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  <front>
    <journal-meta><journal-id journal-id-type="publisher">ACP</journal-id><journal-title-group>
    <journal-title>Atmospheric Chemistry and Physics</journal-title>
    <abbrev-journal-title abbrev-type="publisher">ACP</abbrev-journal-title><abbrev-journal-title abbrev-type="nlm-ta">Atmos. Chem. Phys.</abbrev-journal-title>
  </journal-title-group><issn pub-type="epub">1680-7324</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/acp-21-13553-2021</article-id><title-group><article-title>Water vapor anomaly over the tropical western Pacific in El Niño winters from radiosonde and satellite observations and<?xmltex \hack{\break}?> ERA5 reanalysis data</article-title><alt-title>Water vapor anomaly over the tropical western Pacific in El Niño winters</alt-title>
      </title-group><?xmltex \runningtitle{Water vapor anomaly over the tropical western Pacific in El Ni\~{n}o winters}?><?xmltex \runningauthor{M. Du et al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff2 aff3">
          <name><surname>Du</surname><given-names>Minkang</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="yes" rid="aff1 aff2 aff3">
          <name><surname>Huang</surname><given-names>Kaiming</given-names></name>
          <email>hkm@whu.edu.cn</email>
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff2">
          <name><surname>Zhang</surname><given-names>Shaodong</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff2">
          <name><surname>Huang</surname><given-names>Chunming</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff2">
          <name><surname>Gong</surname><given-names>Yun</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-1206-2087</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff2 aff3">
          <name><surname>Yi</surname><given-names>Fan</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-8368-5081</ext-link></contrib>
        <aff id="aff1"><label>1</label><institution>School of Electronic Information, Wuhan University, Wuhan, China</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>Key Laboratory of Geospace Environment and Geodesy, Ministry of
Education, Wuhan, China</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>State Observatory for Atmospheric Remote Sensing, Wuhan, China</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Kaiming Huang (hkm@whu.edu.cn)</corresp></author-notes><pub-date><day>10</day><month>September</month><year>2021</year></pub-date>
      
      <volume>21</volume>
      <issue>17</issue>
      <fpage>13553</fpage><lpage>13569</lpage>
      <history>
        <date date-type="received"><day>23</day><month>April</month><year>2021</year></date>
           <date date-type="rev-request"><day>29</day><month>April</month><year>2021</year></date>
           <date date-type="rev-recd"><day>1</day><month>August</month><year>2021</year></date>
           <date date-type="accepted"><day>10</day><month>August</month><year>2021</year></date>
      </history>
      <permissions>
        <copyright-statement>Copyright: © 2021 </copyright-statement>
        <copyright-year>2021</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://acp.copernicus.org/articles/.html">This article is available from https://acp.copernicus.org/articles/.html</self-uri><self-uri xlink:href="https://acp.copernicus.org/articles/.pdf">The full text article is available as a PDF file from https://acp.copernicus.org/articles/.pdf</self-uri>
      <abstract><title>Abstract</title>
    <p id="d1e142">Using radiosonde observations at five stations in the tropical
western Pacific and reanalysis data for the 15 years from 2005 to 2019, we
report an extremely negative anomaly in atmospheric water vapor during the
super El Niño winter of 2015/16 and compare the anomaly with that in
the other three El Niño winters of the period. A strong specific humidity anomaly is
concentrated below 8 km of the troposphere with a peak at 2.5–3.5 km, and a
column-integrated water vapor mass anomaly over the five radiosonde sites
has a large negative correlation coefficient of <inline-formula><mml:math id="M1" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.63 with the oceanic
Niño3.4 index but with a lag of about 2–3 months. In general, the
tropical circulation anomaly in the El Niño winter is characterized by
divergence (convergence) in the lower troposphere over the tropical western
(eastern) Pacific; thus, the water vapor decreases over the tropical western
Pacific as upward motion is suppressed. The variability of the Hadley
circulation is quite small and has little influence on the observed water
vapor anomaly. The anomaly of the Walker circulation makes a considerable
contribution to the total anomaly in all four El Niño winters,
especially in the 2006/07 and 2015/16 eastern Pacific (EP) El Niño
events. The monsoon circulation shows a remarkable change from one event to
another, and its anomaly is large in the 2009/10 and 2018/19 central Pacific
(CP) El Niño winters and small in the two EP El Niño winters. The
observed water vapor anomaly is caused mainly by the Walker circulation
anomaly in the super EP event of 2015/16 but is caused by the monsoon circulation
anomaly in the strong CP event of 2009/10. The roles of the Hadley, Walker,
and monsoon circulations in the EP and CP events are confirmed by the
composite EP and CP El Niños based on the reanalysis data for 41 years.
Owing to the anomalous decrease in upward transport of water vapor during
the El Niño winter, lower cloud amounts and more outgoing longwave
radiation over the five stations are clearly presented in satellite
observation. In addition, a detailed comparison of water vapor in the
reanalysis, radiosonde, and satellite data shows a fine confidence level for
the datasets; nevertheless, the reanalysis seems to slightly underestimate
the water vapor over the five stations in the 2009/10 winter.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <label>1</label><title>Introduction</title>
      <p id="d1e161">As a dominant greenhouse gas in the atmosphere, water vapor has a profound
impact on global energy budgets through not only latent heat release upon
phase transitions  (Held and Soden, 2000) but also cloud
formation that reflects longwave radiation from below and shortwave
radiation from above (Stevens et al., 2017); thus, water vapor plays a
substantial role in the formation and evolution of the climate system. The
tropical Pacific is a major convection center and a region with abundant
water vapor. Sea surface temperature (SST) anomalies in the tropical Pacific
have an important influence on water vapor transport, cloud cover, and
precipitation distribution due to the tropical circulation changes caused by
El Niño–Southern Oscillation (ENSO). ENSO is characterized by anomalous
SST in the tropical Pacific. During ENSO, there is significant<?pagebreak page13554?> precipitation
variability in the Euro-Mediterranean (López-Parages and
Rodríguez-Fonseca, 2012), Middle East (Sandeep and Ajayamohan, 2018),
southwest central Asia (Mariotti, 2007), western Africa (Okazaki et al.,
2015), Pacific Ocean (Quartly et al., 2000), and continental USA (Lee et al.,
2014). ENSO has an effect on seasonal rainfall in East Asia by inducing a
weaker and later onset of the Indian monsoon circulation (Dai and Wigley,
2000; Zhao et al., 2010; Yan et al., 2018). Vertical cloud anomalies in the
tropical Atlantic from Aqua Moderate-Resolution Imaging Spectroradiometer
are linked to ENSO-induced shift and weakening of the Walker circulation and
Hadley cell near the Equator (Madenach et al., 2019). The strong 1997/98 El
Niño resulted in cloud structure anomalies and their radiative property
changes over the tropical Pacific (Sun et al., 2012) and increased upper
tropospheric cirrus over the mid-Pacific but decreased cirrus over Indonesia
(Massie et al., 2000). Numerical investigation also indicated that warm-water volume transport and precipitation change are associated with ENSO
(Ishida et al., 2008; Hill et al., 2009).</p>
      <p id="d1e164">El Niño is generally classified into central Pacific (CP) El Niño,
also known as El Niño Modoki, and eastern Pacific (EP) El Niño based
