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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-21-5235-2021</article-id><title-group><article-title>COVID-19 lockdown-induced changes in NO<inline-formula><mml:math id="M1" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> levels across India observed
by multi-satellite and surface observations</article-title><alt-title>COVID-19 lockdown-induced changes in NO<inline-formula><mml:math id="M2" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> levels</alt-title>
      </title-group><?xmltex \runningtitle{COVID-19 lockdown-induced changes in NO${}_{{2}}$ levels}?><?xmltex \runningauthor{A. Biswal et al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff2">
          <name><surname>Biswal</surname><given-names>Akash</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="yes" rid="aff1">
          <name><surname>Singh</surname><given-names>Vikas</given-names></name>
          <email>vikas@narl.gov.in</email>
        <ext-link>https://orcid.org/0000-0003-1931-8409</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Singh</surname><given-names>Shweta</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Kesarkar</surname><given-names>Amit P.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0003-3218-0600</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3">
          <name><surname>Ravindra</surname><given-names>Khaiwal</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff4">
          <name><surname>Sokhi</surname><given-names>Ranjeet S.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff5 aff6">
          <name><surname>Chipperfield</surname><given-names>Martyn P.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-6803-4149</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff5 aff6">
          <name><surname>Dhomse</surname><given-names>Sandip S.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0003-3854-5383</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff5 aff6">
          <name><surname>Pope</surname><given-names>Richard J.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Singh</surname><given-names>Tanbir</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Mor</surname><given-names>Suman</given-names></name>
          
        </contrib>
        <aff id="aff1"><label>1</label><institution>National Atmospheric Research Laboratory, Gadanki, AP, India</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>Department of Environment Studies, Panjab University, Chandigarh 160014,
India</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>Department of Community Medicine and School of Public Health, Post
Graduate Institute of Medical Education and Research (PGIMER), Chandigarh
160012, India</institution>
        </aff>
        <aff id="aff4"><label>4</label><institution>Centre for Atmospheric and Climate Physics Research (CACP), University of
Hertfordshire, Hatfield, UK</institution>
        </aff>
        <aff id="aff5"><label>5</label><institution>School of Earth and Environment, University of Leeds, Leeds, UK</institution>
        </aff>
        <aff id="aff6"><label>6</label><institution>National Centre for Earth Observation, University of Leeds, Leeds, UK</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Vikas Singh (vikas@narl.gov.in)</corresp></author-notes><pub-date><day>1</day><month>April</month><year>2021</year></pub-date>
      
