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  <front>
    <journal-meta>
<journal-id journal-id-type="publisher">AMT</journal-id>
<journal-title-group>
<journal-title>Atmospheric Measurement Techniques</journal-title>
<abbrev-journal-title abbrev-type="publisher">AMT</abbrev-journal-title>
<abbrev-journal-title abbrev-type="nlm-ta">Atmos. Meas. Tech.</abbrev-journal-title>
</journal-title-group>
<issn pub-type="epub">1867-8548</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/amt-9-3567-2016</article-id><title-group><article-title>Satellite observation of atmospheric methane: intercomparison between AIRS
and GOSAT TANSO-FTS retrievals</article-title>
      </title-group><?xmltex \runningtitle{Satellite observation of atmospheric methane}?><?xmltex \runningauthor{M.~Zou et al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Zou</surname><given-names>Mingmin</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2 aff3">
          <name><surname>Xiong</surname><given-names>Xiaozhen</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff4">
          <name><surname>Saitoh</surname><given-names>Naoko</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff5">
          <name><surname>Warner</surname><given-names>Juying</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="yes" rid="aff1">
          <name><surname>Zhang</surname><given-names>Ying</given-names></name>
          <email>zhangying01@radi.ac.cn</email>
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Chen</surname><given-names>Liangfu</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3">
          <name><surname>Weng</surname><given-names>Fuzhong</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="yes" rid="aff1">
          <name><surname>Fan</surname><given-names>Meng</given-names></name>
          <email>fanmeng@radi.ac.cn</email>
        </contrib>
        <aff id="aff1"><label>1</label><institution>The State Key Laboratory of Remote Sensing Science, Institute of Remote
Sensing and Digital Earth, <?xmltex \hack{\newline}?>  Chinese Academy of Sciences, Beijing 100101,
China</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>Earth Resources Technology, Inc., Laurel, MD, USA</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>NOAA Center for Satellite Applications and Research, College Park, MD
20740, USA</institution>
        </aff>
        <aff id="aff4"><label>4</label><institution>Center for Environmental Remote Sensing, Chiba University, 1–33
Yayoi-cho, Inage-ku, Chiba, Japan</institution>
        </aff>
        <aff id="aff5"><label>5</label><institution>Department of Atmospheric and Oceanic Science, University of Maryland,
College Park, MD 20740, USA</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Meng Fan (fanmeng@radi.ac.cn)  and Ying Zhang (zhangying01@radi.ac.cn)</corresp></author-notes><pub-date><day>3</day><month>August</month><year>2016</year></pub-date>
      
      <volume>9</volume>
      <issue>8</issue>
      <fpage>3567</fpage><lpage>3576</lpage>
      <history>
        <date date-type="received"><day>10</day><month>August</month><year>2015</year></date>
           <date date-type="rev-request"><day>14</day><month>October</month><year>2015</year></date>
           <date date-type="rev-recd"><day>5</day><month>July</month><year>2016</year></date>
           <date date-type="accepted"><day>11</day><month>July</month><year>2016</year></date>
      </history>
      <permissions>
<license license-type="open-access">
<license-p>This work is licensed under a Creative Commons Attribution 3.0 Unported License. To view a copy of this license, visit <ext-link ext-link-type="uri" xlink:href="http://creativecommons.org/licenses/by/3.0/">http://creativecommons.org/licenses/by/3.0/</ext-link></license-p>
</license>
</permissions><self-uri xlink:href="https://amt.copernicus.org/articles/9/3567/2016/amt-9-3567-2016.html">This article is available from https://amt.copernicus.org/articles/9/3567/2016/amt-9-3567-2016.html</self-uri>
<self-uri xlink:href="https://amt.copernicus.org/articles/9/3567/2016/amt-9-3567-2016.pdf">The full text article is available as a PDF file from https://amt.copernicus.org/articles/9/3567/2016/amt-9-3567-2016.pdf</self-uri>


