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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">
  <front>
    <journal-meta><journal-id journal-id-type="publisher">NHESS</journal-id><journal-title-group>
    <journal-title>Natural Hazards and Earth System Sciences</journal-title>
    <abbrev-journal-title abbrev-type="publisher">NHESS</abbrev-journal-title><abbrev-journal-title abbrev-type="nlm-ta">Nat. Hazards Earth Syst. Sci.</abbrev-journal-title>
  </journal-title-group><issn pub-type="epub">1684-9981</issn><publisher>
    <publisher-name>Copernicus Publications</publisher-name>
    <publisher-loc>Göttingen, Germany</publisher-loc>
  </publisher></journal-meta>
    <article-meta>
      <article-id pub-id-type="doi">10.5194/nhess-19-2841-2019</article-id><title-group><article-title>Analysis of spatiotemporal variations in middle-tropospheric to upper-tropospheric  methane during the Wenchuan <inline-formula><mml:math id="M1" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">8.0</mml:mn></mml:mrow></mml:math></inline-formula> <?xmltex \hack{\break}?> earthquake by three indices</article-title><alt-title>Spatiotemporal variations in middle-tropospheric</alt-title>
      </title-group><?xmltex \runningtitle{Spatiotemporal variations in middle-tropospheric}?><?xmltex \runningauthor{J.~Cui et al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes" rid="aff1">
          <name><surname>Cui</surname><given-names>Jing</given-names></name>
          <email>jingcui_86@yahoo.com</email>
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Shen</surname><given-names>Xuhui</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Zhang</surname><given-names>Jingfa</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Ma</surname><given-names>Weiyu</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Chu</surname><given-names>Wei</given-names></name>
          
        </contrib>
        <aff id="aff1"><label>1</label><institution>Key Laboratory of Crustal Dynamics, Institute of Crustal Dynamics, <?xmltex \hack{\break}?>China Earthquake Administration, Beijing 100085, China</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>China Earthquake Networks Center, Beijing 100045, China</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Jing Cui (jingcui_86@yahoo.com)</corresp></author-notes><pub-date><day>17</day><month>December</month><year>2019</year></pub-date>
      
      <volume>19</volume>
      <issue>12</issue>
      <fpage>2841</fpage><lpage>2854</lpage>
      <history>
        <date date-type="received"><day>13</day><month>November</month><year>2018</year></date>
           <date date-type="rev-request"><day>7</day><month>January</month><year>2019</year></date>
           <date date-type="rev-recd"><day>18</day><month>September</month><year>2019</year></date>
           <date date-type="accepted"><day>28</day><month>October</month><year>2019</year></date>
      </history>
      <permissions>
        <copyright-statement>Copyright: © 2019 </copyright-statement>
        <copyright-year>2019</copyright-year>
      <license license-type="open-access"><license-p>This work is licensed under the Creative Commons Attribution 4.0 International License. To view a copy of this licence, visit <ext-link ext-link-type="uri" xlink:href="https://creativecommons.org/licenses/by/4.0/">https://creativecommons.org/licenses/by/4.0/</ext-link></license-p></license></permissions><self-uri xlink:href="https://nhess.copernicus.org/articles/.html">This article is available from https://nhess.copernicus.org/articles/.html</self-uri><self-uri xlink:href="https://nhess.copernicus.org/articles/.pdf">The full text article is available as a PDF file from https://nhess.copernicus.org/articles/.pdf</self-uri>
      <abstract><title>Abstract</title>
    <p id="d1e142">This research studied the spatiotemporal variation in methane in the middle to upper troposphere during the Wenchuan earthquake (12 May 2008) using AIRS retrieval data and discussed the methane anomaly mechanism.
Three indices were proposed and used for analysis. Our results show that the methane concentration increased significantly in 2008, with an average increase of <inline-formula><mml:math id="M2" display="inline"><mml:mrow><mml:mn mathvariant="normal">5.12</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">8</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>, compared to the average increase of
<inline-formula><mml:math id="M3" display="inline"><mml:mrow><mml:mn mathvariant="normal">1.18</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">8</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> in the previous 5 years. The absolute local index of change of the environment (ALICE) and differential value (diff) indices can be used to identify methane concentration anomalies. The two indices showed that the methane concentration distribution before and after
the earthquake broke the distribution features of the background field.
As the earthquake approached, areas of high methane concentration gradually
converged towards the west side of the epicenter from both ends of
the Longmenshan fault zone. Moreover, a large anomalous area was centered at the epicenter 8 d before the earthquake occurred, and a trend of strengthening, weakening and strengthening appeared over time.
The gradient index showed that the vertical direction obviously increased before the main earthquake and that the value was positive. The gradient value is negative during coseismic or post-seismic events. The gradient index reflects the gas emission characteristics to some extent. We also determined that the methane release was connected with the deep crust–mantle stress state, as well as micro-fracture generation and expansion. However, due to the lack of any technical means to accurately identify the source and content of methane in the atmosphere before the earthquake, an in-depth discussion has not been conducted, and further studies on this issue may be needed.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <label>1</label><title>Introduction</title>
      <p id="d1e190">The great Wenchuan <inline-formula><mml:math id="M4" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">8.0</mml:mn></mml:mrow></mml:math></inline-formula> earthquake, on 12 May 2008, occurred in the Longmenshan fault zone in western Sichuan Province, China. Its epicenter was located at 30.95<inline-formula><mml:math id="M5" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 103.40<inline-formula><mml:math id="M6" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E. The extent of the earthquake and aftershock affected areas in the northeast along the Longmen Shan fault, a thrust structure along the border of the Tibetan Plateau and the western Sichuan Basin (Fig. <xref ref-type="fig" rid="Ch1.F1"/>). This earthquake was one of the worst continental earthquake events to have struck China in recent decades, and it killed more than 10 000 people in several cities along the western Sichuan basin. A surface rupture more than 200 km long formed along the Yingxiu–Beichuan fault. The Guanxian–Jiangyou fault was also ruptured by surface ruptures that were more than 60 km long, as indicated.
The Longmenshan fault zone has a high dipping angle (more than 50–60<inline-formula><mml:math id="M7" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>) near the surface and a low angle at depth (15–20 km).
This listric shape favors significant strain or energy accumulation, forming large earthquakes. This earthquake was characterized by slow strain accumulation, a long recurrence interval and significant damage power.
It is a new type of earthquake that deserves further study <xref ref-type="bibr" rid="bib1.bibx36" id="paren.1"/>.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1"><?xmltex \currentcnt{1}?><label>Figure 1</label><caption><p id="d1e243">Map of the active faults and the location of the Wenchuan earthquake. LMS denotes the Longmenshan fault zone; XSH denotes the Xianshuihe fault zone; DLS denotes the Daliangshan fault zone; ANH denotes the Anninghe fault zone.</p></caption>
        <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/19/2841/2019/nhess-19-2841-2019-f01.png"/>