on distinct spatial distributions of warming SST anomaly averaged over the
Niño4 and Niño3 regions (Ashok et al., 2007; Yu and Kao, 2009; Yeh
et al., 2009), respectively. The 2006/07 and 2015/16 events are the EP El
Niño because of the stronger SST anomaly during the boreal winter
(December to February, as DJF) in the Niño3 region than in the Niño4
region, while correspondingly the 2009/10 and 2018/19 events are
categorized as the CP El Niño (Yeh et al., 2009). The two types of El
Niño have different effects on precipitation, surface temperature,
moisture transport, and carbon cycle over many parts of the world (Weng et
al., 2008; Kug et al., 2009; Wang et al., 2013; Yeh et al., 2014; Gu and
Adler, 2016; Wang et al., 2018). Su and Jiang (2013) and Takahashi et al. (2013) suggested that the water vapor anomaly over the tropical ocean was mainly
controlled by thermodynamic process during the 2006/07 EP El Niño but
by both dynamic and thermodynamic processes during the 2009/10 CP El
Niño.</p>
      <p id="d1e167">The EP El Niño in 2015/16 winter is one of the strongest ENSO events on
record. Compared to the strong 1982/83 and 1997/98 El Niños, the 2015/16
El Niño shows distinct aspects that indicate that the largest SST anomalies are
extended toward the central Pacific (Paek  et al., 2017; L'Heureux et al.,
2017). Due to their unusual characteristics, the global effects of the 2015/16
event have attracted much attention. Palmeiro et al. (2017) proposed that an
early stratospheric final warming over the polar region and anomalous
precipitation over southern Europe in 2016 were related to the 2015/16 super
El Niño. Li et al. (2018) revealed that the combined effect of the 2015
ENSO warm phase and Madden-Julian Oscillation (MJO)-4 index negative phase
caused a significant deficit of precipitation on the Canadian Prairies in
May and June 2015. A striking freshwater anomaly was observed in the
equatorial Pacific during the onset of the 2015/16 event (Gasparin and Roemmich,
2016), and rainfall <inline-formula><mml:math id="M2" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O in southern Papua was generally
enriched by 1.6 ‰–2 ‰ during the
2015 El Niño more than during the 2013/14 ENSO-normal period (Permana et al.,
2016). Owing to convection anomaly during the 2015/16 El Niño, water
vapor in the tropical lower stratosphere was increased by hydration of the
lower stratosphere through convectively detrained cloud ice (Avery et al.,
2017), and quasi-biennial oscillation in the tropical stratospheric wind was
disrupted because of dramatic relocation of deep convection (Dunkerton,
2016; Newman et al., 2016). Hence, the 2015/16 El Niño had important
influences on the circulation and composition transport and the mass
exchange between the troposphere and stratosphere. In this paper, we
investigate the water vapor anomaly over the tropical western Pacific in the CP
and EP El Niño events from radiosonde and satellite observations, particularly the extreme anomaly in the 2015/16 super El Niño winter, and
explore the contributions of the tropical Hadley, Walker, and monsoon
circulation changes to the observed water vapor anomalies in the different
El Niño events.</p>
      <p id="d1e181">The data used are briefly described in Sect. 2. In Sect. 3, water vapor
anomalies in four El Niño winters are presented, and the relationship
between the ENSO intensity and the water vapor anomaly at the observational
stations is explored. In Sect. 4, we decompose the tropical circulation
into the Hadley, Walker, and monsoon circulation components and estimate the
roles of these circulations in the water vapor variation. Tropical cloud and
outgoing longwave radiation (OLR) are investigated in Sect. 5. A
discussion of the water vapor data quality is provided in Sect. 6.
Finally, we summarize the results in Sect. 7.</p>
</sec>
<sec id="Ch1.S2">
  <label>2</label><title>Data</title>
      <p id="d1e192">In present study, we investigate the atmospheric water vapor by using
radiosonde observations at five tropical stations for 15 years from January
2005 to December 2019, which are provided by the National Oceanic And
Atmosphere Administration (NOAA) at the following website: <uri>https://www.ncei.noaa.gov/pub/data/igra/derived/</uri> (last access: 6 September 2021). The five radiosonde
stations are at Koror (7.33<inline-formula><mml:math id="M3" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 134.48<inline-formula><mml:math id="M4" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E), Yap
(9.48<inline-formula><mml:math id="M5" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 138.08<inline-formula><mml:math id="M6" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E), Guam (13.55<inline-formula><mml:math id="M7" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N,
144.83<inline-formula><mml:math id="M8" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E), Truk (7.47<inline-formula><mml:math id="M9" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 151.85<inline-formula><mml:math id="M10" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E), and
Ponape (6.97<inline-formula><mml:math id="M11" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 158.22<inline-formula><mml:math id="M12" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E), located in the western
Pacific warm pool. A balloon was launched twice daily at 00:00 and 12:00 UTC,
and during balloon ascent the sensing payload on the balloon can obtain many
meteorological parameters, such as atmospheric pressure, temperature,
relative humidity, and wind speed and direction. We plot daily temperature,
relative humidity, and wind speed time series observed by radiosonde to
identify potential outliers, and then the high resistant asymmetric biweight
technique is applied to weed out the outliers (Lanzante, 1996). The outlier
data are very few,<?pagebreak page13555?> and the outliers of temperature, wind, and relative
humidity account for only 0.09 %, 0.08 %, and 0.02 % of all
observational data at the five stations over 15 years, respectively. The
radiosonde data are linearly interpolated to a vertical grid of 50 m, and the
interpolated data below 10 km are utilized to analyze the atmospheric water
vapor variation. The burst height of the balloon is usually more than 30 km; thus,
the data availability below 10 km is high. In the period that we focus on,
the data are missing for about 4, 2, 1, and 4 months over Yap, Guam, Truk, and
Ponape, respectively, and they are almost entirely missing from the several
continuous observational data rather than the balloon burst data below 10 km.</p>
      <p id="d1e289">Specific humidity can be derived from the profile of meteorological
parameters observed by radiosonde. The saturated vapor pressure <inline-formula><mml:math id="M13" display="inline"><mml:mrow><mml:msub><mml:mi>e</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is
calculated according to a modified version of the Magnus formula as follows
(Murray, 1967):
          <disp-formula id="Ch1.E1" content-type="numbered"><label>1</label><mml:math id="M14" display="block"><mml:mrow><mml:msub><mml:mi>e</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">6.1078</mml:mn><mml:mo>×</mml:mo><mml:mi>exp⁡</mml:mi><mml:mfenced close="]" open="["><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mn mathvariant="normal">17.269</mml:mn><mml:mfenced open="(" close=")"><mml:mrow><mml:mi>T</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">273.16</mml:mn></mml:mrow></mml:mfenced></mml:mrow><mml:mrow><mml:mi>T</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">35.86</mml:mn></mml:mrow></mml:mfrac></mml:mstyle></mml:mfenced><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
        where <inline-formula><mml:math id="M15" display="inline"><mml:mi>T</mml:mi></mml:math></inline-formula> is the temperature in units of K. Following this, the specific humidity
<inline-formula><mml:math id="M16" display="inline"><mml:mi>q</mml:mi></mml:math></inline-formula> (g kg<inline-formula><mml:math id="M17" 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>) is determined from the following equations:

              <disp-formula specific-use="gather" content-type="numbered"><mml:math id="M18" display="block"><mml:mtable displaystyle="true"><mml:mlabeledtr id="Ch1.E2"><mml:mtd><mml:mtext>2</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:mi>e</mml:mi><mml:mo>=</mml:mo><mml:mi mathvariant="normal">RH</mml:mi><mml:mo>×</mml:mo><mml:msub><mml:mi>e</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E3"><mml:mtd><mml:mtext>3</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:mi>q</mml:mi><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mn mathvariant="normal">0.622</mml:mn><mml:mi>e</mml:mi></mml:mrow><mml:mrow><mml:mi>p</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">0.378</mml:mn><mml:mi>e</mml:mi></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr></mml:mtable></mml:math></disp-formula>

          where <inline-formula><mml:math id="M19" display="inline"><mml:mi>e</mml:mi></mml:math></inline-formula> is the vapor pressure, RH is the relative humidity, and <inline-formula><mml:math id="M20" display="inline"><mml:mi>p</mml:mi></mml:math></inline-formula> is
the pressure in units of hPa.</p>
      <p id="d1e443">In addition, we use the monthly specific humidity and horizontal winds from
the surface to 300 hPa during the period of 2005–2019, obtained from the
European Centre for Medium-Range Weather Forecasts (ECMWF) ERA5 reanalysis
data, to investigate the water vapor anomaly and tropical atmospheric
circulation in the region of the radiosonde stations. The reanalysis data are
produced by a sequential 4D variational data assimilation scheme, with a
latitudinal and longitudinal resolution of 0.25<inline-formula><mml:math id="M21" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M22" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.25<inline-formula><mml:math id="M23" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> at 37 pressure levels from 1000 to 1 hPa (Hersbach et al.,
2020). The data are available at the website of <uri>https://cds.climate.copernicus.eu/cdsapp#!/dataset/reanalysis-era5-pressure-levels-monthly-means?tab=form</uri> (last access: 6 September 2021).</p>
      <p id="d1e474">To assess the atmospheric water vapor as compared to the reanalysis data and
the radiosonde observations, a further evaluation is carried out using Aqua
atmospheric infrared sounder (AIRS) water vapor mass mixing ratio data from
2005–2019. AIRS is a hyperspectral infrared spectrometer orbiting on the
National Aeronautics and Space Administration (NASA) Aqua spacecraft
launched in May 2002, which can provide accurate measurements of
temperature, moisture, and other atmospheric variables (Aumann et al.,
2003). The data used here are water vapor vertical profiles from Level 3
monthly standard gridded retrieval product version 6, AIRS3STM (Susskind et
al., 2014), which are available at <uri>https://disc.gsfc.nasa.gov/datasets/AIRS3STM_006/summary?keywords=AIRS3STM</uri> (last access: 6 September 2021). The water
vapor data contain eight levels from 1000 and 300 hPa with a latitudinal and
longitudinal grid of 1<inline-formula><mml:math id="M24" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M25" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 1<inline-formula><mml:math id="M26" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> derived from the
average of two observations in two orbital overpasses per day. The
ascending and descending orbits have an equatorial crossing time at 13:30 local
time (LT) and 01:30 LT, respectively.</p>
      <p id="d1e506">The oceanic Niño index (ONI) is applied to discuss the correlation between
the ENSO and the observed water vapor anomaly. ONI is the measurement of
ENSO strength, which is provided by the NOAA at <uri>https://catalog.data.gov/dataset/climate-prediction-center-cpcoceanic-nino-index</uri> (last access: 6 September 2021).
The ONI is defined as a 3-month moving average of extended reconstructed sea
surface temperature (ERSST) V5 sea surface temperature anomalies in the
Niño3.4 region at 5<inline-formula><mml:math id="M27" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N–5<inline-formula><mml:math id="M28" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> S and 120–170<inline-formula><mml:math id="M29" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W (Huang et al., 2017).</p>
      <p id="d1e539">Cloud occurrence probability and OLR flux are also examined since they are
sensitive to water vapor variation (Stevens et al., 2017; Soden et al.
2008). The OLR data are measured by the NOAA-18 satellite, which travel in
sun-synchronous orbit with a 13:55 LT equatorial crossing time (Kramer,
2002). We use the monthly OLR data between 2005 and 2019 from the NOAA
archives with a latitudinal and longitudinal grid of 2.5<inline-formula><mml:math id="M30" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M31" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 2.5<inline-formula><mml:math id="M32" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> (Liebmann and Smith, 1996), which can be accessed through
the website of <uri>https://psl.noaa.gov/data/gridded/data.interp_OLR.html</uri> (last access: 6 September 2021). The Cloud Aerosol Lidar and Infrared Pathfinder Satellite
Observation (CALIPSO) satellite is able to clearly identify cloud vertical structure
(Winker et al., 2007). The satellite has a sun-synchronous orbit
with an equatorial crossing time around 01:30 and 13:30 LT (Stephens et al.,
2002). Here, we use the CALIPSO version 1.00 lidar level 3 cloud occurrence
monthly data in a latitudinal and longitudinal grid of 2<inline-formula><mml:math id="M33" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M34" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 2.5<inline-formula><mml:math id="M35" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> with an altitude resolution of 60 m above the mean sea
level, and the available data are from June 2006 to December 2016, downloaded
from the website of the NASA at <uri>https://asdc.larc.nasa.gov/project/CALIPSO/CAL_LID_L3_Cloud_Occurrence-Standard-V1-00_V1-00</uri> (last access: 6 September 2021)</p>
</sec>
<sec id="Ch1.S3">
  <label>3</label><title>Water vapor anomaly</title>
<sec id="Ch1.S3.SS1">
  <label>3.1</label><?xmltex \opttitle{Water vapor anomaly during El Ni\~{n}o winter}?><title>Water vapor anomaly during El Niño winter</title>
      <p id="d1e615">We derive the profile of specific humidity from the radiosonde observations
according to Eqs. (1)–(3) and then calculate the monthly mean specific
humidity. The monthly mean specific humidities in all the same months are
further averaged to obtain the monthly climatic normal; thus, the monthly
mean water vapor anomaly is determined from the monthly mean series by
subtracting the corresponding month climatic normal. Figure 1 shows the
monthly mean specific<?pagebreak page13556?> humidity anomaly based on the radiosonde observations
at Koror, Yap, Guam, Truk, and Ponape from January 2005 to December 2019.
Atmospheric water vapor is mainly concentrated below 8 km, and thus the large
water vapor anomaly also occurs below 8 km. It can be seen from Fig. 1 that
the observed water vapor anomaly is remarkably negative over the five
stations in the super El Niño winter of 2015–2016. The negative anomaly
in the water vapor reaches a peak value of <inline-formula><mml:math id="M36" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2.06</mml:mn></mml:mrow></mml:math></inline-formula> g kg<inline-formula><mml:math id="M37" 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> around 3 km
in January at Koror, <inline-formula><mml:math id="M38" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3.2</mml:mn></mml:mrow></mml:math></inline-formula> g kg<inline-formula><mml:math id="M39" 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> around 3 km in February at Yap, <inline-formula><mml:math id="M40" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>2.39 g kg<inline-formula><mml:math id="M41" 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> around 2.5 km in January at Guam, <inline-formula><mml:math id="M42" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2.29</mml:mn></mml:mrow></mml:math></inline-formula> g kg<inline-formula><mml:math id="M43" 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> around 3.5 km in February at Truk, and <inline-formula><mml:math id="M44" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2.66</mml:mn></mml:mrow></mml:math></inline-formula> g kg<inline-formula><mml:math id="M45" 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> around 2.5 km in February at
Ponape. In the 2006/07, 2009/10, and 2018/19 El Niño
winters, the observed water vapor also exhibits the negative anomalies in
the lower and middle troposphere. We derive the monthly mean specific
humidity anomaly from the reanalysis data at the radiosonde stations during
the same period, which is also presented in Fig. 1. The ERA5 reanalysis
shows a water vapor anomaly scenario similar to the radiosonde observation.
The negative anomalies in the four El Niño winters are obvious in the
reanalysis data, especially the strong anomaly in the 2015/16 event. Hence,
the El Niño events can lead to the obvious reduction of water vapor in
the region.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1" specific-use="star"><?xmltex \currentcnt{1}?><?xmltex \def\figurename{Figure}?><label>Figure 1</label><caption><p id="d1e728">Specific humidity anomaly between January 2005 and December 2019
derived from (left) radiosonde observations and (right) ERA5 reanalysis data
at <bold>(a, f)</bold> Koror, <bold>(b, g)</bold> Yap, <bold>(c, h)</bold> Guam, <bold>(d, i) </bold> Truk, and <bold>(e, j)</bold> Ponape.</p></caption>
          <?xmltex \igopts{width=398.338583pt}?><graphic xlink:href="https://acp.copernicus.org/articles/21/13553/2021/acp-21-13553-2021-f01.png"/>

        </fig>

      <p id="d1e752">With the help of the ERA5 reanalysis data, we investigate the distribution
of the abnormal water vapor during the four El Niño events. Here, we
introduce an important scalar of column-integrated water vapor mass (CWV),
also called precipitable water, which is expressed as (Viswanadham,
1981),
            <disp-formula id="Ch1.E4" content-type="numbered"><label>4</label><mml:math id="M46" display="block"><mml:mrow><mml:mi>Q</mml:mi><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mn mathvariant="normal">1</mml:mn><mml:mi>g</mml:mi></mml:mfrac></mml:mstyle><mml:msubsup><mml:mo>∫</mml:mo><mml:mrow><mml:msub><mml:mi>P</mml:mi><mml:mi>z</mml:mi></mml:msub></mml:mrow><mml:mrow><mml:msub><mml:mi>P</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:msubsup><mml:mi>q</mml:mi><mml:mi mathvariant="normal">d</mml:mi><mml:mi>p</mml:mi><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
          where <inline-formula><mml:math id="M47" display="inline"><mml:mi>Q</mml:mi></mml:math></inline-formula> is the CWV in units of kg m<inline-formula><mml:math id="M48" 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>, <inline-formula><mml:math id="M49" display="inline"><mml:mrow><mml:mi>g</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">9.8</mml:mn></mml:mrow></mml:math></inline-formula> m s<inline-formula><mml:math id="M50" 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> is the
acceleration due to gravity, and the pressures <inline-formula><mml:math id="M51" 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> and <inline-formula><mml:math id="M52" display="inline"><mml:mrow><mml:msub><mml:mi>p</mml:mi><mml:mi>z</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> denote
the bounds of integration. Considering that atmospheric water
vapor is mainly distributed below 8 km in the tropics due to the rapid
decrease of water vapor with height (Mapes et al., 2017), we choose
<inline-formula><mml:math id="M53" display="inline"><mml:mrow><mml:msub><mml:mi>p</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1000</mml:mn></mml:mrow></mml:math></inline-formula> hPa on the ground and <inline-formula><mml:math id="M54" display="inline"><mml:mrow><mml:msub><mml:mi>p</mml:mi><mml:mi>z</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">300</mml:mn></mml:mrow></mml:math></inline-formula> hPa corresponding to a height of about 9 km. According to Eq. (4), we
calculate the CWV between 30<inline-formula><mml:math id="M55" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> S and 30<inline-formula><mml:math id="M56" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N from January
2005 to December 2019 based on the reanalysis data. Similarly, the monthly
mean CWV and its anomaly can be derived from the CWV series. Figure 2
presents the mean CWV anomalies in the four El Niño winters. In the
2006/07 and 2015/16 EP El Niño events, the positive CWV anomalies appear
in the equatorial central and eastern Pacific, while in 2009/10 and 2018/19
CP El Niño events, the positive anomalies concentrate in the central
Pacific. This is consistent with previous studies (Kug et al., 2009;
Takahashi et al., 2013; Xu et al., 2017). The negative anomalies occur in
the tropical western Pacific and some tropical latitudes off the Equator in
both hemispheres. In the region of the five radiosonde stations, the CWV
anomaly is evidently negative and comparable between the 2009/10 and 2015/16
events, although the two events are classified into different El Niño
types, whereas in the other two events, the water vapor anomaly is weak,
which is in rough agreement with the radiosonde observation in Fig. 1.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2" specific-use="star"><?xmltex \currentcnt{2}?><?xmltex \def\figurename{Figure}?><label>Figure 2</label><caption><p id="d1e911">CWV anomalies averaged over the <bold>(a)</bold> 2006/07, <bold>(b)</bold> 2015/16, <bold>(c)</bold> 2009/10,
and <bold>(d)</bold> 2018/19 winters derived from ERA5 reanalysis data. The blue pluses
denote the five radiosonde stations. The four El Niño events are
classified into (left) EP El Niño and (right) CP El Niño.</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/21/13553/2021/acp-21-13553-2021-f02.png"/>