      <abstract>
    <p>Space-borne observations of atmospheric methane (CH<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> have been made
using the Atmospheric Infrared Sounder (AIRS) on the EOS/Aqua satellite since
August 2002 and the Thermal and Near-infrared Sensor for Carbon Observation
Fourier Transform Spectrometer (TANSO-FTS) on the Greenhouse Gases Observing
Satellite (GOSAT) since April 2009. This study compared the GOSAT TANSO-FTS
thermal infrared (TIR) version 1.0 CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> product with the collocated AIRS
version 6 CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> product using data from 1 August 2010 to 30 June 2012,
including the CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> mixing ratios and the total column amounts. The
results show that at 300–600 hPa, where both AIRS and GOSAT-TIR CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula>
have peak sensitivities, they agree very well, but GOSAT-TIR retrievals tend
to be higher than AIRS in layer 200–300 hPa. At 300 hPa the CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula>
mixing ratio from GOSAT-TIR is, on average, 10.3 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 31.8 ppbv higher
than that from AIRS, and at 600 hPa GOSAT-TIR retrieved CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> is
<inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>16.2 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 25.7 ppbv lower than AIRS CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula>. Comparison of the total
column amount of CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> shows that GOSAT-TIR agrees with AIRS to within
1 % in the mid-latitude regions of the Southern Hemisphere and in the
tropics. In the mid to high latitudes in the Northern Hemisphere, comparison
shows that GOSAT-TIR is <inline-formula><mml:math display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 1–2 % lower than AIRS, and in the
high-latitude regions of the Southern Hemisphere the difference of GOSAT from
AIRS varies from <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>3 % in October to <inline-formula><mml:math display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>2 % in July. The difference
between AIRS and GOSAT TANSO-FTS retrievals is mainly due to the difference
in retrieval algorithms and instruments themselves, and the larger difference
in the high-latitude regions is associated with the low information content
and small degrees of freedom of the retrieval. The degrees of freedom of
GOSAT-TIR retrievals are lower than that of AIRS, which also indicates that
the constraint in GOSAT-TIR retrievals may be too strong. From the good
correlation between AIRS and GOSAT-TIR retrievals and the seasonal variation
they observed, we are confident that the thermal infrared measurements from
AIRS and GOSAT-TIR can provide valuable information to capture the spatial
and temporal variation of CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula>, especially in the mid-upper troposphere,
in most periods and regions.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <title>Introduction</title>
      <p>As the third most important greenhouse gas after
carbon dioxide (CO<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> and water vapor, atmospheric methane (CH<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>
has a lifetime of about 12 years and is more effective in absorbing
long-wave radiation, as its radiative forcing is about 26 times more than
that of CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> on a 100-year time horizon and accounts for 32 % of the
total anthropogenic well-mixed greenhouse gas radiative forcing (IPCC,
2013). Mainly due to the impact of human activities, the concentration of
CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> in the atmosphere has increased from the pre-industrial levels of
about 700 ppb to recent levels of about 1800–1900 ppb.</p>
      <p><?xmltex \hack{\newpage}?>Ground-based networks, such as NOAA/ESRL/GMD (National Oceanic and
Atmospheric Administration, Earth System Research Laboratory, Global
Monitoring Division), provide measurements of CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> at the surface with
a long temporal record but for a limited number of stations, primarily in
the Northern Hemisphere. Aircraft measurements from NOAA/ESRL/GMD (Tans,
2009) and ARIES operated on UK FAAM aircraft (Illingworth et al., 2014), as
well as some research campaigns, provide sparse, intermittent measurements
of CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> vertical profiles. Because of a limited number of in situ
measurements in time and space domain, the quantification of CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> emissions from different sources and in different regions still remains
largely uncertain. In recent years, space-borne measurements of CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula>
from satellites have become available, such as the measurements using the
thermal infrared (TIR) sensors, which include the Atmospheric InfraRed
Sounder (AIRS) on NASA/Aqua (Aumann et al., 2003; Xiong et al., 2008, 2010a, b), the Tropospheric Emission Spectrometer (TES) on NASA/Aura (Payne et
al., 2009; Wecht et al., 2012; Worden et al., 2012), and the Infrared
Atmospheric Sounding Interferometer (IASI) on METOP-A and METOP-B (Xiong et al.,
2013; Crevoisiter et al., 2009, 2013; Razavi et al., 2009). Measurements
using the Near-Infrared (NIR) sensors include the SCanning Imaging
Absorption spectroMeter for Atmospheric CHartographY (SCIAMACHY) instrument
onboard ENVISAT for 2003–2009 (Frankenberg et al., 2008, 2011), and the
Thermal And Near infrared Sensor for carbon Observation (TANSO) onboard the
Greenhouse gases Observation SATellite (GOSAT) from 2009 to present (Yokota
et al., 2009; Paker et al., 2011; Schepers et al., 2012; Saitoh et al.,
2012). These space-borne measurements provide complementary data sources to
surface observations for monitoring atmospheric CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> with a large
spatial and temporal coverage.</p>
      <p>AIRS, GOSAT TANSO-FTS TIR and other thermal infrared sensors, including
TES and IASI, have been used to retrieve atmospheric CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula>, and these
data have been used for analyzing the spatial and temporal variation of
CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula>, so an intercomparison of these two different products from AIRS
and GOSAT will provide useful information to users to better understand the
characteristics of these two products. Validation with AIRS V6 CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> data
was recently made using <inline-formula><mml:math display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 1000 aircraft profiles (Xiong et
al., 2015), and the results show the mean biases of AIRS CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> at layers
343–441 and 441–575 hPa are <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.76 and <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.05 % and the RMSEs
are 1.56  and 1.16 %, respectively. Some correlation of the retrieval
error with degrees of freedom (DOFs) was also found, and the errors in the
spring and in the high northern latitudes are larger than in other seasons
or regions. A comparison between the GOSAT TIR methane retrievals with those
of AIRS therefore represents an indirect validation of the GOSAT data with
in situ measurements. Section 2 provides a brief introduction of these two
instruments, their retrieval algorithms and the data used in this study.
Section 3 shows the comparison results, which include the comparison of the
retrieved profiles, the information content characterized by the DOFs and
the averaging kernels from these two instruments. Both the retrieved
CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> mixing ratios and the total column amounts in different seasons and
different regions are compared. A summary and conclusion are given in
Sect. 4.</p>
</sec>
<sec id="Ch1.S2">
  <?xmltex \opttitle{CH${}_{{4}}$ retrievals from AIRS and GOSAT-TIR}?><title>CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> retrievals from AIRS and GOSAT-TIR</title>
<sec id="Ch1.S2.SS1">
  <title>AIRS instrument and the retrieval algorithm description</title>
      <p>AIRS on the EOS/Aqua satellite was launched in polar orbit (13:30 LST,
ascending node) in May 2002. It has 2378 channels covering 649–1136,
1217–1613 and 2169–2674 cm<inline-formula><mml:math 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> at high spectral resolution (<inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="italic">λ</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi mathvariant="italic">λ</mml:mi><mml:mo>=</mml:mo><mml:mn>1200</mml:mn></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 0.5 cm<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> (Aumann et
al., 2003), and the noise equivalent differential temperature (Ne<inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>T</mml:mi></mml:mrow></mml:math></inline-formula>)
