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  <front>
    <journal-meta><journal-id journal-id-type="publisher">ACP</journal-id><journal-title-group>
    <journal-title>Atmospheric Chemistry and Physics</journal-title>
    <abbrev-journal-title abbrev-type="publisher">ACP</abbrev-journal-title><abbrev-journal-title abbrev-type="nlm-ta">Atmos. Chem. Phys.</abbrev-journal-title>
  </journal-title-group><issn pub-type="epub">1680-7324</issn><publisher>
    <publisher-name>Copernicus Publications</publisher-name>
    <publisher-loc>Göttingen, Germany</publisher-loc>
  </publisher></journal-meta>
    <article-meta>
      <article-id pub-id-type="doi">10.5194/acp-18-4171-2018</article-id><title-group><article-title>Evaluation of modeling NO<inline-formula><mml:math id="M1" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentrations driven by satellite-derived
and bottom-up emission inventories<?xmltex \hack{\break}?> using in situ measurements over China</article-title><alt-title>Evaluation of modeling NO<inline-formula><mml:math id="M2" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentrations over China</alt-title>
      </title-group><?xmltex \runningauthor{F. Liu et al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes" rid="aff1 aff2 aff3">
          <name><surname>Liu</surname><given-names>Fei</given-names></name>
          <email>fei.liu@nasa.gov</email><email>liuf1010@gmail.com</email>
        <ext-link>https://orcid.org/0000-0002-0357-0274</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>van der A</surname><given-names>Ronald J.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-0077-5338</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Eskes</surname><given-names>Henk</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-8743-4455</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff4">
          <name><surname>Ding</surname><given-names>Jieying</given-names></name>
          
        <ext-link>https://orcid.org/0000-0003-1263-2876</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Mijling</surname><given-names>Bas</given-names></name>
          
        </contrib>
        <aff id="aff1"><label>1</label><institution>Royal Netherlands Meteorological Institute (KNMI), Department of
Satellite Observations, De Bilt, the Netherlands</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>Universities Space Research Association (USRA), GESTAR, Columbia, MD,
USA</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>NASA Goddard Space Flight Center, Greenbelt, MD, USA</institution>
        </aff>
        <aff id="aff4"><label>4</label><institution>Department of Geoscience and Remote Sensing (GRS), Delft University of
Technology, Delft, the Netherlands</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Fei Liu (fei.liu@nasa.gov, liuf1010@gmail.com)</corresp></author-notes><pub-date><day>27</day><month>March</month><year>2018</year></pub-date>
      
      <volume>18</volume>
      <issue>6</issue>
      <fpage>4171</fpage><lpage>4186</lpage>
      <history>
        <date date-type="received"><day>19</day><month>May</month><year>2017</year></date>
           <date date-type="rev-request"><day>28</day><month>August</month><year>2017</year></date>
           <date date-type="rev-recd"><day>1</day><month>March</month><year>2018</year></date>
           <date date-type="accepted"><day>2</day><month>March</month><year>2018</year></date>
      </history>
      <permissions>
        
