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<!DOCTYPE article PUBLIC "-//NLM//DTD Journal Publishing with OASIS Tables v3.0 20080202//EN" "journalpub-oasis3.dtd">
<article xmlns:xlink="http://www.w3.org/1999/xlink" xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:oasis="http://docs.oasis-open.org/ns/oasis-exchange/table" xml:lang="en" dtd-version="3.0" article-type="research-article"><?xmltex \bartext{Research article}?>
  <front>
    <journal-meta><journal-id journal-id-type="publisher">ACP</journal-id><journal-title-group>
    <journal-title>Atmospheric Chemistry and Physics</journal-title>
    <abbrev-journal-title abbrev-type="publisher">ACP</abbrev-journal-title><abbrev-journal-title abbrev-type="nlm-ta">Atmos. Chem. Phys.</abbrev-journal-title>
  </journal-title-group><issn pub-type="epub">1680-7324</issn><publisher>
    <publisher-name>Copernicus Publications</publisher-name>
    <publisher-loc>Göttingen, Germany</publisher-loc>
  </publisher></journal-meta>
    <article-meta>
      <article-id pub-id-type="doi">10.5194/acp-22-8617-2022</article-id><title-group><article-title>Improving NO<inline-formula><mml:math id="M1" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emission estimates in Beijing using network observations and a perturbed<?xmltex \hack{\break}?> emissions ensemble</article-title><alt-title>Improving emission estimates using network observations and a PEE​​​​​​​</alt-title>
      </title-group><?xmltex \runningtitle{Improving emission estimates using network observations and a PEE​​​​​​​}?><?xmltex \runningauthor{L. Yuan et al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Yuan</surname><given-names>Le</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-4282-0459</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Popoola</surname><given-names>Olalekan A. M.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0003-2390-8436</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Hood</surname><given-names>Christina</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-9244-5696</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Carruthers</surname><given-names>David</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Jones</surname><given-names>Roderic L.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Sun</surname><given-names>Haitong Zhe</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3">
          <name><surname>Liu</surname><given-names>Huan</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff4">
          <name><surname>Zhang</surname><given-names>Qiang</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="yes" rid="aff1 aff5">
          <name><surname>Archibald</surname><given-names>Alexander T.</given-names></name>
          <email>ata27@cam.ac.uk</email>
        <ext-link>https://orcid.org/0000-0001-9302-4180</ext-link></contrib>
        <aff id="aff1"><label>1</label><institution>Yusuf Hamied Department of Chemistry, University of Cambridge,
Cambridge, CB2 1EW, UK</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>Cambridge Environmental Research Consultants, Cambridge, CB2 1SJ, UK</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>State Key Joint Laboratory of ESPC, State Environmental Protection Key Laboratory of Sources and Control of Air Pollution Complex, International
Joint Laboratory on Low Carbon Clean Energy Innovation,<?xmltex \hack{\break}?> School of the Environment, Tsinghua University, Beijing, 100084, China</institution>
        </aff>
        <aff id="aff4"><label>4</label><institution>Ministry of Education Key Laboratory for Earth System Modeling,
Department of Earth System Science, Tsinghua University, Beijing, 100084,
China</institution>
        </aff>
        <aff id="aff5"><label>5</label><institution>National Centre for Atmospheric Science, Cambridge, CB2 1EW, UK</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Alexander T. Archibald (ata27@cam.ac.uk)</corresp></author-notes><pub-date><day>5</day><month>July</month><year>2022</year></pub-date>
      
      <volume>22</volume>
      <issue>13</issue>
      <fpage>8617</fpage><lpage>8637</lpage>
      <history>
        <date date-type="received"><day>27</day><month>February</month><year>2022</year></date>
           <date date-type="rev-request"><day>9</day><month>March</month><year>2022</year></date>
           <date date-type="rev-recd"><day>8</day><month>June</month><year>2022</year></date>
           <date date-type="accepted"><day>13</day><month>June</month><year>2022</year></date>
      </history>
      <permissions>
        <copyright-statement>Copyright: © 2022 </copyright-statement>
        <copyright-year>2022</copyright-year>
      <license license-type="open-access"><license-p>This work is licensed under the Creative Commons Attribution 4.0 International License. To view a copy of this licence, visit <ext-link ext-link-type="uri" xlink:href="https://creativecommons.org/licenses/by/4.0/">https://creativecommons.org/licenses/by/4.0/</ext-link></license-p></license></permissions><self-uri xlink:href="https://acp.copernicus.org/articles/.html">This article is available from https://acp.copernicus.org/articles/.html</self-uri><self-uri xlink:href="https://acp.copernicus.org/articles/.pdf">The full text article is available as a PDF file from https://acp.copernicus.org/articles/.pdf</self-uri>
      <abstract><title>Abstract</title>

      <p id="d1e196">Emissions inventories are crucial inputs to air quality
simulations and represent a major source of uncertainty. Various methods
have been adopted to optimise emissions inventories, yet in most cases the
methods were only applied to total anthropogenic emissions. We have
developed a new approach that updates a priori emission estimates by source sector, which are particularly relevant for policy interventions. At its core is a perturbed emissions ensemble (PEE), constructed by perturbing parameters in an a priori emissions inventory within their respective uncertainty ranges. This PEE is then input to an air quality model to generate an ensemble of forward simulations. By comparing the simulation outputs with observations from a dense network, the initial uncertainty ranges are constrained, and a posteriori emission estimates are derived. Using this approach, we were able to derive the transport sector NO<inline-formula><mml:math id="M2" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions for a study area centred around Beijing in 2016 based on a priori emission estimates for 2013. The absolute emissions were
found to be 1.5–9 <inline-formula><mml:math id="M3" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<inline-formula><mml:math id="M4" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msup></mml:math></inline-formula> Mg, corresponding to a 57 %–93 % reduction from the 2013 levels, yet the night-time fraction of the emissions was 67 %–178 % higher. These results provide robust and independent evidence
of the trends of traffic emission in the study area between 2013 and 2016
reported by previous studies. We also highlighted the impacts of the
chemical mechanisms in the underlying model on the emission estimates
derived, which is often neglected in emission optimisation studies. This
work paves forward the route for rapid analysis and update of emissions
inventories using air quality models and routine in situ observations, underscoring the utility of dense observational networks. It also highlights some gaps in the current distribution of monitoring sites in Beijing which result in an underrepresentation of large point sources of NO<inline-formula><mml:math id="M5" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <label>1</label><title>Introduction</title>
      <p id="d1e242">Nitrogen dioxide (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>) is an important atmospheric trace gas whose
adverse health impacts have been extensively studied. Controlled human
exposure experiments have shown associations between short-term exposure to
very high levels of NO<inline-formula><mml:math id="M7" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and airway inflammation
(Blomberg et al., 1999), increased bronchial reactivity
(Folinsbee, 1992), increased susceptibility to respiratory virus infections
(Goings et al., 1989), etc. Chronic exposure to lower doses of 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> (e.g. those currently observed in Europe and North America) has also been linked to
lower lung function and deficits in lung function growth among children
(Gauderman et al., 2000; Peters et al., 1999), chronic respiratory symptoms
(Zemp et al., 1999) and increased cardiopulmonary mortality
(Hoek et al., 2002) among adults in epidemiological studies. A key challenge for these epidemiological studies is to separate out the health effects due to NO<inline-formula><mml:math id="M9" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> exposure from those due to exposure to other pollutants, whose
concentrations are often highly correlated with those of 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>.</p>
      <p id="d1e290">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> belongs to the highly reactive group of nitrogen oxides (NO<inline-formula><mml:math id="M12" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>),
whose emissions occur primarily in the form of nitric oxide (NO) with a
small proportion of 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> (i.e. NO<inline-formula><mml:math id="M14" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub><mml:mspace linebreak="nobreak" width="0.125em"/></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M15" display="inline"><mml:mo>=</mml:mo></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>). NO is
quickly oxidised by ozone (O<inline-formula><mml:math id="M18" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>) to NO<inline-formula><mml:math id="M19" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, which, in daylight hours,
rapidly photolyses to reform NO and (via O(<inline-formula><mml:math id="M20" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:math></inline-formula>P)) O<inline-formula><mml:math id="M21" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>. Thus, during
daytime, NO, 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> and O<inline-formula><mml:math id="M23" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> reach a photostationary state, typically
on the timescale of a few minutes (Leighton, 1961). The presence of
volatile organic compounds (VOCs) perturbs this null cycle by producing
hydroperoxyl radicals (HO<inline-formula><mml:math id="M24" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>) and organic peroxy radicals (RO<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>) which
oxidise NO without consuming O<inline-formula><mml:math id="M26" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>, leading to faster NO-to-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>
conversion and net O<inline-formula><mml:math id="M28" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> production. This results in a non-linear response
of O<inline-formula><mml:math id="M29" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> concentrations to reductions in the emissions of NO<inline-formula><mml:math id="M30" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> and
VOCs (Seinfeld and Pandis, 2016). It is therefore crucial to
have accurate emission estimates for developing effective and synergetic
control strategies for these interdependent pollutants
(Cohan et al., 2005).</p>
      <p id="d1e474">NO<inline-formula><mml:math id="M31" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> can be produced from both anthropogenic and natural/biogenic
sources such as fossil fuel combustion, biomass burning, soil microbial
processes and lightning (Lee
et al., 1997). Global total anthropogenic NO<inline-formula><mml:math id="M32" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions flattened
around 2008, as reductions in Europe and North America were offset by
increases in Asia (Hoesly et al.,
2018). China, in particular, witnessed a rapid rise in anthropogenic
NO<inline-formula><mml:math id="M33" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions until 2011–2012 (with the exceptions of a few regions
where the emissions peaked earlier), which resulted from economic growth
along with an absence of regulations (van
der A et al., 2017; Liu et al., 2016; Zheng et al., 2018). Emission
reduction targets were first announced in the 12th Five-Year Plan
(2011–2015) (People's Republic of China, 2011), followed by the
Action Plan on Prevention and Control of Air Pollution (2013–2017)
(State Council of the People's Republic of China, 2013) and the
Three-Year Action Plan for Winning the Blue Sky Defence Battle (2018–2020)
(State Council of the People's Republic of China, 2018). The
main measures implemented included the installation of selective catalytic
reduction equipment in power-generating and industrial facilities and the
implementation of stricter vehicle emission standards combined with
accelerated fleet turnover (Liu
et al., 2020). Decreases in anthropogenic sources are accompanied by an
increased importance of soil NO<inline-formula><mml:math id="M34" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions, which are largely driven by
nitrogen fertiliser application and can reach up to 20 % of the
anthropogenic emissions in the crop-growing season in some regions with high
agricultural activities (Lu et al., 2021). These
emissions are relatively poorly quantified and currently unabated
(State Council of the People's Republic of China, 2018).</p>
      <p id="d1e513">Numerous studies have quantified China's NO<inline-formula><mml:math id="M35" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions and evaluated
the short- or long-term trends in emissions. Some have used a bottom-up
method that combines specific emission factors (i.e. mass of a pollutant
emitted per unit fuel consumption or industrial production) with the
corresponding activity rates (i.e. fuel consumption or industrial
production), thus providing sector- or process-resolved emission estimates
(Liu et al., 2016; Zhang et al., 2009; Zhao et al., 2013; Zheng et al., 2018). However, the underlying data are mostly not immediately available, resulting in an inevitable time lag between the occurrence of emissions and the establishment of an inventory (Janssens-Maenhout
et al., 2015). Moreover, they can introduce potentially large and poorly
quantified uncertainties into the emission estimates (Hong
et al., 2017; Zhao et al., 2011), which can be further propagated through
modelled pollutant concentrations into disease or mortality burden
(Crippa et al., 2019) and economic loss estimates (Solazzo et al., 2018).
Other studies have inferred top-down estimates of emissions using satellite
observations (Ding
et al., 2020; Lin et al., 2010; Qu et al., 2017; Zhang et al., 2012). This
method requires tropospheric column densities of NO<inline-formula><mml:math id="M36" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, which are
retrieved by transforming slant column densities to vertical column
densities, removing the stratospheric contribution and correcting for the
effects of albedo, cloud and aerosols (Leue et al., 2001). Earlier studies
used a mass balance approach that assumes a linear relationship between
emission rates and column densities (Martin et al., 2003) or
between the normalised differences in the two quantities
(Lamsal et al., 2011). The linear coefficient was determined from a chemical transport model (CTM) using an a priori emissions
inventory. The linear relationship in one grid cell is assumed to be
unaffected by atmospheric transport and chemistry in neighbouring grid cells
(Mijling and Van Der A, 2012; Streets et al., 2013). For pollutants of longer
lifetimes or at finer model resolutions, however, it is important to account
for non-local sensitivities of pollutant concentrations to emissions.
Advanced data assimilation techniques such as Kalman filter
(Napelenok et al., 2008), ensemble Kalman filter (Miyazaki et al., 2012)
and four-dimensional variational assimilation (Kurokawa et al., 2009) have
been increasingly adopted to combine satellite observations and CTM
simulations with prior emission estimates to derive a posteriori emission estimates. These inverse methods provide more timely emission estimates of high spatial and temporal coverage (based on the nature of satellite observations). Nonetheless, the derived emission estimates are not resolved by source sector. They are also subject to uncertainties propagated from the satellite retrievals and the model simulations. For instance,
Archer-Nicholls et al. (2021) showed large differences in the 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> column density simulated by
two chemical mechanisms with different treatment of non-methane volatile
organic compounds (NMVOCs), which are integrated into the same model with
identical NO<inline-formula><mml:math id="M38" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions. When used in inverse modelling, these modelled
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> quantities would result in different a posteriori NO<inline-formula><mml:math id="M40" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions.</p>
      <p id="d1e572">This study introduces a novel approach that provides timely updates of a priori emission estimates by source sector using readily available in situ air quality observations. Using this approach, a priori NO<inline-formula><mml:math id="M41" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions in a bottom-up inventory compiled for Beijing for the year 2013 are updated for
2016. Uncertainties associated with emission trends between 2013 and 2016
were sampled by a perturbed emissions ensemble (PEE), which was constructed
on the basis of an expert elicitation. The PEE was then input to an
atmospheric dispersion model to generate an ensemble of air quality
simulations. By comparing the simulated surface concentrations of NO,
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> and O<inline-formula><mml:math id="M43" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> with observations from a dense monitoring network, the
initially estimated uncertainties could be reduced, and a posteriori emissions could be derived. The sensitivity of the results to the chemical mechanisms in the model was also evaluated.</p>
</sec>
<sec id="Ch1.S2">
  <label>2</label><title>Methods</title>
<sec id="Ch1.S2.SS1">
  <label>2.1</label><title>Observations</title>
      <p id="d1e617">Emission estimates were constrained using pollutant concentrations measured
in ground-based networks of high spatio-temporal resolution. 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> and
O<inline-formula><mml:math id="M45" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> are measured hourly at the long-term air quality monitoring sites
operated by the Beijing Municipal Environmental Monitoring Center using
reference instruments. Figure 1 shows the 33 sites that were in operation in
2016 and located within the study area (also see Table S1 in the Supplement), determined by
extent of the base emissions (see Sect. 2.2) and a classification according
to the local environment. Traffic monitoring sites are situated up to 20 m
from the curbside of major roads, while urban and suburban sites monitor air
quality in built-up areas not in close proximity to traffic in the six
central districts and the outer districts, respectively. Clean and regional
background sites that are away from built-up areas and major pollution
sources measure the baseline concentrations. In addition, measurements at
the regional background sites are representative of pollution transport from
and to neighbouring regions (Ministry of Environmental
Protection of the People's Republic of China, 2013). We used provisional
real-time measurements from 2016 archived at <uri>https://quotsoft.net/air/</uri> (last access: 22 August 2020), as ratified historical data are not publicly
available.</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="d1e643">The modelling domain as set by the extent of the base emissions
(see Sect. 2.2) with the locations of air quality measurements used in this
study, including a magnified view of the area within the 5th Ring Road of
Beijing (right panel). Long-term monitoring sites are colour-coded according
to the site type and labelled by their acronyms. Full names and coordinates
are listed in Table S1. Locations of low-cost sensor (SNAQ) measurements are
shown in dark grey, and the coordinates can be found in Table S2. The
weather station where the input meteorological observations were made is
marked by the grey star symbol. The administrative divisions of Beijing are
shown by light grey outlines.</p></caption>
          <?xmltex \igopts{width=426.791339pt}?><graphic xlink:href="https://acp.copernicus.org/articles/22/8617/2022/acp-22-8617-2022-f01.png"/>