at a reference temperature of 250 K ranges from 0.14 K in the 4.2 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>m
region (the lower tropospheric sounding) to 0.35 K in the 15 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>m region
(the upper tropospheric sounding). The spatial resolution of AIRS is 13.5 km
at nadir, and in a 24 h period, AIRS nominally observes the complete
globe twice per day. In order to retrieve CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> in both clear and
partially cloudy scenes, nine AIRS fields of view (FOVs) within the footprint
of the Advanced Microwave Sounding Unit (AMSU) are used to derive a single
cloud-cleared radiance spectrum in a field of regard (FOR). The
cloud-cleared FOR radiance spectrum is then used to retrieve profiles with a
spatial resolution of approximately 45 km (Aumann et al., 2003). The
atmospheric temperature profiles, water vapor profiles, surface temperatures
and surface emissivity are required as inputs to compute the radiances in
the CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> absorption band. The differences between the computed radiances
and the AIRS measured radiances for clear pixels or the derived
cloud-cleared FOR radiances for partially cloudy pixels are used to derive
CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> profiles based on optimal estimation method. A total of 50–60
CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> absorption channels near the 7.66 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>m band are selected for
the retrievals. The AIRS retrieval algorithm is a sequential retrieval
method with multiple steps, in which the temperature and water vapor
profiles are retrieved using appropriate channels in previous steps. Thus
the quality of the CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> retrievals depends on the whole AIRS science
team's efforts in improving the temperature and moisture profiles as well as
surface temperature and emissivity products. More details of AIRS CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> retrievals in its most recent version, i.e., version 6 (V6), can be found
in Xiong et al. (2015).</p>
</sec>
<sec id="Ch1.S2.SS2">
  <title>GOSAT TANSO-FTS TIR and the retrieval algorithm description</title>
      <p>GOSAT was launched into a sun-synchronous orbit on 23 January 2009 by an
H-IIA launch vehicle. GOSAT is on a 666 km orbit and has a 3-day revisit
orbit cycle and a 12-day operation cycle. The local solar time is
13:00 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 15 min. GOSAT carries two sensors: the TANSO-FTS and the
TANSO-CAI. The IFOV of the TANSO-FTS is 10.5 km in diameter, and that of the
TANSO-CAI is 0.5–1.5 km in diameter. TANSO-FTS on board GOSAT makes global
observations, including both nadir and off-nadir measurements, of
approximately 56 000 ground points every 3 days. TANSO-FTS consists of
four spectral bands: Band 1 (0.75–0.78 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>m), Band 2
(1.56–1.72 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>m), Band 3 (1.92–2.08 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>m), and Band 4
(5.5–14.3 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>m). The spectra resolution of Band 4 is 0.2 cm<inline-formula><mml:math 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>
and its signal-to-noise ratio (SNR) averages approximately 300 at Band 4 for
a blackbody temperature of 280 K. (Kuze et al., 2009, 2012; Saitoh et al.,
2009). More information on TANSO-FTS TIR and its calibration can be found in
Kuze et al. (2012). In the TIR retrieval algorithm version 1.0, all the
channels in 7.3–8.8 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>m, which include both the CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> and
N<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O absorption bands, are used for CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> retrieval. In the TANSO-FTS
TIR V1.0 CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> retrieval processing, we simultaneously retrieve H<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O,
N<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O, O<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>, and temperature other than CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula>. We also
simultaneously derive surface temperature and surface emissivity as a
correction parameter of spectral bias inherent in TANSO-FTS TIR V161.160 L1B
spectra in the same manner as CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> retrieval (Saitoh et al., 2016).The
retrieval algorithm is a non-linear maximum a posteriori method with
linear mapping (Rodgers, 2000). The a priori CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> profiles used in the
retrieval are taken from the National Institute for Environmental Studies
(NIES) transport model (Maksyutov et al., 2008; Saeki et al., 2013). Profiles
of temperature and water vapor required for the retrieval are taken from the
Japan Meteorological Agency Grid Point Values (JMA-GPV) data set. Values of
surface emissivities are estimated by a linear regression analysis using the
Advanced Spaceborne Thermal Emission Reflection Radiometer (ASTER) spectral
library (Baldridge et al., 2009), the information of land cover, sea ice,
wind speed, and the vegetation index derived from the TANSO-Cloud and Aerosol
Imager (CAI). Surface temperatures are estimated from the TANSO-FTS TIR
spectra in the window region. The signal-to-noise ratios (SNR) of TANSO-FTS
at around the 7–8 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>m band are estimated to be 70–100, and the
measurement covariance matrix used in the retrieval is based on the SNR
values. The footprint of GOSAT-TANSO is 10.5 km in diameter, and the number
of scan points of GOSAT in cross-track direction is five before July 2010 and
three thereafter.</p>
</sec>
<sec id="Ch1.S2.SS3">
  <title>Data used</title>
      <p>This study is made using the standard products of both sensors. GOSAT
TANSO-FTS TIR Level 2 CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> profile products in version 01.01 for a
2-year period from August 2010 to June 2012 are used, and the data during
this period have been released to all registered users selected under the
GOSAT research announcement. AIRS V6 CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> data are used in this study,
and they are downloaded from Goddard Earth Sciences Data and Information
Services Center (DISC) (<uri>http://mirador.gsfc.nasa.gov/cgi-bin/mirador/presentNavigation.pl?tree=project&amp;project=AIRS</uri>). Only
the data from the ascending mode of AIRS, with quality flag equal to 0 or 1,
are used for comparison with GOSAT-TIR. Note that the number of retrieval
profiles from AIRS is much denser than GOSAT-TIR, as shown in Fig. 1. In
this case, the number of profiles from GOSAT-TIR is 1479, while the number
of the AIRS profiles from ascending node with QC <inline-formula><mml:math display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 0 and 1 is 164 355. The
AIRS retrievals within 1<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> from each GOSAT-TIR measurement and in the
same day were averaged to match up with each GOSAT-TIR measurement. The
errors resulting from the time difference of about 4 h between AIRS and
GOSAT-TIR observations were not accounted for in this study given that
CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> is a long-lived and well-mixed gas. For simplification, in the
comparison of the total column CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula>, the AIRS gridded products from NASA
DISC in 1<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 1<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> were used directly, and the
GOSAT-TIR data were interpolated to the same geographical grid as AIRS.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1"><caption><p>Much larger coverage of AIRS retrievals <bold>(a)</bold> as compared to
GOSAT TANSO-FTS <bold>(b)</bold> as shown from the global CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> total column
density on 4 September 2010. AIRS data from ascending mode with QC <inline-formula><mml:math display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 0, 1
are plotted.</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://amt.copernicus.org/articles/9/3567/2016/amt-9-3567-2016-f01.jpg"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2" specific-use="star"><caption><p>Comparison of the matched-up AIRS CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> profiles versus the
GOSAT-TIR profiles using 1 day of global data on 4 September 2010. <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>N</mml:mi><mml:mo>=</mml:mo><mml:mn>1182</mml:mn></mml:mrow></mml:math></inline-formula>. Lower panel is the mean difference of AIRS minus GOSAT profiles.</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://amt.copernicus.org/articles/9/3567/2016/amt-9-3567-2016-f02.png"/>