        
      <license license-type="open-access"><license-p>This work is licensed under the Creative Commons Attribution 3.0 Unported License. To view a copy of this licence, visit <ext-link ext-link-type="uri" xlink:href="https://creativecommons.org/licenses/by/3.0/">https://creativecommons.org/licenses/by/3.0/</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>
    <p id="d1e156">Chemical transport models together with emission inventories are widely used
to simulate NO<inline-formula><mml:math id="M3" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentrations over China, but validation of the
simulations with in situ measurements has been extremely limited. Here we use
ground measurements obtained from the air quality monitoring network recently
developed by the Ministry of Environmental Protection of China to validate
modeling surface NO<inline-formula><mml:math id="M4" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentrations from the CHIMERE regional
chemical transport model driven by the satellite-derived DECSO and the
bottom-up MIX emission inventories. We applied a correction factor to the
observations to account for the interferences of other oxidized nitrogen
compounds (NO<inline-formula><mml:math id="M5" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mi>z</mml:mi></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>, based on the modeled ratio of 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> to NO<inline-formula><mml:math id="M7" display="inline"><mml:msub><mml:mi/><mml:mi>z</mml:mi></mml:msub></mml:math></inline-formula>.
The model accurately reproduces the spatial variability in 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> from
in situ measurements, with a spatial correlation coefficient of over 0.7 for
simulations based on both inventories. A negative and positive bias is found
for the simulation with the DECSO (slope <inline-formula><mml:math id="M9" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 0.74 and 0.64 for the
daily mean and daytime only) and the MIX (slope <inline-formula><mml:math id="M10" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 1.3 and 1.1)
inventories,
respectively, suggesting an underestimation and overestimation of NO<inline-formula><mml:math id="M11" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>
emissions from corresponding inventories. The bias between observed and
modeled concentrations is reduced, with the slope dropping from 1.3 to 1.0
when the spatial distribution of NO<inline-formula><mml:math id="M12" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions in the DECSO inventory is
applied as the spatial proxy for the MIX inventory, which suggests an
improvement of the distribution of emissions between urban and suburban or rural
areas in the DECSO inventory compared to that used in the bottom-up
inventory. A rough estimate indicates that the observed concentrations, from
sites predominantly placed in the populated urban areas, may be 10–40 %
higher than the corresponding model grid cell mean. This reduces the estimate
of the negative bias of the DECSO-based simulation to the range of <inline-formula><mml:math id="M13" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>30 to
0 % on average and more firmly establishes that the MIX inventory is
biased high over major cities. The performance of the model is comparable
over seasons, with a slightly worse spatial correlation in summer due to the
difficulties in resolving the more active NO<inline-formula><mml:math id="M14" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> photochemistry and larger
concentration gradients in summer by the model. In addition, the model well
captures the daytime diurnal cycle but shows more significant disagreement
between simulations and measurements during nighttime, which likely produces
a positive model bias of about 15 % in the daily mean concentrations.
This is most likely related to the uncertainty in vertical mixing in the
model at night.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <title>Introduction</title>
      <p id="d1e273">Nitrogen dioxide (NO<inline-formula><mml:math id="M15" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> is an important trace gas in the troposphere. It
actively participates in the formation of tropospheric ozone and secondary
aerosols (Seinfeld and Pandis, 2006), which influences human health and
impacts climate significantly. Emissions of NO<inline-formula><mml:math id="M16" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> together with nitric
oxide (NO) that is rapidly converted to 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> in the troposphere during
daytime are closely related to anthropogenic activities, in particular
fossil fuel consumption, which has increased global NO<inline-formula><mml:math id="M18" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> (NO <inline-formula><mml:math id="M19" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> NO<inline-formula><mml:math id="M20" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> emissions by a factor of 3–6 since<?pagebreak page4172?> preindustrial times
(Prather et al., 2001). China is one of the largest contributors to NO<inline-formula><mml:math id="M21" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>
emissions over the world, contributing 18 % of global NO<inline-formula><mml:math id="M22" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>
emissions based on the estimate of EDGAR v4.2 (European Commission (EC):
Joint Research Centre (JRC)/Netherlands Environmental Assessment Agency
(PBL), 2011), as a consequence of the large energy consumption driven by the
rapidly growing economy. A good understanding of NO<inline-formula><mml:math id="M23" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> levels as well as
temporal and spatial variations is urgent to help solve the serious
environmental problems, particularly poor air quality, caused by emissions.</p>
      <p id="d1e362">Chemical transport models (CTMs) have been widely used to provide predictions
of gas-phase pollutants including NO<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 particulate matter
concentrations, which are powerful tools for understanding regional air
pollution issues, assessing emission control scenarios (Kiesewetter et al.,
2014), and analyzing trans-boundary transport (Streets et al., 2007). The
modeled NO<inline-formula><mml:math id="M25" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentrations have received extensive evaluation by
comparing with ground-based measurements (Pay et al., 2012), satellite
observations (Huijnen et al., 2010), and airborne observations (Carmichael et
al., 2003) for regional (Stern et al., 2008) and urban-scale (Terrenoire et
al., 2015) air quality simulations. The results of these intercomparisons
show quite good performance of the models but still suggest uncertainties in
the estimation of the meteorological input data (Bessagnet et al., 2016), the
modeling of NO<inline-formula><mml:math id="M26" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> chemistry (Valin et al., 2011), and particularly
emission inventories (Mues et al., 2014).</p>
      <p id="d1e392">Emission inventories are necessary input to CTMs and recognized as one of
the most important sources of uncertainties. Traditional bottom-up emissions
are calculated by aggregating information from diverse sources of
information such as fuel statistics and measurements of emission factors.
The large uncertainties in energy statistics (Guan et al., 2012) and
applications of non-Chinese emission factors (Streets et al., 2003) have
been propagated into uncertainties in bottom-up inventories for China (Zhao
et al., 2011). The lack of bottom-up inventories for most recent years
introduces additional biases for model simulations because inventories
could quickly become outdated due to the rapidly changing emissions (Zhang
et al., 2007; Liu et al., 2016a). 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> columns detected from space
provide additional constraints to yield a satellite-derived NO<inline-formula><mml:math id="M28" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>
emission inventory. Initially, NO<inline-formula><mml:math id="M29" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions have been estimated from
satellite observations together with CTMs at coarse resolution based on the
assumption of a linear relationship between NO<inline-formula><mml:math id="M30" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> columns and NO<inline-formula><mml:math id="M31" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>
emissions ignoring pollution transport (Martin et al., 2003). More
complicated techniques like the Kalman filter (Napelenok et al., 2008) and
four-dimensional variational data assimilation (4D-Var) (Kurokawa et al.,
2009) have been introduced to take pollution transport into account. In
addition, CTM-independent methods have been developed for point sources
(Beirle et al., 2011; Liu et al., 2016b). The uncertainties in NO<inline-formula><mml:math id="M32" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
column retrievals (Dirksen et al., 2011), in particular for China with high
loadings of aerosols (Ma et al., 2013), together with estimation method
uncertainties result in errors in satellite-derived inventories.</p>
      <p id="d1e450">The modeling of NO<inline-formula><mml:math id="M33" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentrations over China has been evaluated with
space- and ground-based observations. Reported validation studies have
focused on evaluating tropospheric NO<inline-formula><mml:math id="M34" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> column densities simulated by
CTMs driven by bottom-up emission inventories using satellite measurements.
Differences between the simulated NO<inline-formula><mml:math id="M35" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> column densities and observations
of the Global Ozone Monitoring Experiment (GOME) (Ma et al., 2006; Uno et
al., 2007), the Scanning Imaging Absorption Spectrometer for Atmospheric
CHartographY (SCIAMACHY) (Shi et al., 2008), and the Ozone Monitoring
Instrument (OMI) (Wang et al., 2011) have been attributed to uncertainties in
the magnitude and spatial distribution of bottom-up emissions. The validation
of surface 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> concentrations was generally performed for limited time
periods using a limited set of measurement stations (e.g., three large cities
in Wang et al., 2011, one or two sites in Wang et al., 2007, and the city of
Nanjing in Ding et al., 2015), due to the absence of routine monitoring
data. Alternatively, the satellite-derived inventories were compared to
bottom-up inventories directly, which shows considerable disparity (Lin et
al., 2012; Ding et al., 2017a).</p>
      <p id="d1e490">Measurements obtained from the recently developed air quality monitoring
network in China (Zhang and Cao, 2015) provide the means to evaluate the
quality of 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> modeling. We evaluate the surface NO<inline-formula><mml:math id="M38" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
concentrations simulated by a CTM driven by both satellite-derived and
bottom-up inventories with this newly established dataset. To our knowledge,
this is the first time that modeled 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> concentrations over China have
been evaluated with in situ measurements throughout the country, while an
intercomparison for simulations with satellite-derived and bottom-up
inventories is performed simultaneously. We structure the paper as follows.
In Sect. 2.1 and 2.2 the CTM and emission inventories adopted in this study
are described, respectively. The introduction of the in situ measurements from
the air quality monitoring network in China and the correction for
interference of in situ NO<inline-formula><mml:math id="M40" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> data are given in Sect. 2.3 and 2.4,
respectively. Annual mean simulated surface NO<inline-formula><mml:math id="M41" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> values are compared with the
corrected in situ measurements in Sect. 3.1. Further analyses focusing on
seasonality and diurnal cycle are provided in Sect. 3.2 and 3.3, respectively.
Section 4 presents a summary of the major findings in this paper.</p>
</sec>
<sec id="Ch1.S2">
  <title>Methodology</title>
<sec id="Ch1.S2.SS1">
  <title>CHIMERE model</title>
      <p id="d1e549">We used the CHIMERE regional chemical transport model in this study, which is
designed to produce daily forecasts of tropospheric trace gas and aerosol
pollutants and make long-term simulations at a range of spatial scales<?pagebreak page4173?> (Menut
et al., 2013). We use the CHIMERE model v2013b over East Asia (18 to
50<inline-formula><mml:math id="M42" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N and 102 to 132<inline-formula><mml:math id="M43" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E) with a resolution of 0.25<inline-formula><mml:math id="M44" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>
following the configuration in Ding et al. (2015). The CHIMERE simulation was
driven by operational meteorological data from the European Centre for
Medium-Range Weather Forecasts (ECMWF) with a horizontal resolution of
0.25<inline-formula><mml:math id="M45" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>. Atmospheric variables were simulated in eight layers from the
surface to 500 hPa. Tropospheric photochemistry is represented using the
reduced MELCHIOR chemical mechanism (Derognat et al., 2003), including about
120 reactions and 44 gaseous species. An aerosol module accounting both for
inorganic and organic species of primary or secondary origin is included
according to Bessagnet et al. (2004). Boundary conditions for the model
domain were derived from monthly mean climatology based on the second-generation Model for OZone
And Related chemical Tracers (MOZART) (Horowitz et al.,
2003) for gases, the Laboratoire de Météorologie Dynamique Zoom –
Interaction avec la Chimie et les Aérosols (LMDz-INCA; Folberth et al.,
2006) for nitrate and ammonium, and the Georgia Tech/Goddard Global Ozone
Chemistry Aerosol Radiation and Transport (GOCART; Ginoux et al., 2001) for
other aerosols. At default, NO<inline-formula><mml:math id="M46" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions are speciated as 9.2 % of
NO<inline-formula><mml:math id="M47" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, 0.8 % of HONO, and 90 % of NO in the CHIMERE model (Menut et
al., 2013), following the Generation of European Emission Data for Episodes
(GENEMIS) recommendations (Friedrich, 2000; Kurtenbach et al., 2001; Aumont
et al., 2003). Open-access satellite-derived and bottom-up inventories that
provide up-to-date emissions over East Asia were selected to drive the model
in this study, which will be detailed in Sect. 2.2.</p>
</sec>
<sec id="Ch1.S2.SS2">
  <title>Emission inventory</title>
      <p id="d1e613">The satellite-derived NO<inline-formula><mml:math id="M48" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions were estimated by the algorithm
DECSO (Daily Emission estimates Constrained by Satellite Observations) v5
using an extended Kalman filter (Mijling and van der A, 2012; Ding et al.,
2015, 2017b). DECSO uses one forward model run of a CTM to calculate the
response of 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> concentrations to both local and nonlocal NO<inline-formula><mml:math id="M50" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>
emissions. Daily OMI NO<inline-formula><mml:math id="M51" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> observations retrieved with the DOMINO version
2 algorithm (Boersma et al., 2011) are used as a constraint to update
emissions. The DECSO emission data are available at
<uri>www.globemission.eu</uri> (last access: 20 March 2018).</p>
      <p id="d1e655">The bottom-up anthropogenic NO<inline-formula><mml:math id="M52" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions were taken from the MIX
inventory (Li et al., 2017a), a mosaic Asian anthropogenic emission inventory
under the international collaboration framework of the Model Inter-Comparison
Study for Asia (MICS-Asia) and the Task Force on Hemispheric Transport of Air
Pollution (TF HTAP). The MIX inventory is developed for the years 2008 and
2010 by an integration of state-of-the-art regional emission inventories for
all major anthropogenic sources in 29 countries and regions over Asia. The
emissions of China integrated in the MIX inventory are derived from the
Multi-resolution Emission Inventory for China (MEIC:
<uri>http://www.meicmodel.org</uri>, last access: 20 December 2017)
compiled by Tsinghua University. The anthropogenic emissions together with
the biogenic emissions, which were computed automatically in the CHIMERE
model using the global MEGAN (Model of Emissions of Gases and Aerosols from
Nature) model (Guenther et al., 2006), were adopted as the bottom-up inventory.
We refer to this combination as the MIX inventory for brevity hereinafter.
Note that monthly emissions for all inventories above were provided at the
spatial resolution of 0.25<inline-formula><mml:math id="M53" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M54" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.25<inline-formula><mml:math id="M55" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>.</p>
      <p id="d1e695">Both inventories show comparable spatial distributions at national and
regional scales, but distinctions between urban and rural areas (see
Sect. 3.1). The strength of the MIX inventory is that it includes detailed
source-category information (e.g., power plant and transportation sector) for
emissions, which is useful for driving atmospheric models and designing
emission mitigation policies but is not included in DECSO. The advantage of
the DECSO inventory is that emissions are timely updated (as soon as the
satellite observations are available); while bottom-up inventories usually
lag behind a few years and are outdated by the time they become available. In
addition, the spatial information in DECSO is based on OMI NO<inline-formula><mml:math id="M56" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
observations, while MIX relies on spatial proxies like
gross domestic product (GDP) to
allocate emissions due to the lack of data. An in-depth comparison between
inventories has been described by Ding et al. (2017).</p>
      <p id="d1e707">We focused on 2015 as the most recent year with available DECSO emission
estimates and in situ measurements, but we used the MIX inventory for 2010
because the year 2015 is not available yet. However, the use of the 2010 MIX
inventory without scaling is not expected to bring significant bias, as the
similarity of 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 for 2010 and 2015 has been reported by both
the bottom-up inventory MEIC (Liu et al., 2016a) and the satellite-derived
inventory DECSO. For the period of 2010–2012, the NO<inline-formula><mml:math id="M58" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions of
China experienced a rapid growth. A sharp decline in 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 was
observed in the years of 2013–2015, with a peak around 2012 (Liu et al.,
2016a). As a result, the inventory for 2010 is comparable to that for 2015,
even though there is a 5-year lag. Figure 1 compares DECSO 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 for 2015 (a) and 2010 (b), which are consistent in both total
amount (21.5 vs. 21.6 Tg) and spatial distribution (<inline-formula><mml:math id="M61" display="inline"><mml:mi>r</mml:mi></mml:math></inline-formula> <inline-formula><mml:math id="M62" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 0.83).
Figure 1 further displays the spatial distributions of the MIX 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 for 2010 (c). These emissions are significantly higher (39 %)
than the DECSO inventory when averaged over the model domain.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1" specific-use="star"><caption><p id="d1e773">Maps for NO<inline-formula><mml:math id="M64" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions in the DECSO inventory, 2015
<bold>(a)</bold>; the DECSO inventory, 2010 <bold>(b)</bold>; and the MIX Asian
inventory, 2010 <bold>(c)</bold>. The unit is gigagrams of NO<inline-formula><mml:math id="M65" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> per grid cell.</p></caption>
          <?xmltex \igopts{width=497.923228pt}?><graphic xlink:href="https://acp.copernicus.org/articles/18/4171/2018/acp-18-4171-2018-f01.png"/>

