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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-18-15515-2018</article-id><title-group><article-title>A deep stratosphere-to-troposphere ozone transport event over Europe simulated
in CAMS global and regional forecast <?xmltex \hack{\break}?>systems: analysis and evaluation</article-title><alt-title>Stratosphere-to-troposphere ozone transport event in CAMS</alt-title>
      </title-group><?xmltex \runningtitle{Stratosphere-to-troposphere ozone transport event in CAMS}?><?xmltex \runningauthor{D. Akritidis et al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes" rid="aff1">
          <name><surname>Akritidis</surname><given-names>Dimitris</given-names></name>
          <email>dakritid@geo.auth.gr</email>
        <ext-link>https://orcid.org/0000-0003-3104-5271</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Katragkou</surname><given-names>Eleni</given-names></name>
          
        <ext-link>https://orcid.org/0000-0003-0863-3411</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Zanis</surname><given-names>Prodromos</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-3496-2692</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Pytharoulis</surname><given-names>Ioannis</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-5865-5216</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Melas</surname><given-names>Dimitris</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3">
          <name><surname>Flemming</surname><given-names>Johannes</given-names></name>
          
        <ext-link>https://orcid.org/0000-0003-4880-5329</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3">
          <name><surname>Inness</surname><given-names>Antje</given-names></name>
          
        <ext-link>https://orcid.org/0000-0003-0603-5389</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff4">
          <name><surname>Clark</surname><given-names>Hannah</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-5602-5328</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff5">
          <name><surname>Plu</surname><given-names>Matthieu</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-5374-1895</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff6">
          <name><surname>Eskes</surname><given-names>Henk</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-8743-4455</ext-link></contrib>
        <aff id="aff1"><label>1</label><institution>Department of Meteorology and Climatology, School of Geology, Aristotle University of Thessaloniki, Thessaloniki, Greece</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>Laboratory of Atmospheric Physics, Physics Department, Aristotle University of Thessaloniki, Thessaloniki, Greece</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>European Centre for Medium-Range Weather Forecasts, Reading, UK</institution>
        </aff>
        <aff id="aff4"><label>4</label><institution>Laboratoire d'Aérologie, Universíté de Toulouse, CNRS, UPS, Toulouse, France</institution>
        </aff>
        <aff id="aff5"><label>5</label><institution>Centre National de Recherches Météorologiques, Météo-France-CNRS, UMR 3589, Toulouse, France</institution>
        </aff>
        <aff id="aff6"><label>6</label><institution>Royal Netherlands Meteorological Institute (KNMI), De Bilt, the Netherlands</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Dimitris Akritidis (dakritid@geo.auth.gr)</corresp></author-notes><pub-date><day>29</day><month>October</month><year>2018</year></pub-date>
      
      <volume>18</volume>
      <issue>20</issue>
      <fpage>15515</fpage><lpage>15534</lpage>
      <history>
        <date date-type="received"><day>15</day><month>May</month><year>2018</year></date>
           <date date-type="rev-request"><day>31</day><month>May</month><year>2018</year></date>
           <date date-type="rev-recd"><day>30</day><month>September</month><year>2018</year></date>
           <date date-type="accepted"><day>8</day><month>October</month><year>2018</year></date>
      </history>
      <permissions>
        
