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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-22-14177-2022</article-id><title-group><article-title>Temporal variability of tropospheric ozone and ozone profiles in the Korean Peninsula during the East Asian summer monsoon: insights from multiple
<?xmltex \hack{\break}?> measurements and reanalysis datasets</article-title><alt-title>Temporal variability of tropospheric ozone and ozone profiles in the Korean Peninsula</alt-title>
      </title-group><?xmltex \runningtitle{Temporal variability of tropospheric ozone and ozone profiles in the Korean Peninsula}?><?xmltex \runningauthor{J. Bak et al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes" rid="aff1">
          <name><surname>Bak</surname><given-names>Juseon</given-names></name>
          <email>juseonbak@pusan.ac.kr</email>
        <ext-link>https://orcid.org/0000-0002-0421-671X</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff6">
          <name><surname>Song</surname><given-names>Eun-Ji</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-3285-3003</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff5">
          <name><surname>Lee</surname><given-names>Hyo-Jung</given-names></name>
          
        <ext-link>https://orcid.org/0000-0003-3943-2671</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Liu</surname><given-names>Xiong</given-names></name>
          
        <ext-link>https://orcid.org/0000-0003-2939-574X</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3">
          <name><surname>Koo</surname><given-names>Ja-Ho</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff4">
          <name><surname>Kim</surname><given-names>Joowan</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-8609-3425</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff5">
          <name><surname>Jeon</surname><given-names>Wonbae</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-4898-7292</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff5">
          <name><surname>Kim</surname><given-names>Jae-Hwan</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-6794-9534</ext-link></contrib>
        <contrib contrib-type="author" corresp="yes" rid="aff1 aff5">
          <name><surname>Kim</surname><given-names>Cheol-Hee</given-names></name>
          <email>chkim2@pusan.ac.kr</email>
        <ext-link>https://orcid.org/0000-0002-2967-4987</ext-link></contrib>
        <aff id="aff1"><label>1</label><institution>Institute of Environmental Studies, Pusan National University, Busan 46241, South Korea</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>Smithsonian Astrophysical Observatory (SAO), Center for Astrophysics | Harvard &amp; Smithsonian, <?xmltex \hack{\break}?> Cambridge, MA 02138, USA</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>Department of Atmospheric Sciences, Yonsei University, Seoul 03722, South Korea</institution>
        </aff>
        <aff id="aff4"><label>4</label><institution>Department of Atmospheric Sciences, Kongju National University, Kongju 32588, South Korea</institution>
        </aff>
        <aff id="aff5"><label>5</label><institution>Department of Atmospheric Sciences, Pusan National University, Busan 46241, South Korea</institution>
        </aff>
        <aff id="aff6"><label>a</label><institution>currently at: Supercomputer Center, Pukyong National University, Busan 48513, South Korea</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Juseon Bak (juseonbak@pusan.ac.kr) and Cheol-Hee Kim (chkim2@pusan.ac.kr)</corresp></author-notes><pub-date><day>4</day><month>November</month><year>2022</year></pub-date>
      