        </fig>

      <p id="d1e652">In addition, we used high-frequency (20 s) measurements of NO, 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> and
O<inline-formula><mml:math id="M47" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> from November–December 2016, the winter campaign period of the
Atmospheric Pollution &amp; Human Health in a Chinese Megacity (APHH-Beijing)
research programme (Shi et al., 2019). The
measurements were made with low-cost sensors also deployed in a variety of
near-surface locations in Beijing (with an average measurement height of 8
m) and are hereinafter referred to as SNAQ (Sensor Network for Air Quality)
(Fig. 1 and Table S2). The dataset has been validated against reference
instrument measurements also obtained during the campaign and those from the
aforementioned long-term monitoring sites.</p>
</sec>
<sec id="Ch1.S2.SS2">
  <label>2.2</label><title>Perturbed emissions ensemble</title>
      <p id="d1e681">We used a special version of the Multi-resolution Emission Inventory for
China (MEIC) v1.3 (Li et al.,
2017; Zheng et al., 2018) developed for use in the APHH-Beijing programme.
The inventory characterises emissions of CO, NO<inline-formula><mml:math id="M48" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> (and 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>), total
VOC (TVOC), SO<inline-formula><mml:math id="M50" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, PM<inline-formula><mml:math id="M51" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">10</mml:mn></mml:msub></mml:math></inline-formula> and PM<inline-formula><mml:math id="M52" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> from the industry, power,
residential and transport sectors in 2013. It extends 120 and 150 km in
the north–south and east–west directions, respectively, covering most of
Beijing and parts of Hebei Province with 3 km <inline-formula><mml:math id="M53" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 3 km horizontal
resolution. In the vertical, there are seven layers with the top of each
layer at 38, 90, 152, 228, 337, 480 and 660 m above ground, respectively.
Each source sector is associated with a specific set of diurnal, monthly and
vertical variation profiles that is applied to emissions of all pollutants
from the sector. This inventory has been used to simulate street level air
quality (Biggart et al., 2020) and quantify regional pollution transport (Panagi et al., 2020) and has been compared with direct flux measurements
(Squires et al., 2020). To focus on locations where observations were available, we cropped the original extent to a smaller region of 105 km <inline-formula><mml:math id="M54" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 144 km (starting from the Northwest) and used it as the a priori emissions, hereinafter referred to as the base emissions. Annual NO<inline-formula><mml:math id="M55" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions in this region are shown in
Fig. S1 by source sector.</p>
      <p id="d1e753">NO<inline-formula><mml:math id="M56" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> and TVOC emissions in Beijing were reported to have decreased
substantially between 2013 (the year of the emission estimates) and 2016,
when the observations were made (Cheng et al., 2019; Xue et
al., 2020). In the surrounding provinces, NO<inline-formula><mml:math id="M57" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions also revealed a
downward trend, while no apparent trend has been identified for TVOC
emissions (Zheng et al., 2018). In addition to
spatial disparities, emissions from individual source sectors also showed
different patterns. In Beijing, for example, vehicle emission control
contributed the most NO<inline-formula><mml:math id="M58" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> reductions, while the largest TVOC decrease
was found in the petrochemical industry (Cheng et al., 2019; Xue et
al., 2020). Hence, uncertainties associated with the NO<inline-formula><mml:math id="M59" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions from
each sector in the base emissions were estimated separately. Due to a lack
of long-term observations, uncertainties associated with the TVOC emissions
were not investigated, the impact of which on the constrained NO<inline-formula><mml:math id="M60" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>
emissions is discussed in Sect. 4.</p>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T1" specific-use="star"><?xmltex \currentcnt{1}?><label>Table 1</label><caption><p id="d1e804">Emission parameters<inline-formula><mml:math id="M61" display="inline"><mml:msup><mml:mi/><mml:mi mathvariant="normal">a</mml:mi></mml:msup></mml:math></inline-formula> and the respective uncertainty ranges sampled by the initial and the adjusted perturbed emissions ensembles
(PEEs). n/a – not applicable.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="5">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="right"/>
     <oasis:colspec colnum="3" colname="col3" align="right" colsep="1"/>
     <oasis:colspec colnum="4" colname="col4" align="right"/>
     <oasis:colspec colnum="5" colname="col5" align="right"/>
     <oasis:thead>
       <oasis:row>
         <oasis:entry colname="col1">Parameter</oasis:entry>
         <oasis:entry namest="col2" nameend="col3" align="center" colsep="1">Initial </oasis:entry>
         <oasis:entry namest="col4" nameend="col5" align="center">Adjusted </oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"/>
         <oasis:entry rowsep="1" namest="col2" nameend="col3" align="center" colsep="1">PEE </oasis:entry>
         <oasis:entry rowsep="1" namest="col4" nameend="col5" align="center">PEE </oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2">Min</oasis:entry>
         <oasis:entry colname="col3">Max</oasis:entry>
         <oasis:entry colname="col4">Min</oasis:entry>
         <oasis:entry colname="col5">Max</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>
         <oasis:entry colname="col1">Industry sector ground-level NO<inline-formula><mml:math id="M69" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions</oasis:entry>
         <oasis:entry colname="col2">0.4</oasis:entry>
         <oasis:entry colname="col3">1.6</oasis:entry>
         <oasis:entry colname="col4">0.05</oasis:entry>
         <oasis:entry colname="col5">1.6</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Industry sector elevated NO<inline-formula><mml:math id="M70" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions</oasis:entry>
         <oasis:entry colname="col2">0.4</oasis:entry>
         <oasis:entry colname="col3">1.4</oasis:entry>
         <oasis:entry colname="col4">0.05</oasis:entry>
         <oasis:entry colname="col5">1.4</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Power sector NO<inline-formula><mml:math id="M71" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions<inline-formula><mml:math id="M72" display="inline"><mml:msup><mml:mi/><mml:mi mathvariant="normal">b</mml:mi></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col2">0.2</oasis:entry>
         <oasis:entry colname="col3">1.4</oasis:entry>
         <oasis:entry colname="col4">n/a</oasis:entry>
         <oasis:entry colname="col5">n/a</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Power sector NO<inline-formula><mml:math id="M73" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions below 152 m</oasis:entry>
         <oasis:entry colname="col2">n/a</oasis:entry>
         <oasis:entry colname="col3">n/a</oasis:entry>
         <oasis:entry colname="col4">0.05</oasis:entry>
         <oasis:entry colname="col5">1.6</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Power sector NO<inline-formula><mml:math id="M74" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions above 152 m</oasis:entry>
         <oasis:entry colname="col2">n/a</oasis:entry>
         <oasis:entry colname="col3">n/a</oasis:entry>
         <oasis:entry colname="col4">0.05</oasis:entry>
         <oasis:entry colname="col5">1.6</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Residential sector NO<inline-formula><mml:math id="M75" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions</oasis:entry>
         <oasis:entry colname="col2">0.4</oasis:entry>
         <oasis:entry colname="col3">1.5</oasis:entry>
         <oasis:entry colname="col4">0.05</oasis:entry>
         <oasis:entry colname="col5">1.5</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Transport sector NO<inline-formula><mml:math id="M76" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions</oasis:entry>
         <oasis:entry colname="col2">0.4</oasis:entry>
         <oasis:entry colname="col3">2</oasis:entry>
         <oasis:entry colname="col4">0.05</oasis:entry>
         <oasis:entry colname="col5">1.5</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Night-time fraction of transport sector NO<inline-formula><mml:math id="M77" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions<inline-formula><mml:math id="M78" display="inline"><mml:msup><mml:mi/><mml:mi mathvariant="normal">c</mml:mi></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col2">10</oasis:entry>
         <oasis:entry colname="col3">40</oasis:entry>
         <oasis:entry colname="col4">10</oasis:entry>
         <oasis:entry colname="col5">30</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table><table-wrap-foot><p id="d1e816"><inline-formula><mml:math id="M62" display="inline"><mml:msup><mml:mi/><mml:mi mathvariant="normal">a</mml:mi></mml:msup></mml:math></inline-formula> All parameters are defined as ratios of the 2016 emissions to the base emissions from 2013, except for the night-time fraction of transport sector NO<inline-formula><mml:math id="M63" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions which is defined as a percentage (%) of the daily totals in 2016.
<inline-formula><mml:math id="M64" display="inline"><mml:msup><mml:mi/><mml:mi mathvariant="normal">b</mml:mi></mml:msup></mml:math></inline-formula> Power sector NO<inline-formula><mml:math id="M65" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions are effectively represented by one parameter in the initial PEE. In the adjusted PEE, the emissions are split into two parameters, namely emissions below and above 152 m.
<inline-formula><mml:math id="M66" display="inline"><mml:msup><mml:mi/><mml:mi mathvariant="normal">c</mml:mi></mml:msup></mml:math></inline-formula> Night-time fraction of transport sector NO<inline-formula><mml:math id="M67" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions is defined as those occurring during 23:00–06:00 LT in the initial PEE. In the adjusted PEE, it is modified to NO<inline-formula><mml:math id="M68" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emitted during 00:00–05:00 LT from the transport sector.</p></table-wrap-foot></table-wrap>