        
      <license license-type="open-access"><license-p>This work is licensed under the Creative Commons Attribution 4.0 International License. To view a copy of this licence, visit <ext-link ext-link-type="uri" xlink:href="https://creativecommons.org/licenses/by/4.0/">https://creativecommons.org/licenses/by/4.0/</ext-link></license-p></license></permissions><self-uri xlink:href="https://acp.copernicus.org/articles/.html">This article is available from https://acp.copernicus.org/articles/.html</self-uri><self-uri xlink:href="https://acp.copernicus.org/articles/.pdf">The full text article is available as a PDF file from https://acp.copernicus.org/articles/.pdf</self-uri>
      <abstract>
    <p id="d1e199">Stratosphere-to-troposphere transport (STT) is an important natural source of
tropospheric ozone, which can occasionally influence ground-level ozone
concentrations relevant for air quality. Here, we analyse and evaluate the
Copernicus Atmosphere Monitoring Service (CAMS) global and regional forecast
systems during a deep STT event over Europe for the time period from 4 to 9 January 2017. The predominant synoptic condition is described by a deep upper
level trough over eastern and central Europe, favouring the formation of
tropopause folding events along the jet stream axis and therefore the
intrusion of stratospheric ozone into the troposphere. Both global and
regional CAMS forecast products reproduce the “hook-shaped” streamer of
ozone-rich and dry air in the middle troposphere depicted from the observed
satellite images of water vapour. The CAMS global model successfully
reproduces the folding of the tropopause at various European sites, such as
Trapani (Italy), where a deep folding down to 550 hPa is seen. The
stratospheric ozone intrusions into the troposphere observed by WOUDC
ozonesonde and IAGOS aircraft measurements are satisfactorily forecasted up
to 3 days in advance by the CAMS global model in terms of both temporal and
vertical features of ozone. The fractional gross error (FGE) of CAMS ozone
day 1 forecast between 300 and 500 hPa is 0.13 over Prague, while over
Frankfurt it is 0.04 and 0.19, highlighting the contribution of data
assimilation, which in most cases improves the model performance. Finally, the
meteorological and chemical forcing of CAMS global forecast system in the CAMS
regional forecast systems is found to be beneficial for predicting the
enhanced ozone concentrations in the middle troposphere during a deep STT
event.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <title>Introduction</title>
      <?pagebreak page15516?><p id="d1e209">Ozone is a key species in tropospheric chemistry, as it largely regulates the
oxidation capacity of the troposphere <xref ref-type="bibr" rid="bib1.bibx61" id="paren.1"/>. Excessive
ozone concentrations near the earth's surface are known to be a risk to both
public health and ecosystems <xref ref-type="bibr" rid="bib1.bibx34 bib1.bibx84" id="paren.2"/>.
Moreover, tropospheric ozone is an important greenhouse gas
<xref ref-type="bibr" rid="bib1.bibx75" id="paren.3"/>, particularly in the upper troposphere, due to its
high radiative forcing efficiency <xref ref-type="bibr" rid="bib1.bibx44" id="paren.4"/>. Although
photochemistry is the dominant source of tropospheric ozone
<xref ref-type="bibr" rid="bib1.bibx21 bib1.bibx29 bib1.bibx55 bib1.bibx51 bib1.bibx60" id="paren.5"><named-content content-type="pre">e.g.</named-content></xref>,
the downward transport of ozone from the stratosphere is also an important
process in the tropospheric ozone budget
<xref ref-type="bibr" rid="bib1.bibx22 bib1.bibx32 bib1.bibx69 bib1.bibx78 bib1.bibx19 bib1.bibx64 bib1.bibx89 bib1.bibx3" id="paren.6"><named-content content-type="pre">e.g.</named-content></xref>.</p>
      <p id="d1e235">Deep and intense intrusions of stratospheric air penetrating down to lower
tropospheric levels or even to the planetary boundary layer are more relevant
than shallow ones for the atmospheric chemical composition, as they clearly
lead to irreversible mixing of stratospheric and tropospheric air and hence
to tropospheric composition changes affecting local air quality
<xref ref-type="bibr" rid="bib1.bibx77 bib1.bibx17 bib1.bibx18 bib1.bibx36 bib1.bibx2 bib1.bibx20 bib1.bibx4 bib1.bibx48 bib1.bibx49 bib1.bibx26 bib1.bibx47 bib1.bibx54 bib1.bibx42" id="paren.7"/>. Furthermore, recent modelling
studies indicate that the role of stratosphere-to-troposphere transport (STT)
in near-surface ozone may be of even greater importance than anticipated in
the 1990s and 2000s <xref ref-type="bibr" rid="bib1.bibx90 bib1.bibx53 bib1.bibx50 bib1.bibx89" id="paren.8"/>.</p>
      <p id="d1e244">Tropopause folds are considered to be the main mechanism of STT events
<xref ref-type="bibr" rid="bib1.bibx78" id="paren.9"/>. In principle, they are developed in the jet
stream entrance, as a result of the ageostrophic flow, and are associated
with penetrations of stratospheric air into the underlying troposphere
<xref ref-type="bibr" rid="bib1.bibx23" id="paren.10"/>, known as stratospheric intrusions. The key
features of stratospheric intrusions are ozone-rich air, anomalously high
potential vorticity (PV) levels and low water vapour mixing ratio
<xref ref-type="bibr" rid="bib1.bibx39 bib1.bibx85" id="paren.11"/>. Following the transport
into the troposphere, stratospheric air is quasi-adiabatically stirred by
large-scale disturbances, which might result in the development of elongated
streamers that can further dissipate down to smaller scales by
non-conservative processes and lead to irreversible mixing with the
surrounding air <xref ref-type="bibr" rid="bib1.bibx71 bib1.bibx6 bib1.bibx33" id="paren.12"/>. In general, the vast majority
of tropopause folds are of limited vertical extent and their spatio-temporal
occurrence is mostly governed by both the position and the intensity of the
subtropical jet stream <xref ref-type="bibr" rid="bib1.bibx39 bib1.bibx78" id="paren.13"/>.
Thus, the Northern Hemisphere tropopause folds' frequency exhibits a maximum
in the subtropics and during winter
<xref ref-type="bibr" rid="bib1.bibx76 bib1.bibx73" id="paren.14"/>, while during summer a
hotspot of tropopause fold activity is found over the eastern Mediterranean,
the Middle East and the Iran–Afghanistan regions, regulated by the complex
interaction between the subtropical jet and the South Asian Monsoon
anticyclone <xref ref-type="bibr" rid="bib1.bibx81" id="paren.15"/>. Deeper folds are also observed in the
subtropics and further north over the North Atlantic storm track, most often
during winter <xref ref-type="bibr" rid="bib1.bibx76 bib1.bibx73" id="paren.16"/>.</p>
      <p id="d1e272">In the past, several studies have focused on the investigation of the
prevailing synoptic and dynamic conditions governing the formation, evolution
and intensity of tropopause folds and stratospheric intrusions
<xref ref-type="bibr" rid="bib1.bibx71 bib1.bibx6 bib1.bibx66 bib1.bibx45 bib1.bibx83 bib1.bibx86 bib1.bibx7 bib1.bibx46 bib1.bibx10 bib1.bibx33" id="paren.17"><named-content content-type="pre">e.g.</named-content></xref>, while others have explored the impact of tropopause folds
on tropospheric ozone distribution and variability
<xref ref-type="bibr" rid="bib1.bibx9 bib1.bibx5 bib1.bibx24 bib1.bibx11 bib1.bibx13 bib1.bibx77 bib1.bibx88 bib1.bibx17 bib1.bibx19 bib1.bibx79 bib1.bibx80 bib1.bibx3" id="paren.18"><named-content content-type="pre">e.g.</named-content></xref>.</p>
      <p id="d1e286">Copernicus is the European Union's Earth Observation program. The Copernicus
Atmosphere Monitoring
Service<fn id="Ch1.Footn1"><p id="d1e289"><uri>https://atmosphere.copernicus.eu/</uri> (last access:
19 October 2018)</p></fn> (CAMS) is one of the six thematic areas that Copernicus
addresses. CAMS uses a comprehensive global assimilation and forecasting
system that estimates the state of the atmosphere and its composition on a
daily basis, combining information from models and observations, providing
daily 5-day forecasts of atmospheric composition fields, such as chemically
reactive gases and aerosols <xref ref-type="bibr" rid="bib1.bibx31 bib1.bibx41" id="paren.19"/>.
The CAMS global modelling system is also used to provide the boundary
conditions for the CAMS ensemble of regional air quality models, which
produce 4-day forecasts of European air quality. CAMS is in succession to the
EU-funded projects MACC (Monitoring Atmospheric Composition and Climate), and
MACC-II (Interim Implementation), which were established to build and
demonstrate a core capability for providing a comprehensive range of services
related to the chemical and particulate composition of the atmosphere
<xref ref-type="bibr" rid="bib1.bibx38 bib1.bibx30 bib1.bibx28" id="paren.20"/>.</p>
      <p id="d1e301">The aim of this work is a process-oriented analysis and evaluation of the
CAMS global and regional forecast modelling systems for a deep STT event
which affected tropospheric ozone in different parts of Europe. The added