        </fig>

      <p>Comparisons between GOSAT-TIR and AIRS CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> products include (1) CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> profile comparison, (2) comparison of CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> mixing ratios with
and without using the averaging kernels, and (3) comparison of the column-averaged CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> and the total column abundance in different latitude zones
and different times. The CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> total column abundance from AIRS ascending
mode whose unit is molecules cm<inline-formula><mml:math 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> was used. Since the unit of GOSAT-TIR
CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> profile was ppb, pressure profile <inline-formula><mml:math display="inline"><mml:mi mathvariant="bold-italic">P</mml:mi></mml:math></inline-formula>
and surface pressure <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>P</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> are used to convert the unit
of GOSAT-TIR CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> profile. First, pressure gradient is calculated as
            <disp-formula id="Ch1.E1" content-type="numbered"><mml:math display="block"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi mathvariant="bold-italic">P</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:msub><mml:mi mathvariant="bold-italic">P</mml:mi><mml:mrow><mml:mi>i</mml:mi><mml:mo>+</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi mathvariant="bold-italic">P</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
          where <inline-formula><mml:math display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula> denotes layer number; the formula to calculate Tc is
            <disp-formula id="Ch1.E2" content-type="numbered"><mml:math display="block"><mml:mrow><mml:mi mathvariant="normal">Tc</mml:mi><mml:mo>=</mml:mo><mml:mo movablelimits="false">∑</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi mathvariant="bold-italic">P</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mo>⋅</mml:mo><mml:msub><mml:mi mathvariant="bold-italic">X</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mo>/</mml:mo><mml:mfenced close=")" open="("><mml:msub><mml:mi>P</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi>P</mml:mi><mml:mi mathvariant="normal">T</mml:mi></mml:msub></mml:mfenced><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
          where <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>P</mml:mi><mml:mi mathvariant="normal">T</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the top-layer pressure. Pressure profile is included in the
GOSAT-TIR product. As a GOSAT TANSO-FTS TIR CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> profile consists of 22 layers, and AIRS-V6 CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> profile contains 100 layers in the supporting
product and 10 layers in the standard product, interpolation of AIRS
CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> profile from 100 layers to 22 layers was made using the pressure
data included in both CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> products.</p>
      <p>Later in this paper the “differences” between GOSAT-TIR and AIRS CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula>
are calculated as

                <disp-formula specific-use="align" content-type="numbered"><mml:math display="block"><mml:mtable displaystyle="true"><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>X</mml:mi><mml:mo>=</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msub><mml:mi>X</mml:mi><mml:mi mathvariant="normal">G</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi>X</mml:mi><mml:mi mathvariant="normal">A</mml:mi></mml:msub></mml:mrow></mml:mtd></mml:mtr><mml:mlabeledtr id="Ch1.E3"><mml:mtd/><mml:mtd/><mml:mtd><mml:mrow><mml:mi mathvariant="normal">Or</mml:mi><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mo>(</mml:mo><mml:msub><mml:mi>X</mml:mi><mml:mi mathvariant="normal">G</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi>X</mml:mi><mml:mi mathvariant="normal">A</mml:mi></mml:msub><mml:mo>)</mml:mo><mml:mo>/</mml:mo><mml:msub><mml:mi>X</mml:mi><mml:mi mathvariant="normal">A</mml:mi></mml:msub><mml:mo>×</mml:mo><mml:mn>100</mml:mn><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="italic">%</mml:mi><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr></mml:mtable></mml:math></disp-formula>