      <p id="d1e1178">To reduce subjectivity, the uncertainties were determined based on
elicitation of expert knowledge. Table 1 shows the NO<inline-formula><mml:math id="M79" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emission
parameters investigated. To facilitate the expert elicitation and the
subsequent construction of PEEs, the parameters were defined as ratios of
the 2016 values to the corresponding 2013 estimates in the base emissions.
An exception is the last parameter which represents the night-time fraction
(in percentage) of transport sector NO<inline-formula><mml:math id="M80" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions in 2016, irrespective
of that in 2013. It allowed for perturbations to the diurnal distributions
of traffic NO<inline-formula><mml:math id="M81" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions on top of perturbations to the total
magnitude. In the initial PEE (see below and Sect. S1), the night-time
fraction was defined as emissions occurring between 23:00 and 06:00 local time (UTC<inline-formula><mml:math id="M82" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>8) (inclusive) following Biggart et al. (2020), who provided
evidence of an underestimation in the night-time vehicle sources of NO<inline-formula><mml:math id="M83" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>
in the a priori emissions inventory. This was attributed to an underrepresentation
of emissions from heavy duty diesel trucks, which typically travel from
surrounding provinces into Beijing at night, as they are banned from
entering the central urban areas during the day. After reviewing a previous
study which summarised the varying traffic rules and restrictions for
different types of vehicles in Beijing (Zhang
et al., 2019), the definition was modified to traffic NO<inline-formula><mml:math id="M84" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emitted
during 00:00–05:00 LT (inclusive) for the adjusted PEE.</p>
      <p id="d1e1234">To simultaneously perturb the total magnitude and the vertical distribution
of emissions, the three-dimensional industry sector was split into two
parameters, namely ground-level emissions (i.e. from the lowest vertical
layer) and elevated emissions (i.e. from all upper layers). This was also
intended for the power sector. However, as emissions from the sector are
present in all but the lowest layer, their vertical variation profile was
effectively unchanged in the initial PEE. The issue was fixed by introducing
two new parameters for power sources below and above 152 m (top height of
the fourth vertical layer), respectively, for the adjusted PEE.
Residential and transport emissions are only found in the ground layer and
were thus represented each by a single parameter.</p>
      <p id="d1e1237">An online questionnaire was designed for the elicitation (available at
<uri>https://cambridge.eu.qualtrics.com/jfe/form/SV_3eGxf9XvC7WXESV</uri>, last access: 14 April 2022) and circulated via the mailing
list of the APHH-Beijing programme. A total of seven responses was received.
Despite constituting a relatively small group, the participants included
researchers with expertise in compiling an emissions inventory for the region
of interest and researchers who used the same a priori emissions inventory in their own work. The fact that their responses were largely consistent also backs the credibility of the results. Specifically, the participants were invited to advise a lower and an upper bound of uncertainty for each emission
parameter, such that it would be very unlikely for the true value to fall
outside this range. The responses from the first round of elicitation were
sent back to the participants anonymously for review. Finally, the maximum
and minimum values advised by all participants for each parameter in the
second round were adopted (Table 1, “Initial PEE” column). These wide uncertainty ranges also compensated for the small size of the expert group.</p>
      <p id="d1e1243">Model simulations using the initial PEE as inputs showed substantial
overestimation of 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> concentrations, such that many members of the
ensemble were unusable for constraining the emissions (see Sect. S1). Hence,
we designed an adjusted PEE by decreasing the elicited lower bounds of
uncertainty for all parameters concerning the magnitude of NO<inline-formula><mml:math id="M86" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>
emissions from a certain source sector. The upper bound of uncertainty for
the transport emissions was also reduced, as the modelled diurnal
concentration profiles indicated positive biases linked specifically to the
sector. Lastly, the uncertainty range of the night-time fraction of
transport emissions was adjusted following the new definition described
above (Table 1, “Adjusted PEE” column).</p>
      <p id="d1e1264">As this study also sought to improve emission estimates of CO in the base
emissions (the results of which are presented in Yuan et al., 2021), the uncertainty ranges of relevant emission parameters were also elicited and modified in the same processes as the NO<inline-formula><mml:math id="M87" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emission parameters. The 14 parameters in total (i.e. 7 for NO<inline-formula><mml:math id="M88" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>, 7 for CO) determined for the adjusted PEE constituted a 14-dimensional uncertain space, which was probed efficiently using the maximin Latin hypercube sampling, which maximises the minimum inter-sample distance (Johnson et al., 1990).
A rule of thumb is to have a sample size 10 times the dimension
(Loeppky et al., 2009). We drew 140 samples,
effectively doubling the sample size generally required (i.e. if only
NO<inline-formula><mml:math id="M89" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emission parameters were perturbed). A simultaneous perturbation to
both CO and NO<inline-formula><mml:math id="M90" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> was justified by the fact that CO is treated as an
inert pollutant in the model used (see Sect. 2.3); thus varying CO emissions
do not affect the modelled NO<inline-formula><mml:math id="M91" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> concentrations (and vice versa). The
sample values were then used as spatio-temporally uniform scaling factors to
perturb the corresponding values in the base emissions to construct a
140-member PEE, hereinafter referred to as the adjusted PEE. Figure 2 shows
the total NO<inline-formula><mml:math id="M92" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions by source sector and vertical layer and the
mean diurnal variations of NO<inline-formula><mml:math id="M93" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions in the ensemble members. In
each member, the set of scaling factors applied to NO<inline-formula><mml:math id="M94" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> was also applied
to the emissions of 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>, such that primary 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> (<inline-formula><mml:math id="M97" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula>-NO<inline-formula><mml:math id="M98" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, i.e.
the proportion of NO<inline-formula><mml:math id="M99" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emitted directly as NO<inline-formula><mml:math id="M100" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>) in the base emissions remained unchanged, with a value of 6.7 % in all source sectors (and thus grid cells). In reality, however, the <inline-formula><mml:math id="M101" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula>-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> varies between sectors. Much attention has been paid to the <inline-formula><mml:math id="M103" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula>-NO<inline-formula><mml:math id="M104" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> in vehicle exhausts, while little is known about the <inline-formula><mml:math id="M105" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula>-NO<inline-formula><mml:math id="M106" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> in residential emissions. It is thus difficult to evaluate whether the 6.7 % in the base emissions is representative of the aggregated NO<inline-formula><mml:math id="M107" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions in the study area.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2"><?xmltex \currentcnt{2}?><?xmltex \def\figurename{Figure}?><label>Figure 2</label><caption><p id="d1e1454"><bold>(a)</bold> Annual total NO<inline-formula><mml:math id="M108" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions shown by contributions from individual source sectors in the 140-member adjusted perturbed emissions ensemble (PEE) and the base emissions (marked by black frames). <bold>(b)</bold> Vertical distributions of the annual total NO<inline-formula><mml:math id="M109" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions in the adjusted PEE and the base emissions. The height represents the top height (above local ground level) of each vertical layer. <bold>(c)</bold> Annual mean diurnal variations (in local time) in total NO<inline-formula><mml:math id="M110" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions in the adjusted PEE and the base emissions. In panels <bold>(b)</bold> and <bold>(c)</bold>, the base emissions are marked by black lines and triangle symbols, while the adjusted PEE members are colour-coded according to their annual total NO<inline-formula><mml:math id="M111" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions, with darker colours indicating higher values.</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://acp.copernicus.org/articles/22/8617/2022/acp-22-8617-2022-f02.png"/>

        </fig>

</sec>
<sec id="Ch1.S2.SS3">
  <label>2.3</label><title>Model description and simulation setup</title>
      <p id="d1e1522">We used ADMS-Urban (version 4.2), a state-of-the-art urban-scale high-resolution quasi-Gaussian dispersion model (McHugh et
al., 1997; Owen et al., 2000). The model has been applied in air quality
simulations in cities worldwide including Beijing (Biggart
et al., 2020; He et al., 2019; Hood et al., 2018). Dispersion calculations
are based on the state of the atmospheric boundary layer, which is
parameterised based on Monin–Obukhov similarity theory
(Venkatram, 1996). The parameterisation is explained in detail in previous studies (e.g. Biggart et al.,
2020). The minimum required meteorological input data including hourly wind
speed, wind direction and cloud cover were measured at a weather station at
Beijing Capital International Airport (see Fig. 1) and archived in the
NOAA Integrated Surface Database (Smith et al., 2011). Local
disturbance to the mean flow field by individual buildings and street
canyons was not accounted for as such data were unavailable. Nonetheless,
differences in the near-surface dynamics at the weather observatory
(situated in open landscape) and at the measurement sites (the majority of
which are located in built-up areas) were represented by different values of
roughness length and minimum Obukhov length, as described in
Yuan et al. (2021).</p>
      <p id="d1e1525">Chemistry calculations are enabled by two fast chemistry schemes for the
NO<inline-formula><mml:math id="M112" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> photolytic chemistry and the formation of sulfate aerosols,
respectively (Cambridge Environmental Research Consults Limited,
2017). The former is based on the Generic Reaction Set (Azzi et
al., 1992) which reduces the complex mechanisms involving NO<inline-formula><mml:math id="M113" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>, O<inline-formula><mml:math id="M114" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>
and VOCs to seven reactions:


