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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-20-1627-2020</article-id><title-group><article-title>On the limit to the accuracy of regional-scale air quality models</article-title><alt-title>On the limit to the accuracy of regional-scale air quality models</alt-title>
      </title-group><?xmltex \runningtitle{On the limit to the accuracy of regional-scale air quality models}?><?xmltex \runningauthor{S.~T.~Rao et al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes" rid="aff1 aff2">
          <name><surname>Rao</surname><given-names>S. Trivikrama</given-names></name>
          <email>strao@ncsu.edu</email>
        <ext-link>https://orcid.org/0000-0002-3460-7762</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Luo</surname><given-names>Huiying</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-4171-7951</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Astitha</surname><given-names>Marina</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-3892-6672</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3">
          <name><surname>Hogrefe</surname><given-names>Christian</given-names></name>
          
        <ext-link>https://orcid.org/0000-0003-3280-3513</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3">
          <name><surname>Garcia</surname><given-names>Valerie</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3">
          <name><surname>Mathur</surname><given-names>Rohit</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-8927-5876</ext-link></contrib>
        <aff id="aff1"><label>1</label><institution>Department of Marine, Earth, and Atmospheric Sciences, North Carolina
State University, Raleigh, NC, USA</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>Department of Civil and Environmental Engineering, University of
Connecticut, Storrs, CT, USA</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>Center for Environmental Measurement and Modeling, U.S. Environmental
Protection Agency, <?xmltex \hack{\break}?>Research Triangle Park, NC, USA</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">S. Trivikrama Rao (strao@ncsu.edu)</corresp></author-notes><pub-date><day>10</day><month>February</month><year>2020</year></pub-date>
      
