<?xml version="1.0" encoding="UTF-8"?>
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<article xmlns:xlink="http://www.w3.org/1999/xlink" xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:oasis="http://docs.oasis-open.org/ns/oasis-exchange/table" xml:lang="en" dtd-version="3.0"><?xmltex \makeatother\@nolinetrue\makeatletter?>
  <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-18-1013-2018</article-id><title-group><article-title>Pre-seismic anomalies from optical satellite <?xmltex \hack{\break}?>observations: a review</article-title><alt-title>Pre-seismic anomalies</alt-title>
      </title-group><?xmltex \runningtitle{Pre-seismic anomalies}?><?xmltex \runningauthor{Z.-H.~Jiao et al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes" rid="aff1">
          <name><surname>Jiao</surname><given-names>Zhong-Hu</given-names></name>
          <email>jiaozhh@gmail.com</email>
        <ext-link>https://orcid.org/0000-0002-5168-9683</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Zhao</surname><given-names>Jing</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Shan</surname><given-names>Xinjian</given-names></name>
          
        </contrib>
        <aff id="aff1"><label>1</label><institution>State Key Laboratory of Earthquake Dynamics, Institute of Geology,
China Earthquake <?xmltex \hack{\break}?>Administration, Beijing 100029, China</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>Harbin Institute of Technology Shenzhen Graduate School, Shenzhen
518000, China</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Zhong-Hu Jiao (jiaozhh@gmail.com)</corresp></author-notes><pub-date><day>4</day><month>April</month><year>2018</year></pub-date>
      
      <volume>18</volume>
      <issue>4</issue>
      <fpage>1013</fpage><lpage>1036</lpage>
      <history>
        <date date-type="received"><day>11</day><month>June</month><year>2017</year></date>
           <date date-type="rev-request"><day>20</day><month>July</month><year>2017</year></date>
           <date date-type="rev-recd"><day>3</day><month>February</month><year>2018</year></date>
           <date date-type="accepted"><day>17</day><month>February</month><year>2018</year></date>
      </history>
      <permissions>
        
        
      <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>
    <p id="d1e108">Detecting various anomalies using optical satellite data
prior to strong earthquakes is key to understanding and forecasting
earthquake activities because of its recognition of thermal-radiation-related phenomena in seismic preparation phases. Data from
satellite observations serve as a powerful tool in monitoring earthquake
preparation areas at a global scale and in a nearly real-time manner. Over
the past several decades, many new different data sources have been utilized
in this field, and progressive anomaly detection approaches have been
developed. This paper  reviews the progress and development of
pre-seismic anomaly detection technology in this decade. First, precursor
parameters, including parameters from the top of the atmosphere, in the
atmosphere, and on the Earth's surface, are stated and discussed. Second,
different anomaly detection methods, which are used to extract anomalous
signals that probably indicate future seismic events, are presented.
Finally, certain critical problems with the current research are
highlighted, and new developing trends and perspectives for future work are
discussed. The development of Earth observation satellites and anomaly
detection algorithms can enrich available information sources, provide
advanced tools for multilevel earthquake monitoring, and improve short- and
medium-term forecasting, which  play a large and growing role in
pre-seismic anomaly detection research.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

      <?xmltex \hack{\newpage}?>
<sec id="Ch1.S1" sec-type="intro">
  <title>Introduction</title>
      <p id="d1e120">The earthquake is one of the most devastating and catastrophic natural
disasters and exposes human beings to tremendous risks (Geiß and
Taubenböck, 2013). Therefore, strengthening the monitoring research of
seismic activities using different technical means is necessary. Since the
1970s, remote sensing technology has been applied to seismic monitoring. In
the 1980s, thermal infrared (TIR) satellite data were used for the first
time to analyze thermal anomalies prior to earthquakes (Gorny et al., 1988;
Tronin, 1996). Earthquake monitoring based on passive or active remote
sensing data is considered a promising research area by the
international seismology and remote sensing community (Tronin, 2010),
having the advantages of interdisciplinary research and being a new
exploratory technology and tool.</p>
      <p id="d1e123">Satellite remote sensing has its own advantages compared to traditional
approaches of seismic hazard monitoring. Ground stations dedicated to
earthquake monitoring are spatially relatively sparse; thus, their
capability to monitor crustal movement and seismic information is limited.
Meanwhile, global remote sensing data with high spatiotemporal resolution
can be obtained through the advances in satellite technology. Satellite TIR
data are a considerably reliable data source that exhibit  continuity,
stability, and accessibility. These data allow the study of the phenomena of
large-scale and fast-changing seismic thermal anomalies. Satellite anomaly
recognition can quickly capture the anomalies on the macroscopic scale,
which contains thermal information of the Earth's interior caused by the
crustal movement. Moreover, satellite data can reveal large-scale linear
structures and short-term (i.e., from days to weeks) variations of<?pagebreak page1014?> thermal
anomalies over tectonic plate borders and active faults (Filizzola et al.,
2004; Tramutoli et al., 2005; Tronin et al., 2004). After more than 30 years
of research, cases of anomalies monitored by satellite remote sensing
gathered from a large number of earthquakes have been repeatedly tested and
verified. Results show that different anomalies are present in seismogenic
areas before earthquakes with the medium or strong magnitude.</p>
      <p id="d1e126">The sudden dislocation of active faults due to surging tectonic stress
causes tectonic earthquakes. In addition to the considerable amount of
strain energy released during the earthquake itself, the elastic energy
continuously accumulates during the preparation process of the earthquake.
Different theories to explain the physical mechanism of the pre-seismic
anomalies derived from optical satellite data have been proposed. The <inline-formula><mml:math id="M1" display="inline"><mml:mi>p</mml:mi></mml:math></inline-formula>-hole
model (Freund, 2011; Freund et al., 2009) indicates that electronic charge
carriers, also known as positive holes, in crustal rocks are activated by
tectonic stress and flow out of the stressed rock volume and propagate
fleetly. They cause air ionization at the land surface–atmosphere interface
accumulated in a thin surface/subsurface layer and generate
non-thermal infrared emission as a result of the recombination of positive
holes. The rock stress adjustment from active faults probably causes
anomalies of land surface or air temperatures prior to the earthquake, which
could be observed through satellite TIR sensors (Chen et al., 2015; Ren et
al., 2017; Wu et al., 2006). The spatiotemporal evolution of the rock
temperature field is closely related to its deformation. The rock
compression causes the obvious increase of temperature, and rock tension
gives rise to temperature decrease. The solid Earth is about 1650 times of
thermal capacity of the atmosphere. The change of elastic stress of 1 MPa is
likely to bring in the variation of air temperature with the order of 1 K
based on the energy balance. The local greenhouse effect due to the
emanation of CO<inline-formula><mml:math id="M2" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, CH<inline-formula><mml:math id="M3" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula>, etc. has been invoked to explain the
anomalous variations of top-of-atmosphere (TOA) brightness temperature (BT) or
outgoing longwave radiation (OLR) (Ouzounov et al., 2006, 2007; Tronin et al., 2002).
Besides, the increased emission of radon from
active faults and cracks in seismogenic regions is also considered to bring
about  air ionization, which can concentrate water molecules on air ions,
further lead to the anomalies of the atmospheric water vapor and
temperature, and accelerate the latent heat flux before earthquakes
(Pulinets et al., 2006b). It should be noted that the <inline-formula><mml:math id="M4" display="inline"><mml:mi>p</mml:mi></mml:math></inline-formula>-hole model and
temperature response to stress–strain variations in rock are based on
rigorous laboratory experiments. However, when these theories are extended
to the field environment, there are too many factors that influence the
results. In particular, it is difficult to verify these theories, which
hinders forming a complete logical chain. Therefore, much further work must be carried out to apply this mechanism in the very complex field
environment. Other theories also face a similar situation.</p>
      <p id="d1e161">Despite lots of promising research results about pre-seismic anomalies, the
anomaly detection approach is still met with skepticism and controversies
(Geller, 2011; Wyss 1997), because early warning signals from
earthquake-prone regions are diverse, subtle, and often transient. Moreover,
this approach is generally applied with some serious misjudgments and misses
earthquake prediction due to the weak physical basis of pre-seismic
anomalies and perturbations from surface and atmospheric conditions and
human activities (Tronin, 2010). Furthermore, the transfer process of
surface thermal radiation is considerably complex, and numerous factors that
affect the TIR radiation are highly varied. The recognition of pre-seismic
anomalies can be significantly hindered by topography, vegetation, soil
moisture, surface type, and atmospheric conditions. Therefore, various
anomalies caused by seismic activities sink into the background with various
other factors and are considerably weak relative to the surface or
atmospheric thermal radiative variations caused by other natural or
anthropogenic changes and thus can hardly be discerned. Seismic precursor
identification has not yet formed an objective, stable, and verifiable
anomaly detection method; thus, it has not been completely accepted by the
seismic community.</p>
      <p id="d1e165">This paper attentively reviews the advances in pre-seismic anomaly
monitoring through satellite technology mainly over the last decade in terms
of possible earthquake precursors and anomaly detection approaches. Besides,
it is noted that reanalysis datasets can also be used in the anomaly
analyses as mentioned in some studies below. These datasets are created via
geophysical models and data assimilation scheme with spatial continuity and
relatively low spatial resolution. The satellite products and reanalysis
data provide abundant data in this domain. Although inherent physical
problems are always present, this work provides some assistants for attempts
to detect pre-seismic anomalies using satellite datasets.</p>
      <p id="d1e168">The rest of this paper is organized as follows. Section 2 presents the
geophysical variables used for pre-earthquake anomaly detection in a number
of earthquake case studies. Section 3 describes several types of anomaly
detection methods, their basic properties, and recent applications. Section
4 discusses the issues around the pre-seismic anomaly identification by
satellite data products, which prove to be essential hindrances in
earthquake prediction. Finally, Section 5 presents the expected development
and perspectives for the next decades based on the review of current
research status and trend, as well as analysis of existing problems in this domain.</p>
</sec>
<sec id="Ch1.S2">
  <title>Possible seismic precursors</title>
      <p id="d1e177">All types of signals from the Earth–atmosphere system before strong
earthquakes have been analyzed in a large amount of literature. The possible
earthquake precursors used for<?pagebreak page1015?> the anomaly detection involve various
geophysical variables, such as seismic wave velocity, surface deformations,
gravity, geoelectricity, geomagnetism, groundwater chemistry, temperature,
moisture, atmospheric composition, and ionospheric parameters (Cicerone et
al., 2009; Tronin, 2006). Nevertheless, the pre-seismic anomaly analysis of
precursors at a global scale and of high time frequency has to rely heavily
on satellite remote sensing datasets.</p>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T1" specific-use="star"><caption><p id="d1e183">The precursor parameters discussed in following sections.</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">Level</oasis:entry>  
         <oasis:entry colname="col2">Parameter</oasis:entry>  
         <oasis:entry colname="col3">Specific variables</oasis:entry>  
         <oasis:entry colname="col4">Unit</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>  
         <oasis:entry colname="col1">TOA</oasis:entry>  
         <oasis:entry colname="col2">brightness temperature</oasis:entry>  
         <oasis:entry colname="col3">–</oasis:entry>  
         <oasis:entry colname="col4">K</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">  
         <oasis:entry colname="col1"/>  
         <oasis:entry colname="col2">OLR</oasis:entry>  
         <oasis:entry colname="col3">–</oasis:entry>  
         <oasis:entry colname="col4">W m<inline-formula><mml:math id="M5" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">In the atmosphere</oasis:entry>  
         <oasis:entry colname="col2">atmospheric water vapor</oasis:entry>  
         <oasis:entry colname="col3">total column water vapor</oasis:entry>  
         <oasis:entry colname="col4">cm</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1"/>  
         <oasis:entry colname="col2">atmospheric temperature</oasis:entry>  
         <oasis:entry colname="col3">screen-level air temperature</oasis:entry>  
         <oasis:entry colname="col4">K</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1"/>  
         <oasis:entry colname="col2">atmospheric trace gases</oasis:entry>  
         <oasis:entry colname="col3">CH<inline-formula><mml:math id="M6" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula>, CO<inline-formula><mml:math id="M7" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, CO, and O<inline-formula><mml:math id="M8" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula></oasis:entry>  
         <oasis:entry colname="col4">–</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">  
         <oasis:entry colname="col1"/>  
         <oasis:entry colname="col2">aerosols</oasis:entry>  
         <oasis:entry colname="col3">aerosol optical depth (AOD)</oasis:entry>  
         <oasis:entry colname="col4">–</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">At the Earth's surface</oasis:entry>  
         <oasis:entry colname="col2">surface latent heat flux (SLHF)</oasis:entry>  
         <oasis:entry colname="col3">–</oasis:entry>  
         <oasis:entry colname="col4">W m<inline-formula><mml:math id="M9" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1"/>  
         <oasis:entry colname="col2">land surface temperature</oasis:entry>  
         <oasis:entry colname="col3">–</oasis:entry>  
         <oasis:entry colname="col4">K</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1"/>  
         <oasis:entry colname="col2">sea surface temperature</oasis:entry>  
         <oasis:entry colname="col3">–</oasis:entry>  
         <oasis:entry colname="col4">K</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table><table-wrap-foot><p id="d1e186">Note: the en dash (–) indicates no specific variable or unit.</p></table-wrap-foot></table-wrap>