        </fig>

</sec>
<sec id="Ch1.S3.SS2">
  <label>3.2</label><title>Relation between CWV anomaly and ONI</title>
      <p id="d1e940">We choose the reanalysis CWV anomalies at the five radiosonde stations to
discuss the relationship between the water vapor anomaly and the ENSO. The
monthly mean CWV anomaly averaged at the five stations is derived from the
radiosonde and reanalysis data from January 2005 to December 2019.
Considering that the ONI is a 3-month smoothed value, the monthly mean CWV
anomaly is also smoothed in a 3-month moving window. Figure 3 depicts the
ONI and monthly mean CWV anomalies from the radiosonde and reanalysis data.
The CWV anomalies show a similar temporal evolution between the observation
and the reanalysis with a significant correlation coefficient <inline-formula><mml:math id="M57" display="inline"><mml:mrow><mml:mi>R</mml:mi><mml:mo>=</mml:mo></mml:mrow></mml:math></inline-formula> 0.83, but a
negative correlation to the ONI with a delay of around several months. The
correlation coefficient between the CWV anomaly and the ONI is calculated to
be <inline-formula><mml:math id="M58" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.63 (<inline-formula><mml:math id="M59" display="inline"><mml:mo lspace="0mm">-</mml:mo></mml:math></inline-formula>0.62) with a lag of 3 (2) months. One can note from Fig. 3 that
when a strong La Niña occurs with ONI <inline-formula><mml:math id="M60" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M61" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>1.64 in November 2010, the
water vapor anomaly reaches the positive maximum in February and March 2011
from the observation and reanalysis data, respectively. However, for the
2015/16 super El Niño event with the peak of ONI <inline-formula><mml:math id="M62" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 2.6 in December 2015,
an extremely negative anomaly appears in both the observation and
reanalysis. The negative anomaly attained is as large as <inline-formula><mml:math id="M63" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>5.39 and <inline-formula><mml:math id="M64" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>5.75 kg m<inline-formula><mml:math id="M65" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> in February 2016 from the radiosonde and reanalysis data,
respectively. Similarly, the 2009/10 event has a large index of ONI <inline-formula><mml:math id="M66" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 1.6 in
November 2009, which leads to the strong CWV anomalies of <inline-formula><mml:math id="M67" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>2.45 and <inline-formula><mml:math id="M68" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>3.94 kg m<inline-formula><mml:math id="M69" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> in January 2010 from the radiosonde and reanalysis data,
respectively. Hence, the ENSO or SST anomaly plays an important role in the
water vapor variation in the tropical western Pacific.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3"><?xmltex \currentcnt{3}?><?xmltex \def\figurename{Figure}?><label>Figure 3</label><caption><p id="d1e1051">Time series of (red) ONI index and monthly mean CWV anomalies
derived from (blue) radiosonde observation and (green) reanalysis data at
five radiosonde stations.</p></caption>
          <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://acp.copernicus.org/articles/21/13553/2021/acp-21-13553-2021-f03.png"/>

        </fig>

</sec>
</sec>
<sec id="Ch1.S4">
  <label>4</label><title>Contribution from tropical circulations</title>
<sec id="Ch1.S4.SS1">
  <label>4.1</label><title>Tropical atmospheric circulations</title>
      <p id="d1e1076">Besides the SST effect, evaporated sea water is carried to higher levels by
the upward flow, and thus the water vapor variability in the troposphere is
closely related to the atmospheric circulation. In the tropics, there are
several well-known circulations, i.e., the Hadley, Walker, and monsoon
circulations, and each circulation has its own features and driving force,
although these circulations may also be highly coupled with each other. In this
way, we attempt to estimate the contributions of each tropical circulation
to the observed water vapor anomalies in the El Niño events. According
to Helmholtz's theorem, horizontal wind velocity can be decomposed into
rotational and divergent winds,
            <disp-formula id="Ch1.E5" content-type="numbered"><label>5</label><mml:math id="M70" display="block"><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">V</mml:mi><mml:mi>H</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:msub><mml:mi mathvariant="bold-italic">V</mml:mi><mml:mi mathvariant="normal">Ψ</mml:mi></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="bold-italic">V</mml:mi><mml:mi mathvariant="normal">Φ</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mi mathvariant="bold-italic">k</mml:mi><mml:mo>×</mml:mo><mml:mi mathvariant="normal">∇</mml:mi><mml:mi mathvariant="normal">Ψ</mml:mi><mml:mrow class="chem"><mml:mo>-</mml:mo></mml:mrow><mml:mi mathvariant="normal">∇</mml:mi><mml:mi mathvariant="normal">Φ</mml:mi><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
          where <inline-formula><mml:math id="M71" display="inline"><mml:mi mathvariant="normal">Ψ</mml:mi></mml:math></inline-formula> is the stream function; <inline-formula><mml:math id="M72" display="inline"><mml:mi mathvariant="normal">Φ</mml:mi></mml:math></inline-formula> is the velocity potential;
<inline-formula><mml:math id="M73" display="inline"><mml:mi mathvariant="bold-italic">k</mml:mi></mml:math></inline-formula> is the unit vector in the vertical direction; and
<inline-formula><mml:math id="M74" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">V</mml:mi><mml:mi>H</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M75" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">V</mml:mi><mml:mi mathvariant="normal">Ψ</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, and <inline-formula><mml:math id="M76" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">V</mml:mi><mml:mi mathvariant="normal">Φ</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> are the horizontal, rotational, and divergent wind velocities,
respectively. Thermal driving force resulting from differential heating and
temperature contrast is essential to cause atmospheric
convergence and divergence and vertical motion and then the formation of
atmospheric circulation. The stream function involved in the rotation field
has no contribution to the atmospheric vertical motion, while the velocity
potential may be chosen as the indicator of the atmospheric circulations
since it is in connection with the<?pagebreak page13558?> atmospheric convergence and divergence
associated with the upward and downward motions in the tropical region
(Kanamitsu and Krishnamurti, 1978; Newell et al., 1996; Wang, 2002). Because
atmospheric water vapor comes mainly from the lower atmosphere through
transport of ascending flow, we selected the velocity potential at 850 hPa
to represent the characteristics of the tropical circulations in the lower
troposphere since the pressure level was extensively used to investigate the
lower atmospheric circulation (Wang, 2002; Weng et al., 2008; Zhao et al.,
2010). The divergence and velocity potential fields are calculated by using
the ECMWF reanalysis horizontal winds at 850 hPa according to the following
equation (Krishnamurti, 1971; Tanaka et al., 2004):
            <disp-formula id="Ch1.E6" content-type="numbered"><label>6</label><mml:math id="M77" display="block"><mml:mrow><mml:mi>D</mml:mi><mml:mo>=</mml:mo><mml:mi mathvariant="normal">∇</mml:mi><mml:mo>⋅</mml:mo><mml:msub><mml:mi mathvariant="bold-italic">V</mml:mi><mml:mi>H</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mo>-</mml:mo><mml:msup><mml:mi mathvariant="normal">∇</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mi mathvariant="normal">Φ</mml:mi><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
          where <inline-formula><mml:math id="M78" display="inline"><mml:mi>D</mml:mi></mml:math></inline-formula> is the divergence of horizontal wind. In Eq. (6), the negative sign
means that the divergent wind flows from the large velocity potential to the
small velocity potential.</p>
      <p id="d1e1218">Based on the different driving mechanisms and movement features, Tanaka et
al. (2004) decomposed the tropical circulation in the upper troposphere (200 hPa) into the Hadley, Walker, and monsoon circulations, which had the
advantage of being able to quantitatively evaluate the intensity of the three tropical
circulations by means of the separation of the velocity potential into three
orthogonal spatial patterns. Subsequently, Takemoto and Tanaka (2007) used
these circulation definitions to analyze the Hadley, Walker, and monsoon
circulations at 850 hPa in the lower troposphere and compared the three
circulation components with those in the upper troposphere (200 hPa), which
indicated that the velocity potential intensities could be an index of each
circulation in the lower troposphere without a notable influence from the
surface. Considering that atmospheric water vapor is mainly distributed
below 8 km, directly relevant to the lower tropospheric circulation, we
follow the definitions and methodology proposed by Tanaka et al. (2004) to
obtain these tropical circulations at the 850 hPa level for investigating their
contributions to the observed water vapor anomaly in the four El Niño
events. The velocity potential is divided as follows (Tanaka et al., 2004):
            <disp-formula id="Ch1.E7" content-type="numbered"><label>7</label><mml:math id="M79" display="block"><mml:mrow><mml:mi mathvariant="normal">Φ</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:mo>[</mml:mo><mml:mi mathvariant="normal">Φ</mml:mi><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>)</mml:mo><mml:mo>]</mml:mo><mml:mo>+</mml:mo><mml:mover accent="true"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Φ</mml:mi><mml:mo>*</mml:mo></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>)</mml:mo><mml:mo>+</mml:mo><mml:msup><mml:mi mathvariant="normal">Φ</mml:mi><mml:mo>*</mml:mo></mml:msup><mml:msup><mml:mi/><mml:mo>′</mml:mo></mml:msup><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:mrow></mml:math></disp-formula>
          where <inline-formula><mml:math id="M80" display="inline"><mml:mi>x</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math id="M81" display="inline"><mml:mi>y</mml:mi></mml:math></inline-formula>, and <inline-formula><mml:math id="M82" display="inline"><mml:mi>t</mml:mi></mml:math></inline-formula> are the longitude, latitude, and time, respectively. The square
brackets and asterisk denote the zonal mean and the deviation from the zonal
mean, respectively, and the overbar and prime denote the annual mean and the
departure from the annual mean, respectively. The first term on the right of
Eq. (7) is the zonal-mean component of the velocity potential field, defined
as the Hadley circulation because this circulation, driven by the
large-scale meridional differential heating, may be treated as axisymmetric.
The second and third terms on the right are the annual mean of the deviation
from the zonal mean and the deviation from the annual mean, respectively.
The third term is regarded to be the monsoon circulation since the monsoon
circulation has conspicuous seasonal variability as the sea–land heat
contrast changes. The second term is referred to as the Walker circulation.
The separation is not perfect for the Walker circulation without seasonal
variation, as pointed out by Tanaka et al. (2004). The Walker circulation is
induced by the different SST along the Equator. Considering that the El
Niño usually lasts for more than a year, with a maximum ONI in winter,
we chose the period of June to the next May to estimate the Walker
circulation and thus obtain the Walker circulation anomaly during El
Niño relative to its climatic average. In this way, the problem may not
be very serious. The definitions and decomposition of the tropical
circulations have extensively been used to study the influences of the SST
warming pattern on the interannual variation and long-term trend of the
Hadley, Walker, and monsoon circulations in association with the hydrological
cycle (Tanaka et al., 2005; Park and Sohn, 2008; Li and Feng, 2013; Ma and
Xie, 2013).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4"><?xmltex \currentcnt{4}?><?xmltex \def\figurename{Figure}?><label>Figure 4</label><caption><p id="d1e1335">Climatic means of velocity potential (shading) and
divergent wind fields (arrows) at 850 hPa in DJF derived from reanalysis data during
2005–2019. The red pluses denote the five radiosonde stations.</p></caption>
          <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://acp.copernicus.org/articles/21/13553/2021/acp-21-13553-2021-f04.png"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F5" specific-use="star"><?xmltex \currentcnt{5}?><?xmltex \def\figurename{Figure}?><label>Figure 5</label><caption><p id="d1e1347">Anomalies of velocity potential (shading) and divergent
wind (arrows) at 850 hPa in the winters of <bold>(a)</bold> 2006/07, <bold>(b)</bold> 2015/16, <bold>(c)</bold> 2009/10, and <bold>(d)</bold> 2018/19. The blue pluses denote the five radiosonde stations.</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/21/13553/2021/acp-21-13553-2021-f05.png"/>