      <volume>22</volume>
      <issue>21</issue>
      <fpage>14177</fpage><lpage>14187</lpage>
      <history>
        <date date-type="received"><day>28</day><month>June</month><year>2022</year></date>
           <date date-type="rev-request"><day>26</day><month>July</month><year>2022</year></date>
           <date date-type="rev-recd"><day>6</day><month>October</month><year>2022</year></date>
           <date date-type="accepted"><day>7</day><month>October</month><year>2022</year></date>
      </history>
      <permissions>
        <copyright-statement>Copyright: © 2022 </copyright-statement>
        <copyright-year>2022</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="d1e196">We investigate the temporal variations of ground-level ozone and
balloon-based ozone profiles at Pohang (36.02<inline-formula><mml:math id="M1" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 129.23<inline-formula><mml:math id="M2" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E) in
the Korean Peninsula. Satellite measurements and chemical reanalysis products
are also intercompared to address their capability of providing  consistent
information on the temporal and vertical variability of atmospheric ozone.
Sub-seasonal variations of the summertime lower-tropospheric ozone exhibit a
bimodal pattern related to atmospheric weather patterns modulated by the
East Asian monsoon circulation. The peak ozone abundances occur during the
pre-summer monsoon with enhanced ozone formation due to favorable
meteorological conditions (dry and sunny). Ozone concentrations reach their
minimum during the summer monsoon and then re-emerge in autumn before the
winter monsoon arrives. Profile measurements indicate that ground-level
ozone is vertically mixed up to 400 hPa in summer, while the impact of the
summer monsoon on ozone dilution is found up to 600 hPa. Compared to
satellite measurements, reanalysis products largely overestimate ozone
abundances in both the troposphere and stratosphere and give inconsistent
features of temporal variations. Nadir-viewing measurements from the Ozone
Monitoring Instrument (OMI) slightly underestimate the boundary layer ozone
but represent the bimodal peaks of ozone in the lower troposphere and
the interannual changes in the lower-tropospheric ozone in August well, with
higher ozone concentrations during strong El Niño events and  low
ozone concentrations during the 2020 La Niña event.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <label>1</label><title>Introduction</title>
      <p id="d1e226">Ozone in the lower troposphere should be reduced due to its adverse effect
as a key air pollutant and greenhouse gas, whereas stratospheric ozone
should be protected for life on the Earth due to its essential role in
shielding harmful ultraviolet (UV) rays from the sun. Human activities
damage the protective layer of the stratosphere with emissions of
ozone-depleting substances (halogen source gases) and cause emissions
of tropospheric ozone precursors (nitrogen oxides, volatile organic
compounds), which chemically react in the presence of sunlight, producing
tropospheric ozone. The photochemical formation and fate of ozone in the
troposphere complicatedly interact with meteorology and climate
variability (Jacob
and Winner, 2009; Lu et al., 2019; Zhang and Wang, 2016), making it
difficult to evaluate impacts of emission control measures on surface
ozone levels (Dufour et al., 2021). Also, tropospheric
ozone is strongly influenced by either downward transport of stratospheric
air masses or the horizontal transport of polluted air masses
(Langford
et al., 2015; Walker et al., 2010).</p>
      <p id="d1e229">A monsoon is a major atmospheric circulation system affecting air mass
transport, convection, and precipitation in the middle and high latitudes.
Lower-tropospheric ozone and its precursors can be significantly modulated
by monsoonal changes in the physical and chemical processes of production,
as well as deposition and redistribution. The regional seasonality of ozone as well
as the latitudinal differences in ozone seasonality were attributed to the atmospheric circulation driven by the
Asian monsoon
(Worden et al., 2009). In particular,
impacts of the East Asian summer monsoon (EASM) on spatiotemporal variations
of surface layer ozone concentrations over China have been comprehensively
addressed
(Gao
et al., 2021; He et al., 2008; Li et al., 2018; Shen et al., 2022; Yang et
al., 2014; Yin et al., 2019; Zhao et al., 2010). For example,
Yin et al. (2019) characterized the
geographical distribution of ozone in China, with a bimodal structure of
ozone with a summer trough in the southern China, whereas there is a unimodal cycle in
northern China.
Shen et al. (2022) specified the source–receptor relationships of ozone pollution over
central and eastern China, mainly modulated by the monsoon circulation.</p>
      <p id="d1e232">In view of the rainfall characteristics during EASM and its impact on
tropospheric ozone over East Asia, the Korean Peninsula is one of the best
regions worldwide for examining the linkages between ozone and meteorology. The Korean Peninsula is located in the easternmost part of the Asian continent adjacent to the western Pacific where more than half of the total rainfall amount is typically concentrated during a short rainy season called Jangma in summer, largely controlled by the EASM (Choi et al., 2020; Ha et al., 2012). Therefore, understanding EASM-induced changes in chemical composition over the Korean Peninsula is of importance, which has rarely been addressed in the literature, especially for ozone.</p>
      <p id="d1e235">The main objective of this paper is to characterize the temporal variability
of tropospheric ozone and ozone profiles by linking it with the meteorological variability largely controlled by the EASM. Ground-based and balloon-based observations are collected from Pohang station (36.02<inline-formula><mml:math id="M3" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 129.23<inline-formula><mml:math id="M4" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E) as a reference dataset. The ground measurements are used to interpret the sub-seasonal variability of surface ozone, while the vertical seasonality of ozone is investigated from ozonesondes. This paper is a preliminary activity of the Asian Summer Monsoon Chemical and Climate Impact Project (ACCLIP) campaign (<uri>https://www2.acom.ucar.edu/acclip</uri>, last access: 25 October 2022) to investigate the impact of the Asian summer monsoon on regional and global chemistry. The ACCLIP campaign operates two aircraft during the period of July to August in 2022 to measure atmospheric compounds through the entire troposphere to lower troposphere over East Asia and the western Pacific. The second objective of this paper is to evaluate whether the chemical reanalysis data and remote-sensing data could represent a consistent picture of the summer monsoon impact on ozone profile distribution. This evaluation will give insights on the data selection used to fill in the spatiotemporal gaps of the ACCLIP measurements.</p>
</sec>
<sec id="Ch1.S2">
  <label>2</label><title>Data descriptions</title>
<sec id="Ch1.S2.SS1">
  <label>2.1</label><title>Ground measurements</title>
      <p id="d1e274">Surface in situ measurements of O<inline-formula><mml:math id="M5" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> and NO<inline-formula><mml:math id="M6" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> are collected from air
quality monitoring networks of the National Institute of Environmental
Research (NIER) (AirKorea, <uri>http://www.airkorea.or.kr</uri>, last access: 25 October 2022). This network measures hourly air pollutant (O<inline-formula><mml:math id="M7" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>, NO<inline-formula><mml:math id="M8" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, CO, SO<inline-formula><mml:math id="M9" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>) mixing ratios through chemiluminescence technology (Kley and Mcfarland, 1980). The KMA operates automatic synoptic observation system (ASOS) at 102 weather stations. The ASOS measurements are provided on five types of timescales (minutely, hourly, daily, monthly, yearly) via the KMA Weather Data Service (<uri>https://data.kma.go.kr/</uri>, last access: 25 October 2022). We used daily averages of air temperature, relative humidity, solar irradiance, total precipitation, wind speed, and wind direction.</p>