      <p id="d1e402">This paper focuses on several widely studied anomalies associated with
seismic activities from abovementioned datasets. In the 1980s, after the
discovery of thermal anomalies prior to earthquakes, seismic experts
gradually realized the advantages of TIR remote sensing and conducted
relevant studies. For more than 30 years, many geophysical variables, which
can reflect thermal radiation information about the Earth's surface and/or
atmosphere using satellite observations and products (e.g., TOA BT, OLR, surface temperature, and latent heat flux), have been used
to find a correlation between different anomalies and specifications of
time, location, and magnitude of imminent earthquakes. The following sections
contain detailed explanations about these candidate physical quantities
(Table 1) – from TOA to the atmosphere to the Earth's surface – and their
applications in the pre-seismic anomaly analyses.</p>
      <p id="d1e405">A comprehensive table is shown in Table 2 that contains the possible
pre-seismic precursors, the satellite sensors that can retrieve theses
parameters, the spatial and temporal resolutions of these data, and their
retrieval precision. We select some sensors that are still in operation,
have high quality and abundant products, and are widely used in remote sensing
community.</p>
<sec id="Ch1.S2.SS1">
  <title>TOA brightness temperature and OLR</title>
      <p id="d1e414">The TOA BT is a measurement of the radiance of the
TIR radiation at 3–5 <inline-formula><mml:math id="M10" display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>m or 8–14 <inline-formula><mml:math id="M11" display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>m from the Earth's surface,
atmosphere, and clouds to satellite sensors. It is a direct and fundamental
physical quantity expressed by the equivalent blackbody temperature of one
channel (e.g., 11.77–12.27 <inline-formula><mml:math id="M12" display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>m band) in Kelvin. In other words, BT is
not the normal temperature due to ignoring the emissivity effect. Many
satellite sensors obtain TIR measurements, such as the Moderate Resolution
Imaging Spectroradiometer (MODIS), Visible Infrared Imaging Radiometer Suite
(VIIRS), and Advanced Very High Resolution Radiometer (AVHRR) aboard
polar-orbiting satellites and Spinning Enhanced Visible and Infrared Imager
(SEVIRI) and Advanced Himawari Imager (AHI) aboard geostationary satellites.</p>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T2" specific-use="star"><caption><p id="d1e441">A description of different possible pre-seismic precursors derived
from different satellite sensors.</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="left"/>
     <oasis:colspec colnum="5" colname="col5" align="left"/>
     <oasis:thead>
       <oasis:row>  
         <oasis:entry colname="col1">Parameter</oasis:entry>  
         <oasis:entry colname="col2">Satellite</oasis:entry>  
         <oasis:entry colname="col3">Spatial</oasis:entry>  
         <oasis:entry colname="col4">Temporal</oasis:entry>  
         <oasis:entry colname="col5">Precision</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">  
         <oasis:entry colname="col1"/>  
         <oasis:entry colname="col2">sensor</oasis:entry>  
         <oasis:entry colname="col3">resolution</oasis:entry>  
         <oasis:entry colname="col4">resolution</oasis:entry>  
         <oasis:entry colname="col5"/>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>  
         <oasis:entry colname="col1"/>  
         <oasis:entry rowsep="1" colname="col2">MODIS</oasis:entry>  
         <oasis:entry rowsep="1" colname="col3">1 km</oasis:entry>  
         <oasis:entry rowsep="1" colname="col4">4 per day</oasis:entry>  
         <oasis:entry rowsep="1" colname="col5">NE<inline-formula><mml:math id="M15" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:msup><mml:mi>T</mml:mi><mml:mo>∗</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula> 0.05 K for band 31</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1"/>  
         <oasis:entry colname="col2"/>  
         <oasis:entry colname="col3">345 m</oasis:entry>  
         <oasis:entry colname="col4"/>  
         <oasis:entry colname="col5">NE<inline-formula><mml:math id="M16" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>T</mml:mi></mml:mrow></mml:math></inline-formula> 0.07 K for band M15;</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">Brightness</oasis:entry>  
         <oasis:entry rowsep="1" colname="col2">VIIRS</oasis:entry>  
         <oasis:entry rowsep="1" colname="col3">/750 m</oasis:entry>  
         <oasis:entry rowsep="1" colname="col4">2 per day</oasis:entry>  
         <oasis:entry rowsep="1" colname="col5">NE<inline-formula><mml:math id="M17" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>T</mml:mi></mml:mrow></mml:math></inline-formula> 1.5 K for band I5</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">temperature</oasis:entry>  
         <oasis:entry rowsep="1" colname="col2">SEVIRI</oasis:entry>  
         <oasis:entry rowsep="1" colname="col3">2 km</oasis:entry>  
         <oasis:entry rowsep="1" colname="col4">15 min</oasis:entry>  
         <oasis:entry rowsep="1" colname="col5">NE<inline-formula><mml:math id="M18" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>T</mml:mi></mml:mrow></mml:math></inline-formula> 0.25 K for band IR10.8</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1"/>  
         <oasis:entry colname="col2">Himawari</oasis:entry>  
         <oasis:entry colname="col3">2 km</oasis:entry>  
         <oasis:entry colname="col4">10 min</oasis:entry>  
         <oasis:entry colname="col5">NE<inline-formula><mml:math id="M19" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>T</mml:mi></mml:mrow></mml:math></inline-formula> 0.89 K for band 14;</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">  
         <oasis:entry colname="col1"/>  
         <oasis:entry colname="col2">AHI</oasis:entry>  
         <oasis:entry colname="col3"/>  
         <oasis:entry colname="col4"/>  
         <oasis:entry colname="col5">Da (2015)</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1"/>  
         <oasis:entry rowsep="1" colname="col2">NOAA</oasis:entry>  
         <oasis:entry rowsep="1" colname="col3">2.5<inline-formula><mml:math id="M20" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>  
         <oasis:entry rowsep="1" colname="col4">daily</oasis:entry>  
         <oasis:entry rowsep="1" colname="col5"><inline-formula><mml:math id="M21" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 11 W m<inline-formula><mml:math id="M22" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>; Ohring et al. (1984)</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">OLR</oasis:entry>  
         <oasis:entry rowsep="1" colname="col2">CERES</oasis:entry>  
         <oasis:entry rowsep="1" colname="col3">1<inline-formula><mml:math id="M23" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>  
         <oasis:entry rowsep="1" colname="col4">monthly</oasis:entry>  
         <oasis:entry rowsep="1" colname="col5"><inline-formula><mml:math id="M24" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 0.4 W m<inline-formula><mml:math id="M25" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">  
         <oasis:entry colname="col1"/>  
         <oasis:entry colname="col2">AIRS</oasis:entry>  
         <oasis:entry colname="col3">1<inline-formula><mml:math id="M26" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>  
         <oasis:entry colname="col4">monthly</oasis:entry>  
         <oasis:entry colname="col5"><inline-formula><mml:math id="M27" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 1 W m<inline-formula><mml:math id="M28" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">Air</oasis:entry>  
         <oasis:entry rowsep="1" colname="col2">MODIS</oasis:entry>  
         <oasis:entry rowsep="1" colname="col3">5 km</oasis:entry>  
         <oasis:entry rowsep="1" colname="col4">4 per day</oasis:entry>  
         <oasis:entry rowsep="1" colname="col5">1.5 g kg<inline-formula><mml:math id="M29" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>; Seemann et al. (2003)</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">  
         <oasis:entry colname="col1">moisture</oasis:entry>  
         <oasis:entry colname="col2">AIRS</oasis:entry>  
         <oasis:entry colname="col3">45 km</oasis:entry>  
         <oasis:entry colname="col4">2 per day</oasis:entry>  
         <oasis:entry colname="col5">15 %</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">Air</oasis:entry>  
         <oasis:entry rowsep="1" colname="col2">MODIS</oasis:entry>  
         <oasis:entry rowsep="1" colname="col3">5 km</oasis:entry>  
         <oasis:entry rowsep="1" colname="col4">4 per day</oasis:entry>  
         <oasis:entry rowsep="1" colname="col5">1–2 K; Seemann et al. (2003)</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">  
         <oasis:entry colname="col1">temperature</oasis:entry>  
         <oasis:entry colname="col2">AIRS</oasis:entry>  
         <oasis:entry colname="col3">45 km</oasis:entry>  
         <oasis:entry colname="col4">2 per day</oasis:entry>  
         <oasis:entry colname="col5">1 K</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">Trace</oasis:entry>  
         <oasis:entry colname="col2">AIRS</oasis:entry>  
         <oasis:entry colname="col3">1<inline-formula><mml:math id="M30" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>  
         <oasis:entry colname="col4">daily</oasis:entry>  
         <oasis:entry colname="col5">0.5–1.6 % for CH<inline-formula><mml:math id="M31" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula>; Xiong et al. (2008)</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">gases</oasis:entry>  
         <oasis:entry colname="col2"/>  
         <oasis:entry colname="col3"/>  
         <oasis:entry colname="col4"/>  
         <oasis:entry colname="col5"><inline-formula><mml:math id="M32" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula>0.5 % for CO<inline-formula><mml:math id="M33" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>; Maddy et al. (2008)</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">  
         <oasis:entry colname="col1"/>  
         <oasis:entry colname="col2"/>  
         <oasis:entry colname="col3"/>  
         <oasis:entry colname="col4"/>  
         <oasis:entry colname="col5">8–12 % for CO; McMillan et al. (2011)</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1"/>  
         <oasis:entry rowsep="1" colname="col2">MODIS</oasis:entry>  
         <oasis:entry rowsep="1" colname="col3">3 km</oasis:entry>  
         <oasis:entry rowsep="1" colname="col4">4 per day</oasis:entry>  
         <oasis:entry rowsep="1" colname="col5">0.2; Remer et al. (2013)</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">AOD</oasis:entry>  
         <oasis:entry colname="col2">VIIRS</oasis:entry>  
         <oasis:entry colname="col3">6 km</oasis:entry>  
         <oasis:entry colname="col4">2 per day</oasis:entry>  
         <oasis:entry colname="col5"><inline-formula><mml:math id="M34" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 0.05 over ocean  and <inline-formula><mml:math id="M35" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 0.12</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">  
         <oasis:entry colname="col1"/>  
         <oasis:entry colname="col2"/>  
         <oasis:entry colname="col3"/>  
         <oasis:entry colname="col4"/>  
         <oasis:entry colname="col5">over land; Jackson et al. (2013)</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">  
         <oasis:entry colname="col1">SLHF</oasis:entry>  
         <oasis:entry colname="col2">MODIS</oasis:entry>  
         <oasis:entry colname="col3">500 m</oasis:entry>  
         <oasis:entry colname="col4">8 days</oasis:entry>  
         <oasis:entry colname="col5">–</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">Land surface</oasis:entry>  
         <oasis:entry rowsep="1" colname="col2">MODIS</oasis:entry>  
         <oasis:entry rowsep="1" colname="col3">1 km</oasis:entry>  
         <oasis:entry rowsep="1" colname="col4">4 per day</oasis:entry>  
         <oasis:entry rowsep="1" colname="col5">1 K;  Wan (2014)</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">temperature</oasis:entry>  
         <oasis:entry rowsep="1" colname="col2">VIIRS</oasis:entry>  
         <oasis:entry rowsep="1" colname="col3">750 m</oasis:entry>  
         <oasis:entry rowsep="1" colname="col4">daily</oasis:entry>  
         <oasis:entry rowsep="1" colname="col5">2 K;  Guillevic et al. (2014)</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">  
         <oasis:entry colname="col1"/>  
         <oasis:entry colname="col2">SEVIRI</oasis:entry>  
         <oasis:entry colname="col3">2 km</oasis:entry>  
         <oasis:entry colname="col4">15 min</oasis:entry>  
         <oasis:entry colname="col5">1–2 K;  Trigo et al. (2008)</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">Sea surface</oasis:entry>  
         <oasis:entry rowsep="1" colname="col2">MODIS</oasis:entry>  
         <oasis:entry rowsep="1" colname="col3">1 km</oasis:entry>  
         <oasis:entry rowsep="1" colname="col4">daily</oasis:entry>  
         <oasis:entry rowsep="1" colname="col5"><inline-formula><mml:math id="M36" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 0.5 K;  Kilpatrick et al. (2015)</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">temperature</oasis:entry>  
         <oasis:entry colname="col2">VIIRS</oasis:entry>  
         <oasis:entry colname="col3">1.5 km</oasis:entry>  
         <oasis:entry colname="col4">daily</oasis:entry>  
         <oasis:entry colname="col5"><inline-formula><mml:math id="M37" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 0.31 K;  Tu et al. (2015)</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table><table-wrap-foot><p id="d1e444"><inline-formula><mml:math id="M13" display="inline"><mml:msup><mml:mi/><mml:mo>∗</mml:mo></mml:msup></mml:math></inline-formula> NE<inline-formula><mml:math id="M14" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>T</mml:mi></mml:mrow></mml:math></inline-formula> denotes the noise equivalent temperature difference.</p></table-wrap-foot></table-wrap>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1"><caption><p id="d1e1152">Histogram of BT anomalies that occurred before and/or after
earthquakes with different magnitudes (Eleftheriou et al., 2016).</p></caption>
          <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/18/1013/2018/nhess-18-1013-2018-f01.png"/>