        </fig>

      <p id="d1e809">An air quality simulation using the CHIMERE model was conducted for the full
year 2015. Pollutant concentrations including NO<inline-formula><mml:math id="M66" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> were simulated based
on the 2015 DECSO and the 2010 MIX NO<inline-formula><mml:math id="M67" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> inventories, respectively. Note
that the 2010 MIX inventory for other species was used together with both
NO<inline-formula><mml:math id="M68" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> inventories. Because of the inconsistency between the emission
sectors used in the DECSO and the MIX<?pagebreak page4174?> inventories and that in SNAP (Selected
Nomenclature for Air Pollution) 97, which is internally used in the CHIMERE
model, we adopted the sector mapping table as discussed in Ding et
al. (2015). The concentration in the lowest model layer (from the ground up
to 20 m) was used for validation against surface NO<inline-formula><mml:math id="M69" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> observations in
this study. Figure 2 illustrates the annual mean surface NO<inline-formula><mml:math id="M70" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> simulation
using both inventories. Large enhancements are found over industrial regions,
in particular northern China, the North China Plain, and the Yangtze River Delta. The
model run based on the MIX inventory (Fig. 2b) shows overall larger
concentrations than that based on the DECSO inventory (Fig. 2a).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2" specific-use="star"><caption><p id="d1e859">Annual mean surface NO<inline-formula><mml:math id="M71" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentration in 2015 based on the
CHIMERE model driven by the DECSO inventory, 2015 <bold>(a)</bold>; the MIX Asian
inventory, 2010 <bold>(b)</bold>; and the corrected DECSO inventory <bold>(c)</bold>.</p></caption>
          <?xmltex \igopts{width=497.923228pt}?><graphic xlink:href="https://acp.copernicus.org/articles/18/4171/2018/acp-18-4171-2018-f02.png"/>

        </fig>

</sec>
<sec id="Ch1.S2.SS3">
  <title>Ground-level in situ measurements</title>
      <p id="d1e892">The real-time hourly NO<inline-formula><mml:math id="M72" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentrations as well as other major air
pollutants are continuously recorded by the Ministry of Environmental
Protection (MEP) in China and are publicly accessible from the year 2013
onwards (Zhang and Cao, 2015). We obtained the hourly in situ measurements
from a total of 1413 air quality monitoring sites of the MEP network for 323
major cities over the model domain. The majority of those monitoring sites
have
been placed in the city center and are named urban assessing stations in the
official document (MEP, 2013). These are meant to evaluate the overall level
and trend of air quality for areas with the highest concentrations and
highest population exposure. The placement criteria of urban assessing
stations laid down in the legislation (MEP, 2013) ensure that the
measurements are representative for urban areas. Stations are required to be
well distributed within the developed area of the city and not too close to
stationary emission sources (50 m) or roads (10–100 m depending on the
traffic flow). The minimum number of monitoring sites required per city
depends on both the urban population and city size, i.e., at least one
station for an area of <inline-formula><mml:math id="M73" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 50 km<inline-formula><mml:math id="M74" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula> (Table 1). In addition, for areas
with the concentration exceeding grade II of the national ambient air quality
standard (i.e., the annual mean NO<inline-formula><mml:math id="M75" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentration of
40 <inline-formula><mml:math id="M76" display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>g m<inline-formula><mml:math id="M77" 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>; MEP,
2012), the minimum required number of monitoring sites is increased by
50 %. MEP also operates other types of measurement sites, including
regional and background stations to assess the background air pollution
levels and pollutant transport, and source impact and traffic stations close
to emission sources. However, only megacities like Beijing and Guangzhou
operate such non-urban stations. The fact that urban observations
dominate should be kept in mind when comparing the observations with the
model results. The horizontal resolution of the model is limited to
0.25<inline-formula><mml:math id="M78" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>, which will cause representativeness errors (biases) when
comparing the measurements from city stations with the mean of a grid box of
the simulations, which can also include rural areas. Note that only the
measurements for the dates with 24 h valid measurements (larger than 0) are
used for the following analysis in this study.</p>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T1"><caption><p id="d1e961">The requirement for the minimum number of urban stations.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="3">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="right"/>
     <oasis:colspec colnum="3" colname="col3" align="right"/>
     <oasis:thead>
       <oasis:row>  
         <oasis:entry colname="col1">Population of</oasis:entry>  
         <oasis:entry colname="col2">Area of</oasis:entry>  
         <oasis:entry colname="col3">Minimum number</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">  
         <oasis:entry colname="col1">built-up areas/k</oasis:entry>  
         <oasis:entry colname="col2">built-up areas/km<inline-formula><mml:math id="M79" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula></oasis:entry>  
         <oasis:entry colname="col3">of stations</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>  
         <oasis:entry colname="col1">&lt; 250</oasis:entry>  
         <oasis:entry colname="col2">&lt; 20</oasis:entry>  
         <oasis:entry colname="col3">1</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">250–500</oasis:entry>  
         <oasis:entry colname="col2">20–50</oasis:entry>  
         <oasis:entry colname="col3">2</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">500–1000</oasis:entry>  
         <oasis:entry colname="col2">50–100</oasis:entry>  
         <oasis:entry colname="col3">4</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">1000–2000</oasis:entry>  
         <oasis:entry colname="col2">100–200</oasis:entry>  
         <oasis:entry colname="col3">6</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">2000–3000</oasis:entry>  
         <oasis:entry colname="col2">200–400</oasis:entry>  
         <oasis:entry colname="col3">8</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">&gt; 3000</oasis:entry>  
         <oasis:entry colname="col2">&gt; 400</oasis:entry>  
         <oasis:entry colname="col3">10 (1 per 50–60 km<inline-formula><mml:math id="M80" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula>)</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table></table-wrap>

      <p id="d1e1095">Figure 3a displays the heterogeneous spatial distribution of monitoring sites
at the scale of the model grid cell. The over 1000 monitoring sites are
allocated to a total of 594 grid cells based on their geolocations. The sites
belonging to the grid cells with one, two, and three sites account for 17,
21,
and 22 % of the total, respectively (Fig. 3b). We calculated the averaged
distance between monitoring sites by averaging individual pairwise distances
for every two stations in the same grid cell. Because most monitoring sites
are urban stations and are clustered in the city areas, which are often much
smaller than the area of a grid cell (<inline-formula><mml:math id="M81" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 600 km<inline-formula><mml:math id="M82" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>, the averaged
distance is rather small with an average of 3.6 km for all grid<?pagebreak page4175?> cells as
shown in Fig 3c. For megacities with significantly larger built-up areas and
thus more monitoring sites, the distribution of sites is more homogeneous
over the grid cell and results in a lager distance between stations. The
average distance increases from 5 km for grid cells with only one pair of
stations to 11 km for those with over eight stations.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3" specific-use="star"><caption><p id="d1e1120"><bold>(a)</bold> Spatial distribution of in situ measurements. Measurements are
allocated to the CHIMERE model grid cells based on their geolocations. The
magnitude of the size of symbols denotes the number of stations located in
the same grid cell. The color of the symbols denotes the average distance
between stations located in the same grid cell. Triangles and “M”
denote sites located in mountainous areas. <bold>(b)</bold> Histogram of the total number
of grid cells with a certain number of stations. <bold>(c)</bold> Statistics of the
averaged distance among stations located in the same grid cell. The black
and blue horizontal lines are the median and mean of the averaged distance,
respectively; the box denotes the 25 and 75 % percentiles, and the
whiskers denote the 10 and 90 % percentiles. The grey dots denote the
outliers.</p></caption>
          <?xmltex \igopts{width=392.648031pt}?><graphic xlink:href="https://acp.copernicus.org/articles/18/4171/2018/acp-18-4171-2018-f03.png"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4"><caption><p id="d1e1139">Daily mean surface NO<inline-formula><mml:math id="M83" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentrations (<inline-formula><mml:math id="M84" display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>g m<inline-formula><mml:math id="M85" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>
of stations located in the city of Xi'an for the year 2015. The data are
calculated based on the measurements from the air quality monitoring network
of MEP. The measurements from the stations corresponding to the maximum and
minimum annual mean NO<inline-formula><mml:math id="M86" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentrations are displayed in red and blue,
respectively. The measurements from the urban station with lower NO<inline-formula><mml:math id="M87" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
concentrations than suburban stations are displayed in black.</p></caption>
          <?xmltex \igopts{width=233.312598pt}?><graphic xlink:href="https://acp.copernicus.org/articles/18/4171/2018/acp-18-4171-2018-f04.png"/>