</sec>
<sec id="Ch1.S2.SS2">
  <label>2.2</label><title>Ozonesonde measurements</title>
      <p id="d1e337">Ozonesondes are balloon-borne instruments capable of measuring the vertical
distribution of atmospheric ozone from the surface to balloon burst, usually
near 35 km. The electrochemical concentration cell (ECC) sensor is the
most widely employed. ECC ozonesondes have an uncertainty of 5 %–10 % and a precision of 3 %–5 % (Smit et al., 2007). In
South Korea, ECC sondes have been regularly launched only at Pohang station every Wednesday in the afternoon (13:30–15:30 LT) since 1995. Ozonesonde measurements are reported in units of partial pressure (mPa) with vertical resolution of about 100 m by the Korea Meteorological Administration (KMA). Bak et al. (2019) demonstrated that Pohang ozonesonde measurements are a stable set of reference profiles for validating satellite products, with quality comparable to ECC ozonesonde measurements in Japan and Hong Kong. To improve the data quality, we screened out sounding measurements at balloon burst altitudes higher than 200 hPa and observations of either tropospheric ozone column values above 80 DU or stratospheric ozone column values below 100 DU.</p><?xmltex \hack{\newpage}?>
</sec>
<sec id="Ch1.S2.SS3">
  <label>2.3</label><title>Satellite measurements</title>
      <p id="d1e349">Both OMI and MLS were launched on board NASA's EOS-Aura spacecraft in
July 2004 and are still functioning in measuring the Earth's atmospheric
composition. The Aura satellite crosses the Equator at <inline-formula><mml:math id="M10" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 13:30
in the afternoon. OMI is a nadir-viewing imaging spectrometer capable of
daily global mapping at a relatively high spatial resolution of 13 km <inline-formula><mml:math id="M11" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 24–48 km (across <inline-formula><mml:math id="M12" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> along-track). MLS measures
microwave thermal emission from the limb of Earth's atmosphere. Compared to
OMI, MLS makes measurements at a good vertical resolution (<inline-formula><mml:math id="M13" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:math></inline-formula> km) in the upper atmosphere but at relatively coarse horizontal resolutions
(<inline-formula><mml:math id="M14" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">165</mml:mn></mml:mrow></mml:math></inline-formula> km along the orbit track). Version 4.2 of the MLS
standard ozone product is used in this study, only for the recommended
vertical range from 261 to 0.025 hPa (Schwartz et al., 2015). We used OMI
ozone profiles retrieved using the PROFOZ version 2 algorithm, which is in
preparation for reprocessing OMI measurements to release a new version of
the OMPROFOZ research product (Liu
et al., 2010). This retrieval algorithm consists of wavelength and radiometric
calibrations as well as forward modeling simulations, with an optimal estimation
inversion in which a priori knowledge is optimally combined with measurement
information to obtain a better estimate of the state (Rodgers,
2000). The measurement sensitivity inherently decreases toward the surface,
with the increasing dependence of retrievals on the a priori information (Bak et al., 2013).
OMI sensitivity is very low to surface ozone, with its maximum in the free
troposphere (<inline-formula><mml:math id="M15" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">500</mml:mn></mml:mrow></mml:math></inline-formula> hPa) (Shen et al., 2019).</p>
</sec>
<sec id="Ch1.S2.SS4">
  <label>2.4</label><title>Reanalysis data</title>
      <p id="d1e412">The Modern-Era Retrospective Analysis for Research and Applications version
2 (MERRA-2) is NASA's latest reanalysis, spanning the satellite observing
era from 1980 to the present (Gelaro et
al., 2017). In addition to a standard meteorological analysis, a
global O<inline-formula><mml:math id="M16" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> field is driven by atmospheric dynamics and constrained by
satellite O<inline-formula><mml:math id="M17" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> measurements using the GEOS-5 atmospheric model and the
data assimilation system. Since October 2004, MERRA-2 has assimilated
total column ozone from OMI and stratospheric ozone profiles above 215 hPa
from MLS. Note that OMI total column ozone is assimilated to account for the
lower sensitivity of MLS measurements in the lower stratosphere,
specifically in clouded scenes.</p>
      <p id="d1e433">The CAMS reanalysis is the latest global reanalysis dataset of atmospheric
composition produced by the Copernicus Atmosphere Monitoring Service (CAMS),
covering the period from 2003 to the present (Inness et al.,
2019). Compared to MERRA-2, multiple satellite measurements were assimilated
for the CAMS reanalysis with ECMWF's Integrated Forecasting System. These
included total ozone columns from SCIAMACHY, OMI, and GOME-2 as well as
ozone profiles from MIPAS and MLS after 2005.</p>
      <p id="d1e436"><?xmltex \hack{\newpage}?>Both types of reanalysis data have similar temporal and spatial resolutions. The MERRA-2
system produces 3-hourly analyses at 72 sigma–pressure hybrid layers between
the surface and 0.01 hPa, with a horizontal resolution of 0.625<inline-formula><mml:math id="M18" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M19" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.5<inline-formula><mml:math id="M20" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>. The CAMS reanalysis data provide estimates every
3 h with a horizontal resolution of 0.75<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> 0.75<inline-formula><mml:math id="M23" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>.
The vertical resolution of the model consists of 60 hybrid sigma–pressure
(model) levels from the surface to 0.1 hPa. In this study, we used CAMS global
reanalysis (EAC4) monthly averaged fields at 25 pressure levels (1000 hPa to
1 hPa) as well as MERRA-2 monthly mean data at 42 pressure levels (1000 hPa
to 1 hPa). Both datasets provide ozone profiles in the unit of mixing ratio.</p>
</sec>
</sec>
<sec id="Ch1.S3">
  <label>3</label><title>Results and discussion</title>
<sec id="Ch1.S3.SS1">
  <label>3.1</label><title>Temporal variability of ground-level ozone</title>
      <p id="d1e507">Figure 1 shows both interannual and seasonal changes in daily ground-level
concentrations of O<inline-formula><mml:math id="M24" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> averaged at six AirKorea sites located within
Pohang for 16 years (2005–2020) in comparison with its primary precursor
NO<inline-formula><mml:math id="M25" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>. Pohang is a major industrial city on South Korea's east coast,
with the largest population of northern Gyeongsang Province. In this analysis, hourly measurements in the afternoon (13:00–15:00 local time) are first averaged for a given calendar day and then smoothed by a 2-week moving average. The afternoon NO<inline-formula><mml:math id="M26" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> does not change much seasonally. However, the seasonal cycle of ozone is bimodal with peaks in early summer and fall. Ozone concentration rapidly increases from <inline-formula><mml:math id="M27" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">30</mml:mn></mml:mrow></mml:math></inline-formula> ppb in January to primary peak values of <inline-formula><mml:math id="M28" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">55</mml:mn></mml:mrow></mml:math></inline-formula> ppb on average during the period of late May to early June. The second peak of ozone occurs in fall, which is much lower than the major peak.</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="d1e559"><bold>(a)</bold> The 2-week moving averages of daytime ground-level ozone
concentrations monitored at six sites in Pohang, with <bold>(b)</bold> corresponding
NO<inline-formula><mml:math id="M29" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentrations. Different colors represent each year from 2005
to 2020, while the black line represents the mean ozone concentrations from
all years.</p></caption>
          <?xmltex \igopts{width=398.338583pt}?><graphic xlink:href="https://acp.copernicus.org/articles/22/14177/2022/acp-22-14177-2022-f01.png"/>