            where <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>X</mml:mi><mml:mi mathvariant="normal">G</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> denotes the CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> mixing ratios or column amounts from
GOSAT-TIR, and <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>X</mml:mi><mml:mi mathvariant="normal">A</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> from AIRS.</p>
</sec>
</sec>
<sec id="Ch1.S3">
  <title>Results</title>
<sec id="Ch1.S3.SS1">
  <title>Profile comparison</title>
      <p>Figure 2 shows a simple comparison of the GOSAT-TIR profiles and the
coincident AIRS CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> profiles from 1 day of global data on 4 September 2010. They are in a good agreement above 100 hPa and below 400 hPa, with
mean difference no more than 50 ppb, but at 200–300 hPa AIRS CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> spans a
large range and tends to be smaller than GOSAT TIR on average.</p>
      <p>The averaging kernels are defined to provide a characterization of the
relationship between the retrieval and the true state. The retrieval
sensitivity can be obtained from the sum of the rows of the averaging kernel
matrix, which is also referred to as “the area of the averaging kernel”
(Rodgers, 2000). To better demonstrate the differences in sensitivities between
AIRS and GOSAT-TIR retrievals, Fig. 3 shows an example of the averaging
kernels using data at a randomly selected location (38<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> S, 180<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W)
on 4 September 2010. There are 10 retrieval layers for AIRS and 22 for
GOSAT-TIR. The area of the averaging kernels, which is computed as the sum
of all individual kernels, from AIRS is larger than that from GOSAT-TIR, as
shown in Fig. 3. To demonstrate the sensitivity variations in latitudes,
Fig. 4 shows a curtain plot of the area of averaging kernels using 1 day
of global data on 4 September 2010. Overall, the patterns from AIRS are
similar to GOSAT TIR, with both peak sensitivities located in the 300–600 hPa range in the high latitudes and 200–600 hPa in the tropics. The
sensitivities below 800 hPa are small for both, which reflects the major
limitation of TIR in measuring the change of CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> in the lower
troposphere.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3" specific-use="star"><caption><p>The averaging kernels of AIRS and GOSAT TANSO-FTS TIR
V1.0 CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> retrievals on 4 September 2010. There are 10 dashed lines for
AIRS retrievals and 22 dashed lines for GOSAT retrievals, corresponding to the
retrieval layers used in each of them. The black solid line is the area of
kernels divided by 4.</p></caption>
          <?xmltex \igopts{width=369.885827pt}?><graphic xlink:href="https://amt.copernicus.org/articles/9/3567/2016/amt-9-3567-2016-f03.png"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4"><caption><p>The area of the averaging kernels of CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> retrievals
from <bold>(a)</bold> AIRS and <bold>(b)</bold> GOSAT TANSO-FTS V1.0 TIR observations at different
latitudes on 4 September 2010.</p></caption>
          <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://amt.copernicus.org/articles/9/3567/2016/amt-9-3567-2016-f04.png"/>

        </fig>

      <p>The information content, which is usually represented as the DOF, is computed as the trace of the averaging kernel matrix
(Rodgers and Connor, 2003). Figure 5 shows the variation of DOFs at different
latitudes, and on average the DOF of AIRS CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> is approximately 1.1,
whereas the mean DOF for the GOSAT-TIR retrieval of CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> is
approximately 0.61.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F5"><caption><p>Latitudinal variation of DOF for AIRS and GOSAT
TANSO-FTS V1.0 CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> retrievals on 4 September 2010.</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://amt.copernicus.org/articles/9/3567/2016/amt-9-3567-2016-f05.png"/>

        </fig>

</sec>
<sec id="Ch1.S3.SS2">
  <?xmltex \opttitle{Comparison of CH${}_{{4}}$ with and without using the
averaging kernels}?><title>Comparison of CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> with and without using the
averaging kernels</title>
      <p>Since intercomparison is made between two space-based sensors, it is
necessary to take account of the different characteristics of the observing
systems, particularly their averaging kernels, which is usually applied to
the “truth” based on the following equation (Rodgers and Connor, 2003):
            <disp-formula id="Ch1.E4" content-type="numbered"><mml:math display="block"><mml:mrow><mml:mover accent="true"><mml:mi mathvariant="bold-italic">X</mml:mi><mml:mo mathvariant="normal" stretchy="false">^</mml:mo></mml:mover><mml:mo>-</mml:mo><mml:msub><mml:mi mathvariant="bold-italic">X</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mi mathvariant="bold">A</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="bold-italic">X</mml:mi><mml:mo>-</mml:mo><mml:msub><mml:mi mathvariant="bold-italic">X</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub><mml:mo>)</mml:mo><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="bold-italic">ϵ</mml:mi><mml:mi mathvariant="bold">x</mml:mi></mml:msub><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
          where <bold>A</bold> is the averaging kernel. Here we use this equation
to calculate the difference between GOSAT-TIR and AIRS CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula>. So
<inline-formula><mml:math display="inline"><mml:mi mathvariant="bold-italic">X</mml:mi></mml:math></inline-formula> represents the true state of CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> profile;
<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">X</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the mean of comparison ensemble of CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula>
profile, and it can be calculated using a regression-based function of
latitude and longitude; <inline-formula><mml:math display="inline"><mml:mover accent="true"><mml:mi mathvariant="bold-italic">X</mml:mi><mml:mo stretchy="false" mathvariant="normal">^</mml:mo></mml:mover></mml:math></inline-formula> is the retrieved quantity related to the
true profile <inline-formula><mml:math display="inline"><mml:mi mathvariant="bold-italic">X</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">ϵ</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the error. The computed value
of <inline-formula><mml:math display="inline"><mml:mover accent="true"><mml:mi mathvariant="bold-italic">X</mml:mi><mml:mo mathvariant="normal" stretchy="false">^</mml:mo></mml:mover></mml:math></inline-formula> is referred to as the convolved data later in this paper, which
is usually compared with the retrieved CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> mixing ratio in validation
studies. Considering that the AIRS retrieval layers are coarser than those
of GOSAT-TIR, we used the AIRS averaging kernels, <bold>A</bold>, to
convert the GOSAT-TIR CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> profiles, <inline-formula><mml:math display="inline"><mml:mi mathvariant="bold-italic">X</mml:mi></mml:math></inline-formula>, and the
convolved (or smoothed) GOSAT-TIR profiles (<inline-formula><mml:math display="inline"><mml:mrow><mml:mover accent="true"><mml:mi mathvariant="bold-italic">X</mml:mi><mml:mo stretchy="false" mathvariant="normal">^</mml:mo></mml:mover><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> are then used to
derive CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> total column for comparison. This calculation is based on the
Eq. (25) from Rodgers and Connor (2003).
            <disp-formula id="Ch1.E5" content-type="numbered"><mml:math display="block"><mml:mrow><mml:mover accent="true"><mml:mrow><mml:msub><mml:mi>c</mml:mi><mml:mn>12</mml:mn></mml:msub></mml:mrow><mml:mo mathvariant="normal" stretchy="false">^</mml:mo></mml:mover><mml:mo>=</mml:mo><mml:msub><mml:mi>c</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub><mml:mo>+</mml:mo><mml:msubsup><mml:mi mathvariant="bold-italic">a</mml:mi><mml:mn mathvariant="normal">1</mml:mn><mml:mi mathvariant="bold">T</mml:mi></mml:msubsup><mml:mo>(</mml:mo><mml:mover accent="true"><mml:mi mathvariant="bold-italic">X</mml:mi><mml:mo stretchy="false" mathvariant="normal">^</mml:mo></mml:mover><mml:mo>-</mml:mo><mml:msub><mml:mi mathvariant="bold-italic">X</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub><mml:mo>)</mml:mo><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
          where <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">a</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> is the total column averaging
kernel of AIRS CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula>;  <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>c</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the total column derived from
<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">X</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>; and <inline-formula><mml:math display="inline"><mml:mover accent="true"><mml:mrow><mml:msub><mml:mi>c</mml:mi><mml:mn>12</mml:mn></mml:msub></mml:mrow><mml:mo stretchy="false" mathvariant="normal">^</mml:mo></mml:mover></mml:math></inline-formula> is the related total column
using convolved GOSAT-TIR profiles. As the AIRS averaging kernel is a 10 by
10 matrix, the GOSAT-TIR CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> profile and AIRS first-guess profile are
interpolated onto the 10 pressure layers of the AIRS retrieval grid.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F6"><caption><p>Comparison of AIRS and GOSAT-TIR CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> matched-pair
difference. The upper panel shows the statistical histogram of AIRS CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula>
difference to smoothed GOSAT-TIR CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> and the lower panel shows that to
unsmoothed GOSAT-TIR CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula>.</p></caption>
          <?xmltex \igopts{width=170.716535pt}?><graphic xlink:href="https://amt.copernicus.org/articles/9/3567/2016/amt-9-3567-2016-f06.png"/>