        </fig>

      <p id="d1e1162">TOA BT data are some of the most-used remote sensing data in thermal
anomaly detection because of their easy accessibility and data processing.
Several studies indicate that significant BT anomalies existed in
seismically active areas about 1 month to 8 days before earthquakes
(Lisi et al., 2010, 2015; Pergola et al., 2010). The regions
with strong tectonic activities also showed intensive BT anomalies during
the preparatory phases of low-magnitude earthquakes (Lisi et al., 2010).
After a 10-year retrospective correlation analysis in Greece, TOA BT
anomalies are considered to satisfy the qualifications involved in a
multi-parametric system for the time-dependent assessment of seismic hazards
(Eleftheriou et al., 2016). As shown in Fig. 1, BT anomalies mainly occurred
before the earthquake with magnitude greater than 5, but for seismic events
with magnitude less than 5 this anomaly indicator  became less
significant.</p>
      <p id="d1e1165">Another frequently used precursor at TOA is OLR, which is a critical
component of the Earth's energy budget. OLR is the total longwave radiative
flux (W m<inline-formula><mml:math id="M38" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>) in the TIR wavelength from 4 to
100 <inline-formula><mml:math id="M39" display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>m, which is emitted from the Earth and its atmosphere going to space. More
specifically, it is the integrated result of the reflection, absorption, and
emission of longwave radiation by the Earth's surface (land and sea),
atmosphere, aerosols, and clouds, which finally leaves the Earth system. OLR
represents the radiation characteristics of the cloud top when the
instantaneous field of view of satellite sensors is covered by clouds and indicates the longwave
radiation emitted by the surface and atmosphere under cloudless conditions.</p>
      <?pagebreak page1017?><p id="d1e1187">OLR cannot be directly measured but can be derived from measurements of
sensors (e.g., AVHRR; Atmospheric Infrared Sounder, AIRS; and Clouds and
the Earth's Radiant Energy System, CERES). Among them, the National Oceanic
and Atmospheric Administration (NOAA) OLR is the commonly used data product
in various studies and is retrieved from the AVHRR TIR bands (10.5–12.5 <inline-formula><mml:math id="M40" display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>m)
on a <inline-formula><mml:math id="M41" display="inline"><mml:mrow><mml:mn mathvariant="normal">2.5</mml:mn><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">2.5</mml:mn><mml:mo>∘</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula> latitude–longitude
grid with daily and monthly mean values from 1981 to the present (Gruber and
Krueger, 1984). The latest AIRS OLR product, which is retrieved from
hyperspectral TIR data, is AIRS Version 6 Level 3 monthly mean product on a
<inline-formula><mml:math id="M42" display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mo>×</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula> latitude–longitude grid beginning in
September 2002 (Aumann et al., 2003). Finally, the CERES OLR dataset is the
monthly mean value from 2000 in the CERES Energy Balanced and Filled (EBAF) Edition 4.0
datasets on a <inline-formula><mml:math id="M43" display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mo>×</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula> latitude–longitude grid
(Rose et al., 2013).</p>
      <p id="d1e1256">Several studies suggest that OLR can be effectively used as a short-term or
impending earthquake precursor. OLR appeared as a steadily increasing trend
around the epicenter and thus can be used as an indicator of seismic
activity (Ouzounov et al., 2007). Figure 2 presents the time series of daily
OLR anomaly before the <inline-formula><mml:math id="M44" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mtext>w</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> 9.0  Sumatra–Andaman Islands,
North Sumatra,
earthquake (3.09<inline-formula><mml:math id="M45" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 94.26<inline-formula><mml:math id="M46" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E) occurred on 26 December 2004.
After several small peaks beyond the mean field of OLR, an intense
rise showed up shortly following this mega-earthquake. Anomalous OLR
occurred 2 months to several days prior to the main shock with at least
several thousands of square kilometers. OLR anomaly has a direct
significance for earthquakes with magnitude above 5.5 (Eleftheriou et al.,
2016). Anomalous OLR variations can reach 30–45 W m<inline-formula><mml:math id="M47" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> around epicentral
areas 7–8 days prior to the major earthquake (Rawat et al., 2011).
Cumulative elastic energy in the earthquake preparation regions may result
in intensive thermal emissions associated with the release of a large amount
of energy when an earthquake occurs. Increase in surface temperature, air
temperature, water vapor, and other greenhouse gases results in the increase
in OLR and TOA BT, especially around the epicenter under clear sky
conditions (Tramutoli et al., 2005).</p>
      <p id="d1e1300">TOA BT and OLR represent longwave radiation variations of the entire
surface–atmosphere system and are significantly affected by atmospheric
conditions. The height and coverage of clouds have a dominating influence on
the total intensity of longwave radiative fluxes received at the TOA (Turner
et al., 2015). Therefore, eliminating cloud effects is necessary in
applications, which can be difficult when working with low-resolution data.
Meanwhile, OLR anomalies may be the result of other atmospheric effects and
not of increased surface temperature (Tronin, 2010). In the cases under
clear sky conditions, water vapor is another significant factor that has
strong absorption and re-emission capabilities on longwave radiation and
rapidly changes in the spatiotemporal pattern. These situations are
particularly unfavorable for detecting weak pre-seismic anomalies; thus,
land surface  temperature (LST) and similar data products that are not
heavily affected by atmospheric disturbances are preferred (Filizzola et
al., 2004; Lisi et al., 2015).</p>
</sec>
<sec id="Ch1.S2.SS2">
  <title>Atmospheric water vapor and temperature</title>
      <p id="d1e1309">Atmospheric water vapor and temperature are two important physical
quantities that describe the status of the atmosphere, especially in the
atmospheric boundary layer. They have strongly dependencies and thus can
present synchronous responses to the impending earthquakes.</p>
      <p id="d1e1312">Over 99 % of atmospheric moisture is in the form of water vapor, and it is
abundant and highly varies in the atmosphere. Water vapor is
the primary greenhouse gas in the Earth's climate system and influences
long-term climate changes. The water vapor associated with atmospheric
energy drives the development of weather systems and  transfer of heat
from the tropics to the poles. Atmospheric water vapor content can be
referred to as the total column water vapor contained in a vertical column
of atmosphere between the Earth's surface and the TOA, which can be
retrieved from near-infrared, TIR, or passive microwave data (Chesters et
al., 1983; Ferraro et al., 1996; Gao and Kaufman, 2003). For example, the
MODIS total precipitable water product (MOD05_L2 and
MYD05_L2) has two types of data: one using near-infrared
algorithm at the 1 km spatial resolution during the day and the other using
infrared algorithm at 5 km resolution during day and night. In general, the
accuracy of water vapor products ranges from 5 to 10% (Gao and
Kaufman, 2003).</p>
      <p id="d1e1315">Anomalies of atmospheric water vapor content have been observed prior to
several strong earthquakes (Cervone et al., 2004; Dey and Singh, 2003). The
2001 Gujarat earthquake triggered anomalous atmospheric moisture increase of
about 15 mm, which were detected using passive microwave data of the Special
Sensor Microwave Imager (SSM/I; Dey et al., 2004). The anomalous increase of water
vapor level occurred around the epicenter in land regions before the
earthquake and in ocean regions after the earthquake. Meanwhile, AIRS data
led to the discovery of anomalous changes in relative humidity at different
pressure levels reaching 500 hPa, with even larger variations at the lower
levels (Singh et al., 2010a). Dey et al. (2004) related this phenomenon to
the increase of the surface latent heat flux (SLHF), which is discussed in Sect. 2.5.</p>
      <p id="d1e1318">Aside from atmospheric moisture, air temperature (or atmospheric
temperature) is the most commonly measured weather parameter. It refers to
the screen-level air temperature in meteorological terms, which is normally
measured at the attitude of 2 m above the ground surface. Air temperature is
a more complex parameter than LST and is affected by LST, winds,
topography, etc. LST can be estimated based on satellite TIR measurements.
However, air temperature cannot be directly derived from LST, and no
operational remote sensing data product of air temperature is available at
present. The atmospheric profiles provide the air temperature and water
vapor amounts at different altitudinal layers in the vertical atmosphere,
but this air temperature is different from the screen-level temperature. The
atmospheric profiles can be retrieved from TIR multispectral sensors (e.g.,
MODIS) or infrared sounders (e.g., AIRS) (Aumann et al., 2003; Seemann et
al., 2003).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2"><caption><p id="d1e1324">Daily OLR anomaly over the epicenter for <inline-formula><mml:math id="M48" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mtext>w</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> 9.0 Sumatra–Andaman
earthquake (Ouzounov et al., 2007).</p></caption>
          <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/18/1013/2018/nhess-18-1013-2018-f02.png"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3" specific-use="star"><caption><p id="d1e1346">The variation of mean screen-level air temperature around the
epicenter before and after the <inline-formula><mml:math id="M49" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mtext>s</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> 6.0  Kerman earthquake (Alvan et al.,
2013).</p></caption>
          <?xmltex \igopts{width=398.338583pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/18/1013/2018/nhess-18-1013-2018-f03.png"/>

        </fig>

      <p id="d1e1366">Significant near-surface air temperature anomalies related to earthquakes
have been reported in different studies (Panda et al., 2007; Pulinets and
Dunajecka, 2007). An approximate increase of air temperature at 2–4 K in a
north–south pattern along the Nosrātabād fault zone during 18–20 December
was observed prior to the <inline-formula><mml:math id="M50" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mtext>s</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> 6.0 Kerman earthquake in Iran on 20 December 2010 (Fig. 3) (Alvan et al., 2013).
Anomalous changes of air temperature at
different pressure levels from AIRS data were found up to 500 hPa with the
variations<?pagebreak page1018?> becoming larger at the lower levels (Singh et al., 2010a). An
increase in air temperature along with low air humidity has been observed
prior to earthquakes (Pulinets et al., 2006a; Singh et al., 2010a). Ouzounov
et al. (2007) and Pulinets and Dunajecka (2007) consider that the anomalies
in air temperature and relative humidity prior to strong earthquakes
indicated by historical meteorological data are primarily related to the air
ionization caused by increased radon emanations from faults in earthquake
preparation regions. Anomalous areas are considerably larger than seismic
sources, which indicates the difficulty of identifying the epicenter before
a main shock.</p>
</sec>
<sec id="Ch1.S2.SS3">
  <title>Atmospheric trace gases</title>
      <p id="d1e1386">Atmospheric trace gases make up less than 1 % of the Earth's atmosphere by
volume. These gases include CO<inline-formula><mml:math id="M51" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, CH<inline-formula><mml:math id="M52" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula>, O<inline-formula><mml:math id="M53" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>, SO<inline-formula><mml:math id="M54" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, and
NO<inline-formula><mml:math id="M55" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>, which are produced from natural geothermal sources, volcanic activity,
ecosystem, and anthropogenic sources. Trace gas concentrations are crucial in
investigating atmospheric processes. Atmospheric trace gas data, such as
CH<inline-formula><mml:math id="M56" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula>, CO<inline-formula><mml:math id="M57" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, and CO, can be retrieved from satellite measurements
(e.g., AIRS hyperspectral TIR data) (Chahine et al., 2006; Clarisse et al.,
2011).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4" specific-use="star"><caption><p id="d1e1455">The anomalies of CO (mole cm<inline-formula><mml:math id="M58" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> <bold>(a)</bold> and O<inline-formula><mml:math id="M59" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> (DU)
<bold>(b)</bold>;
the red star indicates the epicenter of the 2010 Baja California earthquake
(Cui et al., 2013).</p></caption>
          <?xmltex \igopts{width=497.923228pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/18/1013/2018/nhess-18-1013-2018-f04.png"/>