        </fig>

      <p id="d1e582">In wintertime, the annual minimum ozone concentrations have gradually
increased by <inline-formula><mml:math id="M30" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">10</mml:mn></mml:mrow></mml:math></inline-formula> ppb during last 15 years, whereas the annual
maximum of summertime ozone has rapidly increased from <inline-formula><mml:math id="M31" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">40</mml:mn></mml:mrow></mml:math></inline-formula> to
80 ppb in spite of the reduction of the NO<inline-formula><mml:math id="M32" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> amount by <inline-formula><mml:math id="M33" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">15</mml:mn></mml:mrow></mml:math></inline-formula> ppb or more.</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="d1e627">Daily ground-level ozone concentrations (black) with weekly
moving averages applied (thick line) or not (thin line) at Pohang in
2020. The corresponding meteorological factors are overplotted: surface air
temperature (red, <inline-formula><mml:math id="M34" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C), solar radiation (yellow, MJ m<inline-formula><mml:math id="M35" 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>), and
relative humidity (dark green, %). The bar graph shows the total
precipitation (mm) for each week.</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/22/14177/2022/acp-22-14177-2022-f02.png"/>

        </fig>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T1"><?xmltex \currentcnt{1}?><label>Table 1</label><caption><p id="d1e660">Same as Fig. 2, but for correlation coefficients between ozone and
meteorological variables for pre-summer, summer, and post-summer periods.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="4">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="right"/>
     <oasis:colspec colnum="3" colname="col3" align="right"/>
     <oasis:colspec colnum="4" colname="col4" align="right"/>
     <oasis:thead>
       <oasis:row>
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2">Pre-summer</oasis:entry>
         <oasis:entry colname="col3">Summer</oasis:entry>
         <oasis:entry colname="col4">Post-summer</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2">(Jan–May)</oasis:entry>
         <oasis:entry colname="col3">(Jun–Aug)</oasis:entry>
         <oasis:entry colname="col4">(Sep–Dec)</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>
         <oasis:entry colname="col1">Solar radiation</oasis:entry>
         <oasis:entry colname="col2">0.91</oasis:entry>
         <oasis:entry colname="col3">0.74</oasis:entry>
         <oasis:entry colname="col4">0.51</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Air temperature</oasis:entry>
         <oasis:entry colname="col2">0.79</oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M36" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">0.15</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4">0.69</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Relative humidity</oasis:entry>
         <oasis:entry colname="col2"><inline-formula><mml:math id="M37" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">0.27</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M38" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">0.64</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4">0.59</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table></table-wrap>

      <p id="d1e780">In order to avoid smoothing out important features of intra-summer
variations in ozone and their association with synoptic weather patterns,
daily ozone and meteorological variables are zoomed in for 2020 as a 1-week
moving average (Fig. 2). The local maximum ozone concentrations are
generally tied to the local warm, dry air and intense solar radiation
before the rainy season starts.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3" specific-use="star"><?xmltex \currentcnt{3}?><?xmltex \def\figurename{Figure}?><label>Figure 3</label><caption><p id="d1e785">Wind roses for individual months from June through September in
2020 at Pohang. Note that hourly observations in daytime are used to be
consistent with data processing done in Figs. 1 and 2.</p></caption>
          <?xmltex \igopts{width=398.338583pt}?><graphic xlink:href="https://acp.copernicus.org/articles/22/14177/2022/acp-22-14177-2022-f03.png"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4" specific-use="star"><?xmltex \currentcnt{4}?><?xmltex \def\figurename{Figure}?><label>Figure 4</label><caption><p id="d1e797"><bold>(a)</bold> Monthly variations of layer ozone partial pressures from
ozonesonde soundings obtained from Pohang during the period of 2005 to 2020.
The legend values indicate the midpoint pressure of the layer (hPa). <bold>(b)</bold>
Correlation coefficients of monthly ozone variations between each layer and the
bottom layer (916 hPa in red) and between each layer and the top layer (55 hPa in green).</p></caption>
          <?xmltex \igopts{width=398.338583pt}?><graphic xlink:href="https://acp.copernicus.org/articles/22/14177/2022/acp-22-14177-2022-f04.png"/>