        </fig>

      <p id="d1e1368">We first calculate the divergence field of the horizontal wind at 850 hPa
from 2005 to 2019 by using the reanalysis horizontal wind data, and then the
velocity potential is deduced according to Eq. (6), which is equivalent to
solving the Poisson equation. Next, following Eq. (7), the velocity potential
filed is decomposed into the Hadley, Walker, and monsoon circulation
components. In this way, their monthly climatic mean is derived from their
time series. Figure 4 presents the climatic means of the
velocity potential and divergent wind fields in DJF. We choose the<?pagebreak page13559?> velocity
potential as the proxy of the circulation intensity, and thus the intensity of
the tropical circulation in winter can clearly be seen from Fig. 4. The
prominent negative peak of about <inline-formula><mml:math id="M83" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">81</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mn mathvariant="normal">5</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> m<inline-formula><mml:math id="M84" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula> s<inline-formula><mml:math id="M85" 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> in
the velocity potential is situated in the western Pacific warm pool, and thus
there is the convergence center of horizontal wind field, which induces the
rising motion in the lower troposphere over the region, including the five
radiosonde stations. Hence, the atmospheric water vapor is abundant in this
region due to the transport by the strong ascending flow. In contrast,
the maximum velocity potential of <inline-formula><mml:math id="M86" display="inline"><mml:mrow><mml:mn mathvariant="normal">48</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mn mathvariant="normal">5</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> m<inline-formula><mml:math id="M87" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula> s<inline-formula><mml:math id="M88" 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> appears in the northeastern Pacific Ocean and the southern part of the North
American continent, meaning a downward motion associated with the divergence
center in those regions, as well as less water vapor relative to the western
Pacific warm pool region.</p>
</sec>
<sec id="Ch1.S4.SS2">
  <label>4.2</label><title>Atmospheric circulation anomalies</title>
      <p id="d1e1454">Next, we focus on the tropical circulation anomaly in the four El Niño
events. Figure 5 illustrates the velocity potential and divergent wind
anomalies at 850 hPa in the four winters. Here, we define the velocity
potential value as the circulation index with the units measured by <inline-formula><mml:math id="M89" display="inline"><mml:mrow><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mn mathvariant="normal">5</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> m<inline-formula><mml:math id="M90" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula> s<inline-formula><mml:math id="M91" 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 the velocity potential anomaly is
regarded accordingly as the index of the circulation anomaly. As a consequence, the
positive index of the circulation anomaly indicates the weakened convergence
and rising motion or the strengthened divergence and sinking motion and
vice versa for the negative index of the circulation anomaly. Hence, the
positive and negative indices mean the decrease and increase of water vapor
in the troposphere due to the vertical transport change, respectively. In
Fig. 5, the positive index of the circulation anomaly occurs in the western
Pacific, especially in the 2009/10 and 2015/16 El Niño winters, and thus the
ascending motion is suppressed in that region, and the negative water vapor
anomalies are recorded in the radiosonde observation. On the contrary, there
is the negative index in the equatorial eastern Pacific, which causes
the descending flow to be suppressed. Correspondingly, the positive CWV anomaly
over the equatorial eastern Pacific can be seen from Fig. 2.</p>
      <p id="d1e1489">According to Eq. (7), we calculate the velocity potential of the Hadley,
Walker, and monsoon circulations and their anomaly indices at 850 hPa from
the reanalysis data. Figure 6 presents the velocity potential and anomaly
index of the Hadley circulation in the four El Niño winters. Now that
the Hadley circulation is a tropical circulation driven by the meridional
differential heating in the global radiative process (Oort and Yienger,
1996), this large-scale circulation is very similar in different winters,
with the circulation index increasing from the negative peak at about
12<inline-formula><mml:math id="M92" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> S to positive peak at 23<inline-formula><mml:math id="M93" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, and is little affected
by El Niño, with the anomaly index being less than <inline-formula><mml:math id="M94" display="inline"><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mn mathvariant="normal">5</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> m<inline-formula><mml:math id="M95" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula> s<inline-formula><mml:math id="M96" 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> or 2 units. Even so, the pattern of the Hadley circulation
anomaly is distinguished between the EP El Niño and CP El Niño.
During the 2018/19 (2009/10) CP El Niño winters, the index of the Hadley
circulation anomaly is positive over the entire tropics with the maximum of
1.74 (1.65) units at 3<inline-formula><mml:math id="M97" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N (2<inline-formula><mml:math id="M98" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N). However, in the
2006/07 and 2015/16 EP El Niño winters, the positive index is located at
about 5–30<inline-formula><mml:math id="M99" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, and the negative index occurs over
about 30<inline-formula><mml:math id="M100" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> S–5<inline-formula><mml:math id="M101" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N.  Feng and Li (2013) suggested that the
different patterns of the Hadley circulation anomalies between the CP and EP
El Niños are associated with the contrasting underlying thermal
structure changes because the maximum of the zonal-mean SST anomalies is
moved northward to about 10<inline-formula><mml:math id="M102" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N in the CP event relative to the
maximum around the Equator in the EP event. At the five radiosonde sites,
the averaged anomaly index is 0.29, 1.56, 0.65, and 1.37 units in the
2006/07, 2009/10, 2015/06, and 2018/19 winters, respectively, indicating that
the Hadley circulation is too stable to have a significant impact on the
water vapor variation.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F6" specific-use="star"><?xmltex \currentcnt{6}?><?xmltex \def\figurename{Figure}?><label>Figure 6</label><caption><p id="d1e1603">Velocity potential (black) and anomaly index (orange) of the Hadley
circulation at 850 hPa derived from reanalysis data in the <bold>(a)</bold> 2006/07, <bold>(b)</bold> 2015/16, <bold>(c)</bold> 2009/10, and <bold>(d)</bold> 2018/19 winters.</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/21/13553/2021/acp-21-13553-2021-f06.png"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F7" specific-use="star"><?xmltex \currentcnt{7}?><?xmltex \def\figurename{Figure}?><label>Figure 7</label><caption><p id="d1e1627">Velocity potential(shading) and divergent wind (arrows) of the Walker
circulation and their anomalies at 850 hPa in the <bold>(a, e)</bold> 2006/07, <bold>(b, f)</bold> 2015/16, <bold>(c, g)</bold> 2009/10, and <bold>(d, h)</bold> 2018/19 winters. Panels <bold>(a–d)</bold> show
the velocity potential and divergent wind, and panels <bold>(e–h)</bold> show their
anomalies. The red and blue pluses denote the five radiosonde stations.</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/21/13553/2021/acp-21-13553-2021-f07.png"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F8" specific-use="star"><?xmltex \currentcnt{8}?><?xmltex \def\figurename{Figure}?><label>Figure 8</label><caption><p id="d1e1657">Velocity potential (shading) and divergent (arrow) wind of monsoon
circulation and their anomalies at 850 hPa in <bold>(a, e)</bold> 2006/07, <bold>(b, f)</bold> 2015/16, <bold>(c, g)</bold> 2009/10 and <bold>(d, h)</bold> 2018/19 winters. Panels <bold>(a–d)</bold> denote
the velocity potential and divergent wind, and  <bold>(e)</bold>–<bold>(h)</bold> denote their
anomalies. The blue plus denotes the five radiosonde stations.</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/21/13553/2021/acp-21-13553-2021-f08.png"/>