        </fig>

      <p id="d1e1494">Seismic activities can change atmospheric composition, especially the
increment of greenhouse gases prior to strong earthquakes. A 6 % increase
in the columnar ozone prior to the 2015 Nepal earthquake was observed
(Ganguly, 2016). An increased CO emission at near-surface pressure levels
associated with LST over epicenter areas was detected by the Measurements of
Pollution in the Troposphere (MOPITT) on board the Terra satellite approximately 1 week
before the earthquake (Singh et al., 2010b). Anomalous increases in total
column CO and O<inline-formula><mml:math id="M60" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> occurred over the epicenter areas 1 to 6 months
prior to several strong earthquakes (Cui et al., 2013). Figure 4 indicates
that anomalous CO appeared along the San Andreas Fault, while the anomalies
of O<inline-formula><mml:math id="M61" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> spread over wider areas around the epicenter before and after <inline-formula><mml:math id="M62" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mtext>s</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> 7.1 Baja California earthquake on 5 April 2010. However, these phenomena
are unstable with only parts of studied earthquakes exhibiting anomalous
variations and with persistent time being irregular.</p>
      <p id="d1e1526">Changes in pressure between rocks due to seismic activity are believed to
result in greenhouse gas emissions and local greenhouse effect (Choudhury et
al., 2006; Singh et al., 2010a; Zoback and Gorelick, 2012). The experimental
results show that gases, such as CH<inline-formula><mml:math id="M63" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> and CO<inline-formula><mml:math id="M64" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, can obtain energy
from the transient electric field and cause a temperature increase. The
trace gas anomaly before medium to strong earthquakes was preliminarily
believed to exhibit (1) a sudden release of gas and (2) a static electricity
of field mutation. Earthquakes may lead to the release of underground
carbonaceous gas, which provides a scientific basis for the mechanism of
pre-seismic thermal anomalies. In addition, CO<inline-formula><mml:math id="M65" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>-rich fluids in the deep
crust are considered as the possible important carbonaceous gas source in
the lithosphere–coversphere–atmosphere coupling (LCAC) process (Chiodini
et al., 2011). The anomalies in trace gas concentration can be attributed to
gas emissions in the lithosphere and photochemical reactions (Cui et al.,
2013). The LST anomalies prior to the 2009 <inline-formula><mml:math id="M66" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mtext>w</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> 6.3 L'Aquila earthquake
illustrate the strong correlation with the topographic height and were
clearly distributed over the mountain tops but not the valleys (Piroddi et
al., 2014). The anomalous mechanisms of the activation of electronic charge
carriers and emission of greenhouse gases or radon gas are considered to
demonstrate a consistent manner because of prominent LST anomalies within
the limestone regions in this earthquake case. As a result, LST and air
temperature may increase, resulting in changes in SLHF and atmospheric water
vapor condensation and propagation to the BT observed by satellite sensors.</p>
</sec>
<sec id="Ch1.S2.SS4">
  <title>Aerosols</title>
      <?pagebreak page1019?><p id="d1e1573">Aerosols are the fine solid and liquid particles suspended in the
atmosphere that  are produced from various sources, such as desert dust,
wildfire smoke, sea salt particles, volcanic ash, and urban haze. Aerosols
have different optical and microphysical properties depending on their type
and size distribution. They have an important influence on cloud formation
and are often expressed by the aerosol optical depth (AOD). AOD is a dimensionless physical quantity
used to describe quantitatively the extinction degree of the direct solar
radiation reaching the ground by the absorption and scattering of aerosols.
AOD is defined as the integrated extinction coefficient within a vertical
column of unit cross section along the entire atmospheric path, where the
planetary boundary layer accounts for most of them. For now, most of
multispectral radiometers in the visible, near-infrared, and
shortwave-infrared wavelength regions can be used to retrieve AOD. For
instance, the MODIS daily Level 2 aerosol product (MOD04), which is produced
by the Dark Target and Deep Blue algorithms at a spatial resolution
of 10 km at nadir in  Collection 6 (Levy et al., 2013), includes many
aerosol parameters, such as AOD, aerosol type, angstrom exponent, asymmetry
factor, and single scattering albedo.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F5"><caption><p id="d1e1578">Time series of AOD anomalous values over the epicenter before the
<inline-formula><mml:math id="M67" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mtext>w</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> 8.8 Chile earthquake on 27 February 2010 (Akhoondzadeh, 2015). The
vertical dotted line indicates the time of Chile earthquake, and median and
upper/lower bounds are the blue and green lines, respectively.</p></caption>
          <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/18/1013/2018/nhess-18-1013-2018-f05.png"/>

        </fig>

      <?pagebreak page1020?><p id="d1e1598">Aerosols are also used as indicators in many pre-seismic anomaly studies. AOD
was observed an increase of 40 % prior to the 2015 Nepal earthquake
(Ganguly, 2016). A clear increase in AOD around the epicenter 2 days prior
to the 2010 Chile earthquake was found in Fig. 5 using three anomaly
detection methods in order to reduce uncertainty of detecting anomaly date
(Akhoondzadeh, 2015). An anomalous increase of ground-measured AOD is
quasi-synchronous with several abnormal hydrothermal parameters (Wu et al.,
2016). Over the sea surface, significant changes in aerosol parameters are
considered to be related to the 2001 Gujarat earthquake (Okada et al.,
2004). Although aerosols do not directly relate to the TIR radiation, the
charged aerosol particles play a role in the water vapor condensation and
cloud formation over earthquake fracture areas. A high aerosol concentration
causes stronger electric field intensities and increased infrared emissions
(Liperovsky et al., 2005). Therefore, indirect effects of aerosols on the
pre-seismic anomalies cannot be ignored. Additionally, the air
ionization is a possible reason that keeps aerosols suspended in the
atmosphere for many days before the earthquake, which could be explained by
the <inline-formula><mml:math id="M68" display="inline"><mml:mi>p</mml:mi></mml:math></inline-formula>-hole theory (Freund et al., 2009). The predominantly, sometimes
exclusively, positive airborne ions generated at the Earth's surface rise
through the atmospheric column and attach to aerosol particles; thus the
ionized aerosols can suspend in the atmosphere for a longer time. More field
measurements, which can validate this theory, still need to be carried out.</p>
</sec>
<sec id="Ch1.S2.SS5">
  <title>SLHF</title>
      <p id="d1e1614">SLHF (W m<inline-formula><mml:math id="M69" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> is the flux of the heat absorbed or released by the phase
transition (i.e., condensation, evaporation, and melting) of water from the
Earth's surface to the atmosphere. SLHF is an important component of Earth's
surface energy budget and is mainly affected by the atmospheric relative
humidity, wind speed, surface temperature, and season. Traditionally, SLHF
is measured through the Bowen ratio technique or by the eddy covariance and
can also be obtained from satellite products. MODIS global
evapotranspiration product (MOD16) has a spatial resolution of 1 km at
8-day, monthly, and annual intervals (Mu et al., 2011).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F6"><caption><p id="d1e1634">Time series of SLHF on the epicenter of the 2007 <inline-formula><mml:math id="M70" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mtext>s</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> 6.4 Pu'er
earthquake (Qin et al., 2014a).</p></caption>
          <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/18/1013/2018/nhess-18-1013-2018-f06.png"/>

        </fig>

      <p id="d1e1654">Several studies have reported the abnormal increase of SLHF prior to
earthquakes. The SLHF increased by approximately 50 W m<inline-formula><mml:math id="M71" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>, peaking at 115 W m<inline-formula><mml:math id="M72" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>
over 3–23 days before earthquakes in the Middle East (Mansouri
Daneshvar et al., 2014). SLHF can also be a possible precursor to coastal
earthquakes because anomalous SLHF tends to be more intensive over sea
surface than over land surface (Cervone et al., 2004, 2006).
The analysis of coastal earthquakes shows that the SLHF increased abnormally
a few days before earthquakes, which is the result of the increase in
surface<?pagebreak page1021?> temperature in seismically active areas (Pulinets et al., 2006a).
SLHF anomaly is significantly weaker on land surface than on sea surface due
to obvious differences in air humidity, wind speed, and surface temperature
between sea and land surfaces. However, Qin et al. (2014a) found that
anomalous SLHF, which is indicated by the dashed circle in Fig. 6, occurred
approximately 10 days before the inland Pu'er earthquake (23.8092<inline-formula><mml:math id="M73" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N,
101.15<inline-formula><mml:math id="M74" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E) on 2 June 2007. Conversely, the study of Zhang et
al. (2013) indicates that no significant anomalous variation of SLHF exists
prior to ten studied marine or coastal earthquakes, and that data accuracy
and parameter settings have an important effect on quantification of the
correlation between SLHF anomaly and earthquake's occurrence.</p>
      <p id="d1e1699">SLHF anomaly prior to earthquakes is considered to relate to the
underground fluid movement and the interaction among the underground,
surface, and atmosphere (Alvan et al., 2013). Mansouri Daneshvar et al. (2014)
believed that water vapor responses to seismic preparation phases
follow a seismic-triggered chain, which undergoes air ionization, SLHF
enhancement, water vapor condensation, and increased rainfall. Several
studies have proven that SLHF anomalies before earthquakes are linked with
soil moisture (Cervone et al., 2004; Dey and Singh, 2003). Meanwhile, air
ionization in the lithosphere–atmosphere–ionosphere coupling (LAIC) model
may be responsible for soil moisture and SLHF anomalies due to the increase
of water condensation on newly formed ions (Pulinets and Ouzounov, 2011).</p>
</sec>
<sec id="Ch1.S2.SS6">
  <title>Surface temperature</title>
      <p id="d1e1708">LST, also known as surface skin temperature, represents a remarkably thin
surface layer of medium temperature state, which is affected by solar
radiation, surface albedo, vegetation cover, soil moisture, etc. LST affects
the energy exchange between the surface and boundary layers and determines
the air temperature near the surface. Compared to TOA BT and OLR, LST can
indicate the surface warming process better. MODIS LST data are currently
the most extensively used products in the 1 km spatial resolution with an
inversion accuracy of approximately 1 K (Wan, 2014).</p>
      <p id="d1e1711">LST is suitable for the analysis of inter-monthly variations, which is
beneficial to short-term earthquake monitoring. A 40-day time period is
sufficient for anomaly monitoring (Bhardwaj et al., 2017). The LST prior to
earthquakes usually increased by at least 3–5 K (Ouzounov et al., 2006;
Ouzounov and Freund, 2004; Tronin, 2006). A 1–10 K rise of LST 2 weeks
before the main shock of 2011 Tōhoku earthquake was detected around the
epicenter (Zoran, 2012). Moreover, the study by Bhardwaj et al. (2017) shows
that snow cover levels prior to the 2015 Nepal earthquake noticeably
declined and that snow surface temperature is a highly sensitive precursor
that presented 3–14 K temperature anomaly in 3–17 days prior to this
earthquake. Most studies use nighttime LST data for analysis due to the
absence of solar heating, leading to measurements that are predominantly
gathered from surface and underground thermal sources. However, LST
anomalies can also be significant in the daytime (Blackett et al., 2011;
Panda et al., 2007; Saraf et al., 2008).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F7"><caption><p id="d1e1716">The map of LST anomalies indicated by colored dashed circles over
the study area before the <inline-formula><mml:math id="M75" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mtext>w</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> 6.3 Aquila earthquake on 6 April 2009 (Lisi et
al., 2015).</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/18/1013/2018/nhess-18-1013-2018-f07.png"/>