        </fig>

      <p id="d1e811">The correlation between ozone concentrations and meteorological variables is
quantitatively compared in Table 1 for summer and the post- and pre-summer periods, respectively. Solar insolation amounts are directly linked to ozone
concentrations over all seasons (<inline-formula><mml:math id="M39" display="inline"><mml:mrow><mml:mi>r</mml:mi><mml:mo>=</mml:mo></mml:mrow></mml:math></inline-formula> 0.51–0.91). The significant
relationship between ozone and air temperature is also identified before and
after summer seasons. However, in summer, ozone variations are rarely linked
with temperature variations due to the intense precipitation suppressing
ozone formation. Consequently, the local minimum ozone levels are tied to
the local maximum  relative humidity during the rainy season
(<inline-formula><mml:math id="M40" display="inline"><mml:mrow><mml:mi>r</mml:mi><mml:mo>=</mml:mo><mml:mo>-</mml:mo><mml:mn mathvariant="normal">0.64</mml:mn></mml:mrow></mml:math></inline-formula>). This indicates that both the depth and width of the summer
trough could be highly variable, likely influenced by the strength and
duration of the summer monsoon (Yang et al., 2014; Zhou et al., 2022). Note that the relative humidity is significantly influenced by air temperature, rather than the amount of water vapor in the pre- and post-summer periods. Therefore, in post-summer the correlation of ozone with relative humidity (<inline-formula><mml:math id="M41" display="inline"><mml:mrow><mml:mi>r</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.59</mml:mn></mml:mrow></mml:math></inline-formula>) is likely to arise from the correlation of ozone with air temperature (<inline-formula><mml:math id="M42" display="inline"><mml:mrow><mml:mi>r</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.51</mml:mn></mml:mrow></mml:math></inline-formula>). The rapid drop of <inline-formula><mml:math id="M43" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">10</mml:mn></mml:mrow></mml:math></inline-formula> ppb in ozone from the end of July to early August is hardly explained by the meteorological factors mentioned above; the weather becomes warmer with other meteorological variables (precipitation and solar radiation) being relatively invariant. However, the prevailing wind is characterized by southwesterlies in early August, whereas the northwesterly winds were dominant in July and late August (see Fig. 3). This summer minimum could deepen with the inflow of a poor ozone air mass originating from the southern sea off the Korean Peninsula into inland areas.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F5" specific-use="star"><?xmltex \currentcnt{5}?><?xmltex \def\figurename{Figure}?><label>Figure 5</label><caption><p id="d1e874">Contour plots of monthly ozone profiles in 2020 from <bold>(a)</bold>
ozonesonde, <bold>(b)</bold> MLS, <bold>(c)</bold> OMI, <bold>(d)</bold> OMI a priori, <bold>(e)</bold> MERRA-2, and <bold>(f)</bold> CAMS.
The meteorological variables are superimposed for wind barbs (red symbols),
potential temperatures (black contours), and thermal tropopause heights (white
lines) using monthly MERRA-2 meteorological data. The ozone value of 150 ppb is plotted with green lines to indicate the chemical transition between the
troposphere and stratosphere.</p></caption>
          <?xmltex \igopts{width=398.338583pt}?><graphic xlink:href="https://acp.copernicus.org/articles/22/14177/2022/acp-22-14177-2022-f05.png"/>