                <disp-formula specific-use="gather" content-type="numbered reaction"><mml:math id="M115" display="block"><mml:mtable displaystyle="true"><mml:mlabeledtr id="Ch1.R1"><mml:mtd><mml:mtext>R1</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:mrow class="chem"><mml:mi mathvariant="normal">ROC</mml:mi></mml:mrow><mml:mo>+</mml:mo><mml:mi>h</mml:mi><mml:mi mathvariant="italic">ν</mml:mi><mml:mo>→</mml:mo><mml:mrow class="chem"><mml:mi mathvariant="normal">RP</mml:mi><mml:mo>+</mml:mo><mml:mi mathvariant="normal">ROC</mml:mi></mml:mrow></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.R2"><mml:mtd><mml:mtext>R2</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:mrow class="chem"><mml:mi mathvariant="normal">RP</mml:mi><mml:mo>+</mml:mo><mml:mi mathvariant="normal">NO</mml:mi><mml:mo>→</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.R3"><mml:mtd><mml:mtext>R3</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow><mml:mo>+</mml:mo><mml:mi>h</mml:mi><mml:mi mathvariant="italic">ν</mml:mi><mml:mo>→</mml:mo><mml:mrow class="chem"><mml:mi mathvariant="normal">NO</mml:mi><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.R4"><mml:mtd><mml:mtext>R4</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:mrow class="chem"><mml:mi mathvariant="normal">NO</mml:mi><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:mo>→</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.R5"><mml:mtd><mml:mtext>R5</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:mrow class="chem"><mml:mi mathvariant="normal">RP</mml:mi><mml:mo>+</mml:mo><mml:mi mathvariant="normal">RP</mml:mi><mml:mo>→</mml:mo><mml:mi mathvariant="normal">RP</mml:mi></mml:mrow></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.R6"><mml:mtd><mml:mtext>R6</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:mrow class="chem"><mml:mi mathvariant="normal">RP</mml:mi><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>→</mml:mo><mml:mi mathvariant="normal">SGN</mml:mi></mml:mrow></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.R7"><mml:mtd><mml:mtext>R7</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:mrow class="chem"><mml:mi mathvariant="normal">RP</mml:mi><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>→</mml:mo><mml:mi mathvariant="normal">SNGN</mml:mi></mml:mrow></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.R8"><mml:mtd><mml:mtext>R8</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:mrow class="chem"><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">NO</mml:mi><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>→</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr></mml:mtable></mml:math></disp-formula>

            where ROC, RP, SGN and SNGN represent reactive organic compounds, radical
pool, stable gaseous nitrogen product and stable non-gaseous nitrogen
product, respectively. Reaction (R8) has been added to the scheme in
ADMS-Urban, but its impact is only significant with sustained high levels of
NO concentrations (e.g. 1000 <inline-formula><mml:math id="M116" 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="M117" 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> for several hours) due to a small rate constant (Cambridge Environmental Research Consults
Limited, 2017). It is evident that only Reactions (R3) and (R4) are
conservative chemical reactions, while the rest represent approximations of
multiple reactions lumped together. For example, Reaction (R1) represents
all reactions that produce radicals via the photo-oxidation of VOCs. Thus,
the rate coefficients of these generic reactions have been determined
empirically by fitting the simulation outputs to smog chamber data
(Azzi et al., 1992). The rate constant of the explicit reaction, Reaction (R3), can be calculated from solar radiation, which is often estimated by
ADMS-Urban based on the input meteorological data, when direct measurements
are unavailable (as is the case in this study). By appealing to
NO<inline-formula><mml:math id="M118" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>–O<inline-formula><mml:math id="M119" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> photostationary state, the model also derives a 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>
photolysis rate from the background concentrations of NO, NO<inline-formula><mml:math id="M121" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and
O<inline-formula><mml:math id="M122" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> and takes the lower value between the two (Cambridge
Environmental Research Consults Limited, 2017).</p>
      <p id="d1e1821">Background pollutant concentrations are thus required as an input, not only
to account for pollution sources not included in the input emissions (e.g.
transported from outside the extent of the emissions inventory), but also to
constrain the reaction coefficients for reactive species. As mentioned in
Sect. 2.1, continuous measurements of 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> and O<inline-formula><mml:math id="M124" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> are available
from the long-term monitoring network. In each hour, we input the inverse-distance-weighted mean of the concentrations at two of the clean or regional
background sites (a total of six; see Fig. 1) located to each side of the
incoming wind direction in that hour as the background in the adjusted PEE
simulations. This was different from the initial PEE simulations (see Sect. S1) which used a baseline concentration, defined as the 10th percentile
of the concentrations from all sites in a moving 3 h window. The method of
using a network baseline to represent the non-local pollution signal has
previously been applied to CO, which is inert in ADMS-Urban
(Yuan et al., 2021) and NO<inline-formula><mml:math id="M125" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> and O<inline-formula><mml:math id="M126" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> at a small spatial scale
(Popoola et al., 2018). At larger scales, however, though it has been established that concentrations of total oxidants (O<inline-formula><mml:math id="M127" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> <inline-formula><mml:math id="M128" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> O<inline-formula><mml:math id="M129" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> <inline-formula><mml:math id="M130" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> NO<inline-formula><mml:math id="M131" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>) consist of a local component
that correlates with NO<inline-formula><mml:math id="M132" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions and a NO<inline-formula><mml:math id="M133" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>-independent regional
component (Clapp and Jenkin, 2001; Han et al., 2011), the partition of O<inline-formula><mml:math id="M134" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> between 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> and O<inline-formula><mml:math id="M136" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> may be highly variable in time and space due to their rapid interconversion and reactions with other species. Using values measured at two neighbouring sites away from major sources ensured a more realistic partition of O<inline-formula><mml:math id="M137" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> in the adjusted PEE simulations. The
sensitivity of the simulation output to different definitions of NO<inline-formula><mml:math id="M138" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
and O<inline-formula><mml:math id="M139" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> background concentrations is further investigated in Sect. 4.</p>
      <p id="d1e1975">For NO and TVOC for which long-term measurements were unavailable, we used
upwind concentrations from the Copernicus Atmosphere Monitoring Service
(CAMS) reanalysis dataset (Inness et al., 2019). At each time
step (every 3 h), we calculated the inverse-distance-weighted mean of
the values from the two grid cells in the lowest vertical layer located
directly outside of the modelling domain and to each side of the incoming
wind. The time series obtained was then linearly interpolated to hourly
resolution, as required by ADMS-Urban. As TVOC is not a standard output
variable in the dataset, a sum of the eight available VOC species was used to
approximate TVOC. To validate this approach, we compared the sum of mixing
ratios of 29 VOC species measured at the Institute of Atmospheric Physics,
Chinese Academy of Sciences during the APHH-Beijing winter campaign with the
approximate TVOC mixing ratios from the corresponding grid cell in the
reanalysis product during the same period. Apart from a few peak events not
seen in the latter, the two time series show a good level of agreement, both
in terms of the trend and the magnitude (Fig. 3a). The upwind NO mixing
ratios extracted from the CAMS reanalysis dataset were compared to NO
baseline mixing ratios extracted from the SNAQ measurements. Figure 3b shows
a substantial positive bias in the NO extracted from the reanalysis dataset,
the cause of which remains unknown. To prevent this bias from being
propagated into the modelled concentrations, a bias correction was applied
using empirical quantile mapping. This method equates the (empirically
estimated) cumulative distribution functions (i.e. quantile functions) of
the modelled and observed time series for regularly spaced quantiles
(Boé et al., 2007; Cannon et al., 2015). During the campaign period, this
significantly reduced the bias, while the correlation was only slightly
decreased. However, larger uncertainties would have been introduced when the
transfer function was extrapolated to the entire time series of 2016, which
were unavoidable and difficult to quantify due to a lack of long-term
measurements. Yet these were likely smaller than the uncertainties
associated with using the uncorrected, positively biased values obtained
from the CAMS reanalysis product.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3"><?xmltex \currentcnt{3}?><?xmltex \def\figurename{Figure}?><label>Figure 3</label><caption><p id="d1e1981"><bold>(a)</bold> Mixing ratios of TVOC at the Institute of Atmospheric Physics (IAP), Chinese Academy of Sciences, during the APHH-Beijing winter campaign from the Copernicus Atmosphere Monitoring Service (CAMS) reanalysis dataset, compared to observations. TVOC from the reanalysis product was approximated by the sum of eight available VOC species. The observed TVOC was calculated as the sum of 29 VOC species measured. <bold>(b)</bold> Original and bias-corrected upwind mixing ratios of NO from the reanalysis dataset (the latter were input as background pollution levels in the PEE simulations), compared to baseline (10th percentile) mixing ratios from the SNAQ measurements. For each reanalysis time series, the data and the normalised mean bias (NMB) and Pearson's correlation coefficient (<inline-formula><mml:math id="M140" display="inline"><mml:mi>r</mml:mi></mml:math></inline-formula>) are shown in the same colour.</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://acp.copernicus.org/articles/22/8617/2022/acp-22-8617-2022-f03.png"/>

        </fig>

      <p id="d1e2002">The input meteorology data and background pollutant concentrations described
above provided the same lateral boundary conditions for the 140 adjusted PEE
simulations, among which only the emissions of NO<inline-formula><mml:math id="M141" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> (and 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>)
varied. An additional simulation forced with these boundary conditions and
the base emissions was also performed and is hereinafter referred to as the
base run. All 141 simulations were run for the whole year of 2016 to produce
hourly pollutant concentrations at each measurement location (see Fig. 1).
Output of these simulations was then compared to measurements to derive a posteriori emission estimates.</p>
</sec>
</sec>
<sec id="Ch1.S3">
  <label>3</label><title>Results</title>
      <p id="d1e2032">We first evaluated the performance of the adjusted PEE simulations in
modelling NO<inline-formula><mml:math id="M143" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentrations at the long-term monitoring sites using
mean square error (MSE). It is a compact indicator of model performance
whose merit is demonstrated in the following. The MSE is calculated as

          <disp-formula id="Ch1.E9" content-type="numbered"><label>1</label><mml:math id="M144" display="block"><mml:mrow><mml:mi mathvariant="normal">MSE</mml:mi><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mn mathvariant="normal">1</mml:mn><mml:mi>n</mml:mi></mml:mfrac></mml:mstyle><mml:msubsup><mml:mo>∑</mml:mo><mml:mrow><mml:mi>i</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow><mml:mi>n</mml:mi></mml:msubsup><mml:msup><mml:mfenced open="(" close=")"><mml:mrow><mml:msub><mml:mi mathvariant="normal">mod</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi mathvariant="normal">obs</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:mfenced><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
        where <inline-formula><mml:math id="M145" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">obs</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the observed value for a given averaging period <inline-formula><mml:math id="M146" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula> (e.g. an hour, a day, a month), <inline-formula><mml:math id="M147" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">mod</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the corresponding simulation output and <inline-formula><mml:math id="M148" display="inline"><mml:mi>n</mml:mi></mml:math></inline-formula> represents the number of the available observations.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4" specific-use="star"><?xmltex \currentcnt{4}?><?xmltex \def\figurename{Figure}?><label>Figure 4</label><caption><p id="d1e2132">Mean square errors (MSEs) in <bold>(a)</bold> hourly NO<inline-formula><mml:math id="M149" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentrations and <bold>(b)</bold> daily maximum 8 h mean (MDA8) O<inline-formula><mml:math id="M150" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> concentrations associated with the adjusted perturbed emissions ensemble (PEE) simulations, arranged in ascending order of the input annual total NO<inline-formula><mml:math id="M151" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions (from left to right) and the base run (marked by black frames) at each long-term monitoring site. In each panel, the MSEs are grouped into quartiles and colour-coded accordingly. The monitoring sites are arranged and colour-coded according to the site type: urban site (magenta), traffic monitoring site (purple), suburban site (orange), clean site (light green) and regional background site (green).</p></caption>
        <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/22/8617/2022/acp-22-8617-2022-f04.png"/>