value of this work is the linkage between the global and regional services
offered by CAMS, via the comparison of an ensemble of high-resolution
forecast simulations by the CAMS regional air quality models, with a forecast
simulation by the global CAMS model in an event of a deep STT. It also
investigates whether representations of upper tropospheric dynamical and chemical
processes in the CAMS global forecasting system are realistic and how
adequately the global forcing can contribute to accurate regional air quality
forecasts. This paper is structured in the following way. Section <xref ref-type="sec" rid="Ch1.S2"/> describes the CAMS forecasting system and the observational
validation data used in this study. Section <xref ref-type="sec" rid="Ch1.S3"/> shows the
results, and Sect. <xref ref-type="sec" rid="Ch1.S4"/> presents the main conclusions.</p>
</sec>
<sec id="Ch1.S2">
  <title>CAMS forecasting systems and observational data</title>
<sec id="Ch1.S2.SS1">
  <title>Composition in the ECMWF Integrated Forecasting System (IFS)</title>
      <?pagebreak page15517?><p id="d1e321">The operational CAMS global forecasting system uses fully
integrated chemistry in the European Centre for Medium-Range Weather
Forecasts (ECMWF) Integrated Forecasting System (IFS). The IFS meteorology
drives atmospheric composition changes, and the IFS simulates atmospheric
chemistry at a resolution of about 40 km <xref ref-type="bibr" rid="bib1.bibx31" id="paren.21"/>.
CAMS uses the IFS data assimilation system to assimilate observations of
atmospheric composition and includes weather–chemistry feedbacks <xref ref-type="bibr" rid="bib1.bibx41" id="paren.22"><named-content content-type="post">and
references therein</named-content></xref>. For ozone the CAMS near-real-time system
only assimilates satellite retrievals. These include total column ozone
retrievals from the Ozone Monitoring Instrument (OMI) and the Global Ozone
Monitoring Experiment-2 (GOME-2) on Metop-A and Metop-B, profile data from
the Microwave Limb Sounder (MLS) and partial columns from Solar Backscatter
Ultra-Violet (SBUV/2) and from the Ozone Mapping and Profiler Suite (OMPS).
Details of the ECMWF's 4-D data assimilation system for aerosol, greenhouse
gases and reactive gases can be found in <xref ref-type="bibr" rid="bib1.bibx41" id="text.23"/>.</p>
      <p id="d1e335">In addition to chemistry, IFS also includes greenhouse gases
<xref ref-type="bibr" rid="bib1.bibx27 bib1.bibx57 bib1.bibx1" id="paren.24"/> and aerosols
<xref ref-type="bibr" rid="bib1.bibx12 bib1.bibx62" id="paren.25"/>. IFS applies the Carbon
Bond 2005 (CB05) chemical mechanism, which describes tropospheric chemistry
with 55 species and 126 reactions <xref ref-type="bibr" rid="bib1.bibx31" id="paren.26"/>.
Stratospheric ozone chemistry in IFS is parameterized by the
Cariolle scheme <xref ref-type="bibr" rid="bib1.bibx14 bib1.bibx15" id="paren.27"/>.
Chemical tendencies of stratospheric and tropospheric ozone are merged at an
empirical interface of the diagnosed tropopause height in IFS
<xref ref-type="bibr" rid="bib1.bibx31" id="paren.28"/>. In this paper we use IFS day 1 forecasts of
ozone, geopotential, <inline-formula><mml:math id="M1" display="inline"><mml:mi>u</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M2" display="inline"><mml:mi>v</mml:mi></mml:math></inline-formula> wind components, specific humidity, relative
humidity and PV. In order to assess the impact of chemical data assimilation
on ozone representation during an STT event, an additional IFS control run
without data assimilation (free running ozone) is used for intercomparison.
Moreover, to evaluate the forecast performance of CAMS global forecast system
during the STT event the IFS day 2 to day 5 forecasts of ozone are also used.</p>
</sec>
<sec id="Ch1.S2.SS2">
  <title>CAMS air quality regional ensemble</title>
      <p id="d1e374">The CAMS regional forecasting service is operated by
Météo-France and provides daily 4-day forecasts of the main air
pollutants and pollens, from seven state-of-the-art regional atmospheric
chemistry models
(<uri>http://atmosphere.copernicus.eu/documentation-regional-systems</uri>, last access: 19 October 2018) and
from the median ensemble calculated from the seven model forecasts. The 96 h
forecasts are available with an hourly resolution and a spatial resolution of
0.1<inline-formula><mml:math id="M3" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> from the surface up to 5 km. Currently the CAMS regional
ensemble (RegEns) consists of the following regional models: CHIMERE from
INERIS (National Institute for Industrial Environment and Risks)
<xref ref-type="bibr" rid="bib1.bibx59" id="paren.29"/>, EMEP from MET-Norway <xref ref-type="bibr" rid="bib1.bibx72" id="paren.30"/>,
EURAD-IM from the University of Cologne <xref ref-type="bibr" rid="bib1.bibx58" id="paren.31"/>, LOTOS-EUROS
from KNMI (Royal Netherlands Meteorological Institute) and TNO (Netherlands
Organisation for Applied Scientific Research) <xref ref-type="bibr" rid="bib1.bibx70" id="paren.32"/>, MATCH
from SMHI (Swedish Meteorological and Hydrological Institute)
<xref ref-type="bibr" rid="bib1.bibx68" id="paren.33"/>, MOCAGE from Météo-France
<xref ref-type="bibr" rid="bib1.bibx37" id="paren.34"/> and SILAM from FMI (Finnish Meteorological Institute)
<xref ref-type="bibr" rid="bib1.bibx74" id="paren.35"/>. All regional model data are produced on a
horizontal domain of 25<inline-formula><mml:math id="M4" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W–45<inline-formula><mml:math id="M5" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E and
30–70<inline-formula><mml:math id="M6" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, covering a large European domain. The RegEns
members have been documented and evaluated during the MACC projects
<xref ref-type="bibr" rid="bib1.bibx56" id="paren.36"/>. The ozone results from RegEns and RegEns members
presented here correspond to day 1 forecasts. The meteorological conditions
in every model are driven by the operational ECMWF meteorological forecasts,
which are at 10 km horizontal resolution during the period of study. The
anthropogenic emissions are issued from the TNO MACC-III emission inventory
over Europe for the year 2011, which is an updated version of the TNO MACC-II
inventory <xref ref-type="bibr" rid="bib1.bibx43" id="paren.37"/>. All models use the concentrations of gas and aerosol species from the global CAMS
system as lateral boundary
conditions, which makes the regional model outputs consistent with the global
model output. The differences between the seven models thus come from the
different representation of the chemistry and aerosols, of the physical and
dynamical processes and of the natural emissions inside the domain.
Table <xref ref-type="table" rid="Ch1.T1"/> presents the CAMS models and simulations used in the
present study.</p>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T1" specific-use="star"><caption><p id="d1e450">CAMS models and simulations used in the present study.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="2">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="left"/>
     <oasis:thead>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">CAMS models and simulations</oasis:entry>
         <oasis:entry colname="col2">Description</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">CAMS</oasis:entry>
         <oasis:entry colname="col2">Copernicus Atmosphere Monitoring Service</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">IFS (CAMS global)</oasis:entry>
         <oasis:entry colname="col2">ECMWF Integrated Forecasting System</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">RegEns (CAMS regional ensemble)</oasis:entry>
         <oasis:entry colname="col2">Median ensemble of the seven CAMS regional model forecasts</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">IFS Forecast day 1</oasis:entry>
         <oasis:entry colname="col2">IFS forecast 1 day in advance</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">IFS Forecast day 2</oasis:entry>
         <oasis:entry colname="col2">IFS forecast 2 days in advance</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">IFS Forecast day 3</oasis:entry>
         <oasis:entry colname="col2">IFS forecast 3 days in advance</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">IFS Forecast day 4</oasis:entry>
         <oasis:entry colname="col2">IFS forecast 4 days in advance</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">IFS Forecast day 5</oasis:entry>
         <oasis:entry colname="col2">IFS forecast 5 days in advance</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">IFS no DA Forecast day 1</oasis:entry>
         <oasis:entry colname="col2">IFS forecast 1 day in advance without the use of data assimilation</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">RegEns Forecast day 1</oasis:entry>
         <oasis:entry colname="col2">Regional ensemble forecast 1 day in advance</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table></table-wrap>