        </fig>

      <?pagebreak page13561?><p id="d1e1688">Figure 7 depicts the velocity potential and anomaly index of the Walker
circulation at 850 hPa in the El Niño winters. Relative to the Hadley
circulation, the Walker circulation is the local circulation formed over the
tropical Pacific with intense ascending flow in the western Pacific and
descending flow in the eastern Pacific, and thus the circulation  has a high variability associated with the SST anomaly caused by ocean current. As the Walker
circulation is directly related to ENSO, the scenarios of the Walker
circulation anomalies are roughly consistent with each other among the four
El Niño events. In general, the positive and negative indices of the
Walker circulation anomaly are located in the western and eastern Pacific,
opposite to the circulation index, respectively, which illustrates that the
Walker circulation anomaly in El Niño suppresses the strong rising in
the western Pacific and sinking in the eastern Pacific. Nevertheless, the
strength of the circulation anomaly is the significant difference among the
four events. In the 2015/16 winter, the Walker circulation anomaly, with
peak indices as large as 26.8 and <inline-formula><mml:math id="M103" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>27.7 units in the equatorial Pacific, is
much stronger than in the other three winters. Hence, the Walker circulation
variation plays a key role in the CWV anomaly during the 2015/16 super El
Niño event.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F9"><?xmltex \currentcnt{9}?><?xmltex \def\figurename{Figure}?><label>Figure 9</label><caption><p id="d1e1700"><bold>(a)</bold> Indices of Hadley (red), Walker (yellow), monsoon (blue),
and total (orange) circulation anomalies and <bold>(b)</bold> CWV anomalies derived
from radiosonde (azure) and reanalysis (green) data at five radiosonde
stations in four El Niño winters.</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://acp.copernicus.org/articles/21/13553/2021/acp-21-13553-2021-f09.png"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F10" specific-use="star"><?xmltex \currentcnt{10}?><?xmltex \def\figurename{Figure}?><label>Figure 10</label><caption><p id="d1e1717">Anomalies of <bold>(a, b)</bold> CWV and velocity potential and divergent wind
at 850 hPa in the <bold>(c, d)</bold> total, <bold>(e, f)</bold> Walker, and <bold>(g, h)</bold> monsoon circulations
for composite EP and CP El Niños derived from reanalysis data. The left
and right columns correspond to the composite EP and CP El Niños,
respectively. The shading and arrows in  <bold>(c–h)</bold> denote the velocity
potential and divergent wind anomalies, respectively. The red and blue pluses
denote the five radiosonde stations.</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/21/13553/2021/acp-21-13553-2021-f10.png"/>

        </fig>

      <p id="d1e1741">The velocity potential and anomaly index of the monsoon circulation in the
four El Niño winters are plotted in Fig. 8. The monsoon circulation in
the lower atmosphere blows from the land to the sea in winter, and thus it can
be<?pagebreak page13562?> seen from Fig. 8 that the pattern of the monsoon circulation is evidently
different from that of the Walker circulation shown in Fig. 7. The anomaly
of the monsoon circulation is sensitive to the type of El Niño, which is
also distinguished from that of the Walker circulation. Early studies showed
that the CP and EP El Niños have different effects on Indian and
eastern Asian monsoon rainfall (Weng et al., 2008; Wang et al., 2013). The
monsoon circulation anomaly at the radiosonde stations has an index around
zero in the EP El Niño events, which is far weaker relative to the large
positive index in the CP El Niño events, similar to previous
investigations (Fan et al., 2017). In the 2009/10 El Niño event, the
pronounced anomaly with a peak index of 17.8 units takes place in the
western Pacific, which implies that the monsoon circulation anomaly has an
important influence on the negative water vapor anomaly in the radiosonde
observation.</p>
</sec>
<sec id="Ch1.S4.SS3">
  <label>4.3</label><title>Contribution to water vapor anomaly</title>
      <p id="d1e1752">We estimate the contributions of the Hadley, Walker, and monsoon circulation
anomalies to the water vapor anomaly observed by the radiosonde in the four
El Niño events by means of comparing the indices of the circulation
anomalies. Figure 9 illustrates the indices of the circulation anomalies at
850 hPa and the CWV anomalies derived from the radiosonde and reanalysis
data, and these circulation anomaly indices and CWV anomalies are the values
averaged at the five radiosonde sites in winter. It can be seen from Fig. 9 that the CWV anomalies in the reanalysis and radiosonde
data qualitatively increase with the increasing index of the total circulation anomaly. As
discussed above, the contribution of the Hadley circulation anomaly is very
small with a maximum of only 1.56 units in the 2009/10 event. The anomaly
of the Walker circulation makes a considerable contribution in each case,
especially for the EP El Niño events, and it is the strongest in the three
tropical circulation anomalies. The index of the Walker circulation anomaly
counts for 92.3 %<?pagebreak page13563?> of the total anomaly index (23.89 units) in the 2015/16
El Niño winter and even exceeds the total index in the 2006/07 event
owing to the negative anomaly of the monsoon circulation. The anomaly of the
monsoon circulation shows an evident change from one event to another
because it is sensitive to the local heat contrast and the El Niño
shift. In the western Pacific, the CP El Niño can lead to the obvious
positive anomaly of the monsoon circulation. The index of the monsoon
circulation anomaly is about 69.7 % (44.7 %) of the total anomaly index
in the 2009/10 (2018/19) CP El Niño winter. Consequently, for the two
intense El Niño events, the water vapor anomaly is caused mainly by the
Walker circulation anomaly in the 2015/16 EP event but by the monsoon
circulation anomaly in the 2009/10 CP event. The Walker and
monsoon circulation anomalies nearly equally (and oppositely) contribute to the
CWV anomaly in the 2018/19 (2006/07) event. Therefore, outside of the Hadley
circulation anomaly, the Walker and monsoon circulation anomalies may have
the largest differences in their contributions to water vapor
variation in different El Niño events. In addition, in the 2015/16 and
2018/19 winters, the reanalysis CWV anomalies of <inline-formula><mml:math id="M104" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>4.34 and <inline-formula><mml:math id="M105" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>1.30 kg m<inline-formula><mml:math id="M106" 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>
are roughly consistent with <inline-formula><mml:math id="M107" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>4.46 and <inline-formula><mml:math id="M108" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>1.54 kg m<inline-formula><mml:math id="M109" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> in the radiosonde
observation, respectively. However, in the first two events, there is a
distinct difference in the CWV anomaly between the reanalysis and radiosonde
data, and we will discuss the discrepancy in detail below.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F11"><?xmltex \currentcnt{11}?><?xmltex \def\figurename{Figure}?><label>Figure 11</label><caption><p id="d1e1810">Distribution of cloud occurrence between 0<inline-formula><mml:math id="M110" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N and
15<inline-formula><mml:math id="M111" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N in <bold>(a)</bold> all winters and the <bold>(b)</bold> 2006/07, <bold>(c)</bold> 2009/10, and <bold>(d)</bold> 2015/16 winters derived from CALIPSO from June 2006 to December 2016.</p></caption>
          <?xmltex \igopts{width=227.622047pt}?><graphic xlink:href="https://acp.copernicus.org/articles/21/13553/2021/acp-21-13553-2021-f11.png"/>

        </fig>

      <p id="d1e1850">In order to obtain the general features of water vapor and circulation
anomalies in the EP and CP El Niño events, we extend the reanalysis data
back to 1979 to examine two types of composite El Niño events. There are
six EP El Niño events in the winters of 1982/83, 1986/87, 1991/92,
1997/98, 2006/07, and 2015/16 and five CP El Niño events in the 1994/95,
2002/03, 2004/05, 2009/10, and 2018/19 winters for the 41 years from 1979 to
2019, which are averaged as the composite EP and CP El Niños,
respectively. We calculate the CWV anomalies in the two composite events
based the climatic mean CWV in 41 winters, and the corresponding velocity
potential and divergent wind anomalies of the Walker, monsoon, and total
circulations from the reanalysis horizontal wind at 850 hPa, which are shown
in Fig. 10. The Hadley circulation anomaly (not presented) is very small,
and its patterns in the composite EP and CP El Niños are also analogous
to those in the EP and CP events shown in Fig. 6, respectively. On the
whole, Fig. 10 illustrates that the total circulation anomaly is stronger in
EP event than in CP event and that the CWV anomaly is larger in EP event
relative to that in CP event. The Walker circulation plays an important role
in the total circulation anomaly, especially in EP El Niño. Despite
significant variability from one event to another, the monsoon circulation
anomaly not only has a larger proportion of the total anomaly but also has a
slightly higher intensity in CP El Niño than in EP El Niño. At the
five radiosonde stations, the composite events indicate that the CWV anomaly
is about <inline-formula><mml:math id="M112" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>4.36 and <inline-formula><mml:math id="M113" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>1.74 kg m<inline-formula><mml:math id="M114" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> in the EP and CP El Niños,
respectively. The index of the Walker circulation anomaly accounts for about
75.8 % (47.8 %) of the total anomaly index in EP (CP) El Niño, while
for the monsoon circulation, the anomaly index of 6.16 (4.66) units
contributes to 49.6 % (18.4 %) of the total anomaly index in CP (EP) El
Niño. Therefore, the relative importance of the Hadley, Walker, and
monsoon circulation anomalies in the composite El Niños is roughly in
accordance with that in the case study above. In addition, at the radiosonde
sites, the CP El Niño can generally cause an intense monsoon circulation
anomaly, which is comparable to and even larger than the Walker circulation
anomaly; thus, the CP El Niño in the winter of 2009/10 may induce a quite
strong monsoon circulation anomaly now that the 2009/10 event is the
strongest CP El Niño from the 1980s onwards, as observed by satellite (Lee and
McPhaden, 2010).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F12" specific-use="star"><?xmltex \currentcnt{12}?><?xmltex \def\figurename{Figure}?><label>Figure 12</label><caption><p id="d1e1882">OLR anomalies averaged over the <bold>(a)</bold> 2006/07, <bold>(b)</bold> 2015/16, <bold>(c)</bold> 2009/10,
and <bold>(d)</bold> 2018/19 winters. The blue pluses denote the five radiosonde stations.</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/21/13553/2021/acp-21-13553-2021-f12.png"/>