        </fig>

      <p id="d1e1197">In our analysis, we excluded in situ measurements from cities with
unexpected discrepancies between urban and suburban stations. Because only
large cities potentially place the monitoring sites outside urban areas
related to the rapid expansion of built-up areas, we classified stations as
urban and suburban by visually inspecting satellite imagery from Google
Earth for large cities with over four stations. We calculated the annual
mean NO<inline-formula><mml:math id="M88" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> of each station. When the NO<inline-formula><mml:math id="M89" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentration of urban
stations is less than that of suburban stations, the measurements
behave differently than expected. The cities (four in total) detected to
have unexpected measurements are labeled as “unselected” and discarded
from the validation dataset. Note that suburban stations presenting higher
NO<inline-formula><mml:math id="M90" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> levels than urban stations but close to large emission sources,
e.g., industrial park and airport, are understandable and thus are not
excluded from the database. Figure 4 presents the daily average surface
NO<inline-formula><mml:math id="M91" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> abundance for the city of Xi'an. Only the dates with 24 h valid
measurements (lager than 0) are used for the time series illustration here.
The expected enhancement in winter highlighted by both urban (red line) and
suburban (blue line) stations has not been detected for the urban station
with lower annual mean NO<inline-formula><mml:math id="M92" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> abundance than suburban stations (black
line), which provides further support for excluding the Xi'an measurements
from the model evaluation.</p>
</sec>
<sec id="Ch1.S2.SS4">
  <title>Correction factor</title>
      <p id="d1e1251">NO<inline-formula><mml:math id="M93" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentrations are measured using commercial chemiluminescence
analyzers (Zhang and Cao, 2015), which are subject to a systematic
overestimation of ambient NO<inline-formula><mml:math id="M94" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentrations (Steinbacher et al.,
2007). 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> is catalytically transformed into NO by a molybdenum
converter and subsequently measured with chemiluminescence. However, other
reactive oxidized nitrogen compounds (NO<inline-formula><mml:math id="M96" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mi>z</mml:mi></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> such as peroxyacetyl nitrate
(PAN) and nitric acid are also partly converted to NO, resulting in an
overestimation of the measured NO<inline-formula><mml:math id="M97" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>.</p>
      <p id="d1e1302">We applied a correction factor proposed by Lamsal et al. (2008) to account
for the interferences of other oxidized nitrogen compounds, based on the
modeled ratio of 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> to NO<inline-formula><mml:math id="M99" display="inline"><mml:msub><mml:mi/><mml:mi>z</mml:mi></mml:msub></mml:math></inline-formula>. The correction factor (CF) was
calculated from the local chemical concentrations as follows:
            <disp-formula id="Ch1.E1" content-type="numbered"><mml:math id="M100" display="block"><mml:mrow><mml:mi mathvariant="normal">CF</mml:mi><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msub><mml:mrow class="chem"><mml:mi mathvariant="normal">NO</mml:mi></mml:mrow><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow><mml:mrow><mml:msub><mml:mrow class="chem"><mml:mi mathvariant="normal">NO</mml:mi></mml:mrow><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:mo>∑</mml:mo><mml:mi mathvariant="normal">AN</mml:mi><mml:mo>+</mml:mo><mml:mn mathvariant="normal">0.95</mml:mn><mml:mo>×</mml:mo><mml:mi mathvariant="normal">PAN</mml:mi><mml:mo>+</mml:mo><mml:mn mathvariant="normal">0.35</mml:mn><mml:mo>×</mml:mo><mml:msub><mml:mrow class="chem"><mml:mi mathvariant="normal">HNO</mml:mi></mml:mrow><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
          where <inline-formula><mml:math id="M101" display="inline"><mml:mo>∑</mml:mo></mml:math></inline-formula>AN is the sum of all alkyl nitrate concentrations.</p>
      <p id="d1e1385">Figure 5 shows the seasonal means of the correction factors determined with
concentrations of the interfering species<?pagebreak page4176?> predicted by the CHIMERE model
driven by the DECSO inventory. Consistent with the findings in Europe
(Huijnen et al., 2010) and the US (Lamsal et al., 2008), the correction
factor (difference with the ideal value of 1.0) is largest over polluted urban
regions, where NO<inline-formula><mml:math id="M102" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> is a larger fraction of total oxidized
nitrogen compounds. The correction factor tends to be closer to unity in
winter, when the NO<inline-formula><mml:math id="M103" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> photochemistry is slower and thus NO<inline-formula><mml:math id="M104" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> has a
larger relative contribution to total oxidized nitrogen compounds. The
correction factor derived from simulations with the MIX inventory (not
shown) shows a similar pattern to Fig. 5, but with a larger number of
values close to 1 related to the larger emissions. Hourly correction factors
for individual hours of each day during the year for all individual stations
have been applied to the in situ measurements. It is difficult to quantify
the accuracy of the correction factors and errors, as the collocated
measurements of other oxidized nitrogen compounds are not publicly available.
We used the standard deviation of the daily means of correction factors
within a season as a measure of its uncertainty. The average standard
deviations for all sites are 10 %, which is comparable to the uncertainty
level pointed out by the study of McLinden et al. (2014).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F5" specific-use="star"><caption><p id="d1e1417">Seasonally averaged correction factors for interference in
NO<inline-formula><mml:math id="M105" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> measurements using chemiluminescence analyzers as estimated from a
CHIMERE simulation driven by the DECSO emission inventory for the year 2015.</p></caption>
          <?xmltex \igopts{width=497.923228pt}?><graphic xlink:href="https://acp.copernicus.org/articles/18/4171/2018/acp-18-4171-2018-f05.png"/>