</sec>
<sec id="Ch1.S2.SS3">
  <title>Observational data</title>
      <p id="d1e574">The observational data used in this paper include
images by the Meteosat Second Generation (MSG) (Geo-Stationary) Satellite
(NERC Satellite Receiving Station, Dundee University, Scotland,
<uri>http://www.sat.dundee.ac.uk/</uri>, last access: 17 March 2017). MSG carries
the Spinning Enhanced Visible and InfraRed Imager (SEVIRI) instrument, which
has the capacity to observe the Earth in 12 spectral channels. Here, we
present images from the mid-infrared/water vapour channel (5.35–7.15 <inline-formula><mml:math id="M7" display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>m) for 12:00 Z
on 6 January 2017 and 12:00 Z on 7 January 2017. Radiosonde data in the form of
skew-T log-P diagrams (taken from the Wyoming University, Department of
Atmospheric Science, <uri>http://weather.uwyo.edu/upperair/sounding.html</uri>
last access: 27 April 2018) are used from four European stations:
<list list-type="order"><list-item>
      <p id="d1e592">Norderney (10113), Germany, 53.71<inline-formula><mml:math id="M8" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N–7.15<inline-formula><mml:math id="M9" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E (12:00 Z on 3 January 2017 and 12:00 Z
on 4 January 2017);</p></list-item><list-item>
      <p id="d1e614">Muenchen-Oberschleißheim (10868), Germany, 48.25<inline-formula><mml:math id="M10" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N–11.55<inline-formula><mml:math id="M11" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E (00:00 Z on 4 January 2017 and 12:00 Z
on 5 January 2017);</p></list-item><list-item>
      <p id="d1e636">Trapani (16429), Italy, 37.91<inline-formula><mml:math id="M12" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N–12.50<inline-formula><mml:math id="M13" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E (00:00 Z on 5 January 2017 and 00:00 Z
on 6 January 2017);</p></list-item><list-item>
      <?pagebreak page15518?><p id="d1e658">Heraklion (16754), Greece, 35.33<inline-formula><mml:math id="M14" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N–25.18<inline-formula><mml:math id="M15" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E (12:00 Z on 5 January 2017 and 00:00 Z
on 8 January 2017).</p></list-item></list>
Ozonesonde data over Prague [STN242], Czech Republic (50.00<inline-formula><mml:math id="M16" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N–14.44<inline-formula><mml:math id="M17" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E), are obtained from
the World Ozone and Ultraviolet Radiation Data Center (WOUDC) <xref ref-type="bibr" rid="bib1.bibx87" id="paren.38"/> for 11:00 Z on 2 January 2017 and
11:00 Z on 4 January 2017 (last access: 9 June 2017).</p>
      <p id="d1e702">Also used are aircraft ozone measurements from the IAGOS (In-service Aircraft
for a Global Observing System) programme, for which instruments are carried on
commercial airlines. In IAGOS CORE, instruments measure ozone, carbon
monoxide and water vapour, along with meteorological parameters and cloud
particles. Details of the IAGOS project can be found in
<xref ref-type="bibr" rid="bib1.bibx65" id="text.39"/>, with the technical aspects of the instrumentation,
operations and validation in <xref ref-type="bibr" rid="bib1.bibx63" id="text.40"/>. Ozone and
carbon monoxide are provided to CAMS in near-real time for monitoring
atmospheric composition. For the purposes of this validation in near-real
time, the data are provided after only an initial validation. After the
instruments have been operating for a period of 6–12 months, they are then
calibrated in the laboratory and a final version of the data is released. The
data used here have therefore been validated but not yet calibrated. However,
the ozone measurements are not expected to change significantly. Landing and
take-off profiles are compared with the models at Frankfurt Airport. It
should be noted that the profiles are not strictly vertical. To this end, and
in order to perform a more realistic evaluation of CAMS models, according to
the flight position (longitude, latitude, pressure), the respective grid
points are extracted at the nearest time to that of the take-off or landing
for both IFS and RegEns. It is noteworthy to mention that both ozonesondes
and IAGOS profiles are not assimilated, and hence they constitute completely
independent validation data.</p><?xmltex \hack{\newpage}?>
</sec>
</sec>
<sec id="Ch1.S3">
  <title>Results</title>
<sec id="Ch1.S3.SS1">
  <title>Synoptic analysis</title>
      <p id="d1e724">In early January 2017, severe winter weather struck
several European regions, namely the Baltic Sea, northern Germany, Italy, the
Balkan Peninsula and Turkey, with flooding, extreme cold and snow
<xref ref-type="bibr" rid="bib1.bibx52" id="paren.41"/>. The international news media reported that at least 61 people
died because of the extremely cold weather conditions in central, eastern and
southern Europe <xref ref-type="bibr" rid="bib1.bibx8" id="paren.42"/>. The prevailing synoptic conditions associated
with these weather events are depicted in Fig. <xref ref-type="fig" rid="Ch1.F1"/>, which
presents the temporal evolution (every 12 h) of IFS geopotential height,
wind speed and wind direction at 300 hPa during the time period 3–9 January 2017. An upper level ridge gradually formed over the eastern Atlantic
and western Europe in conjunction with a deep upper level trough over eastern
and central Europe. Additionally, the jet stream was found on the western
side of the upper level trough, with wind speeds occasionally exceeding 65 <inline-formula><mml:math id="M18" display="inline"><mml:mrow><mml:mi mathvariant="normal">m</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">s</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> (12:00 Z on 4 January 2017 and 00:00 Z on 5 January 2017). This synoptic
situation resulted in the advection of very cold arctic air masses towards
eastern, central and southern Europe and favoured the formation of
tropopause folds along the path of the jet stream. In its later stage (00:00 Z on 8 January 2017 and after), the southernmost part of the system detached from the
main stream, forming a cut-off low over the Balkans. The IFS temperatures at
850 hPa, averaged from 00:00 Z on 7 January to 21:00 Z on 10 January 2017, were below
<inline-formula><mml:math id="M19" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">14</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M20" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C in most of the Balkans, reaching values below <inline-formula><mml:math id="M21" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">18</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M22" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C in
the western Balkans (not shown). To stress the exceptional intensity of the cold
intrusion, it is noted that the monthly mean climatological temperatures for
January at 850 hPa, derived from ERA-Interim reanalyses for the 1981–2010
period, are not lower than <inline-formula><mml:math id="M23" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">4</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M24" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C in the Balkan region (not shown).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1" specific-use="star"><caption><p id="d1e812">IFS geopotential height (in gpm; contours), wind speed (in <inline-formula><mml:math id="M25" display="inline"><mml:mrow><mml:mi mathvariant="normal">m</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">s</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>;
colour shaded) and wind direction (vectors) at 300 hPa, during the
period from 12:00 Z on 3 January 2017 to 00:00 Z on 9 January 2017 (12 h interval). Also
shown are the locations of the observational sites (blue text) used
in the study.</p></caption>
          <?xmltex \igopts{width=483.69685pt}?><graphic xlink:href="https://acp.copernicus.org/articles/18/15515/2018/acp-18-15515-2018-f01.jpg"/>