        </fig>

      <p id="d1e1736">The pre-seismic anomalies in epicentral areas before strong earthquakes are
related to the increase in air temperature, LST, and soil temperature at
shallow layers. LST anomaly indicated by MODIS data was consistent with
anomalous air temperature variations observed at the meteorological station
close to the epicenter (Akhoondzadeh, 2013). The anomalous temperature
variations are related to the seismic deformation and follow the fault
evolution under seismic stress changes (Ma et al., 2008). Thus, LST is more
useful in detecting anomalies than TOA BT or OLR because it is less affected
by the atmosphere, which allows it to produce a higher signal-to-noise ratio
(SNR) (Aliano et al.,<?pagebreak page1022?> 2008; Lisi et al., 2015). Figure 7 shows the spatial
and temporal evolution of the sequence of LST anomalies by different colored
dashed circles (Lisi et al., 2015). The green dashed circle indicates the
possible local warming effect caused by clouds. The LST anomalies which
followed the main tectonic lineaments (green lines) in central Italy (black
circle), the Balkan region (blue circle), and the Padania plain (purple
circle) were possibly associated with the medium–strong earthquakes.
Meanwhile, LST, as a thermodynamic parameter of dynamic equilibrium, derived
by remote sensing data contains a degree of uncertainty due to the influence
of surface types, processes of surface energy balance, and atmospheric
turbulence.</p>
      <p id="d1e1740">Several cases of marine earthquake monitoring using remote sensing TIR data
have been successful. Sea surface temperature (SST) anomaly can be related
to seismicity (Ouzounov and Freund, 2004), but SST is strongly influenced by
weather conditions and currents. Seawater has a large thermal inertia that
allows its temperature to change more slowly; therefore, some mechanisms of
LST anomalies are not applicable to SST anomalies. The study of the 2000
Blanco earthquake sequence shows that ocean hydrothermal system can be
altered by large earthquakes and significant decline of temperature was
observed following the main shock (Dziak et al., 2003). Ouzounov et al. (2006)
analyzed the decrease of SST before the <inline-formula><mml:math id="M76" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mtext>s</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> 6.8 2003 Boumerdès
earthquake and implied that this phenomenon was attributed to the upwelling
of cold water from the deep ocean caused by crustal deformation. Freund et
al. (2009) disagreed with his explanation and offered a physically
meaningful mechanism to explain the phenomenon of SST anomalies. The <inline-formula><mml:math id="M77" display="inline"><mml:mi>p</mml:mi></mml:math></inline-formula> holes
activated by the tectonic stress transfer from the sea floor to the
ground-to-water interface and generate the oxidation from H<inline-formula><mml:math id="M78" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O to
H<inline-formula><mml:math id="M79" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O<inline-formula><mml:math id="M80" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, which changes the thermal radiation balance of the sea
surface.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F8" specific-use="star"><caption><p id="d1e1790">Pre-seismic anomaly detection methods. The blue boxes indicate six
classes that discussed below and white boxes are the subclasses of each
method.</p></caption>
          <?xmltex \igopts{width=497.923228pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/18/1013/2018/nhess-18-1013-2018-f08.png"/>

        </fig>

</sec>
</sec>
<sec id="Ch1.S3">
  <title>Anomaly detection methods</title>
      <p id="d1e1806">The pre-seismic anomaly can generally be defined as the departure of a
current observation value from the long-term average reference (Ouzounov et
al., 2007). It is used to relate seismicity to temporal and spatial
variations of thermal-radiation-related signals from satellite observations.
Different data processing methods have been proposed in this domain over the
past years. These methods aim to detect pre-seismic anomalies, attempt to
point out possible future strong earthquake in terms of time, spatial, and
magnitude windows within stated limits, and estimate the probability of this
earthquake's occurrence. Figure 8 presents the methods that are classified
and discussed below.</p><?xmltex \hack{\newpage}?>
<sec id="Ch1.S3.SS1">
  <title>Visual interpretation</title>
      <p id="d1e1815">Visual interpretation method is a type of manual analysis method that
interprets the relationship between an earthquake and the relevant
parameters through a time series of visible and near-infrared or TIR data
before and after the target earthquake. The observed quantity, such as
surface temperature, is measured in considerably greater amounts prior to
the earthquake around epicenter areas compared to other time period and
neighboring regions. The method is simple and effective; thus, it is always
used in interpreting preliminary pre-seismic anomalies. Several studies have
utilized this method, such as in the aerosol anomaly (Qin et al., 2014b),
SLHF anomaly (Dey and Singh, 2003), anomalies of multiple parameters
(Pulinets et al., 2006a; Singh et al., 2010a), and BT anomalies of AVHRR and
MODIS data (Saraf et al., 2012).</p>
      <p id="d1e1818">Visual interpretation is mainly based on experience interpretation, which
results in strong subjectivity and does not allow current computer
technology to deal with massive amounts of satellite data. From Fig. 9, we
can distinguish the LST anomalies around the epicenter, but this difference
is subtle causing the randomicity during the anomaly recognition. In
addition, visually identifying abnormal information can be difficult and
calls for further processing, such as the use of pseudo-color synthesis,
difference method, and fault profile line method. At the same time,
increasingly sophisticated anomaly detection algorithms have been applied to
extract signals about pre-seismic anomalies with increases in data source
and amount and the quantitative requirement of further research.</p>
</sec>
<sec id="Ch1.S3.SS2">
  <title>Image difference methods</title>
      <p id="d1e1827">The simple image difference method involves identifying the differences in
the same region over a series of images captured at different times for
qualitative analysis. If the difference exceeds the pre-defined threshold,
then the observed precursor value could be regarded as an anomaly that may
be associated with an impending earthquake. This method eliminates the
influence of background signals and highlights the spatial distribution of
pre-seismic anomalies to a certain extent. For example, TIR images captured
before and after earthquakes were used to calculate difference values that
highlight anomalous variations (Ma et al., 2008; Tronin et al., 2002). The
method that uses BT difference has a certain ability to identify cloud
pixels but cannot eliminate background influence. Therefore, temperature
anomaly is introduced through normalizing the area-averaged LST by
subtracting and dividing by multiyear mean LST (Zoran, 2012).</p>
      <?pagebreak page1023?><p id="d1e1830">The general anomaly method is to find the difference between current data
during an earthquake and the long-term average value (also called a
reference value) in order to improve result robustness and eliminate
potential bias (Mahmood et al., 2017; Qin et al., 2014a; Wu et al., 2016).
This method can be expressed as

                <disp-formula specific-use="align" content-type="numbered"><mml:math id="M81" display="block"><mml:mtable displaystyle="true"><mml:mlabeledtr id="Ch1.E1"><mml:mtd/><mml:mtd><mml:mstyle class="stylechange" displaystyle="true"/></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:mi mathvariant="normal">GA</mml:mi><mml:mfenced open="(" close=")"><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi></mml:mfenced><mml:mo>=</mml:mo><mml:mi>v</mml:mi><mml:mfenced close=")" open="("><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>,</mml:mo><mml:mi>t</mml:mi></mml:mfenced><mml:mo>-</mml:mo><mml:mi mathvariant="italic">μ</mml:mi><mml:mfenced open="(" close=")"><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi></mml:mfenced><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E2"><mml:mtd/><mml:mtd><mml:mstyle displaystyle="true" class="stylechange"/></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:mi mathvariant="italic">μ</mml:mi><mml:mfenced close=")" open="("><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi></mml:mfenced><mml:mo>=</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mn mathvariant="normal">1</mml:mn><mml:mi>N</mml:mi></mml:mfrac></mml:mstyle><mml:munderover><mml:mo movablelimits="false">∑</mml:mo><mml:mrow><mml:mi>t</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow><mml:mi>N</mml:mi></mml:munderover><mml:mi>v</mml:mi><mml:mfenced close=")" open="("><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>,</mml:mo><mml:mi>t</mml:mi></mml:mfenced><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr></mml:mtable></mml:math></disp-formula>

            where <inline-formula><mml:math id="M82" display="inline"><mml:mrow><mml:mi>v</mml:mi><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>,</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> is the value of a pixel at a spatial location
<inline-formula><mml:math id="M83" display="inline"><mml:mrow><mml:mfenced open="(" close=")"><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi></mml:mfenced></mml:mrow></mml:math></inline-formula> and time <inline-formula><mml:math id="M84" display="inline"><mml:mi>t</mml:mi></mml:math></inline-formula> of satellite data required, which can be TOA
BT, OLR, or LST. <inline-formula><mml:math id="M85" display="inline"><mml:mrow><mml:mi mathvariant="italic">μ</mml:mi><mml:mfenced open="(" close=")"><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi></mml:mfenced></mml:mrow></mml:math></inline-formula> is the average value at the
same position in the same or similar time slot of years using multiyear
data. In other words, the anomaly is the difference between what is
happening and what is expected over a long-term average trend. General
anomaly method is an improvement of the image difference method (Qin et al.,
2012).</p>
      <p id="d1e1992">Given complex influences and possible uncertainties with respect to seasons,
local weather, topography, and surface inhomogeneity, the pre-seismic
anomaly is a weak signal in the strong background level. Thus, understanding
variations of the background field and the variation trend of each
influencing factor over time are the key to the anomaly detection. The
establishment of a regional reference field based on multiyear data is a basic
procedure to identify pre-seismic anomaly, because the reference field can
express the trend of physical quantity in the spatiotemporal pattern and
relieve random variability due to local meteorological factors. General
anomaly method is used to eliminate this tendency change of current
observation, thereby highlighting the pre-seismic anomaly. The <inline-formula><mml:math id="M86" display="inline"><mml:mi>k</mml:mi></mml:math></inline-formula> times
standard deviation (<inline-formula><mml:math id="M87" display="inline"><mml:mi mathvariant="italic">δ</mml:mi></mml:math></inline-formula>) is generally the reference level relative to
the long-term normal field. Beyond <inline-formula><mml:math id="M88" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M89" display="inline"><mml:mrow><mml:mi>k</mml:mi><mml:mi mathvariant="italic">δ</mml:mi></mml:mrow></mml:math></inline-formula> from the mean value of
the reference field is regard as the anomaly. A positive anomaly means that
the value is higher than the normal trend, whereas a negative anomaly
indicates a lower value than the normal value.</p>
      <p id="d1e2026">The thermal anomaly is a weak signal under strong interference, thus
isolating it by simple comparison or threshold is difficult. This may also
be an important reason that not all earthquakes exhibit significant
pre-seismic anomalies. The eddy field method is used to calculate and add
the difference data between adjacent lattice points of the data to obtain
the spatial distribution of the vorticity value (Ouzounov et al., 2007). The
formula is as follows:

                <disp-formula specific-use="align" content-type="numbered"><mml:math id="M90" display="block"><mml:mtable displaystyle="true"><mml:mtr><mml:mtd><mml:mstyle class="stylechange" displaystyle="true"/></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:mi mathvariant="normal">EF</mml:mi><mml:mfenced open="(" close=")"><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi></mml:mfenced><mml:mo>=</mml:mo><mml:mn mathvariant="normal">4</mml:mn><mml:mo>×</mml:mo><mml:mi>v</mml:mi><mml:mfenced open="(" close=")"><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi></mml:mfenced><mml:mo>-</mml:mo><mml:mi>v</mml:mi><mml:mfenced close=")" open="("><mml:mi>x</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>,</mml:mo><mml:mi>y</mml:mi></mml:mfenced><mml:mo>-</mml:mo><mml:mi>v</mml:mi><mml:mfenced close=")" open="("><mml:mi>x</mml:mi><mml:mo>+</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>,</mml:mo><mml:mi>y</mml:mi></mml:mfenced></mml:mrow></mml:mtd></mml:mtr><mml:mlabeledtr id="Ch1.E3"><mml:mtd/><mml:mtd><mml:mstyle class="stylechange" displaystyle="true"/></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><?xmltex \hspace*{5mm}?><mml:mo>-</mml:mo><mml:mi>v</mml:mi><mml:mfenced open="(" close=")"><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mfenced><mml:mo>-</mml:mo><mml:mi>v</mml:mi><mml:mfenced close=")" open="("><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>+</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mfenced><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr></mml:mtable></mml:math></disp-formula>

            where <inline-formula><mml:math id="M91" display="inline"><mml:mrow><mml:mi mathvariant="normal">EF</mml:mi><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> is the eddy value at spatial location <inline-formula><mml:math id="M92" display="inline"><mml:mrow><mml:mfenced close=")" open="("><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi></mml:mfenced></mml:mrow></mml:math></inline-formula>, and <inline-formula><mml:math id="M93" display="inline"><mml:mi>v</mml:mi></mml:math></inline-formula> is the observation value of a pixel. This method can
highlight anomalous changes in the neighborhood and is used for
earthquake-related anomaly detection by NOAA OLR data (Ouzounov et al.,
2007; Xiong et al., 2010).</p>
      <p id="d1e2175">Furthermore, normalization by <inline-formula><mml:math id="M94" display="inline"><mml:mi>z</mml:mi></mml:math></inline-formula> score (ZS) is as an anomaly index, which
hereafter is referred to as the ZS method (Ouzounov et al., 2011). The ZS
index is defined as<?pagebreak page1024?> follows:<?xmltex \hack{\newpage}?>