        </fig>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T2" specific-use="star"><caption><p id="d1e1439">Correlation coefficient, regression slope, root-mean-square error
(RMSE), and normalized mean error (NME) in 2015 of the simulated surface
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> concentrations driven by DECSO 2015, MIX Asian 2010, and the
corrected DECSO emission inventory versus the corrected in situ measurements.
The intercept is set to 0 when performing the regression. The unit of RMSE is
<inline-formula><mml:math id="M107" display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>g m<inline-formula><mml:math id="M108" 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>.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="13">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="right"/>
     <oasis:colspec colnum="3" colname="col3" align="right"/>
     <oasis:colspec colnum="4" colname="col4" align="right"/>
     <oasis:colspec colnum="5" colname="col5" align="right" colsep="1"/>
     <oasis:colspec colnum="6" colname="col6" align="right"/>
     <oasis:colspec colnum="7" colname="col7" align="right"/>
     <oasis:colspec colnum="8" colname="col8" align="right"/>
     <oasis:colspec colnum="9" colname="col9" align="right" colsep="1"/>
     <oasis:colspec colnum="10" colname="col10" align="right"/>
     <oasis:colspec colnum="11" colname="col11" align="right"/>
     <oasis:colspec colnum="12" colname="col12" align="right"/>
     <oasis:colspec colnum="13" colname="col13" align="right"/>
     <oasis:thead>
       <oasis:row>  
         <oasis:entry colname="col1">Category</oasis:entry>  
         <oasis:entry rowsep="1" namest="col2" nameend="col5" align="center" colsep="1">DECSO </oasis:entry>  
         <oasis:entry rowsep="1" namest="col6" nameend="col9" align="center" colsep="1">MIX </oasis:entry>  
         <oasis:entry rowsep="1" namest="col10" nameend="col13" align="center">Corrected DECSO </oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">  
         <oasis:entry colname="col1"/>  
         <oasis:entry colname="col2"><inline-formula><mml:math id="M109" display="inline"><mml:mi>r</mml:mi></mml:math></inline-formula></oasis:entry>  
         <oasis:entry colname="col3">Slope</oasis:entry>  
         <oasis:entry colname="col4">RMSE</oasis:entry>  
         <oasis:entry colname="col5">NME</oasis:entry>  
         <oasis:entry colname="col6"><inline-formula><mml:math id="M110" display="inline"><mml:mi>r</mml:mi></mml:math></inline-formula></oasis:entry>  
         <oasis:entry colname="col7">Slope</oasis:entry>  
         <oasis:entry colname="col8">RMSE</oasis:entry>  
         <oasis:entry colname="col9">NME</oasis:entry>  
         <oasis:entry colname="col10"><inline-formula><mml:math id="M111" display="inline"><mml:mi>r</mml:mi></mml:math></inline-formula></oasis:entry>  
         <oasis:entry colname="col11">Slope</oasis:entry>  
         <oasis:entry colname="col12">RMSE</oasis:entry>  
         <oasis:entry colname="col13">NME</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>  
         <oasis:entry colname="col1">Main sample</oasis:entry>  
         <oasis:entry colname="col2">0.73</oasis:entry>  
         <oasis:entry colname="col3">0.74</oasis:entry>  
         <oasis:entry colname="col4">11.6</oasis:entry>  
         <oasis:entry colname="col5">0.32</oasis:entry>  
         <oasis:entry colname="col6">0.85</oasis:entry>  
         <oasis:entry colname="col7">1.3</oasis:entry>  
         <oasis:entry colname="col8">14.8</oasis:entry>  
         <oasis:entry colname="col9">0.36</oasis:entry>  
         <oasis:entry colname="col10">0.72</oasis:entry>  
         <oasis:entry colname="col11">1.0</oasis:entry>  
         <oasis:entry colname="col12">10.5</oasis:entry>  
         <oasis:entry colname="col13">0.29</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">Main sample (daytime)</oasis:entry>  
         <oasis:entry colname="col2">0.76</oasis:entry>  
         <oasis:entry colname="col3">0.64</oasis:entry>  
         <oasis:entry colname="col4">12.1</oasis:entry>  
         <oasis:entry colname="col5">0.39</oasis:entry>  
         <oasis:entry colname="col6">0.84</oasis:entry>  
         <oasis:entry colname="col7">1.1</oasis:entry>  
         <oasis:entry colname="col8">11.3</oasis:entry>  
         <oasis:entry colname="col9">0.31</oasis:entry>  
         <oasis:entry colname="col10">0.76</oasis:entry>  
         <oasis:entry colname="col11">0.89</oasis:entry>  
         <oasis:entry colname="col12">8.8</oasis:entry>  
         <oasis:entry colname="col13">0.26</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">Unselected</oasis:entry>  
         <oasis:entry colname="col2">0.63</oasis:entry>  
         <oasis:entry colname="col3">1.0</oasis:entry>  
         <oasis:entry colname="col4">9.2</oasis:entry>  
         <oasis:entry colname="col5">0.25</oasis:entry>  
         <oasis:entry colname="col6">0.81</oasis:entry>  
         <oasis:entry colname="col7">1.5</oasis:entry>  
         <oasis:entry colname="col8">19.7</oasis:entry>  
         <oasis:entry colname="col9">0.56</oasis:entry>  
         <oasis:entry colname="col10">0.61</oasis:entry>  
         <oasis:entry colname="col11">1.3</oasis:entry>  
         <oasis:entry colname="col12">15.9</oasis:entry>  
         <oasis:entry colname="col13">0.42</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">Mountainous</oasis:entry>  
         <oasis:entry colname="col2">0.51</oasis:entry>  
         <oasis:entry colname="col3">0.35</oasis:entry>  
         <oasis:entry colname="col4">15.0</oasis:entry>  
         <oasis:entry colname="col5">0.65</oasis:entry>  
         <oasis:entry colname="col6">0.77</oasis:entry>  
         <oasis:entry colname="col7">0.77</oasis:entry>  
         <oasis:entry colname="col8">11.3</oasis:entry>  
         <oasis:entry colname="col9">0.44</oasis:entry>  
         <oasis:entry colname="col10">0.51</oasis:entry>  
         <oasis:entry colname="col11">0.50</oasis:entry>  
         <oasis:entry colname="col12">13.0</oasis:entry>  
         <oasis:entry colname="col13">0.53</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">Northern</oasis:entry>  
         <oasis:entry colname="col2">0.92</oasis:entry>  
         <oasis:entry colname="col3">0.20</oasis:entry>  
         <oasis:entry colname="col4">14.9</oasis:entry>  
         <oasis:entry colname="col5">0.85</oasis:entry>  
         <oasis:entry colname="col6">0.81</oasis:entry>  
         <oasis:entry colname="col7">0.62</oasis:entry>  
         <oasis:entry colname="col8">10.4</oasis:entry>  
         <oasis:entry colname="col9">0.44</oasis:entry>  
         <oasis:entry colname="col10">0.92</oasis:entry>  
         <oasis:entry colname="col11">0.27</oasis:entry>  
         <oasis:entry colname="col12">14.1</oasis:entry>  
         <oasis:entry colname="col13">0.79</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">&lt; Four stations</oasis:entry>  
         <oasis:entry colname="col2">0.77</oasis:entry>  
         <oasis:entry colname="col3">0.65</oasis:entry>  
         <oasis:entry colname="col4">11.3</oasis:entry>  
         <oasis:entry colname="col5">0.40</oasis:entry>  
         <oasis:entry colname="col6">0.83</oasis:entry>  
         <oasis:entry colname="col7">0.99</oasis:entry>  
         <oasis:entry colname="col8">9.2</oasis:entry>  
         <oasis:entry colname="col9">0.29</oasis:entry>  
         <oasis:entry colname="col10">0.76</oasis:entry>  
         <oasis:entry colname="col11">0.90</oasis:entry>  
         <oasis:entry colname="col12">9.3</oasis:entry>  
         <oasis:entry colname="col13">0.30</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">Densely located (“L”)</oasis:entry>  
         <oasis:entry colname="col2">0.55</oasis:entry>  
         <oasis:entry colname="col3">0.74</oasis:entry>  
         <oasis:entry colname="col4">13.7</oasis:entry>  
         <oasis:entry colname="col5">0.53</oasis:entry>  
         <oasis:entry colname="col6">0.87</oasis:entry>  
         <oasis:entry colname="col7">0.78</oasis:entry>  
         <oasis:entry colname="col8">7.4</oasis:entry>  
         <oasis:entry colname="col9">0.25</oasis:entry>  
         <oasis:entry colname="col10">0.57</oasis:entry>  
         <oasis:entry colname="col11">0.99</oasis:entry>  
         <oasis:entry colname="col12">15.0</oasis:entry>  
         <oasis:entry colname="col13">0.52</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table></table-wrap>

</sec>
</sec>
<?pagebreak page4177?><sec id="Ch1.S3">
  <title>Results and discussion</title>
<sec id="Ch1.S3.SS1">
  <title>Annual intercomparison</title>
      <p id="d1e1903">We compare the modeled surface NO<inline-formula><mml:math id="M112" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> with the corrected in situ
measurements throughout China. In general, the spatial distribution of
annual mean NO<inline-formula><mml:math id="M113" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentrations from the CHIMERE model simulations is
well in line with that from in situ measurements, with a correlation
coefficient of over 0.7. However, the modeled NO<inline-formula><mml:math id="M114" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> is biased compared
to ground measurements. The differences of annual mean NO<inline-formula><mml:math id="M115" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
concentrations between simulations and measurements are given in Fig. 6. The
CHIMERE simulations with the DECSO inventory show considerably lower
NO<inline-formula><mml:math id="M116" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentrations than the in situ measurements, with a negative
difference for nearly 90 % of all grid cells. Conversely, the CHIMERE
simulations with the MIX inventory are generally higher than the in situ
measurements for grid cells corresponding to large cities: A positive bias
is found for 70 % of the grid cells with over four monitoring sites.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F6" specific-use="star"><caption><p id="d1e1953">The normalized difference of annual mean surface NO<inline-formula><mml:math id="M117" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
concentrations between model simulations and the corrected in situ
measurements in 2015. The simulated NO<inline-formula><mml:math id="M118" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentrations driven by
<bold>(a)</bold> the DECSO inventory, 2015; <bold>(b)</bold> the MIX Asian inventory, 2010; and <bold>(c)</bold> the
corrected DECSO inventory are subtracted from the corrected in situ
measurements to derive the differences. The mean of the differences is
further subtracted from the differences to derive the normalized
differences. The magnitude of the size of symbols denotes the number of
stations located in the same model grid cell. The color of the symbols
denotes the difference of NO<inline-formula><mml:math id="M119" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentrations. Grid cells with densely
located stations are labeled with “L”. The outline of circles
corresponding to “main sample” (see Table 2) is highlighted in black.</p></caption>
          <?xmltex \igopts{width=483.69685pt}?><graphic xlink:href="https://acp.copernicus.org/articles/18/4171/2018/acp-18-4171-2018-f06.png"/>