        </fig>

      <p id="d1e838">The horizontal thermal advection at 850 hPa was calculated at 3 h
intervals, using the IFS data and employing second-order centred finite
differences for the estimation of the horizontal derivatives. Cold advection
at 850 hPa<?pagebreak page15519?> occurred in large parts of central, eastern and southern Europe
in early January. Strong negative values of the horizontal thermal advection
(<inline-formula><mml:math id="M26" display="inline"><mml:mrow><mml:mo>&lt;</mml:mo><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1.5</mml:mn></mml:mrow></mml:math></inline-formula> K hr<inline-formula><mml:math id="M27" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>) were exhibited continuously in large parts of Italy
(5–7 January), the northern Balkans and central Europe (4–9 January), the western
Balkans along the Adriatic coast (5–11 January) and northern Greece,
southern FYROM (former Yugoslav Republic of Macedonia) and southwest Bulgaria
(6–9 January). The latter maximum in cold advection resulted in a record
period of 7 (5) consecutive days with frost (maximum daily temperature below
0 <inline-formula><mml:math id="M28" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C) from 6 to 12 (7 to 11) January at Thessaloniki (northern
Greece), which is located a few metres above sea level.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2" specific-use="star"><caption><p id="d1e877">Meteosat water vapour (5.35–7.15 <inline-formula><mml:math id="M29" display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>m) satellite images <bold>(a, b)</bold>, IFS
specific humidity (in <inline-formula><mml:math id="M30" display="inline"><mml:mrow><mml:mi mathvariant="normal">g</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">kg</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>; colour shaded) and PV (1.5 pvu; contours)
at 500 hPa <bold>(c, d)</bold>, and IFS ozone mixing ratio (in ppb; colour shaded)
at 500 hPa <bold>(e, f)</bold> at 12:00 Z on 6 January 2017 and 12:00 Z on 7 January 2017 respectively.
Also shown are the locations of the observational sites (red and blue text)
used in the study. Satellite images source: NERC Satellite Receiving Station,
Dundee University, Scotland; <uri>http://www.sat.dundee.ac.uk/</uri> (last access: 17 March 2017).</p></caption>
          <?xmltex \igopts{width=483.69685pt}?><graphic xlink:href="https://acp.copernicus.org/articles/18/15515/2018/acp-18-15515-2018-f02.jpg"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3" specific-use="star"><caption><p id="d1e925">IFS ozone mixing ratio (in ppb; colour shaded), geopotential height
(in gpm, black contours) and PV (1.5 pvu; blue contours) at 500 hPa during the period from 12:00 Z on 4 January 2017 to 12:00 Z on 8 January 2017 (12 h
interval). Also shown are the locations of the observational sites
(red text) used in the study.</p></caption>
          <?xmltex \igopts{width=483.69685pt}?><graphic xlink:href="https://acp.copernicus.org/articles/18/15515/2018/acp-18-15515-2018-f03.jpg"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4" specific-use="star"><caption><p id="d1e936">RegEns ozone mixing ratio (in ppb; colour shaded) at 5000 m during
the period from 12:00 Z on 4 January 2017 to 12:00 Z on 8 January 2017 (12 h interval).
Also shown are the locations of the observational sites (blue text)
used in the study. </p></caption>
          <?xmltex \igopts{width=483.69685pt}?><graphic xlink:href="https://acp.copernicus.org/articles/18/15515/2018/acp-18-15515-2018-f04.jpg"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F5" specific-use="star"><caption><p id="d1e947"><bold>(a)</bold> Norderney, Germany location. <bold>(b)</bold> Skew-T log-P diagrams at 12:00 Z on 3 January 2017
and <bold>(c)</bold> 12:00 Z on 4 January 2017. <bold>(d)</bold> Vertical profiles of IFS (blue) and RegEns (red)
ozone mixing ratio (ppb) at 12:00 Z on 3 January 2017 (solid line) and 12:00 Z on 4 January 2017
(dashed line). The red bars denote the standard deviation among the regional
ensemble members. Also shown are sonde (dashed black line) and IFS relative
humidity (dashed cyan line) at 12:00 Z on 4 January 2017. <bold>(e)</bold> Longitude–pressure vertical
cross section at 53.6<inline-formula><mml:math id="M31" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N of IFS ozone mixing ratio (in ppb; colour shaded),
wind speed (in <inline-formula><mml:math id="M32" display="inline"><mml:mrow><mml:mi mathvariant="normal">m</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">s</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>; black contours) and PV (2 pvu; blue contours)
at 12:00 Z on 4 January 2017. <bold>(f)</bold> IFS ozone (blue) and specific humidity (orange) time
series at 400 hPa.</p></caption>
          <?xmltex \igopts{width=369.885827pt}?><graphic xlink:href="https://acp.copernicus.org/articles/18/15515/2018/acp-18-15515-2018-f05.jpg"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F6" specific-use="star"><caption><p id="d1e1003"><bold>(a)</bold> Muenchen, Germany location. <bold>(b)</bold> Skew-T log-P diagrams at 00:00 Z on 4 January 2017
and <bold>(c)</bold> 12:00 Z on 5 January 2017. <bold>(d)</bold> Vertical profiles of IFS (blue) and RegEns (red)
ozone mixing ratio (ppb) at 00:00 Z on 4 January 2017 (solid line) and 12:00 Z on 5 January 2017
(dashed line). The red bars denote the standard deviation among the regional
ensemble members. Also shown are sonde (dashed black line) and IFS relative
humidity (dashed cyan line) at 12:00 Z on 5 January 2017. <bold>(e)</bold> Longitude–pressure vertical
cross section at 48.4<inline-formula><mml:math id="M33" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N of IFS ozone mixing ratio (in ppb; colour shaded),
wind speed (in <inline-formula><mml:math id="M34" display="inline"><mml:mrow><mml:mi mathvariant="normal">m</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">s</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>; black contours) and PV (2 pvu; blue contours)
at 12:00 Z on 5 January 2017. <bold>(f)</bold> IFS ozone (blue) and specific humidity (orange) time
series at 400 hPa.</p></caption>
          <?xmltex \igopts{width=369.885827pt}?><graphic xlink:href="https://acp.copernicus.org/articles/18/15515/2018/acp-18-15515-2018-f06.jpg"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F7" specific-use="star"><caption><p id="d1e1058"><bold>(a)</bold> Trapani, Italy location. <bold>(b)</bold> Skew-T log-P diagrams at 00:00 Z on 5 January 2017
and <bold>(c)</bold> 00:00 Z on 6 January 2017. <bold>(d)</bold> Vertical profiles of IFS (blue) and RegEns (red)
ozone mixing ratio (ppb) at 00:00 Z on 5 January 2017 (solid line) and 00:00 Z on 6 January 2017
(dashed line). The red bars denote the standard deviation among the regional
ensemble members. Also shown are sonde (dashed black line) and IFS relative
humidity (dashed cyan line) at 00:00 Z on 6 January 2017. <bold>(e)</bold> Longitude–pressure vertical
cross section at 38<inline-formula><mml:math id="M35" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N of IFS ozone mixing ratio (in ppb; colour shaded),
wind speed (in <inline-formula><mml:math id="M36" display="inline"><mml:mrow><mml:mi mathvariant="normal">m</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">s</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>; black contours) and PV (2 pvu; blue contours)
at 00:00 Z on 6 January 2017. <bold>(f)</bold> IFS ozone (blue) and specific humidity (orange) time
series at 400 hPa.</p></caption>
          <?xmltex \igopts{width=369.885827pt}?><graphic xlink:href="https://acp.copernicus.org/articles/18/15515/2018/acp-18-15515-2018-f07.jpg"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F8"><caption><p id="d1e1113"><bold>(a)</bold> Three-dimensional (longitude, latitude, pressure (hPa))
spatial distribution of IFS ozone concentrations exceeding 80 ppb at 00:00 Z
on 6 January 2017. <bold>(b)</bold> Three-dimensional (longitude, latitude, pressure
(hPa)) IFS ozone concentrations' isosurface of 100 ppb at 00:00 Z on 6 January 2017.</p></caption>
          <?xmltex \igopts{width=227.622047pt}?><graphic xlink:href="https://acp.copernicus.org/articles/18/15515/2018/acp-18-15515-2018-f08.jpg"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F9" specific-use="star"><caption><p id="d1e1129"><bold>(a)</bold> Heraklion, Greece location. <bold>(b)</bold> Skew-T log-P diagrams at 12:00 Z on 5 January 2017
and <bold>(c)</bold> 00:00 Z on 8 January 2017. <bold>(d)</bold> Vertical profiles of IFS (blue) and RegEns (red)
ozone mixing ratio (ppb) at 12:00 Z on 5 January 2017 (solid line) and 00:00 Z on 8 January 2017
(dashed line). The red bars denote the standard deviation among the regional
ensemble members. Also shown are sonde (dashed black line) and IFS relative
humidity (dashed cyan line) at 00:00 Z on 8 January 2017. <bold>(e)</bold> Latitude–pressure vertical
cross section at 25.2<inline-formula><mml:math id="M37" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E of IFS ozone mixing ratio (in ppb; colour shaded),
wind speed (in <inline-formula><mml:math id="M38" display="inline"><mml:mrow><mml:mi mathvariant="normal">m</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">s</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>; black contours) and PV (2 pvu; blue contours)
at 00:00 Z on 8 January 2017. <bold>(f)</bold> IFS ozone (blue) and specific humidity (orange) time
series at 400 hPa.</p></caption>
          <?xmltex \igopts{width=369.885827pt}?><graphic xlink:href="https://acp.copernicus.org/articles/18/15515/2018/acp-18-15515-2018-f09.jpg"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F10" specific-use="star"><caption><p id="d1e1185">Vertical profiles of ozone mixing ratio (ppb) over Prague, Czech Republic
(14.44<inline-formula><mml:math id="M39" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E, 50<inline-formula><mml:math id="M40" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N), for ozonesondes (black line), IFS forecast day 1 (dark blue line),
IFS forecast day 2 (coral line), IFS forecast day 3 (green line), IFS forecast day 4 (light blue line),
IFS forecast day 5 (orange line), IFS no DA (without data assimilation) forecast day 1 (grey line) and
RegEns (red line) at <bold>(a)</bold> 11:00 Z on 2 January 2017 and <bold>(b)</bold> 11:00 Z on 4 January 2017. Also shown are sonde (black dashed line)
and IFS forecast day 1 relative humidity (cyan dashed line). The red bars denote the standard
deviation among the regional ensemble members. The numbers on the right of the diagrams show the FGE values
of IFS ozone (with the corresponding colour) at 300–500 hPa.
</p></caption>
          <?xmltex \igopts{width=312.980315pt}?><graphic xlink:href="https://acp.copernicus.org/articles/18/15515/2018/acp-18-15515-2018-f10.jpg"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F11"><caption><p id="d1e1220">Profiles of ozone mixing ratio (ppb) over the broader area of Frankfurt
(8.5<inline-formula><mml:math id="M41" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E, 50<inline-formula><mml:math id="M42" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N) for IAGOS (black line), IFS forecast day 1 (dark blue line),
IFS forecast day 2 (coral line), IFS forecast day 3 (green line), IFS forecast day 4 (light
blue line), IFS forecast day 5 (orange line), IFS no DA (without data assimilation) forecast
day 1 (grey line) and RegEns (red line) during <bold>(a)</bold> 13:00 Z on 4 January 2017, <bold>(b)</bold> 06:00 Z
on 5 January 2017, and <bold>(c)</bold> 13:00 Z on 5 January 2017. The red bars denote the standard deviation among the regional ensemble members.
The numbers above the diagrams show the FGE values of IFS ozone (with the corresponding colour)
at 300–500 hPa <bold>(a,  b)</bold> and 400–600 hPa <bold>(c)</bold>.</p></caption>
          <?xmltex \igopts{width=216.240945pt}?><graphic xlink:href="https://acp.copernicus.org/articles/18/15515/2018/acp-18-15515-2018-f11.jpg"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F12"><caption><p id="d1e1265">FGE values of IFS ozone for forecast days 1–5 over Prague (11:00 Z on 4 January 2017) and Frankfurt
(13:00 Z on 4 January 2017, 06:00 Z on 5 January 2017 and 13:00 Z on 5 January 2017). The dashed coloured horizontal lines
represent the FGE values of IFS no DA ozone for forecast day 1.</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://acp.copernicus.org/articles/18/15515/2018/acp-18-15515-2018-f12.png"/>

