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  <front>
    <journal-meta><journal-id journal-id-type="publisher">NHESS</journal-id><journal-title-group>
    <journal-title>Natural Hazards and Earth System Sciences</journal-title>
    <abbrev-journal-title abbrev-type="publisher">NHESS</abbrev-journal-title><abbrev-journal-title abbrev-type="nlm-ta">Nat. Hazards Earth Syst. Sci.</abbrev-journal-title>
  </journal-title-group><issn pub-type="epub">1684-9981</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/nhess-19-1839-2019</article-id><title-group><article-title>The impact of lightning and radar reflectivity factor data assimilation on the very short-term rainfall forecasts of RAMS@ISAC: application to two case studies in Italy</article-title><alt-title>The impact of lightning and radar reflectivity factor data assimilation</alt-title>
      </title-group><?xmltex \runningtitle{The impact of lightning and radar reflectivity factor data assimilation}?><?xmltex \runningauthor{S. Federico et al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes" rid="aff1">
          <name><surname>Federico</surname><given-names>Stefano</given-names></name>
          <email>s.federico@isac.cnr.it</email>
        <ext-link>https://orcid.org/0000-0001-7890-9394</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Torcasio</surname><given-names>Rosa Claudia</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-5461-9728</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Avolio</surname><given-names>Elenio</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-9692-6208</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3">
          <name><surname>Caumont</surname><given-names>Olivier</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-6470-2023</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Montopoli</surname><given-names>Mario</given-names></name>
          
        <ext-link>https://orcid.org/0000-0003-0099-0393</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Baldini</surname><given-names>Luca</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-5217-1205</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff4">
          <name><surname>Vulpiani</surname><given-names>Gianfranco</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-8008-8799</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Dietrich</surname><given-names>Stefano</given-names></name>
          
        <ext-link>https://orcid.org/0000-0003-3808-365X</ext-link></contrib>
        <aff id="aff1"><label>1</label><institution>ISAC-CNR, via del Fosso del Cavaliere 100, 00133 Rome, Italy</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>ISAC-CNR, zona Industriale comparto 15, 88046, Lamezia Terme, Italy</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>CNRM UMR 3589, University of Toulouse, Météo-France, CNRS, 42 avenue G. Coriolis, 31057 Toulouse, France</institution>
        </aff>
        <aff id="aff4"><label>4</label><institution>Dipartimento Protezione Civile Nazionale Ufficio III – Attività Tecnico Scientifiche per la Previsione e Prevenzione <?xmltex \hack{\break}?>dei Rischi, 00189, Rome, Italy</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Stefano Federico (s.federico@isac.cnr.it)</corresp></author-notes><pub-date><day>23</day><month>August</month><year>2019</year></pub-date>
      
      <volume>19</volume>
      <issue>8</issue>
      <fpage>1839</fpage><lpage>1864</lpage>
      <history>
        <date date-type="received"><day>4</day><month>November</month><year>2018</year></date>
           <date date-type="rev-request"><day>23</day><month>November</month><year>2018</year></date>
           <date date-type="rev-recd"><day>12</day><month>June</month><year>2019</year></date>
           <date date-type="accepted"><day>8</day><month>July</month><year>2019</year></date>
      </history>
      <permissions>
        <copyright-statement>Copyright: © 2019 </copyright-statement>
        <copyright-year>2019</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://nhess.copernicus.org/articles/.html">This article is available from https://nhess.copernicus.org/articles/.html</self-uri><self-uri xlink:href="https://nhess.copernicus.org/articles/.pdf">The full text article is available as a PDF file from https://nhess.copernicus.org/articles/.pdf</self-uri>
      <abstract><title>Abstract</title>
    <p id="d1e166">In this paper, we study the impact of lightning and radar reflectivity
factor data assimilation on the precipitation VSF (very short-term forecast,
3 h in this study) for two severe weather events that occurred in Italy.
The first case refers to a moderate and localized rainfall over central
Italy that occurred on 16 September 2017. The second case occurred on 9 and 10 September 2017 and was very intense and caused damages in several geographical areas, especially in Livorno (Tuscany) where nine people died.</p>
    <p id="d1e169">The first case study was missed by several operational forecasts, including
that performed by the model used in this paper, while the Livorno case was
partially predicted by operational models.</p>
    <p id="d1e172">We use the RAMS@ISAC model (Regional Atmospheric Modelling System at
Institute for Atmospheric Sciences and Climate of the Italian National
Research Council), whose 3D-Var extension to the assimilation of radar
reflectivity factor is shown in this paper for the first time.</p>
    <p id="d1e175">Results for the two cases show that the assimilation of lightning and radar
reflectivity factor, especially when used together, have a significant and
positive impact on the precipitation forecast. For specific time intervals,
the data assimilation is of practical importance for civil protection
purposes because it changes a missed forecast of intense precipitation (<inline-formula><mml:math id="M1" display="inline"><mml:mrow><mml:mo>≥</mml:mo><mml:mn mathvariant="normal">40</mml:mn></mml:mrow></mml:math></inline-formula> mm in 3 h) to a correct one.</p>
    <p id="d1e188">While there is an improvement of the rainfall VSF thanks to the lightning
and radar reflectivity factor data assimilation, its usefulness is partially
reduced by the increase in false alarms, especially when both datasets
are assimilated.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <label>1</label><title>Introduction</title>
      <p id="d1e200">Initial conditions of numerical weather prediction (NWP) models are a key
point for a good forecast (Stensrud and Fritsch, 1994; Alexander et al.,
1999). Today limited-area models are operational at the kilometric scale
(<inline-formula><mml:math id="M2" display="inline"><mml:mrow><mml:mi mathvariant="italic">&lt;</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mn mathvariant="normal">5</mml:mn></mml:mrow></mml:math></inline-formula> km) and data assimilation of observations with high
spatio-temporal resolution as lightning or radar reflectivity
factor<fn id="Ch1.Footn1"><p id="d1e214">Throughout the paper we use the expression radar
reflectivity factor, which is the quantity provided by the radar (and
expressed in millimetres to the sixth power per cubic metre or <inline-formula><mml:math id="M3" display="inline"><mml:mi>Z</mml:mi></mml:math></inline-formula>) after conversion from the received
power. The radar reflectivity factor is different from reflectivity and is
obtained in the special case of Rayleigh scattering. Reflectivity is not the
quantity that radars usually provide and display on their screens, although
most people refer to it.</p></fn> is crucial to correctly represent the state of
the atmosphere at local scale (Weisman et al., 1997; Weygandt et al., 2008).</p>
      <p id="d1e225">The assimilation of radar reflectivity factor is useful to
improve the weather forecast considering the high spatio-temporal resolution
of radar data.</p>
      <?pagebreak page1840?><p id="d1e228">First attempts to assimilate radar reflectivity factor are reported in Sun
and Crook (1997, 1998), who expanded VDRAS (Variational Doppler Radar
Analysis System) to include microphysical retrieval. Following these
studies, several systems to assimilate radar observations, both Doppler
velocity and reflectivity factor, were developed (Xue et al., 2003; Zhao et
al., 2006; Xu et al., 2010). All these studies showed the stability and
robustness of assimilating radar observations as well as the improvement of
weather forecast.</p>
      <p id="d1e231">In addition to direct methods, which assimilate the radar reflectivity
factor adjusting the hydrometeor contents, there are indirect methods
adjusting other variables. In particular, the method of Caumont et al. (2010) assimilates the relative humidity field. It consists of two different
steps: a 1-D retrieval of relative humidity (pseudo-profile), which depends
on the radar reflectivity factor observations, followed by 3D-Var
assimilation of the pseudo-profile. This method has the advantage of reducing
the computational cost at the kilometric scale.</p>
      <p id="d1e235">The choice of updating the moisture field directly is motivated by its
greater impact on analyses and forecasts in comparison to that of
hydrometeor-related quantities (e.g. Fabry and Sun, 2010).</p>
      <p id="d1e238">Caumont et al. (2010) showed that the method improved the weather prediction
of a heavy precipitation event in southern France and of an 8 d long
assimilation cycle experiment.</p>
      <p id="d1e241">The method was applied in other studies (Wattrelot et al., 2014, using the
AEROME model; Ridal and Dahlbom, 2017; using the HARMONIE model), or modified
using 4D-Var in place of 3D-Var (Ikuta and Honda, 2011; using the JNoVa
model), showing its capability to improve the weather forecast. The method is
also used in the operational context (Wattrelot et al., 2014).</p>
      <p id="d1e244">Lightning is another important source of asynoptic data due to its ability
to precisely locate the convection with few temporal gaps (Mansell et al.,
2007). In the last 2 decades, there have been attempts to assimilate
lightning into meteorological models at both low horizontal resolution,
which needs a cumulus parameterization scheme to simulate convection, and at
convection-permitting scales.</p>
      <p id="d1e247">First attempts to assimilate lightning in NWP models were based on
relationships between lightning and rainfall rate estimated by microwave
sensors on board polar-orbiting satellites (Alexander et al., 1999; Chang et
al., 2001; Jones and Macpherson, 1997; Pessi and Businger, 2009). In this
approach, the rainfall rate was computed as a function of the density of
lightning observations and then transformed into latent heat, which was
assimilated. The results of these studies showed a positive impact of the
lightning data assimilation on the forecast up to 24 h also for fields at the
large scale, such as sea-level pressure.</p>
      <p id="d1e250">The study of Papadopoulos  et al. (2005) used lightning to locate convection
and the simulated water vapour profile was nudged towards vertical profiles
recorded during convective events.</p>
      <p id="d1e254">Mansell et al. (2007) modified the Kain–Fritsch (Kain and Fritsch, 1993)
cumulus convective scheme to force convection when and where flashes are
observed while the convection scheme was not activated in the model
simulation, demonstrating the potential of lightning to improve the
convection forecast. A similar approach was introduced by Giannaros et al. (2016) into WRF, showing the positive impact of lightning data assimilation
on the precipitation forecast up to 24 h for eight convective events that
occurred over Greece.</p>
      <p id="d1e257">Fierro et al. (2012) introduced a methodology to assimilate lightning at
convection-resolving scales by modifying the water vapour mixing ratio
simulated by WRF according to a function depending on the flash rate and on
the simulated graupel mixing ratio. The water vapour could be assimilated by
nudging (Fierro et al., 2012) or 3D-Var (Fierro e al., 2016).</p>
      <p id="d1e260">Qie et al. (2014), using WRF, adopted the methodology of Fierro et al. (2012) to assimilate ice crystals, graupel, and snow, showing promising
results for deep convective events in China.</p>
      <p id="d1e263">Fierro et al. (2015) studied the performance of the Fierro et al. (2012)
method for 67 d spanning the 2013 warm season over the contiguous US, giving a
statistically robust estimation of the performance of the method. The
computationally inexpensive lightning data assimilation method improved
the short-term (<inline-formula><mml:math id="M4" display="inline"><mml:mrow><mml:mo>≤</mml:mo><mml:mn mathvariant="normal">6</mml:mn></mml:mrow></mml:math></inline-formula> h) precipitation forecast of high
impact weather considerably.</p>
      <p id="d1e276">Lynn et al. (2015) and Lynn (2017) also applied the method of Fierro et al. (2012) to boost the local thermal buoyancy where and when lightning is observed.
Results show that lightning data assimilation improved lightning forecast.
Importantly, Lynn et al. (2015) offer an approach to address spurious
convection (i.e. convection removal), which is a more challenging problem
to tackle.</p>
      <p id="d1e279">Federico et al. (2017a) implemented the methodology of Fierro et al. (2012)
in the RAMS@ISAC model, showing the systematic and significant improvement of
the precipitation forecast at the very short range (3 h) for 20 case
studies that occurred over Italy; the impact of lightning data assimilation for
longer forecast ranges (6–24 h; Federico et al., 2017b) showed a considerable
impact on the 6 h precipitation forecast, with smaller (negligible) effects
at 12 h (24 h).</p>
      <p id="d1e283">In this paper, we study the impact of radar reflectivity factor and
lightning data assimilation on the very short-term (3 h) rainfall prediction
for two case studies in Italy. We use the method of Fierro et al. (2012) to
assimilate lightning and the method of Caumont et al. (2010) to assimilate
the radar reflectivity factor. The case studies occurred in September 2017.
The first case, hereafter referred to as Serrano, occurred on 16 September and was characterized by moderate-intense and localized rainfall.
The second case, hereafter referred to as Livorno, occurred on 9–10 September, and was characterized by deep convection and very intense
precipitation in several parts of Italy. Even if the Livorno case occurred
before the Serrano case, we reverse the chronological<?pagebreak page1841?> order in the
discussion, ordering the event from the less to the most intense.</p>
      <p id="d1e286">The forecast of severe events at the local scale still remains challenging
because of the multitude of physical processes involved over a wide range of
scales (Stensrud et al., 2009). The Serrano case study, being localized in
space, poses challenges in forecasting the exact position and timing of
convection initiation; the Livorno event involves the interaction between a
high-impact storm and the complex orography of Italy, which is difficult to
simulate at the local scale. For the above reasons the forecast of both
events was challenging, as confirmed by the poor forecast of RAMS@ISAC
without data assimilation. The difficulty to timely and accurately forecast
the precipitation field for the two case studies is the reason for choosing
them as test cases.</p>
      <p id="d1e289">This paper presents for the first time the assimilation of the total
lightning (intra-cloud <inline-formula><mml:math id="M5" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> cloud to ground) and radar reflectivity factor in
RAMS@ISAC and shows how the assimilation of radar reflectivity factor works
together with total lightning data assimilation. Also, this paper shows that
the precipitation forecast using cloud-scale observations over complex
terrain can be accurate, contributing to a number of works on the same
subject.</p>
      <p id="d1e299">The paper is organized as follows: Sect. 2 gives details on the synoptic
environment of the case studies showing daily precipitation, lightning, and
radar observations; Sect. 3 gives details on the meteorological model,
lightning, and radar data assimilation; Sect. 4 shows the results for three
very short-term forecasts (VSFs), one for Serrano and two for Livorno;
Discussion and conclusions are given in Sect. 5. This paper has additional
material where we discuss (a) how the lightning and radar reflectivity
factor data assimilation impacts the total water field evolution, (b) the
sensitivity of the results to the choice of key parameters of lightning data
assimilation, (c) the sensitivity of the results to two aspects of the radar
formulation, (d) the sensitivity of the results to two aspects of RAMS@ISAC
setting, and (e) the impact of lightning data assimilation for a well- predicted
case study. The Supplement also gives the form of the radar forward
operator.</p>
</sec>
<sec id="Ch1.S2">
  <label>2</label><title>The case studies</title>
<sec id="Ch1.S2.SS1">
  <label>2.1</label><title>The 16 September 2017 (Serrano) case study</title>
      <p id="d1e317">On 16 September 2017 Italy was under the influence of a cyclone that
developed to the lee of the Alps. The storm crossed Italy from NW to SE
leaving light precipitation over most of the peninsula with moderate
rainfall over central Italy. Figure 1 shows the precipitation recorded by
the Italian rain gauge network on 16 September 2017. Light precipitation
(<inline-formula><mml:math id="M6" display="inline"><mml:mrow><mml:mi mathvariant="italic">&lt;</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mn mathvariant="normal">5</mml:mn></mml:mrow></mml:math></inline-formula> mm d<inline-formula><mml:math id="M7" 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>) is reported by 1018 rain gauges out of the 1666 stations
measuring precipitation (<inline-formula><mml:math id="M8" display="inline"><mml:mrow><mml:mo>≥</mml:mo><mml:mn mathvariant="normal">0.2</mml:mn></mml:mrow></mml:math></inline-formula> mm d<inline-formula><mml:math id="M9" 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>) on this day. A total of 14 stations
over central Italy recorded more than 50 mm d<inline-formula><mml:math id="M10" 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>. The maximum precipitation
was 90 mm d<inline-formula><mml:math id="M11" 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> in Città di Castello (Umbria region, Fig. 1). Because
the meteorological radar closest to the maximum precipitation is over Mount
Serrano (Fig. 1), hereafter this event will be referred to as Serrano.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1"><?xmltex \currentcnt{1}?><label>Figure 1</label><caption><p id="d1e392">Daily precipitation over Italy on 16 September 2017. Only
rain gauges observing at least 0.2 mm d<inline-formula><mml:math id="M12" 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> are shown. The first number in the
figure title within brackets represents the available rain gauges, while the
second number represents rain gauges observing at least 0.2 mm d<inline-formula><mml:math id="M13" 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>. The
lowest precipitation class is represented by smaller dots, the largest by a
red square. The locations of Città di Castello and Mount Serrano are
indicated.</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/19/1839/2019/nhess-19-1839-2019-f01.png"/>