        </fig>

      <p>Figure 6 shows the distribution of the absolute differences between GOSAT-TIR
CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> and AIRS CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> column mixing ratios. The upper panel gives the
statistical histogram of AIRS CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> difference to smoothed GOSAT-TIR
CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula>, while the lower panel shows that to unsmoothed GOSAT-TIR
CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula>. According to Fig. 6, the number of matched pairs with
small differences increases after smoothing. A comparison of the column-averaged mixing ratio, <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>X</mml:mi><mml:mrow><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>, in Fig. 7 also shows that the correlation
coefficient between AIRS and GOSAT TANSO-FTS TIR retrievals increases from
0.88 to 0.91 after using the smoothed data, and the mean difference
decreases from <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>21.32  to <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>2.78 ppb. The mean difference and standard
deviation between AIRS and the smoothed GOSAT-TIR data are smaller than
those without smoothing using the averaging kernels, demonstrating that
applying the averaging kernels helps achieve better agreements in the
intercomparison between two different measurements, as suggested by Rogers
and Connor (2003).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F7"><caption><p>Comparison of <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>X</mml:mi><mml:mrow><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> between AIRS and <bold>(a)</bold> unsmoothed
GOSAT TANSO-FTS TIR <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>X</mml:mi><mml:mrow><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> and <bold>(b)</bold> smoothed GOSAT-TIR <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>X</mml:mi><mml:mrow><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> using
AIRS averaging kernel. Global data on 4 September 2010 are used.</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://amt.copernicus.org/articles/9/3567/2016/amt-9-3567-2016-f07.png"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F8"><caption><p>Comparisons of AIRS and GOSAT TANSO-FTS TIR smoothed
CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> at four retrieval pressure levels of 272–343 hPa, 343–441 hPa,
441–575 hPa and 575–777 hPa (the mean effective pressures are 307, 391, 506
and 671 hPa respectively) using 1 day of data on 4 September 2010.</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://amt.copernicus.org/articles/9/3567/2016/amt-9-3567-2016-f08.png"/>