      <volume>21</volume>
      <issue>6</issue>
      <fpage>5235</fpage><lpage>5251</lpage>
      <history>
        <date date-type="received"><day>1</day><month>October</month><year>2020</year></date>
           <date date-type="rev-request"><day>13</day><month>October</month><year>2020</year></date>
           <date date-type="rev-recd"><day>9</day><month>February</month><year>2021</year></date>
           <date date-type="accepted"><day>2</day><month>March</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="d1e225">We have estimated the spatial changes in NO<inline-formula><mml:math id="M3" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> levels over different
regions of India during the COVID-19 lockdown (25 March–3 May 2020) using the satellite-based tropospheric column NO<inline-formula><mml:math id="M4" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> observed by
the Ozone Monitoring Instrument (OMI) and the Tropospheric Monitoring
Instrument (TROPOMI), as well as surface NO<inline-formula><mml:math id="M5" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentrations obtained
from the Central Pollution Control Board (CPCB) monitoring network. A
substantial reduction in 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> levels was observed across India during
the lockdown compared to the same period during previous business-as-usual
years, except for some regions that were influenced by anomalous fires in
2020. The reduction (negative change) over the urban agglomerations was
substantial (<inline-formula><mml:math id="M7" display="inline"><mml:mo lspace="0mm">∼</mml:mo></mml:math></inline-formula> 20 %–40 %) and directly proportional to the
urban size and population density. Rural regions across India also
experienced lower 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> values by <inline-formula><mml:math id="M9" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 15 %–25 %. Localised
enhancements in NO<inline-formula><mml:math id="M10" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> associated with isolated emission increase
scattered across India were also detected. Observed percentage changes in
satellite and surface observations were consistent across most regions and
cities, but the surface observations were subject to larger variability
depending on their proximity to the local emission sources. Observations
also indicate NO<inline-formula><mml:math id="M11" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> enhancements of up to <inline-formula><mml:math id="M12" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 25 % during
the lockdown associated with fire emissions over the north-east of India
and some parts of the central regions. In addition, the cities located near the
large fire emission sources show much smaller NO<inline-formula><mml:math id="M13" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> reduction than other
urban areas as the decrease at the surface was masked by enhancement in
NO<inline-formula><mml:math id="M14" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> due to the transport of the fire emissions.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <label>1</label><title>Introduction</title>
      <p id="d1e341">Nitrogen oxides, NO<inline-formula><mml:math id="M15" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> (NO <inline-formula><mml:math id="M16" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> NO<inline-formula><mml:math id="M17" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>), are one of the major air
pollutants, as defined by various national environmental agencies across the
world, due to their adverse impact on human health (Mills et al., 2015).
Furthermore, tropospheric levels of NO<inline-formula><mml:math id="M18" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> can affect tropospheric ozone
formation (Monks et al., 2015), contribute to secondary aerosol
formation (Lane et al., 2008) and acid deposition, and impact climatic cycles
(Lin et al., 2015). The major anthropogenic sources of NO<inline-formula><mml:math id="M19" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions
include the combustion of fossil fuels in road transport, aviation,
shipping, industries, and thermal power plants (e.g. USEPA and CATC, 1999; Ghude et
al., 2013; Hilboll et al., 2017). Other sources include open biomass burning
(OBB), mainly large-scale forest fires (e.g. Hilboll et al., 2017),
lightning (e.g. Solomon et al., 2007), and emissions from soil (e.g. Ghude
et al., 2010). NO<inline-formula><mml:math id="M20" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> hotspots are often observed over regions with large
thermal power plants and industries as well as urban areas with significant
traffic volumes causing large localised emissions (e.g. Prasad et al.,
2012; Hilboll et al., 2013; Ghude et al., 2013).</p>
      <?pagebreak page5236?><p id="d1e397">With growing scientific awareness of the adverse impacts of air
pollution, the number of air quality monitoring stations has expanded
to over 10 000 across the globe (Venter et al., 2020). Additionally,
multiple satellite instruments such as the Global Ozone Monitoring
Instrument (GOME) on ERS-2, the Scanning Imaging Absorption Spectrometer for
Atmospheric Cartography (SCIAMACHY, 2002–2012) on Envisat, the Ozone
Monitoring Instrument (OMI, 2005–present) on Aura, GOME-2 (2007–present) on
MetOp, and the TROPOspheric Monitoring Instrument (TROPOMI, 2017–present) on
Sentinel-5P (S5P) have monitored NO<inline-formula><mml:math id="M21" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> pollution from the space for over
2 decades. Surface sites typically measure NO<inline-formula><mml:math id="M22" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> in concentration
quantities (e.g. in units of <inline-formula><mml:math id="M23" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>g m<inline-formula><mml:math id="M24" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>), but satellite 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> measurements
are retrieved as integrated vertical columns (e.g. tropospheric vertical
column density, VCD<inline-formula><mml:math id="M26" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">trop</mml:mi></mml:msub></mml:math></inline-formula>). The latter is preferred for studying NO<inline-formula><mml:math id="M27" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
trends and variabilities because of global spatial coverage and
spatio-temporal coincidence with ground-based measurements (Martin et al.,
2006; Kramer et al., 2008; Lamsal et al., 2010; Ghude et al., 2011).
NO<inline-formula><mml:math id="M28" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> has been reported to increase in south Asian countries (Duncan et
al., 2016; Hilboll et al., 2017; ul-Haq et al., 2017) and decrease over Europe
(van der A et al., 2008; Curier et al., 2014; Georgoulias et al., 2019) and
the United States (Russell et al., 2012; Lamsal et al., 2015). In the case
of India, a tropospheric 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> increase was observed during the 2000s
(e.g. Mahajan et al., 2015), but since 2012 it has either stabilised or
even declined owing to the combined effect of economic slowdown and adoption
of cleaner technology (e.g. Hilboll et al., 2017). However, thermal power
plants, megacities, large urban areas, and industrial regions remain NO<inline-formula><mml:math id="M30" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
emission hotspots (Ghude et al., 2008, 2013; Prasad et al., 2012; Hilboll et
al., 2013, 2017; Duncan et al., 2016). Moreover, despite the measures taken
to control NO<inline-formula><mml:math id="M31" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions, urban areas often exceed national ambient air
quality standards in India (Sharma et al., 2013; Nori-Sarma et al., 2020;
Hama et al., 2020) and thus require a detailed scenario analysis.</p>
      <p id="d1e502">The nationwide lockdown in various countries during March–May 2020, due to
the outbreak of COVID-19, reduced traffic and industrial activities,
leading to a significant reduction of 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>. Studies using space-based
and surface observations of NO<inline-formula><mml:math id="M33" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> have reported reductions in the range
of <inline-formula><mml:math id="M34" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 30 %–60 % for China, South Korea, Malaysia, Western
Europe, and the USA (Bauwens et al., 2020; Kanniah et al., 2020; Muhammad
et al., 2020; Tobías et al., 2020; Dutheil et al., 2020; Liu et al.,
2020; Huang and Sun, 2020; Naeger and Murphy, 2020; Barré et al., 2020;
Goldberg et al., 2020) against the same period in previous years, with the
observed reductions strongly linked to the restrictions imposed on vehicular
movement. The lockdown in India was implemented in various phases starting
on the 25 March 2020 (MHA, 2020; Singh et al., 2020). The lockdown
restrictions in the first two phases (phase 1: 25 March–14 April 2020 and phase 2: 15 April–3 May 2020) were the
strictest, during which all non-essential services and offices were closed,
and the movement of the people was restricted, resulting in a considerable
reduction in the anthropogenic emissions. The restrictions were relaxed in a
phased manner from the third phase onwards in less affected areas by
permitting activities and partial movement of people (MHA, 2020).</p>
      <p id="d1e530">A decline in NO<inline-formula><mml:math id="M35" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> levels over India during the lockdown has been
reported from both surface observations (Singh et al., 2020; Sharma et al.,
2020; Mahato et al., 2020) and satellite observations (ESA, 2020;
Biswal et al., 2020; Siddiqui et al., 2020; Pathakoti et al., 2020) against
the previous year or average of a few previous years. A detailed study by
Singh et al. (2020) based on 134 sites across India reported a decline of
<inline-formula><mml:math id="M36" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 30 %–70 % in NO<inline-formula><mml:math id="M37" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> during lockdown with respect to the mean of
2017–2019, with the largest reduction being observed during peak morning
traffic hours and late evening hours. While Sharma et al. (2020) reported a
smaller decrease (18 %) in NO<inline-formula><mml:math id="M38" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> for selected sites against the levels
during 2017–2019, Mahato et al. (2020) found a decrease of over 50 % in
Delhi for the first phase of lockdown against previous years (2017–2019),
which was also confirmed by Singh et al. (2020) for the extended period of
analysis. The satellite-based studies by Biswal et al. (2020) and Pathakoti
et al. (2020) estimated the change in NO<inline-formula><mml:math id="M39" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> levels using OMI
observations, whereas Siddiqui et al. (2020) used TROPOMI to compute the
change over eight major urban centres of India. Biswal et al. (2020)
reported that the average OMI NO<inline-formula><mml:math id="M40" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> over India decreased by 12.7 %,
13.7 %, 15.9 %, and 6.1 % during the subsequent weeks of the
lockdown relative to similar periods in 2019. Similarly, Pathakoti et al. (2020) reported a decrease of 17 % in average OMI NO<inline-formula><mml:math id="M41" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> over India
compared to the pre-lockdown period and a decrease of 18 % against the
previous 5-year average. Moreover, both studies reported a larger reduction
of more than 50 % over Delhi. Similarly, Siddiqui et al. (2020) also
reported an average reduction of 46 % in the eight cities during the
first lockdown phase with respect to the pre-lockdown phase. While recent
studies have used either only satellite observations or only surface
observations, this study goes further by adopting an integrated approach by
combining both measurement types to investigate NO<inline-formula><mml:math id="M42" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> level changes over
India in response to the COVID-19 pandemic using OMI, TROPOMI, and surface
observations over different regions. As both OMI and TROPOMI have similar
local overpass times of approximately 13:30 (Penn and Holloway, 2020; van
Geffen et al., 2020), diurnal influences on the retrievals of NO<inline-formula><mml:math id="M43" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> for
both instruments are similar. Moreover, as both instruments use nearly
similar retrieval schemes (i.e. differential optical absorption
spectroscopy, DOAS), their NO<inline-formula><mml:math id="M44" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> measurements are believed to be
comparable with a suitable degree of confidence (van Geffen et al., 2020;
Wang et al., 2020). Any product differences are likely to be caused by
inconsistent inputs/processing of the retrievals (e.g. derivation of the
stratospheric slant column, the a priori tropospheric NO<inline-formula><mml:math id="M45" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> profile, and the
treatment of aerosols/clouds in the calculation of the air mass factor; van
Geffen et al., 2019; Lamsal et al., 2021).</p>
      <?pagebreak page5237?><p id="d1e632">We estimate the changes in the NO<inline-formula><mml:math id="M46" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> levels over different land-use
categories (i.e. urban, cropland, and forestland) and urban sizes. In
addition to this, we investigate the spatial agreement between population
density and NO<inline-formula><mml:math id="M47" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> spatial variability observed at the surface. A key
benefit of this study will be to understand and assess the impact of reduced
anthropogenic activity on NO<inline-formula><mml:math id="M48" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> levels, not only over the urban areas but
also over the rural areas (cropland and forestland). This study thus
provides an improved understanding of the spatial variations of tropospheric
NO<inline-formula><mml:math id="M49" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> for future air quality management in India.</p>
</sec>
<sec id="Ch1.S2">
  <label>2</label><title>Data and methodology</title>
<sec id="Ch1.S2.SS1">
  <label>2.1</label><title>Data</title>
      <p id="d1e686">Satellite observations of VCD<inline-formula><mml:math id="M50" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">trop</mml:mi></mml:msub></mml:math></inline-formula> NO<inline-formula><mml:math id="M51" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> were obtained from OMI
(2016–2020) and TROPOMI (2019–2020). Surface NO<inline-formula><mml:math id="M52" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> observations
(2016–2020) at 139 sites across India were from the Central Pollution
Control Board (CPCB). The period from 25 March to 3 May each
year is defined as the analysis period. Average NO<inline-formula><mml:math id="M53" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> levels during the
analysis period in 2020 and previous years are referred to as lockdown (LDN)
NO<inline-formula><mml:math id="M54" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and business-as-usual (BAU) NO<inline-formula><mml:math id="M55" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, respectively. The BAU years
for OMI and CPCB are 2016–2019, whereas for TROPOMI the BAU year is 2019
because of the unavailability of earlier observations.</p>
      <p id="d1e744">NO<inline-formula><mml:math id="M56" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> data were analysed for six geographical regions (north, Indo-Gangetic Plain (IGP), north-west, north-east, central, and south) of India
(Fig. S1 in the Supplement). The NO<inline-formula><mml:math id="M57" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> changes over various land-use
categories (i.e. urban, cropland, and forestland) have been analysed using
spatially collocated land-use land cover (LULC) data (NRSC, 2012) and OMI- and TROPOMI-observed VCD<inline-formula><mml:math id="M58" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">trop</mml:mi></mml:msub></mml:math></inline-formula> NO<inline-formula><mml:math id="M59" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>. Visible Infrared Imaging
Radiometer Suite (VIIRS) fire count data were used to study the fire
anomalies during the LDN and other analysis periods.</p>
<sec id="Ch1.S2.SS1.SSS1">
  <label>2.1.1</label><?xmltex \opttitle{OMI NO${}_{{2}}$}?><title>OMI NO<inline-formula><mml:math id="M60" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula></title>
      <p id="d1e799">OMI has a nadir footprint of approximately 13 km <inline-formula><mml:math id="M61" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 24 km, measuring
in the ultraviolet–visible (UV–Vis) spectral range of 270–500 nm (Boersma et
al., 2011). It uses differential optical absorption spectroscopy (DOAS) to