      <volume>20</volume>
      <issue>3</issue>
      <fpage>1627</fpage><lpage>1639</lpage>
      <history>
        <date date-type="received"><day>12</day><month>July</month><year>2019</year></date>
           <date date-type="rev-request"><day>30</day><month>August</month><year>2019</year></date>
           <date date-type="rev-recd"><day>27</day><month>December</month><year>2019</year></date>
           <date date-type="accepted"><day>10</day><month>January</month><year>2020</year></date>
      </history>
      <permissions>
        <copyright-statement>Copyright: © 2020 S. Trivikrama Rao et al.</copyright-statement>
        <copyright-year>2020</copyright-year>
      <license license-type="open-access"><license-p>This work is licensed under the Creative Commons Attribution 4.0 International License. To view a copy of this licence, visit <ext-link ext-link-type="uri" xlink:href="https://creativecommons.org/licenses/by/4.0/">https://creativecommons.org/licenses/by/4.0/</ext-link></license-p></license></permissions><self-uri xlink:href="https://acp.copernicus.org/articles/20/1627/2020/acp-20-1627-2020.html">This article is available from https://acp.copernicus.org/articles/20/1627/2020/acp-20-1627-2020.html</self-uri><self-uri xlink:href="https://acp.copernicus.org/articles/20/1627/2020/acp-20-1627-2020.pdf">The full text article is available as a PDF file from https://acp.copernicus.org/articles/20/1627/2020/acp-20-1627-2020.pdf</self-uri>
      <abstract><title>Abstract</title>
    <p id="d1e141">Regional-scale air pollution models are routinely being
used worldwide for research, forecasting air quality, and regulatory
purposes. It is well recognized that there are both reducible (systematic)
and irreducible (unsystematic) errors in the meteorology–atmospheric-chemistry modeling systems. The inherent (random) uncertainty stems from our
inability to properly characterize stochastic variations in atmospheric
dynamics and chemistry and from the incommensurability associated with
comparisons of the volume-averaged model estimates with point measurements.
Because stochastic variations are not being explicitly simulated in
the current generation of regional-scale meteorology–air quality models, one
should expect to find differences between the model estimates and
corresponding observations. This paper presents an observation-based
methodology to determine the expected errors from current-generation
regional air quality models even when the model design, physics, chemistry,
and numerical analysis, as well as its input data, were “perfect”. To this
end, the short-term synoptic-scale fluctuations embedded in the daily
maximum 8 <inline-formula><mml:math id="M1" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">h</mml:mi></mml:mrow></mml:math></inline-formula> ozone time series are separated from the longer-term forcing
using a simple recursive moving average filter. The inherent uncertainty
attributable to the stochastic nature of the atmosphere is determined based
on <inline-formula><mml:math id="M2" display="inline"><mml:mrow><mml:mn mathvariant="normal">30</mml:mn><mml:mo>+</mml:mo></mml:mrow></mml:math></inline-formula> years of historical ozone time series data measured at various
monitoring sites in the contiguous United States (CONUS). The results reveal that
the expected root mean square error (RMSE) at the median and 95th percentile
is about 2 and 5 <inline-formula><mml:math id="M3" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">ppb</mml:mi></mml:mrow></mml:math></inline-formula>, respectively, even for perfect air quality
models driven with perfect input data. Quantitative estimation of the
limit to the model's accuracy will help in objectively assessing the current
state of the science in regional air pollution models, measuring progress in
their evolution, and providing meaningful and firm targets for improvements
in their accuracy relative to ambient measurements.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <label>1</label><title>Introduction</title>
      <p id="d1e179">Confidence in model estimates of pollutant distributions is established
through direct comparisons of modeled concentrations with corresponding
observations made at discrete locations for retrospective cases. Pinder et
al. (2008) discussed the reducible (i.e., structural and parametric)
uncertainties that are attributable to the errors in model input data (e.g.,
meteorology, emissions, and initial and boundary conditions) as well as our
incomplete or inadequate understanding of the relevant atmospheric processes
(e.g., chemical transformation, planetary boundary layer evolution, transport
and dispersion, deposition, rain, and clouds).
Inherent or irreducible (random or unsystematic) uncertainties stem from our
inability to properly characterize the stochastic nature of the atmosphere
(Wilmott, 1981;  Wilmott et al., 1985; Fox, 1984; Rao et al., 1985, 2011a, b; Dennis et al., 2010) and from the incommensurability associated with comparing the
volume-averaged model estimates with point measurements (e.g., McNair et
al., 1996; Swall and Foley, 2009). Also, without completely knowing the
three-dimensional initial physical and chemical state of the atmosphere, its
future state cannot be simulated accurately (Lamb, 1984; Lamb and Hati,
1987; Lewellen and Sykes, 1989; Pielke, 1998; Gilliam et al., 2015). Given
the presence of the irreducible uncertainties, precise replication of
observed concentrations or their changes by the models cannot be expected
(Dennis et al.,<?pagebreak page1628?> 2010; Rao et al., 2011a; Porter et al., 2015; Astitha et al.,
2017).</p>
      <p id="d1e182">Whereas an air quality model's prediction represents some
time-/space-averaged concentrations, an observation at any given time at a
monitoring location reflects an individual event or specific realization out
of a population that will almost always differ from the model estimate even
if the model and its input data were perfect (Rao et al., 1985).
Consequently, comparisons of modeled and observed concentrations paired in
space and time indicate biases and errors in simulating absolute levels of
pollutant concentrations at individual monitoring sites (Porter et al.,
2015). The scientific discussion on modeling uncertainty goes back more than
3 decades with the current practice including data assimilation,
ensemble modeling, and model performance evaluation (e.g., Fox, 1981, 1984;
Lamb, 1984; Demerjian, 1985; Oreskes et al., 1994; Pielke, 1998; Lewellen
and Sykes, 1989; Lee et al., 1997; Carmichael et al., 2008; Hogrefe et al.,
2001a, b; Biswas and Rao, 2001; Grell and Baklanov, 2011; Gilliam et
al., 2006; Herwehe et al., 2011; Baklanov et al., 2014; Bocquet et al.,
2015; Solazzo and Galmarini, 2015a; Ying and Zhang, 2018; McNider and
Pour-Biazar, 2020; Stockwell et al., 2020). While ever-improving process
knowledge and increasing computational power will continue to help reduce
the structural and parametric uncertainties in air quality models, the
inherent uncertainty associated with our inability to properly characterize
the stochastic nature of the atmosphere will always result in some mismatch
between the model results and measurements; this could lead to speculation
on the inferred accuracy of the future states simulated by the
regional-scale air quality models (Dennis et al., 2010; Rao et al., 2011a;
Porter et al., 2015; Astitha et al., 2017; Luo et al., 2019).</p>
      <p id="d1e185">The sensitivity of model results to meteorology, chemical mechanisms, and
emissions has been examined in numerous studies (e.g., Vautard et al., 2012;
Sarwar et al., 2013; Pierce et al., 2010; Napelenok et al., 2011; Kang et
al., 2013). Herwehe et al. (2011) attributed the differences in ground-level
ozone predictions between the Weather Research and Forecasting (WRF) model coupled with Chemistry (WRF-Chem) and the modeling system consisting of WRF and the Community Multiscale Air Quality (CMAQ) model (WRF-QMAC) to the way
meteorology and chemistry interactions are handled within these two modeling
systems. Thomas et al. (2019) examined the ozone predictions in the
mid-Atlantic region of the United States during June 2016 through a series
of simulations with WRF-Chem, focusing on the sensitivity to the
meteorological initial/boundary conditions (IC/BCs), emissions inventory
(EI), and planetary boundary layer (PBL) scheme. Ying and Zhang (2018)
discussed the use of satellite-based observations for improving the
predictability of multiscale tropical weather and equatorial waves. Ensemble
modeling is being advocated for quantifying the uncertainty in model
predictions; however, the spread in the model estimates for the variable of
interest reflects the impact of our incomplete or inadequate knowledge of
the physical and chemical processes (i.e., the reducible errors stemming
from structural and parametric uncertainty) occurring in the atmosphere
(Solazzo and Galmarini, 2015b; Thomas et al., 2019; Stockwell et al., 2020).
McNider and Pour-Biazar (2020) reviewed the many issues in predicting the
prevailing meteorology for regional air quality simulations and indicated
that errors in the specification of the physical atmosphere such as
temperature, winds, and mixing heights can affect the air quality
predictions. Stockwell et al. (2020) discussed the problems relating to the
atmospheric chemical mechanisms currently being used for simulating air
quality. The current generation of regional models consider only the mean
values of a meteorological variable for a given timescale and the average
rate constant derived from gas chamber experiments for chemical reactions
and does not include their fluctuations in solving the equations of motion
for each time step. Further, the current operational regional-scale
meteorological and air quality models do not explicitly simulate the
stochastic nature of the atmosphere and, as such, typically miss the extreme
values at both the low and high ends of the concentration distribution
function.</p>
      <p id="d1e188">In most applications of regional-scale air quality models, statistical
metrics such as bias, the root mean square error (RMSE), correlation, and the index
of agreement are used to judge the quality of model predictions and
determine if the model is suitable for forecasting or regulatory purposes
(e.g., Fox, 1981, 1984; Solazzo et al., 2012; Appel et al., 2012; Simon et
al., 2012; Foley et al., 2014; Ryan, 2016; Emery et al., 2016; Zhang et al.,
2016; U.S. Environmental Protection Agency, 2018). While significant improvements in the formulation,
physical and chemical parameterizations, and numerical techniques have been
implemented in atmospheric models over the past 3 decades, it is not
clear if the improvement claimed in the model's performance relative to the
routine network measurements is statistically significant based on these
metrics (Hogrefe et al., 2008). Also, no assessments have been made to date
on the errors that are to be expected even from “perfect” regional-scale
air quality modeling systems. To estimate such irreducible model errors due
to atmospheric stochasticity (which we consider to be the errors that are
expected even from a perfect model – devoid of structural and parametric
uncertainties – with perfect – error-free – inputs), we analyzed the
observed daily maximum 8 <inline-formula><mml:math id="M4" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">h</mml:mi></mml:mrow></mml:math></inline-formula> (DM8HR) ozone time series data at monitoring
locations across the contiguous United States (CONUS) during the 1981–2014
time period and present the results of this analysis in Sect. 3.1. In
Sect. 3.2, we illustrate how this information could be used in guiding
model development specifically aimed at addressing reducible errors in the
synoptic (SY) component by contrasting the results from Sect. 3.1 with analysis
using the synoptic component from a 21-year simulation performed with the
fully coupled WRF-CMAQ simulations covering the 1990–2010 period. Since we
relied on multi-decadal historical ozone observations to assess the<?pagebreak page1629?> impact
of the stochastic nature of the atmosphere, the results presented here are
applicable to both forecasting and retrospective applications of current
regional-scale air quality models.</p>
</sec>
<sec id="Ch1.S2">
  <label>2</label><title>Data and methods</title>
      <p id="d1e207">Ground-level DM8HR ozone data covering CONUS during May to September in
each year were obtained from the U.S. Environmental Protection Agency's
(EPA) Air Quality System (AQS) (see <uri>https://www.epa.gov/aqs</uri>, last access: 3 February 2020). A
valid ozone season consists of at least 80 % data coverage during May to
September at each station. A total 185 monitoring stations with at least 30
valid years (to provide enough variety of synoptic conditions, denoted
hereafter as <inline-formula><mml:math id="M5" display="inline"><mml:mrow><mml:mn mathvariant="normal">30</mml:mn><mml:mo>+</mml:mo></mml:mrow></mml:math></inline-formula> in this paper) from the year 1981 to 2014 are analyzed.
Also, fully coupled WRF-CMAQ model simulations over CONUS for the
1990–2010 period were utilized in this study to demonstrate a new
perspective on model performance evaluation. To ensure better
characterization of the prevailing meteorology (i.e., synoptic forcing) in
the retrospective 21-year WRF-CMAQ simulations, four-dimensional data
assimilation (FDDA) was utilized following the methodology suggested by
Gilliam et al. (2012) and modified for fully coupled meteorology–chemistry
model applications as described in Hogrefe et al. (2015). The model setup
and performance evaluation of these historical multiyear WRF-CMAQ
simulations have been published by Xing et al. (2015), Gan et al. (2015),
and Astitha et al. (2017). Time-varying chemical lateral boundary conditions
are nested from the 108 <inline-formula><mml:math id="M6" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">km</mml:mi></mml:mrow></mml:math></inline-formula> hemispheric WRF-CMAQ simulation from 1990 to 2010
(Xing
et al., 2015).</p>
      <p id="d1e231">It has been shown that time series of the daily maximum 8 <inline-formula><mml:math id="M7" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">h</mml:mi></mml:mrow></mml:math></inline-formula> ozone
concentrations contain fluctuations operating on different timescales
(e.g., intra-day forcing induced by the fast-changing emissions and
atmospheric boundary layer evolution; diurnal forcing induced by the day and
night differences; and synoptic forcing induced by the passage of weather
systems across the country, sub-seasonal forcing due to the Madden–Julian
Oscillation – MJO, and long-term forcing induced by emissions,
El Niño–Southern Oscillation – ENSO, climate change, and other slow-varying
processes such as seasonal and sub-seasonal variations in the atmospheric
deposition and stratosphere–troposphere exchange processes) as noted by Rao
et al. (1997), Vukovich (1997), Hogrefe et al. (2000), Porter et al. (2015), Astitha et al. (2017), Xing et al. (2016), and Mathur et al. (2017). Variations in the 8 <inline-formula><mml:math id="M8" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">h</mml:mi></mml:mrow></mml:math></inline-formula> ozone can be thought of comprising of the
baseline (BL) of pollution that is created by various emitting sources and
modulated by the prevailing synoptic weather conditions (Rao et al., 1996, 2011b). Thus, the magnitude of the baseline concentration and the
strength of the synoptic component should be viewed as the necessary
and sufficient conditions for how high ozone levels can reach on a given day
(Astitha et al., 2017). Scale separation can be achieved by applying
filtering methods such as the empirical mode decomposition (EMD; Huang et al.,
1998), elliptic filter (Poularika, 1998), Kolmogorov–Zurbenko (KZ) filter
(Rao and Zurbenko, 1994), adaptive filter technique (Zurbenko et al.,
1996), and wavelet (Lau and Weng, 1995). Because improved complete ensemble
empirical mode decomposition with adaptive noise (Improved CEEMDAN; Colominas et al., 2014; a
version of the empirical mode decomposition method) and KZ filter yielded
similar results for the DM8HR time series data as shown in Figs. 1–2
discussed in the next section, only the results from the KZ filter are
presented in the subsequent analysis for quantifying the impact of the
stochastic nature of the atmosphere on observed and simulated ozone
concentrations. Furthermore, the KZ filtering is a simple method and works
well even in the presence of missing data (Hogrefe et al., 2003). In this
study, we used the KZ<inline-formula><mml:math id="M9" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">5</mml:mn><mml:mo>,</mml:mo><mml:mn mathvariant="normal">5</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula> with a window size of 5 <inline-formula><mml:math id="M10" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">d</mml:mi></mml:mrow></mml:math></inline-formula> and five iterations
on raw ozone time series [<inline-formula><mml:math id="M11" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> (<inline-formula><mml:math id="M12" display="inline"><mml:mi>t</mml:mi></mml:math></inline-formula>)] in the same manner as in Luo et al. (2019), Porter et al. (2015), and Rao et al. (2011b). The size of the window
and the number of iterations determine the desired scale separation. The
KZ<inline-formula><mml:math id="M13" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">5</mml:mn><mml:mo>,</mml:mo><mml:mn mathvariant="normal">5</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula> filtering process helps separate the synoptic-scale
weather-induced variations embedded in the May–September DM8HR time series
data (short-term component) from the long-term baseline
component.