        </fig>

</sec>
</sec>
<sec id="Ch1.S5" sec-type="conclusions">
  <label>5</label><title>Changes in cloud and OLR</title>
      <p id="d1e1913">Using the cloud occurrence from the CALIPSO from June 2006 to December 2016, we calculate tropical cloud fraction between 0 and
15<inline-formula><mml:math id="M115" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N in the 2006/07, 2009/10, and 2015/16 winters and its climatic
mean in winter, which is shown in Fig. 11. We also compute the OLR anomalies
over 30<inline-formula><mml:math id="M116" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> S–30<inline-formula><mml:math id="M117" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N in the four El Niño winters based
on the monthly OLR data between 2005 and 2019. Figure 12 shows<?pagebreak page13564?> the OLR
anomalies in the four El Niño events. In the western Pacific, the strong
rising flow carries abundant water vapor to high level due to the
convergence of horizontal wind field in winter, as shown in Fig. 4, and then
the water vapor condenses to form clouds as it cools, and thus there are clouds
over the tropical western Pacific. In the El Niño events, the cloud
amount decreases from about 80 to 160<inline-formula><mml:math id="M118" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E but tends to
increase between about 160<inline-formula><mml:math id="M119" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E to 120<inline-formula><mml:math id="M120" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W because of the
tropical circulation changes. Owing to the reflection effect of cloud on
OLR, the OLR change is opposite to the variation of cloud amount. In the
2009/10 and 2015/16 strong El Niño winters, the OLR is obviously
enhanced in the tropical northwest Pacific and significantly reduced in the
equatorial central eastern Pacific as the cloud occurrence changes. Hence, the
cloud and OLR have a clear response to the water vapor anomaly in the El
Niño events.</p>
      <p id="d1e1971">As described above, the reanalysis CWV anomalies at the radiosonde stations in
the 2009/10 winter have almost the same intensity as that in the 2015/16
winter, but the radiosonde observation indicates that the water vapor
reduction is evidently lower in the 2009/10 winter than in the 2015/16
winter. As shown in Figs. 11 and 12, the satellite observation shows that
there is less cloud occurrence and more OLR at the radiosonde stations in
the 2015/16 winter compared with in the 2009/10 winter. Therefore, this
supports the radiosonde observation that the water vapor over the radiosonde
stations in the 2009/10 winter may be moister than in the reanalysis.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F13"><?xmltex \currentcnt{13}?><?xmltex \def\figurename{Figure}?><label>Figure 13</label><caption><p id="d1e1976">Scatterplots of monthly mean CWV in winter derived from <bold>(a–e)</bold> radiosonde and <bold>(f–j)</bold> AIRS observations against corresponding CWV from ERA5
reanalysis and <bold>(k–o)</bold> climatic mean CWV difference (blue lines) between
radiosonde and ERA5 reanalysis data and (red lines) between AIRS and ERA5
reanalysis data at five stations during 2005–2019. In <bold>(a–j)</bold>, the red,
blue, and gray dots denote the CWV values in the 2009/10 winter; the
2006/2007, 2015/2016, and 2018/2019 winters; and the other winters,
respectively.</p></caption>
        <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://acp.copernicus.org/articles/21/13553/2021/acp-21-13553-2021-f13.png"/>

      </fig>

</sec>
<sec id="Ch1.S6">
  <label>6</label><title>Discussion</title>
      <p id="d1e2005">In the ERA5 reanalysis data, water vapor is calculated by a humidity
analysis scheme introduced by Hólm (2003), which involves nonlinear
transformation of the humidity control variable to render the humidity
background errors nearly Gaussian. The transformation normalizes relative
humidity increments by a factor that varies as a function of background
errors of relative humidity and vertical level (Dee et al., 2011). For the
ERA5 humidity analysis, measurements from radiosondes, surface synoptic
observations, aircraft, and satellite observations are assimilated (Andersson
et al., 2007). To date, the reliability and accuracy of ERA5 water vapor
products have been extensively estimated. Overall, ERA5-retrieved
precipitable water vapor (PWV) performs well over the Indian Ocean (Lees et
al., 2020), central Asia (Jiang et al., 2019), the Antarctic (Ye et al., 2007), the
East African tropical region (Ssenyunzi et al., 2020), and Varanasi (Kumar et
al., 2021), which can be seen via comparisons with ground-based observations, satellite
retrievals, and other reanalysis datasets. Nevertheless, some discrepancies
can be noticed over small tropical islands characterized by steep orography
(Lees et al., 2020), and it is reported that although PWV from the ERA5
reanalysis is in good agreement with the retrievals from the Global Navigation
Satellite System over 268 stations, there is a bias of 4 mm PWV in the southwest of
South America and western China due to the terrain limitations and fewer
observations (Wang et al., 2020).</p>
      <p id="d1e2008">Since the CWV anomalies look more or less different between the radiosonde
and reanalysis data, we compare the CWV in the ERA5 reanalysis with that in
the radiosonde and satellite observations at the five stations and attempt
to explain the different CWV anomalies between the reanalysis data and
radiosonde observations in the 2006/07 and 2009/10 events. By using the
reanalysis data and measurements of radiosondes and AIRS on the Aqua satellite
for the 15-year period from 2005 to 2019, we calculate the monthly mean CWV
at the five radiosonde sites, and Fig. 13 depicts the monthly mean CWV in
winter as scatterplots of the reanalysis vs. radiosonde data and the
reanalysis vs. AIRS data. Following this, the climatic mean difference is derived
from these monthly mean CWV series in 2005–2019, which is also presented in
Fig. 13. At the five stations, the monthly mean CWV in winter is distributed
between 30 and 60 kg m<inline-formula><mml:math id="M121" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> in all three datasets, and the CWV is
obviously shifted to the<?pagebreak page13565?> low values in the El Niño winter, indicating
the negative anomaly in the El Niño event. The correlation of the mean
CWV series between the reanalysis and observations is quite high with the
minimum coefficient of 0.88, and the root mean square (rms) of the mean
CWV differences between the reanalysis and observations is less than 2.32 kg m<inline-formula><mml:math id="M122" 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>. Meanwhile, the difference in the climatic mean CWV is mainly
concentrated in the range of 0–2 kg m<inline-formula><mml:math id="M123" 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>, except for several months at the
Guam station, and thus the relative difference in the monthly mean CWV between
the reanalysis and observations is generally smaller than 5 %. These
comparisons and analyses confirm a fine confidence level of the ERA5
reanalysis and observational datasets. Nevertheless, there are still very
small discrepancies among these data, and the discrepancy is relatively
large between the radiosonde and reanalysis data compared to between the satellite
and reanalysis data, which may be attributed to the different sampling times between the radiosonde and AIRS. It can be noted
from Fig. 13 that the red dots representing the reanalysis vs. radiosonde
data in the 2009/10 winter show a relatively large scatter around the symmetric
axis, indicating a relatively large discrepancy in the CWV anomalies between
the reanalysis data and radiosonde observation in this event, as in previous
reports of some discrepancies over small tropical islands or in the regions
with fewer observations (Lees et al., 2020; Wang et al., 2020). In comparison
to the reanalysis data, the CWV derived from AIRS also shows the largest
difference of 1.31 kg m<inline-formula><mml:math id="M124" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> in the 2009/10 event, while the differences
are less than 1 kg m<inline-formula><mml:math id="M125" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> in the other three events.</p>
      <p id="d1e2071">Based on specific humidity in the reanalysis and radiosonde data, the CWV is
calculated to be 44.87 (44.10), 43.06 (40.23), 41.16 (39.83), and 44.07
(42.87) kg m<inline-formula><mml:math id="M126" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> in the radiosonde (reanalysis) data in the 2006/07,
2009/10, 2015/16, and 2018/19 events, respectively. In fact, the relative
difference in the CWV between the radiosonde and reanalysis data is very
small, with only 1.7 % in the 2006/07 winter and 6.6 % in the 2009/10
winter. The CWV average in winter is 45.61 (44.17) kg m<inline-formula><mml:math id="M127" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> in the
radiosonde (reanalysis) data from 2005 to 2019, and thus the CWV anomaly in the
radiosonde (reanalysis) data is <inline-formula><mml:math id="M128" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.74 (<inline-formula><mml:math id="M129" display="inline"><mml:mo lspace="0mm">-</mml:mo></mml:math></inline-formula>0.07) kg m<inline-formula><mml:math id="M130" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> in the 2006/07
event and <inline-formula><mml:math id="M131" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>2.55 (<inline-formula><mml:math id="M132" display="inline"><mml:mo lspace="0mm">-</mml:mo></mml:math></inline-formula>3.94) kg m<inline-formula><mml:math id="M133" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> in the 2009/10 event. This means that
the discrepancy in the CWV anomaly looks quite large in Fig. 9,
especially in the 2006/07 event, but the differences in both the CWV and CWV
anomaly values are small between the radiosonde and reanalysis. Even so, the
relatively large discrepancy between the reanalysis data and the radiosonde
and AIRS observations in the 2009/10 event, as shown in Figs. 1 and 13, and
the cloud and OLR measurements in Figs. 11 and 12 seem to suggest that the
reanalysis data underestimates the tropospheric water vapor over the
radiosonde stations in the 2009/10 winter.</p>
</sec>
<sec id="Ch1.S7">
  <label>7</label><title>Summary</title>
      <p id="d1e2159">In this paper, we report the significantly negative water vapor anomaly in
the troposphere during four El Niño winters at five radiosonde
stations in the tropical western Pacific based on radiosonde and
reanalysis data for 15 years from 2005 to 2019 and study the relationship
between the water vapor anomaly and the El Niño index and the
contribution of the different tropical circulation anomalies to the observed
water vapor anomaly in the El Niño events.</p>
      <p id="d1e2162">The radiosonde observation shows that the negative water vapor anomaly
arises in the El Niño winters, specifically<?pagebreak page13566?> showing an extremely negative
anomaly in the 2015/16 super El Niño event. The prominent specific
humidity anomaly is concentrated below 8 km in the troposphere with the peak
at the height of about 2.5–3.5 km. The local CWV anomaly has a large
negative correlation coefficient of <inline-formula><mml:math id="M134" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.63 with the ONI in the Niño3.4
region but has a lag of about 2–3 months. The reanalysis data reveal that
the negative water vapor anomaly occurs widely in the tropical northwestern
Pacific, while the positive anomaly correspondingly takes place in the
equatorial central eastern Pacific. The 2015/16 El Niño event (with
ONI <inline-formula><mml:math id="M135" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 2.6) is the strongest during the 15 years, leading to the extreme
anomaly in the water vapor over the tropical Pacific.</p>
      <p id="d1e2179">The atmospheric water vapor from tropical sea water evaporation is affected not only
by the SST but also by the vertical motion of the atmosphere, which
can transport the water vapor from near the sea surface up to high levels.
By using the definitions and method introduced by Tanaka et al. (2004), we
decompose the tropical circulation into the Hadley, Walker, and monsoon
circulations to estimate their contributions to the observed water vapor
anomaly in the four El Niño events. In general, the tropical circulation
anomaly in the El Niño winter is characterized by divergence
(convergence) at 850 hPa in the tropical western (eastern) Pacific, and thus the
CWV decreases over the tropical western Pacific as the ascending flow is
suppressed. As the large-scale meridional circulation is driven by the
differential heating, the variation of the Hadley circulation is pretty
small with an anomaly index of less than 2 units. At the radiosonde stations,
the anomaly of the Walker circulation makes a considerable contribution to
the total anomaly in all the El Niño winters, especially in the 2006/07
and 2015/16 EP El Niño events. The monsoon circulation exhibits an
obvious variability from one event to another, and its anomaly is large in
the 2009/10 and 2018/19 CP El Niño winters and small in the 2006/07 and
2015/16 EP El Niño winters. Therefore, the observed water vapor anomaly
is caused mainly by the Walker circulation anomaly in the 2015/16 super EP
event but by the monsoon circulation anomaly in the 2009/10 strong CP event. Based on the reanalysis data back to 1979, we examine the
general features of water vapor and circulation anomalies in the two types
of composite El Niño events. The roles of the Hadley, Walker, and monsoon
circulations in the composite EP and CP El Niños are consistent with
those in the EP and CP case events.</p>
      <p id="d1e2182">Because of the reduction in the upward transport of water vapor over the
tropical western Pacific in the El Niño events, the satellite
observations show that, relative to the climatic means, the cloud decreases
and that the OLR is accordingly strengthened, particularly during the strong El
Niño winters of 2009/10 and 2015/16. In addition, a detailed comparison
of water vapor in the reanalysis, radiosonde, and satellite data shows a high
confidence level of these datasets; nevertheless, the reanalysis seems to
slightly underestimate the water vapor over the five radiosonde stations in
the 2009/10 winter.</p>
</sec>