        </fig>

      <p id="d1e1274">To further explore the meteorological conditions and to investigate the case
of stratospheric intrusions into the troposphere during the examined period,
several stratospheric tracers are analysed from both IFS and observations.
The water vapour satellite images at 12:00 Z on 6 and 7 January 2017, presented
in Fig. <xref ref-type="fig" rid="Ch1.F2"/>a and b, respectively, display a “hook-shaped”
streamer of dry air (dark shades) extending from north-eastern Europe to the
central Mediterranean. This is a typical pattern encountered during STT
events <xref ref-type="bibr" rid="bib1.bibx88 bib1.bibx36 bib1.bibx2" id="paren.43"/>.
The<?pagebreak page15520?> fields of IFS specific humidity at 500 hPa on the same days
(Fig. <xref ref-type="fig" rid="Ch1.F2"/>c and d) resemble the observed satellite images. These
depict a hook-shaped region of air with low specific humidity, affirming that
the presence of dry air in the troposphere is captured well by the IFS
global model. The respective PV isosurfaces of 1.5 pvu
(Fig. <xref ref-type="fig" rid="Ch1.F2"/>c and d) overlap the band of dry air in the
troposphere, while high ozone concentrations, up to 130 ppb, are also found
over this dry streamer (Fig. <xref ref-type="fig" rid="Ch1.F2"/>e and f). Altogether,
Fig. <xref ref-type="fig" rid="Ch1.F2"/> indicates that this dry air with relatively high PV
values and high ozone concentrations is of stratospheric origin.</p>
</sec>
<sec id="Ch1.S3.SS2">
  <title>Tropospheric ozone distribution in CAMS models</title>
      <p id="d1e1297">Figure <xref ref-type="fig" rid="Ch1.F3"/> presents the evolution (12 h
interval) of ozone concentrations exceeding 50 ppb, geopotential height and
PV isosurfaces of 1.5 pvu from IFS at 500 hPa for the time period 4–8 January 2017, to examine ozone enhanced in the middle troposphere owing to
STT in relation to the predominant synoptic–dynamic conditions. At 12:00 Z on 4 January 2017<?pagebreak page15521?> a streamer of high ozone concentrations with values up to about
100 ppb is found over the Baltic Sea and northern Germany, near the ridge exit
and trough entrance, where convergence and descending motions prevail, and in
the vicinity of the jet stream (Fig. <xref ref-type="fig" rid="Ch1.F1"/>). During the next 24 h as the system moves further south, the streamer of high ozone
concentrations crosses central Europe following the path of the jet stream.
At 00:00 Z and 12:00 Z on 6 January 2017 ozone concentrations exceeding 130 ppb, linked
with high PV values (<inline-formula><mml:math id="M43" display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">1.5</mml:mn></mml:mrow></mml:math></inline-formula> pvu), are found over the central Mediterranean,
highlighting the vertical transport of ozone from the stratosphere down to
the middle troposphere. During the next 48 h, the high ozone streamer
moves further eastward, affecting the island of Crete (7 and 8 January 2017),
and gradually dissipates.</p>
      <p id="d1e1314">In order to explore the capability of the regional models to reproduce the
enhanced ozone seen in the mid-troposphere due to STT, the fields of RegEns
ozone exceeding 50 ppb at 5000 m are shown in Fig. <xref ref-type="fig" rid="Ch1.F4"/> for
the same dates as in Fig. <xref ref-type="fig" rid="Ch1.F3"/>. Visual inspection of
Fig. <xref ref-type="fig" rid="Ch1.F4"/> indicates that the RegEns compares well with IFS as
it synchronously captures the spatial distribution of ozone concentrations.
In more detail, the hook-shaped patterns of high ozone are seen well in the
CAMS regional product, with ozone mixing ratios exceeding 90 ppb at 12:00 Z on 6 January 2017 over the central Mediterranean. Although the spatio-temporal
features of ozone in the RegEns agree well with that of the IFS, in
quantitative terms, there are discrepancies between the regional and the
global product. This is likely due to the fact that (a) the RegEns is
presented at a 5000 m level (the uppermost level available) and the IFS at 500 hPa, (b) different resolution and advection schemes are used in global and
regional models and (c) pressure and temperature values from the US Standard
Atmosphere <xref ref-type="bibr" rid="bib1.bibx82" id="paren.44"/> were used for units' conversion in RegEns.
Considering the ERA-Interim <xref ref-type="bibr" rid="bib1.bibx25" id="paren.45"/> temperatures during the period
of interest for the units conversion may result in even lower RegEns ozone
concentrations of up to <inline-formula><mml:math id="M44" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">7</mml:mn></mml:mrow></mml:math></inline-formula> % in the regions exhibiting the lower
temperatures (not shown). Overall, the agreement between the CAMS global and
regional products highlights the critical role that the IFS boundary
conditions and meteorological<?pagebreak page15522?> drivers play in the regional models for
forecasting an STT event and the induced downward transport of ozone.</p>
</sec>
<sec id="Ch1.S3.SS3">
  <title>Vertical structure and analysis of STT event</title>
      <p id="d1e1346">Four sites are selected (Norderney, Germany; Muenchen,
Germany; Trapani, Italy; Heraklion, Greece), located within the system
transit path with available radiosonde observations, in order to study the
vertical structure of the STT event and the subsequent transport of
stratospheric ozone into the troposphere. To better depict the impact of STT
on tropospheric ozone, two dates for analysis are selected for each site: one
prior and one during the STT occurrence.</p>
      <p id="d1e1349">Starting from Norderney (see location in Fig. <xref ref-type="fig" rid="Ch1.F5"/>a), the skew-T log-P diagrams for 12:00 Z on 3 January 2017 and 12:00 Z on 4 January 2017 are
presented in Fig. <xref ref-type="fig" rid="Ch1.F5"/>b and c, respectively. As can be seen from
the comparison between the two figures, a distinct decrease of humidity
(departure of dew-point curve (left) and temperature curve (right)) is found
at 12:00 Z on 4 January 2017 between 250 and 400 hPa, while the tropopause drops
to approximately 400 hPa. Furthermore, the vertical profile of the IFS ozone
mixing ratio over Norderney during the examined dates
(Fig. <xref ref-type="fig" rid="Ch1.F5"/>d) indicates a remarkable increase of ozone down to
400 hPa, verifying the aforementioned observed folding of the tropopause.
The vertical profiles of the observed and IFS relative humidity
(Fig. <xref ref-type="fig" rid="Ch1.F5"/>d) show a sharp decrease at 400 hPa, revealing that
the intrusion of dry stratospheric air in the troposphere is captured well by
the IFS. A comprehensive view of the induced stratospheric intrusion over
Norderney is provided through the longitude–pressure cross section at
53.6<inline-formula><mml:math id="M45" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, showing ozone, PV (2 pvu isosurface) and wind speed at
12:00 Z on 4 January 2017 (Fig. <xref ref-type="fig" rid="Ch1.F5"/>e). An impressive downward
penetration of ozone-rich and PV-rich (<inline-formula><mml:math id="M46" display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> pvu) air down to approximately
600 hPa is found in the free troposphere and over the greater Norderney
longitude band. The 2 pvu PV isosurface (dynamical tropopause; e.g.
<xref ref-type="bibr" rid="bib1.bibx40" id="altparen.46"/>) illustrates the tropopause folding on the right side
of the jet stream (black contours) and down to 450 hPa at 5<inline-formula><mml:math id="M47" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E. The
stratospheric origin of ozone in the upper troposphere over Norderney is also
supported by the IFS ozone and specific humidity time series at 400 hPa,
revealing a significant anti-correlation at the 95 % confidence level
(Fig. <xref ref-type="fig" rid="Ch1.F5"/>f). The respective diagrams for Muenchen are presented
in Fig. <xref ref-type="fig" rid="Ch1.F6"/> for 00:00 Z on 4 January 2017 and 12:00 Z on 5 January 2017.
Similarly, an intrusion of dry air is observed in the upper and middle
troposphere (down to 550 hPa) at 12:00 Z on 5 January 2017
(Fig. <xref ref-type="fig" rid="Ch1.F6"/>b and c), which, along with the sharp increase/decrease
of IFS ozone/relative humidity above 550 hPa (Fig. <xref ref-type="fig" rid="Ch1.F6"/>d), partially seen in RegEns ozone vertical profiles, indicates the
downward transport of dry stratospheric air into the troposphere. The
longitude–pressure cross section over Muenchen at 12:00 Z on 5 January 2017
(Fig. <xref ref-type="fig" rid="Ch1.F6"/>e) depicts the folding of the tropopause (2 pvu
isosurface) in the vicinity of the jet stream and the associated vertical
transport of ozone-rich air down to 600 hPa. In support of the above, the
distinct<?pagebreak page15524?> increase of IFS ozone at 400 hPa is combined with a sharp decrease
of IFS specific humidity (significant anti-correlation at the 95 %
confidence level) (Fig. <xref ref-type="fig" rid="Ch1.F6"/>f).</p>
      <p id="d1e1407">A period of 12 h later (00:00 Z on 6 January 2017), and as the system moved further
south, a dramatic decrease of humidity is observed in the middle troposphere
and down to approximately 550 hPa over Trapani (Fig. <xref ref-type="fig" rid="Ch1.F7"/>b and
c), with specific and relative humidity at 500 hPa dropping from
0.75 <inline-formula><mml:math id="M48" display="inline"><mml:mrow><mml:mi mathvariant="normal">g</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">kg</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> and 58 % (00:00 Z on 5 January) to
0.01 <inline-formula><mml:math id="M49" display="inline"><mml:mrow><mml:mi mathvariant="normal">g</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">kg</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> and 2 % (00:00 Z on 6 January 2017) respectively. The
IFS specific humidity values at 500 hPa for the same dates are
0.49 and 0.025 <inline-formula><mml:math id="M50" display="inline"><mml:mrow><mml:mi mathvariant="normal">g</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">kg</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>, respectively. On top of
that, the vertical profiles of the observed and IFS relative humidity
(Fig. <xref ref-type="fig" rid="Ch1.F7"/>d) indicate that the sharp decrease of humidity is reproduced
well by the CAMS global model. The IFS system captures the
dynamical features of the stratospheric intrusion as it is depicted in the