              <disp-formula specific-use="gather" content-type="numbered"><mml:math id="M14" display="block"><mml:mtable displaystyle="true"><mml:mlabeledtr id="Ch1.E1"><mml:mtd><mml:mtext>1</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:mtext>BL</mml:mtext><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo><mml:mo>=</mml:mo><mml:msub><mml:mtext>KZ</mml:mtext><mml:mrow><mml:mn mathvariant="normal">5</mml:mn><mml:mo>,</mml:mo><mml:mn mathvariant="normal">5</mml:mn></mml:mrow></mml:msub><mml:mfenced open="(" close=")"><mml:mrow><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mfenced></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E2"><mml:mtd><mml:mtext>2</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:mtext>SY</mml:mtext><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo><mml:mo>=</mml:mo><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo><mml:mo>-</mml:mo><mml:msub><mml:mtext>KZ</mml:mtext><mml:mrow><mml:mn mathvariant="normal">5</mml:mn><mml:mo>,</mml:mo><mml:mn mathvariant="normal">5</mml:mn></mml:mrow></mml:msub><mml:mfenced open="(" close=")"><mml:mrow><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mfenced></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E3"><mml:mtd><mml:mtext>3</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo><mml:mo>=</mml:mo><mml:mtext>SY</mml:mtext><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo><mml:mo>+</mml:mo><mml:mtext>BL</mml:mtext><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr></mml:mtable></mml:math></disp-formula>