      </fig>

      <p id="d1e2174">At each site, MSE is calculated for the hourly 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> concentration
output by each adjusted PEE simulation and the base run. Figure 4a shows a
distinct trend of increasing MSEs with growing annual total NO<inline-formula><mml:math id="M153" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>
emissions, such that at most sites, the base run with input emissions at the
upper end of the scale (see Fig. 2a) is outperformed by most of the PEE
simulations. Although a single MSE does not differentiate between over- and
underestimation, this clear positive association between MSEs and NO<inline-formula><mml:math id="M154" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>
emissions suggests that NO<inline-formula><mml:math id="M155" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions are positively biased, both in
the base emissions and in most members of the PEE. If NO<inline-formula><mml:math id="M156" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions
were negatively biased in a considerable subset of the ensemble members, the
MSEs would first decrease as emissions increased, until the absolute bias in
the emissions reached a minimum. It is also evident that the base run is
generally associated with larger errors at urban and traffic monitoring
sites compared to other sites. Moreover, the increase in MSEs with
increasing emissions is more rapid at these locations, resulting in a wider
range of errors associated with the ensemble of simulations. This is an
indication that the base emissions are larger in magnitude in the central
areas (where these sites are situated; see Fig. 1) than in the periphery and
are overestimated to a larger extent. Though spatially uniform scaling
factors were applied within the study area, regions with higher base
emissions would show larger variations in the perturbed emissions and thus
model errors. This highlights a potential issue associated with spatially
uniform perturbations to spatially non-uniform emissions.</p>
      <p id="d1e2223">Due to the important role of O<inline-formula><mml:math id="M157" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> in converting NO into NO<inline-formula><mml:math id="M158" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, the
adjusted PEE simulations' performance in modelling the O<inline-formula><mml:math id="M159" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>
concentrations was also evaluated. In other words, this was to ensure that
the underlying chemical mechanisms were correctly modelled and that
simulations with lower NO<inline-formula><mml:math id="M160" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions showed better agreement with
NO<inline-formula><mml:math id="M161" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> observations for the right reasons. We calculated the MSEs in
maximum daily 8 h mean (MDA8) O<inline-formula><mml:math id="M162" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> concentrations<fn id="Ch1.Footn1"><p id="d1e2281">The
adjusted PEE simulations' performance in modelling the hourly O<inline-formula><mml:math id="M163" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>
concentrations was also evaluated. The median MSEs in hourly O<inline-formula><mml:math id="M164" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>
concentrations of all simulations are dominated by the mMSE, and their
association with the input NO<inline-formula><mml:math id="M165" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions is substantially weaker than
the association between median MSEs in MDA8 O<inline-formula><mml:math id="M166" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> concentrations and
NO<inline-formula><mml:math id="M167" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions.</p></fn>. Among the numerous O<inline-formula><mml:math id="M168" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> metric available, the
MDA8 O<inline-formula><mml:math id="M169" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> is widely used for model–observation comparison due to its
relevance in regulation and health impact assessments
(Lefohn et al., 2018). Figure 4b
shows that as with NO<inline-formula><mml:math id="M170" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, the base run is also generally associated with
higher MSEs than many PEE simulations. At more sites, however, the positive
association between model error and NO<inline-formula><mml:math id="M171" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions seen in Fig. 4a
breaks down (e.g. at DSH and MTG) or even becomes reversed (e.g. at HR and
LLH). This underscores the complex effects of non-linear chemistry and
suggests that the MSEs in MDA8 O<inline-formula><mml:math id="M172" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> are less strongly associated with
the input NO<inline-formula><mml:math id="M173" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions, the reason for which can be revealed by a
breakdown of the MSE.</p>
      <p id="d1e2385">The MSE can be mathematically decomposed into the sum of three terms
(Solazzo and Galmarini, 2016):
          <disp-formula id="Ch1.E10" content-type="numbered"><label>2</label><mml:math id="M174" display="block"><mml:mtable rowspacing="0.2ex" class="split" displaystyle="true" columnalign="right left"><mml:mtr><mml:mtd><mml:mrow><mml:mi mathvariant="normal">MSE</mml:mi></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mo>=</mml:mo><mml:mfenced close="]" open="["><mml:mrow><mml:msup><mml:mfenced open="(" close=")"><mml:mrow><mml:mover accent="true"><mml:mi mathvariant="normal">mod</mml:mi><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>-</mml:mo><mml:mover accent="true"><mml:mi mathvariant="normal">obs</mml:mi><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:mrow></mml:mfenced><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:mfenced><mml:mo>+</mml:mo><mml:mfenced close="]" open="["><mml:mrow><mml:msup><mml:mfenced close=")" open="("><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi mathvariant="normal">mod</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:mi>r</mml:mi><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi mathvariant="normal">obs</mml:mi></mml:msub></mml:mrow></mml:mfenced><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:mfenced></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mo>+</mml:mo><mml:mfenced open="[" close="]"><mml:mrow><mml:msubsup><mml:mi mathvariant="italic">σ</mml:mi><mml:mi mathvariant="normal">obs</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msubsup><mml:mo>×</mml:mo><mml:mfenced open="(" close=")"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>-</mml:mo><mml:msup><mml:mi>r</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:mfenced></mml:mrow></mml:mfenced><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:math></disp-formula>
        where <inline-formula><mml:math id="M175" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi mathvariant="normal">mod</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M176" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi mathvariant="normal">obs</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> represent the standard deviation of the modelled and observed values, respectively, and <inline-formula><mml:math id="M177" display="inline"><mml:mi>r</mml:mi></mml:math></inline-formula> is the Pearson's correlation coefficient between model outputs and observations. The first term in Eq. (2) represents the bias component of model error, and it is
largely introduced by external forcings, for example, input emissions and
boundary conditions. The second term is the variance error which is
associated with the processes resolved in a model. A trade-off between bias
and variance, in other words, accuracy and precision, is often inevitable in
complex models (Sun and Archibald, 2021). The last term, by
definition, represents the proportion of the observed variance unexplained
by the model. It summarises all non-systematic errors, including the noise
and inherent variability (e.g. due to turbulence closure) in the
observations as well as errors arising from the linearisation of non-linear
processes and is referred to as the minimum achievable MSE (mMSE). The MSE
is thus a well-rounded metric suitable for operational model evaluation, and
its decomposition provides indications of possible sources of model error
(Solazzo and Galmarini, 2016).</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="d1e2506">Error component with the highest contribution to the mean square
errors (MSEs) in <bold>(a)</bold> hourly NO<inline-formula><mml:math id="M178" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentrations and <bold>(b)</bold> daily maximum 8 h mean (MDA8) O<inline-formula><mml:math id="M179" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> concentrations associated with the adjusted perturbed emissions ensemble (PEE) simulations, arranged in ascending order of the input annual total NO<inline-formula><mml:math id="M180" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions (from left to right) and the base run (marked by black frames) at each long-term monitoring site. The monitoring sites are arranged and colour-coded according to the site type: urban site (magenta), traffic monitoring site (purple), suburban site (orange), clean site (light green) and regional background site (green).</p></caption>
        <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/22/8617/2022/acp-22-8617-2022-f05.png"/>

      </fig>

      <p id="d1e2548">The values of MSEs shown in Fig. 4 were decomposed according to Eq. (2), and
the term with the largest contribution to the MSE associated with each
simulation at each site is shown in Fig. 5. There are striking differences
in the attribution of error for hourly 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> and MDA8 O<inline-formula><mml:math id="M182" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>. Variance
errors have the largest share in the MSEs in hourly 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> concentrations
associated with most of the adjusted PEE simulations at over half of the
reference sites. At another <inline-formula><mml:math id="M184" display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">4</mml:mn></mml:mrow></mml:math></inline-formula> of the sites, all of which are urban or
traffic monitoring sites, bias accounts for most of the errors in the bulk
of the simulations. This is another indication of a higher degree of
overestimation in the central areas in the base emissions and subsequently
in many members of the adjusted PEE. For most sites (regardless of the site
type), simulations using the lowest annual total NO<inline-formula><mml:math id="M185" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions are
associated with MSEs that are mostly made up by the mMSE.</p>
      <p id="d1e2599">At the urban and traffic monitoring sites where the MSEs in hourly NO<inline-formula><mml:math id="M186" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
associated with the ensemble simulations are mainly made up of the bias
error, the bias also happens to be the largest term in most MSEs in MDA8
O<inline-formula><mml:math id="M187" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> (Fig. 5b). At most other sites (including all suburban, clean and
regional background sites), however, the MSEs in MDA8 O<inline-formula><mml:math id="M188" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> are dominated
by the mMSE, irrespective of the input NO<inline-formula><mml:math id="M189" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions. This explains the
weaker association between the total MSEs in MDA8 O<inline-formula><mml:math id="M190" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> and the emissions
revealed in Fig. 4b, as the mMSE is much less dependent on model inputs. A
further breakdown of the mMSEs (Fig. S4) reveals that variances in the
observations of MDA8 O<inline-formula><mml:math id="M191" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> are substantially higher than those in the
observed hourly NO<inline-formula><mml:math id="M192" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentrations. Despite considerably better
correlation between model outputs and the observations, these large
variances in the observations result in mMSEs in MDA8 O<inline-formula><mml:math id="M193" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> concentrations
that are only moderately smaller than those associated with hourly NO<inline-formula><mml:math id="M194" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
concentrations. Meanwhile, the MSEs in O<inline-formula><mml:math id="M195" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> are considerably lower than
those in NO<inline-formula><mml:math id="M196" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>; the largest share of the mMSEs in the former is thus
explained. Because of this dependence on the observations and the weaker
connection to external drivers, the mMSE is often considered the least
concerning component of model error (Solazzo and Galmarini, 2016).</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="d1e2705">Decomposed median mean square errors (MSEs) in <bold>(a)</bold> hourly 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> concentrations and <bold>(b)</bold> daily maximum 8 h mean (MDA8) O<inline-formula><mml:math id="M198" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> concentrations associated with the adjusted perturbed emissions ensemble (PEE) simulations, arranged in ascending order of the input annual total NO<inline-formula><mml:math id="M199" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions (from left to right) and the base run (marked by black frames).</p></caption>
        <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/22/8617/2022/acp-22-8617-2022-f06.png"/>

      </fig>

      <p id="d1e2747">As the distributions of the 33 MSEs (i.e. one for each long-term monitoring
site) associated with individual PEE simulations are mostly non-Gaussian, we
used the median MSE to represent a simulation's average performance for a
certain pollutant across all sites within the modelling domain. A breakdown
of the median MSEs (Fig. 6) is consistent with the findings described above:
with more accurate (lower) input NO<inline-formula><mml:math id="M200" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions, a simulation's average
performance for hourly 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> can be improved substantially to a point
that the remaining model error consists mostly of the non-systematic mMSE.
The average performance for MDA8 O<inline-formula><mml:math id="M202" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> is less strongly associated with
NO<inline-formula><mml:math id="M203" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions, as it is dominated by the mMSE in the majority of the
PEE simulations. These associations between median MSEs and input emissions
are also tested using simple linear regression (Fig. S5). Though both
regression models are statistically significant (<inline-formula><mml:math id="M204" display="inline"><mml:mi>p</mml:mi></mml:math></inline-formula> value <inline-formula><mml:math id="M205" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> 0.001), more
variability in the modelled hourly NO<inline-formula><mml:math id="M206" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> is explained, compared to that
in the modelled MDA8 O<inline-formula><mml:math id="M207" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>. The scatter of the points around the
regression line reveals the variations in model performance with varying mix
of source sectors, given similar strengths of total emissions (note that
these are represented on an ordinal scale in Figs. 4–6). This also
demonstrates the importance of using network observations as constraints.
With spatially uniform perturbations, it is likely that several different
combinations of emission parameter values result in similar concentrations
at a particular location. The risk of constraining the parameter values to
just one of the possible combinations is reduced, when observations that
sample a wide range of local environments are used.</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="d1e2821">Average performance of the adjusted perturbed emissions ensemble
(PEE) simulations and the base run (marked with black strokes) as a function
of emission parameter values. The scales on the <inline-formula><mml:math id="M208" display="inline"><mml:mi>x</mml:mi></mml:math></inline-formula> axes correspond to the
uncertainty ranges in Table 1, “Adjusted PEE” column. The top-performing 25 %, 20 %, 15 %, 10 %, 5 % and 1 % of the simulations are coloured in a darkening green shade, as measured by their median mean square errors (MSEs) in hourly 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> concentrations at the long-term monitoring sites across the modelling domain (see Fig. 6) in all panels except in panel <bold>(g)</bold>, where median mean square errors in the annual mean diurnal variations of NO<inline-formula><mml:math id="M210" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentrations are used (note the different scale on the <inline-formula><mml:math id="M211" display="inline"><mml:mi>y</mml:mi></mml:math></inline-formula> axis).</p></caption>
        <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/22/8617/2022/acp-22-8617-2022-f07.png"/>