      </fig>

      <p id="d1e252">The variation in soil gas concentration serves as a useful tool for monitoring earthquakes. Numerous field investigations have indicated that large amounts of gases are emitted from active fault zones before, during and after great earthquakes. The increased gas emanation from the Earth’s crust in the vicinity of active tectonic faults is triggered by a chain of physical processes and chemical reactions from the ground surface. This complex chain leads to geochemical, atmospheric, ionospheric and magnetospheric anomalies <xref ref-type="bibr" rid="bib1.bibx5 bib1.bibx19 bib1.bibx16" id="paren.2"/>. The number of pre-earthquake thermal, surface latent heat flux and outgoing longwave radiation anomalies apparently results from earthquake-related gas emission from the lithosphere <xref ref-type="bibr" rid="bib1.bibx28 bib1.bibx4 bib1.bibx27 bib1.bibx16 bib1.bibx26" id="paren.3"/>. Thermal <xref ref-type="bibr" rid="bib1.bibx39" id="paren.4"/>, ionospheric <xref ref-type="bibr" rid="bib1.bibx12 bib1.bibx13 bib1.bibx41" id="paren.5"/>, electromagnetic <xref ref-type="bibr" rid="bib1.bibx37" id="paren.6"/>
and aerosol <xref ref-type="bibr" rid="bib1.bibx21" id="paren.7"/> anomalies were found before the Wenchuan earthquake of 12 May 2008.</p>
      <p id="d1e275">As the second most important greenhouse gas after carbon dioxide (<inline-formula><mml:math id="M8" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>), methane (<inline-formula><mml:math id="M9" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>) is approximately 20 times better at warming the atmosphere than <inline-formula><mml:math id="M10" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> by weight and plays an important role in atmospheric chemistry. Some people have speculated that thermal abnormalities before earthquakes are related to the release of <inline-formula><mml:math id="M11" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>. The <inline-formula><mml:math id="M12" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> release mechanism has been investigated and results indicate strong methane emissions when friction is applied to marl-type rock <xref ref-type="bibr" rid="bib1.bibx15 bib1.bibx9" id="paren.8"/>. <xref ref-type="bibr" rid="bib1.bibx35" id="text.9"/> indicated that the Wenchuan earthquake of 12 May 2008 was caused by the rapid migration and expansion of a large amount of highly pressurized and dense <inline-formula><mml:math id="M13" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> gas in crustal rock masses <xref ref-type="bibr" rid="bib1.bibx35" id="paren.10"/>. Sample results indicated that <inline-formula><mml:math id="M14" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> was discharged from a shallow reservoir through
faults or fractures caused by the earthquake <xref ref-type="bibr" rid="bib1.bibx40" id="paren.11"/>. This study chooses to study the spatiotemporal variations in <inline-formula><mml:math id="M15" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> during the
<inline-formula><mml:math id="M16" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">8.0</mml:mn></mml:mrow></mml:math></inline-formula> Wenchuan earthquake from satellite observations.</p>
      <p id="d1e395"><inline-formula><mml:math id="M17" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> satellite observations have begun to be applied to seismological studies over recent years. The total column of <inline-formula><mml:math id="M18" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> associated with the 12 May 2008 Wenchuan earthquake was investigated using satellite data from the AQUA Atmospheric Infrared Sounder (AIRS), and this work indicates that a large amount of <inline-formula><mml:math id="M19" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> was emitted from underground into the atmosphere along the Longmenshan fault zone, from approximately 1.5 months before to 3 months after the earthquake, and the closer to the epicenter, the larger the amount of emitted gas. The peak values were found at intersection areas <xref ref-type="bibr" rid="bib1.bibx35 bib1.bibx3" id="paren.12"/>. However, the same column concentration might correspond to this distinct vertical structure. It is difficult to say whether the <inline-formula><mml:math id="M20" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> anomaly is due to local sources or other atmospheric movements. The gas profile can help us understand the terrestrial emission caused by the earthquake. Recently, NASA declared that the total column values reported for <inline-formula><mml:math id="M21" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> constituents
are dominated by the initial guess of each and should not be used for research purposes
(<uri>https://docserver.gesdisc.eosdis.nasa.gov/repository/Mission/AIRS/3.7_ScienceDataProductValidation/V6_Data_Disclaimer.pdf</uri>, last access: 30 November 2019). Previous work has shown that an AIRS for tropospheric observation can be used to carry out the study with considerable precision <xref ref-type="bibr" rid="bib1.bibx38 bib1.bibx34" id="paren.13"/>.</p>
      <p id="d1e462">Systematic observation of the vertical variation in <inline-formula><mml:math id="M22" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> is scarce.
The focus of this study is to examine the spatiotemporal variation in <inline-formula><mml:math id="M23" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> in the middle to upper troposphere during the Wenchuan earthquake (12 May 2008) using AIRS retrieval data and to discuss the mechanism of the methane anomaly. Three indices were proposed and used for analysis: the absolute local index of change of the environment (ALICE) was used for anomaly detection, the vertical concentration gradient (gradient) was proposed for studying the vertical variation, and the successive differential value (diff) was chosen for showing the time variation. These three indices analyzed the spatial and temporal distribution of <inline-formula><mml:math id="M24" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> before and after the earthquake from horizontal scales, vertical scales and timescales, helping us understand lithospheric and atmospheric interactions during seismic activity.</p>
</sec>
<sec id="Ch1.S2">
  <label>2</label><title>Data and methods</title>
      <p id="d1e506">The version 6 and level 3 standard gridded product of 8 d <inline-formula><mml:math id="M25" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> volume-mixing ratios in a descending model (local nighttime), with 1<inline-formula><mml:math id="M26" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula><inline-formula><mml:math id="M27" display="inline"><mml:mrow><mml:mo>×</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula><inline-formula><mml:math id="M28" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> of spatial resolution, were obtained from the NASA Goddard Earth Sciences Data and Information Services Center (DISC) (<uri>http://disc.gsfc.nasa.gov/AIRS/ index.shtml/</uri>, last access: 30 November 2019). The peak sensitivity of the AIRS to methane retrieval occurs at 300 hPa, and the channels near 7.6 <inline-formula><mml:math id="M29" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>m are most sensitive to the middle to upper troposphere <xref ref-type="bibr" rid="bib1.bibx34" id="paren.14"/>.
Therefore, the volume mixing ratio of the middle troposphere (400 hPa, approximately 5 km), the upper middle troposphere (300 hPa, approximately 7 km) and the upper troposphere (200 hPa, approximately 11 km) in the descending orbit data was used.</p>
      <p id="d1e561">To extract the methane spatiotemporal anomalies before and after the earthquake, three parameters were applied: the absolute local index of change of the environment (ALICE) <xref ref-type="bibr" rid="bib1.bibx25 bib1.bibx3" id="paren.15"/>,
the vertical concentration gradient (gradient) and the successive differential (diff), all carried out on the basis of eliminating the multiyear background. The background field can partially remove the influence of natural sources such as seasonal changes and surface vegetation, effectively capturing emergency information such as earthquakes, reducing “non-seismic anomalies” to a certain extent, providing criteria for the extraction of seismic anomalies and reducing the misjudgment and leakage of seismic anomalies. It was calculated by Eq. (<xref ref-type="disp-formula" rid="Ch1.E1"/>):

              <disp-formula specific-use="align" content-type="numbered"><mml:math id="M30" display="block"><mml:mtable displaystyle="true"><mml:mlabeledtr id="Ch1.E1"><mml:mtd><mml:mtext>1</mml:mtext></mml:mtd><mml:mtd><mml:mstyle class="stylechange" displaystyle="true"/></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><?xmltex \hack{\hbox\bgroup\fontsize{8.5}{8.5}\selectfont$\displaystyle}?><mml:msub><mml:mi>G</mml:mi><mml:mi mathvariant="normal">ref</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>,</mml:mo><mml:mi>t</mml:mi><mml:mo>,</mml:mo><mml:mi>l</mml:mi><mml:mo>)</mml:mo><mml:mo>=</mml:mo><mml:munderover><mml:mo movablelimits="false">∑</mml:mo><mml:mrow><mml:mi>i</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow><mml:mi>N</mml:mi></mml:munderover><mml:msub><mml:mi>G</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>,</mml:mo><mml:mi>t</mml:mi><mml:mo>,</mml:mo><mml:mi>l</mml:mi><mml:mo>)</mml:mo><mml:mo>/</mml:mo><mml:mi>N</mml:mi><?xmltex \hack{$\egroup}?><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E2"><mml:mtd><mml:mtext>2</mml:mtext></mml:mtd><mml:mtd><mml:mstyle displaystyle="true" class="stylechange"/></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><?xmltex \hack{\hbox\bgroup\fontsize{8.5}{8.5}\selectfont$\displaystyle}?><mml:mi mathvariant="italic">σ</mml:mi><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>,</mml:mo><mml:mi>t</mml:mi><mml:mo>,</mml:mo><mml:mi>l</mml:mi><mml:mo>)</mml:mo><mml:mo>=</mml:mo><mml:msqrt><mml:mrow><mml:munderover><mml:mo movablelimits="false">∑</mml:mo><mml:mrow><mml:mi>i</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow><mml:mi>N</mml:mi></mml:munderover><mml:msup><mml:mfenced close="]" open="["><mml:mrow><mml:msub><mml:mi>G</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>,</mml:mo><mml:mi>t</mml:mi><mml:mo>,</mml:mo><mml:mi>l</mml:mi><mml:mo>)</mml:mo><mml:mo>-</mml:mo><mml:msub><mml:mi>G</mml:mi><mml:mi mathvariant="normal">ref</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>,</mml:mo><mml:mi>t</mml:mi><mml:mo>,</mml:mo><mml:mi>l</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mfenced><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>/</mml:mo><mml:mo>(</mml:mo><mml:mi>N</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>)</mml:mo></mml:mrow></mml:msqrt><?xmltex \hack{$\egroup}?><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr></mml:mtable></mml:math></disp-formula>