          Because we are working with the daily maximum 8 <inline-formula><mml:math id="M15" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">h</mml:mi></mml:mrow></mml:math></inline-formula> ozone data, the Nyquist
interval is 2 <inline-formula><mml:math id="M16" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">d</mml:mi></mml:mrow></mml:math></inline-formula>, indicating that the dynamical features having timescales less than 2 <inline-formula><mml:math id="M17" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">d</mml:mi></mml:mrow></mml:math></inline-formula> (e.g., intra-day forcing from fast changing
emissions and chemical transformations, boundary layer evolution, and diurnal
forcing due to night vs. day differences) are not resolvable in this
analysis (see Fig. 2 in Dennis et al., 2010). The 50 % cutoff frequency
for the KZ<inline-formula><mml:math id="M18" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">5</mml:mn><mml:mo>,</mml:mo><mml:mn mathvariant="normal">5</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula> is <inline-formula><mml:math id="M19" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">24</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M20" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">d</mml:mi></mml:mrow></mml:math></inline-formula>, and, hence, timescales less
than those associated with large-scale weather fluctuations are embedded
in the short-term or SY forcing. The KZ filtering is applied to both DM8HR
observations and modeled DM8HR time series. Once the baseline is separated
from the original DM8HR time series from all monitoring stations, then the
synoptic forcing in the historical ozone time series data is used to
estimate the variability in ozone concentrations that can be expected
because of the chaotic/stochastic nature of the atmosphere by taking into
account the relationship between the strength of synoptic forcing and mean
of baseline ozone at each location over CONUS; this methodology was applied
to both measured and modeled ozone concentrations (see details in Luo et
al., 2019). Whereas the focus of Luo et al. (2019) was on transforming the
deterministic modeling results into a probabilistic framework for assessing
the efficacy of different emission control strategies<?pagebreak page1630?> in achieving
compliance with the ozone standard, this paper is aimed at quantifying the
model performance errors to be expected at each monitoring site over CONUS
even from perfect regional-scale ozone models driven with perfect
input data from the ever-present stochastic nature of the atmosphere.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1" specific-use="star"><?xmltex \currentcnt{1}?><label>Figure 1</label><caption><p id="d1e507">Results of the application of the Improved CEEMDAN technique (a
modified version of EMD), which is designed for analyzing
non-stationary and non-linear time series (TS) data to the daily maximum 8 <inline-formula><mml:math id="M21" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">h</mml:mi></mml:mrow></mml:math></inline-formula>
ozone time series data at the Altoona, PA, site. The numbers on the right
side represent the timescale (in days) associated with each IMF. Note that the
power spectrum of raw ozone time series (upper right panel) shows that the
energy in the 1–10 <inline-formula><mml:math id="M22" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">d</mml:mi></mml:mrow></mml:math></inline-formula> (synoptic) timescale is an order of magnitude less
than that in the longer (baseline) timescale.</p></caption>
        <?xmltex \igopts{width=483.69685pt}?><graphic xlink:href="https://acp.copernicus.org/articles/20/1627/2020/acp-20-1627-2020-f01.png"/>

      </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2" specific-use="star"><?xmltex \currentcnt{2}?><label>Figure 2</label><caption><p id="d1e535"><bold>(a)</bold> Raw observed (OBS) DM8HR ozone time series (black) and the embedded
baseline (BL; red for EMD and blue for KZ) at Altoona, PA, in 2010. <bold>(b)</bold> Time series of synoptic (SY) forcing (red for EMD and blue for KZ). Panels <bold>(c)</bold> and
<bold>(d)</bold> show their corresponding power spectra. Panels <bold>(c)</bold> and <bold>(d)</bold> compare the
power spectra of the baseline forcing <bold>(c)</bold> and the synoptic forcing <bold>(d)</bold> derived from KZ filtering and EMD (sum of IMF1 and IMF2). Notice that most of the energy in the baseline time series is in the longer timescale, while most of the energy of the short-term component is in the
high-frequency range. The similarity of results from both scale separation
techniques demonstrates that the two scales of interest (i.e., baseline and
synoptic forcing) have been extracted reasonably well by these two methods.</p></caption>
        <?xmltex \igopts{width=398.338583pt}?><graphic xlink:href="https://acp.copernicus.org/articles/20/1627/2020/acp-20-1627-2020-f02.png"/>