        </fig>

      <p id="d1e1999">Grid cells are classified into five categories, i.e., mountainous, northern,
&lt; four stations, densely located, and main sample, and the
corresponding scatter plots of corrected measurements against simulations are
shown in Fig. 7. We define a grid cell as “mountainous” where the average
elevation is higher than 1000 m and the standard deviation of elevations is
over 15 % of the mean, based on the topographic data from the 30 arcsec
global land topography “GTOPO30” archived by the US Geological Survey
(available at <uri>https://lta.cr.usgs.gov/GTOPO30</uri>, last access: 10 July 2017, rescaled to 0.05<inline-formula><mml:math id="M120" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>). The grid cells higher than
45<inline-formula><mml:math id="M121" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N are classified as “northern”. The grid cells with less than
four measurement stations are classified as “&lt; four stations”. The
grid cells with only densely located stations (see definition later in this
section) are classified as “densely located”. Note that the priority of the
category of mountainous, northern, &lt; four stations, and densely
located is from high to low when we perform the classification in this study.
For instance, for grid cells that meet the criteria of both mountainous and
northern, we classify them as mountainous. The remaining<?pagebreak page4178?> grid cells are
classified as “main sample”. The results for the daytime period
(08:00–19:00 LT) are displayed separately.
The correlation coefficient, regression slope, and root-mean-square error for
the individual categories compared to measurements are given in Table 2.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F7" specific-use="star"><caption><p id="d1e2026">Scatter plots of the simulated annual mean surface NO<inline-formula><mml:math id="M122" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
concentrations in 2015 driven by <bold>(a)</bold> the DECSO inventory, 2015; <bold>(b)</bold> the MIX
Asian inventory, 2010; and <bold>(c)</bold> the corrected DECSO inventory and the
corrected in situ measurements. The orange dots correspond to the grid cells
with a latitude higher than 45<inline-formula><mml:math id="M123" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N. The pink dots correspond to the
grid cells labeled with “L” in Fig. 6. The corrected DECSO
inventory is derived by scaling the total amount of NO<inline-formula><mml:math id="M124" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions from
the DECSO inventory to that from the MIX inventory. The intercept is set to
0 when performing the regression.</p></caption>
          <?xmltex \igopts{width=483.69685pt}?><graphic xlink:href="https://acp.copernicus.org/articles/18/4171/2018/acp-18-4171-2018-f07.png"/>

        </fig>

      <p id="d1e2072">Significant regional differences are found. The small slope over mountainous
regions could be related to model limitations to resolve cities in the
valleys. Furthermore, we may expect difficulties for the model in describing
NO<inline-formula><mml:math id="M125" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentrations over complex terrain. For mountainous regions, the
lower slope may also be related to the large uncertainties in the
meteorological parameters associated with the difficulties in resolving the
characterization of small-scale orography in the ECMWF model (Beljaars et
al., 2004). The errors on meteorological parameters, such as mixing height
and temperature (Hongisto, 2005) and wind fields (Minguzzi et al., 2005), can
introduce biases for air quality simulations. In addition, the accuracy of
the DECSO algorithm highly relies on the appropriate wind fields because
DECSO performs trajectory analysis to account for NO<inline-formula><mml:math id="M126" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> transport away
from the source when calculating the sensitivity of concentrations to
emissions (Mijling and van der A, 2012). In this way, uncertainties in
meteorological parameters are amplified in the DECSO inventory, resulting in
a worse agreement for mountainous areas (<inline-formula><mml:math id="M127" display="inline"><mml:mi>r</mml:mi></mml:math></inline-formula> <inline-formula><mml:math id="M128" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 0.51) compared to the MIX
inventory (<inline-formula><mml:math id="M129" display="inline"><mml:mi>r</mml:mi></mml:math></inline-formula> <inline-formula><mml:math id="M130" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 0.77).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F8" specific-use="star"><caption><p id="d1e2124">Correlation among the number of stations in the same model grid
cell, ratio of the simulated annual mean surface 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> concentrations in
2015 driven by <bold>(a)</bold> the DECSO inventory, 2015, or <bold>(b)</bold> the MIX
Asian inventory, 2010, to the corrected in situ measurements, and the average
distance among stations located in the same grid cell. The magnitude of the
size of the circle denotes the average distance between stations located in
the same grid cell. The diamond denotes the average ratio of simulations to
measurements for grid cells with different numbers of stations.</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/18/4171/2018/acp-18-4171-2018-f08.png"/>

        </fig>

      <p id="d1e2148">The CHIMERE model accurately reproduces the spatial variability in NO<inline-formula><mml:math id="M132" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
for northern grid cells with a high correlation coefficient of 0.92 and 0.81
for the simulations with the DECSO and the MIX inventories, respectively, but
with a large negative bias. The bias could be related to model uncertainties
in NO<inline-formula><mml:math id="M133" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> sinks for high latitudes (Ding et al., 2017b), indicated by the
sensitivity studies of modeled NO<inline-formula><mml:math id="M134" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> columns to errors in chemical
parameters associated with NO<inline-formula><mml:math id="M135" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> sinks (Lin et al., 2012; Stavrakou et
al., 2013). Additionally, the bias is particularly significant for the
simulations with the DECSO inventory, showing a slope of merely 0.20. This
could be further explained by the general underestimation of NO<inline-formula><mml:math id="M136" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>
emissions caused by the bias in NO<inline-formula><mml:math id="M137" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> tropospheric columns of DOMINO v2
for this area (Ding et al., 2017b), partly due to a bias in the calculation
of air mass factor for retrievals at large solar zenith angles by the
radiance transfer model (Lorente et al., 2017) and possibly biases in the
estimated stratospheric background.</p>
      <p id="d1e2206">Figure 8 depicts the ratio of the simulated annual mean surface 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>
concentrations to the corrected in situ measurements sorted by the number of
stations located in the same grid cell from small to large. It is
interesting to note that the ratio is small for grid cells with less than
four
stations, but increases along with the increase in the number of stations
from four to nine, ranging from 0.6 to 1.0 and 0.9 to 1.8 for the simulations with
the DECSO and the MIX inventories, respectively. The trend in the ratio
suggests that the representativeness of in situ measurements for the average
NO<inline-formula><mml:math id="M139" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> levels of a grid cell improves with increasing numbers of stations
or city size. For grid cells with less than four stations, the model with
its limited spatial resolution cannot be expected to accurately resolve the
spatial gradient of pollutants towards the city center in relatively smaller
urban areas. Similarly, the in situ measurements for stations located close
together are expected to be less representative of the grid cell mean
compared to the homogeneously distributed stations. This is in agreement
with the tendency that grid cells with lower average measurement station
distances (&lt; 10 km) tend to show<?pagebreak page4179?> lower ratios (&lt; 0.5) in
Fig. 8, in particular for grid cells with a larger number of stations. We
select the grid cells with over four stations but lower average distances
than the 10 % percentiles in Fig. 3c and name them densely
located. We analyze the performance of the model in those grid cells with
only densely clustered stations (labeled with “L” in Fig. 6). Not
surprisingly, the simulations for those grid cells show larger discrepancies
compared to the measurements, and also the correlation coefficient of
simulations with the DECSO inventory drops down to a rather low value of
0.55 (Table 2).</p>
      <p id="d1e2228">We exclude grid cells in the special categories discussed above (i.e.,
mountainous, northern, &lt; four stations, and densely located
stations) to draw conclusions on the ability of the model to reproduce the
measurements. Statistical values (correlation, slope, root-mean-square error)
for the remaining grid cells (main sample) are given along with the plots in
Fig. 7. A slope of 0.74 and 1.3 is found for the simulation with the DECSO
and the MIX inventories, respectively. As mentioned before, the majority of
stations are located in urban, populated, and polluted areas and the model
resolution of 0.25<inline-formula><mml:math id="M140" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> will not be enough to represent the existing
NO<inline-formula><mml:math id="M141" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> gradients, thus we may expect a negative representativity offset in
the modeled surface concentration, even for the main sample obtained after
data screening (Irie et al., 2012; Lin et al., 2014). We select grid cells
with over four stations, which potentially place one or two stations<?pagebreak page4180?> in
background areas, to give a rough estimate of the offset. The background
stations are defined as stations located far away from urban areas on the
basis of a visual inspection of satellite imagery from Google Earth. Not
surprisingly, the measurement from the background station which is expected
to better represent the grid cell mean is smaller than the average value of
measurements from all stations located in the same grid cell. The ratios of
annual mean measurements from the background stations to the mean of
corresponding measurements from all stations range from 0.64 to 0.86, with an
average of 0.74. That is, the average negative representativity offset may
reach 25 %. The ratio is closer to 1 in winter (0.83 on average) due to
the reduced spatial gradients in 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> caused by a longer NO<inline-formula><mml:math id="M143" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>
lifetime, which will be discussed in detail in Sect. 3.2. Thus, the slopes of
0.74 and 1.3 for DECSO and MIX actually indicate a slightly negative and more
significantly positive bias, respectively.</p>
      <p id="d1e2267">A positive bias may indicate an overestimation of NO<inline-formula><mml:math id="M144" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions, or
errors in the spatial downscaling of the bottom-up emission totals, although
biases from the description of the chemistry, transport, and removal
processes in the model cannot be ruled out. The overestimation of the MIX
results over large cities are consistent with previous findings that
regional inventories like MIX have large positive biases in urban areas
(Zheng et al., 2017). The reason for the positive biases will be discussed
in detail later in this section. Uncertainties in the DECSO results may be
attributed to biases in the OMI tropospheric NO<inline-formula><mml:math id="M145" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> column densities, or
representation errors introduced by the projection of the CTM onto the
measured NO<inline-formula><mml:math id="M146" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> satellite footprint (Ding et al., 2017b). OMI NO<inline-formula><mml:math id="M147" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
observations have been reported to be systematically smaller than those from
ground-based measurements (e.g., MAX-DOAS) over polluted regions (Shaiganfar
et al., 2011; Ma et al., 2013; Ialongo et al., 2016) due to their different
spatial representativeness (Irie et al., 2012; Lin et al., 2014) and
uncertainties in NO<inline-formula><mml:math id="M148" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> vertical column retrieval, including the shielding
effect of aerosols (Shaiganfar et al., 2011) and the varying observation
geometry (Vasilkov et al., 2017). In addition, the fact that the adopted
model resolution is not sufficient to accurately model nonlinear effects in
the 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> loss rate may contribute to the negative bias (Valin et al.,
2011).</p>
      <p id="d1e2325">Regional bottom-up inventories tend to have large positive biases in urban
areas. Those inventories usually downscale local emissions from regional
totals (provincial totals are used in the MEIC/MIX inventory for China) and
distribute them to grid cells using spatial proxies (e.g., population
density and GDP). However, the spatial proxies may not match the locations
of the individual emitting sources, especially for industrial plants located
far away from urban centers that tend to have a larger population density
and GDP (Liu et al., 2017). Such a decoupling will result in an
overestimation of emissions over urban areas, which has been proven by the
comparison of proxy-based regional inventory with high-resolution urban
inventories developed from the extensive use of information of individual
emitting sources (Zheng et al., 2017).</p>
      <p id="d1e2328">In order to better compare the spatial distributions of the two inventories
and identify the sensitivity of model performance to spatial distributions of
emissions, we further evaluate the impact of the spatial distribution of
emissions on simulating NO<inline-formula><mml:math id="M150" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> by applying the same spatial proxy for
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 in both inventories. We scale the total amount of
emissions of the 2015 DECSO inventory over the domain adopted in this study
to that of the 2010 MIX inventory but kept the DECSO spatial distribution
(hereinafter referred to as the corrected DECSO inventory; see Fig. 2). We then compare
the modeled 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> using the corrected DECSO inventory with in situ
measurements in Fig. 6c. It is interesting to see that many high values in
the MIX simulation are not reproduced by the simulation with the corrected
DECSO inventory. We further assess the simulation results with the corrected
DECSO inventory in Fig. 7c. The simulation with the MIX inventory tends to
cluster the pollutants more over urban areas than that with the corrected
DECSO inventory, indicating that the modeled NO<inline-formula><mml:math id="M153" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> is sensitive to the
spatial distribution of emissions. The large bias in the MIX inventory is
reduced significantly, with a slope decreasing from 1.3 to 1.0, which suggests
an improvement of the distribution of emissions between urban and
suburban or rural areas.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F9"><caption><p id="d1e2369">Monthly mean ratio of simulated surface NO<inline-formula><mml:math id="M154" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentrations
driven by the DECSO inventory, 2015 (red bar), and the MIX Asian inventory,
2010 (blue bar), with the corrected in situ measurements (left axis). The
correlation coefficient of the simulated NO<inline-formula><mml:math id="M155" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentrations versus the
corrected in situ measurements is displayed on the right axis.</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://acp.copernicus.org/articles/18/4171/2018/acp-18-4171-2018-f09.png"/>