      </fig>

      <p id="d1e2865">On account of the analysis above, we only used observations of NO<inline-formula><mml:math id="M212" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> to
constrain NO<inline-formula><mml:math id="M213" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions, which is also in line with numerous top-down
emission optimisation studies using satellite observations of column
NO<inline-formula><mml:math id="M214" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> (Lamsal
et al., 2011; Martin et al., 2003; Napelenok et al., 2008; Qu et al., 2017).
Figure 7 shows the average performance for hourly NO<inline-formula><mml:math id="M215" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> of individual PEE
simulations against the value set for each emission parameter in Table 1.
Figure 7f reveals a strong positive correlation between the median MSE in
hourly NO<inline-formula><mml:math id="M216" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> of a simulation and the input transport sector NO<inline-formula><mml:math id="M217" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>
emissions. Simulations with a median MSE within the first quartile are
forced with transport emissions 6 %–65 % of those in the base emissions. This range continues to reduce (from both ends) with improving simulation performance, such that when the median MSE falls below the 10th
percentile, the corresponding traffic emissions are only 7 %–43 % of those in the base emissions. The range determined by the top-performing 5 % of the simulations (i.e. with a median MSE within the fifth percentile)
remains the same, while it can be further constrained one-sidedly to
7 %–18 % if only the top 1 % were considered. However, as the top 1 % of a 140-member ensemble contains (maximally) two simulations, the difference in whose average performance is marginal (<inline-formula><mml:math id="M218" display="inline"><mml:mo lspace="0mm">≤</mml:mo></mml:math></inline-formula> 1.5 %), this range was considered not robust.</p>
      <p id="d1e2930">In addition to the total magnitude, the night-time fraction of the transport
sector NO<inline-formula><mml:math id="M219" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions could also be constrained (Fig. 7g). Instead of
hourly NO<inline-formula><mml:math id="M220" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, performance of the adjusted PEE simulations was evaluated
against the observed annual mean diurnal variations 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> at each
long-term monitoring site. The median of all 33 MSEs in the diurnal profiles
at individual sites modelled by a simulation was also used to represent its
average performance in modelling the different diurnal profiles observed
within the study area (see Fig. S3). Though not as evident as the case of
total transport emissions, the range of the night-time fraction also becomes
narrower with improving model skill. Amongst simulations with a median MSE
in diurnal NO<inline-formula><mml:math id="M222" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> profiles within the 15th percentile, 11 %–29 % of the transport emissions occur at night (in contrast to the 9 % in the base emissions). In the top 5 % of the simulations, this fraction varies
between 15 % and 25 %.</p>
      <p id="d1e2970">Emission parameters for other source sectors could not be constrained with
strong confidence (Fig. 7a–e), as the ranges of parameter values only start
to noticeably differ from the full uncertainty range when the median MSE in
hourly 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> falls within the 10th percentile or even below. The
residential sector is the smallest source sector of NO<inline-formula><mml:math id="M224" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> in the base
emissions (see Fig. 2a). A source apportionment of the base run reveals that
its contribution to the annual mean NO<inline-formula><mml:math id="M225" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> concentrations at individual
long-term monitoring sites varies between 3 % and 8 % (Fig. S6). It can thus be expected that even a 150 % increase, i.e. its upper bound of
uncertainty (see Table 1, “Adjusted PEE” column), is not sufficient to cause substantial changes in the simulation performance for NO<inline-formula><mml:math id="M226" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>, based on which the emissions can be constrained.</p>
      <p id="d1e3009">Interestingly, Fig. S6 also reveals that at most sites, the contribution of
NO<inline-formula><mml:math id="M227" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> base emissions from the power sector to the modelled annual mean
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> concentrations is even smaller than that from the residential
sector, though the emissions are over 2 times higher (see Fig. 2a). This
is attributable to the nature of the power sector, which is characterised by
a few large point sources emitting at elevated levels. These sources undergo
greater dispersion before reaching the surface-based monitoring sites
(compared to ground-level emissions); thus their impact at most sites is
small. As an example, the annual mean NO<inline-formula><mml:math id="M229" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> concentration simulated at
the site NZG is very similar to that modelled at the site GC, yet less than
3 % of this concentration stems from NO<inline-formula><mml:math id="M230" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions from the power
sector, as opposed to the 11 % share at GC (Fig. S6). This can be
explained by Fig. S7 in which the concentration resulted from power
emissions is further apportioned to each grid cell. It is evident that the
concentration at GC is predominantly contributed by the grid cell directly
to its west. In fact, this grid cell contains the highest power emissions of
NO<inline-formula><mml:math id="M231" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> within the study area. In comparison, the site NZG is located at
some distance from other grid cells with relatively large power sources. The
contributions of these grid cells to the NO<inline-formula><mml:math id="M232" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> concentrations at NZG are
smaller. The differences are about 1 order of magnitude, as the
contributions are log-transformed in the figure.</p>
      <p id="d1e3067">The fact that emissions released at higher levels are not well sampled by
the existing surface-based monitoring sites also applies for those of
NO<inline-formula><mml:math id="M233" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> from industrial sources (emitted at up to 152 m). In addition,
emissions from both source sectors were separated into two parameters and
perturbed simultaneously (i.e. in an uncorrelated matter) for varying
vertical distributions. The uncertainty range of the sum of the two
parameters, i.e. the total power or industrial emissions, was thus smaller
than the individual uncertainty ranges and may not be sufficiently large to
capture the actual emissions.</p>
      <p id="d1e3079">The short-term, independent SNAQ measurements of NO<inline-formula><mml:math id="M234" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> were also used to
constrain the emission parameters following the same approach (Fig. S8).
Similarly, adjusted PEE simulations showing better performance for hourly
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> concentrations and mean diurnal variations of 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>
concentrations (over the measurement period) at SNAQ sites are associated
with lower transport sector total emissions, but a higher percentage of
these emissions occur at night. In the top-performing 5 % of the
simulations, total traffic emissions are 7 %–43 % of those in the base emissions, while the night-time fraction varies between 15 % and 26 %. The fact that the uncertainty ranges constrained by the short-term SNAQ measurements are consistent with those using long-term reference measurement demonstrates the robustness of both this approach and the findings. This also supports the use of low-cost sensors for this particular application, as they are more affordable for deployment in a dense network.</p>
</sec>
<sec id="Ch1.S4">
  <label>4</label><title>Discussion</title>
      <p id="d1e3117">According to the base emissions, total NO<inline-formula><mml:math id="M237" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions from the transport
sector were 2.1 <inline-formula><mml:math id="M238" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<inline-formula><mml:math id="M239" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">5</mml:mn></mml:msup></mml:math></inline-formula> Mg within the study area which extends over most of Beijing and parts of Hebei Province in 2013, 9 % of which occurred during 00:00–05:00 LT. Based on the top 5 % of the adjusted PEE simulations for modelling 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> hourly concentrations and diurnal profiles, we found that transport NO<inline-formula><mml:math id="M241" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions were likely to have decreased to 1.5–9 <inline-formula><mml:math id="M242" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<inline-formula><mml:math id="M243" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msup></mml:math></inline-formula> Mg (i.e. a 57 %–93 % reduction) in 2016, and the night-time fraction was between 15 % and 25 %.</p>
      <p id="d1e3180">An exact comparison of these results with findings of previous studies is
not possible, as the emissions were investigated over different spatial
and/or temporal scales. However, it is possible to compare the relative
changes in emissions. Biggart et al. (2020) found that total NO<inline-formula><mml:math id="M244" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions rates from the same a priori emissions inventory (and all
source sectors) were 1.8 times higher than those from an optimised emissions
inventory (with which ADMS-Urban simulated NO<inline-formula><mml:math id="M245" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> and 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>
concentrations that were in much better agreement with the corresponding
observations), though their investigation was focused on a small domain in
urban Beijing and the duration of the APHH-Beijing winter campaign only.
They also found that the modelled mean diurnal variations in 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> concentrations at most sites could be substantially improved when the
night-time fraction of NO<inline-formula><mml:math id="M248" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions was increased by 25 % and
50 %. Nonetheless, as mentioned in Sect. 2.2, this was defined as NO<inline-formula><mml:math id="M249" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emitted between 23:00 and 06:00 LT from all source sectors.</p>
      <p id="d1e3238">Squires et al. (2020)
compared NO<inline-formula><mml:math id="M250" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emission rates in the same a priori emissions with flux
measurements made from a tower in central Beijing (where SNAQ39 was also
deployed; see Fig. 1) during the APHH-Beijing winter campaign. The study
area was also smaller than that in this work, as the flux footprint (i.e.
the upwind source area of the measured fluxes) was on average within 2 km
(maximal 7 km) of the tower. Compared to the measured fluxes, the emissions
rates were found to be overestimated by a mean factor of 9.9. They further
considered emissions only from the transport and residential sectors (as no
industrial or power sources were identified within the average footprint)
and reduced these by 30 %, yet these were still on average 3.3 times
higher than the fluxes. They also found much smoother diurnal variations in
the NO<inline-formula><mml:math id="M251" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> fluxes compared to those in the emission rates, indicating that
the night-time fraction was underestimated in the latter.</p>
      <p id="d1e3259">In the standard MEIC v1.3 (from which the a priori emissions were downscaled and re-gridded), annual NO<inline-formula><mml:math id="M252" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions from the transport sector were
estimated to be 1.05 <inline-formula><mml:math id="M253" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<inline-formula><mml:math id="M254" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">5</mml:mn></mml:msup></mml:math></inline-formula> Mg in Beijing and 6.59 <inline-formula><mml:math id="M255" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<inline-formula><mml:math id="M256" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">5</mml:mn></mml:msup></mml:math></inline-formula> Mg in Hebei Province in 2013. In 2016, these figures decreased to 8.87 <inline-formula><mml:math id="M257" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<inline-formula><mml:math id="M258" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msup></mml:math></inline-formula> and 5.68 <inline-formula><mml:math id="M259" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<inline-formula><mml:math id="M260" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">5</mml:mn></mml:msup></mml:math></inline-formula> Mg, respectively,
corresponding to reductions by 15.5 % and 13.8 %, which are
substantially lower than the reductions reported in this work. A slightly
larger reduction of 20 % (from 1.44 <inline-formula><mml:math id="M261" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<inline-formula><mml:math id="M262" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">5</mml:mn></mml:msup></mml:math></inline-formula> Mg in 2013 to
1.15 <inline-formula><mml:math id="M263" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<inline-formula><mml:math id="M264" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">5</mml:mn></mml:msup></mml:math></inline-formula> Mg in 2016) was estimated for vehicle (including on- and off-road vehicles) sources of NO<inline-formula><mml:math id="M265" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> in Beijing by
Cheng et al. (2019), who used a bottom-up emissions
inventory for Beijing which was compiled from the county level and
associated with finer spatial resolutions than MEIC established from the
province level. They also concluded that vehicle emission control measures