      </fig>

</sec>
<sec id="Ch1.S3">
  <label>3</label><title>Results and discussion</title>
<sec id="Ch1.S3.SS1">
  <label>3.1</label><title>Analysis of ambient ozone data</title>
      <p id="d1e583">Using both Improved CEEMDAN and KZ filtering methods, we separated the
synoptic forcing (timescale <inline-formula><mml:math id="M23" display="inline"><mml:mrow><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">24</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M24" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">d</mml:mi></mml:mrow></mml:math></inline-formula>) and baseline (timescale
<inline-formula><mml:math id="M25" display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> month) forcing embedded in the time series of observed and
modeled daily maximum 8 <inline-formula><mml:math id="M26" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">h</mml:mi></mml:mrow></mml:math></inline-formula> ozone concentrations. To illustrate, the
results from the application of Improved CEEMDAN to the daily maximum 8 <inline-formula><mml:math id="M27" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">h</mml:mi></mml:mrow></mml:math></inline-formula>
ozone time series data measured at Altoona, PA, are presented in Fig. 1. The
top left panel displays the raw ozone time series, while the top of the right
panel shows its power spectrum. The seven intrinsic mode functions (IMFs) and
the residual on the left side as well as their corresponding power spectra on the
right reveal that most of the synoptic-scale features in ozone data are
imbedded in IMFs 1 and 2. The baseline ozone is extracted by removing the
first two IMFs from the raw ozone time series. To illustrate the concept of
the ozone baseline, DM8HR time series measured in 2010 at Altoona, PA, are
presented in Fig. 2a together with the embedded baseline concentration as
extracted by the KZ<inline-formula><mml:math id="M28" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">5</mml:mn><mml:mo>,</mml:mo><mml:mn mathvariant="normal">5</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula> and Improved CEEMDAN. It is evident that high
ozone levels are always associated with the elevated baseline. The
difference between the raw ozone time series and baseline, denoted as the
short-term or synoptic forcing, is displayed in Fig. 2b. The power
spectra, displayed in Fig. 2c and d, reveal both methods yielded good scale
separation. Due to the good agreement between both scale separation
techniques, only the results from the KZ filter are presented for the
remainder of the paper.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3" specific-use="star"><?xmltex \currentcnt{3}?><label>Figure 3</label><caption><p id="d1e647"><bold>(a)</bold> Comparison between the observed cumulative distribution function
(CDF) for 2010 shown in red with <inline-formula><mml:math id="M29" display="inline"><mml:mrow><mml:mn mathvariant="normal">30</mml:mn><mml:mo>+</mml:mo></mml:mrow></mml:math></inline-formula> pseudo-observation CDFs generated
from historical DM8HR ozone time series shown in gray at a suburban site at
Altoona, PA (AQS station identifier 420130801). The blue line represents
the average of the <inline-formula><mml:math id="M30" display="inline"><mml:mrow><mml:mn mathvariant="normal">30</mml:mn><mml:mo>+</mml:mo></mml:mrow></mml:math></inline-formula> gray lines. <bold>(b)</bold> Display of various
statistical performance (perf.) metrics (standard deviation – std, root mean square error
– RMSE, and bias) derived by comparing the actual observed and pseudo ozone
values in panel <bold>(a)</bold>. <bold>(c)</bold> Normalized statistical metrics of the normalized
mean error (NME), normalized mean bias (NMB), and coefficient of variation (CV).
Notice the large variability occurring at the lower and upper percentiles.</p></caption>
          <?xmltex \igopts{width=483.69685pt}?><graphic xlink:href="https://acp.copernicus.org/articles/20/1627/2020/acp-20-1627-2020-f03.png"/>

        </fig>

      <p id="d1e687">Once the scale separation is achieved with the KZ<inline-formula><mml:math id="M31" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">5</mml:mn><mml:mo>,</mml:mo><mml:mn mathvariant="normal">5</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula>, we
superimposed the SY forcing imbedded in <inline-formula><mml:math id="M32" display="inline"><mml:mrow><mml:mn mathvariant="normal">30</mml:mn><mml:mo>+</mml:mo></mml:mrow></mml:math></inline-formula> years of historical DM8HR
ozone time series measured at a given location on the baseline component of
the ozone time series at that location to generate <inline-formula><mml:math id="M33" display="inline"><mml:mrow><mml:mn mathvariant="normal">30</mml:mn><mml:mo>+</mml:mo></mml:mrow></mml:math></inline-formula> reconstructed or
pseudo ozone distributions. Illustrative results using Eq. (3) at a suburban
location in Altoona, PA, are presented for the 2010 base year in Fig. 3a; it
should be noted that the linear relationship between the strength of SY
(defined as the standard deviation of the data in the synoptic component)
and the magnitude of the BL (defined as the mean of the data in the baseline
component) has been taken into account in generating <inline-formula><mml:math id="M34" display="inline"><mml:mrow><mml:mn mathvariant="normal">30</mml:mn><mml:mo>+</mml:mo></mml:mrow></mml:math></inline-formula> years of adjusted
SY forcing as illustrated in Luo et al. (2019). As expected, there is
excellent agreement between the average of <inline-formula><mml:math id="M35" display="inline"><mml:mrow><mml:mn mathvariant="normal">30</mml:mn><mml:mo>+</mml:mo></mml:mrow></mml:math></inline-formula> values (solid blue line)
and observed ozone in 2010 at each percentile of the concentration
distribution function (red line). Also, the original cumulative distribution
function (CDF) in 2010 (red line) is constrained within the <inline-formula><mml:math id="M36" display="inline"><mml:mrow><mml:mn mathvariant="normal">30</mml:mn><mml:mo>+</mml:mo></mml:mrow></mml:math></inline-formula> CDFs of
pseudo distributions (Fig. 3a); note that it is equally likely for any of these
<inline-formula><mml:math id="M37" display="inline"><mml:mrow><mml:mn mathvariant="normal">30</mml:mn><mml:mo>+</mml:mo></mml:mrow></mml:math></inline-formula> CDFs to occur because of the stochastic nature of the atmosphere even
though the individual event in 2010 yielded the CDF shown in red. As
mentioned before, an ozone mixing ratio at any given probability point on the
red line in Fig. 3a reflects an individual event, while ozone values at the
same probability in different CDFs (gray lines) reflect the population
stemming from the stochastic nature of the atmosphere. In other words, there
are <inline-formula><mml:math id="M38" display="inline"><mml:mrow><mml:mn mathvariant="normal">30</mml:mn><mml:mo>+</mml:mo></mml:mrow></mml:math></inline-formula> dynamically consistent ozone time series attributable to the 2010
baseline (given 2010 emissions) for examining the inherent variability due
to atmospheric stochasticity. It is evident in Fig. 3a that there is larger
variability at the lower and upper percentiles than that in interquartile
range, revealing that the tails of the concentration distribution function
are subject to large inherent uncertainty. Using these <inline-formula><mml:math id="M39" display="inline"><mml:mrow><mml:mn mathvariant="normal">30</mml:mn><mml:mo>+</mml:mo></mml:mrow></mml:math></inline-formula>
pseudo-observation ozone mixing ratios and the actual observed ozone values
at each percentile, statistical metrics such as bias, the RMSE, the coefficient of
variation (<inline-formula><mml:math id="M40" display="inline"><mml:mrow><mml:mtext>CV</mml:mtext><mml:mo>=</mml:mo><mml:mtext>standard deviation</mml:mtext><mml:mo>/</mml:mo><mml:mtext>mean</mml:mtext></mml:mrow></mml:math></inline-formula>), the normalized mean error (NME), and
the normalized mean bias (NMB) are presented in Fig. 3b and c (see Emery et al.,
2016, for the description of the statistical metrics considered here). As
expected, the lower and upper tails of the distribution are prone to large
errors. These results demonstrate the presence of substantial natural
variability at the upper 95th percentile, which is of primary interest in
regulatory analyses. The extreme values are better described in statistical
terms rather than in deterministic sense (Rao and Visalli, 1981; Hogrefe and Rao, 2001; Luo et al.,
2019).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4" specific-use="star"><?xmltex \currentcnt{4}?><label>Figure 4</label><caption><p id="d1e804">Box plots of statistical metrics based on the results from the
analysis of DM8HR data at 185 monitoring sites: <bold>(a)</bold> standard deviation, <bold>(b)</bold> root mean square error, <bold>(c)</bold> mean bias, <bold>(d)</bold> coefficient of variation, <bold>(e)</bold> normalized mean error, and <bold>(f)</bold> normalized mean bias. The lower and upper
edges of the boxes represent the 25th and 75th percentile values, while the
whiskers represent the 5th and 95th percentiles. See data analysis
procedures using the ozone baseline observed in the year 2010 as the target
baseline in Eqs. (7) and (8) of Luo et al. (2019).</p></caption>
          <?xmltex \igopts{width=483.69685pt}?><graphic xlink:href="https://acp.copernicus.org/articles/20/1627/2020/acp-20-1627-2020-f04.png"/>