        </fig>

</sec>
<sec id="Ch1.S3.SS2">
  <label>3.2</label><title>Temporal variability of ozone profiles</title>
      <p id="d1e910">To understand the seasonality of ozone profiles, ozonesonde measurements
collected at Pohang station are climatologically averaged for each month and
each pressure bin (<?xmltex \hack{\mbox\bgroup}?><inline-formula><mml:math id="M44" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">0.5</mml:mn></mml:mrow></mml:math></inline-formula><?xmltex \hack{\egroup}?> km intervals). Ozonesonde soundings
mainly measure ozone in the lower atmosphere below 10 hPa, while space-based
limb soundings mainly measure ozone in the upper atmosphere above 215 hPa.
However, both sounding measurements provide limited spatiotemporal
information. OMI nadir measurements and reanalysis data provide daily
global maps of ozone profiles, but the reliability of those data products
should be assured before using them to interpret ozone variability and its
linkage to the monsoon circulation. As shown in Fig. 4a, two kinds of
seasonal patterns are identified with a bimodal structure of layer ozone
partial pressures in the lower troposphere (LT), whereas there is a unimodal cycle in
the upper troposphere and lower stratosphere (UTLS). The LT ozone
concentrations peak in June and October with a global minimum in
winter as well as a local summer minimum in late July and early August,
which is consistent with surface measurements. The concentrations of UTLS
ozone are relatively higher in March due to the stratospheric intrusion,
while the minimum concentrations appear broadly over the summer and early
fall due to the rise of the tropopause, which is a common feature of ozone
in the extratropical UTLS
(Gettelman et al.,
2011; Rao et al., 2003). In order to quantify the similarity of seasonal
variations, the correlation coefficient is calculated for temporal ozone
changes between each layer and the top and bottom layer. As shown in Fig. 4b
the seasonality of ozone at 50 hPa is significantly correlated down to
<inline-formula><mml:math id="M45" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">300</mml:mn></mml:mrow></mml:math></inline-formula> hPa, with a correlation coefficient larger than
0.8. In addition, ozone in the boundary layer is significantly correlated
with the lower-tropospheric ozone up to 700 hPa (<inline-formula><mml:math id="M46" display="inline"><mml:mrow><mml:mi>r</mml:mi><mml:mi mathvariant="italic">&gt;</mml:mi><mml:mn mathvariant="normal">0.9</mml:mn></mml:mrow></mml:math></inline-formula>) as well
as the upper-tropospheric ozone up to <inline-formula><mml:math id="M47" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">300</mml:mn></mml:mrow></mml:math></inline-formula> hPa (<inline-formula><mml:math id="M48" display="inline"><mml:mrow><mml:mi>r</mml:mi><mml:mo>=</mml:mo></mml:mrow></mml:math></inline-formula> 0.7–0.8).
This illustrates that 300 hPa could be regarded as a chemical barrier
working as a boundary between the troposphere and stratosphere at Pohang.</p>
      <p id="d1e968">In Fig. 5, monthly averaged ozonesonde profiles are presented for 2020 and
compared as a reference to assess satellite measurements and reanalysis
products. This contour map of ozonesondes clearly illustrates the intrusion
depth of stratospheric air masses down to <inline-formula><mml:math id="M49" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">300</mml:mn></mml:mrow></mml:math></inline-formula> hPa during spring months (Fig 5a). The mixing depth of ozone that forms near the ground level is also identified, which is bounded up to <inline-formula><mml:math id="M50" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">400</mml:mn></mml:mrow></mml:math></inline-formula> hPa in the summer and <inline-formula><mml:math id="M51" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">600</mml:mn></mml:mrow></mml:math></inline-formula> hPa in other seasons. The minimum ozone concentration is typically found just below the thermal tropopause. The August minimum of lower-tropospheric ozone vertically extends above <inline-formula><mml:math id="M52" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">600</mml:mn></mml:mrow></mml:math></inline-formula> hPa. This air mass is much cleaner compared to the winter ozone concentration over the lower troposphere. The dominant factor suppressing the ozone formation is long-lasting summer precipitation from early July to mid-August in 2020 (Fig. 2). The southerly wind that blows on the observation site is relatively strong compared to June and July. Therefore, we could interpret the inland polluted air masses as likely to be diluted with inflows of maritime clean air masses as mentioned above. In the lower troposphere, a minor peak of ozone concentrations is also identified in spring, which is not visible in time series plots of surface measurements (Fig. 2). The springtime peak is mainly originated by fair weather accelerating the formation of ground-level ozone with the wintertime accumulation of ozone and its processors; it could be partly attributed to the dynamical processes transporting  ozone-rich air from the UTLS and upwind areas. In Fig. 5b–f, OMI, MERRA-2, and CAMS ozone profiles are qualitatively evaluated with respect to the capability to reproduce the seasonality of ozone profiles at this location. The ozone minimum of the summer monsoon season is detected from all ozone products, but it is much broader than that in ozonesondes due to both the limited time resolution of ozonesonde measurements and the limited spatial resolution of OMI and reanalysis products. OMI also shows  very good agreement with ozonesondes in terms of reproducing the boundary layer ozone extending up to the free troposphere and the low ozone concentration below the tropopause. In addition, the vertical gradient of ozone enhancement above the tropopause is consistently reproduced from OMI, ozonesondes, and MLS. The spring ozone peak near the surface is not detectable from OMI measurements due to the limited sensitivity to relatively shallow boundary layers compared to summer (Shen et al., 2019). In Fig. 5d, an OMI a priori profile is also presented to highlight the fact that the summer minimum is derived from the independent information of OMI measurements rather than a priori information. It also illustrates that the summer minimum is a regional feature of tropospheric ozone seasonality not represented in the climatological data in which long-term global measurements are composited as a function of month and latitude.</p>
      <p id="d1e1011">Both MERRA-2 and CAMS considerably overestimate ozone abundances in both the
troposphere and stratosphere in spite of the fact that MLS measurements are commonly
employed for assimilating stratospheric ozone profiles. In MERRA-2, the
bimodal peaks (April and October) of the lower-tropospheric ozone are
inconsistent with others (early summer, September). We also compare how each
ozone product represents the tropopause against thermally defined tropopause
heights using the World Meteorological Organization (WMO) definition
(WMO, 1957). There is no universal method to define the
ozonepause height, but threshold values of 100 to 150 ppb in ozone mixing
ratios were used to discriminate stratospheric and tropospheric air masses
(e.g.,
Hsu et al., 2005; Prather et al., 2011). In this paper, the 150 ppb value is
selected due to similarities of thermal tropopauses with ozone surfaces of
150 hPa from ozonesonde measurements. As shown, the ozone surfaces at 150 ppb of reanalysis products are positioned in the free troposphere due to the
overestimation errors. Both ozonesondes and Aura measurements show some
consistency between their ozone and thermal tropopause pressures. In
particular, OMI shows strong consistency with the fact that retrievals
near the tropopause are largely constrained with the a priori state taken
from the tropopause-based ozone profile climatology
(Bak et al., 2013).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F6"><?xmltex \currentcnt{6}?><?xmltex \def\figurename{Figure}?><label>Figure 6</label><caption><p id="d1e1017">Annual variations of (top) the lower-tropospheric ozone (750–950 hPa) in August from various ozone products, along with (bottom) the wind
speeds at 850 hPa.</p></caption>
          <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://acp.copernicus.org/articles/22/14177/2022/acp-22-14177-2022-f06.png"/>