                <disp-formula specific-use="align" content-type="numbered"><mml:math id="M95" display="block"><mml:mtable displaystyle="true"><mml:mlabeledtr id="Ch1.E4"><mml:mtd/><mml:mtd><mml:mstyle displaystyle="true" class="stylechange"/></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:mi mathvariant="normal">ZS</mml:mi><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>,</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mi>v</mml:mi><mml:mfenced close=")" open="("><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>,</mml:mo><mml:mi>t</mml:mi></mml:mfenced><mml:mo>-</mml:mo><mml:mi mathvariant="italic">μ</mml:mi><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>)</mml:mo></mml:mrow><mml:mrow><mml:mi mathvariant="italic">δ</mml:mi><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E5"><mml:mtd/><mml:mtd><mml:mstyle displaystyle="true" class="stylechange"/></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:mi mathvariant="italic">δ</mml:mi><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>)</mml:mo><mml:mo>=</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msqrt><mml:mrow><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mn mathvariant="normal">1</mml:mn><mml:mrow><mml:mi>N</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:mfrac></mml:mstyle><mml:munderover><mml:mo movablelimits="false">∑</mml:mo><mml:mrow><mml:mi>t</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow><mml:mi>N</mml:mi></mml:munderover><mml:msup><mml:mfenced close=")" open="("><mml:mi>v</mml:mi><mml:mfenced close=")" open="("><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>,</mml:mo><mml:mi>t</mml:mi></mml:mfenced><mml:mo>-</mml:mo><mml:mi mathvariant="italic">μ</mml:mi><mml:mfenced close=")" open="("><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi></mml:mfenced></mml:mfenced><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:msqrt><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr></mml:mtable></mml:math></disp-formula>

            where <inline-formula><mml:math id="M96" display="inline"><mml:mrow><mml:mi mathvariant="italic">δ</mml:mi><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> is the standard deviation of this reference field. This
method is similar to the robust satellite technique (RST) method, which
introduces the concept of SNR. The difference between current and mean
values of a reference field represents the signal part, and the standard
deviation of a reference field is the noise part. A higher SNR indicates a
greater possibility of anomalies prior to an earthquake (Tramutoli et al.,
2001).</p>
</sec>
<sec id="Ch1.S3.SS3">
  <title>RST method</title>
      <p id="d1e2365">At present, RST, which is extensively used in the anomaly detection, is a
multi-temporal statistical method for analyzing long-term satellite records
with similar observation conditions (e.g., same month, same time of day, and
same sensor data) (Genzano et al., 2015; Lisi et al., 2010; Pergola et al.,
2010; Tramutoli et al., 2005). RST combines the neighborhood difference in
the eddy field method and the normalization of the reference field in the ZS
method, and it clearly defines the mathematical expression of the
pre-seismic anomaly in statistics. This method considers the statistical
characteristics of the historical data in seismically active areas to
discriminate the possible pre-seismic abnormal behavior of current signals.
It is also considered applicable to different atmosphere and surface
conditions and different satellite observation geometries and can reduce
the probability of occurrence of false anomalies (Filizzola et al., 2004;
Pergola et al., 2010).</p>
      <p id="d1e2368">The robust estimator of TIR anomalies (RETIRA) index is used to express the
intensity of anomalies in RST method,  as follows:

                <disp-formula specific-use="align" content-type="numbered"><mml:math id="M97" display="block"><mml:mtable rowspacing="5.690551pt" displaystyle="true"><mml:mlabeledtr id="Ch1.E6"><mml:mtd/><mml:mtd><mml:mstyle displaystyle="true" class="stylechange"/></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:msub><mml:mo>⊗</mml:mo><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>v</mml:mi></mml:mrow></mml:msub><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>,</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo><mml:mo>=</mml:mo><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>v</mml:mi><mml:mfenced open="(" close=")"><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>,</mml:mo><mml:mi>t</mml:mi></mml:mfenced><mml:mo>-</mml:mo><mml:msub><mml:mi mathvariant="italic">μ</mml:mi><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>v</mml:mi></mml:mrow></mml:msub><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>)</mml:mo></mml:mrow><mml:mrow><mml:msub><mml:mi mathvariant="italic">δ</mml:mi><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>v</mml:mi></mml:mrow></mml:msub><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E7"><mml:mtd/><mml:mtd><mml:mstyle displaystyle="true" class="stylechange"/></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>v</mml:mi><mml:mfenced open="(" close=")"><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>,</mml:mo><mml:mi>t</mml:mi></mml:mfenced><mml:mo>=</mml:mo><mml:mi>v</mml:mi><mml:mfenced close=")" open="("><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>,</mml:mo><mml:mi>t</mml:mi></mml:mfenced><mml:mo>-</mml:mo><mml:mover accent="true"><mml:mi>v</mml:mi><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr></mml:mtable></mml:math></disp-formula>

            where <inline-formula><mml:math id="M98" display="inline"><mml:mrow><mml:mover accent="true"><mml:mi>v</mml:mi><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> is the spatially average value in the
homogeneous neighborhood, such that <inline-formula><mml:math id="M99" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>v</mml:mi><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>,</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> represents
the difference between the value of a pixel in (<inline-formula><mml:math id="M100" display="inline"><mml:mi>x</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math id="M101" display="inline"><mml:mrow><mml:mi>y</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> and ambient homogeneous
pixels; <inline-formula><mml:math id="M102" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">μ</mml:mi><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>v</mml:mi></mml:mrow></mml:msub><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M103" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">δ</mml:mi><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>v</mml:mi></mml:mrow></mml:msub><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> are, respectively, the mean and standard
deviation in (<inline-formula><mml:math id="M104" display="inline"><mml:mi>x</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math id="M105" display="inline"><mml:mrow><mml:mi>y</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> of the reference field calculated from <inline-formula><mml:math id="M106" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>v</mml:mi><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>,</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> in the same or similar time slot from many years, which are
referred to Eq. (2) and (5). The RETIRA index is further used to indicate
the relationship with future seismic activity. Generally, a value greater
than 3 to 4 is used as the threshold for the presence of anomalies that are
associated with possible earthquake occurrences (Eleftheriou et al., 2016;
Lisi et al., 2010, 2015).</p>
      <p id="d1e2670">If continuous and large-scale anomalies appear from a time series of images
within study areas, then they can be considered as pre-seismic anomalies
(Aliano et al., 2008). Therefore, an index of significant sequences of
thermal anomalies (SSTAs), which measures the persistence and continuity of
thermal anomalies in temporal and spatial patterns, is defined to remove
problematic values as far as possible (Genzano et al., 2015; Lisi et al.,
2015). SSTAs standards include the following: (1) relative strength, in which the RETIRA
index is greater than or equal to 3; (2) spatial persistence, in which the area of
thermal anomalous pixels in the region of <inline-formula><mml:math id="M107" display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mo>×</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula> is larger than 150 km<inline-formula><mml:math id="M108" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula>; and (3) temporal continuity, in which the
phenomenon of thermal anomalies occurs at least once within 7 days before or
after current time.</p>
      <p id="d1e2702">The purpose of SSTAs is similar to that of a deviation–time–space–thermal
(DTS-T) anomaly recognition method proposed by Wu et al. (2012), which is
applied to analyses of several large earthquakes. The DTS-T method defines a
normalized quantitative index to express the stability of thermal anomalies
considering the significance of numerical differences, synchronization of
time, and adjacency of geographical location. Both indices are intended to
improve the stability of detected thermal anomalies that are related to
impending earthquakes as much as possible. In addition, geostationary
satellite data are more advantageous than polar-orbiting satellite data in
the anomaly detection (Aliano et al., 2008; Lisi et al., 2015) because
they have higher temporal resolution and a fixed observation geometry, and
thereby its data have a higher SNR in detecting seismically related
anomalies when using RST-based method. The principle of this algorithm is
concise; however, the impact of short-term meteorological warming is
also difficult to eliminate. Therefore, this method should be combined with other
data to identify the interpretation of anomaly detection results.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F9" specific-use="star"><caption><p id="d1e2708">Time series of MODIS LST for the Dalbandin earthquake on 19 January 2011
(Saraf et al., 2012).</p></caption>
          <?xmltex \igopts{width=483.69685pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/18/1013/2018/nhess-18-1013-2018-f09.png"/>

        </fig>

</sec>
<sec id="Ch1.S3.SS4">
  <title>Methods based on wavelet transform</title>
      <p id="d1e2724">Wavelet analysis is one of the most popular seismic anomaly detection
methods in recent years. Wavelet decomposition, wavelet packet, and power
spectrum are used in determining the transformation and decomposition of TIR
signals to extract useful feature signals for identifying pre-seismic
anomalies. Wavelet transform has the feature of multi-resolution analysis,
which can characterize the local characteristics of the signal in
time–frequency domain.</p>
      <p id="d1e2727">The influence factors of surface thermal radiation are complex and varied;
therefore, influences of various field sources are difficult to separate.
Furthermore, non-tectonic factors, such as landforms, land covers, and
meteorology, always have greater effects on thermal radiation than tectonic
activities or thermal radiation induced by earthquakes. The weak signal
under strong interference is difficult to separate, resulting in unstable
results of anomaly detection methods. Continuous TIR radiation data can be
considered to include the long-period components (e.g., the basic radiation
field<?pagebreak page1025?> of the Earth, the interannual or seasonal radiation field, and
terrain induced radiation field), the short-period components (e.g., diurnal
radiation field, cloud and cold air flow in several hours to days, and
thermal radiation components caused by tectonic movements or earthquakes),
and the last residual factors (e.g., high-frequency noise components).
Wavelet transform can decompose the time series signal into signals of
different frequency bands that correspond to the above different components;
thus, studying the energy variation in each frequency band is convenient.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F10" specific-use="star"><caption><p id="d1e2732">The spatiotemporal evolution of BT anomalies derived by the RPS
method for the 2008 <inline-formula><mml:math id="M109" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mtext>s</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> 8.0 Wenchuan earthquake (Zhang et al., 2010).</p></caption>
          <?xmltex \igopts{width=483.69685pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/18/1013/2018/nhess-18-1013-2018-f10.jpg"/>