        </fig>

      <?xmltex \floatpos{p}?><fig id="Ch1.F2"><?xmltex \currentcnt{2}?><label>Figure 2</label><caption><p id="d1e427"><bold>(a)</bold> Geopotential height (filled contours), temperature (contours),
and wind vectors at 500 hPa on 16 September 2017 at 00:00 UTC. Maximum velocity
is 31 m s<inline-formula><mml:math id="M14" 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>; <bold>(b)</bold> equivalent potential temperature (filled contours), sea-level
pressure (contours), and wind vectors at 24 m above the surface (maximum
value 13 m s<inline-formula><mml:math id="M15" 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>). A low-pressure pattern forms over northern Italy, with a
front in the western Mediterranean.</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/19/1839/2019/nhess-19-1839-2019-f02.jpg"/>

        </fig>

      <p id="d1e466">The synoptic conditions during the event are shown in Fig. 2. At 500 hPa
(Fig. 2a), a trough, elongated in the SW–NE direction, extends over western
Europe and air masses are advected from SW towards the western Alps. The
interaction between the airflow and the Alps generates a low pressure to the
lee of the Alps over northern Italy.</p>
      <p id="d1e469">The analysis at the surface (Fig. 2b) shows the meteorological front
represented by the equivalent potential temperature gradient between air
masses advected over the Mediterranean Sea from the NW and air masses advected
from the south over the Tyrrhenian Sea. The advection of warm unstable air
masses towards central Italy is notable.</p>
      <p id="d1e472">Infrared satellite images (Fig. 3), from 00:00 UTC on 16 September to 00:00 UTC
on 17 September, show that the cold front structure moved slowly from NW to
SE. Interestingly, at 00:00 UTC on 16 September, the
well-defined cloud system over central Italy (red circle of Fig. 3a) that
caused most of the daily precipitation observed between 43.50 and 45.0<inline-formula><mml:math id="M16" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N is apparent.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3" specific-use="star"><?xmltex \currentcnt{3}?><label>Figure 3</label><caption><p id="d1e486"><bold>(a)</bold> Satellite images (METEOSAT second generation) of the infrared
channel, 10.8 <inline-formula><mml:math id="M17" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>m, at 00:00   and 12:00 UTC on 16 September, and at 00:00 UTC on
17 September 2017. A well-defined cloud system is apparent inside the red
circle of the image at 00:00 UTC on 16 September 2017. Source: <uri>https://www.sat24.com</uri> (last access: 8 August 2019); © EUMETSAT.</p></caption>
          <?xmltex \igopts{width=497.923228pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/19/1839/2019/nhess-19-1839-2019-f03.jpg"/>

        </fig>

      <p id="d1e508">The well-defined cloud system over central Italy is also shown in the radar
constant-altitude plan position indicator (CAPPI) at 3 km above sea level at
02:00 UTC on 16 September (Fig. 4). This CAPPI is formed by interpolating all
the<?pagebreak page1842?> available data from the federated Italian radar network coordinated by
the Department of Civil Protection (22 radars; see Sect. 3.3 for
their positions) and it is also referred to as the national radar composite
(hereafter also mosaic). Several convective cells exceeding 35 dBz can be
noted over central-northern Italy. Importantly, the cloud system over
central Italy shown by the satellite infrared channel at 00:00 UTC (Fig. 3a)
and that of the radar at 02:00 UTC have similar positions, showing that the
cloud system was active for several hours over central Italy.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4"><?xmltex \currentcnt{4}?><label>Figure 4</label><caption><p id="d1e514">National radar mosaic at 3 km above the sea level observed at 02:00 UTC on 16 September 2017.</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/19/1839/2019/nhess-19-1839-2019-f04.png"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F5"><?xmltex \currentcnt{5}?><label>Figure 5</label><caption><p id="d1e525">Lightning density (number of lightning strikes per 16 km<inline-formula><mml:math id="M18" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula> for the
whole day) recorded on 16 September 2017. The total number of flashes is
shown in the title.</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/19/1839/2019/nhess-19-1839-2019-f05.png"/>

        </fig>

      <p id="d1e543">Figure 5 shows the lightning recorded by LINET (lightning detection network; Betz et al.,
2009) on 16 September 2017. More than 105 000 flashes were recorded; most of
them occurred in the afternoon and evening, but a secondary maximum occurred
in the night, from 00:00  to 06:00 UTC. In this phase, more than 3000 flashes
were observed over central Italy.</p>
</sec>
<sec id="Ch1.S2.SS2">
  <label>2.2</label><title>The 9–10 September 2017 (Livorno) case study</title>
      <p id="d1e554">On 9 and 10 September 2017, Italy was hit by a severe storm
characterized by intense and widespread rainfall over the country. Figure 6a
shows the precipitation on  9 September recorded by the Italian rain gauge
network. Rainfall was intense over the Alps, where the maximum daily
precipitation was observed (193 mm d<inline-formula><mml:math id="M19" 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>), and over Liguria, with
precipitation of the order of 30–50 mm d<inline-formula><mml:math id="M20" 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>. One station over Tuscany
reported 90 mm d<inline-formula><mml:math id="M21" 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>, showing that intense precipitation had already started over
the region. The storm on  9 September was intense: 20 rain gauges reported
more than 100 mm d<inline-formula><mml:math id="M22" 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> and 70 rain gauges more than 60 mm d<inline-formula><mml:math id="M23" 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>. In most cases,
this precipitation occurred within a few hours.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F6"><?xmltex \currentcnt{6}?><label>Figure 6</label><caption><p id="d1e619"><bold>(a)</bold> As in Fig. 1 but for <bold>(a)</bold> 9 September 2017 and <bold>(b)</bold> 10 September 2017.</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/19/1839/2019/nhess-19-1839-2019-f06.jpg"/>

        </fig>

      <p id="d1e636">The following day (see Fig. 6b) had higher rainfall. Precipitation
occurred mainly over central Italy, especially over Lazio, and over northern
Italy, in particular over the northeast. In Tuscany, the two stations close
to the sea, in the Livorno area, recorded about 150 mm d<inline-formula><mml:math id="M24" 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> mostly falling
between 00:00 and 06:00 UTC.</p>
      <p id="d1e652">Synoptic conditions leading to this storm are shown in Fig. 7. At 500 hPa
(Fig. 7a) a trough extended from northern Europe towards the
Mediterranean. The interaction between the air masses and western Alps
generated a low-pressure system to the lee of the Alps, which crossed the
whole peninsula from NW to SE. It is noted that the divergent flow over central
and northern Italy favoured upward motions.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F7"><?xmltex \currentcnt{7}?><label>Figure 7</label><caption><p id="d1e657"><bold>(a)</bold> Geopotential height (filled contours), temperature (contours),
and wind vectors at 500 hPa at 00:00 UTC on 10 September 2017. Maximum velocity
is 37 m s<inline-formula><mml:math id="M25" 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>; <bold>(b)</bold> equivalent potential temperature (filled contours), sea-level
pressure (contours), and wind vectors at 24 m above the surface (maximum
value 15 m s<inline-formula><mml:math id="M26" 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>).</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/19/1839/2019/nhess-19-1839-2019-f07.jpg"/>

        </fig>

      <p id="d1e695">At the surface, Fig. 7b, the equivalent temperature gradient over the
western Mediterranean is caused by the contrast between pre-existing air masses
over the sea and air masses advected from France towards the
Mediterranean. The pressure field at the surface advects air masses from the
south over the Tyrrhenian Sea. These warm and humid air masses feed the
cyclone during its development.</p>
      <p id="d1e698">From a synoptic point of view, the Livorno and Serrano cases were similar and
represented two cyclones developing<?pagebreak page1843?> to the lee of the Alps (Buzzi and
Tibaldi, 1978). However, the Livorno case was more intense than Serrano.</p>
      <p id="d1e701">The notable intensity of the Livorno case is confirmed by the lightning
observations (Fig. 8). During the evening of 9 September (after 18:00 UTC)
about 38 000 flashes were recorded by LINET. On 10 September about 290 000
flashes were recorded over Italy, following the movement of the storm from
NW to SE. Therefore, more than 300 000 flashes were recorded from 18:00 UTC on
9 September to 00:00 UTC on 11 September, which is more than 3 times
those recorded for Serrano.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F8"><?xmltex \currentcnt{8}?><label>Figure 8</label><caption><p id="d1e707"><bold>(a)</bold> Lightning density (lightning number per 16 km<inline-formula><mml:math id="M27" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula> for the
whole day) recorded on  9 September 2017; <bold>(b)</bold> as in <bold>(a)</bold> for 10 September 2017.
The number of flashes on each day is shown in the title.</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/19/1839/2019/nhess-19-1839-2019-f08.jpg"/>

        </fig>

      <p id="d1e733">Thermal infrared satellite images (channel, 10.8 <inline-formula><mml:math id="M28" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>m; Fig. 9) show the
extension of the cloud coverage every 12 h. It is very evident that the
cloud system was associated with a cold front over Europe. More
specifically, the satellite image at 00:00 UTC shows the cloud system over the
Livorno area (red circle in Fig. 9b), before the most intense
precipitation period over Tuscany (00:00–06:00 UTC), while Fig. 9c shows the
cloud system over central Italy (orange circle), at the end of the period of
intense precipitation over Lazio (06:00–12:00 UTC).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F9" specific-use="star"><?xmltex \currentcnt{9}?><label>Figure 9</label><caption><p id="d1e746"><bold>(a)</bold> Satellite images (METEOSAT second generation) of the infrared
channel, 10.8 <inline-formula><mml:math id="M29" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>m, at 12:00 UTC on 9 September 2017, at 00:00 and 12:00 UTC on
10 September 2017. The red circle in Fig. 9b and the orange circle in
Fig. 9c show the Livorno and Lazio areas, respectively. Source: <uri>https://www.sat24.com</uri>; © EUMETSAT.</p></caption>
          <?xmltex \igopts{width=497.923228pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/19/1839/2019/nhess-19-1839-2019-f09.jpg"/>