        </fig>

</sec>
<sec id="Ch1.S3.SS3">
  <label>3.3</label><title>Interannual variability of lower-tropospheric ozone in summer</title>
      <p id="d1e1034">In this section, we focus on the ozone changes related to interannual
meteorological variabilities, along with the evaluation of different ozone
products. In Fig. 6, time series of the mean ozone mixing ratio in the
lower troposphere (750–950 hPa) in August are compared. The summer monsoon
typically ends in the late July and early August over the Korean Peninsula, and hence the ozone abundance in August is sensitive to the intensity and
duration of the monsoon season. OMI and ozonesondes show a similar long-term
change, except for much more fluctuation in time series of ozonesondes due
to insufficient samplings (weekly observations) used in monthly averages. A
noticeable correlation (<inline-formula><mml:math id="M53" display="inline"><mml:mrow><mml:mi>r</mml:mi><mml:mo>=</mml:mo><mml:mo>-</mml:mo><mml:mn mathvariant="normal">0.52</mml:mn></mml:mrow></mml:math></inline-formula>) exists between wind speeds and ozone mixing ratios (ozonesonde). Low wind speed could enhance the accumulation of ozone precursors and the rate of ozone formation. Accordingly, both ozonesondes and OMI measurements detect higher ozone abundances in August from 2014 to 2017 when the wind speeds are relatively lower. As shown in Fig. 7a–c, where the monthly meteorological fields at 850 hPa in 2015 are presented from the MERRA-2 product, the western North Pacific Subtropical High (WNPSH) was broken in August, and hence the weather was likely to be calm and dry over the Korean Peninsula. Compared to the past few years, a lower amount of ozone is detected in 2020 from ozonesonde measurements. In August 2020, the lower-tropospheric southwesterly winds blow from the western North Pacific to the Korean Peninsula across the edge of the WNPSH, and the rain belt was activated over the Korean Peninsula (Fig. 7d–f). Therefore, the weather was windy and wet, suppressing ozone formation in August 2020.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F7" specific-use="star"><?xmltex \currentcnt{7}?><?xmltex \def\figurename{Figure}?><label>Figure 7</label><caption><p id="d1e1053">The monthly meteorological fields at 850 hPa for <bold>(a–c)</bold> 2015 and <bold>(d–f)</bold> 2020. The wind vectors are drawn with the orange arrows. The geopotential heights are superimposed with black lines. The variations of precipitation are shown in green shades. Note that we use MERRA-2 meteorological variables except for the precipitation data taken from the GPCP Version 2.3 Combined Precipitation Data Set (Adler et al., 2018).</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/22/14177/2022/acp-22-14177-2022-f07.png"/>

        </fig>

      <p id="d1e1068"><?xmltex \hack{\newpage}?>MERRA-2 ozone shows no annual variation before 2020, unlike other ozone
measurements and products. CAMS also shows higher ozone concentrations
correlated with wind speeds, but these are less consistent with ozonesonde
measurements compared to OMI. How the El Niño–Southern Oscillation
(ENSO) cycle interacts with the East Asian monsoon has not been established.
According to the Oceanic Niño Index, the 2015–2016 El Niño event,
the warm phase of the ENSO, was one of the strongest events ever recorded,
whereas the 2020–2021 La Niña event was also abnormally strong. There
were a lot of unprecedented weather events in South Korea during these super
El Niño and La Niña periods, such as
unprecedented summer rainfall in 2020 and unprecedented summer heatwaves in
2015–2016 (Yoon et al., 2018).
Therefore, we could relate the higher ozone amount in August 2015–2017 and
the lower ozone amount in August 2020 to a climatic forcing on the strength
and position of the WNPSH and hence the East Asian summer climate.</p>
</sec>
</sec>
<sec id="Ch1.S4" sec-type="conclusions">
  <label>4</label><title>Summary and conclusions</title>
      <p id="d1e1081">In this paper, atmospheric ozone variabilities over the Korean Peninsula and
their linkages to the East Asian summer monsoon are vertically characterized
using multiple ozone measurements made by surface observations, balloon-borne
ozonesondes, OMI, and MLS. MERRA-2 and CAMS are also integrated in this analysis for the evaluation against ozonesondes. Surface in situ measurements
at six urban sites in Pohang are averaged, while satellite and reanalysis
datasets are spatially interpolated onto the Pohang ozonesonde site. Surface
measurements clearly show the impact of frequent weather changes (dry and
wet) on ozone concentrations in spring. The seasonality of ozone becomes very complicated in late spring to early fall, depending on monsoon strengths and lengths. The peak concentration of ozone occurs in the pre-summer monsoon season (<inline-formula><mml:math id="M54" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">70</mml:mn></mml:mrow></mml:math></inline-formula> ppb) and in the post-summer monsoon season (<inline-formula><mml:math id="M55" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">50</mml:mn></mml:mrow></mml:math></inline-formula> ppb). During the summer monsoon, ozone concentrations decrease down to <inline-formula><mml:math id="M56" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">30</mml:mn></mml:mrow></mml:math></inline-formula> ppb, which is even lower than that in the winter when the air temperature and solar insolation are lowest. The vertical structures of ozone concentrations driven by stratospheric dynamics and synoptic-scale tropospheric weather disturbances are characterized from ozonesonde soundings. Stratospheric intrusions actively occur from March to May and modulate the upper-tropospheric ozone down to <?xmltex \hack{\mbox\bgroup}?><inline-formula><mml:math id="M57" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">300</mml:mn></mml:mrow></mml:math></inline-formula><?xmltex \hack{\egroup}?> hPa. We identified ozone enhancements in the boundary layer extending up to 400 hPa in June. In August monsoon-induced ozone dilution occurs in the lower troposphere up to <inline-formula><mml:math id="M58" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">600</mml:mn></mml:mrow></mml:math></inline-formula> hPa. The ozone minimum also occurs just below the tropopause, which is deepest from summer to early fall with the troposphere being extending upward to <inline-formula><mml:math id="M59" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">100</mml:mn></mml:mrow></mml:math></inline-formula> hPa. Both satellite and
reanalysis datasets show the capability to reproduce general features of
ozone seasonality such as bimodal peaks in ground-level ozone and the spring
maximum in UTLS ozone. However, MERRA-2 and CAMS products significantly
overestimate ozone abundances in the UTLS, and hence middle-tropospheric
ozone concentrations exceed 150 ppb, which is used as a chemical proxy to
distinguish between stratospheric air and tropospheric air. In general, OMI
shows  good agreement with ozonesonde measurements with respect to both
seasonal tendency and quantitative terms, but it slightly underestimates
ground-level ozone due to the limited vertical sensitivity. The lower-tropospheric ozone in August shows monsoon-induced interannual
variabilities with higher concentrations during the super El Niño and
lower concentration during the significant La Niña period, which is common from ozonesonde and OMI measurements. However, MERRA-2 rarely shows long-term changes in August ozone in the lower troposphere. On the other hand, CAMS is annually correlated with ozonesonde measurements, but with the systematic positive biases of <inline-formula><mml:math id="M60" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">40</mml:mn></mml:mrow></mml:math></inline-formula> ppb. In conclusion, OMI could play a
vital role in studying the impact of summer-monsoon-derived atmospheric
circulation and weather on ozone seasonality. The analysis results of this
study could be a useful reference for the upcoming results from the ACCLIP
campaign performed in the summer of 2022 to gather comprehensive, integrated datasets of two airborne observations (flight operations from S. Korea) as well as ground and balloon measurements over East Asia and the western Pacific. ACCLIP measurements could provide useful ideas for better understanding the spatiotemporal variation of ozone in the Korean Peninsula in terms of continuous ozone increase near the surface (Yoo et al., 2015), high ozone in the free troposphere (Crawford et al., 2021), and the relationship between stratospheric ozone intrusion and atmospheric circulation (Park et al., 2012).</p>
</sec>