        </fig>

      <p>To show the impact of using averaging kernels in the intercomparison, Fig. 8
shows the scatter plot of AIRS versus GOSAT-TIR CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> mixing ratios in
four retrieval layers of 272–343, 343–441, 441–575 and 575–777 hPa. The correlation coefficients between AIRS and the smoothed GOSAT-TIR
values are 0.70, 0.70, 0.79 and 0.87 in these four layers respectively,
while the correlation coefficients between AIRS and GOSAT-TIR without
smoothing are 0.36, 0.45, 0.57 and 0.75 respectively.</p>
      <p>In next sections, we will focus on the comparison of the total abundance
between AIRS and GOSAT-TIR retrievals without applying averaging kernel for
smoothing.</p>
</sec>
<sec id="Ch1.S3.SS3">
  <?xmltex \opttitle{Comparison of CH${}_{{4}}$ total column abundance in
different latitude zones}?><title>Comparison of CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> total column abundance in
different latitude zones</title>
      <p>As the sensitivity of TIR measurements is impacted by the surface thermal
contrast and the water vapor content in the atmosphere (Deeter et al., 2007;
Xiong et al., 2010b), the sensitivity varies with latitudes and seasons.
Below we compare the differences between AIRS and GOSAT TANSO-FTS TIR
retrieved total column abundance in six latitude zones from south to north
with an interval of 30<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>. As shown in Figs. 9 and 10, the correlations
between AIRS and GOSAT-TIR are reasonably good, and the correlation
coefficient for the least correlated case is 0.83 in zone 30–60<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> S. The split of CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> daily comparison is due to these data being located in the
high mountains between Chile and Bolivia in South America. This reflects
a larger uncertainty in the mountain or coastline regions for AIRS and/or
GOSAT. To show the change of their differences with time,
Figs. 9 and 10 also show the monthly means of the differences from August 2010 to June 2012. In the tropics their differences are less than 1 % in
all seasons, but in the mid to high latitudes in the Northern Hemisphere,
GOSAT-TIR is <inline-formula><mml:math display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 1–2 % lower than AIRS, with
the largest bias occurring in September. At high latitudes in the
Southern Hemisphere (60–90<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> S) the differences of GOSAT from AIRS show
a large variation with time, i.e., from <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>3 % in October to <inline-formula><mml:math display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>2 % in
July. This large difference in the high attitudes in the Southern Hemisphere
is related to the very low DOFs, particularly in GOSAT-TIR retrievals (see
Fig. 5), and the large uncertainties in the retrieval of atmospheric states
when there is snow/ice coverage over the ocean during October to July.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F9"><caption><p>Scatter plot of AIRS versus GOSAT TANSO-FTS TIR CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula>
total column density over three latitude zones in the Northern Hemisphere using
data from 1 August 2010 to 30 June 2012 (left panels). Right panels show the
variation of the mean difference in each month, and the bars are the
standard deviation.</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://amt.copernicus.org/articles/9/3567/2016/amt-9-3567-2016-f09.png"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F10"><caption><p>Same as Fig. 8 but for three latitude zones in the
Southern Hemisphere.</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://amt.copernicus.org/articles/9/3567/2016/amt-9-3567-2016-f10.png"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F11"><caption><p><bold>(a)</bold> Means of relative errors of GOSAT-TIR total
column CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> relative to AIRS total column CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> in every 15<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>
zonal using data from 1 August 2010 to 30 June 2012. <bold>(b)</bold> 15<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>
zonal means of AIRS CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> total column.</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://amt.copernicus.org/articles/9/3567/2016/amt-9-3567-2016-f11.png"/>

        </fig>

      <p>To better show the difference between GOSAT-TIR and AIRS in different
latitudes, we computed the mean difference over a 2-year period from
1 August 2010 to 30 June 2012 and in each 15<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> zone. As shown in Fig. 11, the
standard deviations in the Southern Hemisphere high latitudes are much
larger than in the other latitudes, and the mean differences are smaller
from 60<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> S to 10<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N but increase in the Northern Hemisphere to
<inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>1.5 % at 60<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N.</p><?xmltex \hack{\newpage}?><?xmltex \floatpos{t}?><fig id="Ch1.F12" specific-use="star"><caption><p>Trends of CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> monthly averaged total column
amounts  in different latitudes using AIRS and GOSAT-TIR products from
1 August 2010 to 30 June 2012. The left panels are the comparison in the
Northern Hemisphere and the right panels are the comparison in the Southern
Hemisphere.</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://amt.copernicus.org/articles/9/3567/2016/amt-9-3567-2016-f12.png"/>

        </fig>

</sec>
<sec id="Ch1.S3.SS4">
  <title>Comparison of seasonal cycles from AIRS and GOSAT</title>
      <p>Using the monthly averaged total column density of CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> from AIRS and
GOSAT products, we compared the seasonal cycles of CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> from 1 August 2010
to 30 June 2012. The left panels in Fig. 12 are the comparisons in the
Northern Hemisphere, and the right panels are the comparisons in the Southern
Hemisphere. Again, GOSAT-TIR agrees with AIRS to within 1 % in the
mid-latitude regions of the Southern Hemisphere and in the tropics. However,
the seasonal variation in the tropics from AIRS observations is larger than
that from GOSAT. In the mid to high latitudes in the Northern Hemisphere,
GOSAT-TIR is <inline-formula><mml:math display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 1–2 % lower than AIRS, but the seasonal
variations agree well. In the high-latitude regions in the Southern
Hemisphere, the seasonal variation of the total column of CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> is large,
which is due to a lot of data points with very low total column of CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> observed during October–January from both AIRS and GOSAT-TIR. However,
AIRS and GOSAT agree well in capturing the variation even though their
difference is relatively larger than in other regions (see Fig. 10).</p>
</sec>
</sec>
<sec id="Ch1.S4" sec-type="conclusions">
  <title>Summary and conclusions</title>
      <p>A thorough comparison of AIRS V6 and GOSAT TANSO-FTS TIR V1.0 CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula>
products using 2 years of data (1 August 2010 to 30 June 2012) has been
made. In this comparison, AIRS measurements within a collocation window of
1<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> by 1<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> from each GOSAT-TIR measurement in the same day were
used. Both the CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> mixing ratios and total column amounts have been
compared. To understand the differences in the retrievals from these two
different instruments, we also compared the differences in the averaging
kernels and the DOFs and examined the use of averaging kernels on the
comparison results.</p>
      <p>The peak sensitive layers of AIRS and GOSAT-TIR are at similar height, which
is at 200–600 hPa in the tropics and 300–600 hPa in the high-latitude
regions. However, due to the lower SNR of GOSAT TANSO-FTS spectra in the 7–8 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>m CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> band, or over-constraint in the GOSAT retrieval algorithm,
the DOF of GOSAT-TIR V1.0 retrievals is lower than AIRS.</p>
      <p><?xmltex \hack{\newpage}?>The comparisons of the profiles showed that the AIRS CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> is similar to
GOSAT-TIR CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula>, except that the AIRS values tend to be lower than
GOSAT-TIR at 200–300 hPa. At 300 hPa, the CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> mixing ratios from GOSAT
are 10.3 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 31.8 ppbv higher than AIRS, and at 600 hPa, the GOSAT-TIR
CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> is <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>16.2 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 25.7 ppb lower than AIRS. Between 300 and 600 hPa, where they have peak sensitivities, AIRS and
GOSAT-TIR agree very well. As expected, applying the averaging kernels to
smooth the GOSAT-TIR retrievals results in a better agreement between GOSAT with
AIRS products.</p>
      <p>The comparison of the total column amounts of CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> shows that the
correlation coefficients between AIRS and GOSAT TANSO-FTS TIR are more than
0.8 in all cases, and the GOSAT-TIR CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> agrees with AIRS to within
1 % in the mid-latitudes of the Southern Hemisphere and tropics, but in
the mid to high latitudes of the Northern Hemisphere, GOSAT-TIR is
<inline-formula><mml:math display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 1–2 % lower than AIRS depending on different seasons. In
the high latitudes of the Southern Hemisphere the bias varies from <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>3 % in
October to <inline-formula><mml:math display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>2 % in July. This large difference in high-latitude regions
is associated with the low information content (or DOFs) and larger
uncertainties in the retrievals of both AIRS (Xiong et al., 2015) and GOSAT.
Thus a much stricter quality control should be used as suggested by Xiong et
al. (2015). We also found AIRS and GOSAT-TIR have a good agreement in
capturing the monthly variation of CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> density.</p>
      <p>In this study, the time difference between AIRS and GOSAT-TIR measurements
has not been taken into account. So, the differences, if they could have
been measured at the same time, could be slightly smaller than what we
presented here. These results demonstrate that the thermal infrared sensors
such as AIRS and GOSAT TANSO-FTS TIR can provide valuable consistent
information of CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> in the mid-upper troposphere. Further comparisons
using more recent data as well as direct comparison with aircraft
measurements are ongoing.</p>
</sec>
<sec id="Ch1.S5">
  <title>Data availability</title>
      <p>The data set of AIRS V6
CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> product used in this study is available at Goddard Earth Sciences Data
and Information Services Center (DISC)
(<uri>http://mirador.gsfc.nasa.gov/cgi-bin/mirador/presentNavigation.pl?tree=project&amp;project=AIRS</uri>). And the GOSAT TANSO-FTS TIR Level 2 CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> product can be freely
download at GOSAT user interface gateway (GUIG)
(<uri>https://data.gosat.nies.go.jp/GosatUserInterfaceGateway/guig/GuigPage/open.do</uri>).</p>
</sec>