          where <inline-formula><mml:math id="M31" display="inline"><mml:mrow><mml:msub><mml:mi>G</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>x</mml:mi></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M32" display="inline"><mml:mi>y</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math id="M33" display="inline"><mml:mi>t</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math id="M34" display="inline"><mml:mrow><mml:mi>l</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> means the gas value in the <inline-formula><mml:math id="M35" display="inline"><mml:mi>l</mml:mi></mml:math></inline-formula> layer of the atmospheric pressure, measured at time <inline-formula><mml:math id="M36" display="inline"><mml:mi>t</mml:mi></mml:math></inline-formula>, corresponding to a location at (centered on) the coordinates (<inline-formula><mml:math id="M37" display="inline"><mml:mi>x</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math id="M38" display="inline"><mml:mi>y</mml:mi></mml:math></inline-formula>); <inline-formula><mml:math id="M39" display="inline"><mml:mrow><mml:msub><mml:mi>G</mml:mi><mml:mi mathvariant="normal">ref</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>x</mml:mi></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M40" display="inline"><mml:mi>y</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math id="M41" display="inline"><mml:mi>t</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math id="M42" display="inline"><mml:mrow><mml:mi>l</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> means the reference fields for the study area, defined as a time average gas value; <inline-formula><mml:math id="M43" display="inline"><mml:mrow><mml:mi mathvariant="italic">σ</mml:mi><mml:mo>(</mml:mo><mml:mi>x</mml:mi></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M44" display="inline"><mml:mi>y</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math id="M45" display="inline"><mml:mi>t</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math id="M46" display="inline"><mml:mrow><mml:mi>l</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> is the standard deviation of historical records collected under the temporal constraint. For this study, <inline-formula><mml:math id="M47" display="inline"><mml:mi>N</mml:mi></mml:math></inline-formula> was defined as 5 years, from 2003 to 2007; <inline-formula><mml:math id="M48" display="inline"><mml:mi>t</mml:mi></mml:math></inline-formula> is the time of the measurement acquisition with <inline-formula><mml:math id="M49" display="inline"><mml:mrow><mml:mi>t</mml:mi><mml:mo>∈</mml:mo><mml:mi mathvariant="italic">τ</mml:mi></mml:mrow></mml:math></inline-formula>, where <inline-formula><mml:math id="M50" display="inline"><mml:mi mathvariant="italic">τ</mml:mi></mml:math></inline-formula> defines the homogeneous domain of the satellite imagery collected in the same time slot of the day and period (month) of the year; and <inline-formula><mml:math id="M51" display="inline"><mml:mi>l</mml:mi></mml:math></inline-formula> was defined as three layers (400 hPa, 300 and 200 hPa).</p>
      <p id="d1e956">The absolute local index of change of the environment (ALICE) is calculated
by Eq. (<xref ref-type="disp-formula" rid="Ch1.E3"/>) <xref ref-type="bibr" rid="bib1.bibx25 bib1.bibx3" id="paren.16"/>:
          <disp-formula id="Ch1.E3" content-type="numbered"><label>3</label><mml:math id="M52" display="block"><mml:mrow><?xmltex \hack{\hbox\bgroup\fontsize{8.5}{8.5}\selectfont$\displaystyle}?><mml:mi mathvariant="normal">ALICE</mml:mi><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>,</mml:mo><mml:mi>t</mml:mi><mml:mo>,</mml:mo><mml:mi>l</mml:mi><mml:mo>)</mml:mo><mml:mo>=</mml:mo><mml:mfenced close="]" open="["><mml:mrow><mml:mi>G</mml:mi><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>,</mml:mo><mml:mi>t</mml:mi><mml:mo>,</mml:mo><mml:mi>l</mml:mi><mml:mo>)</mml:mo><mml:mo>-</mml:mo><mml:msub><mml:mi>G</mml:mi><mml:mi mathvariant="normal">ref</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>,</mml:mo><mml:mi>t</mml:mi><mml:mo>,</mml:mo><mml:mi>l</mml:mi><mml:mo>)</mml:mo><mml:mo>/</mml:mo><mml:mi mathvariant="italic">σ</mml:mi><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>,</mml:mo><mml:mi>t</mml:mi><mml:mo>,</mml:mo><mml:mi>l</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mfenced><mml:mo>.</mml:mo><?xmltex \hack{$\egroup}?></mml:mrow></mml:math></disp-formula>
        The vertical concentration gradient (gradient) is used to characterize
the vertical variation in gas and is calculated by Eqs. (<xref ref-type="disp-formula" rid="Ch1.E4"/>) to (<xref ref-type="disp-formula" rid="Ch1.E7"/>):

              <disp-formula specific-use="align" content-type="numbered"><mml:math id="M53" display="block"><mml:mtable displaystyle="true"><mml:mlabeledtr id="Ch1.E4"><mml:mtd><mml:mtext>4</mml:mtext></mml:mtd><mml:mtd><mml:mstyle displaystyle="true" class="stylechange"/></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><?xmltex \hack{\hbox\bgroup\fontsize{8}{8}\selectfont$\displaystyle}?><mml:mi mathvariant="normal">gradient</mml:mi><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>,</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo><mml:mo>=</mml:mo><mml:mfenced open="[" close="]"><mml:mrow><mml:mi>G</mml:mi><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>,</mml:mo><mml:mi>t</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>l</mml:mi><mml:mo>)</mml:mo><mml:mo>-</mml:mo><mml:msub><mml:mi>G</mml:mi><mml:mi mathvariant="normal">ref</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>,</mml:mo><mml:mi>t</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>l</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mfenced><mml:mo>/</mml:mo><mml:mi mathvariant="italic">σ</mml:mi><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>,</mml:mo><mml:mi>t</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>l</mml:mi><mml:mo>)</mml:mo><?xmltex \hack{$\egroup}?><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E5"><mml:mtd><mml:mtext>5</mml:mtext></mml:mtd><mml:mtd><mml:mstyle class="stylechange" displaystyle="true"/></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><?xmltex \hack{\hbox\bgroup\fontsize{8.5}{8.5}\selectfont$\displaystyle}?><mml:mi>G</mml:mi><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>,</mml:mo><mml:mi>t</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>l</mml:mi><mml:mo>)</mml:mo><mml:mo>=</mml:mo><mml:mi>G</mml:mi><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>,</mml:mo><mml:mi>t</mml:mi><mml:mo>,</mml:mo><mml:mi>l</mml:mi><mml:mo>)</mml:mo><mml:mo>-</mml:mo><mml:mi>G</mml:mi><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>,</mml:mo><mml:mi>t</mml:mi><mml:mo>,</mml:mo><mml:mi>l</mml:mi><mml:mo>+</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>)</mml:mo><?xmltex \hack{$\egroup}?><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E6"><mml:mtd><mml:mtext>6</mml:mtext></mml:mtd><mml:mtd><mml:mstyle class="stylechange" displaystyle="true"/></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><?xmltex \hack{\hbox\bgroup\fontsize{8.5}{8.5}\selectfont$\displaystyle}?><mml:msub><mml:mi>G</mml:mi><mml:mi mathvariant="normal">ref</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>,</mml:mo><mml:mi>t</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>l</mml:mi><mml:mo>)</mml:mo><mml:mo>=</mml:mo><mml:munderover><mml:mo movablelimits="false">∑</mml:mo><mml:mrow><mml:mi>i</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow><mml:mi>N</mml:mi></mml:munderover><mml:msub><mml:mi>G</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>,</mml:mo><mml:mi>t</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>l</mml:mi><mml:mo>)</mml:mo><mml:mo>/</mml:mo><mml:mi>N</mml:mi><?xmltex \hack{$\egroup}?><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E7"><mml:mtd><mml:mtext>7</mml:mtext></mml:mtd><mml:mtd><mml:mstyle displaystyle="true" class="stylechange"/></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><?xmltex \hack{\hbox\bgroup\fontsize{8}{8}\selectfont$\displaystyle}?><mml:mi mathvariant="italic">σ</mml:mi><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>,</mml:mo><mml:mi>t</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>l</mml:mi><mml:mo>)</mml:mo><mml:mo>=</mml:mo><mml:msqrt><mml:mrow><mml:munderover><mml:mo movablelimits="false">∑</mml:mo><mml:mrow><mml:mi>i</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow><mml:mi>N</mml:mi></mml:munderover><mml:msup><mml:mfenced open="[" close="]"><mml:mrow><mml:msub><mml:mi>G</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>,</mml:mo><mml:mi>t</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>l</mml:mi><mml:mo>)</mml:mo><mml:mo>-</mml:mo><mml:msub><mml:mi>G</mml:mi><mml:mi mathvariant="normal">ref</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>,</mml:mo><mml:mi>t</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>l</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mfenced><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>/</mml:mo><mml:mo>(</mml:mo><mml:mi>N</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>)</mml:mo></mml:mrow></mml:msqrt><?xmltex \hack{$\egroup}?><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr></mml:mtable></mml:math></disp-formula>