        </fig>

      <p id="d1e832">Ozone time series at 185 monitoring stations covering CONUS, having at least
80 % data completeness, are analyzed in the above manner, and the results
are displayed as box plots in Fig. 4. Note the presence of large variability
in the CV, NME, NMB, and bias at the lower and upper percentiles (Fig. 4). The RMSE expected for the ozone mixing ratios in the interquartile range
is <inline-formula><mml:math id="M41" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">1.5</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M42" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">ppb</mml:mi></mml:mrow></mml:math></inline-formula>, but it is <inline-formula><mml:math id="M43" display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">5</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M44" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">ppb</mml:mi></mml:mrow></mml:math></inline-formula> for the upper 95th
percentile (Fig. 4b). The spatial distribution of the RMSE at the 50th and 95th
percentiles is displayed in Fig. 5a and b, respectively. The RMSE at the
upper 95th percentile is very high at some monitoring sites in California
and Michigan (Fig. 5b). Monitoring stations situated in the urban areas,
near large bodies of water, and in regions of complex terrain influenced
predominantly by local conditions tend to exhibit higher RMSE values. The elevation
of the monitoring sites is displayed in Fig. 5c.</p>

      <?xmltex \floatpos{p}?><fig id="Ch1.F5" specific-use="star"><?xmltex \currentcnt{5}?><label>Figure 5</label><caption><p id="d1e873">Spatial distribution of the lower bound for the RMSE or expected
RMSE at each monitoring site over CONUS <bold>(a)</bold> at the median and <bold>(b)</bold> at the
95th percentile. <bold>(c)</bold> Elevation (km) above the mean sea level of each
monitoring site.</p></caption>
          <?xmltex \igopts{width=483.69685pt}?><graphic xlink:href="https://acp.copernicus.org/articles/20/1627/2020/acp-20-1627-2020-f05.png"/>

        </fig>

</sec>
<sec id="Ch1.S3.SS2">
  <label>3.2</label><title>Analysis of modeled ozone concentrations</title>
      <p id="d1e899">The analysis in the previous section quantified the inherent stochastic
variability that is present in the SY component using long-term records of
ozone observations. In this section, we analyze long-term records of model
simulations in an attempt to quantify the error associated with the modeled
SY<?pagebreak page1631?> component that results both from not explicitly representing stochastic
variations in atmospheric dynamics in the current generation regional air
quality models and from other reducible sources of model error. The model
simulations were performed with the fully coupled WRF-CMAQ system with a
36 <inline-formula><mml:math id="M45" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">km</mml:mi></mml:mrow></mml:math></inline-formula> horizontal grid cell size and covered the 21-year period from 1990 to
2010 (Gan et al., 2015). In this section, we examine the impact of
superimposing different SY forcings embedded in ozone observations vs. those
in the WRF-CMAQ model on the observed baseline concentration. To provide an
illustration of the differences between observed and modeled time series
over this period, Fig. 6a displays a scatter plot of the strength of the
SY component (standard deviation of data in the SY component) vs. the mean
of the baseline component for both observations and model simulations
at the Altoona, PA, site. While both observations and WRF-CMAQ simulations
show a strong correlation between these two variables, it is evident that at
this monitoring location the standard deviation (i.e., strength) of the SY
component is substantially lower for the WRF-CMAQ simulations for a given
mean of the BL component (i.e., for any given year). The year-to-year
variation in the observed and modeled mean of the BL and strength of SY forcing,
displayed in Fig. 6b, reveals that the model overestimated the BL and
underestimated the strength of SY forcing. The 36 <inline-formula><mml:math id="M46" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">km</mml:mi></mml:mrow></mml:math></inline-formula> grid may be better for
representing the large-scale synoptic forcing associated with the
translation of weather systems than the meso-scale weather and urban
influences (both dynamics and chemistry) that are embedded in the observed
SY component. Meteorological modeling with higher horizontal grid resolution
might be able to capture the land–sea breeze, lake–sea breeze, and terrain
influences that observations are seeing at certain monitoring locations.</p>

      <?xmltex \floatpos{p}?><fig id="Ch1.F6" specific-use="star"><?xmltex \currentcnt{6}?><label>Figure 6</label><caption><p id="d1e920"><bold>(a)</bold> Scatter plot of the standard deviation (i.e., strength) of the
synoptic (SY) component vs. the mean of the baseline (BL) component for each of the 21 years from 1990 to 2010 at the Altoona, PA, monitoring site. Observations are
shown in red, while WRF-CMAQ results are shown in blue. <bold>(b)</bold> Inter-annual
variability in the mean of the baseline component and standard deviation of
the synoptic component in the WRF-CMAQ model and observations at the
Altoona, PA, site. Although year-to-year variation is captured, the model has
overestimated the baseline forcing and underestimated the synoptic forcing.</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/20/1627/2020/acp-20-1627-2020-f06.png"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F7" specific-use="star"><?xmltex \currentcnt{7}?><label>Figure 7</label><caption><p id="d1e936"><bold>(a)</bold> Comparison between the observed CDF overlaid on 21 “pseudo-simulated” or reconstructed ozone CDFs with SY generated from
modeled DM8HR ozone time series at a suburban site at Altoona, PA (AQS
station identifier 420130801). <bold>(b)</bold> Display of various statistical performance (perf.) metrics
derived by comparing the actual observed and pseudo-simulated ozone values
in panel <bold>(a)</bold>. <bold>(c)</bold> Normalized statistical metrics. <bold>(d)</bold> Difference between the
pseudo-simulated CDFs shown in panel <bold>(a)</bold> and the pseudo-observed CDFs as
shown in panel <bold>(a)</bold> but calculated from 21 years (1990–2010) of observations
only. The gray lines represent the differences for a specific SY year, while
the blue line represents the differences between the means of the 21
reconstructions. <bold>(e)</bold> Difference between the absolute performance metrics for
pseudo-simulations shown in panel <bold>(b)</bold> and those calculated for
pseudo-observations as shown in panel <bold>(b)</bold> but calculated for 21 years
(1990–2010) only. <bold>(f)</bold> As in panel <bold>(e)</bold> but for normalized performance metrics.</p></caption>
          <?xmltex \igopts{width=483.69685pt}?><graphic xlink:href="https://acp.copernicus.org/articles/20/1627/2020/acp-20-1627-2020-f07.png"/>