contributed the most to the total reductions in NO<inline-formula><mml:math id="M266" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions over this
period. According to the <italic>China Vehicle Environmental Management Annual Reports</italic>, NO<inline-formula><mml:math id="M267" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions from on-road vehicles were
7 <inline-formula><mml:math id="M268" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<inline-formula><mml:math id="M269" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msup></mml:math></inline-formula> Mg in Beijing and 5.2 <inline-formula><mml:math id="M270" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<inline-formula><mml:math id="M271" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">5</mml:mn></mml:msup></mml:math></inline-formula> Mg in Hebei
Province in 2013. These fell by 14 % and 10 %, respectively, to 6 <inline-formula><mml:math id="M272" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<inline-formula><mml:math id="M273" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msup></mml:math></inline-formula> and 4.7 <inline-formula><mml:math id="M274" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<inline-formula><mml:math id="M275" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">5</mml:mn></mml:msup></mml:math></inline-formula> Mg in 2016, despite an increase in vehicle ownership (Ministry of Environmental Protection of the
People's Republic of China, 2014, 2017).</p>
      <p id="d1e3466">The downward trends in traffic sources of NO<inline-formula><mml:math id="M276" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> between 2013 and 2016
found by this study, and the studies and reports mentioned above contrast
with the results in Xue et al. (2020). Based on yet another bottom-up emissions inventory for Beijing, they showed that mobile (i.e. on-road and off-road vehicles) sources of NO<inline-formula><mml:math id="M277" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> increased from 9.6 <inline-formula><mml:math id="M278" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<inline-formula><mml:math id="M279" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msup></mml:math></inline-formula> to 1.1 <inline-formula><mml:math id="M280" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<inline-formula><mml:math id="M281" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">5</mml:mn></mml:msup></mml:math></inline-formula> Mg over the same period. Though they found a 20 % reduction in the total anthropogenic
NO<inline-formula><mml:math id="M282" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions from 2013 to 2016, this was primarily attributed to
optimised energy structure in the industry, power and residential sectors.
In this study, we found that amongst the top-performing 5 % of the
adjusted PEE simulations, the reduction in total NO<inline-formula><mml:math id="M283" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions from the
base emissions varies between 59 % and 74 % (due to reductions from
transport sources only, with other sources fixed). These conflicting
findings again highlight the presence of inherent uncertainties in emissions
inventories, the impact of which on the results of this work is discussed in
the following, along with the impact of other sources of uncertainty.</p>
      <p id="d1e3538">Two types of uncertainties may be associated with the base emissions.
Inherent uncertainties due to underlying emission factors and activity rates
were estimated to be <inline-formula><mml:math id="M284" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula>31 % for NO<inline-formula><mml:math id="M285" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions in MEIC
(Cheng et al., 2019), which are smaller than the uncertainty
ranges in Table 1, suggesting that the trends in (real-world) emissions from
2013 to 2016 represent a larger source of uncertainty when using the 2013
base emissions for 2016 simulations. Additional uncertainties may have been
introduced when the standard MEIC v1.3 was downscaled and re-gridded to the
a priori emissions inventory used in this work. As an example,
Zheng et al. (2017) compared MEIC with
another emissions inventory with a much larger share of point sources (which
were allocated directly to grid cells) and different sets of spatial proxies
to allocate non-point sources. They found that NO<inline-formula><mml:math id="M286" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emission fluxes from
the most populated grid cells in Hebei Province were overestimated by
46 %–140 % in MEIC, mainly driven by spatial proxies that over-allocated industrial emissions to urban areas. Such uncertainties may have contributed to the spatial inhomogeneities of the biases in the base emissions revealed in Fig. 4 and, to a certain extent, propagated into the derived emission estimates, as spatially uniform perturbations were applied when constructing the adjusted PEE. Hence, biases in the spatial distribution of emissions may also be present in the a posteriori estimates, despite improvement in terms of the total
magnitude. In comparison, the propagation of inherent uncertainties in the
base emissions is of less concern. Though most emission parameters were
defined relative to the corresponding values in the base emissions for an
efficient perturbation, their uncertainty ranges were ultimately constrained
solely by the observations.</p>
      <p id="d1e3566">Uncertainties in the observational constraints are also twofold. While those
due to measurement errors are most likely small, as demonstrated by the
consistency in the results derived using two independent sets of
observations, the underrepresentation of the existing observations of power
and industrial sources prohibited an update of emission strengths from these
sources.</p>
      <p id="d1e3569">Another source of uncertainty is the input lateral boundary conditions which
include meteorology and background pollution levels. The impacts of
uncertainties in the input meteorological observations (i.e. due to
measurement errors) are minimal, as reported in Yuan et al. (2021) using simulations forced with perturbed meteorological data. The effect of uncertainties associated with different background concentrations of NO<inline-formula><mml:math id="M287" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> and O<inline-formula><mml:math id="M288" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> on the constrained NO<inline-formula><mml:math id="M289" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions is discussed next in the context of uncertainties in the underlying chemical mechanisms in ADMS-Urban.</p>
      <p id="d1e3599">The chemical partition of NO<inline-formula><mml:math id="M290" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions into 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> concentrations by
the model represents a potentially important source of uncertainty. Many
studies that infer NO<inline-formula><mml:math id="M292" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions from satellite observations of the
tropospheric NO<inline-formula><mml:math id="M293" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> column assumed an accurate representation of NO<inline-formula><mml:math id="M294" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>
chemistry in the CTM used. However, Valin et al. (2011) demonstrated the
presence of biases in the modelled NO<inline-formula><mml:math id="M295" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> column that are dependent on the
horizontal resolution of the model, which has implications on the inference
of NO<inline-formula><mml:math id="M296" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions when matching the modelled column to satellite
observations. These biases result from an inaccurate representation 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> lifetime (and thus concentration) at coarse resolution, which is
determined primarily by OH concentration in daytime, which, in turn, has a
non-linear dependence on NO<inline-formula><mml:math id="M298" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> concentration.</p>
      <p id="d1e3684">While 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> rapidly interconverts with NO in the presence of sunlight via
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> photolysis and reactions of NO with O<inline-formula><mml:math id="M301" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> and peroxy radicals, it
is also oxidised by hydroxyl radicals (OH) to nitric acid (HNO<inline-formula><mml:math id="M302" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>), which
can then be removed from the atmosphere via wet/dry deposition. At night, NO
oxidation continues, but it cannot be converted from 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> as no
photolysis takes place. With very low concentrations of OH, 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> is
mainly oxidised by O<inline-formula><mml:math id="M305" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> to form the nitrate radical (NO<inline-formula><mml:math id="M306" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>), which further
reacts with 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> and reaches an equilibrium with dinitrogen pentoxide
(N<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>O<inline-formula><mml:math id="M309" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">5</mml:mn></mml:msub></mml:math></inline-formula>). 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> also hydrolyses on aerosol surfaces to form
nitrous acid (HONO). NO<inline-formula><mml:math id="M311" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>, N<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>O<inline-formula><mml:math id="M313" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">5</mml:mn></mml:msub></mml:math></inline-formula> and HONO are described as
night-time reservoirs of NO<inline-formula><mml:math id="M314" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>, as they can regenerate NO or NO<inline-formula><mml:math id="M315" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
after sunrise (Seinfeld and Pandis, 2016). These reservoir
species are absent in the semi-empirical chemical mechanism in ADMS-Urban
described in Sect. 2.3.</p>
      <p id="d1e3843">The SNAQ measurements which included NO allowed for an evaluation of the
NO<inline-formula><mml:math id="M316" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> photolytic chemistry in ADMS-Urban. Han et al. (2011) demonstrated
the presence of a strong linear relationship between NO<inline-formula><mml:math id="M317" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> and NO during
night-time and between NO<inline-formula><mml:math id="M318" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> and NO<inline-formula><mml:math id="M319" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> during the day in observations
from Tianjin, another megacity not far from Beijing. Following this
approach, simple linear regression models were fitted to the SNAQ-measured
hourly averaged mixing ratios of NO and 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>, as a function of the
corresponding mixing ratios of NO<inline-formula><mml:math id="M321" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>. In addition, a linear function was
fitted between log-transformed mixing ratios of O<inline-formula><mml:math id="M322" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> and
(non-logarithmic) mixing ratios of NO<inline-formula><mml:math id="M323" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> due to a negative correlation
between the two (Fig. S9a). Additional linear functions were also fitted to
daytime or night-time data only. Data from the individual SNAQ sites were
not differentiated because of the short duration of operation at each site.
Consistent with findings by Han
et al. (2011), a good linear correlation can be found between the daytime
mixing ratios of 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> and NO<inline-formula><mml:math id="M325" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>, while there is a strong correlation
between night-time mixing ratios of NO and NO<inline-formula><mml:math id="M326" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>. The lowest coefficients
of determination are calculated for O<inline-formula><mml:math id="M327" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> as a function of NO<inline-formula><mml:math id="M328" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>, which
is consistent with the finding of Figs. 4 and 5 that O<inline-formula><mml:math id="M329" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>
concentrations are less strongly dependent on NO<inline-formula><mml:math id="M330" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions (Fig. S9b).</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="d1e3985">Slopes of linear regression models fitted between the modelled
hourly mixing ratios of NO, NO<inline-formula><mml:math id="M331" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, log-transformed O<inline-formula><mml:math id="M332" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> and those of
NO<inline-formula><mml:math id="M333" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> at all SNAQ sites by <bold>(a)</bold> the top-performing 5 % of the adjusted perturbed emissions ensemble simulations (PEE) and the base run, <bold>(b)</bold> the background concentration sensitivity simulations and the best PEE simulation R97, <bold>(c)</bold> the ROC concentration sensitivity simulations and the best PEE simulation R97, compared to the corresponding slopes fitted to SNAQ measurements. The slopes for log-transformed O<inline-formula><mml:math id="M334" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> as a function of NO<inline-formula><mml:math id="M335" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> are exponentiated. Details of the background concentration sensitivity simulations are provided in Table S3. The simulations Si and Sii represent a doubling and halving of the ROC concentrations (by modifying the reactivity coefficient) in R97, respectively. In all panels, daytime is defined as complete hours between sunrise and sunset in Beijing during November–December 2016, namely 08:00–15:00 LT.</p></caption>
        <?xmltex \igopts{width=355.659449pt}?><graphic xlink:href="https://acp.copernicus.org/articles/22/8617/2022/acp-22-8617-2022-f08.png"/>