        </fig>

      <p id="d1e768">We conclude the synoptic analysis of the case study with two CAPPIs at 3 km
observed by the radar network of the Department of Civil Protection. The
CAPPI in Fig. 10a, at 00:00 UTC on 10 September, shows the cloud system over
Tuscany with reflectivity factors up to 40 dBz. Other clouds caused rainfall
over northern Italy. The CAPPI of Fig. 10a<?pagebreak page1844?> is the last one assimilated by
the 00:00–03:00 UTC VSF on 10 September described in detail in Sect. 4.2.1.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F10"><?xmltex \currentcnt{10}?><label>Figure 10</label><caption><p id="d1e773"><bold>(a)</bold> National radar mosaic at 3 km above the sea level observed at
00:00 UTC on 10 September 2017; <bold>(b)</bold> as in <bold>(a)</bold> at 06:00 UTC.</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/19/1839/2019/nhess-19-1839-2019-f10.jpg"/>

        </fig>

      <p id="d1e791">Figure 10b shows the CAPPI of the national radar mosaic at 3 km above the
sea level and at 06:00 UTC. The cloud system is moving towards central Italy
with reflectivity factors up to 45 dBz. Other cloud systems are apparent
over northern Italy. Figure 10a–b represent the movement of the
storm towards the SE well and Fig. 10b shows the last CAPPI assimilated by the
06:00–09:00 UTC VSF shown in Sect. 4.2.2.</p>
</sec>
</sec>
<sec id="Ch1.S3">
  <label>3</label><title>Data and methods</title>
<sec id="Ch1.S3.SS1">
  <label>3.1</label><title>RAMS@ISAC and simulations set-up</title>
      <p id="d1e810">The RAMS@ISAC is used as a NWP driver in this work. The model is based on the
RAMS 6.0 model (Cotton et al., 2003)<?pagebreak page1845?> with the addition of four main
features, as well as a number of minor improvements. First, it implements
additional single-moment microphysical schemes, whose performance is shown
in Federico (2016): among them, the WSM6 (Hong and Lim, 2006) is used in
this paper. Second, it predicts the occurrence of lightning following the
diagnostic method of Dahl et al. (2011), with the implementation discussed
in Federico et al. (2014). Third, the model assimilates lightning through
nudging (Fierro et al., 2012, 2015; Federico et al., 2017a). Fourth, the
model implements a 3D-Var data assimilation system (Federico, 2013,
hereafter also RAMS-3DVar), whose extension to the radar reflectivity factor
is presented in this paper (Sect. 3.3).</p>
      <p id="d1e813">The list of the physical parameterization schemes used in the simulations of
RAMS@ISAC is shown in Table 1.</p>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T1" specific-use="star"><?xmltex \currentcnt{1}?><label>Table 1</label><caption><p id="d1e819">RAMS@ISAC physical parameterizations used in this paper.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="2">
     <oasis:colspec colnum="1" colname="col1" align="justify" colwidth="142.26378pt"/>
     <oasis:colspec colnum="2" colname="col2" align="justify" colwidth="330.051969pt"/>
     <oasis:thead>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">Physical parameterization</oasis:entry>
         <oasis:entry colname="col2">Selected scheme</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">Parameterized cumulus convection</oasis:entry>
         <oasis:entry colname="col2">Modified Kuo scheme to account for updraft and downdraft (Molinari and Corsetti, 1985). The scheme is applied to R10 only.</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">Explicit precipitation parameterization</oasis:entry>
         <oasis:entry colname="col2">Bulk microphysics with six hydrometeors (cloud, rain, graupel, snow, ice, water vapour). Described in Hong and Lim (2006).</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">Exchange between the surface, the biosphere, and atmosphere</oasis:entry>
         <oasis:entry colname="col2">LEAF3 (Walko et al., 2000). LEAF includes prognostic equations for soil temperature and moisture for multiple layers, vegetation temperature and surface water, and temperature and water vapour mixing ratio of canopy air.</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">Sub-grid mixing</oasis:entry>
         <oasis:entry colname="col2">The turbulent mixing in the horizontal directions is parameterized following Smagorinsky (1963), and vertical diffusion is parameterized according to the Mellor and Yamada (1982) scheme, which employs a prognostic turbulent kinetic energy.</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Radiation scheme</oasis:entry>
         <oasis:entry colname="col2">Chen–Cotton (Chen and Cotton, 1983). The scheme accounts for condensate in the atmosphere.</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table></table-wrap>

      <p id="d1e892">Considering the domains and the configuration of the grids (Fig. 11 and
Table 2), two different set-ups are used for Serrano and Livorno. For the
first case, we use the domains D1 and D2, while for Livorno we also use the
domain D3. The first domain covers a large part of Europe and extends over North Africa. Grid horizontal resolution is 10 km (R10). The second
domain covers all of Italy and part of Europe and the grid has 4 km
horizontal resolution (R4). The third domain covers the Tuscany region, has
<inline-formula><mml:math id="M30" display="inline"><mml:mrow><mml:mn mathvariant="normal">4</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:math></inline-formula> km horizontal resolution (R1), and it is used for Livorno to represent the precipitation field over Tuscany with higher spatial detail. The fine
structures of the precipitation field are smeared out over Tuscany using
only domains D1 and D2. The operational implementation of the RAMS@ISAC
model uses the domains D1 and D2 and no refinements for specific areas of
Italy are used because this would require a computing power which is not
currently available. Also, grid refinements over Italy would require careful
testing of the model performance and data assimilation system, which are out
of the scope of this paper.</p>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T2"><?xmltex \currentcnt{2}?><label>Table 2</label><caption><p id="d1e910">Basic parameters of the RAMS@ISAC grids (R10, R4, and R1,
corresponding, respectively, to the domains D1, D2, and D3). NNXP is the
number of grid points in the WE direction, NNYP is the number of grid points
in the NS direction, NNZP is the number of vertical levels, DX is the size
of the grid spacing in the WE direction, and DY is the grid spacing in the SN
direction. Lx, Ly, and Lz are the domain extensions in the NS, WE, and
vertical directions. CENTLON and CENTLAT are the coordinates of the grid
centres.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="4">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="left"/>
     <oasis:colspec colnum="3" colname="col3" align="left"/>
     <oasis:colspec colnum="4" colname="col4" align="left"/>
     <oasis:thead>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2">R10, D1</oasis:entry>
         <oasis:entry colname="col3">R4, D2</oasis:entry>
         <oasis:entry colname="col4">R1, D3</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>
         <oasis:entry colname="col1">NNXP</oasis:entry>
         <oasis:entry colname="col2">301</oasis:entry>
         <oasis:entry colname="col3">401</oasis:entry>
         <oasis:entry colname="col4">203</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">NNYP</oasis:entry>
         <oasis:entry colname="col2">301</oasis:entry>
         <oasis:entry colname="col3">401</oasis:entry>
         <oasis:entry colname="col4">203</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">NNZP</oasis:entry>
         <oasis:entry colname="col2">36</oasis:entry>
         <oasis:entry colname="col3">36</oasis:entry>
         <oasis:entry colname="col4">36</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Lx</oasis:entry>
         <oasis:entry colname="col2">3000 km</oasis:entry>
         <oasis:entry colname="col3">1600 km</oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M31" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">270</mml:mn></mml:mrow></mml:math></inline-formula> km</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Ly</oasis:entry>
         <oasis:entry colname="col2">3000 km</oasis:entry>
         <oasis:entry colname="col3">1600 km</oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M32" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">270</mml:mn></mml:mrow></mml:math></inline-formula> km</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Lz</oasis:entry>
         <oasis:entry colname="col2"><inline-formula><mml:math id="M33" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">22400</mml:mn></mml:mrow></mml:math></inline-formula> m</oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M34" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">22400</mml:mn></mml:mrow></mml:math></inline-formula> m</oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M35" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">22400</mml:mn></mml:mrow></mml:math></inline-formula> m</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">DX</oasis:entry>
         <oasis:entry colname="col2">10 km</oasis:entry>
         <oasis:entry colname="col3">4 km</oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M36" display="inline"><mml:mrow><mml:mn mathvariant="normal">4</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:math></inline-formula> km</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">DY</oasis:entry>
         <oasis:entry colname="col2">10 km</oasis:entry>
         <oasis:entry colname="col3">4 km</oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M37" display="inline"><mml:mrow><mml:mn mathvariant="normal">4</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:math></inline-formula> km</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">CENTLAT (<inline-formula><mml:math id="M38" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>)</oasis:entry>
         <oasis:entry colname="col2">43.0<inline-formula><mml:math id="M39" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N</oasis:entry>
         <oasis:entry colname="col3">43.0<inline-formula><mml:math id="M40" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N</oasis:entry>
         <oasis:entry colname="col4">43.7<inline-formula><mml:math id="M41" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">CENTLON (<inline-formula><mml:math id="M42" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>)</oasis:entry>
         <oasis:entry colname="col2">12.5<inline-formula><mml:math id="M43" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E</oasis:entry>
         <oasis:entry colname="col3">12.5<inline-formula><mml:math id="M44" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E</oasis:entry>
         <oasis:entry colname="col4">11.0<inline-formula><mml:math id="M45" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table></table-wrap>

      <p id="d1e1237">All domains share the same vertical grid, which covers the troposphere and
the lower stratosphere. Vertical levels are more packed close to the ground.
Among the 36 levels used in this paper 10 are below 1 km, 14 below 2 km, and
17 below 3 km. The first vertical level is at 50 m above the surface in the
terrain following coordinates used by RAMS@ISAC; level 21 is at 5122 m.
Above 6 km the model levels are about 1000 m apart, while the maximum
allowed distance between two levels is 1200 m. The complete list of the
vertical levels is shown in the Supplement of this paper (Table S2 in the Supplement).</p>
      <p id="d1e1240">The vertical grid is the same as the operational setting of RAMS@ISAC and is
a compromise between vertical resolution and computing time. The number of
vertical levels will be increased to 42, starting from September 2019, to
better resolve the phenomena in this direction (planetary boundary layer
processes, vertical motions, interaction between air masses and orography,
etc.). Nevertheless the current setting was successfully applied to the
forecast of several heavy precipitation events over Italy. A sensitivity
test, using 42 vertical levels for the Livorno case, shows similar results
to those reported in Sect. 4. Details on this simulation can be found in
the Supplement of this paper.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F11"><?xmltex \currentcnt{11}?><label>Figure 11</label><caption><p id="d1e1245">The three domains used in RAMS@ISAC. The model grid over domain
D1 has 301 grid points in the NS and WE directions and has 10 km horizontal
resolution; the model grid over domain D2 has 401 grid points in the NS and
WE directions and has 4 km horizontal resolution. The model grid over domain
D3 has 203 grid points in the NS and WE directions and has <inline-formula><mml:math id="M46" display="inline"><mml:mrow><mml:mn mathvariant="normal">4</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:math></inline-formula> km horizontal
resolution. All grids have the same 36 vertical levels spanning the
0–22.4 km vertical layer.</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/19/1839/2019/nhess-19-1839-2019-f11.png"/>

        </fig>

      <p id="d1e1267">The nesting between the first and second domains is one-way, while the
nesting between the second and the third domains is two-way.</p>
      <p id="d1e1270">VSF was implemented as shown in Fig. 12. First a run with the R10
configuration was performed using the 0.25<inline-formula><mml:math id="M47" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> horizontal resolution
Global Forecast System (GFS) analysis–forecast cycle issued at 12:00 UTC as initial and boundary
conditions. The R10 run, which started at 12:00 UTC on 16 September for Serrano and
at 12:00 UTC on 9 September for Livorno, lasted 36 h and does not assimilate
either radar reflectivity factor or lightning. The R10 run was not updated
after the acquisition of new data by the analysis system and this is a
limitation of the results shown in this paper.<?pagebreak page1846?> However, a sensitivity test
for the Livorno case study showed that this limitation does not have a
significant impact on the results presented in the next section. Details on
this experiment can be found in the Supplement of this paper.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F12" specific-use="star"><?xmltex \currentcnt{12}?><label>Figure 12</label><caption><p id="d1e1284">The implementation of RAMS@ISAC very short-term forecast.</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/19/1839/2019/nhess-19-1839-2019-f12.png"/>