        </fig>

      <?pagebreak page1633?><p id="d1e982">To isolate the impact of model imperfections on only the SY timescale on
errors across the ozone distribution, we assume that the model perfectly
reproduces the “true” BL depicted by the observed 2010 BL. We then use this
perfect modeled BL and reconstruct “pseudo-simulated” ozone time series,
like what was done in Fig. 3, except for using the SY component embedded in
the 21 years of coupled WRF-CMAQ simulations. The rationale for this
analysis is to quantify the amount of model error present in the current
simulations that could conceivably be reduced through improving the
representation of synoptic and mesoscale processes and/or increased
horizontal resolution with appropriate data assimilation techniques. Figure 7a
displays the CDF of actual observed ozone (red line) overlaid on 21
pseudo-simulated ozone CDFs (gray lines, with averages of all 21
pseudo-simulated ozone percentiles shown in blue) at the Altoona, PA, site,
while Fig. 7b and c display absolute and normalized performance metrics.
Figure 7a confirms that the coupled WRF-CMAQ SY components have less
intra-annual variability than observed SY components, causing overestimation
at the low end and underestimation at the high end of the observed CDF for
all 21 years of reconstruction; these results imply that the model's results
at the upper and lower percentiles will always tend to be unreliable or
prone to large errors even when the baseline concentration is predicted
perfectly. The U shape of the absolute and relative error curves in Fig. 7b and c is similar to the corresponding curves in Fig. 3, but the larger
magnitude at the high and low end of the distribution indicates that the
effects of the underestimated intra-annual SY variability (note that the
distribution of modeled values in Fig. 7a is much flatter, i.e., with a
higher kurtosis, than that of the observations) outweigh those errors
attributable to the stochastic variability presented in Fig. 3. The shape
of the absolute and normalized bias curves deviates from those shown for the
pseudo-observations in Fig. 3b–c and, thus, this also reveals the effect of
the underestimation of the intra-annual SY variability. Figure 7d–f present
differences between the curves shown in Fig. 7a–c and a version of Fig. 3a–c computed from the 1990–2010 data instead of <inline-formula><mml:math id="M47" display="inline"><mml:mrow><mml:mn mathvariant="normal">30</mml:mn><mml:mo>+</mml:mo></mml:mrow></mml:math></inline-formula> years of historical
ozone observations. Panels (e) and (f) show that at the 50th percentile,
the differences in the error curves are close to zero, since both the
pseudo-simulations and pseudo-observations used the same observed BL
component. At the upper percentiles, the differences reach 3–5 <inline-formula><mml:math id="M48" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">ppb</mml:mi></mml:mrow></mml:math></inline-formula>,
providing an estimate of the reducible error in simulating the extreme
values at this location because of the differences in the observed SY and
WRF-CMAQ SY components at this location; high-resolution meteorological
modeling may help address these reducible errors.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F8" specific-use="star"><?xmltex \currentcnt{8}?><label>Figure 8</label><caption><p id="d1e1005">Errors in the 21 “pseudo-simulated” or reconstructed ozone time
series with SY generated from modeled DM8HR ozone time series using BL
obtained from observations at <bold>(a)</bold> the median and <bold>(b)</bold> 95th percentile.</p></caption>
          <?xmltex \igopts{width=483.69685pt}?><graphic xlink:href="https://acp.copernicus.org/articles/20/1627/2020/acp-20-1627-2020-f08.png"/>