retrieve VCD<inline-formula><mml:math id="M62" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">trop</mml:mi></mml:msub></mml:math></inline-formula> (i.e. VCD<inline-formula><mml:math id="M63" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">trop</mml:mi></mml:msub></mml:math></inline-formula> is the difference between the
total and stratospheric slant columns divided by the tropospheric air mass
factor; Boersma et al., 2004). Here, we use the OMI NO<inline-formula><mml:math id="M64" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> 30 %
Cloud-Screened Tropospheric Column L3 Global Gridded (Version 4) at a
0.25<inline-formula><mml:math id="M65" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M66" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.25<inline-formula><mml:math id="M67" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> (<inline-formula><mml:math id="M68" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">25</mml:mn></mml:mrow></mml:math></inline-formula> km <inline-formula><mml:math id="M69" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 25 km) spatial grid from the NASA Goddard Earth Sciences Data
and Information Services Center (GESDISC), available at
(<uri>https://disc.gsfc.nasa.gov/datasets/OMNO2d_003/summary</uri>, last access: 1 January 2021).
Details of the retrieval scheme and OMI data product Version 4 are discussed
by Krotkov et al. (2019) and Lamsal et al. (2021) and for older versions
by, for example, Celarier et al. (2008) and Krotkov et al. (2017).</p>
</sec>
<sec id="Ch1.S2.SS1.SSS2">
  <label>2.1.2</label><?xmltex \opttitle{TROPOMI NO${}_{{2}}$}?><title>TROPOMI NO<inline-formula><mml:math id="M70" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula></title>
      <p id="d1e899">TROPOMI has a nadir-viewing spectral range of 270–500 nm (UV–Vis), 675–775 nm (near-infrared, NIR), and 2305–2385 nm (shortwave-infrared, SWIR). In
the UV-Vis and NIR wavelengths, TROPOMI has an unparalleled spatial
footprint of 3.5 km <inline-formula><mml:math id="M71" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 7.0 km, along with 7 km <inline-formula><mml:math id="M72" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 7 km in
the SWIR (Veefkind et al., 2012). Details of the TROPOMI scheme and data are
discussed by Eskes et al. (2019) and Van Geffen et al. (2019). The TROPOMI
VCD<inline-formula><mml:math id="M73" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">trop</mml:mi></mml:msub></mml:math></inline-formula> NO<inline-formula><mml:math id="M74" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> over India for the analysis period was obtained at 3.5 km <inline-formula><mml:math id="M75" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 7 km resolution from <uri>http://www.temis.nl/airpollution/no2.php</uri> (last access: 25 December 2020) and re-gridded at a spatial
resolution of 0.05<inline-formula><mml:math id="M76" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M77" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.05<inline-formula><mml:math id="M78" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> (<inline-formula><mml:math id="M79" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">5</mml:mn></mml:mrow></mml:math></inline-formula> km <inline-formula><mml:math id="M80" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 5 km) based on the gridding methodology of Pope et al. (2018). The source data are filtered to remove pixels with QA (quality
assurance) values greater than 50, which removes cloud fraction less than
0.2, part of the scenes covered by snow/ice, errors, and problematic
retrievals (Eskes et al., 2019).</p>
      <p id="d1e987">Although substantial differences are found between OMI and TROPOMI (such as
the differences in the orbit and spatial resolution; van Geffen et al.,
2020), they exhibit good correlation with the surface observations (Chan et
al., 2020; Wang et al., 2020) but are <inline-formula><mml:math id="M81" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">30</mml:mn></mml:mrow></mml:math></inline-formula> % lower than the
multi-axis differential optical absorption spectroscopy (MAX-DOAS)
observations. Overall, TROPOMI has been reported to be superior to OMI (van
Geffen et al., 2020). Detailed descriptions of the recent retrieval schemes
used for TROPOMI and OMI data products are provided in van Geffen et al. (2019) and Lamsal et al. (2021), respectively. Analysis of differences
between these two satellite data products is beyond the scope of this study.</p>
</sec>
<sec id="Ch1.S2.SS1.SSS3">
  <label>2.1.3</label><?xmltex \opttitle{Surface NO${}_{{2}}$ concentration}?><title>Surface NO<inline-formula><mml:math id="M82" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentration</title>
      <p id="d1e1019">The hourly averaged surface NO<inline-formula><mml:math id="M83" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentration at 139 sites (Fig. S1)
for 2016–2020 across India was acquired from the CPCB CAAQMS (Continuous
Ambient Air Quality Monitoring Stations) portal (<uri>https://app.cpcbccr.com/ccr/#/caaqm-dashboard-all/caaqm-landing</uri>, last access: 1 December 2020). The
data were further quality-controlled by removing the outliers, constant
values, and sites with less than 60 % data during the analysis period.
Details of the surface observations are explained in Singh et al. (2020).</p>
</sec>
<sec id="Ch1.S2.SS1.SSS4">
  <label>2.1.4</label><title>Land use land cover data</title>
      <p id="d1e1042">The high-resolution (50 m <inline-formula><mml:math id="M84" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 50 m) LULC data mapped with level-III
classification for 18 major categories (NRSC, 2012) were obtained from the
Bhuvan geo-platform (<uri>https://bhuvan-app1.nrsc.gov.in/thematic/thematic/index.php</uri>, last access: 3 January 2020) of the Indian
Space Research Organisation (ISRO). To quantify the changes over urban, crop,
and forest areas, the OMI and TROPOMI NO<inline-formula><mml:math id="M85" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> at urban grids<?pagebreak page5238?> (category 1),
cropland (category 2 to 5), and forestland (category 7 to 10) were extracted
for further analysis. In order to match the OMI and TROPOMI grid resolution
with the Indian LULC, the dominant LULC was considered within the OMI and
TROPOMI grid. Figure S2 shows the high-resolution LULC data used
in this study for cropland, forestland, and urban areas separately. Urban
areas were further divided into four sizes (10–50, 50–100,
100–200, and greater than 200 km<inline-formula><mml:math id="M86" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula>) to study the change in
NO<inline-formula><mml:math id="M87" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> with respect to the size of the urban agglomeration.</p>
</sec>
<sec id="Ch1.S2.SS1.SSS5">
  <label>2.1.5</label><title>VIIRS fire counts</title>
      <p id="d1e1090">The VIIRS aboard the Suomi National Polar-orbiting Partnership (S-NPP)
satellite provides daily global fire count at a 375 m <inline-formula><mml:math id="M88" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 375 m
spatial resolution (Schroeder et al., 2014; Li et al., 2018). The fire count
data over India during the analysis period from 2016 to 2020 were obtained
from the FIRMS (Fire Information for Resource Management System) web portal
(<uri>https://firms.modaps.eosdis.nasa.gov/download/</uri>, last access: 25 December 2020). The fire
count data were gridded at 5 km <inline-formula><mml:math id="M89" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 5 km for each year by summing the
fire counts falling on each spatially overlapping grid. The burnt area was
calculated from the fire counts by multiplication by the VIIRS grid size
(Prosperi et al., 2020).</p>
</sec>
<sec id="Ch1.S2.SS1.SSS6">
  <label>2.1.6</label><title>Population data</title>
      <p id="d1e1118">The gridded population density (people per hectare, pph) data for 2020 were
taken from Worldpop. (2017). Worldpop estimates the population density to be
approximately 100 m <inline-formula><mml:math id="M90" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 100 m (near the Equator) by disaggregating
census data for population mapping using a random forest estimation technique
with remotely sensed and ancillary data. Details of the population mapping
methodology can be found in Stevens et al. (2015).</p>
</sec>
<sec id="Ch1.S2.SS1.SSS7">
  <label>2.1.7</label><title>Google mobility change</title>
      <p id="d1e1136">Google estimated the change in people's movement from 15 February 2020
onwards based on Google Maps information on people's locations at places of retail
and recreation, grocery and pharmacy stores, parks, transit stations, workplaces,
and residential places, etc. The changes were estimated with reference to the
baseline days that represent a normal value for that day of the week. The
baseline day is the median value from the 5-week period 3 January–6 February 2020. The Google mobility change dataset provided an excellent proxy for the
anthropogenic activity change and has therefore been used for several
purposes of air quality studies such as lockdown emission estimation and
temporal relation with pollutant species (Archer et al., 2020; Forster et
al., 2020; Gama et al., 2020; Guevara et al., 2021) during the lockdown
period of 2020. The Google mobility data and reports are available from
Google (2020).</p>
</sec>
<sec id="Ch1.S2.SS1.SSS8">
  <label>2.1.8</label><title>Meteorological data</title>
      <p id="d1e1147">The Copernicus Climate Change Service (C3S) provides the ERA5 reanalysis
(Hersbach et al., 2020) meteorological data with an improved vertical,
temporal, and spatial coverage. The monthly mean meteorological data
(temperature, wind speed, and planetary boundary layer height) at
0.25<inline-formula><mml:math id="M91" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M92" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.25<inline-formula><mml:math id="M93" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> resolution for March, April, and
May 2016–2020 were used for the analysis. For details, see <uri>https://www.ecmwf.int/en/forecasts/datasets/reanalysis-datasets/era5</uri> (last
access: 25 January 2021).</p>
</sec>
<sec id="Ch1.S2.SS1.SSS9">
  <label>2.1.9</label><title>Analysis methodology</title>
      <p id="d1e1187">The change in the NO<inline-formula><mml:math id="M94" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> levels for each analysis period has been
calculated by subtracting the BAU NO<inline-formula><mml:math id="M95" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> from LDN NO<inline-formula><mml:math id="M96" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>. We calculate
the percentage change (<inline-formula><mml:math id="M97" display="inline"><mml:mi>D</mml:mi></mml:math></inline-formula>) using the following equation:
              <disp-formula id="Ch1.Ex1"><mml:math id="M98" display="block"><mml:mrow><mml:mi>D</mml:mi><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mo>(</mml:mo><mml:mi mathvariant="normal">LDN</mml:mi><mml:mo>-</mml:mo><mml:mi mathvariant="normal">BAU</mml:mi><mml:mo>)</mml:mo></mml:mrow><mml:mi mathvariant="normal">BAU</mml:mi></mml:mfrac></mml:mstyle><mml:mo>×</mml:mo><mml:mn mathvariant="normal">100</mml:mn><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula>
            The analysis was done over the whole of India as well as over the separately
considered regions and selected LULC categories using the open-source
geographic information system QGIS.</p>
</sec>
</sec>
</sec>
<sec id="Ch1.S3">
  <label>3</label><title>Results and discussion</title>
<sec id="Ch1.S3.SS1">
  <label>3.1</label><title>Meteorological variations</title>
      <p id="d1e1272">Air pollutant concentration over a region is governed by emission sources
and prevailing meteorological conditions. Meteorological factors (e.g. wind, temperature, radiation, and rainfall) can affect the NO<inline-formula><mml:math id="M99" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
concentration (Barré et al., 2020) as well as biogenic emissions
(Guenther et al., 2012). The meteorological variations between years can
cause <inline-formula><mml:math id="M100" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 15 % variations in monthly column NO<inline-formula><mml:math id="M101" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> values
(Goldberg et al., 2020). However, the NO<inline-formula><mml:math id="M102" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> levels are likely to be
similar under similar meteorological conditions. Recent studies (e.g. Singh
et al., 2020; Navinya et al., 2020; Sharma et al., 2020) have shown that
meteorological conditions remained relatively consistent over recent years
during the lockdown period and therefore assumed that the changes in the
pollution levels during the lockdown are primarily driven by the emission
changes. However, it is important to highlight the meteorological
differences during the study period to assess the uncertainties associated
with meteorological differences.</p>
      <?pagebreak page5239?><p id="d1e1309">We used monthly mean ERA-5 reanalysis data (Hersbach et al., 2020) at
0.25<inline-formula><mml:math id="M103" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M104" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.25<inline-formula><mml:math id="M105" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> resolution for March, April, and
May for BAU as well as LDN periods at the satellite local overpass time. We
considered temperature (<inline-formula><mml:math id="M106" display="inline"><mml:mi>T</mml:mi></mml:math></inline-formula>), wind speed (WS), and boundary layer height (BLH)
in our analysis. Figure 1a–c show the spatial variation in these
quantities during BAU (left column), LDN (middle column) and the calculated
difference (LDN<inline-formula><mml:math id="M107" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>BAU, right column). The probability density function (PDF)
using kernel density estimation (KDE) of the meteorological parameters is
also shown (Fig. S3) for the BAU (blue) and LDN (red). KDE is a
non-parametric way to estimate the PDF. The peak of the distribution shows
the most probable value, and the width of the distribution shows the
variability. The temperature difference between LDN and BAU shows a slight
reduction (<inline-formula><mml:math id="M108" display="inline"><mml:mo lspace="0mm">∼</mml:mo></mml:math></inline-formula> 0–3 K range) during the lockdown. Wind speed
values also show a reduction (up to 2 m s<inline-formula><mml:math id="M109" 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>) during the lockdown,
although the reduction is mainly seen in certain parts of central India.
Reduction in the BLH is also seen in most parts of India. In general, the
meteorological parameters during the lockdown were similar. However, the PDF
(Fig. S3) during BAU and LDN shows a small reduction (less than 5 %) in
temperature and wind speed and <inline-formula><mml:math id="M110" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 10 % reduction in BLH.
Although small, this weather variability can further add to the variability
in the NO<inline-formula><mml:math id="M111" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> levels. However, during the lockdown in India, the NO<inline-formula><mml:math id="M112" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
change was more sensitive to the emission change than the meteorology
variability. Shi et al. (2021) compared the detrended and de-weathered
change in NO<inline-formula><mml:math id="M113" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> observed over selected cities in India, Europe, China,
and the USA. While the reduction in NO<inline-formula><mml:math id="M114" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> was highest for Delhi
(<inline-formula><mml:math id="M115" display="inline"><mml:mo lspace="0mm">∼</mml:mo></mml:math></inline-formula> 50 %), the difference between a detrended and
de-weathered change in NO<inline-formula><mml:math id="M116" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> observed over Delhi was much smaller
(<inline-formula><mml:math id="M117" display="inline"><mml:mo lspace="0mm">∼</mml:mo></mml:math></inline-formula> 2 %) as compared to the difference calculated for other
cities. This suggests that weather variability did not have much impact on
NO<inline-formula><mml:math id="M118" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> levels over India and that most of the changes were driven by a change
in the anthropogenic emissions.</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="d1e1449">Spatial map showing the variation in surface meteorological parameters (<bold>a</bold> temperature, <bold>b</bold> wind speed, and <bold>c</bold> BLH) from ERA-5 by comparing BAU (left column), LDN (middle column), and observed difference (LDN <inline-formula><mml:math id="M119" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula> BAU, right column).</p></caption>
          <?xmltex \igopts{width=426.791339pt}?><graphic xlink:href="https://acp.copernicus.org/articles/21/5235/2021/acp-21-5235-2021-f01.png"/>