        </fig>

      <p id="d1e1293">Starting from 12:00 UTC, 10 VSFs were performed using R4 for Serrano and both R4
and R1 for Livorno. The VSF lasted 9 h and used R10 simulation as initial and
boundary conditions (one-way nesting). The 9 h forecast was divided into two
parts: the first 6 h are the assimilation stage when RAMS@ISAC
simulation was adjusted by data assimilation, whereas the last 3 h
are the forecast stage, without data assimilation. During the assimilation
stage, flashes are assimilated by nudging (Sect. 3.2), while radar
reflectivity factor is assimilated every hour by RAMS-3DVar (Sect. 3.3).</p>
      <p id="d1e1296">It is noted that data assimilation is performed over the domain D2 (R4)
only, and the innovations are transferred to the domain D3 (R1) for the
Livorno case by the two-way nesting. The domain D3 is used for the Livorno
case to refine the resolution of the precipitation field over Tuscany and to
show the spatial and temporal precision of the precipitation forecast over
Tuscany using data assimilation. However, its usage is exceptional because,
as stated above, Italy is a complex orographic country and grid refinements
for specific areas are used only after the occurrence of the event. For this
reason, the domain D3 is usually not used in RAMS@ISAC and no statistics
about the background error are available for this grid.</p>
      <p id="d1e1300">Because lightning and radar reflectivity factors are cloud-scale
observations, their assimilation at higher horizontal resolution by 3D-Var
is foreseeable in future works.</p>
      <p id="d1e1303">The verification of the VSF for precipitation was done by visual comparison
of the model output with the rain gauge network of the Department of Civil
Protection, which has more than 3000 rain gauges all over Italy.</p>
      <?pagebreak page1847?><p id="d1e1306">In addition we considered the FBIAS (frequency bias; range [0, <inline-formula><mml:math id="M48" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mi mathvariant="normal">∞</mml:mi></mml:mrow></mml:math></inline-formula>)), where 1 is the perfect score, i.e. when no misses and false alarms
occur), POD (probability of detection; range [0, 1], where 1 is the perfect
score and 0 the worst value), ETS (equitable threat score; range [<inline-formula><mml:math id="M49" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:math></inline-formula>, 1],
where 1 is the perfect score and 0 is a useless forecast), and TS (threat score;
range [0, 1], where 1 is the perfect score and 0 the worst value). Scores were
computed from <inline-formula><mml:math id="M50" display="inline"><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mo>×</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> dichotomous contingency tables (Wilks, 2006) for different
rainfall thresholds and for different neighbourhood radii. Moreover,
performance diagrams (Roebber, 2009) were used to summarize the scores.</p>
</sec>
<sec id="Ch1.S3.SS2">
  <label>3.2</label><title>Lightning data assimilation</title>
      <p id="d1e1353">Lightning data are provided by LINET (lightning detection network;  Betz et
al., 2009; nowcast, 2019), which has more than 500 sensors worldwide with
the greatest density over Europe (more than 200 sensors). The network has a
good<?pagebreak page1848?> coverage over central Europe, and western Mediterranean (from 10<inline-formula><mml:math id="M51" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W to 35<inline-formula><mml:math id="M52" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E and from 30  to 60<inline-formula><mml:math id="M53" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N). The area of good coverage includes the region
considered in this paper.</p>
      <p id="d1e1383">LINET exploits the VLF and LF (very low frequency and low frequency) electromagnetic bands and provides measurements of
both intra-cloud (IC) and cloud-to-ground (CG) discharges. IC strokes are
detected as long as lightning occurs within 120 km of the nearest sensor
thanks to optimized hardware and advanced techniques of data processing
(TOA-3D; Betz et al., 2004). According to Betz et al. (2009), LINET has a
location accuracy of 125 m for an average distance of 200 km among the
sensors verified by strikes into towers of known positions.</p>
      <p id="d1e1386">The good performance of the LINET network and its ability to detect IC
strokes is shown in Lagouvardos et al. (2009) for a storm in southern
Germany, while the good performance over Italy, including both CG and IC
strokes, is discussed in Petracca et al. (2014).</p>
      <p id="d1e1389">The lightning data assimilation scheme is that of Fierro et al. (2012, 2014,
2015) and uses the total lightning, i.e. intra-cloud plus cloud-to-ground
flashes.</p>
      <p id="d1e1393">The method starts by computing the water vapour mixing ratio <inline-formula><mml:math id="M54" display="inline"><mml:mrow><mml:msub><mml:mi>q</mml:mi><mml:mi>v</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>:
            <disp-formula id="Ch1.E1" content-type="numbered"><label>1</label><mml:math id="M55" display="block"><mml:mrow><mml:msub><mml:mi>q</mml:mi><mml:mi>v</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mi>A</mml:mi><mml:msub><mml:mi>q</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub><mml:mo>+</mml:mo><mml:mi>B</mml:mi><mml:msub><mml:mi>q</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub><mml:mi>tanh⁡</mml:mi><mml:mo>(</mml:mo><mml:mi>C</mml:mi><mml:mi>X</mml:mi><mml:mo>)</mml:mo><mml:mo>(</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>-</mml:mo><mml:mi>tanh⁡</mml:mi><mml:mo>(</mml:mo><mml:mi>D</mml:mi><mml:msubsup><mml:mi>q</mml:mi><mml:mi mathvariant="normal">g</mml:mi><mml:mi mathvariant="italic">α</mml:mi></mml:msubsup><mml:mo>)</mml:mo><mml:mo>)</mml:mo><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
          where coefficients are set to <inline-formula><mml:math id="M56" display="inline"><mml:mrow><mml:mi>A</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.86</mml:mn></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M57" display="inline"><mml:mrow><mml:mi>B</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.15</mml:mn></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M58" display="inline"><mml:mrow><mml:mi>C</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.30</mml:mn></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M59" display="inline"><mml:mrow><mml:mi>D</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.25</mml:mn></mml:mrow></mml:math></inline-formula>, and
<inline-formula><mml:math id="M60" display="inline"><mml:mrow><mml:mi mathvariant="italic">α</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">2.2</mml:mn></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M61" display="inline"><mml:mrow><mml:msub><mml:mi>q</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the saturation mixing ratio at the model
atmospheric temperature, and <inline-formula><mml:math id="M62" display="inline"><mml:mrow><mml:msub><mml:mi>q</mml:mi><mml:mi mathvariant="normal">g</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the graupel mixing ratio (g kg<inline-formula><mml:math id="M63" 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>). <inline-formula><mml:math id="M64" display="inline"><mml:mi>X</mml:mi></mml:math></inline-formula> is the number of total flashes (IC<inline-formula><mml:math id="M65" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>CG) falling in a grid box
of domain D2 (R4) in the past 5 min. The mixing ratio <inline-formula><mml:math id="M66" display="inline"><mml:mrow><mml:msub><mml:mi>q</mml:mi><mml:mi>v</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> of Eq. (1) is computed only for grid points where flashes are recorded. More
specifically, for each grid point we consider the number of flashes falling
in a grid box centred at the grid point in the last 5 min. The mixing
ratio of Eq. (1) is compared with that predicted by the model. If the
mixing ratio of Eq. (1) is larger than the simulated one, the latter is
nudged towards the value of Eq. (1), otherwise the modelled mixing ratio is
left unchanged. This method can only add water vapour to the forecast.</p>
      <p id="d1e1593">The check and eventual substitution of the water vapour is performed every
5 min and it is made within the mixed phase layer zone (0 and <inline-formula><mml:math id="M67" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">25</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M68" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C), wherein electrification processes caused by the
collision of ice and graupel are the most active (Takahashi, 1978; Emersic
and Sounders, 2010; Fierro et al., 2015).</p>
      <p id="d1e1615">The scheme of Fierro et al. (2012, 2015) was adapted to RAMS@ISAC in
Federico et al. (2017a). In particular, the coefficient <inline-formula><mml:math id="M69" display="inline"><mml:mi>C</mml:mi></mml:math></inline-formula> of Eq. (1) was
rescaled from that of Fierro et al. (2012) considering the different
spatio-temporal resolution of gridded lightning data; then the coefficient <inline-formula><mml:math id="M70" display="inline"><mml:mi>C</mml:mi></mml:math></inline-formula>
was tuned (increased) by sensitivity tests considering two case studies of
HyMeX-SOP1 (15 and 27 October 2012; HyMeX stands for the Hydrological cycle
in the Mediterranean Experiment – First Special Observing Period occurring
between 6 September and 6 November 2012; Ducrocq et al., 2014). The <inline-formula><mml:math id="M71" display="inline"><mml:mi>C</mml:mi></mml:math></inline-formula>
constant was adapted subjectively as a compromise of increasing the hits and
minimizing false alarms. POD and ETS scores were considered metrics for
this purpose. Then, Eq. (1) was applied to 20 case studies of
HyMeX-SOP1 giving a statistically significant (90 %, or 95 % depending on
the rainfall threshold) improvement of the RAMS@ISAC precipitation VSF (3 h).</p>
      <p id="d1e1639">Nevertheless, a definitive statistic on the performance of rainfall VSF to
nudging formulation in RAMS@ISAC is missing and further studies are needed
in this direction. Also, the optimal choice of the coefficients <inline-formula><mml:math id="M72" display="inline"><mml:mrow><mml:mi>A</mml:mi><mml:mo>,</mml:mo><mml:mi>B</mml:mi><mml:mo>,</mml:mo><mml:mi>C</mml:mi><mml:mo>,</mml:mo><mml:mi>D</mml:mi></mml:mrow></mml:math></inline-formula>,
and <inline-formula><mml:math id="M73" display="inline"><mml:mi mathvariant="italic">α</mml:mi></mml:math></inline-formula> is case dependent.</p>
      <p id="d1e1669">Fierro et al. (2012) applied the method using Earth Networks Total Lightning Network (ENTLN), which has a
detection efficiency (DE) greater than 50 % for IC over Oklahoma, where
the ENTLN data were used. The emphasis on IC flashes in the set-up of Fierro
et al. (2012) is given because observational and model studies have provided
evidence that IC flashes correlate better than CG flashes with various
measures of intensifying convection (updraft strength, volume, graupel mass
flux, etc.; MacGorman et al. 1989, 2005, 2011; Carey and Rutledge, 1998;
Wiens et al., 2005; Kuhlman et al. 2006; Fierro et al., 2006; Deierling
and Petersen, 2008). For these reasons methods using
both IC and CG flashes perform better than those using CG only, CG
flashes being correlated with the descent of reflectivity cores and the onset of
the demise of the storm's updraft core (MacGorman and Nielsen, 1991).</p>
      <p id="d1e1672">The analysis of the case studies shows that IC strokes are about 30 % of
the total number of strokes reported by LINET. Also, the fraction of IC
strokes to the total strokes depends<?pagebreak page1849?> on the position. For example, for the
Serrano case, the fraction of IC strokes detected by LINET over the area hit
by the largest precipitation is more than 50 % while over the Adriatic Sea
it decreases to 10 %.</p>
      <p id="d1e1676">It is also noted that the detection efficiency (DE) for IC strokes cannot be
reliably compared between LINET and ENTLN because the area is different and
the technical details about IC detection remain unclear (type of signals,
VLF–LF or very high frequency (VHF), discrimination IC or CG).</p>
      <p id="d1e1679">For all the above reasons the application of the Fierro method to RAMS@ISAC
is not straightforward and it is appropriate to study the dependence of the
rainfall VSF on the nudging formulation. This subject is studied in the
Supplement of this paper (Supplement Sect. S3) and the results show that
the choice of the coefficient of Eq. (1) used in this paper is reasonable.</p>
      <p id="d1e1682">It is finally noted that despite the limitations noted above, the lightning
data assimilation, with the setting of this paper, had a significant and
positive impact on RAMS@ISAC rainfall VSF (Federico et al., 2017a, b).</p>
</sec>
<sec id="Ch1.S3.SS3">
  <label>3.3</label><title>Radar data assimilation</title>
      <p id="d1e1693">The method assimilates CAPPI of radar reflectivity factor operationally
provided by the Italian Department of Civil Protection (DPC). Radar data are
provided over a regular Cartesian grid with 1 km horizontal resolution and
for three vertical levels (2, 3, 5 km above the sea level). The CAPPIs at 2,
3, and 5 km can be considered under-sampled vertical profiles. CAPPIs are
composed starting from the 22 radars of the Italian Radar Network (Fig. 13), 19 operating at the C band (i.e. 5.6 GHz) and 3 at the X band (i.e. 9.37 GHz). The data quality control and CAPPI composition is performed by DPC. Data
quality processing chain aims at identifying most of the uncertainty sources
as clutter, partial beam blocking, and beam broadening. The radar
observations are processed according to nine steps detailed in Vulpiani et
al. (2014), Petracca et al. (2018), and references therein.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F13"><?xmltex \currentcnt{13}?><label>Figure 13</label><caption><p id="d1e1698">The radar network of the Department of Civil Protection. Green
radars operate with dual polarization; blue radars have single polarization.</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/19/1839/2019/nhess-19-1839-2019-f13.png"/>