          where gradient (<inline-formula><mml:math id="M54" display="inline"><mml:mi>x</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math id="M55" display="inline"><mml:mi>y</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math id="M56" display="inline"><mml:mi>t</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math id="M57" display="inline"><mml:mrow><mml:mi>l</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> stands for vertical concentration gradient value at level <inline-formula><mml:math id="M58" display="inline"><mml:mi>l</mml:mi></mml:math></inline-formula>, measured at time <inline-formula><mml:math id="M59" display="inline"><mml:mi>t</mml:mi></mml:math></inline-formula>, corresponding to a location at (centered on) the coordinates (<inline-formula><mml:math id="M60" display="inline"><mml:mi>x</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math id="M61" display="inline"><mml:mi>y</mml:mi></mml:math></inline-formula>); <inline-formula><mml:math id="M62" display="inline"><mml:mrow><mml:mi>G</mml:mi><mml:mo>(</mml:mo><mml:mi>x</mml:mi></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M63" display="inline"><mml:mi>y</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math id="M64" display="inline"><mml:mi>t</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math id="M65" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>l</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> means the vertical difference of adjacent layers; <inline-formula><mml:math id="M66" display="inline"><mml:mrow><mml:msub><mml:mi>G</mml:mi><mml:mi mathvariant="normal">ref</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>x</mml:mi></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M67" display="inline"><mml:mi>y</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math id="M68" display="inline"><mml:mi>t</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math id="M69" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>l</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> means the reference fields of the vertical difference for the study area, defined as a time average gas value; <inline-formula><mml:math id="M70" display="inline"><mml:mrow><mml:mi mathvariant="italic">σ</mml:mi><mml:mo>(</mml:mo><mml:mi>x</mml:mi></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M71" display="inline"><mml:mi>y</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math id="M72" display="inline"><mml:mi>t</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math id="M73" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>l</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> is the standard deviation of historical records collected under the temporal constraint; and <inline-formula><mml:math id="M74" display="inline"><mml:mi>l</mml:mi></mml:math></inline-formula> was defined as three layers (400, 300 and 200 hPa).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2" specific-use="star"><?xmltex \currentcnt{2}?><label>Figure 2</label><caption><p id="d1e1670">The 5-year (2003 to 2007) average distribution of 8 d nighttime <inline-formula><mml:math id="M75" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> volume mixing ratios at 200 hPa.</p></caption>
        <?xmltex \igopts{width=298.753937pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/19/2841/2019/nhess-19-2841-2019-f02.png"/>

      </fig>

      <p id="d1e1690">Successive differential value (diff) refers to the difference of the adjacent time gas value and was calculated by Eqs. (<xref ref-type="disp-formula" rid="Ch1.E8"/>) to (<xref ref-type="disp-formula" rid="Ch1.E11"/>):