        </fig>

      <p id="d1e2752">The relative power spectrum (RPS) method performs wavelet transform on time
series data to realize bandpass filtering, remove long- and short-period
components, and retain certain intermediate frequency band information that
may be connected with seismic-related signal changes and is expressed in the
form of power spectrum. RPS method was used to analyze BT anomalies of the
2008 Wenchuan earthquake (Zhang et al., 2010). Figure 10 presents the
obvious BT anomalies from 25 April to 19 June 2008 over the Longmenshan
fault zone and demonstrates the good results of the RPS method. The wavelet
transform is initially used to process the multiyear data after cloud
filtering and filling in of missing data. For each pixel, the basic
temperature field, annual variation temperature field, daily variation
temperature field, and other factors can be separated, and remaining
information may include earthquake-related information. The RPS is then
calculated by Fourier transform with a certain time window and sliding
window length.  On the basis of TOA BT, the RPS approach was used to analyze
pre-seismic anomalies, but non-seismic anomalies always appeared (Xie et
al., 2013).</p>
      <p id="d1e2756">The wavelet transform method is used to eliminate low-frequency annual and
seasonal components and high-frequency random components, such as local
meteorological conditions and human activities. The local maxima are then
extracted from time series of MODIS LST data by a predefined threshold, which
is sensitive to peak changes (Saradjian and Akhoondzadeh, 2011). Another
wavelet maxima method proposed by Cervone et al. (2004) uses one-dimensional
wavelet transform to identify the isolated local maxima. The maxima mostly
associated with impending earthquakes are then refined based on the
geometrical continuity from spatial<?pagebreak page1026?> and temporal constraints to remove wrong
maxima lines due to significant noise in input data. Wavelet maxima method
is further utilized to analyze the result of eddy field method (Xiong et
al., 2010).</p>
      <p id="d1e2759">Wavelet transform is based on the communication theory, and thus its
mathematical and physical foundation is complete, making it a highly
promising method. The time series physical quantities derived from remote
sensing are taken as the input information via a series of filtering<?pagebreak page1027?> and
other processing, and finally pre-seismic anomalies are extracted. Wavelet
transform can decompose the time series data into mutually independent
frequency components almost without loss of information. Each component has
a different dominant factor, thereby making the physical meaning much
clearer than other methods. However, the determination of high- and
low-frequency signals in this method requires  geography- and
geology-related knowledge with a certain arbitrariness. Although this
algorithm achieves a high degree of decomposition and analysis of, for example, TIR
signals, the mechanism that relates to earthquake preparation must  be
further improved. Moreover, wavelet transform requires continuous time
series of input data, but missing values in TIR data always appear due to
cloud cover. Thus, the interpolation of missing data is required, which
brings in uncertainties with regard to real values.</p>
</sec>
<sec id="Ch1.S3.SS5">
  <title>Multiparameter comprehensive analysis</title>
      <p id="d1e2768">Single precursor in pre-seismic monitoring research shows its limitations.
Changes in various land, ocean, and atmospheric parameters before and after
strong earthquakes can be observed from satellite platforms, along with
ground measurements. Comprehensive utilization of multiple precursors
provides another promising choice, which can raise the reliability and
credibility of the relationship between different anomalies and imminent
seismic events (Eleftheriou et al., 2016; Singh et al., 2010a). The
preliminary step is to identify which precursors present anomalous
variations prior to strong earthquakes around the epicenter. OLR, air
temperature, and relative humidity were used in the seismic anomaly analysis
for the 2005 <inline-formula><mml:math id="M110" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mtext>w</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> 7.6 Kashmir and 2013 <inline-formula><mml:math id="M111" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mtext>w</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> 7.7 Awaran earthquakes (Mahmood et al.,
2017). Singh et al. (2007) analyzed changes in SLHF, atmospheric water
vapor, SST, wind, cloud liquid water, precipitation rate, and chlorophyll
concentrations prior to and after the 2004 Sumatra earthquake. In short, many
geophysical parameters show abnormal variations prior to earthquakes to some
extent.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F11" specific-use="star"><caption><p id="d1e2795">Time series of four seismic precursor parameters at the
epicentral pixel from March to April 2009: volumetric soil moisture level 1
<bold>(a)</bold>, soil temperature level 1 <bold>(b)</bold>, precipitable water of the entire
atmosphere column <bold>(c)</bold>, and near-surface air temperature at a height of
2 m <bold>(d)</bold> (Wu et al., 2016).</p></caption>
          <?xmltex \igopts{width=327.206693pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/18/1013/2018/nhess-18-1013-2018-f11.png"/>