        </fig>

      <p id="d1e1707">Radial velocity is not assimilated into RAMS@ISAC because it is not
operationally processed, and the scan strategy being optimized for quantitative precipitation estimation (QPE) purposes.
Furthermore, the implementation of a radial velocity data assimilation
scheme is under development in RAMS-3DVar and it is not currently available
for testing. For these reasons, we did not consider the assimilation of this
parameter.</p>
      <p id="d1e1711">Before entering data assimilation, the Cartesian grid is downscaled to 5 km
by 5 km in order to reduce the numerical cost of the data assimilation and
the effect of correlated observation errors (Rohn et al., 2001). Thus, the
radar grid (Fig. 4, for example) is a Cartesian grid with 5 km
grid spacing and three vertical levels.</p>
      <p id="d1e1714">It is important to note that pure sampling of the data could result in
implementation of errors (for example reflectivity given by insects or
birds) or extremes. Creating super-observations would reduce this problem,
the main drawback being missing very localized phenomena. While the
aim of this paper is to present the update of the data assimilation system
of RAMS@ISAC and its application to two challenging cases, the problem of
using super-observations will be considered in future studies because it
impacts the results.</p>
      <p id="d1e1717">The methodology to assimilate radar reflectivity factor is that of Caumont
et al. (2010), named 1D+3D-Var, which is a two-step process: first, using a
Bayesian approach inspired by GPROF (Goddard profiling algorithm; Olson et
al., 1996; Kummerow et al., 2001), 1-D pseudo-profiles of model variables are
computed, and second those pseudo-profiles are assimilated by 3D-Var. Both steps
are discussed below.</p>
      <p id="d1e1720">The first step computes a pseudo-profile of relative humidity, weighting the
model profiles of relative humidity around the radar profile (Bayesian
approach). The pseudo-profile is computed by
            <disp-formula id="Ch1.E2" content-type="numbered"><label>2</label><mml:math id="M74" display="block"><mml:mrow><mml:msubsup><mml:mi mathvariant="bold-italic">z</mml:mi><mml:mi mathvariant="normal">o</mml:mi><mml:mi mathvariant="normal">p</mml:mi></mml:msubsup><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:munder><mml:mo movablelimits="false">∑</mml:mo><mml:mi>i</mml:mi></mml:munder><mml:mi mathvariant="bold-italic">R</mml:mi><mml:msub><mml:mi mathvariant="bold-italic">H</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:msub><mml:mi>W</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow><mml:mrow><mml:munder><mml:mo movablelimits="false">∑</mml:mo><mml:mi>j</mml:mi></mml:munder><mml:msub><mml:mi>W</mml:mi><mml:mi>j</mml:mi></mml:msub></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
          where <inline-formula><mml:math id="M75" display="inline"><mml:mrow><mml:mi mathvariant="bold-italic">R</mml:mi><mml:msub><mml:mi mathvariant="bold-italic">H</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the RAMS@ISAC vertical profile of relative humidity at a
grid point inside a square of <inline-formula><mml:math id="M76" display="inline"><mml:mrow><mml:mn mathvariant="normal">50</mml:mn><mml:mo>×</mml:mo><mml:mn mathvariant="normal">50</mml:mn></mml:mrow></mml:math></inline-formula> km<inline-formula><mml:math id="M77" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula> centred at the radar vertical
profile, <inline-formula><mml:math id="M78" display="inline"><mml:mrow><mml:msub><mml:mi>W</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the weight of each profile, and <inline-formula><mml:math id="M79" display="inline"><mml:mrow><mml:msubsup><mml:mi mathvariant="bold-italic">z</mml:mi><mml:mi mathvariant="normal">o</mml:mi><mml:mi mathvariant="normal">p</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula> is the
relative humidity pseudo-profile. The weights are determined by the
agreement between the simulated and observed reflectivity factors:
            <disp-formula id="Ch1.E3" content-type="numbered"><label>3</label><mml:math id="M80" display="block"><mml:mrow><mml:msub><mml:mi>W</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mi>exp⁡</mml:mi><mml:mfenced close="}" open="{"><mml:mrow><mml:mo>-</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mn mathvariant="normal">1</mml:mn><mml:mn mathvariant="normal">2</mml:mn></mml:mfrac></mml:mstyle><mml:msup><mml:mfenced open="[" close="]"><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">z</mml:mi><mml:mi mathvariant="normal">o</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi>h</mml:mi><mml:mi>z</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="bold">x</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:mfenced><mml:mi>T</mml:mi></mml:msup><mml:msubsup><mml:mi mathvariant="bold">R</mml:mi><mml:mi>z</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msubsup><mml:mfenced open="[" close="]"><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">z</mml:mi><mml:mi mathvariant="normal">o</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi>h</mml:mi><mml:mi>z</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="bold">x</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:mfenced></mml:mrow></mml:mfenced><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
          where <inline-formula><mml:math id="M81" display="inline"><mml:mrow><mml:msub><mml:mi>h</mml:mi><mml:mi>z</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the forward observation operator, transforming the
background column <inline-formula><mml:math id="M82" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold">x</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> into the observed reflectivity<?pagebreak page1850?> factor. The radar
forward observation operator is taken from the RIP (Read/Interpolate/Plot)
software (<uri>https://dtcenter.org/wrf-nmm/users/OnLineTutorial/NMM/RIP/index.php</uri>, last
access: 3 March 2019) and is given in the Supplement of this
paper (Sect. S8). It assumes a Marshall–Palmer hydrometeor
size distribution and Rayleigh scattering, and depends on the mixing ratios of
rain, graupel, and snow.</p>
      <p id="d1e1941">The matrix <inline-formula><mml:math id="M83" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold">R</mml:mi><mml:mi>z</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> in Eq. (3) is diagonal and its value is <inline-formula><mml:math id="M84" display="inline"><mml:mrow><mml:mi>n</mml:mi><mml:msup><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>,
where <inline-formula><mml:math id="M85" display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula> is 1 dBz and <inline-formula><mml:math id="M86" display="inline"><mml:mi>n</mml:mi></mml:math></inline-formula> is the number of available observations in the
vertical profile (from 1 to 3). In this way, we give more weight to vertical
profiles containing more data.</p>
      <p id="d1e1982">The error of radar data is assumed to be small (1 dBz) for two reasons: (a) reflectivity data are carefully checked by the Civil Protection Department;
(b) the performance of the control simulation, not assimilating any data, is
rather poor for the case studies. This setting, however, could not be
optimal for cases when the control forecast performs better. A sensitivity
test using <inline-formula><mml:math id="M87" display="inline"><mml:mrow><mml:mi mathvariant="italic">σ</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">5</mml:mn></mml:mrow></mml:math></inline-formula> dBz for the Livorno case showed small differences
compared to <inline-formula><mml:math id="M88" display="inline"><mml:mrow><mml:mi mathvariant="italic">σ</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> dBz. The results of this sensitivity test are
detailed in the Supplement of this paper (Sect. S4).</p>
      <p id="d1e2010">It is important to point out that the 50 km length scale of the above step
does not represent the horizontal correlation length scale of the background
error, which determines the horizontal spread of the innovations in the
3D-Var data assimilation (the latter length scale is between 14 and 25 km
depending on the level). The 50 km length scale is used to set a square for
computing the pseudo-profile of relative humidity (Eq. 2). This profile
is given by a weighted average whose weights are determined by the agreement
between the simulated and observed reflectivity factors. The larger the
agreement the larger the weight. This distance is appropriate because the
spatial error of meteorological models in simulating meteorological
features, for example fronts, can be of this order. The control simulation
of the two events considered in this paper confirms this choice.</p>
      <p id="d1e2013">The method is not able to force convection when the model has no rain, snow,
or graupel in a square around (<inline-formula><mml:math id="M89" display="inline"><mml:mrow><mml:mn mathvariant="normal">50</mml:mn><mml:mo>×</mml:mo><mml:mn mathvariant="normal">50</mml:mn></mml:mrow></mml:math></inline-formula> km<inline-formula><mml:math id="M90" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula>) a radar profile with a
reflectivity factor greater than zero. In this case, the pseudo-profile of
relative humidity is assumed saturated above the lifting condensation level
and with no data below (Caumont et al., 2010).</p>
      <p id="d1e2037">It is also noted that the method is able to reduce spurious convection when
the reflectivity factor is simulated but not observed because the
pseudo-profile of relative humidity gives more weight to the drier relative
humidity profiles simulated by RAMS@ISAC inside the <inline-formula><mml:math id="M91" display="inline"><mml:mrow><mml:mn mathvariant="normal">50</mml:mn><mml:mo>×</mml:mo><mml:mn mathvariant="normal">50</mml:mn></mml:mrow></mml:math></inline-formula> km<inline-formula><mml:math id="M92" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula> square
centred at the radar profile. Of course, the ability to reduce spurious
convection depends on the availability of dry model profiles around the
specific radar profile (see the example below). Finally, if the observed
profile is dry and the profile simulated by RAMS@ISAC is dry too, the
pseudo-profile is not computed.</p>
      <p id="d1e2061">In summary, pseudo-profiles are computed for each profile of the radar grid
whenever reflectivity is observed or simulated.</p>
      <p id="d1e2064">The pseudo-profiles computed with the procedure introduced above are then
used as observations in the RAMS-3DVar data assimilation (Federico, 2013),
minimizing the cost function:
            <disp-formula id="Ch1.E4" content-type="numbered"><label>4</label><mml:math id="M93" display="block"><mml:mtable class="split" rowspacing="0.2ex" columnspacing="1em" displaystyle="true" columnalign="right left"><mml:mtr><mml:mtd><mml:mrow><mml:mi>J</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="bold-italic">x</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mn mathvariant="normal">1</mml:mn><mml:mn mathvariant="normal">2</mml:mn></mml:mfrac></mml:mstyle><mml:mo>(</mml:mo><mml:mi mathvariant="bold-italic">x</mml:mi><mml:mo>-</mml:mo><mml:msub><mml:mi mathvariant="bold-italic">x</mml:mi><mml:mi mathvariant="normal">b</mml:mi></mml:msub><mml:msup><mml:mo>)</mml:mo><mml:mi>T</mml:mi></mml:msup><mml:msup><mml:mi mathvariant="bold">B</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup><mml:mo>(</mml:mo><mml:mi mathvariant="bold-italic">x</mml:mi><mml:mo>-</mml:mo><mml:msub><mml:mi mathvariant="bold-italic">x</mml:mi><mml:mi mathvariant="normal">b</mml:mi></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mo>+</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mn mathvariant="normal">1</mml:mn><mml:mn mathvariant="normal">2</mml:mn></mml:mfrac></mml:mstyle><mml:mo>(</mml:mo><mml:msubsup><mml:mi mathvariant="bold-italic">z</mml:mi><mml:mi mathvariant="normal">o</mml:mi><mml:mi mathvariant="normal">p</mml:mi></mml:msubsup><mml:mo>-</mml:mo><mml:mi>h</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="bold-italic">x</mml:mi><mml:mo>)</mml:mo><mml:msup><mml:mo>)</mml:mo><mml:mi>T</mml:mi></mml:msup><mml:msup><mml:mi mathvariant="bold">R</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup><mml:mo>(</mml:mo><mml:msubsup><mml:mi mathvariant="bold-italic">z</mml:mi><mml:mi mathvariant="normal">o</mml:mi><mml:mi mathvariant="normal">p</mml:mi></mml:msubsup><mml:mo>-</mml:mo><mml:mi>h</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="bold-italic">x</mml:mi><mml:mo>)</mml:mo><mml:mo>)</mml:mo><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:math></disp-formula>
          where <inline-formula><mml:math id="M94" display="inline"><mml:mi mathvariant="bold-italic">x</mml:mi></mml:math></inline-formula> is the state vector giving the analysis when <inline-formula><mml:math id="M95" display="inline"><mml:mi>J</mml:mi></mml:math></inline-formula> is minimized,
<inline-formula><mml:math id="M96" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">x</mml:mi><mml:mi mathvariant="normal">b</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the background, <inline-formula><mml:math id="M97" display="inline"><mml:mi mathvariant="bold">B</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M98" display="inline"><mml:mi mathvariant="bold">R</mml:mi></mml:math></inline-formula> are
the background and observation error matrices,
<inline-formula><mml:math id="M99" display="inline"><mml:mrow><mml:msubsup><mml:mi mathvariant="bold-italic">z</mml:mi><mml:mi mathvariant="normal">o</mml:mi><mml:mi mathvariant="normal">p</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula> is the pseudo-vertical-profile
computed by Eq. (2), and <inline-formula><mml:math id="M100" display="inline"><mml:mi>h</mml:mi></mml:math></inline-formula> is the forward observation operator transforming
the state vector (RAMS@ISAC water vapour mixing ratio) into observations.
The cost function in RAMS-3DVar is implemented in incremental form (Courtier
et al., 1994) and its minimization is performed by the conjugate-gradient
method (Press et al., 1992). No multi-scale approach is used.</p>
      <p id="d1e2260">The background error matrix is divided into three components along the three
spatial directions (<inline-formula><mml:math id="M101" display="inline"><mml:mrow><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>,</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula>). The <bold>B</bold><inline-formula><mml:math id="M102" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="bold-italic">x</mml:mi></mml:msub></mml:math></inline-formula> and
<inline-formula><mml:math id="M103" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold">B</mml:mi><mml:mi mathvariant="bold-italic">y</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> matrices account for the spatial correlation of
the background error. The correlations are Gaussian with length scales
between 14 and 25 km, depending on the vertical level. These distances are
computed using the National Meteorological Center (NMC) method (Barker et al., 2012) applied to the
HyMeX-SOP1 period. It is again stressed that the spread of the innovations
along the horizontal spatial directions in the 3D-Var analysis is determined
by the length scales of <inline-formula><mml:math id="M104" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold">B</mml:mi><mml:mi mathvariant="bold-italic">x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and
<inline-formula><mml:math id="M105" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold">B</mml:mi><mml:mi mathvariant="bold-italic">y</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> matrices.</p>
      <p id="d1e2324">The <inline-formula><mml:math id="M106" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold">B</mml:mi><mml:mi mathvariant="bold-italic">z</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> matrix contains the error for the water vapour mixing ratio,
which is the control variable used in RAMS-3DVar. This error is about 2 g kg<inline-formula><mml:math id="M107" 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>
at the surface and decreases with height. In particular, it is larger than
0.5 g kg<inline-formula><mml:math id="M108" 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> below 4 km, and less than 0.2 g kg<inline-formula><mml:math id="M109" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> above 5 km. The vertical
decorrelation of the background error depends on the level and can be
roughly estimated to be 500–2000 m. The observation error matrix <inline-formula><mml:math id="M110" display="inline"><mml:mi mathvariant="bold">R</mml:mi></mml:math></inline-formula> in Eq. (4) is diagonal and observation errors are uncorrelated. This choice
is partially justified due to the sampling of radar reflectivity factor
observation by choosing one point every five grid points in both horizontal
directions of the radar Cartesian grid. However, correlation observation
errors have a significant impact on the final analysis, as shown for example
in Stewart et al. (2013), and different choices of the matrix <inline-formula><mml:math id="M111" display="inline"><mml:mi mathvariant="bold">R</mml:mi></mml:math></inline-formula> will be considered in future studies.</p>
      <?pagebreak page1851?><p id="d1e2389">The value of the elements on the diagonal of <inline-formula><mml:math id="M112" display="inline"><mml:mi mathvariant="bold">R</mml:mi></mml:math></inline-formula> depends on the
vertical level and is one-fourth of the diagonal element of the
<inline-formula><mml:math id="M113" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold">B</mml:mi><mml:mi mathvariant="bold-italic">z</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> matrix at the corresponding height. With these
settings, larger weights are given to the observations than to the
background, and analyses strongly adjust the background towards observations.
<inline-formula><mml:math id="M114" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold">B</mml:mi><mml:mi mathvariant="bold-italic">z</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> matrix is computed using the NMC method (Parrish
and Derber, 1992; Barker et al., 2004) applied to HyMeX-SOP1; this choice
is motivated by the fact that HyMeX-SOP1 contains several heavy
precipitation events over Italy and the background error matrix is
representative of the convective environment of the cases considered in this
paper. In particular, 10 out of 20 declared IOPs (intense observing periods)
of HyMeX-SOP1 occurred in Italy (Ferretti et al., 2014). In contrast, the
period of September 2017, especially before the events selected in this
study, was characterized by fair and stable weather conditions over Italy and
the background error matrix for September 2017 is less representative of the
convective environment that characterizes the events of this paper.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F14"><?xmltex \currentcnt{14}?><label>Figure 14</label><caption><p id="d1e2423"><bold>(a)</bold> RAMS@ISAC reflectivity factor simulated 3 km above sea level
at 06:00 UTC on 10 September 2017; <bold>(b)</bold> relative humidity difference between the
analysis and the background at 06:00 UTC at the 3.2 km level in the terrain
following the vertical coordinate of RAMS@ISAC.</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/19/1839/2019/nhess-19-1839-2019-f14.jpg"/>