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

      <p id="d1e1162">Ozonesonde data are available at <ext-link xlink:href="https://doi.org/10.14287/10000008" ext-link-type="DOI">10.14287/10000008</ext-link> (WOUDC, 2022). AirKorea data are available at <uri>https://www.airkorea.or.kr/web/pastSearch?pMENU_NO=123</uri> (NIER, 2022). ASOS: <uri>https://data.kma.go.kr/data/grnd/selectAsosRltmList.do?pgmNo=36</uri> (Korea Meteorological Administration, 2022). OMI ozone profile retrievals are attainable upon request (juseonbak@pusan.ac.kr). The MLS Version 4.2 ozone profile is available at <ext-link xlink:href="https://doi.org/10.5067/Aura/MLS/DATA2017" ext-link-type="DOI">10.5067/Aura/MLS/DATA2017</ext-link> (Schwartz et al., 2015). MERRA-2 reanalysis data are available at <ext-link xlink:href="https://doi.org/10.5067/2E096JV59PK7" ext-link-type="DOI">10.5067/2E096JV59PK7</ext-link> (GMAO, 2015). CAMS global reanalysis (EAC4) data are available at <uri>https://ads.atmosphere.copernicus.eu/</uri> (Copernicus, 2022). The GPCP Version 2.3 Combined Precipitation Data Set is available in Adler et al. (2018).</p>
  </notes><notes notes-type="authorcontribution"><title>Author contributions</title>

      <p id="d1e1187">JB and CHK designed the research; E-JS interpreted the
reanalysis products, and HJL and WJ contributed to analyzing surface
measurements. XL contributed to OMI ozone profile retrievals. CHK and JaK  provided oversight and guidance for connecting the weather
condition and air pollutant concentrations. JHK and JoK  contributed to the interpretation of the results. JB led the writing of the paper; all co-authors contributed to discussion and edited the paper.</p>
  </notes><notes notes-type="competinginterests"><title>Competing interests</title>

      <p id="d1e1193">The contact author has declared that none of the authors has any competing interests.</p>
  </notes><notes notes-type="disclaimer"><title>Disclaimer</title>

      <p id="d1e1199">Publisher's note: Copernicus Publications remains neutral with regard to jurisdictional claims in published maps and institutional affiliations.</p>
  </notes><notes notes-type="sistatement"><title>Special issue statement</title>

      <p id="d1e1205">This article is part of the special issue “Atmospheric ozone and related species in the early 2020s: latest results and trends (ACP/AMT inter-journal SI)”. It is a result of the 2021 Quadrennial Ozone Symposium (QOS) held online on 3–9 October 2021.</p>
  </notes><ack><title>Acknowledgements</title><p id="d1e1211">We thank the KMA, NIER, NASA, and Copernicus for providing their
measurements and analysis data. We hope that the 2022 ACCLIP campaign could
successfully be processed in South Korea and the research outcome would be
fascinating. We would like to acknowledge the Basic Science Research Program
(2020R1A6A1A03044834 and 2021R1A2C1004984). Research at Pukyong National University is supported by Korea Institute of Marine Science &amp; Technology Promotion (KIMST) funded by the Ministry of Oceans and Fisheries (20210605, Korea-Arctic Ocean Warming and Response of Ecosystem, KOPRI).</p></ack><notes notes-type="financialsupport"><title>Financial support</title>

      <p id="d1e1216">This research has been supported by the Basic Science Research Program through the National Research Foundation of Korea (NRF) funded by the Ministry of Education (grant nos. 2020R1A6A1A03044834 and 2021R1A2C1004984).</p>
  </notes><notes notes-type="reviewstatement"><title>Review statement</title>

      <p id="d1e1222">This paper was edited by Suvarna Fadnavis and reviewed by two anonymous referees.</p>
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