        </fig>

</sec>
<sec id="Ch1.S3.SS2">
  <label>3.2</label><title>Fire count anomalies during the lockdown</title>
      <p id="d1e1482">Forest fires are an important source of surface NO<inline-formula><mml:math id="M120" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and VCD<inline-formula><mml:math id="M121" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">trop</mml:mi></mml:msub></mml:math></inline-formula>
NO<inline-formula><mml:math id="M122" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> (Sahu et al., 2015; Yarragunta et al., 2020), depending on the
occurrence time and the intensity of fires (Mebust et al., 2011). Also, as
the forest fire plumes can be transported longer distances (Alonso-Blanco et
al., 2018), forest-fire-related NO<inline-formula><mml:math id="M123" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> can contribute to regional and
global air pollution. In India, forest fires are prevalent as 36 % of the
country's forest cover is prone to frequent fires, of which nearly 10 % is extremely to very highly prone to fires (ISFR, 2019). Long-term
satellite-derived fire counts suggest that Indian fire activities typically
peak during March–May (Sahu et al., 2015), predominantly over the north,
central, and north-east regions (Venkataraman et al., 2006; Ghude et al.,
2013). However, the spatial and temporal distribution of fire events is
largely heterogeneous (Sahu et al., 2015), meaning an abrupt increase or
decrease in fire activity could significantly impact NO<inline-formula><mml:math id="M124" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> levels over
anomalous regions during the lockdown.</p>
      <p id="d1e1530">An investigation of fire counts during the 2020 lockdown (LDN analysis
period), when compared with the corresponding 2016–2020 average, highlights
a substantial decrease over the eastern part of central India and an
increase over the western part of central India and the north-east. In Fig. 2a
widespread fire activity (counts of 10–50) is shown across India, such as
the central region (Madhya Pradesh, Chhattisgarh, Odisha), parts of Andhra
Pradesh, the Western Ghats in Maharashtra, and the north-east region (Assam,
Meghalaya, Tripura, Mizoram, and Manipur). The fire anomaly during the
lockdown (Fig. 2b) shows positive fire counts (5–20) over the north-east
region, west of Madhya Pradesh in central India, and scattered locations in
South India. The negative fire anomalies (<inline-formula><mml:math id="M125" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">20</mml:mn></mml:mrow></mml:math></inline-formula> to <inline-formula><mml:math id="M126" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">5</mml:mn></mml:mrow></mml:math></inline-formula>) observed over the
central region (Chhattisgarh and Odisha) suggest a decrease in fire
activity during the 2020 lockdown period. To minimise the impact of fire
emission in our analysis, we have considered the grids with zero fire
anomaly to assess the changes in NO<inline-formula><mml:math id="M127" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> during the lockdown. By
considering the grids with zero fire anomaly, we excluded almost all the
grids which have recorded fire activity during the analysis period. However,
the impact of long-range transport of forest fire plumes cannot be ignored.</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="d1e1564">Spatial distribution of the 5 km <inline-formula><mml:math id="M128" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 5 km gridded VIIRS fire
counts. <bold>(a)</bold> Average fire counts during the analysis period (25 March–3 May 2016–2020). <bold>(b)</bold> Gridded fire anomaly during the lockdown in
2020.</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/21/5235/2021/acp-21-5235-2021-f02.png"/>

        </fig>

</sec>
<sec id="Ch1.S3.SS3">
  <label>3.3</label><?xmltex \opttitle{VCD${}_{\mathrm{trop}}$ NO${}_{{2}}$ over India during lockdown period}?><title>VCD<inline-formula><mml:math id="M129" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">trop</mml:mi></mml:msub></mml:math></inline-formula> NO<inline-formula><mml:math id="M130" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> over India during lockdown period</title>
      <p id="d1e1613">The spatial distribution of VCD<inline-formula><mml:math id="M131" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">trop</mml:mi></mml:msub></mml:math></inline-formula> NO<inline-formula><mml:math id="M132" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> is largely determined by
local emission sources; therefore, NO<inline-formula><mml:math id="M133" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> hotspots are found over urban
regions, thermal power plants, and major industrial corridors. For the Indian
subcontinent, maximum NO<inline-formula><mml:math id="M134" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> is observed during winter to pre-monsoon
(December–May) and minimum NO<inline-formula><mml:math id="M135" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> during the monsoon (June–September). Region-specific
peaks such as the wintertime peak (December–January) in the IGP are associated with
anthropogenic emissions, or the summertime peak (March–April) in central India
and north-east India is associated with enhanced biomass burning activities
(Ghude et al., 2008, 2013; Hilboll et al., 2017).</p>
      <p id="d1e1661">We compare the LDN mean VCD<inline-formula><mml:math id="M136" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">trop</mml:mi></mml:msub></mml:math></inline-formula> NO<inline-formula><mml:math id="M137" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> with the BAU mean for OMI and
TROPOMI. The spatial distribution of the BAU and LDN VCD<inline-formula><mml:math id="M138" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">trop</mml:mi></mml:msub></mml:math></inline-formula> NO<inline-formula><mml:math id="M139" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
observed by OMI and TROPOMI is shown in Fig. 3a–d. The mean VCD<inline-formula><mml:math id="M140" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">trop</mml:mi></mml:msub></mml:math></inline-formula>
NO<inline-formula><mml:math id="M141" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> from the two instruments shows similar spatial distributions during
the LDN and BAU analysis period. In BAU years, the NO<inline-formula><mml:math id="M142" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> hotspots are
seen over the large fossil-fuel-based thermal power plants (<inline-formula><mml:math id="M143" display="inline"><mml:mo lspace="0mm">∼</mml:mo></mml:math></inline-formula> 1000 <inline-formula><mml:math id="M144" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<inline-formula><mml:math id="M145" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:math></inline-formula> molec. cm<inline-formula><mml:math id="M146" 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>), urban areas (<inline-formula><mml:math id="M147" display="inline"><mml:mo lspace="0mm">∼</mml:mo></mml:math></inline-formula> 400–700 <inline-formula><mml:math id="M148" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<inline-formula><mml:math id="M149" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:math></inline-formula> molec. cm<inline-formula><mml:math id="M150" 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 industrial areas.
Scattered sources are also present in western India, covering the industrial
corridor of Gujarat and Mumbai, various locations of south India, and
densely populated areas (e.g. IGP). The spatial distribution showed
significant changes during the lockdown in 2020. The details of absolute and
percentage changes are discussed in the subsequent sections.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3"><?xmltex \currentcnt{3}?><?xmltex \def\figurename{Figure}?><label>Figure 3</label><caption><p id="d1e1801">Spatial distribution of mean VCD<inline-formula><mml:math id="M151" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">trop</mml:mi></mml:msub></mml:math></inline-formula> NO<inline-formula><mml:math id="M152" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> (molec. cm<inline-formula><mml:math id="M153" 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>) during the analysis period (25 March–3 May) for
<bold>(a)</bold> OMI NO<inline-formula><mml:math id="M154" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> during business as usual (BAU, 2016–2019), <bold>(b)</bold> OMI NO<inline-formula><mml:math id="M155" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
during the lockdown (LDN, 2020), <bold>(c)</bold> TROPOMI NO<inline-formula><mml:math id="M156" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> during BAU (2019), and
<bold>(d)</bold> TROPOMI NO<inline-formula><mml:math id="M157" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> during LDN (2020).</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://acp.copernicus.org/articles/21/5235/2021/acp-21-5235-2021-f03.png"/>

        </fig>

</sec>
<sec id="Ch1.S3.SS4">
  <label>3.4</label><title>Changes observed by OMI and TROPOMI</title>
      <?pagebreak page5241?><p id="d1e1897">There is a substantial reduction in VCD<inline-formula><mml:math id="M158" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">trop</mml:mi></mml:msub></mml:math></inline-formula> NO<inline-formula><mml:math id="M159" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> between the LDN
and BAU (Fig. 4a and c). A large reduction in the number of hotspots,
mainly urban areas, is seen in both OMI and TROPOMI observations. However,
hotspots due to coal-based power plants remain during the lockdown as
electricity production was continued. Over the NO<inline-formula><mml:math id="M160" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> hotspots, there
has been an absolute decrease of over 150 <inline-formula><mml:math id="M161" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<inline-formula><mml:math id="M162" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:math></inline-formula> molec. cm<inline-formula><mml:math id="M163" 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="M164" display="inline"><mml:mo lspace="0mm">∼</mml:mo></mml:math></inline-formula> 250 <inline-formula><mml:math id="M165" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<inline-formula><mml:math id="M166" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:math></inline-formula> molec. cm<inline-formula><mml:math id="M167" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> over
megacities) detected by both OMI and TROPOMI. The rural VCD<inline-formula><mml:math id="M168" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">trop</mml:mi></mml:msub></mml:math></inline-formula>
NO<inline-formula><mml:math id="M169" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> has typically reduced by approximately 30–100 <inline-formula><mml:math id="M170" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<inline-formula><mml:math id="M171" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:math></inline-formula> molec. cm<inline-formula><mml:math id="M172" 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>, representing a percentage decrease of
30 %–50 % for OMI and 20 %–30 % for TROPOMI (Fig. 4b and d). For urban
regions, both OMI and TROPOMI see a decrease of approximately 50 %, but
reductions in smaller urban areas are clearly noticeable in the TROPOMI
data, given its better spatial resolution. Both instruments observe an
increase in VCD<inline-formula><mml:math id="M173" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">trop</mml:mi></mml:msub></mml:math></inline-formula> NO<inline-formula><mml:math id="M174" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> in the north-eastern regions and moderate
enhancement over the western and central regions. These enhancements are
linked with the biomass burning activities during this period (Fig. 2).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4"><?xmltex \currentcnt{4}?><?xmltex \def\figurename{Figure}?><label>Figure 4</label><caption><p id="d1e2058"><bold>(a, c)</bold> Absolute change and <bold>(b, d)</bold> percentage change in VCD<inline-formula><mml:math id="M175" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">trop</mml:mi></mml:msub></mml:math></inline-formula>
NO<inline-formula><mml:math id="M176" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> during the analysis period for LDN year compared to BAU years as
observed by OMI <bold>(a, b)</bold> and TROPOMI <bold>(c, d)</bold>.</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://acp.copernicus.org/articles/21/5235/2021/acp-21-5235-2021-f04.png"/>