        </fig>

      <p id="d1e2437">Because it is the first time that we show the assimilation of radar
reflectivity factor in RAMS@ISAC, it is useful to discuss an example of
analysis. We select the analysis of the Livorno case study at 06:00 UTC. The
observed CAPPI at 3 km above sea level is shown in Fig. 10b. The
corresponding CAPPI simulated by the background is shown in Fig. 14a. In
general, the comparison between simulated and observed reflectivity factor
highlights the difficulty of the model to represent convection properly. In
particular, the model is able to represent the convection over northern
Italy but it has poor performance over Sardinia, south of Sicily, and over
central Italy. The difference between the analysis and background relative
humidity after and before the analysis is shown in Fig. 14b (absolute
values less than 1 % are suppressed in the figure for clarity). Both
positive (convection enhancing) and negative (convection suppressing)
adjustments are found. Over central Italy, Sardinia, and south of Sicily
relative humidity is increased because the model does not simulate the
observed reflectivity (Fig. 10b). The occurrence of this condition added
most of the water vapour to the RAMS@ISAC simulations for the case studies
of this paper. Over northern Italy the model is partially dried for two
different reasons: in the northwest of Italy because RAMS@ISAC simulates
unobserved reflectivity, in the north and northeast of Italy because the
model simulates larger values of reflectivity factor compared to the
observations. The RAMS-3DVar reduces the relative humidity field north from
Corsica island, where the RAMS@ISAC predicted unobserved reflectivity, while
RAMS-3DVar did not suppress the unobserved convection west of Sardinia
because the pseudo-profiles computed over this area were not appreciably
drier than the background.</p>
      <p id="d1e2440">Cross correlations among different variables of the data assimilation system
are neglected in this study and the application of RAMS-3DVar affects
the water vapour mixing ratio only. Cross correlations among different
variables can improve the performance of the data assimilation system, and an
example of their impact in RAMS-3DVar is shown in Federico (2013).
Nevertheless, the impact of cross correlations among different variables in
the precipitation VSF will be explored in future works.</p>
      <p id="d1e2444">Since lightning data assimilation also adjusts the water vapour mixing
ratio, it follows that the data assimilation presented in this study adjusts
only this parameter.</p>
      <p id="d1e2447">Despite the fact that both radar reflectivity factor and lightning adjust
the water vapour mixing ratio, different impacts on the VSF can be expected a priori
because radar reflectivity factor and lightning are different types of
observations and because they are used in different ways in the data
assimilation system.</p>
      <p id="d1e2450">In particular, lightning is recorded when deep convection develops, while
radar reflectivity factor is observed also for light stratiform rain.
Flashes of ground-based networks, such as LINET, are available over the open sea,
even if with a reduced detection efficiency, while radar reflectivity factor
is confined to the range of coastal radars in the network.<?pagebreak page1852?> Lightning has a
seasonal dependence over Italy, with the maximum in summer and autumn, while
radar reflectivity factor is available in all seasons.</p>
      <p id="d1e2453">Also, differences in data assimilation of lightning and radar reflectivity
factor play a role. In addition to the methods used to assimilate
observations, lightning saturates the layer from 0 <inline-formula><mml:math id="M115" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C to <inline-formula><mml:math id="M116" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">25</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M117" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C
where and when it is detected, while radar reflectivity factor can be
assimilated by pseudo-profiles or by saturation above the lifting
condensation level where observed reflectivity is greater than zero.</p>
      <p id="d1e2484">Therefore, despite both observations adjusting the same model prognostic
variable, which is a drawback of the methodology presented in this paper,
the impacts of lightning and radar reflectivity factor is expected to be
different as will be evident from the results of this paper.</p>
      <p id="d1e2487">There are, however, advantages using the methodology of this paper. In
addition to being simple, it does not rely on approximate relationship
between radar reflectivity factor and hydrometeor mixing ratio, leaving to
the model the task of evolving the water vapour added and subtracted. Also, the
impact of the data assimilation on model results is substantial (Fabry and
Sun, 2010; Caumont et al., 2010), as also shown by the results of this
paper.</p>
      <p id="d1e2491">Lightning and radar data assimilation may produce sharp gradients in the
vertical direction caused by the addition of water vapour to specific
layers. In the case of lightning, the water vapour is added by nudging to
reduce sharp gradients. However, radar data assimilation, which accounts for
the largest mass of water added to RAMS@ISAC (see Sect. S2), directly adjusts the water vapour into the model.
Our experience with RAMS@ISAC, however, shows that results are reliable and
the sudden addition of water vapour does not cause shocks to the model
simulation, despite the notable gradients of specific humidity.</p>
      <p id="d1e2494">It is finally noted that the data assimilation increases or decreases the water
vapour in the model depending on the cases. The eventual increase or decrease
in the forecasted rainfall depends on the physical and dynamical processes
occurring in the meteorological model, without any specific tuning.</p>
</sec>
</sec>
<sec id="Ch1.S4">
  <label>4</label><title>Results</title>
      <p id="d1e2506">In this section, we discuss the most intense phase of the Serrano case, 03:00–06:00 UTC on 16 September, and two VSFs forecasts, 00:00–03:00 UTC and 06:00–09:00 UTC on 10 September, for the Livorno case. The two VSF for Livorno correspond to the
most intense phase of the storm in Livorno and to a very intense phase over the
Lazio region, central Italy. The aim of the section is to show the notable
improvement given by lightning and radar reflectivity factor data
assimilation to the VSF.</p>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T3" specific-use="star"><?xmltex \currentcnt{3}?><label>Table 3</label><caption><p id="d1e2512">Types of simulations performed.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="4">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="justify" colwidth="142.26378pt"/>
     <oasis:colspec colnum="3" colname="col3" align="justify" colwidth="165.025984pt"/>
     <oasis:colspec colnum="4" colname="col4" align="justify" colwidth="93.894094pt"/>
     <oasis:thead>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">Experiment</oasis:entry>
         <oasis:entry colname="col2">Description</oasis:entry>
         <oasis:entry colname="col3">Data assimilated</oasis:entry>
         <oasis:entry colname="col4">Model variable impacted</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">CTRL</oasis:entry>
         <oasis:entry colname="col2">Control run</oasis:entry>
         <oasis:entry colname="col3">None</oasis:entry>
         <oasis:entry colname="col4">None</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">RAD</oasis:entry>
         <oasis:entry colname="col2">Radar data assimilation</oasis:entry>
         <oasis:entry colname="col3">Reflectivity factor CAPPI (RAMS-3DVar)</oasis:entry>
         <oasis:entry colname="col4">Water vapour mixing ratio</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">LIGHT</oasis:entry>
         <oasis:entry colname="col2">Lightning data assimilation <?xmltex \hack{\hfill\break}?>(<inline-formula><mml:math id="M118" display="inline"><mml:mrow><mml:mi>A</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.85</mml:mn></mml:mrow></mml:math></inline-formula>; <inline-formula><mml:math id="M119" display="inline"><mml:mrow><mml:mi>B</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.16</mml:mn></mml:mrow></mml:math></inline-formula> in Eq. 1)</oasis:entry>
         <oasis:entry colname="col3">Lightning density (nudging)</oasis:entry>
         <oasis:entry colname="col4">Water vapour mixing ratio</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">RADLI</oasis:entry>
         <oasis:entry colname="col2">Radar <inline-formula><mml:math id="M120" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> lightning data assimilation (<inline-formula><mml:math id="M121" display="inline"><mml:mrow><mml:mi>A</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.86</mml:mn></mml:mrow></mml:math></inline-formula>; <inline-formula><mml:math id="M122" display="inline"><mml:mrow><mml:mi>B</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.15</mml:mn></mml:mrow></mml:math></inline-formula> in Eq. 1)</oasis:entry>
         <oasis:entry colname="col3">Reflectivity factor CAPPI (RAMS-3D-Var) <inline-formula><mml:math id="M123" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> lightning density (nudging)</oasis:entry>
         <oasis:entry colname="col4">Water vapour mixing ratio</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table></table-wrap>

      <p id="d1e2674">We consider four types of VSF (Table 3): (a) CTRL, without radar reflectivity
factor or lightning data assimilation; (b) LIGHT, assimilating lightning but
not radar reflectivity factor; (c) RAD, assimilating radar reflectivity
factor but not lightning; and (d) RADLI, assimilating both lightning and radar
reflectivity factor.</p>
      <p id="d1e2678">Several aspects of lightning and radar reflectivity factor data assimilation
are considered in the Supplement  of this paper: (a) the relative
contribution to the total water mass given by lightning and radar
reflectivity factor data assimilation (Sect. S2); (b) the sensitivity of
the precipitation VSF to the nudging formulation (Sect. S3); (c) the
sensitivity of rainfall VSF to two specific aspects of radar reflectivity
factor data assimilation (Sect. S4); (d) the sensitivity of rainfall VSF to the
RAMS@ISAC setting (Sect. S5); (e) the impact of lightning data assimilation
for a case study well predicted by the control forecast (Sect. S6); (f) different plots of Figs. 15–17 (Sect. S7), and (g) the radar forward
operator used in RAMS-3DVar (Sect. S8).</p>

      <?xmltex \floatpos{p}?><fig id="Ch1.F15" specific-use="star"><?xmltex \currentcnt{15}?><label>Figure 15</label><caption><p id="d1e2683"><bold>(a)</bold> Rainfall reported by rain gauges between 03:00 and 06:00 UTC on 16 September 2017. Only rain gauges observing at least 0.2 mm every 3 h are shown. The
first number in the title within brackets represents the available
rain gauges, while the second number represents those observing at least 0.2 mm every 3 h; <bold>(b)</bold> rainfall VSF of CTRL for the same time interval as in <bold>(a)</bold>; <bold>(c)</bold> as in
<bold>(b)</bold> for RAD forecast; <bold>(d)</bold> as in <bold>(b)</bold> for LIGHT forecast; <bold>(e)</bold> as in <bold>(b)</bold> for RADLI
forecast; <bold>(f)</bold> performance diagram: black symbols are for the nearest
neighbourhood and for the 1 mm every 3 h threshold; red symbols are for the nearest
neighbourhood and for the 30 mm every 3 h threshold; blue symbols are for the 25 km
neighbourhood radii and for the 1 mm every 3 h threshold; green symbols are for the 25 km
neighbourhood radii and for the 30 mm every 3 h threshold.</p></caption>
        <?xmltex \igopts{width=497.923228pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/19/1839/2019/nhess-19-1839-2019-f15.jpg"/>