              <disp-formula specific-use="align" content-type="numbered"><mml:math id="M76" display="block"><mml:mtable displaystyle="true"><mml:mlabeledtr id="Ch1.E8"><mml:mtd><mml:mtext>8</mml:mtext></mml:mtd><mml:mtd><mml:mstyle class="stylechange" displaystyle="true"/></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><?xmltex \hack{\hbox\bgroup\fontsize{8}{8}\selectfont$\displaystyle}?><mml:mi mathvariant="normal">diff</mml:mi><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>t</mml:mi><mml:mo>,</mml:mo><mml:mi>l</mml:mi><mml:mo>)</mml:mo><mml:mo>=</mml:mo><mml:mfenced close="]" open="["><mml:mrow><mml:mi>G</mml:mi><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>t</mml:mi><mml:mo>,</mml:mo><mml:mi>l</mml:mi><mml:mo>)</mml:mo><mml:mo>-</mml:mo><mml:msub><mml:mi>G</mml:mi><mml:mi mathvariant="normal">ref</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>t</mml:mi><mml:mo>,</mml:mo><mml:mi>l</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mfenced><mml:mo>/</mml:mo><mml:mi mathvariant="italic">σ</mml:mi><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>t</mml:mi><mml:mo>,</mml:mo><mml:mi>l</mml:mi><mml:mo>)</mml:mo><?xmltex \hack{$\egroup}?><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E9"><mml:mtd><mml:mtext>9</mml:mtext></mml:mtd><mml:mtd><mml:mstyle displaystyle="true" class="stylechange"/></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><?xmltex \hack{\hbox\bgroup\fontsize{8.5}{8.5}\selectfont$\displaystyle}?><mml:mi>G</mml:mi><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>t</mml:mi><mml:mo>,</mml:mo><mml:mi>l</mml:mi><mml:mo>)</mml:mo><mml:mo>=</mml:mo><mml:mi>G</mml:mi><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>,</mml:mo><mml:mi>t</mml:mi><mml:mo>+</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>,</mml:mo><mml:mi>l</mml:mi><mml:mo>)</mml:mo><mml:mo>-</mml:mo><mml:mi>G</mml:mi><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>,</mml:mo><mml:mi>t</mml:mi><mml:mo>,</mml:mo><mml:mi>l</mml:mi><mml:mo>)</mml:mo><?xmltex \hack{$\egroup}?><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E10"><mml:mtd><mml:mtext>10</mml:mtext></mml:mtd><mml:mtd><mml:mstyle displaystyle="true" class="stylechange"/></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><?xmltex \hack{\hbox\bgroup\fontsize{8.5}{8.5}\selectfont$\displaystyle}?><mml:msub><mml:mi>G</mml:mi><mml:mi mathvariant="normal">ref</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>t</mml:mi><mml:mo>,</mml:mo><mml:mi>l</mml:mi><mml:mo>)</mml:mo><mml:mo>=</mml:mo><mml:munderover><mml:mo movablelimits="false">∑</mml:mo><mml:mrow><mml:mi>i</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow><mml:mi>N</mml:mi></mml:munderover><mml:msub><mml:mi>G</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>t</mml:mi><mml:mo>,</mml:mo><mml:mi>l</mml:mi><mml:mo>)</mml:mo><mml:mo>/</mml:mo><mml:mi>N</mml:mi><?xmltex \hack{$\egroup}?><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E11"><mml:mtd><mml:mtext>11</mml:mtext></mml:mtd><mml:mtd><mml:mstyle class="stylechange" displaystyle="true"/></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><?xmltex \hack{\hbox\bgroup\fontsize{7.8}{7.8}\selectfont$\displaystyle}?><mml:mi mathvariant="italic">σ</mml:mi><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>t</mml:mi><mml:mo>,</mml:mo><mml:mi>l</mml:mi><mml:mo>)</mml:mo><mml:mo>=</mml:mo><mml:msqrt><mml:mrow><mml:munderover><mml:mo movablelimits="false">∑</mml:mo><mml:mrow><mml:mi>i</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow><mml:mi>N</mml:mi></mml:munderover><mml:msup><mml:mfenced close="]" open="["><mml:mrow><mml:msub><mml:mi>G</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>t</mml:mi><mml:mo>,</mml:mo><mml:mi>l</mml:mi><mml:mo>)</mml:mo><mml:mo>-</mml:mo><mml:msub><mml:mi>G</mml:mi><mml:mrow><mml:mi>r</mml:mi><mml:mi>e</mml:mi><mml:mi>f</mml:mi></mml:mrow></mml:msub><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>t</mml:mi><mml:mo>,</mml:mo><mml:mi>l</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mfenced><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>/</mml:mo><mml:mo>(</mml:mo><mml:mi>N</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>)</mml:mo></mml:mrow></mml:msqrt><mml:mo>.</mml:mo><?xmltex \hack{$\egroup}?></mml:mrow></mml:mtd></mml:mlabeledtr></mml:mtable></mml:math></disp-formula></p>
</sec>
<sec id="Ch1.S3">
  <label>3</label><title>Results</title>
<sec id="Ch1.S3.SS1">
  <label>3.1</label><title>Reference field</title>
      <p id="d1e2130">The 8 d average background field at different <inline-formula><mml:math id="M77" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> heights in the study area was obtained and is shown in Figs. <xref ref-type="fig" rid="Ch1.F2"/>–<xref ref-type="fig" rid="Ch1.F4"/>.
These figures show that the <inline-formula><mml:math id="M78" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> concentration in the study area decreased significantly from the middle troposphere to the upper troposphere, and the average methane concentrations (from 9 March to 15 August 2008) in each stratum were 1.794, 1.775 and 1.762 ppm for the middle, upper middle and upper troposphere, respectively. This indicates that the middle troposphere is significantly affected by terrestrial emission sources.</p>
      <p id="d1e2159">The distribution of <inline-formula><mml:math id="M79" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> has obvious seasonal characteristics, and the seasonal cycles at different heights are similar. The <inline-formula><mml:math id="M80" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mixing ratio has a weak high value during March and then decreases during April–May. It starts to increase in June and stays high during July and August, especially over the Sichuan basin. The relatively high values at different times are mostly located at a structural confluence or at tectonic plate boundaries except for late July and August. Earth gas emissions may be the main cause of the high long-term values at that location (<uri>http://www.climatechange2013.org/images/report/P36Doc3_WGI-12_Approved-SPM.pdf</uri>, last access: 4 December 2019). Why does the <inline-formula><mml:math id="M81" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> begin to increase in early summer? Studies have shown <inline-formula><mml:math id="M82" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> emissions significantly correlate with temperature. When the temperature is
<inline-formula><mml:math id="M83" display="inline"><mml:mrow><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">15</mml:mn></mml:mrow></mml:math></inline-formula><inline-formula><mml:math id="M84" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>, the Earth seldom produces <inline-formula><mml:math id="M85" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, and when the temperature reaches 35<inline-formula><mml:math id="M86" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>, <inline-formula><mml:math id="M87" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> production can be many times higher than at 25<inline-formula><mml:math id="M88" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <xref ref-type="bibr" rid="bib1.bibx11 bib1.bibx24 bib1.bibx8 bib1.bibx23 bib1.bibx22" id="paren.17"/>. Therefore, the <inline-formula><mml:math id="M89" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> concentration in the troposphere is higher during July and August. The <inline-formula><mml:math id="M90" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> rice paddy emission, local emissions (such as from gas leakage or energy use) and transport (such as the meridional and zonal advection, convection from the lower troposphere, or stratosphere–troposphere exchange) also increase in early summer <xref ref-type="bibr" rid="bib1.bibx33" id="paren.18"/>.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3" specific-use="star"><?xmltex \currentcnt{3}?><label>Figure 3</label><caption><p id="d1e2299">The 5-year (2003 to 2007) average distribution of 8 d nighttime <inline-formula><mml:math id="M91" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VMR at 300 hPa.</p></caption>
          <?xmltex \igopts{width=298.753937pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/19/2841/2019/nhess-19-2841-2019-f03.png"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4" specific-use="star"><?xmltex \currentcnt{4}?><label>Figure 4</label><caption><p id="d1e2322">The 5-year (2003 to 2007) average distribution of 8 d nighttime <inline-formula><mml:math id="M92" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VMR at 400 hPa.</p></caption>
          <?xmltex \igopts{width=298.753937pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/19/2841/2019/nhess-19-2841-2019-f04.png"/>

        </fig>

      <p id="d1e2342">The results of the background field analysis show that the <inline-formula><mml:math id="M93" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> concentration is greatly influenced by the season, structure and underlying surface, and they present a typical spatial and temporal distribution of methane in southwestern China <xref ref-type="bibr" rid="bib1.bibx38" id="paren.19"/>. Gas emanates from the Earth’s crust continuously, even without earthquakes.</p>
</sec>
<sec id="Ch1.S3.SS2">
  <label>3.2</label><title>Anomalous gas</title>
      <p id="d1e2367">The three indices mentioned above have been applied to identify the spatial and temporal variation in middle-tropospheric and upper-tropospheric methane anomalies associated
with the Wenchuan <inline-formula><mml:math id="M94" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">8.0</mml:mn></mml:mrow></mml:math></inline-formula> earthquake using AIRS data.</p>
<sec id="Ch1.S3.SS2.SSS1">
  <label>3.2.1</label><title>ALICE index result</title>
      <p id="d1e2392">Figures <xref ref-type="fig" rid="Ch1.F5"/>–<xref ref-type="fig" rid="Ch1.F7"/> show that as the earthquake approached, the methane concentration near the LMS fault zone gradually increased and the range gradually expanded. High values began to appear in the northern section of the LMS fault zone on 25 March and began to increase in large areas on 4 May, showing a significant north–south distribution through the LMS fault zone. From 12 to 19 May, the high value decreased near the epicenter but remained in large parts of the study area and persisted in large areas after the earthquake. From 7 July, the northern section of the LMS fault zone again showed high accumulation. From 23 July to 7 August, the high-value zone reached the maximum, and all along the LMS fault zone it showed a NE distribution. Then the high-value areas began to weaken on 8 August. This circle was probably caused by the big aftershocks on 24 July and 1 August.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F5" specific-use="star"><?xmltex \currentcnt{5}?><label>Figure 5</label><caption><p id="d1e2401">ALICE index of 8 d <inline-formula><mml:math id="M95" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VMR at 200 hPa.</p></caption>
            <?xmltex \igopts{width=284.527559pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/19/2841/2019/nhess-19-2841-2019-f05.png"/>

          </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F6" specific-use="star"><?xmltex \currentcnt{6}?><label>Figure 6</label><caption><p id="d1e2423">ALICE index of 8 d <inline-formula><mml:math id="M96" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VMR at 300 hPa.</p></caption>
            <?xmltex \igopts{width=284.527559pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/19/2841/2019/nhess-19-2841-2019-f06.png"/>

          </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F7" specific-use="star"><?xmltex \currentcnt{7}?><label>Figure 7</label><caption><p id="d1e2446">ALICE index of 8 d <inline-formula><mml:math id="M97" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VMR at 400 hPa.</p></caption>
            <?xmltex \igopts{width=284.527559pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/19/2841/2019/nhess-19-2841-2019-f07.png"/>

          </fig>

</sec>
<sec id="Ch1.S3.SS2.SSS2">
  <label>3.2.2</label><title>Vertical concentration gradient index result</title>
      <p id="d1e2474">The vertical concentration gradient stands for the vertical rate of change.
Figures <xref ref-type="fig" rid="Ch1.F8"/> and <xref ref-type="fig" rid="Ch1.F9"/> show the value changing obviously
at the Bayan Har block and plate boundary. The highest values appeared at the Bayan Har block, the XSH, ANH and DLS faults and lasted until 12 May before the earthquake. The values were positive before 12 May. They weaken and even turn negative after 12 May, especially during 23 July to 7 August. The overall shape is still closely related to the fault and basin edge. We will discusses this later.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F8" specific-use="star"><?xmltex \currentcnt{8}?><label>Figure 8</label><caption><p id="d1e2483">Gradient of 400 to 300 hPa.</p></caption>
            <?xmltex \igopts{width=284.527559pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/19/2841/2019/nhess-19-2841-2019-f08.png"/>