        </fig>

<?xmltex \hack{\newpage}?>
</sec>
<sec id="Ch1.S3.SS5">
  <label>3.5</label><?xmltex \opttitle{Changes in NO${}_{{2}}$ over different land use types}?><title>Changes in NO<inline-formula><mml:math id="M177" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> over different land use types</title>
      <p id="d1e2117">Anthropogenic NO<inline-formula><mml:math id="M178" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions are typically more localised in urban and
industrial centres, while biogenic sources (e.g. soil) are more important
in rural regions. OBB activities peak in March–April (Sahu et al., 2015) and
represent more sporadic sources. As the lockdown is expected to have reduced
urban anthropogenic NO<inline-formula><mml:math id="M179" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> sources (as shown in Fig. 4), it is important
to assess the lockdown impact over the rural regions such as cropland and
forestland as well. This section estimates the changes in VCD<inline-formula><mml:math id="M180" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">trop</mml:mi></mml:msub></mml:math></inline-formula>
NO<inline-formula><mml:math id="M181" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> over different land types such as cropland, forestland, and urban
areas (Fig. S2). Industrial emissions are often part of the urban
agglomerates scattered around the city and are part of urban emissions. To
minimise the impact of OBB emissions in our analysis, we exclude grids with
fire anomalies (Fig. 2) and those containing thermal power plants (Fig. S2d). However, absolute separation of the impact of long-range
transportation is beyond the scope of this study.</p>
<sec id="Ch1.S3.SS5.SSS1">
  <label>3.5.1</label><title>Changes over cropland and forestland</title>
      <p id="d1e2163">The changes in VCD<inline-formula><mml:math id="M182" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">trop</mml:mi></mml:msub></mml:math></inline-formula> NO<inline-formula><mml:math id="M183" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> observed by OMI and TROPOMI over the
cropland (Fig. S2a) in different regions<?pagebreak page5242?> of India are shown in Fig. 5a and
b and Table S1 in the Supplement. A decline in VCD<inline-formula><mml:math id="M184" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">trop</mml:mi></mml:msub></mml:math></inline-formula> NO<inline-formula><mml:math id="M185" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> has been observed over
croplands in all regions except for the north-east. A higher percentage
decline was observed over IGP and south regions by both the satellites.
While VCD<inline-formula><mml:math id="M186" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">trop</mml:mi></mml:msub></mml:math></inline-formula> NO<inline-formula><mml:math id="M187" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> has decreased, prominent enhancements have been
observed over the north-east and few grids in central and north-west
regions. These enhancements can be attributed to the impact of nearby forest
fires (Fig. 2). The observed changes over the forestland (Fig. S2c) over
different regions of India are shown in Fig. 5c–d and Table S1.
The average VCD<inline-formula><mml:math id="M188" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">trop</mml:mi></mml:msub></mml:math></inline-formula> NO<inline-formula><mml:math id="M189" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> has declined over forestland in all the
regions except for the north-east, where VCD<inline-formula><mml:math id="M190" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">trop</mml:mi></mml:msub></mml:math></inline-formula> NO<inline-formula><mml:math id="M191" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> was enhanced
due to the positive fire anomaly (Fig. 2) during the analysis period. It can
be noted that although we have taken the grids with zero fire anomaly, the
effect of a nearby grid exhibiting positive fire anomaly cannot be ignored
due to atmospheric dispersion and mixing. The inter-comparison of the
changes observed by two satellites suggests that OMI data indicate a larger
reduction in VCD<inline-formula><mml:math id="M192" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">trop</mml:mi></mml:msub></mml:math></inline-formula> NO<inline-formula><mml:math id="M193" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> than TROPOMI in most of the regions.</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="d1e2278">Observed change in VCD<inline-formula><mml:math id="M194" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">trop</mml:mi></mml:msub></mml:math></inline-formula> NO<inline-formula><mml:math id="M195" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> between LDN and BAU from OMI
and TROPOMI for different regions shown as <bold>(a)</bold> a violin plot of the absolute
change over cropland, <bold>(b)</bold> the percentage change over cropland, <bold>(c)</bold> a violin plot
of the absolute change over forestland, and <bold>(d)</bold> the percentage change over
forestland. A violin plot is a combination of a box plot and a kernel
density estimation (KDE) plot. KDE is a non-parametric way to estimate the
probability density function (PDF). The red lines in the violin plot show
the interquartile range; the blue line shows the median value; the yellow
star shows the mean value. The vertical lines in the bar plot show the
standard deviation. The abbreviations NWest and NEast are for north-west and
north-east regions, respectively.</p></caption>
            <?xmltex \igopts{width=426.791339pt}?><graphic xlink:href="https://acp.copernicus.org/articles/21/5235/2021/acp-21-5235-2021-f05.png"/>

          </fig>

</sec>
<sec id="Ch1.S3.SS5.SSS2">
  <label>3.5.2</label><title>Changes over urban regions</title>
      <p id="d1e2326">We analysed the changes in VCD<inline-formula><mml:math id="M196" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">trop</mml:mi></mml:msub></mml:math></inline-formula> NO<inline-formula><mml:math id="M197" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> over the urban areas
(Fig. S2b) in different regions of India. The calculated actual and
percentage changes observed by OMI and TROPOMI are shown in Fig. 6 and in
Table S1. The mean changes observed by OMI and TROPOMI show similar
variations in different regions. The changes observed over urban areas are
larger than those observed over the forest and croplands. In contrast to the
cropland and forestland, TROPOMI observed a larger reduction in VCD<inline-formula><mml:math id="M198" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">trop</mml:mi></mml:msub></mml:math></inline-formula>
NO<inline-formula><mml:math id="M199" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> than OMI in most of the regions. Densely populated IGP with the
largest urban agglomeration shows the maximum change in VCD<inline-formula><mml:math id="M200" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">trop</mml:mi></mml:msub></mml:math></inline-formula>
NO<inline-formula><mml:math id="M201" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> followed by the central and north-west regions. The VCD<inline-formula><mml:math id="M202" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">trop</mml:mi></mml:msub></mml:math></inline-formula>
NO<inline-formula><mml:math id="M203" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> over the urban areas in the north-east region is likely to be
influenced by the nearby forest fires through atmospheric dispersion and
mixing, resulting in the enhancement of VCD<inline-formula><mml:math id="M204" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">trop</mml:mi></mml:msub></mml:math></inline-formula> NO<inline-formula><mml:math id="M205" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> over the urban
grids.</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="d1e2422">Observed change in VCD<inline-formula><mml:math id="M206" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">trop</mml:mi></mml:msub></mml:math></inline-formula> NO<inline-formula><mml:math id="M207" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> between LDN and BAU from OMI
and TROPOMI for different regions shown as <bold>(a)</bold> a violin plot of the absolute
change over urban areas, <bold>(b)</bold> the percentage change over the urban area, <bold>(c)</bold> a violin plot of the observed change over different sized urban areas, and <bold>(d)</bold> the percentage change over different sized urban areas.</p></caption>
            <?xmltex \igopts{width=398.338583pt}?><graphic xlink:href="https://acp.copernicus.org/articles/21/5235/2021/acp-21-5235-2021-f06.png"/>