      
      </body>
    <back><ack><title>Acknowledgements</title><p>This work was supported by the Key Program of the National Natural Science
Foundation of China (no. 41130528), National Natural Science Foundation of China
(nos. 41401387 and 41201353). This study was performed within the framework of the
GOSAT Research Announcement.<?xmltex \hack{\newline}?><?xmltex \hack{\newline}?>
Edited by: J. Worden<?xmltex \hack{\newline}?>
Reviewed by:  three anonymous referees</p></ack><ref-list>
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    </app></app-group></back>
    <!--<article-title-html>Satellite observation of atmospheric methane: intercomparison between AIRS
and GOSAT TANSO-FTS retrievals</article-title-html>
<abstract-html><p class="p">Space-borne observations of atmospheric methane (CH<sub>4</sub>) have been made
using the Atmospheric Infrared Sounder (AIRS) on the EOS/Aqua satellite since
August 2002 and the Thermal and Near-infrared Sensor for Carbon Observation
Fourier Transform Spectrometer (TANSO-FTS) on the Greenhouse Gases Observing
Satellite (GOSAT) since April 2009. This study compared the GOSAT TANSO-FTS
thermal infrared (TIR) version 1.0 CH<sub>4</sub> product with the collocated AIRS
version 6 CH<sub>4</sub> product using data from 1 August 2010 to 30 June 2012,
including the CH<sub>4</sub> mixing ratios and the total column amounts. The
results show that at 300–600 hPa, where both AIRS and GOSAT-TIR CH<sub>4</sub>
have peak sensitivities, they agree very well, but GOSAT-TIR retrievals tend
to be higher than AIRS in layer 200–300 hPa. At 300 hPa the CH<sub>4</sub>
mixing ratio from GOSAT-TIR is, on average, 10.3 ± 31.8 ppbv higher
than that from AIRS, and at 600 hPa GOSAT-TIR retrieved CH<sub>4</sub> is
−16.2 ± 25.7 ppbv lower than AIRS CH<sub>4</sub>. Comparison of the total
column amount of CH<sub>4</sub> shows that GOSAT-TIR agrees with AIRS to within
1 % in the mid-latitude regions of the Southern Hemisphere and in the
tropics. In the mid to high latitudes in the Northern Hemisphere, comparison
shows that GOSAT-TIR is  ∼  1–2 % lower than AIRS, and in the
high-latitude regions of the Southern Hemisphere the difference of GOSAT from
AIRS varies from −3 % in October to +2 % in July. The difference
between AIRS and GOSAT TANSO-FTS retrievals is mainly due to the difference
in retrieval algorithms and instruments themselves, and the larger difference
in the high-latitude regions is associated with the low information content
and small degrees of freedom of the retrieval. The degrees of freedom of
GOSAT-TIR retrievals are lower than that of AIRS, which also indicates that
the constraint in GOSAT-TIR retrievals may be too strong. From the good
correlation between AIRS and GOSAT-TIR retrievals and the seasonal variation
they observed, we are confident that the thermal infrared measurements from
AIRS and GOSAT-TIR can provide valuable information to capture the spatial
and temporal variation of CH<sub>4</sub>, especially in the mid-upper troposphere,
in most periods and regions.</p></abstract-html>
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