          </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F9" specific-use="star"><?xmltex \currentcnt{9}?><label>Figure 9</label><caption><p id="d1e2494">Gradient of 300 to 200 hPa.</p></caption>
            <?xmltex \igopts{width=298.753937pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/19/2841/2019/nhess-19-2841-2019-f09.png"/>

          </fig>

<?xmltex \hack{\newpage}?>
</sec>
<sec id="Ch1.S3.SS2.SSS3">
  <label>3.2.3</label><title>Successive differential value</title>
      <p id="d1e2513">The trend of the reflected gas concentration over time was reflected
by the difference change, and the result of 20080317 represented the difference between 17 and 09 March. The places with rapid changes mainly occur at plate boundaries and tectonic intersections. Figure <xref ref-type="fig" rid="Ch1.F10"/> shows that the LMS fault zone began to show an abnormally high value on 25 March and then the high-value area gradually increased. On 10 April, high values appeared at the Bayan Har block, the XSH, ANH and DLS faults, and lasted until 12 May before the earthquake. The value of the entire LMS fault zone was high during 12 May. The next cycle began on 7 July, when high values first appeared in the northern section of the LMS fault zone, followed by all four LMS, XSH, ANH and DLS fault zones on 23 July. Two large aftershocks were reported on 24 July and 1 August.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F10" specific-use="star"><?xmltex \currentcnt{10}?><label>Figure 10</label><caption><p id="d1e2520">Distribution of the successive differential value at 300 hPa.</p></caption>
            <?xmltex \igopts{width=298.753937pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/19/2841/2019/nhess-19-2841-2019-f10.png"/>

          </fig>

</sec>
</sec>
</sec>
<sec id="Ch1.S4">
  <label>4</label><title>Discussion</title>
      <p id="d1e2539">Background field analysis can help us understand the gas distribution in the study area and has a certain reference role for the extraction and analysis of late abnormal changes. We have found that the <inline-formula><mml:math id="M98" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> concentration is greatly influenced by season, structure and underlying surface and presents a typical spatial and temporal distribution in southwestern China.
Comparing our work with that of the GPS velocity field, the high-value area of the background field corresponds to the area of high GPS velocity <xref ref-type="bibr" rid="bib1.bibx32" id="paren.20"/>. Long-term stress accumulation causes deep-Earth gases to be expelled along fissures or structural weaknesses <xref ref-type="bibr" rid="bib1.bibx31" id="paren.21"/>.</p>
      <p id="d1e2559">Three indices have been used to see if anomalous <inline-formula><mml:math id="M99" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> could be identified. The <inline-formula><mml:math id="M100" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> spatial variations were most likely caused by geological processes and/or the action of crustal stress in the lithosphere resulting in the Wenchuan earthquake. A large amount of <inline-formula><mml:math id="M101" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> was emitted from underground into the atmosphere along plate boundaries and tectonic belts from approximately 1.5 months before to 3 months after the earthquake, and the closer to the epicenter, the larger the amount of emitted gas. A large anomalous area occurs centered at the epicenter 8 d before the earthquake. A crucial question in this field of research refers to how we can link an individual precursor with a distinctive stage of the earthquake preparation.</p>
      <p id="d1e2595">The generation of such a seismic anomaly requires physical and chemical transformations that occur in a spatially extended preparation (activation) zone of an impending earthquake. Earthquakes, in general, exhibit complex correlations in time, space and magnitude. It is widely accepted that the observed earthquake scaling laws indicate the existence of phenomena closely associated with the proximity of the system to a critical point <xref ref-type="bibr" rid="bib1.bibx30" id="paren.22"/>. Therefore, such a requirement is satisfied during the appearance of the “critical window”, i.e., the epoch during which the short-range correlations have evolved to long-range ones in an extended area, where the “critical radius <inline-formula><mml:math id="M102" display="inline"><mml:mi>R</mml:mi></mml:math></inline-formula>” is given by the empirical relation <inline-formula><mml:math id="M103" display="inline"><mml:mrow><mml:mi>log⁡</mml:mi><mml:mi>R</mml:mi><mml:mo>≈</mml:mo><mml:mn mathvariant="normal">0.5</mml:mn><mml:mi>M</mml:mi></mml:mrow></mml:math></inline-formula> and where <inline-formula><mml:math id="M104" display="inline"><mml:mi>M</mml:mi></mml:math></inline-formula> is the earthquake magnitude <xref ref-type="bibr" rid="bib1.bibx1" id="paren.23"/>. Note that, based on the recently introduced concept of “natural time” by <xref ref-type="bibr" rid="bib1.bibx29" id="text.24"/>, it has been shown that the foreshock seismic activity that occurs in the region around the epicenter of the upcoming significant shock from a few days to 1 week before the main shock occurrence behaves as critical phenomenon.</p>
      <p id="d1e2638">Therefore, the hypothesis that the large anomaly in methane 8 d
before the earthquake occurred corresponds to the critical point window of the earthquake preparation process cannot be excluded. Accumulated experimental evidence supports the aforementioned hypothesis as follows.</p>
      <p id="d1e2642">The earthquake preparatory process has various facets that correspondingly reflect different precursors. Importantly, precursors emerge during the same period, from a few days up to one week before the main shock occurrence, while they behave as critical phenomena as well. Characteristically, such as precursors are (i) ultra-low-frequency magnetic field variations recorded by ground-based magnetic observatories before significant earthquakes (e.g.,
<xref ref-type="bibr" rid="bib1.bibx2 bib1.bibx17" id="altparen.25"/>) and (ii) megahertz-fracture-induced megahertz electromagnetic anomalies<xref ref-type="bibr" rid="bib1.bibx6" id="paren.26"/>. The generation of such a seismic anomaly also requires physical and chemical transformations which occur in a spatially extended preparation (activation) zone of an impending earthquake.</p>
      <p id="d1e2651">Characteristic precursors are the short-lived seismo-ionospheric EM precursors and EM anomalies rooted in preseismic lithosphere–atmosphere–ionosphere coupling <xref ref-type="bibr" rid="bib1.bibx20 bib1.bibx18" id="paren.27"/>. <xref ref-type="bibr" rid="bib1.bibx20" id="text.28"/> provide strong evidence for the occurrence of ionospheric precursors well before the main shock: ionospheric precursors within 5 d before the seismic shock were registered in 73 % of the cases for earthquakes with a magnitude of 5 and in 100 % of the cases for earthquakes with a magnitude of 6.</p>
      <p id="d1e2660">To further verify that the increase in <inline-formula><mml:math id="M105" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> concentration is related to earthquakes, we compared and analyzed the variation in overall methane concentration and anomaly index in the study area for non-seismic years
(Figs. <xref ref-type="fig" rid="Ch1.F11"/> and <xref ref-type="fig" rid="Ch1.F12"/>, there was no large earthquake during 2003 to 2007). Compared with 2003–2007 (Fig. <xref ref-type="fig" rid="Ch1.F11"/>),
the <inline-formula><mml:math id="M106" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> concentration increased significantly in 2008, with an average increase of <inline-formula><mml:math id="M107" display="inline"><mml:mrow><mml:mn mathvariant="normal">5.12</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">8</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>, compared with the average increase of <inline-formula><mml:math id="M108" display="inline"><mml:mrow><mml:mn mathvariant="normal">1.18</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">8</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> in the past 5 years (Fig. <xref ref-type="fig" rid="Ch1.F11"/>),
especially between 25 March and 21 June. The results from the past 5 years showed that the concentration of <inline-formula><mml:math id="M109" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> increased significantly due to seasonal influence from 21 June, showing a rapid increase in the slope of the curve (Table <xref ref-type="table" rid="Ch1.T1"/>). Although there was a certain increase in 2008, the curve slope was relatively small (Table <xref ref-type="table" rid="Ch1.T1"/>),
which may be due to the large amount of <inline-formula><mml:math id="M110" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> released by the aftershock earthquake. The increasing trend of <inline-formula><mml:math id="M111" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> concentration caused by seasonal change weakened between 25 March and 21 June 2008.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F11"><?xmltex \currentcnt{11}?><label>Figure 11</label><caption><p id="d1e2770">Comparison of the average <inline-formula><mml:math id="M112" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VMR in the study area from 2003 to 2008 (300 hPa).</p></caption>
        <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/19/2841/2019/nhess-19-2841-2019-f11.png"/>