      </fig>

<sec id="Ch1.S4.SS1">
  <label>4.1</label><?xmltex \opttitle{Serrano: 03:00--06:00\,UTC on 16 September 2017}?><title>Serrano: 03:00–06:00 UTC on 16 September 2017</title>
      <p id="d1e2730">In this period, an intense and localized storm hit central Italy, while
light precipitation occurred over northern Italy (Fig. 15a). Considering
the storm over central Italy, 10 rain gauges observed more than 30 mm every 3 h, six
more than 40 mm every 3 h, three more than 50 mm every 3 h, and one more than 60 mm every 3 h, the
maximum observed value being 63 mm every 3 h.</p>
      <p id="d1e2733">The CTRL forecast, Fig. 15b, misses the rainfall over central Italy and
considerably underestimates the precipitation area over northern Italy,
giving unsatisfactory results.</p>
      <p id="d1e2736">The assimilation of the radar reflectivity factor improves the forecast, as
shown in Fig. 15c. In particular, RAD forecast shows localized
precipitation (30–35 mm every 3 h) close to the area were the most abundant
precipitation was observed. Maximum precipitation is underestimated. Also,
the RAD forecast better represents the precipitation over northern Italy
compared to CTRL.</p>
      <p id="d1e2740">The rainfall forecast of LIGHT, Fig. 15d, shows some improvements compared
to CTRL because the precipitation over central Italy has a maximum of 25–30 mm every 3 h, close to the area where the maximum precipitation was observed.
LIGHT; however, it has a worse performance compared to RAD because it
underestimates the precipitation area over northern Italy. LIGHT
underestimates the maximum precipitation in central Italy.</p>
      <p id="d1e2743">The RADLI forecast, Fig. 15e, has the best performance. The precipitation
over central Italy is well represented because the maximum rainfall (40–45 mm every 3 h) is in reasonable agreement with observations, and also because the
area of intense precipitation (<inline-formula><mml:math id="M124" display="inline"><mml:mrow><mml:mi mathvariant="italic">&gt;</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mn mathvariant="normal">25</mml:mn></mml:mrow></mml:math></inline-formula> mm every 3 h) is elongated in the
SW–NE direction in agreement with rain gauge observations. The precipitation
over northern Italy is well represented by RADLI.</p>
      <?pagebreak page1854?><p id="d1e2757">A performance diagram for 1 mm every 3 h and 30 mm every 3 h and for 4 and 25 km
neighbourhood radii is shown in Fig. 15f. Different radii are considered
to account for the well-known double penalty error (Mass et al., 2002;
Mittermaier et al., 2013) caused by displacement errors of the detailed
precipitation forecast in convection-allowing grids. RADLI has the best
performance thanks to the synergistic contribution of lightning and radar
reflectivity factor data assimilation.</p>
</sec>
<sec id="Ch1.S4.SS2">
  <label>4.2</label><title>Livorno</title>
      <p id="d1e2768">The Livorno case study lasted for several hours starting at 18:00 UTC on 9 September 2017 and ending more than a day later. The most intense phase in
Livorno and its surroundings was observed during the night between 9 and 10 September. In the following, we will show two representative VSFs (3 h),
including the most intense phase in Livorno.</p>

      <?xmltex \floatpos{p}?><fig id="Ch1.F16" specific-use="star"><?xmltex \currentcnt{16}?><label>Figure 16</label><caption><p id="d1e2773"><bold>(a)</bold> Rainfall reported by rain gauges between 00:00 and 03:00 UTC on 10 September 2017. Only stations reporting at least 0.2 mm every 3 h are shown. The
first number in the title within brackets represents the number of
rain gauges available over the domain, while the second number shows those
observing at least 0.2 mm every 3 h; <bold>(b)</bold> rainfall VSF of CTRL for the same time
interval as in <bold>(a)</bold>; <bold>(c)</bold> as in <bold>(b)</bold> for the RAD forecast; <bold>(d)</bold> as in <bold>(b)</bold> for the LIGHT
forecast; <bold>(e)</bold> as in <bold>(b)</bold> for the RADLI forecast. Labels A and B help to identify
the positions of two rainfall maxima discussed in the text; <bold>(f)</bold> performance
diagram: black symbols are for the nearest neighbourhood and for the 1 mm every 3 h
threshold; red symbols are for the nearest neighbourhood and for the 30 mm every 3 h
threshold; blue symbols are for the 25 km neighbourhood radii and for the 1 mm every 3 h
threshold; green symbols are for the 25 km neighbourhood radii and for the 30 mm every 3 h
threshold.</p></caption>
          <?xmltex \igopts{width=455.244094pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/19/1839/2019/nhess-19-1839-2019-f16.jpg"/>

        </fig>

<sec id="Ch1.S4.SS2.SSS1">
  <label>4.2.1</label><?xmltex \opttitle{Livorno: 00:00--03:00\,UTC on 10 September 2017}?><title>Livorno: 00:00–03:00 UTC on 10 September 2017</title>
      <p id="d1e2820">This period represents the most intense phase of the storm in Livorno. In
particular, the rain gauge close to the label A (Fig. 16a) reported 151 mm every 3 h (Collesalvetti), while the one close to the label B measured 82 mm every 3 h.
Among the 518 rain gauges reporting valid data, 75 observed more than 10 mm every 3 h, 31 more than 20 mm every 3 h, 17 more than 30 mm every 3 h, 9 more than 40 mm every 3 h,
and 6 more than 50 mm every 3 h.</p>
      <p id="d1e2823">The CTRL precipitation forecast is shown in Fig. 16b. The forecast is poor
because it misses the precipitation swath from the coast towards NE. A
precipitation swath is forecasted about 50 km to the north of the real
occurrence, but it is less wide compared to the observations.</p>
      <p id="d1e2826">The RAD forecast, Fig. 16c, shows that the assimilation of radar
reflectivity factor gives a clear improvement of the forecast. The largest
precipitation in the coastal part of the swath (we searched for the maximum
in the area with longitudes between 10.20  and 10.70<inline-formula><mml:math id="M125" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E and latitudes between
43.10  and 43.60<inline-formula><mml:math id="M126" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N) is 94 mm every 3 h. Another local maximum is in the southern
part of the domain (label B of Fig. 16a). The location of this maximum is
well represented, but the forecasted value (55 mm every 3 h) underestimated the
observed maximum (82 mm every 3 h).</p>
      <p id="d1e2848">An improvement, compared to both CTRL and RAD, is given by the assimilation
of lightning (Fig. 16d). The maximum value close to Livorno, i.e. in the
coastal part of the swath, is 158 mm every 3 h.</p>
      <p id="d1e2851">The LIGHT simulation shows the local maximum in the southern part of the domain
(about 50 mm every 3 h), but the amount is underestimated.</p>
      <p id="d1e2854">Figure 16e shows the RADLI rainfall forecast. The precipitation swath from
coastal Tuscany towards the NE is more intense compared to LIGHT and RAD. The
maximum rainfall accumulated close to Livorno is 186 mm every 3 h. Also, the second
precipitation maximum in the southern part of the domain reaches 70 mm every 3 h in
good agreement with observations (82 mm every 3 h). RADLI is the only run giving a
satisfactory precipitation VSF over southeastern Emilia Romagna
(northeastern part of the domain), to the lee of the Apennines. It is also
noted that the main precipitation swath forecasted by RADLI is too broad in
the direction crossing the swath compared to the observations. This is
confirmed by the FBIAS of RADLI (not shown), which is more than 3 for
thresholds larger than 42 mm every 3 h.</p>
      <p id="d1e2857">The performance diagram (Fig. 16f) shows that LIGHT has better scores than
RAD for this VSF.</p>
</sec>
<sec id="Ch1.S4.SS2.SSS2">
  <label>4.2.2</label><?xmltex \opttitle{Livorno: 06:00--09:00\,UTC on 10 September 2017}?><title>Livorno: 06:00–09:00 UTC on 10 September 2017</title>
      <p id="d1e2870">In this period, the most intense precipitation occurred over the coastal
part of Lazio (Fig. 17a). In more detail, among the 2695 rain gauges
reporting valid data over the domain of Fig. 17a, 307 reported more than
10 mm every 3 h, 132 more than 20 mm every 3 h, 86 more than 30 mm every 3 h, 66 more than 40
mm every 3 h, 49 more than 50 mm every 3 h, and 35 more than 60 mm every 3 h. Among the 35
rain gauges measuring more than 60 mm every 3 h, 33 were over Lazio, showing the
heavy rainfall that occurred over the region.</p>

      <?xmltex \floatpos{p}?><fig id="Ch1.F17" specific-use="star"><?xmltex \currentcnt{17}?><label>Figure 17</label><caption><p id="d1e2875"><bold>(a)</bold> Rainfall reported by rain gauges between 06:00 and 09:00 UTC on 10 September 2017. For this time period 2695 rain gauges reported valid
observations in the domain. However only stations reporting at least 0.2 mm every 3 h are shown The first number in the title within brackets represents the
number of rain gauges available over the domain, while the second number
shows those observing at least 0.2 mm every 3 h; <bold>(b)</bold> rainfall VSF of CTRL in the
same time interval as <bold>(a)</bold>; <bold>(c)</bold> as in <bold>(b)</bold> for the RAD forecast; <bold>(d)</bold> as in <bold>(b)</bold> for the
LIGHT forecast; <bold>(e)</bold> as in <bold>(b)</bold> for the RADLI forecast; <bold>(f)</bold> performance diagram:
black symbols are for the nearest neighbourhood and for the 1 mm every 3 h threshold;
red symbols are for the nearest neighbourhood and for the 30 mm every 3 h threshold;
blue symbols are for 25 km neighbourhood radii and for the 1 mm every 3 h threshold;
green symbols are for 25 km neighbourhood radii and for the 30 mm every 3 h threshold.</p></caption>
            <?xmltex \igopts{width=455.244094pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/19/1839/2019/nhess-19-1839-2019-f17.jpg"/>

          </fig>

      <p id="d1e2914">Some precipitation persisted over Tuscany but the rainfall is much lower
compared to the previous 6 h (the rainfall over Tuscany between 03:00 and 06:00 UTC was
very intense, not shown).</p>
      <?pagebreak page1857?><p id="d1e2918">Figure 17b shows the rainfall simulated by CTRL. The forecast is
unsatisfactory, mainly for the following two reasons: (a) heavy precipitation
is simulated over Tuscany (<inline-formula><mml:math id="M127" display="inline"><mml:mrow><mml:mi mathvariant="italic">&gt;</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mn mathvariant="normal">75</mml:mn></mml:mrow></mml:math></inline-formula> mm every 3 h), also close to the Livorno
area; (b) precipitation is missed over central Italy. The rainfall over the NE of
Italy is well represented in space, but overestimated.</p>
      <p id="d1e2932">Considering the evolution of the CTRL forecast for the two VSFs of Livorno, we
conclude that it was able to predict abundant rain over Livorno, but the
rainfall forecast was delayed compared to the real occurrence. A similar
behaviour was found in Ricciardelli et al. (2018) using the WRF model,
showing that the results of this paper for Livorno are likely not tied to
the specific model used.</p>
      <p id="d1e2935">The rainfall simulated by RAD (Fig. 17c) clearly improves the forecast
compared to CTRL. First, the precipitation over Lazio is well predicted.
Second, the precipitation over Tuscany is less than for CTRL, showing the
ability of radar reflectivity factor data assimilation to dry the model when
it predicts reflectivity that is not observed. It is noted, however, that
the area of intense rainfall (<inline-formula><mml:math id="M128" display="inline"><mml:mrow><mml:mi mathvariant="italic">&gt;</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mn mathvariant="normal">60</mml:mn></mml:mrow></mml:math></inline-formula> mm every 3 h) is overestimated by
RAD, which has a wet forecast. The wet bias of the RAD forecast is apparent
in the representation of the rainfall VSF shown in the Supplement
of this paper (Fig. S12).</p>
      <p id="d1e2949">The LIGHT forecast, Fig. 17d, shows a worse performance compared to RAD for
this time period. The precipitation forecast is mainly over Tuscany, where
it is overestimated, with a small precipitation spot over Lazio.</p>
      <p id="d1e2952">The precipitation forecast of RADLI, Fig. 17e, represents the
precipitation over Lazio very well, and the rainfall amount is better predicted
compared to RAD. The precipitation over Sardinia is well represented by
RADLI as well as the precipitation over the central Alps, giving the best
results among all VSFs.</p>
      <p id="d1e2955">Figure 17f shows the better performance of RAD compared to LIGHT for this
precipitation VSF. RADLI has the best performance and is closer to the upper
right corner of the diagram.</p>
      <p id="d1e2959">To better understand the changes of the precipitation VSF for different data
assimilation set-ups, Fig. 18 shows maps of water vapour mixing ratio
averaged between 3 and 10 km at the end of the assimilation phase (06:00 UTC on
10 September 2017). It is important to note that those maps contain the
effects of both data assimilation and model evolution.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F18" specific-use="star"><?xmltex \currentcnt{18}?><label>Figure 18</label><caption><p id="d1e2964">Water vapour mixing ratio averaged between 3 and 10 km at 06:00 UTC
on 10 September 2017 for <bold>(a)</bold> CTRL, <bold>(b)</bold> RAD, <bold>(c)</bold> LIGHT, and <bold>(d)</bold> RADLI.</p></caption>
            <?xmltex \igopts{width=426.791339pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/19/1839/2019/nhess-19-1839-2019-f18.jpg"/>

