current Voronoi fracture parameters underestimate the
largest block sizes and result in an overall smaller range of values. In
terms of the smaller grains, the 2 cm minimum size of the 1000 fragment
model is sufficient to capture the lower size limit of the 24 m<inline-formula><mml:math id="M44" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:math></inline-formula> event.
Ultimately more investigation needs to be done into fine-tuning the
parameters of the Voronoi fracturing process in order to produce grain sizes
with a broader range of values and that more accurately reflect the sizes
produced by events in our study area. In order to do this, complete grain
size distributions for events in our rockfall database, and from other
events in the literature, will need to be generated.</p>
</sec>
</sec>
<sec id="Ch1.S6" sec-type="conclusions">
  <label>6</label><title>Conclusions</title>
      <p id="d1e1462">Five rockfall simulations were run based on TLS change detection inputs from
events identified at our field sites in south-central British Columbia. The
simulations utilized high-resolution 3-D meshes generated from 6–10 cm TLS
point clouds, and complex rockfall volumes, extracted from pre- and
post-event scans. The fracturing of source rockfall volumes enabled the
modelling of fragmental rockfall runout, taking into consideration the
interaction of fragments with each other as well as slope-stopping features
such as gullies and ditches. The results of this work demonstrate the
ability of our rockfall modelling prototype to produce runout material
accumulations which agree well with observed change from the actual events.
With no direct observations of rockfall runout, or on-site measurement, the
conversion of post-simulation mesh data in order to produce simulated change
detection presents a novel way to perform rockfall runout comparisons in the
absence of other data types.</p>
      <p id="d1e1465">The application of the technique to mitigation design was also discussed,
demonstrating the potential of the model to be used for investigating the
effectiveness of rockfall catchment ditches. This type of analysis,
visualizing the accumulation of rockfall runout volume downslope, could also
be applied to the assessment of other countermeasure options such as lock
block retaining walls or rock sheds. The ability to perform these types of
analyses is limited in industry standard rockfall modelling programs, as
they are often able to simulate only a single moving block at a time. While
these models are very useful for single block falls, and regional runout
assessments, they are unable to capture the build-up of rockfall material on
the slope, which can affect the path of subsequent rockfall fragments and
the effectiveness of retaining structures. The simulation of these falls as
multiple moving bodies in our technique is able to capture this interaction
between rockfall material and the finite capacity of the structures used for
rockfall protection.</p>
</sec>

      
      </body>
    <back><notes notes-type="dataavailability"><title>Data availability</title>

      <p id="d1e1472">The underlying research data for this project cannot be made publicly
available as they are commercially sensitive and permission must be granted
by our industry partners to access the data. Sample code and descriptions of
how to set up rockfall simulations using the Unity 3D software can be found in
Sala (2018, <uri>https://qspace.library.queensu.ca/handle/1974/24940</uri>).</p>
  </notes><notes notes-type="authorcontribution"><title>Author contributions</title>

      <p id="d1e1481">ZS was responsible for the development of the fragmental rockfall
simulations and analysis of simulated and actual change detection results.
DJH provided technical guidance on the framework of the study and the
overall goals of the work in the context of railway hazard management. RH
provided technical guidance on the development of the game-engine simulation
and analysis techniques presented. ZS was responsible for manuscript
preparation. DJH and RH reviewed and edited the manuscript.</p>
  </notes><notes notes-type="competinginterests"><title>Competing interests</title>

      <p id="d1e1487">The authors declare that they have no conflicts of interest.</p>
  </notes><ack><title>Acknowledgements</title><p id="d1e1493">This research work was supported by the Railway Ground Hazards Research
Program, funded by CN Rail, Canadian Pacific and an NSERC CRD grant, and
supported by Transport Canada and the Geological Survey of Canada. Special
thanks to the members of the Queen's University RGHRP group who participated in the
collection of the data used for this research, to Trevor Evans of CN for field
campaign support and expertise related to railway operations, and to Dave
Gauthier for regular discussion surrounding the technical and written
components of this work.</p></ack><notes notes-type="financialsupport"><title>Financial support</title>

      <p id="d1e1498">This research has been supported by the NSERC (grant no. 470162).</p>
  </notes><notes notes-type="reviewstatement"><title>Review statement</title>

      <p id="d1e1504">This paper was edited by Oded Katz and reviewed by two anonymous referees.</p>
  </notes><ref-list>
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    <!--<article-title-html>Simulation of fragmental rockfalls detected using terrestrial laser scans from rock slopes in south-central  British Columbia, Canada</article-title-html>
<abstract-html><p>Rockfall presents an ongoing challenge to the safe
operation of transportation infrastructure, creating hazardous conditions
which can result in damage to roads and railways, as well as loss of life.
Rockfall risk assessment frameworks often involve the determination of
rockfall runout in an attempt to understand the likelihood that rockfall
debris will reach an element at risk. Rockfall modelling programs which
simulate the trajectory of rockfall material are one method commonly used to
assess potential runout. This study aims to demonstrate the effectiveness of
a rockfall simulation prototype which uses the Unity 3D game engine. The
technique is capable of simulating rockfall events comprised of many mobile
fragments, a limitation of many industry standard rockfall modelling
programs. Five fragmental rockfalls were simulated using the technique, with
slope and rockfall geometries constructed from high-resolution terrestrial
laser scans. Simulated change detection was produced for each of the events
and compared to the actual change detection results for each rockfall as a
basis for testing model performance. In each case the simulated change
detection results aligned well with the actual observed change in terms of
location and magnitude. An example of how the technique could be used to
support the design of rockfall catchment ditches is shown. Suggestions are
made for future development of the simulation technique with a focus on
better informing simulated rockfall fragment size and the timing of
fragmentation.</p></abstract-html>
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