        </fig>

      <p id="d1e2397">Note that due to the lack of the 2015 inventory, the use of the 2010 MIX
emissions for other species including SO<inline-formula><mml:math id="M156" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, CO, and non-methane volatile organic compounds (NMVOCs) in both the MIX
and the DECSO simulations may introduce uncertainties in simulating
NO<inline-formula><mml:math id="M157" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>. The anthropogenic emissions of SO<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>, CO, and NMVOCs for China
have been reported to decrease by 2, 5, and increase by 21 % from 2010 to
2015, respectively (Li et al., 2017b). In gas-phase chemistry, the principal
sink of NO<inline-formula><mml:math id="M159" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> is oxidation to HNO<inline-formula><mml:math id="M160" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>. The influence of the growth in
NMVOCs on the oxidizing power of the atmosphere is partially compensated<?pagebreak page4181?> for by
the reduction in CO, as CO and hydrocarbons play similar roles in depleting
oxidants following the HO<inline-formula><mml:math id="M161" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>–NO<inline-formula><mml:math id="M162" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>–CO–hydrocarbon chemical mechanisms
(Jacob, 2000). Additionally, SO<inline-formula><mml:math id="M163" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> influences NO<inline-formula><mml:math id="M164" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
concentrations by forming aerosols, concentrations of which have an impact on
photolysis rates and thus photochemical reaction rates associated with
NO<inline-formula><mml:math id="M165" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> (Mailler et al., 2017). However, the emission changes are rather
small compared to the uncertainties in bottom-up estimates, which are even
smaller than the discrepancies among estimates from different bottom-up
inventories. Thus we believe the uncertainties arising from the use of the 2010
inventory are not significant. A sensitive analysis will be further expected
to quantify the influence of emissions of other species on simulated
NO<inline-formula><mml:math id="M166" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F10" specific-use="star"><caption><p id="d1e2502">Diurnal variability in hourly average NO<inline-formula><mml:math id="M167" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentrations.
Values shown are annual averages for the year 2015. On the left axis the solid line
represents the corrected in situ measurement. The dotted line represents the
simulation driven by the DECSO inventory, 2015 (blue), and the MIX Asian
inventory, 2010 (red). On the right axis the grey line represents the 24 h
profiles applied over the daily emissions to obtain hourly data in the
CHIMERE model.</p></caption>
          <?xmltex \igopts{width=312.980315pt}?><graphic xlink:href="https://acp.copernicus.org/articles/18/4171/2018/acp-18-4171-2018-f10.png"/>