          </fig>

      <p id="d1e2462">We have also analysed the change in the VCD<inline-formula><mml:math id="M208" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">trop</mml:mi></mml:msub></mml:math></inline-formula> NO<inline-formula><mml:math id="M209" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> over urban
areas of different sizes. We have taken the urban areas of sizes more than
10 km<inline-formula><mml:math id="M210" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula> and grouped them into four bins of size 10–50, 50–100, 100–200, and greater than 200 km<inline-formula><mml:math id="M211" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula>. We then calculate
the changes observed for all the cities filling into the respective bins.
Figure 6c–d show the absolute and percentage change in VCD<inline-formula><mml:math id="M212" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">trop</mml:mi></mml:msub></mml:math></inline-formula>
NO<inline-formula><mml:math id="M213" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, as observed by OMI and TROPOMI, respectively. A significant
reduction of 50–150 <inline-formula><mml:math id="M214" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<inline-formula><mml:math id="M215" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:math></inline-formula> molec. cm<inline-formula><mml:math id="M216" 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> (20–40 %) was observed over the urban area of different sizes. The actual
reduction in VCD<inline-formula><mml:math id="M217" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">trop</mml:mi></mml:msub></mml:math></inline-formula> NO<inline-formula><mml:math id="M218" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> is greater for the larger urban area, with
peak reductions for the urban area bin (<inline-formula><mml:math id="M219" display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">200</mml:mn></mml:mrow></mml:math></inline-formula> km<inline-formula><mml:math id="M220" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula>) for both
OMI and TROPOMI. The greater reduction in the larger urban areas is mainly
due to the reduction in local emission sources, as evidenced by the Google
mobility reduction, which is higher for larger cities than the smaller ones
(Fig. S6).</p>
</sec>
<sec id="Ch1.S3.SS5.SSS3">
  <label>3.5.3</label><title>Changes over thermal power plants</title>
      <p id="d1e2595">Thermal power plants (TPPs) are the hotspots of NO<inline-formula><mml:math id="M221" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> pollution. These
are scattered across the nation, with the majority of them in Madhya Pradesh,
Bihar, Uttar Pradesh, Odisha, Gujarat, Chhattisgarh, West Bengal, and Tamil
Nadu (Fig. S2d). During the lockdown period, TPPs were still operated to
fulfil electricity demands. In this section, we analyse the changes
observed over TPPs. The changes in VCD<inline-formula><mml:math id="M222" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">trop</mml:mi></mml:msub></mml:math></inline-formula> NO<inline-formula><mml:math id="M223" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> observed by OMI and
TROPOMI over the TPPs are shown in Fig. S5. A decrease in mean VCD<inline-formula><mml:math id="M224" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">trop</mml:mi></mml:msub></mml:math></inline-formula>
NO<inline-formula><mml:math id="M225" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> levels over TPPs has been observed that is in line with the power
sector report, which mentions that during April 2020, energy demand met for
India decreased by 24 % as compared to April 2019 (POSOCO, 2021). Also,
there is a drop (<inline-formula><mml:math id="M226" display="inline"><mml:mo lspace="0mm">∼</mml:mo></mml:math></inline-formula> 30 %) in thermal power production during
the lockdown compared to the respective period of 2019.</p>
</sec>
</sec>
<sec id="Ch1.S3.SS6">
  <label>3.6</label><title>Inter-comparison of changes observed by OMI, TROPOMI and surface observation</title>
      <p id="d1e2660">Figure 7a–b show the relationship of OMI and TROPOMI NO<inline-formula><mml:math id="M227" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> with surface
NO<inline-formula><mml:math id="M228" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> for the BAU and LDN periods, respectively. During BAU, there are
reasonable positive correlations between the satellite instruments and the
surface sites (OMI: 0.48, 95 % CI 0.33–0.60 and TROPOMI: 0.52, 95 %
CI 0.37–0.64). In LDN, these correlations drop to 0.36 (95 % CI 0.20–0.49) and 0.28 (95 % CI 0.12–0.43), respectively. The decrease in the
correlation during LDN could be due to the decrease in the signal-to-noise
ratio, potentially linked with the primary reduction in urban NO<inline-formula><mml:math id="M229" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
levels. We also determined the correlation between satellite- and
surface-observed changes during the lockdown (Fig. 7c), finding values of
0.44 (95 % CI 0.28–0.57) for OMI and 0.49 (95 % CI 0.33–0.63) for
TROPOMI. This indicates that the lockdown NO<inline-formula><mml:math id="M230" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> reductions appear to be
present in both measurement types, providing us with confidence in the
observed changes detected in this study. The correlation observed over India
in this study is lower than that reported for the USA (Lamsal et al., 2015).
The low correlation between OMI and surface NO<inline-formula><mml:math id="M231" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> has been reported
previously by Ghude et al. (2011). While they report the temporal correlation
for a single site, our study reports the spatial correlation representing
the satellites' ability to capture the spatial heterogeneity. One of the
reasons for the lower correlation could be the choice of surface station.
Generally, urban background sites are preferred for this kind of analysis.
However, the surface NO<inline-formula><mml:math id="M232" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> monitoring station type classification is not
available for the CPCB sites. Therefore, sites used in the analysis could be
potentially impacted by traffic emissions, resulting in lower correlation.
Another reason is that in situ measurements are more sensitive to the local
emission sources than remotely<?pagebreak page5243?> sensed measurements and therefore have
larger variability, resulting in low correlation. Proper classification of
the monitoring stations could provide a better assessment of satellite-based
observations.</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="d1e2720">Scatter plots between surface- and satellite-observed NO<inline-formula><mml:math id="M233" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> for <bold>(a)</bold> business as usual (BAU) and <bold>(b)</bold> lockdown (LDN). Panel <bold>(c)</bold> shows a scatter plot of observed absolute change (LDN <inline-formula><mml:math id="M234" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula> BAU) in surface and satellite NO<inline-formula><mml:math id="M235" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>. The values shown in the brackets are the correlation coefficients with 95 % confidence intervals (CIs).</p></caption>
          <?xmltex \igopts{width=441.017717pt}?><graphic xlink:href="https://acp.copernicus.org/articles/21/5235/2021/acp-21-5235-2021-f07.png"/>

        </fig>

      <?pagebreak page5244?><p id="d1e2764">The LDN NO<inline-formula><mml:math id="M236" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> percentage change, observed by surface and spatially
co-located satellite measurements, is shown in Fig. 8a for various Indian
regions. For this comparison, the number of available CPCB surface
monitoring stations was 17, 15, 81, 25, and 1 for central, north-west, IGP,
south, and north-east regions (north region data not available),
respectively. Most of the CPCB stations are in urban areas, so our results
reflect changes in predominantly urban-sourced NO<inline-formula><mml:math id="M237" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>. At all surface
sites in all regions, there was a percentage reduction greater than 20 %
(Fig. 8a). Satellite observations show a similar trend except for the
north-east region, where enhancements are due to forest fires. Both OMI and
TROPOMI observed the highest reduction (<inline-formula><mml:math id="M238" display="inline"><mml:mo lspace="0mm">∼</mml:mo></mml:math></inline-formula> 50 %) over IGP. A
smaller average reduction of <inline-formula><mml:math id="M239" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 20 % over central India
might be due to the aggregate effect of power plants, forest fires, and
prevalent biomass burning activities during this season. While the effect of
forest fires can be observed in the column NO<inline-formula><mml:math id="M240" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, its impact on the
surface NO<inline-formula><mml:math id="M241" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> is minimal. For the central, IGP, and south regions, the
mean percentage change observed by the surface monitoring station is
comparable to that observed by the satellites.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F8" specific-use="star"><?xmltex \currentcnt{8}?><?xmltex \def\figurename{Figure}?><label>Figure 8</label><caption><p id="d1e2821"><bold>(a)</bold> Box plot showing the percentage change between LDN and BAU in
NO<inline-formula><mml:math id="M242" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> levels observed by ground and satellite measurements at CPCB
monitoring locations in different regions. <bold>(b)</bold> Bar chart showing the
percentage change in NO<inline-formula><mml:math id="M243" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> levels observed in megacities in India for the
same measurements as panel <bold>(a)</bold>. The vertical line in the bar chart is the
standard deviation.</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/21/5235/2021/acp-21-5235-2021-f08.png"/>