      </fig>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T1"><?xmltex \currentcnt{1}?><label>Table 1</label><caption><p id="d1e2793">Linear fitting between 21 June and 1 September for different years.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="3">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="left"/>
     <oasis:colspec colnum="3" colname="col3" align="center"/>
     <oasis:thead>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">Year</oasis:entry>
         <oasis:entry colname="col2">Linear equation</oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M113" display="inline"><mml:mi>R</mml:mi></mml:math></inline-formula> square</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>
         <oasis:entry colname="col1">2003</oasis:entry>
         <oasis:entry colname="col2"><inline-formula><mml:math id="M114" display="inline"><mml:mrow><mml:mi>y</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.9272</mml:mn><mml:mi>x</mml:mi><mml:mo>+</mml:mo><mml:mn mathvariant="normal">174.15</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">0.9788</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">2004</oasis:entry>
         <oasis:entry colname="col2"><inline-formula><mml:math id="M115" display="inline"><mml:mrow><mml:mi>y</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.6044</mml:mn><mml:mi>x</mml:mi><mml:mo>+</mml:mo><mml:mn mathvariant="normal">176.53</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">0.9051</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">2005</oasis:entry>
         <oasis:entry colname="col2"><inline-formula><mml:math id="M116" display="inline"><mml:mrow><mml:mi>y</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.6916</mml:mn><mml:mi>x</mml:mi><mml:mo>+</mml:mo><mml:mn mathvariant="normal">175.51</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">0.9404</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">2006</oasis:entry>
         <oasis:entry colname="col2"><inline-formula><mml:math id="M117" display="inline"><mml:mrow><mml:mi>y</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.715</mml:mn><mml:mi>x</mml:mi><mml:mo>+</mml:mo><mml:mn mathvariant="normal">176.76</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">0.9847</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">2007</oasis:entry>
         <oasis:entry colname="col2"><inline-formula><mml:math id="M118" display="inline"><mml:mrow><mml:mi>y</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.7058</mml:mn><mml:mi>x</mml:mi><mml:mo>+</mml:mo><mml:mn mathvariant="normal">175.25</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">0.9484</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">2008</oasis:entry>
         <oasis:entry colname="col2"><inline-formula><mml:math id="M119" display="inline"><mml:mrow><mml:mi>y</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.4387</mml:mn><mml:mi>x</mml:mi><mml:mo>+</mml:mo><mml:mn mathvariant="normal">181.43</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">0.8066</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table></table-wrap>

      <p id="d1e3001">We also compare the ALICE result with 2008 and 2007 (Figs. <xref ref-type="fig" rid="Ch1.F12"/> and <xref ref-type="fig" rid="Ch1.F13"/>). The distribution of the ALICE index of 8 d <inline-formula><mml:math id="M120" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VMR at 300 hPa during 2007 is very different from 2008.
In 2007, the index results were similar on the whole to stable features
with no significant differences. The average value is almost always between <inline-formula><mml:math id="M121" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> to 2, except for on 7 February 2007. However, the average value for 2008 is over 2 after 10 April 2008, 1 month before the earthquake. Although gaseous anomalies can be affected by climate change, weather patterns, human activity, vegetation coverage and many other factors beyond seismic activity,
these effects may be local and can be eliminated by calculation with
Eqs (<xref ref-type="disp-formula" rid="Ch1.E1"/>) to (<xref ref-type="disp-formula" rid="Ch1.E11"/>). Therefore, the identified anomalies of <inline-formula><mml:math id="M122" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VMR can be considered earthquake-related <xref ref-type="bibr" rid="bib1.bibx3" id="paren.29"/>. <inline-formula><mml:math id="M123" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> is an important greenhouse gas in addition to carbon dioxide, and previous work shows that the obvious anomalies of thermal infrared brightness temperature appeared on 25 April and were mainly distributed in the LMS fault zone and its southern region <xref ref-type="bibr" rid="bib1.bibx39" id="paren.30"/>. These results correspond well with our work.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F12" specific-use="star"><?xmltex \currentcnt{12}?><label>Figure 12</label><caption><p id="d1e3064">ALICE index of 8 d <inline-formula><mml:math id="M124" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VMR at 300 hPa during 2007.</p></caption>
        <?xmltex \igopts{width=298.753937pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/19/2841/2019/nhess-19-2841-2019-f12.png"/>

      </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F13"><?xmltex \currentcnt{13}?><label>Figure 13</label><caption><p id="d1e3086">Comparison of the average ALICE index from 2007 and 2008.</p></caption>
        <?xmltex \igopts{width=227.622047pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/19/2841/2019/nhess-19-2841-2019-f13.png"/>