vertical profiles of ozone, showing increased concentrations at 00:00 Z on 6 January 2017 down to 600 hPa, which is also seen in CAMS RegEns
(Fig. <xref ref-type="fig" rid="Ch1.F7"/>d). The intense tropopause folding over Trapani is
illustrated in Fig. <xref ref-type="fig" rid="Ch1.F7"/>e, with the dynamical tropopause dropping
down to 550 hPa and ozone-rich air penetrating down to 800 hPa. Again, a
significant anti-correlation at the 95 % confidence level is found
between the IFS ozone and specific<?pagebreak page15526?> humidity time series at 400 hPa,
indicating that the ozone increase results from the downward transport of
ozone from the stratosphere (Fig. <xref ref-type="fig" rid="Ch1.F7"/>f). The three-dimensional
field of IFS ozone concentrations exceeding 80 ppb at 00:00 Z on 6 January 2017
is presented in Fig. <xref ref-type="fig" rid="Ch1.F8"/>a, depicting the stratospheric ozone
intrusion into the troposphere and over the broader Trapani region. The
three-dimensional IFS ozone concentration isosurface of 100 ppb
(Fig. <xref ref-type="fig" rid="Ch1.F8"/>b) resembles the folding of the tropopause along a
north-east-oriented conceivable axis, which coincides with the high wind speed
flow in the upper troposphere (Fig. <xref ref-type="fig" rid="Ch1.F1"/>). Later on and over
Heraklion (see location in Fig. <xref ref-type="fig" rid="Ch1.F9"/>a), the skew-T log-P
diagrams for 12:00 Z on 5 January 2017 and 00:00 Z on 8 January 2017
(Fig. <xref ref-type="fig" rid="Ch1.F9"/>b and c) and the respective vertical profiles of IFS
ozone and relative humidity (Fig. <xref ref-type="fig" rid="Ch1.F9"/>d) reveal the presence of
dry ozone-rich air in the upper and middle troposphere (down to 500 hPa).
The increase in IFS ozone time series at 400 hPa is synchronized with the
decrease of IFS specific humidity (significant anti-correlation at the
95 % confidence level), indicating that dry stratospheric air rich in
ozone is transported into the troposphere over Heraklion
(Fig. <xref ref-type="fig" rid="Ch1.F9"/>f). A more illustrative representation of the
development and evolution of the examined STT event is provided in the
three-dimensional animation (from 12:00 Z on 3 January 2017 to 21:00 Z on 8 January 2017 with 3 h interval) of IFS ozone concentrations exceeding
80 ppb in the Supplement.</p>
</sec>
<sec id="Ch1.S3.SS4">
  <title>Comparison with profile observations</title>
      <p id="d1e1493">In order to evaluate the forecasting capability of both
IFS and RegEns regarding the downward transport of ozone during the examined
STT event, we compare CAMS forecasts with profile observations from
ozonesondes (WOUDC) and aircraft measurements (IAGOS). Two sites located
across the passage of the examined system with available observational data
during the examined period were selected: (a) Prague (ozonesondes) and
(b) Frankfurt (aircraft measurements). The model error is quantified using
the fractional gross error (FGE), which ranges between 0 and 2 and behaves
symmetrically with respect to under- and overestimation:
            <disp-formula id="Ch1.E1" content-type="numbered"><mml:math id="M51" display="block"><mml:mrow><mml:mi mathvariant="normal">FGE</mml:mi><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mn mathvariant="normal">2</mml:mn><mml:mi>N</mml:mi></mml:mfrac></mml:mstyle><mml:munderover><mml:mo movablelimits="false">∑</mml:mo><mml:mi>i</mml:mi><mml:mi>N</mml:mi></mml:munderover><mml:mfenced close="|" open="|"><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi>O</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi>O</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:mfrac></mml:mstyle></mml:mfenced><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
          where <inline-formula><mml:math id="M52" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> represents the model value for level <inline-formula><mml:math id="M53" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math id="M54" display="inline"><mml:mrow><mml:msub><mml:mi>O</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the corresponding observed value and <inline-formula><mml:math id="M55" display="inline"><mml:mi>N</mml:mi></mml:math></inline-formula> is the
number of sample values.</p>
      <p id="d1e1586">Figure <xref ref-type="fig" rid="Ch1.F10"/> displays the vertical profiles of observed and forecasted (IFS and RegEns) ozone
concentrations over Prague at 11:00 Z (12:00 Z for CAMS models) on 2 January 2017 (prior the STT event) and 11:00 Z (12:00 Z
for CAMS models) on 4 January 2017 (during the STT event). The intercomparison between the observed vertical
profiles of ozone on the two dates indicates a distinct increase of ozone concentrations in the upper
troposphere, probably related to the vertical transport of ozone from the stratosphere, reaching down to approximately 500 hPa.
In support of the above findings, the respective vertical profiles of the observed and IFS relative humidity both
show a distinct decrease at 500 hPa. Although the CAMS global model seems to underestimate (overestimate)
ozone in (above) the free troposphere, the transition from the neutral condition to the STT event is
captured well by the IFS day 1 forecast (Fig. <xref ref-type="fig" rid="Ch1.F10"/>), with an FGE value of 0.13 (300–500 hPa) on 4 January 2017.
Whilst data assimilation resulted in overestimating ozone near the tropopause compared with the control
run (Fig. <xref ref-type="fig" rid="Ch1.F10"/>a), it is clearly beneficial in reproducing the increase of ozone in the upper
troposphere during the STT event (Fig. <xref ref-type="fig" rid="Ch1.F10"/>b). Notably, the respective FGE value for the
control run at 4 January 2017 is 0.29, revealing an improvement in model performance due to data
assimilation. Ozone in the RegEns forecast is higher within the planetary boundary layer than<?pagebreak page15527?> in
IFS, with a relatively small spread among the RegEns members (Fig. <xref ref-type="fig" rid="Ch1.F10"/>a). In the
free troposphere, the range of regional variability increases; however the RegEns remains close to the
global forecast. The RegEns is also able to reproduce the ozone enhancement, following the IFS forecast closely
(Fig. <xref ref-type="fig" rid="Ch1.F10"/>b). Day 1 to day 5 forecasts of IFS ozone indicate that the observed ozone increase in
upper troposphere during the STT event is satisfactorily forecasted up to 3 days in advance, with FGE values
not higher than 0.22 (Fig. <xref ref-type="fig" rid="Ch1.F10"/>b).</p>
      <p id="d1e1604">Three ozone profiles from aircraft measurements (two take-offs and one landing) over the broader region of Frankfurt
at 13:00 Z on 4 January 2017, 6:00 Z on 5 January 2017 and 13:00 Z on 5 January 2017 are compared with the respective IFS and RegEns
ozone profiles in Fig. <xref ref-type="fig" rid="Ch1.F11"/>. At 13:00 Z (12:00 Z for CAMS models) on 4 January 2017, the profile of the IFS ozone
day 1 forecast is found to be in very good agreement with the IAGOS data, both depicting the increase of ozone down
to approximately 500 hPa (Fig. <xref ref-type="fig" rid="Ch1.F11"/>a). The FGE was 0.04 for the 300–500 hPa altitude range. The
respective profiles 17 h later (06:00 Z on 5 January 2017) also reveal enhanced ozone concentrations in the upper
troposphere, which are captured by the IFS day 1 forecast (Fig. <xref ref-type="fig" rid="Ch1.F11"/>b) (FGE <inline-formula><mml:math id="M56" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 0.19 at 300–500 hPa). Finally,
at 13:00 Z (12:00 Z for CAMS models) on 5 January 2017, the IFS<?pagebreak page15529?> day 1 forecast is found to overestimate the observed high
ozone concentrations between 250 and 350 hPa, while it qualitatively captures the observed high ozone pattern
in the middle troposphere between 400 and 600 hPa (Fig. <xref ref-type="fig" rid="Ch1.F11"/>c) (FGE <inline-formula><mml:math id="M57" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 0.30 at 400–600 hPa). The
advantageous role of data assimilation can be affirmed from the intercomparison with the IFS control run, which
exhibits FGE values of 0.34, 0.30 and 0.12 for the three dates respectively. A better agreement with observations
is found for IFS when implementing data assimilation at 13:00 Z on 4 January 2017 and 06:00 Z on 5 January 2017
(Fig. <xref ref-type="fig" rid="Ch1.F11"/>a and b), while at 13:00 Z on 5 January 2017 (Fig. <xref ref-type="fig" rid="Ch1.F11"/>c), although the control run
performs better in terms of bias, the data assimilation seems to help in the direction of reproducing the observed
ozone peak in the middle troposphere. Concerning the RegEns, due to its limited vertical profile, up to about 550 hPa,
the evaluation of its forecast performance is restricted. Nevertheless, there is a clear signal of increased ozone in
the uppermost vertical level during all three dates. Regarding the forecast performance of CAMS global model, a relatively
good agreement with observations is seen up to forecast day 3 at 13:00 Z on 4 January 2017 and 06:00 Z on 5 January 2017 (FGE values
not higher than 0.25) (Fig. <xref ref-type="fig" rid="Ch1.F11"/>a and b), while at 13:00 Z on 5 January 2017 the observed ozone peak in the middle
troposphere is somehow captured up to forecast day 3 but overestimated. Figure <xref ref-type="fig" rid="Ch1.F12"/> depicts the FGE values
of IFS ozone in relation to the forecast day for the observational instances of Prague and Frankfurt. Overall, a
satisfactory forecast performance is revealed up to 3 days in advance with FGE values not higher than 0.3.
Forecast day 1 exhibits the best agreement with observations, while after forecast day 3, more discrepancies are found
between the forecast and the observations (see also Figs. <xref ref-type="fig" rid="Ch1.F10"/> and <xref ref-type="fig" rid="Ch1.F11"/>).</p>
</sec>
</sec>
<?pagebreak page15530?><sec id="Ch1.S4" sec-type="conclusions">
  <title>Conclusions</title>
      <p id="d1e1650">We examined a deep STT event over Europe during the time period from 4 to 9 January 2017 in the CAMS global
and regional forecast systems, assessing their capability to reproduce several key meteorological and chemical
features of the event, with the aid of radiosonde, ozonesonde and aircraft observational data. The main results
of the current study can be summarized as follows:</p>
      <p id="d1e1653"><list list-type="bullet">
          <list-item>