        </fig>

      <p id="d1e2816">Anomalous variations of parameters in the surface, atmosphere, and ionosphere
prior to earthquakes present interrelations with one another and show the
existence of strong coupling effects (Singh et al., 2007). Multiparametric
analysis of the 2008 Wenchuan earthquake by Jing et al. (2013) indicates
different response times for different parameters. Anomalous OLR occurred
first, followed by air temperature, relative humidity, and air pressure
presented abnormal variations. Finally, SLHF anomaly occurred the day before
the main shock. Wu et al. (2016) used multiple parameters from reanalysis
datasets and ground measurements to interpret the potential LCAC process. In
Fig. 11, the precursor parameters of soil moisture, soil temperature, total
column water vapor, and screen-level air temperature present
quasi-synchronous anomalies in the time window between 29 March and 1 April
2009 preceding the <inline-formula><mml:math id="M112" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mtext>w</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> 6.3 L'Aquila earthquake. Anomalous multiple parameters
also indicate that the process of energy transfer is caused by tectonic
activities, which is from the deep of crust to the land surface and then to
the atmosphere. Multiparametric analysis helps in better understanding the
sequence of processes that occurs in the lithosphere, hydrosphere, and
atmosphere (Mansouri Daneshvar and Freund, 2017).</p>
</sec>
<sec id="Ch1.S3.SS6">
  <title>Other methods</title>
      <p id="d1e2836">The night thermal gradient (NTG) method calculates the linear trend of the
nighttime surface temperature using geostationary satellite LST data with
high temporal resolution (Piroddi and Ranieri, 2012; Piroddi et al., 2014).
In general, the surface temperature at night gradually decreases and reaches
the minimum in the early morning, and thus an NTG value greater than 0 is
regarded as an abnormal temperature increase. Furthermore, the most
intensive anomalies of soil and air temperature are spatially coincident
with TIR anomaly detected by NTG method (Wu et al., 2016). This approach is
highly suitable for the geostationary satellite data that have continuous
time series observations.</p>
      <p id="d1e2839">The interquartile method is used to establish upper and lower boundaries of
temperature changes. The values that exceed boundaries are considered
anomalous values that are associated with possible near-future earthquakes
(Akhoondzadeh, 2013; Saradjian and Akhoondzadeh, 2011). This method is only
sensitive to the highest intensity anomaly, and its formula is as follows:
            <disp-formula id="Ch1.E8" content-type="numbered"><mml:math id="M113" display="block"><mml:mrow><mml:mi>M</mml:mi><mml:mo>-</mml:mo><mml:mi>k</mml:mi><mml:mo>⋅</mml:mo><mml:mtext>IQR</mml:mtext><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mo>&lt;</mml:mo><mml:mi>V</mml:mi><mml:mo>&lt;</mml:mo><mml:mi>M</mml:mi><mml:mo>-</mml:mo><mml:mi>k</mml:mi><mml:mo>⋅</mml:mo><mml:mtext>IQR</mml:mtext><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
          where <inline-formula><mml:math id="M114" display="inline"><mml:mi>M</mml:mi></mml:math></inline-formula> is the median value, <inline-formula><mml:math id="M115" display="inline"><mml:mi>k</mml:mi></mml:math></inline-formula> is a threshold value, IQR is the interquartile
range between 75th and 25th percentiles, and <inline-formula><mml:math id="M116" display="inline"><mml:mi>V</mml:mi></mml:math></inline-formula> is the observed value. This
equation can be reformed as
            <disp-formula id="Ch1.E9" content-type="numbered"><mml:math id="M117" display="block"><mml:mrow><mml:mfenced open="|" close="|"><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mi>V</mml:mi><mml:mo>-</mml:mo><mml:mi>M</mml:mi></mml:mrow><mml:mtext>IQR</mml:mtext></mml:mfrac></mml:mstyle></mml:mfenced><mml:mo>&lt;</mml:mo><mml:mi>k</mml:mi><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula>
          The interquartile method is analogous to the ZS method, in which the average
value and standard deviation are substituted by the medium value and
interquartile range, respectively.</p>
      <p id="d1e2923">A variety of machine learning methods have been used in the anomaly
detection, which show great advantages in various fields in recent years and
may have a considerable potential in this field. Autoregressive integrated
moving average, artificial neural network (ANN), support vector machine, and
adaptive network-based fuzzy inference system (ANFIS) have been compared for
detecting thermal and total electron content anomalies (Akhoondzadeh, 2013).
ANN model can handle well the noise in input data. ANFIS that integrates
both ANN and fuzzy inference systems is more effective at modeling
nonlinear time series predictions than other methods. However, machine
learning methods are always required to set certain empirical parameters,
and appropriate selection of these parameters is a challenging task<?pagebreak page1028?> in
phases of model training and prediction. The Kalman filter method is an
iterative optimization system with high predictive power and is also used
for detecting surface temperature anomalies (Saradjian and Akhoondzadeh,
2011). This approach takes advantage of predicting nonlinear times series
data with non-normal distribution, such as the occurrence of LST anomalies.
These methods are more complex and have not been widely used in the anomaly
detection as other abovementioned methods. The comparison among these
methods with different independent properties should be conducted based on
more earthquake cases in order to screen out more effective approaches.</p>
</sec>
</sec>
<?pagebreak page1029?><sec id="Ch1.S4">
  <title>Issues in pre-seismic anomaly detection</title>
      <p id="d1e2934">We review the possible precursors for pre-earthquake anomaly detection in
Sect. 2 and state several frequently used anomaly detection
methods in Sect. 3. Although these precursors and methods give us some
promising results in which we see some significant anomalies prior to
many earthquake cases, we still need to critique and more deeply analyze them in order to achieve the further goal, i.e., forecasting
moderate and strong earthquakes ahead. Accordingly, in this section, we
point out the misunderstandings in the above-stated studies from the
perspective of data sources and several other aspects.</p>
      <p id="d1e2937">The anomalous phenomena often occur prior to various earthquake cases,
whereas the features of these phenomena are often different. The
interference of clouds is often highly serious, thereby resulting in faint
and unstable evolution patterns in anomalous areas, although certain cases
show clear characteristics of this evolution. Even though many hypotheses
have been used to explain the mechanism of pre-seismic anomalies, the
physical mechanisms that drive various pre-seismic anomalies are yet
insufficiently validated and consequently not widely accepted. Thus far,
objective, stable, and testable detection methods or precursors are still
unavailable for pre-seismic anomalies based on current research and
technology. Therefore, the anomaly detection has not become a
well-recognized technology in the scientific community.
<list list-type="order"><list-item>
      <p id="d1e2942">Some important concerns of mentioned studies are the reasonable
definition of “pre-seismic anomaly” and quantitatively measuring its
quantity. Given that different definitions are used for different methods,
data sources, or even earthquake cases, one method based on one type of data
source may get a good result for one earthquake, but it may be invalid when
using these standards in other earthquakes or the prediction. The arbitrary
definition confuses anomalous signals by earthquake events and impedes
identifying abnormal variations from complicated background signals.</p></list-item><list-item>
      <p id="d1e2946">Quantitatively validating results by anomaly detection methods is
difficult partly because of the previous difficulty of the definition.
Whether anomalies detected in one earthquake case are general or incidental
phenomena is often controversial. One of the general strategies is based on
the validation and confutation method for verification (Genzano et al.,
2015; Lisi et al., 2010, 2015; Xiong et al., 2013). In the
validation phase, anomalies associated with earthquakes should be found;
however, no anomalies should be confirmed in the confutation phase.
Nevertheless, the validation and confutation approach alone is not enough.
Most research results are based on and limited to a handful of case studies.
Therefore, obtaining convincing conclusion from statistical results is
difficult when earthquake cases are insufficient in the statistics analysis
(Pulinets and Dunajecka, 2007).</p></list-item><list-item>
      <p id="d1e2950">Providing complete spatiotemporal data is difficult because of
atmospheric interference, cloud cover, and instrument performance. Satellite
remote sensing on polar-orbiting or geostationary platforms provides the
most important data sources at regional or global scales, which are
beneficial for global seismic monitoring studies. Surface data products,
such as LST, can be used in analyzing pre-seismic anomalies to mitigate the
atmospheric effect. However, the greatest weakness of TIR remote sensing is
that it cannot penetrate clouds to obtain surface thermal radiation
information. This weakness results in the existence of a large number of
missing pixels in the data product, seriously affects anomaly detection,
hinders the understanding of spatiotemporal evolution of pre-seismic
anomalies in a broader time scale, and finally leads to many cases of
omission or false positive rates (Lisi et al., 2015). Therefore, addressing
the significant issue of cloud interference is critical in the anomaly
detection when monitoring the seismically active regions.</p></list-item><list-item>
      <p id="d1e2954">Other factors, including the surface (e.g., topography, geomorphology,
and land covers) and atmosphere (e.g., cloud, precipitation, and wind), also
strongly influence the change of surface thermal radiation (Chen et al.,
2013, 2014). Satellite thermal anomalies (e.g., air temperature
or OLR anomalies) are vulnerable to local atmospheric conditions, such as
the inversion of air temperature, thereby resulting in inaccuracies in
detecting earthquake anomalies. Thus, more attention should be given to the
possibility that other causes other than seismic activities should be
responsible for the extracted all kinds of anomalies. In particular,
anthropogenic activities in factories and urban areas also have a
significant effect on the anomaly detection (Piroddi and Ranieri, 2012). For
instance, removing the normal fluctuations of thermal emission related to
meteorological or artificial factors from the earthquake-imposed thermal
anomalies is an urgent problem that must be solved.</p></list-item><list-item>
      <p id="d1e2958">Nowadays, the data with low spatial resolution have been successfully
used in the anomaly detection, such as NOAA OLR data with 2.5<inline-formula><mml:math id="M118" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>
spatial resolution (Liebmann, 1996). The spatial scale of OLR anomaly from
<inline-formula><mml:math id="M119" display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mo>×</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula> NOAA data is approximately 1000–2000 km from epicenters (Xiong and Shen, 2017), which is an unexpected result for
the seismic activity monitoring. However, the use of satellite data with a
high spatial resolution (e.g., 1 km) can provide richer and deeper
information. This way, the spatial location of different anomalies can be
better correlated with seismic activity areas, which is more conducive to
studying the characteristics of spatial anomalies, rather than limited<?pagebreak page1030?> to
single point or local areas. For example, high- or low-temperature bands
occur before rock bursts, and the main ruptures may occur along these band
areas and result in temperature anomalies; however, data with coarse
resolution are difficult to accurately capture such active tectonic
positions.</p></list-item><list-item>
      <p id="d1e2991">The mechanism of pre-seismic anomalies is still inconclusive. Several
mechanisms for generation of pre-seismic anomalies detected by satellites
sensors have been proposed and are in discussion (Saraf et al., 2009;
Tramutoli et al., 2013). The p-hole theory has been proposed to
explain this phenomenon. The electronic charge carriers (positive holes)
release when the peroxy links break in the stressed rocks, arrive at the
Earth's surface and lead to the ionization of air at the ground–air
interface. And the recombination of charge carriers at the surface leads to
a spectroscopically distinct, non-thermal infrared emission (Freund, 2011; Freund
et al., 2009). Besides, a unified LAIC model is proposed in which the radon
emission in fault zones plays an important role (Molchanov et al., 2004;
Pulinets and Ouzounov, 2011). Later, Wu et al. (2016) added the coversphere
to the LAIC model after analyzing its importance in the understanding of
mechanisms and geophysical processes in earthquake preparation areas. The
radon emission in fault zones plays an important role in the LAIC model,
but is physically impossible based on the <inline-formula><mml:math id="M120" display="inline"><mml:mi>p</mml:mi></mml:math></inline-formula>-hole model (Freund,
2011; Freund et al., 2009). Radon is very rare in the average crustal rocks.
Moreover, the measurements of radon emanation on the ground or in the
underground shows that radon emission increases only by a factor of about 10
prior to an earthquake. These insufficient radon atoms cannot bring in a
significant increase of the air conductivity by a factor of 100–250.
Therefore, further validation of these distinctive models is required from
physical simulation experiences and synergetic measurements of
multiparameter in the field. This situation leads to weak physical mechanism
of detection algorithms and arbitrary explanations about results of various
anomalies. These defects seriously restrict the application and
popularization of this approach.</p></list-item></list></p>
</sec>
<sec id="Ch1.S5" sec-type="conclusions">
  <title>Future development and perspectives</title>
      <p id="d1e3007">Thus far, no single measurable geophysical variable and data analysis method
illustrates considerable potential for a sufficiently reliable and effective
operational earthquake forecasting practice. Forecasting moderate and strong
earthquakes in the future several months to days at the regional or global
scale is of high social value, which is the advantage of satellite
monitoring. Based on the discussion in the preceding section, the following
perspectives are expected.
<list list-type="order"><list-item>
      <p id="d1e3012">Passive microwave remote sensing can obtain surface BT data under clouds,
which is less affected by atmospheric conditions. Although passive microwave
data generally have lower spatial resolution (10–50 km in the nadir view)
than that of TIR data (1–5 km), they remain sufficient for monitoring
pre-seismic anomalies at a global scale (Lisi et al., 2015). The fusion of
TIR and passive microwave data is an important aspect for realizing the
global observation of surface temperature (Duan et al., 2017; Wang et al.,
2014). The data fusion technique can take advantage of the high precision
and spatial resolution of satellite TIR data and the ability of microwave to penetrate clouds. The improvement of spatial resolution of
prospective passive microwave sensors could be favorable to matching
different data sources.</p></list-item><list-item>
      <p id="d1e3016">A variety of precursors has been used in the pre-seismic anomaly
detection with different uncertainties. Thus, joint application and analysis
of multiple parameters could be a choice to enhance the robustness about the
earthquake forecasting. The results of multiparameter anomaly detection are
combined to form a more reliable collective result, which reduces false
anomaly recognitions and uncertainties, therefore improving the stability and
accuracy of earthquake prediction. At the same time, ground measurements,
such as surface and air temperatures along the most important and active
faults, can provide a better understanding and supplement the missing data of
satellite imageries due to persistent cloud cover. Furthermore, other
geophysical data, such as underground temperature, geomagnetism, gravity,
properties of groundwater, and gases, can be combined with satellite data
at the local, regional, or global scales. This integrated study from
different levels of the space, aerial platform, terrestrial surface, and
underground will promote pre-seismic monitoring research (Venkatanathan et
al., 2017).</p></list-item><list-item>
      <p id="d1e3020">A global-scale monitoring system based on a number of satellite data
products, from polar-orbiting and geostationary satellites, can offer
complete earthquake case analysis that renders a better solution for
detecting and analyzing the signals prior to major earthquakes. Furthermore,
abundant satellite data, which are long, global  time series of continuous
measurements, can support the sufficient long-term correlation research for
various candidate precursors. Eleftheriou et al. (2016) analyzed <inline-formula><mml:math id="M121" display="inline"><mml:mrow><mml:mi>M</mml:mi><mml:mo>≥</mml:mo><mml:mn mathvariant="normal">4</mml:mn></mml:mrow></mml:math></inline-formula>
earthquakes using OLR data in Greece for 10 years. Xiong and Shen (2017)
also performed preliminary work on such global statistics of pre-seismic OLR
anomalies. The statistical uncertainties can serve as a priori knowledge to
determine weight coefficients of precursors in a multiparametric monitoring
system.</p></list-item><list-item>
      <p id="d1e3036">In the near future, remote sensing data, which are applicable to seismic
activity monitoring, will be further<?pagebreak page1031?> increased with higher spatial, temporal,
or spectral resolutions. Thus, emerging technologies can be integrated to
improve the predictive efficacy. The ultrahigh spectral TIR data could be
used to derive surface temperature, emissivity, atmospheric profiles of
temperature and humidity, and concentrations of gas composition
simultaneously. Applying these parameters to joint monitoring of the seismic
activity is a possible development direction. New satellite projects, such as
TwinSat, which integrates multiple observation technologies and ground
measurements, can improve the understanding of seismic-triggered LAIC
mechanism (Chmyrev et al., 2013).</p></list-item><list-item>
      <p id="d1e3040">Several methods can be synthetically applied to improve the efficacy of
the anomaly detection, because utilizing only a single approach to identify
the pre-earthquake anomaly is not statistically robust (Bhardwaj et al.,
2017). Moreover, integrating multiple methods has shown good potential
in improving the capability of detecting actual anomalies. Given that
qualitative analysis is subjectively influenced, developing quantitative
anomaly detection method is a promising direction, which is also beneficial
in realizing the comprehensive application of various methods.
(Akhoondzadeh, 2013; Saradjian and Akhoondzadeh, 2011). For example,
probability models that can integrate multiple methods or even various
precursor variables may provide a more credible prediction with quantitative
statistical uncertainties, other than the qualitative voting selection.
Meanwhile, developing new algorithms based on novel data mining techniques
(e.g., machine learning), which explore the possibility of enhancing the
performance in earthquake prediction, can optimize this multi-method scheme.</p></list-item><list-item>
      <p id="d1e3044">The evaluation of anomaly detection algorithms can contribute to the
investigation of the defects of methods and verify their validity. Building the
quantitative determination of indicators and anomaly-identifying standards
in the evaluation is imperative, which is the basis for quantitatively
estimating the efficacy of methods and comparability among them. According
to these indicators and standards, the big data statistical analysis based
on long-term series of remote sensing data and global earthquake cases is an
important means to establishing the statistical relationship between
pre-seismic anomalies and earthquake events. In view of mathematics, these
steps can maximally eliminate subjectivity. Furthermore, the credibility of
anomalies derived by satellite data can be improved only after several means
of verification and in-depth reveal of the regularity and precursory
characteristics of the earthquake. Analyses of detection results should
combine with fault activities, crustal stress changes, and underground heat
flow. The spatial distribution of various anomalies, such as LST anomaly,
should be consistent with the fault activity mode and its mechanical model.
After excluding the influence of non-tectonic factors, the derived anomalies
should be analyzed together with measurements from other means (e.g.,
meteorological data). More importantly, the proposed methods could be easily
inspected by other researchers to ensure the reproducibility, thereby
increasing statistical significance of detection results. Thus, anomaly
detection criteria should be clearly established and strictly used in other
earthquake case studies and subsequent earthquake prediction (Zhang et al.,
2013).</p></list-item><list-item>
      <p id="d1e3048">The study of geophysical mechanisms and development of theoretical models
about pre-seismic anomalies should be strengthened or even updated. The
numerical simulation based on knowledge of seismotectonics can be used to
establish the relationship between anomalous signals and seismic events. The
diagnostic index with practical value could be created based on this
relationship, and the problem of anomaly index construction may be
theoretically solved. Meanwhile, the former theories should also be examined
with new minds and technologies. For example, the micro-fracturing theory is
somehow fragile (Freund, 2011). By the basic definition, fracturing can
create new surfaces and is possible only if empty space is created between
the two sides of the crack. For the rocks at seismogenic depth (7–45 km and
deeper), the overload is so large that the possibility of creating any
micro- or macro-fracturing is very small. In other words, the difference
between hydrostatic and lithostatic pressure becomes so large that open
porosity of rocks cannot be maintained. Besides, the synergistic
observations of relevant parameters from underground to ionosphere in
seismically active regions are necessary to validate these theoretical
models.</p></list-item></list>
Nonetheless, further efforts on satellite anomaly detection are required to
study the physical mechanism, new satellite data, and anomaly detection
approaches. Although various techniques with different measurements and
approaches have been used in this field for decades and show the potential
and possibility for the recognition of seismic precursors, no  technique
has the full ability to forecast imminent strong earthquakes in the short
(e.g., a few weeks) or long term (e.g., several years). Additionally, current
pre-seismic anomalies monitoring techniques from optical satellite
observations could also not forewarn the earthquake or reduce the seismic
risk in practice. Despite the difficulties in pre-seismic monitoring,
previous studies have shown that, to some extent, a link exists between a
variety of anomalies of satellite observations and seismic activities.
Therefore, the practicality of the anomaly detection in earthquake
monitoring could be advanced from many perspectives based on existing
research foundation. The anomalies which might be induced by seismic
activities theoretically should be contained within the temporal and spatial
distributions of satellite spectral information. Thus, the researches on the
pre-earthquake anomalies monitoring from satellite platforms are of high
scientific interest with the rapid development of remote sensing technology.
Analyzing the correlation between different anomalies and seismicity
provides a promising way for short-term earthquake prediction and
accelerates the present capability on seismic hazard assessment and early
warning.</p>
</sec>

      
      </body>
    <back><notes notes-type="dataavailability">

      <p id="d1e3056">No data sets were used in this article.</p>
  </notes><notes notes-type="authorcontribution">

      <p id="d1e3062">ZHJ designed the framework and
wrote the manuscript. JZ and XS modified the paper
and gave useful comments and suggestions.</p>
  </notes><notes notes-type="competinginterests">

      <p id="d1e3068">The authors declare that they have no conflict of
interest.</p>
  </notes><ack><title>Acknowledgements</title><p id="d1e3074">This work is founded by Basic Science Research
Plan of Institute of Geology, China Earthquake Administration (grant nos.
IGCEA1515 and IGCEA1620), and Scientific Research Project of Shanghai Science
and Technology Commission (grant no. 14231202600). Additionally, we wish to thank
Prof. Shunyun Chen (State Key Laboratory of Earthquake Dynamics, Institute
of Geology, China Earthquake Administration), who discussed the physical
mechanism of the pre-seismic anomalies with us and helped to modify the
corresponding sections of this paper. Special thanks are also given to
two reviewers for their valuable comments and suggestions that greatly
improved this paper.<?xmltex \hack{\newline}?><?xmltex \hack{\newline}?>
Edited by: Jean-Philippe Malet<?xmltex \hack{\newline}?>
Reviewed by: Maria Fabrizia Buongiorno and one anonymous <?xmltex \hack{\break}?>referee</p></ack><ref-list>
    <title>References</title>

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<abstract-html><p>Detecting various anomalies using optical satellite data
prior to strong earthquakes is key to understanding and forecasting
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satellite observations serve as a powerful tool in monitoring earthquake
preparation areas at a global scale and in a nearly real-time manner. Over
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different anomaly detection methods, which are used to extract anomalous
signals that probably indicate future seismic events, are presented.
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discussed. The development of Earth observation satellites and anomaly
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advanced tools for multilevel earthquake monitoring, and improve short- and
medium-term forecasting, which  play a large and growing role in
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