      </fig>

      <p id="d1e3095">Compared with the non-seismic years from 2003 to 2007 (no earthquake <inline-formula><mml:math id="M125" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M126" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">5.0</mml:mn></mml:mrow></mml:math></inline-formula>), the study area before and after the Wenchuan earthquake showed a significantly increased <inline-formula><mml:math id="M127" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> anomaly. It is well known that <inline-formula><mml:math id="M128" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> is in a supercritical or critical state at high temperature and pressure 10–20 km below the surface and that its physical and chemical properties are relatively stable during periods of
weak tectonic activity. However, this state is also very easy to break with active geological activity. For example, the sudden expansion of the volume of cracks or cavities caused by the change of tectonic stress field can easily change the internal fluid state and cause the supercritical fluid-phase transition <xref ref-type="bibr" rid="bib1.bibx14" id="paren.31"/>. As soon as the phase transition process begins, fluid volume and fracture expansion are triggered, resulting in a large amount of fluid spilling over the surface and spreading into the atmosphere, which is then observed by ground-based instruments or
satellites <xref ref-type="bibr" rid="bib1.bibx15 bib1.bibx9" id="paren.32"/>.</p>
      <p id="d1e3149">Before the Wenchuan earthquake, various GPS observation points and level observations showed accelerated activity of different degrees.
The LMS fault activity is characterized by a transition from tensile to compressive, and acceleration occlusion occurs near the fault field.
Accelerated uplift and extension of the crust appeared in the Bayan Har block
<xref ref-type="bibr" rid="bib1.bibx7 bib1.bibx10" id="paren.33"/>, indicating that when the main section of the LMS fault zone is still in the state of friction lock,
the relatively weak Bayan Har block shows the uplift and expansion of a large
number of tensile cracks under long-term tectonic stress. It is with this process that the underground fluid surges up and overflows the surface
on a large scale and then spreads and rises to the upper troposphere,
resulting in the high <inline-formula><mml:math id="M129" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> concentration region on the western side of the LMS in Figs. <xref ref-type="fig" rid="Ch1.F5"/>–<xref ref-type="fig" rid="Ch1.F10"/> before the earthquake.
Many NW fracture surfaces were found on the western side of the LMS after the
Wenchuan earthquake. With the occurrence of such cracks, microcracks or pre-slip, supercritical <inline-formula><mml:math id="M130" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> inside the crust can well up and overflow, resulting in increased atmospheric <inline-formula><mml:math id="M131" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> concentration.</p>
      <p id="d1e3194">Figures <xref ref-type="fig" rid="Ch1.F5"/> to <xref ref-type="fig" rid="Ch1.F10"/> show that the <inline-formula><mml:math id="M132" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> concentration in the inner area of the Sichuan Basin on the eastern side of the LMS fault zone is at a low level before and after the earthquake
and occasionally increases temporarily. The occasional short rise may be due to <inline-formula><mml:math id="M133" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> release and diffusion from the surrounding fault zone.
Although there are a large number of oil and gas deposits in the sedimentary
cover of the Sichuan Basin, the present tectonic activity is relatively weak,
and it is difficult to produce such phenomena as rupture and expansion in the upper crust, thus large-scale release of <inline-formula><mml:math id="M134" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and other fluids will not occur.</p>
      <p id="d1e3234">The migration or release of underground fluids such as <inline-formula><mml:math id="M135" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> is inevitably completed by other seismic processes in the pre-earthquake period,
which is also an important model of energy conversion and accumulation
from the deep part of the crust and mantle to the shallow part of the crust.
Therefore, it can be inferred that the phase transition process of underground fluids such as <inline-formula><mml:math id="M136" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> was mainly completed before the earthquake, so there was an abnormal increase before the earthquake. During the earthquake and coseismic activity, the abnormal increase in fluid concentration such as <inline-formula><mml:math id="M137" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> may also occur, which is mainly caused by local fluid release in the brittle layer of the upper crust <xref ref-type="bibr" rid="bib1.bibx31" id="paren.34"/>. The range is mainly limited to the vicinity of the earthquake rupture zone, which is not on the same order of magnitude as the regional <inline-formula><mml:math id="M138" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> release from the deep part. For example, the gradient shows that the values are positive before 12 May and become weak and even turn negative after 12 May  (Figs. <xref ref-type="fig" rid="Ch1.F8"/> and <xref ref-type="fig" rid="Ch1.F9"/>). The <inline-formula><mml:math id="M139" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> in the upper layer may be deep gas released before the earthquake and locally released after the earthquake decreases, so the concentration of the lower layer decreases and the gradient becomes negative.
The iteration of positive and negative values can also indicate geogenic emissions.</p>
      <p id="d1e3300">The aforementioned results seem to support the hypothesis that the observed anomaly in terms of spatiotemporal variation in methane is rooted in the stage of critical point epoch of the earthquake preparation process.</p>
</sec>
<sec id="Ch1.S5" sec-type="conclusions">
  <label>5</label><title>Conclusions</title>
      <p id="d1e3312">This study has examined the spatiotemporal variation in <inline-formula><mml:math id="M140" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> in the middle to upper troposphere during the Wenchuan earthquake (12 May 2008), using AIRS retrieval data, and discusses the mechanism of the methane anomaly. The <inline-formula><mml:math id="M141" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> concentration increased significantly in 2008, with an average increase of <inline-formula><mml:math id="M142" display="inline"><mml:mrow><mml:mn mathvariant="normal">5.12</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">8</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>, compared with <inline-formula><mml:math id="M143" display="inline"><mml:mrow><mml:mn mathvariant="normal">1.18</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">8</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> in the past 5 years. Three indices were proposed and used. The absolute local index of change of the environment (ALICE) was used for anomaly detection,
the vertical concentration gradient (gradient) was used for the study of vertical variation and the successive differential value (diff) was chosen to show time variation.
The three indices analyzed the spatial and temporal distribution of <inline-formula><mml:math id="M144" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> before and after the earthquake from horizontal scales, vertical scales and timescales. Through this work, the following conclusions are obtained.</p>
      <p id="d1e3384">The background field of <inline-formula><mml:math id="M145" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> is greatly influenced by season, structure and underlying surface and presents a typical spatial and temporal distribution of methane in southwestern China. Gas emanates from the earth's crust continuously, even without earthquakes.</p>
      <p id="d1e3398">The <inline-formula><mml:math id="M146" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> concentrations in the upper and middle atmosphere before and after the Wenchuan earthquake have a certain temporal and spatial variation. The ALICE and diff indices could be used to identify the <inline-formula><mml:math id="M147" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> concentration anomaly. The research results indicate that the <inline-formula><mml:math id="M148" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> concentration distribution before and after the earthquake breaks the distribution features of the background field. The <inline-formula><mml:math id="M149" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> concentration distribution starts from both ends and gradually gathers
around the epicenter. Moreover, a large anomalous area occurs centered at the
epicenter 8 d before the earthquake, and a trend of strengthening,
weakening and strengthening appears over time.</p>
      <p id="d1e3445">The gradient method can reflect the change in gas concentration in the vertical direction. The results show that the vertical direction obviously increases before the main earthquake, and the value is positive. The gradient value is negative during coseismic or post-seismic events. It may be that the gas before the main earthquake mainly comes from deep fluid-phase transitions, whereas the coseismic or post-seismic gas may mainly come from the locally closed fluid in the brittle layer of the crust. However, due to the lack of any technical means to accurately identify the source and content of methane in the atmosphere before the earthquake, an in-depth discussion has not been conducted, and further studies on this issue may be needed.
The gradient index can reflect the characteristics of gas emission to some extent.</p>
</sec>

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

      <p id="d1e3452">The data used to support the findings of this study are available from the
corresponding author upon request. It is also possible to download all of the original
study data from the NASA Goddard Earth Sciences Data and Information Services
Center (DISC)
(<uri>https://disc.gsfc.nasa.gov/datasets/AIRS3ST8_006/summary?keywords=%22AIRS%22</uri>, last access: 11 December 2019). Please click button under “data access” to
access the data when logging into the website. We set the date range from 9 September 2003 to
15 August 2008. The latitude and longitude range was set to 27–35<inline-formula><mml:math id="M150" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 99–109<inline-formula><mml:math id="M151" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E. The descending
<inline-formula><mml:math id="M152" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VMR of the methane variables has been chosen for study.</p>
  </notes><notes notes-type="authorcontribution"><title>Author contributions</title>

      <p id="d1e3490">JC designed this study, performed most of the data analysis and wrote the paper. XS contributed to the discussions.</p>
  </notes><notes notes-type="competinginterests"><title>Competing interests</title>

      <p id="d1e3496">The authors declare that they have no conflict of interest.</p>
  </notes><ack><title>Acknowledgements</title><p id="d1e3502">The authors would like to thank NASA for making the AIRS
dataset available. The authors wish to thank the anonymous reviewers for their
constructive comments that helped improve the scholarly quality of the paper.</p></ack><notes notes-type="financialsupport"><title>Financial support</title>

      <p id="d1e3507">This research has been supported by the National Natural Science Foundation of China (grant no. 41602223), National Key R&amp;D Program of China (grant no. 2018YFC1503505), and the Institute of Crustal Dynamics, China Earthquake Administration (grant no. ZDJ2018-18).</p>
  </notes><notes notes-type="reviewstatement"><title>Review statement</title>

      <p id="d1e3513">This paper was edited by Filippos Vallianatos and reviewed by two anonymous referees.</p>
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    <!--<article-title-html>Analysis of spatiotemporal variations in middle-tropospheric to upper-tropospheric  methane during the Wenchuan <i>M</i><sub>s</sub> = 8.0  earthquake by three indices</article-title-html>
<abstract-html><p>This research studied the spatiotemporal variation in methane in the middle to upper troposphere during the Wenchuan earthquake (12 May 2008) using AIRS retrieval data and discussed the methane anomaly mechanism.
Three indices were proposed and used for analysis. Our results show that the methane concentration increased significantly in 2008, with an average increase of 5.12×10<sup>−8</sup>, compared to the average increase of
1.18×10<sup>−8</sup> in the previous 5 years. The absolute local index of change of the environment (ALICE) and differential value (diff) indices can be used to identify methane concentration anomalies. The two indices showed that the methane concentration distribution before and after
the earthquake broke the distribution features of the background field.
As the earthquake approached, areas of high methane concentration gradually
converged towards the west side of the epicenter from both ends of
the Longmenshan fault zone. Moreover, a large anomalous area was centered at the epicenter 8&thinsp;d before the earthquake occurred, and a trend of strengthening, weakening and strengthening appeared over time.
The gradient index showed that the vertical direction obviously increased before the main earthquake and that the value was positive. The gradient value is negative during coseismic or post-seismic events. The gradient index reflects the gas emission characteristics to some extent. We also determined that the methane release was connected with the deep crust–mantle stress state, as well as micro-fracture generation and expansion. However, due to the lack of any technical means to accurately identify the source and content of methane in the atmosphere before the earthquake, an in-depth discussion has not been conducted, and further studies on this issue may be needed.</p></abstract-html>
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