        </fig>

      <p id="d1e2856">We have inter-compared the percentage change in NO<inline-formula><mml:math id="M244" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> observed at the
surface and satellite over the major Indian cities (i.e. New Delhi,
Chennai, Mumbai, Bangalore, Ahmedabad, Kolkata, and Hyderabad; Fig. 8b). A
significant reduction in the range of <inline-formula><mml:math id="M245" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 25 %–75 % is
observed, consistent in all observational sources used in this study. A
similar reduction observed by the satellites over the cities in other parts
of the world has been reported (Tobías et al., 2020; Naeger and Murphy,
2020; Kanniah et al., 2020; Huang and Sun, 2020). The satellites observe the
largest reduction over Delhi and the smallest over Kolkata. While the
observed decline is comparable for cities, Ahmedabad and Kolkata showed
smaller declines than observed by ground measurements. Also, the reduction
observed at the surface has a larger spatial variability than the one
observed from the space. This is potentially linked to the influence of the
local emissions which could not be detected by the space-based instruments
because of relatively large satellite footprints. The results of percentage
change observed by OMI are consistent with the change reported by Pathakoti
et al. (2020), although Siddiqui et al. (2020) reported a higher decline of
NO<inline-formula><mml:math id="M246" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> using TROPOMI. This is because we computed the changes between
lockdown and BAU during the same period of the year, whereas Siddiqui et al. (2020) estimated the changes between the pre-lockdown NO<inline-formula><mml:math id="M247" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and the
lockdown NO<inline-formula><mml:math id="M248" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, which includes the seasonal component of NO<inline-formula><mml:math id="M249" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>. We have also analysed the changes in VCD<inline-formula><mml:math id="M250" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">trop</mml:mi></mml:msub></mml:math></inline-formula> NO<inline-formula><mml:math id="M251" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> observed by
both OMI and TROPOMI for the other major cities (Guttikunda et al., 2019),
as shown in Fig. S4. A reduction of over 20 % was observed in most cities
except for a few in north-east and central India. Cities showing
enhancement or smaller reductions reflect the enhanced fire activities in
the north-east and central Indian regions. TROPOMI can capture the reduction
over the cities near the fire-prone areas (e.g. Indore and Bhopal) because
of its higher spatial resolution.</p>
</sec>
<sec id="Ch1.S3.SS7">
  <label>3.7</label><?xmltex \opttitle{Correlation of tropospheric columnar NO${}_{{2}}$ with the population density}?><title>Correlation of tropospheric columnar NO<inline-formula><mml:math id="M252" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> with the population density</title>
      <?pagebreak page5245?><p id="d1e2948">In this section, we examine the VCD<inline-formula><mml:math id="M253" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">trop</mml:mi></mml:msub></mml:math></inline-formula> NO<inline-formula><mml:math id="M254" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and population
relationship for India except where fire anomalies or large thermal power
plants existed. The scatter density plots between VCD<inline-formula><mml:math id="M255" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">trop</mml:mi></mml:msub></mml:math></inline-formula> NO<inline-formula><mml:math id="M256" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and
population density for the BAU and LDN analysis period are shown in Fig. 9
for OMI and TROPOMI. The data were log-transformed to establish the log–log
relationship as neither dataset is normally distributed. As the observed
changes had negative values, this log transformation was obtained by adding
a constant value (Ekwaru and Veugelers, 2018), which was later subtracted
when plotting to display the corresponding NO<inline-formula><mml:math id="M257" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> values. Both OMI and
TROPOMI NO<inline-formula><mml:math id="M258" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> show a similar relationship with the population density,
with correlations of <inline-formula><mml:math id="M259" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 0.65 during the LDN and BAU periods,
suggesting a strong dependence upon the population (i.e. anthropogenic
emissions). The slopes of the lines in Fig. 9a, b, d, and e show that
VCD<inline-formula><mml:math id="M260" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">trop</mml:mi></mml:msub></mml:math></inline-formula> NO<inline-formula><mml:math id="M261" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> follows a power-law scaling with population density
(Lamsal et al., 2013). During BAU, the VCD<inline-formula><mml:math id="M262" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">trop</mml:mi></mml:msub></mml:math></inline-formula> NO<inline-formula><mml:math id="M263" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> observed over a
grid increased by factors of 10<inline-formula><mml:math id="M264" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mn mathvariant="normal">0.28</mml:mn></mml:msup><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1.9</mml:mn></mml:mrow></mml:math></inline-formula> and 10<inline-formula><mml:math id="M265" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mn mathvariant="normal">0.20</mml:mn></mml:msup><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1.58</mml:mn></mml:mrow></mml:math></inline-formula>
for OMI and TROPOMI, respectively, with a 10-fold increase in the
population density. The rate of increase of the VCD<inline-formula><mml:math id="M266" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">trop</mml:mi></mml:msub></mml:math></inline-formula> NO<inline-formula><mml:math id="M267" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> during
LDN was 10<inline-formula><mml:math id="M268" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mn mathvariant="normal">0.23</mml:mn></mml:msup><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1.7</mml:mn></mml:mrow></mml:math></inline-formula> and 10<inline-formula><mml:math id="M269" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mn mathvariant="normal">0.16</mml:mn></mml:msup><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1.45</mml:mn></mml:mrow></mml:math></inline-formula> times for OMI and
TROPOMI, respectively, which was lower than BAU. The correlation during the
LDN period was marginally lower than the BAU period. This could be due to a
larger reduction in the NO<inline-formula><mml:math id="M270" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> levels in the densely populated grids. The
changes observed in the VCD<inline-formula><mml:math id="M271" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">trop</mml:mi></mml:msub></mml:math></inline-formula> NO<inline-formula><mml:math id="M272" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> during the LDN (Fig. 9c and
f) were negatively correlated (i.e. reduction was positively correlated)
with the population density. The linear relation suggests an increase in the
reduction with an increase in the population density; however, some grids
exhibit enhancements in VCD<inline-formula><mml:math id="M273" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">trop</mml:mi></mml:msub></mml:math></inline-formula> NO<inline-formula><mml:math id="M274" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> due to the local emissions.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F9" specific-use="star"><?xmltex \currentcnt{9}?><?xmltex \def\figurename{Figure}?><label>Figure 9</label><caption><p id="d1e3172">Scatter density plot between the VCD<inline-formula><mml:math id="M275" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">trop</mml:mi></mml:msub></mml:math></inline-formula> NO<inline-formula><mml:math id="M276" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> (<inline-formula><mml:math id="M277" display="inline"><mml:mrow><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> molec. cm<inline-formula><mml:math id="M278" 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 population density (pph) for the analysis period in different years. <bold>(a)</bold> Business as usual (BAU, 2016–2019) observed by OMI; <bold>(b)</bold> lockdown (LDN, 2020) observed by OMI; <bold>(c)</bold> changes (LDN <inline-formula><mml:math id="M279" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula> BAU) observed by OMI; <bold>(d)</bold> BAU (2019) observed by TROPOMI; <bold>(e)</bold> LDN (2020) observed by TROPOMI; <bold>(f)</bold> LND-BAU changes observed by TROPOMI. The linear best fit lines show the log–log relationship between VCD<inline-formula><mml:math id="M280" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">trop</mml:mi></mml:msub></mml:math></inline-formula> NO<inline-formula><mml:math id="M281" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> (<inline-formula><mml:math id="M282" display="inline"><mml:mi>Y</mml:mi></mml:math></inline-formula>) and population density (<inline-formula><mml:math id="M283" display="inline"><mml:mi>X</mml:mi></mml:math></inline-formula>) given by equation <inline-formula><mml:math id="M284" display="inline"><mml:mrow><mml:mi>y</mml:mi><mml:mo>=</mml:mo><mml:mi mathvariant="italic">β</mml:mi><mml:mo>⋅</mml:mo><mml:mi>x</mml:mi><mml:mo>+</mml:mo><mml:mi>c</mml:mi></mml:mrow></mml:math></inline-formula>, where <inline-formula><mml:math id="M285" display="inline"><mml:mrow><mml:mi>y</mml:mi><mml:mo>=</mml:mo><mml:mi>log⁡</mml:mi><mml:mo>(</mml:mo><mml:mi>Y</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M286" display="inline"><mml:mrow><mml:mi>x</mml:mi><mml:mo>=</mml:mo><mml:mi>log⁡</mml:mi><mml:mo>(</mml:mo><mml:mi>X</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M287" display="inline"><mml:mrow><mml:mi>c</mml:mi><mml:mo>=</mml:mo><mml:mi>log⁡</mml:mi><mml:mo>(</mml:mo><mml:mi>C</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>. Therefore, the equation can be written as <inline-formula><mml:math id="M288" display="inline"><mml:mrow><mml:mi>log⁡</mml:mi><mml:mo>(</mml:mo><mml:mi>Y</mml:mi><mml:mo>)</mml:mo><mml:mo>=</mml:mo><mml:mi mathvariant="italic">β</mml:mi><mml:mo>⋅</mml:mo><mml:mi>log⁡</mml:mi><mml:mo>(</mml:mo><mml:mi>X</mml:mi><mml:mo>)</mml:mo><mml:mo>+</mml:mo><mml:mi>log⁡</mml:mi><mml:mo>(</mml:mo><mml:mi>C</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> or <inline-formula><mml:math id="M289" display="inline"><mml:mrow><mml:mi>Y</mml:mi><mml:mo>=</mml:mo><mml:mi>C</mml:mi><mml:mo>⋅</mml:mo><mml:msup><mml:mi>X</mml:mi><mml:mi mathvariant="italic">β</mml:mi></mml:msup></mml:mrow></mml:math></inline-formula>, where <inline-formula><mml:math id="M290" display="inline"><mml:mi mathvariant="italic">β</mml:mi></mml:math></inline-formula> is the slope of the line.</p></caption>
          <?xmltex \igopts{width=384.112205pt}?><graphic xlink:href="https://acp.copernicus.org/articles/21/5235/2021/acp-21-5235-2021-f09.png"/>

        </fig>

</sec>
<sec id="Ch1.S3.SS8">
  <label>3.8</label><?xmltex \opttitle{Linking the mobility change with NO${}_{{2}}$ change}?><title>Linking the mobility change with NO<inline-formula><mml:math id="M291" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> change</title>
      <p id="d1e3441">In order to link the observed reduction in NO<inline-formula><mml:math id="M292" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> levels with the traffic
emissions over the urban areas, Fig. 10 shows the 7 d moving average
of the daily percentage change observed by OMI, TROPOMI, and CPCB across
urban India from 1 March to 31 May 2020 against the
Google mobility percentage reduction for three mobility categories: transit
stations, workplace, and residential. Transit stations and workplace, proxies
for traffic emissions (Forster et al., 2020), show a sharp decline
(<inline-formula><mml:math id="M293" display="inline"><mml:mo lspace="0mm">∼</mml:mo></mml:math></inline-formula> 70 %) due to the lockdown. The signatures of reduced
traffic can be seen even before the start of lockdown in mid-March 2020. The
decrease in the workplaces resulted in the enhancement (25 %–30 %) of people at a residential location. The percentage reductions observed by
satellites and surface monitoring are consistent with each other and follow
the same trend of the workplaces and transit stations. The reductions
observed by satellites and surface monitoring are <inline-formula><mml:math id="M294" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 20 %
lower than the reductions in workplaces and transit stations, which are
compensated for by the enhancement in residential emissions. Surface (CPCB)
measurements exhibit higher correlation (<inline-formula><mml:math id="M295" display="inline"><mml:mo lspace="0mm">∼</mml:mo></mml:math></inline-formula> 0.9 and 0.8, with
and without moving average) with the mobility reduction compared to the
satellite observation, which has a relatively weaker correlation
(<inline-formula><mml:math id="M296" display="inline"><mml:mo lspace="0mm">∼</mml:mo></mml:math></inline-formula> 0.8 and 0.5). The positive correlation of NO<inline-formula><mml:math id="M297" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
reduction with workplaces and transit stations suggests that the reduction
observed over the urban areas was linked with reduced traffic emissions due
to travel restrictions for COVID-19 containment. Moreover, the mobility
reduction was higher for larger cities as compared to the smaller ones (Fig. S6).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F10" specific-use="star"><?xmltex \currentcnt{10}?><?xmltex \def\figurename{Figure}?><label>Figure 10</label><caption><p id="d1e3493">Temporal evolution of estimated change (7 d rolling mean) of
satellite-observed VCD<inline-formula><mml:math id="M298" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">trop</mml:mi></mml:msub></mml:math></inline-formula> NO<inline-formula><mml:math id="M299" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and surface-measured NO<inline-formula><mml:math id="M300" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> for the
period 1 March–31 May 2020 from the baseline.</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/21/5235/2021/acp-21-5235-2021-f10.png"/>