        </fig>

      <?pagebreak page1636?><p id="d1e1020">Figure 8a and b display the RMSE at the median and 95th percentile for
the pseudo-simulated ozone values at each monitoring site. For the
50th percentile, the RMSE values range from 0.2 to 3.2 ppb over
CONUS with a median value of 1 ppb, while at the 95th percentile, the
RMSE values range from 1 to 15 ppb with a median value of 4 ppb across
all sites over CONUS. The values are highest along the California coast and
near Great Lakes, possibly due to inadequacies in simulating the land–sea
breeze and land–lake breeze regimes, respectively, with modeling at 36 <inline-formula><mml:math id="M49" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">km</mml:mi></mml:mrow></mml:math></inline-formula>
grid cells. Air quality modeling uncertainty even for the retrospective
modeling cases, outside of the chemistry formulation and boundary
conditions, is attributed primarily to meteorology and emissions inputs.
Vautard et al. (2012) and McNider and Pour-Biazar (2020) concluded that
major challenges remain in the simulation of prevailing meteorology (e.g.,
errors in wind speed, PBL, night-time meteorology, nocturnal transport
aloft, and clouds) in retrospective air quality modeling. Based on the
retrospective ozone episodic modeling with the WRF-CMAQ model using various
sets of equally likely initial conditions for meteorology along with FDDA,
Gilliam et al. (2015) confirmed the presence of sizable spread in WRF
solutions, including common weather variables of temperature, wind, boundary
layer depth, clouds, and radiation, thereby causing a relatively large range
of ozone concentrations. Also, pollutant transport is altered by hundreds of
kilometers over several days. Ozone concentrations of the ensemble varied by as
much as 10–20 ppb (or 20 %–30 %) in areas that typically have higher
pollution levels. As model improvements are made, one can quantitatively
assess how close the predictions of the improved model are for each
percentile for the given base year simulation to the expected errors from a
perfect model with perfect input, i.e., the target RMSE shown in
Fig. 5a and b. Perhaps, the next generation of regional-scale meteorological
and air quality models might be capable of explicitly simultaneously
treating the mean and fluctuation components for all variables within the
deterministic–stochastic modeling framework to properly account for the
stochastic nature of the atmosphere.</p>
</sec>
</sec>
<sec id="Ch1.S4" sec-type="conclusions">
  <label>4</label><title>Conclusions</title>
      <p id="d1e1040">Regardless of how accurate the regional air quality model is, the stochastic
variations in the atmosphere cannot be consistently reproduced by the
deterministic numerical models. In this study, we demonstrate how to
quantify this irreproducible stochastic component by isolating the synoptic
forcing imbedded in <inline-formula><mml:math id="M50" display="inline"><mml:mrow><mml:mn mathvariant="normal">30</mml:mn><mml:mo>+</mml:mo></mml:mrow></mml:math></inline-formula> years of historical observations and assess the
performance of the 36 <inline-formula><mml:math id="M51" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">km</mml:mi></mml:mrow></mml:math></inline-formula> fully coupled WRF-CMAQ model in simulating 21 years
of ozone concentrations over the contiguous US. Observation-based analysis
reveals that on average, the irreducible error attributable to the
stochastic nature of the atmosphere ranges from <inline-formula><mml:math id="M52" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> ppb at the
50th percentile to <inline-formula><mml:math id="M53" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">5</mml:mn></mml:mrow></mml:math></inline-formula> ppb at the 95th percentile.
To improve regional-scale ozone air quality models, attention should be paid
to accurately simulate the baseline concentration by focusing on the quality
of the emission inventory and the model's treatment for the boundary
conditions and slow-changing (operating on sub-seasonal, seasonal, and
longer-term timescales) atmospheric processes. Also, errors in reproducing
the synoptic forcing can possibly be reduced with high-resolution
meteorological modeling using appropriate data assimilation techniques.
Nonetheless, these results demonstrate the presence of large variability in
the upper tail of the DM8HR <inline-formula><mml:math id="M54" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> concentration cumulative distribution
even with perfect models using perfect input data. Having
this quantitative estimation of practical limits for a model's accuracy helps
in objectively assessing the current state of regional-scale air quality
models, measuring progress in their evolution, and providing meaningful and
firm targets for improvements in their accuracy relative to measurements
from routine networks.</p>
</sec>

      
      </body>
    <back><notes notes-type="codeavailability"><title>Code availability</title>

      <p id="d1e1097">Source code for version 5.0.2 of the Community
Multiscale Air Quality (CMAQ) modeling system can be downloaded from
<uri>https://github.com/USEPA/CMAQ/tree/5.0.2</uri> (last access: 3 February 2020) (US EPA Office of Research and Development, 2014, <ext-link xlink:href="https://doi.org/10.5281/zenodo.1079898" ext-link-type="DOI">10.5281/zenodo.1079898</ext-link>). For further
information, please visit the U.S. Environmental Protection Agency website
for the CMAQ system at <uri>https://www.epa.gov/cmaq</uri> (last access: 3 February 2020).</p>
  </notes><notes notes-type="dataavailability"><title>Data availability</title>

      <p id="d1e1112">All ozone observations used in this article are
available from <uri>https://aqs.epa.gov/aqsweb/airdata/download_files.html</uri>  (AQS) (last access: 3 February 2020). Paired ozone observation and CMAQ model data used in the
analysis will be made available at
<uri>https://edg.epa.gov/metadata/catalog/main/home.page</uri> (last access: 3 February 2020). Raw CMAQ model outputs
are available on request from the EPA authors.</p>
  </notes><notes notes-type="authorcontribution"><title>Author contributions</title>

      <p id="d1e1124">STR conceptualized the idea. STR, CH, VG, and
RM designed the analysis approach. CH and RM post-processed previously
conducted model simulations. HL performed data analyses and prepared the
illustrations. STR prepared the paper with contributions from all
co-authors.</p>
  </notes><notes notes-type="competinginterests"><title>Competing interests</title>

      <p id="d1e1130">The authors declare that they have no conflict of interest.</p>
  </notes><notes notes-type="disclaimer"><title>Disclaimer</title>

      <p id="d1e1136">The views expressed in this paper are those of the
authors and do not necessarily represent the view or policies of the U.S.
Environmental Protection Agency.</p>
  </notes><ack><title>Acknowledgements</title><p id="d1e1142">The authors thank the reviewers for their constructive comments that have helped improve the paper.</p></ack><notes notes-type="reviewstatement"><title>Review statement</title>

      <p id="d1e1147">This paper was edited by Leiming Zhang and reviewed by two anonymous referees.</p>
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<abstract-html><p>Regional-scale air pollution models are routinely being
used worldwide for research, forecasting air quality, and regulatory
purposes. It is well recognized that there are both reducible (systematic)
and irreducible (unsystematic) errors in the meteorology–atmospheric-chemistry modeling systems. The inherent (random) uncertainty stems from our
inability to properly characterize stochastic variations in atmospheric
dynamics and chemistry and from the incommensurability associated with
comparisons of the volume-averaged model estimates with point measurements.
Because stochastic variations are not being explicitly simulated in
the current generation of regional-scale meteorology–air quality models, one
should expect to find differences between the model estimates and
corresponding observations. This paper presents an observation-based
methodology to determine the expected errors from current-generation
regional air quality models even when the model design, physics, chemistry,
and numerical analysis, as well as its input data, were <q>perfect</q>. To this
end, the short-term synoptic-scale fluctuations embedded in the daily
maximum 8&thinsp;h ozone time series are separated from the longer-term forcing
using a simple recursive moving average filter. The inherent uncertainty
attributable to the stochastic nature of the atmosphere is determined based
on 30+ years of historical ozone time series data measured at various
monitoring sites in the contiguous United States (CONUS). The results reveal that
the expected root mean square error (RMSE) at the median and 95th percentile
is about 2 and 5&thinsp;ppb, respectively, even for perfect air quality
models driven with perfect input data. Quantitative estimation of the
limit to the model's accuracy will help in objectively assessing the current
state of the science in regional air pollution models, measuring progress in
their evolution, and providing meaningful and firm targets for improvements
in their accuracy relative to ambient measurements.</p></abstract-html>
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