        </fig>

</sec>
<sec id="Ch1.S3.SS2">
  <title>Seasonality</title>
      <p id="d1e2526">Figure 9 compares the monthly mean NO<inline-formula><mml:math id="M168" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentrations simulated by the
CHIMERE model using the two inventories with the in situ measurements. The
spatial correlation between the modeled NO<inline-formula><mml:math id="M169" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentrations and the
in situ measurements shows a weak dependence on season, which is slightly
worse in summer (July). The correlation coefficients range from 0.64 (July)
to 0.73 (January) and from 0.80 (July) to 0.83 (January) for the
simulations with the DECSO and the MIX inventories, respectively. A possible
explanation for the somewhat higher correlation in January is the smaller
model error in winter than in summer, as indicated by previous findings in
both China (Lin et al., 2012) and Europe (Huijnen et al., 2010). This may be
related to the difficulties in resolving the more active NO<inline-formula><mml:math id="M170" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>
photochemistry in summer by the model. For instance, the model with a
horizontal resolution of 0.25<inline-formula><mml:math id="M171" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> is not able to fully resolve the
spatial gradients of NO<inline-formula><mml:math id="M172" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> close to strong emission sources, but such an
impact is smaller in winter than in other seasons, as the NO<inline-formula><mml:math id="M173" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> gradients
in a grid cell are smeared out due to the longer NO<inline-formula><mml:math id="M174" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> lifetime in
winter.</p>
      <p id="d1e2593">The seasonal difference is pronounced when comparing the magnitude of the
NO<inline-formula><mml:math id="M175" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentrations in Fig. 9. In general, a smaller ratio between
modeled NO<inline-formula><mml:math id="M176" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentrations and in situ measurements is detected in
winter. The ratio reaches the lowest values in January, which is consistent
with the general underestimation of simulations in winter as indicated by Lin
et al. (2012). For simulations with the DECSO inventory, the ratio deviating
more significantly from unity in winter might be due to systematic biases in
the OMI NO<inline-formula><mml:math id="M177" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> observations during winter as well. Biases in OMI
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> column densities over polluted regions are introduced by the high
aerosol loading, most of which are scattering aerosols in China, as aerosols
are not explicitly considered in the cloud retrieval or the air mass factor calculation
in the operational NO<inline-formula><mml:math id="M179" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> product (Castellanos et al., 2015; Chimot et al.,
2016; Wang et al., 2017). The aerosols' effect may be more significant in
winter due to the higher aerosol concentrations and larger solar zenith
angle (Ma et al., 2013). Additionally, the DECSO algorithm is more vulnerable
to biased observations as a result of the smaller number of useful
observations in wintertime because of the filtering of snow-covered regions.
Conversely, the simulations with the MIX inventory show ratios ranging
from 1.09 to 1.22 in the second half of the year. This may signal an
overestimation of total emissions, as pointed out in Sect. 3.1. In addition,
the assumptions used in the MIX inventory for the distribution of monthly
emissions over the year may also contribute to the bias. For example, higher
power and industrial emissions are assumed in the second half of the year due
to larger industrial productions and thus power generations to meet the
annual total production target (Li et al., 2017a).</p>
</sec>
<sec id="Ch1.S3.SS3">
  <title>Diurnal cycle</title>
      <p id="d1e2647">Figure 10 presents the diurnal variability in hourly-averaged surface
NO<inline-formula><mml:math id="M180" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentrations. The simulations with both inventories and the in
situ measurements exhibit a broadly similar daily variation (<inline-formula><mml:math id="M181" display="inline"><mml:mi>r</mml:mi></mml:math></inline-formula> <inline-formula><mml:math id="M182" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 0.81).
The distinct peak in 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 in the morning hours (around
08:00 LT) and in the afternoon (around 20:00 LT) detected by the
measurements has been well captured by the model, which can be attributed to
increasing (traffic) emissions in the rush hours indicated by the Selected
Nomenclature for sources of Air Pollution Prototype (SNAP) diurnal profiles
of emissions (Menut et al., 2012) adopted in the CHIMERE model (grey line).
Both simulations and measurements show a drop in NO<inline-formula><mml:math id="M184" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentrations
during daytime with the same timing and amplitude, related to the varying
chemical loss rate of NO<inline-formula><mml:math id="M185" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> driven by NO<inline-formula><mml:math id="M186" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> photochemistry. However,
the disagreement between simulated and measured values is larger at night,
which may point to problems regarding the treatment of boundary layer mixing.
NO<inline-formula><mml:math id="M187" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentrations simulated by the model cannot reproduce the observed
temporal pattern at night but present constantly high values, probably
caused by unrealistically low boundary layer heights and too little vertical
turbulence in the model (Bessagnet et al., 2016). This has been further
confirmed by the earlier evaluation of the diurnal cycle of trace gases as
modeled by CHIMERE in Lampe et al. (2009).</p>
      <p id="d1e2719">We separately evaluated the model performance for the daytime period
(08:00–19:00), when the pattern of diurnal variations simulated by the
CHIMERE model is closer to what is observed by the in situ measurements. Not
surprisingly, a larger negative slope of 0.64 is obtained for the simulation
with the DECSO inventory compared to the surface observations, while the
slope for the simulation with the MIX inventory has been reduced
significantly to a value of 1.1 (Table 2) due to the tendency of
overestimating NO<inline-formula><mml:math id="M188" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentrations during night in the model. Note that
the slope close to unity for the simulation with the MIX inventory during
daytime does not necessarily imply a perfect emission inventory, but still
indicates a potential overestimation because we expect a slope smaller than 1
(in the range of 0.64–0.86; see Sect. 3.1) when comparing model simulations
with in situ<?pagebreak page4182?> measurements which are mainly situated in populated
high-concentration areas.</p>
</sec>
</sec>
<sec id="Ch1.S4" sec-type="conclusions">
  <title>Conclusions</title>
      <p id="d1e2738">In this work we evaluated the surface NO<inline-formula><mml:math id="M189" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentrations from the
CHIMERE CTM, driven by both satellite-derived and bottom-up emission
inventories, using the measurements from the ground-based air quality
monitoring network of MEP. To our knowledge, this result is the first
validation of modeling NO<inline-formula><mml:math id="M190" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> results with this widespread in situ
network, which became recently available. Our study demonstrates the
capabilities of CTMs such as CHIMERE, combined with satellite observations,
to simulate NO<inline-formula><mml:math id="M191" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentrations at the surface over China. MEP in situ
measurements can serve as a useful dataset for evaluating model simulations,
but a careful selection of measurements and scaling correction is necessary
to represent the averaged 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> level over the area of a grid cell.
Measurements with unexpected lower annual mean NO<inline-formula><mml:math id="M193" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentrations at
urban stations compared to those at suburban stations have been discarded
from the final analysis.</p>
      <p id="d1e2786">The model accurately reproduces the spatial variability in annual mean
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> from in situ measurements over China, with a spatial correlation
coefficient of over 0.7. In situ measurements used in this study are
expected to have a positive bias when compared to model simulations due to
a combination of preferential placement of monitors in polluted locations
and the limitation of model resolution to resolve large NO<inline-formula><mml:math id="M195" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> gradients
over urban areas. The estimated bias is 25 % (ranging between 10 % and
40 %), indicated by the ratios of annual mean measurements from the
background stations, which is expected to better represent the grid cell mean
to the mean of corresponding measurements from all stations for selected
grid cells with over four stations. The bias is especially pronounced for grid
cells with too few stations (less than four in this study) or stations located
close together. Negative biases have been widely detected for mountainous
and northern regions, which are most likely related to the representative
issue discussed above, but model uncertainties in meteorological parameters
and NO<inline-formula><mml:math id="M196" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> sinks will also play a role. For other regions, a negative and
positive difference has been found for the simulation with the DECSO
(slope <inline-formula><mml:math id="M197" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 0.74) and the MIX (slope <inline-formula><mml:math id="M198" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 1.3) inventories, respectively, suggesting an
underestimation and overestimation of 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 corresponding
inventories. The bias between observed and modeled concentrations was
reduced significantly, with the slope decreasing from 1.3 to 1.0, when the
spatial distribution of 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 in the DECSO inventory is applied
as the spatial proxy for the MIX inventory. The reduced bias suggests an
improvement of the distribution of emissions between urban and
suburban or rural areas in the DECSO inventory compared to that used in the
bottom-up inventory, which shed light on addressing the spatial errors in
bottom-up inventories. Conversely, we also show that the correlation
coefficient of the simulated 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> concentrations versus the in situ
measurements is slightly higher in the MIX-based simulations compared to
the DECSO simulations. However, this does not necessarily contradict the
findings that the spatial distribution of NO<inline-formula><mml:math id="M202" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions is more
reasonable in DECSO, considering the difference in<?pagebreak page4183?> correlation coefficient
is minor but the bias in the MIX-based simulations is significant.
Nevertheless, the good performance of the satellite-derived emission
inventory, in particular the spatial distribution of emissions, has been
confirmed by the widespread in situ measurements over China for the first
time in this study. The magnitude of satellite-derived emissions shows a
slightly negative bias by taking the negative representativity offset of
in situ measurements into account, which is attributed to biases in the OMI
tropospheric NO<inline-formula><mml:math id="M203" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> column densities, or representation errors introduced
by the projection of the CTM onto the measured NO<inline-formula><mml:math id="M204" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> satellite
footprint. In addition, satellite-derived NO<inline-formula><mml:math id="M205" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions succeed in
detecting the emission trend for the period of 2010–2015, which is consistent
with that in bottom-up emissions (Liu et al., 2016a; van der A et al.,
2017).</p>
      <p id="d1e2895">The performance of the model is comparable over seasons, with a slightly
better spatial correlation in winter. This is in line with previous findings
of a lower model uncertainty in winter due to the difficulties in resolving
the more active NO<inline-formula><mml:math id="M206" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> photochemistry and larger concentration gradients in
summer by the model. In addition, the daytime diurnal cycle has been well
captured by the model. However, the disagreement between simulations and
measurements is in general larger during nighttime, which is most likely
related to the uncertainty in vertical mixing in the model. This nighttime
issue causes an estimated bias of about <inline-formula><mml:math id="M207" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>15 % in the daily mean
NO<inline-formula><mml:math id="M208" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentrations.</p>
      <p id="d1e2923">Note that the validation performed in this study is focused on urban areas,
which may bring a systematic bias to the conclusive statements, as discussed
above. In the future analysis focusing on rural areas is expected to give a
more complete picture of the performance of CTMs with inventories. In
addition, an in-depth comparison of multiple models with variable chemistry
schemes (e.g., Huijnen et al., 2010) is further required to quantify the
influence of chemical mechanisms on simulated 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>. In order to support
model validation, the introduction of additional background stations, as
well as the provision of detailed information about the stations, including
classification and height, would be very valuable.</p>
</sec>

      
      </body>
    <back><notes notes-type="dataavailability">

      <p id="d1e2940">Measurements from the ground-based air quality monitoring
network of MEP were obtained from <uri>www.pm25.in</uri>(last access: 1 March 2017). The CHIMERE
model outputs are available upon request from the corresponding author.</p>
  </notes><notes notes-type="competinginterests">

      <p id="d1e2949">The authors declare that they have no conflict of
interest.</p>
  </notes><ack><title>Acknowledgements</title><p id="d1e2955">This research was funded by the MarcoPolo project of the European Union
Seventh Framework Programme (FP7/2007-2013) under grant agreement number
606953. We acknowledge Tsinghua University for providing the MIX emission
inventory. We acknowledge IPSL/LMD, INERIS, and IPSL/LISA in France for
providing the CHIMERE model. We thank the three anonymous reviewers for helpful comments during the discussion phase of the paper.
<?xmltex \hack{\newline}?><?xmltex \hack{\newline}?>
Edited by: Jason West<?xmltex \hack{\newline}?>
Reviewed by: three anonymous referees</p></ack><ref-list>
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    <!--<article-title-html>Evaluation of modeling NO<sub>2</sub> concentrations driven by satellite-derived and bottom-up emission inventories using in situ measurements over China</article-title-html>
<abstract-html><p>Chemical transport models together with emission inventories are widely used
to simulate NO<sub>2</sub> concentrations over China, but validation of the
simulations with in situ measurements has been extremely limited. Here we use
ground measurements obtained from the air quality monitoring network recently
developed by the Ministry of Environmental Protection of China to validate
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chemical transport model driven by the satellite-derived DECSO and the
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The model accurately reproduces the spatial variability in NO<sub>2</sub> from
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between simulations and measurements during nighttime, which likely produces
a positive model bias of about 15 % in the daily mean concentrations.
This is most likely related to the uncertainty in vertical mixing in the
model at night.</p></abstract-html>
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