        </fig>

</sec>
<sec id="Ch1.S3.SS9">
  <label>3.9</label><title>Limitations of this study</title>
      <p id="d1e3537">This study has few limitations that need to be considered while interpreting
the results. The observed changes in the NO<inline-formula><mml:math id="M301" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> levels are the combined
effect of changes in the emissions, local meteorology, large-scale dynamics,
and non-linear chemistry. The variability in NO<inline-formula><mml:math id="M302" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, caused by weather
patterns and non-linear chemistry is not included in the present work. Our
study does not distinguish the differences in the upwind and downwind
transport of plumes originating from urban areas and thermal power plants.
Moreover, the estimates can be biased by the forest-fire plumes, which can
be transported over a long distance. These limitations warrant a detailed
modelling study to quantify the impact of long-range transport of plumes in
the drastic reduction of urban emissions. One of the limitations arises due
to the unavailability of the surface monitoring classification according to
its location and vicinity of the local sources, which restricted a proper
assessment of the space-based NO<inline-formula><mml:math id="M303" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> observation. To overcome this
limitation, proper classification of the monitoring stations (Geiger et al.,
2013) based on the environment type and vicinity of the sources will be
helpful in air quality assessment.</p>
</sec>
</sec>
<sec id="Ch1.S4" sec-type="conclusions">
  <label>4</label><title>Conclusions and discussion</title>
      <p id="d1e3576">The changes in NO<inline-formula><mml:math id="M304" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> levels over India during the COVID-19 lockdown
(25 March–3 May 2020) have been studied using satellite-based
VCD<inline-formula><mml:math id="M305" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">trop</mml:mi></mml:msub></mml:math></inline-formula> NO<inline-formula><mml:math id="M306" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> observed by OMI and TROPOMI and surface NO<inline-formula><mml:math id="M307" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
concentrations obtained from CPCB. The changes between lockdown (LDN) and
the same period during business-as-usual (BAU) years have been estimated
over different land-use categories (e.g. urban, cropland, and forestland)
across six geographical regions of<?pagebreak page5246?> India. Also, the changes observed from
space and at the surface have been inter-compared, and the correlation with
the population density has been studied.</p>
      <?pagebreak page5247?><p id="d1e3615">Overall, a significant reduction in NO<inline-formula><mml:math id="M308" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> levels of up to <inline-formula><mml:math id="M309" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 70 % was observed over India during the lockdown compared to the same
period during BAU. The usual prominent NO<inline-formula><mml:math id="M310" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> hotspots observed by OMI and
TROPOMI over urban agglomerations during BAU were barely noticeable during
the lockdown. However, despite the reduction in electricity production, the
coal-based thermal power plants continued to be major NO<inline-formula><mml:math id="M311" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> hotspots
during the lockdown. Some of the largest reductions in NO<inline-formula><mml:math id="M312" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> were
observed to be over the urban areas of the IGP region. The reduction
observed for urban agglomerations was over 150 <inline-formula><mml:math id="M313" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<inline-formula><mml:math id="M314" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:math></inline-formula> molec. cm<inline-formula><mml:math id="M315" 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="M316" display="inline"><mml:mo lspace="0mm">∼</mml:mo></mml:math></inline-formula> 30 %) and even more for megacities
showing a reduction of around 250 <inline-formula><mml:math id="M317" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<inline-formula><mml:math id="M318" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:math></inline-formula> molec. cm<inline-formula><mml:math id="M319" 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>
(50 %). The reduction observed over the urban areas was linked with
reduced traffic emissions due to travel restrictions for COVID-19 containment.
The decrease was also observed over rural regions. Average declines of
NO<inline-formula><mml:math id="M320" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> in the ranges of 14 %–30 %, 8 %–28 %, and 10 %–24 % were observed
by OMI, and 22 %–27 %, 6 %–18 %, and 3 %–21 % were observed by TROPOMI over
the urban, cropland, and forestland, respectively, in different regions of
India. In contrast, an average enhancement over north-east India was
observed due to positive fire anomalies during the lockdown. Although we
have considered the grids with zero fire anomaly during the lockdown, the
fire emissions can still enhance NO<inline-formula><mml:math id="M321" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> levels over grids with no fire
activity because of horizontal transport.</p>
      <p id="d1e3744">The observed changes in VCD<inline-formula><mml:math id="M322" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">trop</mml:mi></mml:msub></mml:math></inline-formula> NO<inline-formula><mml:math id="M323" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> were found to be spatially
positively correlated with surface NO<inline-formula><mml:math id="M324" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentrations, indicating that
the lockdown NO<inline-formula><mml:math id="M325" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> changes appear to be present in both measurement
types. The TROPOMI NO<inline-formula><mml:math id="M326" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> showed a better correlation with surface
NO<inline-formula><mml:math id="M327" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and was more sensitive to the changes than the OMI because of the
finer resolution. Therefore, TROPOMI can provide a better estimate of
NO<inline-formula><mml:math id="M328" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> associated with fine-scale heterogeneous emissions. Also,
VCD<inline-formula><mml:math id="M329" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">trop</mml:mi></mml:msub></mml:math></inline-formula> NO<inline-formula><mml:math id="M330" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> was found to exhibit a good correlation with the
population density, suggesting a strong dependence on the anthropogenic emissions. The changes observed in the VCD<inline-formula><mml:math id="M331" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">trop</mml:mi></mml:msub></mml:math></inline-formula>
NO<inline-formula><mml:math id="M332" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> during the lockdown were negatively correlated (i.e. reduction was
positively correlated), with the population density suggesting a larger
reduction for the densely populated cities. However, the influence of local
emissions can be different in different cities.</p>
      <p id="d1e3847">The analysis presented in this work shows a significant change in NO<inline-formula><mml:math id="M333" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
levels across India. The observed reductions can be linked with the control
measures taken to prevent the spread of the COVID-19 that restricted
people's movement, resulting in a significant reduction in anthropogenic
emissions. As an important message to policymakers, this study indicates the
level of decrease in NO<inline-formula><mml:math id="M334" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> that is possible if dramatic reductions in key
emission sectors such as road traffic were incorporated into air quality
management strategies.</p>
</sec>

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

      <p id="d1e3873">OMI data are available at the NASA Goddard Earth Sciences Data and Information Services Center (GESDISC) (<uri>https://disc.gsfc.nasa.gov/datasets/OMNO2d_003/summary</uri>, GESDISC, 2021). TROPOMI data are obtained from (<uri>http://www.temis.nl/airpollution/no2.php</uri>,  TEMIS, 2020). Surface measured NO<inline-formula><mml:math id="M335" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> data across India are available at CPCB site (<uri>https://app.cpcbccr.com/ccr/</uri>, CPCB, 2020). VIIRS fire count data are available at the FIRMS web portal (<uri>https://firms.modaps.eosdis.nasa.gov/</uri>, FIRMS, 2020). India Population data used in this study are available at the <uri>https://www.worldpop.org/</uri> (<ext-link xlink:href="https://doi.org/10.5258/SOTON/WP00532" ext-link-type="DOI">10.5258/SOTON/WP00532</ext-link>, WorldPop., 2017). The LULC data for India are available at the Bhuvan, (<uri>https://bhuvan.nrsc.gov.in</uri>, Bhuvan, 2020) Indian Geo-Platform of Indian Space Research Organisation. ERA5 meteorology data are available at CDC (<uri>https://cds.climate.copernicus.eu/cdsapp</uri>, CDC, 2021). The mobility data are available on Google platform (<uri>https://www.google.com/covid19/mobility</uri>, Google, 2020).</p>
  </notes><app-group>
        <supplementary-material position="anchor"><p id="d1e3913">The supplement related to this article is available online at: <inline-supplementary-material xlink:href="https://doi.org/10.5194/acp-21-5235-2021-supplement" xlink:title="pdf">https://doi.org/10.5194/acp-21-5235-2021-supplement</inline-supplementary-material>.</p></supplementary-material>
        </app-group><notes notes-type="authorcontribution"><title>Author contributions</title>

      <p id="d1e3922">AB and VS conceived the study, analysed the data and interpreted the results with SS. MPC, SSD, RJP provided the processed TROPOMI data and provided useful discussion on satellite products. APK, KR, RSS, MPC, SSD, RJP, TS, SM provided useful discussion on the results. AB, VS, SS wrote the first draft and finalised the paper with input from all co-authors.</p>
  </notes><notes notes-type="competinginterests"><title>Competing interests</title>

      <p id="d1e3928">The authors declare that they have no conflict of interest.</p>
  </notes><ack><title>Acknowledgements</title><p id="d1e3934">The authors are thankful to the director, National Atmospheric Research
Laboratory (NARL, India), for encouragement to conduct this research and
provision of the necessary support. Akash Biswal and Shweta Singh greatly acknowledge the Ministry of
Earth Sciences (MoES, India) for the research fellowship. We acknowledge and
thank Central Pollution Control Board (CPCB), Ministry of Environment,
Forest and Climate Change (MoEFCC, India) for making air quality
data publicly available. We acknowledge Bhuvan, Indian Geo-Platform of Indian Space
Research Organisation (ISRO), National Remote Sensing Centre (NRSC), for
providing high-resolution LULC data. The authors gratefully acknowledge OMI,
TROPOMI, and ERA5 science teams for making data publicly available. We also
acknowledge the NASA Goddard Earth Sciences Data and Information Services
Center, Tropospheric Emission Monitoring Internet Service and Climate Data
Store. We also acknowledge Google community mobility data and report. We
acknowledge support from the Air Pollution and Human Health for an Indian
Megacity project PROMOTE funded by UK NERC and the Indian MOES (grant no. NE/P016391/1).</p></ack><notes notes-type="financialsupport"><title>Financial support</title>

      <p id="d1e3939">This research has been supported by the Natural Environment Research Council, UK (grant no. NE/P016391/1), and the Ministry of Earth Sciences, India.</p>
  </notes><notes notes-type="reviewstatement"><title>Review statement</title>

      <p id="d1e3945">This paper was edited by Andreas Hofzumahaus and reviewed by two anonymous referees.</p>
  </notes><ref-list>
    <title>References</title>

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    <!--<article-title-html>COVID-19 lockdown-induced changes in NO<sub>2</sub> levels across India observed by multi-satellite and surface observations</article-title-html>
<abstract-html><p>We have estimated the spatial changes in NO<sub>2</sub> levels over different
regions of India during the COVID-19 lockdown (25 March–3 May 2020) using the satellite-based tropospheric column NO<sub>2</sub> observed by
the Ozone Monitoring Instrument (OMI) and the Tropospheric Monitoring
Instrument (TROPOMI), as well as surface NO<sub>2</sub> concentrations obtained
from the Central Pollution Control Board (CPCB) monitoring network. A
substantial reduction in NO<sub>2</sub> levels was observed across India during
the lockdown compared to the same period during previous business-as-usual
years, except for some regions that were influenced by anomalous fires in
2020. The reduction (negative change) over the urban agglomerations was
substantial ( ∼ &thinsp;20&thinsp;%–40&thinsp;%) and directly proportional to the
urban size and population density. Rural regions across India also
experienced lower NO<sub>2</sub> values by  ∼ &thinsp;15&thinsp;%–25&thinsp;%. Localised
enhancements in NO<sub>2</sub> associated with isolated emission increase
scattered across India were also detected. Observed percentage changes in
satellite and surface observations were consistent across most regions and
cities, but the surface observations were subject to larger variability
depending on their proximity to the local emission sources. Observations
also indicate NO<sub>2</sub> enhancements of up to  ∼ &thinsp;25&thinsp;% during
the lockdown associated with fire emissions over the north-east of India
and some parts of the central regions. In addition, the cities located near the
large fire emission sources show much smaller NO<sub>2</sub> reduction than other
urban areas as the decrease at the surface was masked by enhancement in
NO<sub>2</sub> due to the transport of the fire emissions.</p></abstract-html>
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