      <p id="d1e1658">A deep upper level trough extending over central Europe favoured the development of tropopause
folds and subsequently STT events along the jet stream axis at the west flank of the trough between 4 and 9 January 2017.</p>
          </list-item>
          <list-item>

      <p id="d1e1664">The hook-shaped streamer of dry stratospheric air in the middle troposphere seen in water
vapour satellite images is reproduced well by the CAMS forecast systems, with tongues of anomalously high ozone
concentrations in both CAMS global and regional models.</p>
          </list-item>
          <list-item>

      <p id="d1e1670">The observed (radiosondes) folding of the tropopause over various European sites is accurately
reproduced by the CAMS global model. The vertical profiles and cross sections of IFS ozone and PV indicate that
the vertical extent of the observed tropopause drop is well captured at all four of the sites studies.</p>
          </list-item>
          <list-item>

      <p id="d1e1676">The CAMS global system is found to be capable of capturing the evolution and vertical
characteristics of the observed ozone field over Prague during the STT event. The observed ozone increase in the
upper troposphere due to the stratospheric ozone downward transport is relatively well captured by the IFS. In
addition, the global CAMS ozone forecasts in the greater Frankfurt area reveal an enhancement of ozone concentrations
in the upper and middle troposphere as a result of the STT, which is in good agreement with the ozone measured by
the IAGOS aircraft.</p>
          </list-item>
          <list-item>

      <p id="d1e1682">The evaluation of IFS ozone forecasts indicates that the CAMS global system is capable of forecasting
the enhanced ozone concentrations during the STT event over Prague and Frankfurt up to 3 days in advance, both
qualitatively and quantitatively.</p>
          </list-item>
          <list-item>

      <p id="d1e1689">Figures <xref ref-type="fig" rid="Ch1.F10"/>, <xref ref-type="fig" rid="Ch1.F11"/> and <xref ref-type="fig" rid="Ch1.F12"/> show that
the use of data assimilation in the IFS is generally beneficial in forecasting the vertical and temporal variability
of ozone during the examined STT event. Nevertheless, there are still discrepancies from the observations near the
tropopause region as the sharp gradients around the tropopause are difficult to capture in global models
<xref ref-type="bibr" rid="bib1.bibx16 bib1.bibx35" id="paren.47"/>.</p>
          </list-item>
          <list-item>

      <p id="d1e1704">Despite the limited vertical profile of RegEns forecast data, the CAMS regional models show
an increase of ozone in the uppermost level for all instances in which the STT reached or exceeded that level.</p>
          </list-item>
        </list></p>
      <p id="d1e1709">Overall, this process-oriented analysis and evaluation study indicates that the CAMS global and regional
forecast modelling systems are able to capture the specific regional meteorological and air quality characteristics
of a specific deep STT event over Europe in January 2017. It also highlights the importance of data assimilation
in the CAMS global model as well as of the meteorological and chemical forcing in the CAMS regional forecast systems.</p>
</sec>

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

      <p id="d1e1717">The CAMS global and regional forecast data were
processed within the framework of the service element CAMS_84. Both CAMS
global and regional forecast products can be obtained from
<uri>https://atmosphere.copernicus.eu/</uri> (last access: 19 October 2018). The
satellite images were obtained from the NERC Satellite Receiving Station,
Dundee University, Scotland, at <uri>http://www.sat.dundee.ac.uk/</uri> (last access:
17 March 2017). The radiosonde data were obtained from Wyoming
University, Department of Atmospheric Science, at <uri>http://weather.uwyo.edu/upperair/sounding.html</uri> (last access:
27 April 2018). The ozonesonde data were obtained from the World Ozone and
Ultraviolet Radiation Data Center (WOUDC) at <uri>https://woudc.org/</uri> (last
access: 9 June 2017). The IAGOS aircraft ozone measurements were provided by
Hannah Clark (Hannah.Clark@aero.obs-mip.fr) and will shortly be available in
the database at <uri>http://www.iagos.fr</uri> (last access: 19 October 2018) or
directly via the AERIS website at <uri>http://www.aeris-data.fr</uri> (last access:
19 October 2018).</p>
  </notes><app-group>
        <supplementary-material position="anchor"><p id="d1e1739">The supplement related to this article is available online at: <inline-supplementary-material xlink:href="https://doi.org/10.5194/acp-18-15515-2018-supplement" xlink:title="zip">https://doi.org/10.5194/acp-18-15515-2018-supplement</inline-supplementary-material>.</p></supplementary-material>
        </app-group><notes notes-type="authorcontribution">

      <p id="d1e1748">DA, EK and PZ designed the study. EK collected
the forecast data. DA performed the data analysis and wrote the paper. IP
contributed to the synoptic analysis. JF and AI contributed to the IFS
results' interpretation and JF performed the IFS control simulation without
the use of data assimilation. HC provided the IAGOS aircraft measurements. HE
is coordinating CAMS84 (global and regional a posteriori validation,
including focus on the Arctic and Mediterranean areas). MP is coordinating
CAMS50 (regional production). All authors contributed to interpretation of the
results and the writing of the paper.</p>
  </notes><notes notes-type="competinginterests">

      <p id="d1e1754">The authors declare that they have no conflict of
interest.</p>
  </notes><ack><title>Acknowledgements</title><p id="d1e1760">This work is performed within the framework of the service element “CAMS_84:
Global and regional a posteriori validation, including focus on the Arctic
and Mediterranean areas” of the Copernicus Atmospheric Monitoring Services
(CAMS). ECMWF is the operator of CAMS on behalf of the European Union
(Delegation Agreement signed on 11 November 2014). The<?pagebreak page15531?> CAMS_84 work is financially
supported by ECMWF via its main contractor, Royal Netherlands Meteorological
Institute KNMI. The authors acknowledge the strong support of the European
Commission, Airbus and the Airlines (Lufthansa, Air-France, Austrian, Air
Namibia, Cathay Pacific, Iberia, China Airlines, Hawaiian Airlines so far)
who have carried the MOZAIC or IAGOS equipment and performed the maintenance since
1994. In its last 10 years of operation, MOZAIC has been funded by INSU-CNRS
(France), Météo-France, Université Paul Sabatier (Toulouse, France) and
Research Center Jülich (FZJ, Jülich, Germany). IAGOS has been
additionally funded by the EU projects IAGOS-DS and IAGOS-ERI. The
MOZAIC-IAGOS database is supported by AERIS (CNES and INSU-CNRS). Data are
also available via the AERIS website at <uri>https://www.aeris-data.fr</uri> (last access: 19 October 2018). The authors
acknowledge the use of Copernicus Atmosphere Monitoring Service Information (2017). We also acknowledge the WOUDC, the Department of Atmospheric Science
of Wyoming University and the NERC Satellite Receiving Station of Dundee University for the free use of ozonesonde data, radiosonde data and
satellite images respectively. AUTH (Aristotle University of Thessaloniki)
authors acknowledge the support of the scientific computing services of the
AUTH-IT Center (<uri>http://it.auth.gr</uri>, last access: 19 October 2018). Finally, the authors would like to
acknowledge the free use of Python (<uri>https://www.python.org</uri>, last access: 19 October 2018), Ferret
(<uri>http://ferret.pmel.noaa.gov/Ferret/</uri>, last access: 19 October 2018) and Mayavi
<xref ref-type="bibr" rid="bib1.bibx67" id="paren.48"/> software for the analysis and graphics of the
paper.<?xmltex \hack{\newline}?><?xmltex \hack{\newline}?> Edited by: Geraint
Vaughan<?xmltex \hack{\newline}?>
Reviewed by: two anonymous referees</p></ack><ref-list>
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    <!--<article-title-html>A deep stratosphere-to-troposphere ozone transport event over Europe simulated in CAMS global and regional forecast systems: analysis and evaluation</article-title-html>
<abstract-html><p>Stratosphere-to-troposphere transport (STT) is an important natural source of
tropospheric ozone, which can occasionally influence ground-level ozone
concentrations relevant for air quality. Here, we analyse and evaluate the
Copernicus Atmosphere Monitoring Service (CAMS) global and regional forecast
systems during a deep STT event over Europe for the time period from 4 to 9 January 2017. The predominant synoptic condition is described by a deep upper
level trough over eastern and central Europe, favouring the formation of
tropopause folding events along the jet stream axis and therefore the
intrusion of stratospheric ozone into the troposphere. Both global and
regional CAMS forecast products reproduce the <q>hook-shaped</q> streamer of
ozone-rich and dry air in the middle troposphere depicted from the observed
satellite images of water vapour. The CAMS global model successfully
reproduces the folding of the tropopause at various European sites, such as
Trapani (Italy), where a deep folding down to 550&thinsp;hPa is seen. The
stratospheric ozone intrusions into the troposphere observed by WOUDC
ozonesonde and IAGOS aircraft measurements are satisfactorily forecasted up
to 3 days in advance by the CAMS global model in terms of both temporal and
vertical features of ozone. The fractional gross error (FGE) of CAMS ozone
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