      </fig>

      <p id="d1e4049">We then fitted linear models to the corresponding output (i.e. for the same
locations and time frame) from the top-performing 5 % of the adjusted PEE
simulations (see Sect. 3). These are compared with models fitted to the SNAQ
measurements with respect to the slope, as it indicates the number of
changes in NO, NO<inline-formula><mml:math id="M336" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and (log-transformed) O<inline-formula><mml:math id="M337" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> as NO<inline-formula><mml:math id="M338" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>
increases/decreases, which is directly related to the input NO<inline-formula><mml:math id="M339" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>
emissions. As can been seen from Fig. 8a, the modelled slopes of the linear
models between NO<inline-formula><mml:math id="M340" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and NO<inline-formula><mml:math id="M341" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> are higher, whereas modelled slopes for
NO as a function of NO<inline-formula><mml:math id="M342" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> are lower compared to those observed,
irrespective of the time of day. The discrepancies between modelled and
observed slopes for O<inline-formula><mml:math id="M343" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> as a function of NO<inline-formula><mml:math id="M344" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> are relatively small.
This suggests that with similar concentrations of NO<inline-formula><mml:math id="M345" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> as observed, the
top-performing adjusted PEE simulations tend to overestimate NO<inline-formula><mml:math id="M346" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> while
underestimating NO. In other words, lower NO<inline-formula><mml:math id="M347" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions may be needed
for the model to simulate NO<inline-formula><mml:math id="M348" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentrations that are consistent with
the observations. This suggests that the constrained emission estimates of
NO<inline-formula><mml:math id="M349" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> are indeed sensitive to the NO<inline-formula><mml:math id="M350" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> photolytic chemistry in
ADMS-Urban and, in this case, may be low-biased.</p>
      <p id="d1e4189">There are several possible explanations for the model's tendency to
partition more (less) NO<inline-formula><mml:math id="M351" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> into NO<inline-formula><mml:math id="M352" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> (NO). As described in Sect. 2.3, the reaction with O<inline-formula><mml:math id="M353" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> (Reaction R4) and reactions with the HO<inline-formula><mml:math id="M354" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> or
RO<inline-formula><mml:math id="M355" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> (Reaction R2) are the two pathways of NO oxidation to form NO<inline-formula><mml:math id="M356" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> in ADMS-Urban. Organic radicals are produced via Reaction (R1) in which ROC is defined as the proportion of TVOC that is reactive and calculated by
multiplying the TVOC concentrations with a reactivity coefficient. In
ADMS-Urban version 4.2 (used in this study), a coefficient of 0.1 is
adopted. It is set to 0.05 in the most up-to-date version 5
(Cambridge Environmental Research Consults Limited, 2017,
2020). As a secondary pollutant, modelled O<inline-formula><mml:math id="M357" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> concentrations depend on
the input background levels, for which there is no widely accepted
definition. To investigate the sensitivity of the model output to these two
NO oxidation pathways, a series of sensitivity simulations were performed.
All simulations were input with the same NO<inline-formula><mml:math id="M358" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> (and VOC) emissions as
R97, the adjusted PEE simulation with the best performance in simulating
hourly NO<inline-formula><mml:math id="M359" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentrations at the long-term monitoring sites. Again,
simple linear regression models were fitted between hourly mixing ratios of
NO, NO<inline-formula><mml:math id="M360" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, (log-transformed) O<inline-formula><mml:math id="M361" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> and NO<inline-formula><mml:math id="M362" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> output by these
simulations.</p>
      <p id="d1e4302">Figure 8b shows that different definitions of background NO<inline-formula><mml:math id="M363" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and/or
O<inline-formula><mml:math id="M364" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> (see Table S3) indeed have an impact on the modelled NO-to-NO<inline-formula><mml:math id="M365" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
conversion. For example, in the sensitivity simulation S5 input with the
lowest background levels of NO<inline-formula><mml:math id="M366" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and O<inline-formula><mml:math id="M367" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>, the modelled slopes for
NO<inline-formula><mml:math id="M368" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> as a function of NO<inline-formula><mml:math id="M369" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> are considerably lower than the
corresponding slopes modelled by R97 and thus closer to the observed
slopes. Also, the slopes between NO and NO<inline-formula><mml:math id="M370" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> associated with outputs
from S5 are higher than those found in outputs from R97 and agree better
with the observed slopes. However, it is important to underscore that this
does not suggest that the 10th percentile concentration is most
representative of the background concentrations of NO<inline-formula><mml:math id="M371" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and O<inline-formula><mml:math id="M372" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>. It
simply highlights the impact of the input background concentrations of
reactive pollutants on the model outputs of relevant species (and thus on
the emission estimates inferred on the basis of these model outputs), which
can be comparable to the impact of varying the input NO<inline-formula><mml:math id="M373" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions
(amongst the top-performing 5 % of the adjusted PEE simulations) shown in
Fig. 8a. This calls for further research into appropriate definitions for
background levels of NO<inline-formula><mml:math id="M374" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> and O<inline-formula><mml:math id="M375" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> within a vast and heterogeneous
urban area like the modelling domain in this study. Also, it is worth noting
that the modelled chemistry is also influenced by the input background
levels of NO. However, the specific sensitivities were not investigated, as
the upwind concentrations extracted from the CAMS reanalysis dataset are the
only set of NO observations available long-term.</p>
      <p id="d1e4425">The effect of organic radicals on the partition of NO<inline-formula><mml:math id="M376" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> between NO<inline-formula><mml:math id="M377" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
and NO is shown in Fig. 8c by varying the concentrations of ROC. As
explained above, ROC concentrations are controlled by both the TVOC
concentrations (that result from the input emissions and background levels
of VOC) and a reactivity coefficient which was set to 0.1 in R97 (as with
other adjusted PEE simulations). With fixed TVOC concentrations, using a
coefficient of 0.2 doubles the ROC available to produce HO<inline-formula><mml:math id="M378" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and
RO<inline-formula><mml:math id="M379" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, leading to an even more pronounced overestimation of NO<inline-formula><mml:math id="M380" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>,
accompanied by an underestimation of NO. In contrast, halving the ROC
concentrations by using a coefficient of 0.05 partitions less of the
NO<inline-formula><mml:math id="M381" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emitted into NO<inline-formula><mml:math id="M382" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>. This highlights that the emissions and
background concentrations of VOC (which are not evaluated in this study due
to a lack of observations) also have an impact on the modelled NO<inline-formula><mml:math id="M383" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>
photolytic chemistry and thus the a posteriori emission estimates of NO<inline-formula><mml:math id="M384" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>. It is also worth noting that biogenic VOCs are likely underestimated in the current simulations, as these are only represented by one of the eight species (i.e. isoprene) output by the CAMS reanalysis product used to approximate the background levels of TVOC and are not represented at all in the base emissions (which include anthropogenic sources only). Despite having low concentrations in the study area (compared to anthropogenic VOCs)
(Mo et al., 2018), they are associated with high radical
production and thus O<inline-formula><mml:math id="M385" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> creation potentials. Unlike background
concentrations of NO<inline-formula><mml:math id="M386" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> and O<inline-formula><mml:math id="M387" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>, however, the effect of VOCs on the
modelled NO<inline-formula><mml:math id="M388" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>–O<inline-formula><mml:math id="M389" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> chemistry is restricted to daylight hours, as they
only produce radicals in the presence of solar radiation in the model.</p>
      <p id="d1e4556">Another factor that affects the modelled NO<inline-formula><mml:math id="M390" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> photolytic chemistry is
the <inline-formula><mml:math id="M391" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula>-NO<inline-formula><mml:math id="M392" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> in the input emissions (see Sect. 3.1). Although not
investigated with sensitivity experiments, it can be expected that a higher
<inline-formula><mml:math id="M393" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula>-NO<inline-formula><mml:math id="M394" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> would result in higher NO<inline-formula><mml:math id="M395" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentrations and lower NO
concentrations simulated by the model, thus further increasing the
discrepancies between the modelled and observed slopes of linear functions,
whilst a lower <inline-formula><mml:math id="M396" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula>-NO<inline-formula><mml:math id="M397" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> would have the opposite effect.</p>
</sec>
<sec id="Ch1.S5" sec-type="conclusions">
  <label>5</label><title>Conclusions</title>
      <p id="d1e4635">We developed a novel approach to update a priori emission estimates using
ground-based network measurements as constraints and an ensemble of forward
simulations which are input with a PEE. Using this approach, we were able to
update the transport sector NO<inline-formula><mml:math id="M398" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions in Beijing from a 2013
emissions inventory for the year 2016. The updated emissions are
substantially lower with a higher proportion occurring at night-time and are
broadly consistent with findings of several previous studies. It would be
possible to also update emissions from other (non-negligible) source
sectors, provided that appropriate measurements were available.</p>
      <p id="d1e4647">As with existing emission optimisation techniques, this approach is
sensitive to the chemical mechanisms in the underlying model, the
uncertainties of which can be propagated into uncertainties in the emission
estimates. Nonetheless, this approach has several unique advantages.
Compared to inverse modelling techniques, the construction of a PEE and the
forward simulations is rapidly executable. Even when the Gaussian
dispersion model used in this study is replaced with a CTM for more explicit
representations of chemistry, the efficiency can be maintained via parallel
computing. Also, surface-based measurements of ambient concentrations are
used as constraints, which are readily available and closer to the sources
of emissions than the satellite-based measurements. This proximity to
emission sources may be particularly important for capturing the high
temporal and spatial variability of highly reactive species. For example,
Qu et al. (2021) found that in comparison to
surface concentrations, the NO<inline-formula><mml:math id="M399" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> column showed a muted response to the
step decrease in NO<inline-formula><mml:math id="M400" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions in the United States during the COVID-19 crisis.
Most importantly, this approach allows for an update of emissions by source
sector, which is more relevant for policy interventions than total
emissions, as they directly reflect the (in)effectiveness of the
corresponding pollution control measures. Hence, we believe that this
approach, particularly combined with low-cost sensors, has great potential
in providing timely updates of emissions in regions undergoing rapid
changes, where emissions inventories may be biased or outdated as soon as
they have been compiled, and computing facilities may be limited.</p>
</sec>

      
      </body>
    <back><notes notes-type="codedataavailability"><title>Code and data availability</title>

      <p id="d1e4672">Codes used to generate the perturbed emissions ensemble using the R language are available at <uri>https://github.com/yuanle731/PEE</uri> (last access: 28 June 2022; <ext-link xlink:href="https://doi.org/10.5281/zenodo.6778166" ext-link-type="DOI">10.5281/zenodo.6778166</ext-link>, Yuan, 2022). The Multi-resolution Emission Inventory for China (MEIC) is available upon request at <uri>http://www.meicmodel.org</uri> (last access: 28 June 2022). Long-term air quality monitoring data from Beijing are archived at <uri>https://quotsoft.net/air/</uri>, and the 2016 data used in this work are available at <ext-link xlink:href="https://doi.org/10.17863/CAM.85111" ext-link-type="DOI">10.17863/CAM.85111</ext-link> (Beijing Municipal Ecological and Environmental Monitoring Center and Wang, 2022).</p>
  </notes><app-group>
        <supplementary-material position="anchor"><p id="d1e4690">The supplement related to this article is available online at: <inline-supplementary-material xlink:href="https://doi.org/10.5194/acp-22-8617-2022-supplement" xlink:title="pdf">https://doi.org/10.5194/acp-22-8617-2022-supplement</inline-supplementary-material>.</p></supplementary-material>
        </app-group><notes notes-type="authorcontribution"><title>Author contributions</title>

      <p id="d1e4699">LY developed the methodology with advice from ATA and performed and analysed the model simulations with advice from ATA, OAMP, RLJ, CH, DC, HZS and HL. OAMP and RLJ provided the low-cost sensor measurements and advised on data processing. CH and DC provided the licence of ADMS-Urban and advised on the simulation setup. QZ provided the Multi-resolution Emission Inventory for China. LY prepared the manuscript with contributions from all co-authors.</p>
  </notes><notes notes-type="competinginterests"><title>Competing interests</title>

      <p id="d1e4705">At least one of the (co-)authors is a member of the editorial board of <italic>Atmospheric Chemistry and Physics</italic>. The peer-review process was guided by an independent editor, and the authors also have no other competing interests to declare.</p>
  </notes><notes notes-type="disclaimer"><title>Disclaimer</title>

      <p id="d1e4714">Publisher’s note: Copernicus Publications remains neutral with regard to jurisdictional claims in published maps and institutional affiliations.</p>
  </notes><ack><title>Acknowledgements</title><p id="d1e4720">This work was supported by the Royal Society of the United Kingdom through a
Newton Advanced Fellowship (NAF/R1/201166) and the Tsinghua University Initiative Scientific Research Program. Alexander T. Archibald acknowledges the National Centre for Atmospheric Science and the Met
Office through the Clean Air SPF for funding. We thank Oliver Wild, Michael
Hollaway and Michael Biggart for processing the base emissions. Thanks also
go to Sue Grimmond and Simone Kotthaus for providing mixed-layer height
measurements and comments on the manuscript.</p></ack><notes notes-type="financialsupport"><title>Financial support</title>

      <p id="d1e4725">This research has been supported by the Royal Society of the United Kingdom through a Newton Advanced Fellowship (grant no. NAF/R1/201166), the Tsinghua University Initiative Scientific Research Program, the National Centre for Atmospheric Science (Clean Air SPF) and the Met Office (Clean Air SPF).</p>
  </notes><notes notes-type="reviewstatement"><title>Review statement</title>

      <p id="d1e4731">This paper was edited by Andreas Hofzumahaus and reviewed by two anonymous referees.</p>
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