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

      <p id="d1e2189">The radiosonde observations are provided by NOAA at the
following website: <uri>https://www.ncei.noaa.gov/pub/data/igra/derived/</uri> (NOAA, 2004).  The
ERA5 reanalysis data are from the ECMWF: <uri>https://cds.climate.copernicus.eu/cdsapp#!/dataset/reanalysis-era5-pressure-levels-monthly-means?tab=form</uri> (Hersbach et al., 2019). The Niño3.4 index
is from NOAA: <uri>https://catalog.data.gov/dataset/climate-prediction-center-cpcoceanic-nino-index</uri> (NOAA, 2021).
The OLR data are from NOAA: <uri>https://downloads.psl.noaa.gov/Datasets/interp_OLR/</uri> (NOAA, 2003).   The cloud occurrence monthly data are from NASA: <uri>https://search.earthdata.nasa.gov/search/granules?p=C1575511329-LARC_ASDC&amp;pg[0][v]=f&amp;tl=1630929576.307!3!!</uri> (NASA, 2018). The AIRS water vapor data are
available from NASA: <ext-link xlink:href="https://doi.org/10.5067/Aqua/AIRS/DATA321" ext-link-type="DOI">10.5067/Aqua/AIRS/DATA321</ext-link> (AIRS Science Team and Teixeira, 2013).</p>
  </notes><notes notes-type="authorcontribution"><title>Author contributions</title>

      <p id="d1e2214">KH and MD proposed the scientific ideas. MD and KH
completed the analysis and the manuscript. SZ, CH, YG, and FY discussed the
results in the manuscript.</p>
  </notes><notes notes-type="competinginterests"><title>Competing interests</title>

      <p id="d1e2220">The contact author has declared that neither they nor their co-authors have any competing interests.</p>
  </notes><notes notes-type="disclaimer"><title>Disclaimer</title>

      <p id="d1e2226">Publisher's note: Copernicus Publications remains neutral with regard to jurisdictional claims in published maps and institutional affiliations.</p>
  </notes><ack><title>Acknowledgements</title><p id="d1e2232">This work was supported by the National Natural Science
Foundation of China (grant nos. 41974176 and 41674151).</p></ack><notes notes-type="financialsupport"><title>Financial support</title>

      <p id="d1e2238">This research has been supported by the National Natural Science Foundation of China (grant nos. 41974176 and 41674151).</p>
  </notes><notes notes-type="reviewstatement"><title>Review statement</title>

      <p id="d1e2244">This paper was edited by Bryan N. Duncan and reviewed by two anonymous referees.</p>
  </notes><ref-list>
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    <!--<article-title-html>Water vapor anomaly over the tropical western Pacific in El Niño winters from radiosonde and satellite observations and ERA5 reanalysis data</article-title-html>
<abstract-html><p>Using radiosonde observations at five stations in the tropical
western Pacific and reanalysis data for the 15 years from 2005 to 2019, we
report an extremely negative anomaly in atmospheric water vapor during the
super El Niño winter of 2015/16 and compare the anomaly with that in
the other three El Niño winters of the period. A strong specific humidity anomaly is
concentrated below 8&thinsp;km of the troposphere with a peak at 2.5–3.5&thinsp;km, and a
column-integrated water vapor mass anomaly over the five radiosonde sites
has a large negative correlation coefficient of −0.63 with the oceanic
Niño3.4 index but with a lag of about 2–3 months. In general, the
tropical circulation anomaly in the El Niño winter is characterized by
divergence (convergence) in the lower troposphere over the tropical western
(eastern) Pacific; thus, the water vapor decreases over the tropical western
Pacific as upward motion is suppressed. The variability of the Hadley
circulation is quite small and has little influence on the observed water
vapor anomaly. The anomaly of the Walker circulation makes a considerable
contribution to the total anomaly in all four El Niño winters,
especially in the 2006/07 and 2015/16 eastern Pacific (EP) El Niño
events. The monsoon circulation shows a remarkable change from one event to
another, and its anomaly is large in the 2009/10 and 2018/19 central Pacific
(CP) El Niño winters and small in the two EP El Niño winters. The
observed water vapor anomaly is caused mainly by the Walker circulation
anomaly in the super EP event of 2015/16 but is caused by the monsoon circulation
anomaly in the strong CP event of 2009/10. The roles of the Hadley, Walker,
and monsoon circulations in the EP and CP events are confirmed by the
composite EP and CP El Niños based on the reanalysis data for 41 years.
Owing to the anomalous decrease in upward transport of water vapor during
the El Niño winter, lower cloud amounts and more outgoing longwave
radiation over the five stations are clearly presented in satellite
observation. In addition, a detailed comparison of water vapor in the
reanalysis, radiosonde, and satellite data shows a fine confidence level for
the datasets; nevertheless, the reanalysis seems to slightly underestimate
the water vapor over the five stations in the 2009/10 winter.</p></abstract-html>
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