          </fig>

      <p id="d1e2985">The comparison between CTRL (Fig. 18a) and RAD (Fig. 18b) shows that RAD
has a line of high water vapour values over central Italy, extending over
the Tyrrhenian Sea and Sardinia, which is not simulated by CTRL. This line
results from both radar data assimilation and convection, which transports
water vapour from lower to upper levels. The comparison between CTRL and RAD
shows the substantial impact of radar reflectivity factor data assimilation
on the model evolution despite not using the relationship between
hydrometeor mixing ratios and radar reflectivity factor in data
assimilation.</p>
      <p id="d1e2988">LIGHT averaged water vapour (Fig. 18c) over the Tyrrhenian Sea and west of
Sicily is higher compared to CTRL because of lightning data assimilation and
model processes. Convection develops over Tuscany, northern Lazio, and NE of
Italy, causing the increase in averaged water vapour in those areas.</p>
      <p id="d1e2991">Because RAD and LIGHT both assimilate water vapour it is important to
highlight the differences between the two fields. First, LIGHT it is not
able to represent a compact line of high water vapour over central Italy
that, in the following hours, caused high precipitation over Lazio. Second,
averaged water vapour simulated by RAD is larger than for LIGHT over central
Italy, which is caused by deeper convection developing in RAD than in LIGHT,
as well as by the different contributions of data assimilation. Finally,
RADLI (Fig. 18d) is similar to RAD but it also shares features with LIGHT such
as the increase in water vapour over the Tyrrhenian Sea.</p>
      <p id="d1e2995">It is also interesting to compare vertical cross sections of relative
humidity for different data assimilation set-ups. Figure 19 show the
longitude-height cross sections of relative humidity from different data
assimilation configurations.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F19" specific-use="star"><?xmltex \currentcnt{19}?><label>Figure 19</label><caption><p id="d1e3000">Relative humidity longitude–height cross section at 42<inline-formula><mml:math id="M129" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N and at 06:00 UTC on 10 September 2017 for <bold>(a)</bold> CTRL, <bold>(b)</bold> RAD, <bold>(c)</bold> LIGHT, and <bold>(d)</bold> RADLI. Only the longitude range between 5  and 17<inline-formula><mml:math id="M130" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E and the vertical range
between 0 and 10 km are shown for clarity.</p></caption>
            <?xmltex \igopts{width=426.791339pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/19/1839/2019/nhess-19-1839-2019-f19.jpg"/>

          </fig>

      <p id="d1e3040">Comparing RAD and CTRL the difference of the relative
humidity field over the Tyrrhenian Sea and western part of Italy is evident (more
specifically at longitudes between 10.5 and 12.5).</p>
      <p id="d1e3043">LIGHT shows two areas with high relative humidity: west of Corsica and over
the Tyrrhenian Sea. The wet area west of Corsica is caused by the
assimilation of lightning (Fig. 8b) and it is not simulated by RAD because
Corsica is not well sampled by the radar network and because of different
model evolutions. Lightning data assimilation also increases the humidity
over the Tyrrhenian Sea and over the western part of Italy, as shown by the
comparison with CTRL; nevertheless its effect is lower compared to radar
reflectivity factor data assimilation.</p>
      <p id="d1e3046">RADLI has features of both lightning and radar reflectivity factor data
assimilation.</p>
      <p id="d1e3050">So, considering the results of Figs. 18 and 19 as well as the rainfall VSF,
the impact of lightning and radar reflectivity factors on the VSF can be very
different despite both adjusting the water vapour mixing ratio.</p>
</sec>
</sec>
</sec>
<sec id="Ch1.S5" sec-type="conclusions">
  <label>5</label><title>Discussion and conclusions</title>
      <p id="d1e3064">In this paper, we showed the impact of lightning and radar reflectivity
factor data assimilation on the very short-term precipitation forecast (3 h)
for two case studies that occurred in Italy. We used the RAMS@ISAC model, whose 3D-Var
extension to the assimilation of radar reflectivity factor is shown in this
paper for the first time.</p>
      <p id="d1e3067">The first case study occurred on 16 September 2017 and it is a moderate case
with localized rainfall over central Italy. It was chosen because the
control forecast, i.e. without radar reflectivity factor or lightning data
assimilation, missed the event. The second event, occurring on 9–10 September 2017, was characterized by exceptional rainfall over several parts<?pagebreak page1858?> of Italy.
This event was partially represented by the control forecast. In particular,
the forecast of the event was incorrect because (a) the control forecast was
delayed compared to the observations and (b) the control forecast missed the
rainfall over central Italy (Lazio Region).</p>
      <p id="d1e3070">It is important to recall that the impact of the lightning data assimilation
on the precipitation forecast of RAMS@ISAC was already studied for the
HyMeX-SOP1 period (Federico et al., 2017a,  b), and a robust statistic is
already available. The results of this study confirm the important role of
the lightning data assimilation on the rainfall forecast for the other two case
studies. However, considering the assimilation of radar reflectivity factor,
and its combination with lightning data assimilation in RAMS@ISAC, the
results of this paper are new.</p>
      <p id="d1e3073">Because we analysed only two case studies, no definitive conclusions can be
derived on the performance of RAMS@ISAC with radar reflectivity factor data
assimilation. There are, however, a few points worth mentioning.</p>
      <p id="d1e3077">The VSF performance of RAMS@ISAC is systematically improved by the
assimilation of radar reflectivity factor. This improvement is of paramount
importance for some specific VSFs (for example for the 00:00–03:00 UTC of Livorno),
when the control forecast missed the event while it was correctly predicted
by radar reflectivity factor data assimilation. Sometimes the improvement of
reflectivity factor data assimilation has a small impact on the precipitation
forecast, as for the period 18:00–21:00 UTC on 9 September 2017 (Livorno, not
shown; see the discussion paper Federico et al. (2018) for a description of
this VSF). This suggests that there is room<?pagebreak page1859?> for improvement for all
components of the VSF: observations, data assimilation, and meteorological
model.</p>
      <p id="d1e3080">Lightning and radar observations are different and both add value to the
VSF. Some examples have been shown: the light precipitation over northern
Italy for Serrano forecasted assimilating radar reflectivity factor well,
while it does not simulate assimilating flashes because they are too few in
this area to force convection; lightning data assimilation represents
the deep convection occurring during the intense phase of the Livorno case better
(00:00–03:00 UTC), especially because it is able to force convection where it
occurs, reducing false alarms. The ability of lightning data assimilation to
reduce false alarms compared to RAD and RADLI is shown by the fact that
the ETS score for LIGHT is sometimes the best among all simulations (see
also Sect. S2). These
results also show that the influence of different observations depends on
the meteorological situation.</p>
      <p id="d1e3083">The model configuration assimilating both radar reflectivity factor and
lightning (RADLI) is able to retain important features of both data
assimilations. For example, the simulation of the Livorno case in the phase
06:00–09:00 UTC was able to simulate the heavy precipitation over Lazio thanks to
the radar reflectivity factor data assimilation and the precipitation over
Sardinia, as well as the moderate precipitation over the central Alps, thanks to
lightning data assimilation.</p>
      <p id="d1e3086">The property of RADLI to retain the precipitation features of both RAD and
LIGHT is shown by the POD score, which is the best, for most cases and
thresholds, for RADLI.</p>
      <p id="d1e3089">Another interesting feature is the considerable improvement of the POD of
RADLI compared to CTRL for the lowest thresholds.</p>
      <p id="d1e3092">It is also underlined that the data assimilated, both lightning and radar
reflectivity factor, are available in real time and could be used for an
operational implementation of the VSF.</p>
      <p id="d1e3096">It is worth noting that several sensitivity tests were conducted for the
case studies, whose results are shown in the Supplement. In
particular, we studied the sensitivity of the rainfall VSF to (a) nudging
formulation used for lightning data assimilation, (b) increasing the
observation error of<?pagebreak page1860?> radar reflectivity factor, (c) changing the shape of the
searching area to compute the relative humidity pseudo-profiles, (d) updating
initial and boundary conditions (IC and BC) as new observations are available, and (e) increasing the vertical
resolution of RAMS@ISAC by using 42 vertical levels. All these sensitivity
tests confirm the findings of this paper.</p>
      <p id="d1e3099">The above results are promising and deserve future studies to better
understand the role of radar reflectivity factor data assimilation and its
interaction with lightning data assimilation to improve the precipitation
forecast, especially at the very short range (0–3 h).</p>
      <p id="d1e3102">There are, however, less satisfactory aspects of assimilating both radar
reflectivity factor and lightning data. In particular, the wet bias of RAD
and RADLI forecast is the main drawback of the results of this paper. To
reduce the moisture added by radar and lightning data assimilation, further
research is needed and different approaches are possible (Fierro et al.,
2016). In particular, (a) assimilating for a shorter time (0–6 h in this
paper), (b) reducing the length scales of the 3D-Var in the horizontal
directions to limit the spreading of the innovations, or assuming an
innovation equal to zero for grid points without lightning and with zero
reflectivity factor, (c) reducing the amount of water vapour added to the
model (for example reducing the values of A and B constants for lightning
data assimilation or relaxing the request of saturation when radar
reflectivity is observed in areas where the model has zero reflectivity), and (d) adding moisture to a shallower vertical layer are options.</p>
      <p id="d1e3105">It is also noted that a combination of heating and moistening could provide
the same buoyancy with less water vapour addition (Marchand and Fuelberg,
2014) and this approach could be used in future studies.</p>
      <p id="d1e3108">In addition to the acquisition of more case studies, there are two
directions of future development of this work. The lightning data
assimilation can be formulated by 3D-Var, using a strategy similar to the
radar reflectivity factor in which pseudo-profiles of relative humidity are
first generated where flashes are recorded and then assimilated by 3D-Var.
This methodology was already reported in Fierro et al. (2016). The
assimilation of both radar reflectivity factor and lightning using
RAMS-3DVar will be explored in future studies.</p>
      <p id="d1e3111">Another important point to study is how long the innovations introduced by
data assimilation last in the forecast. While in this study we consider the
VSF at 3 h, future studies must explore longer time ranges. This kind of
study was performed for lightning data assimilation (Fierro et al., 2015;
Federico et al., 2017b; Lynn et al., 2015, among others) and for radar data
assimilation (Hu et al., 2006; Jones et al., 2014, among others), using a
rationale similar to that used in this paper.</p>
      <p id="d1e3115">In general, the performance of the forecast and the impact of lightning and
radar data assimilation decrease with forecast range because boundary
conditions propagate inside the domain and because model errors grow and
eventually become dominant. Improving the data assimilation system also
contributes to a longer resilience of model performance. The studies cited
above showed that lightning and radar data assimilation can have an impact
up to 24 h depending on several factors (meteorological model, data
assimilation, quality of the data, meteorological conditions, initial and
boundary conditions).</p>
      <p id="d1e3118">A study considering both radar reflectivity factor and lightning should be
performed to understand the resilience of the innovations introduced by data
assimilation.</p>
</sec>

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

      <p id="d1e3125">The output of the RAMS@ISAC model and RAMS-3DVar are available upon request to the corresponding author. Radar and rain gauge data can be requested from the Department of Civil Protection (see the authors addresses). LINET data  can be requested from Nowcast (<uri>https://www.nowcast.de</uri>, nowcast, 2019).</p>
  </notes><app-group>
        <supplementary-material position="anchor"><p id="d1e3131">The supplement related to this article is available online at: <inline-supplementary-material xlink:href="https://doi.org/10.5194/nhess-19-1839-2019-supplement" xlink:title="pdf">https://doi.org/10.5194/nhess-19-1839-2019-supplement</inline-supplementary-material>.</p></supplementary-material>
        </app-group><notes notes-type="authorcontribution"><title>Author contributions</title>

      <p id="d1e3140">The idea of the study followed from discussions between SF and SD. The model and the RAMS-3DVar simulations were performed by SF, RCT, and EA. The data assimilation of radar reflectivity factor and radar data analysis were carried out by LB, OC, MM, and GV. Lightning data assimilation was performed by SF and SD. All authors contributed to writing and reviewing the paper.</p>
  </notes><notes notes-type="competinginterests"><title>Competing interests</title>

      <p id="d1e3146">The authors declare that they have no conflict of interest.</p>
  </notes><notes notes-type="sistatement"><title>Special issue statement</title>

      <p id="d1e3152">This article is part of the special issue “Hydrological cycle in the Mediterranean (ACP/AMT/GMD/HESS/NHESS/OS inter-journal SI)”. It is not associated with a conference.</p>
  </notes><ack><title>Acknowledgements</title><p id="d1e3158">This work is a contribution to the HyMeX programme. Part of the computational
time used for this paper was granted by the ECMWF (European Centre for
Medium-Range Weather Forecasts) throughout the special project SPITFEDE.
LINET data were provided by Nowcast GmbH (<uri>https://www.nowcast.de/</uri>) within a
scientific agreement between Hans Dieter Betz and the Satellite Meteorological Group
of CNR-ISAC in Rome.</p><p id="d1e3163">We acknowledge the three anonymous reviewers and the editor for the substantial
improvement of the quality of the paper in the review process.</p></ack><notes notes-type="financialsupport"><title>Financial support</title>

      <?pagebreak page1861?><p id="d1e3168">This work was partially funded by the agreement between CNR-ISAC and the Italian Department of Civil Protection.</p>
  </notes><notes notes-type="reviewstatement"><title>Review statement</title>

      <p id="d1e3174">This paper was edited by Christian Barthlott and reviewed by three anonymous referees.</p>
  </notes><ref-list>
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    <!--<article-title-html>The impact of lightning and radar reflectivity factor data assimilation on the very short-term rainfall forecasts of RAMS@ISAC: application to two case studies in Italy</article-title-html>
<abstract-html><p>In this paper, we study the impact of lightning and radar reflectivity
factor data assimilation on the precipitation VSF (very short-term forecast,
3&thinsp;h in this study) for two severe weather events that occurred in Italy.
The first case refers to a moderate and localized rainfall over central
Italy that occurred on 16 September 2017. The second case occurred on 9 and 10 September 2017 and was very intense and caused damages in several geographical areas, especially in Livorno (Tuscany) where nine people died.</p><p>The first case study was missed by several operational forecasts, including
that performed by the model used in this paper, while the Livorno case was
partially predicted by operational models.</p><p>We use the RAMS@ISAC model (Regional Atmospheric Modelling System at
Institute for Atmospheric Sciences and Climate of the Italian National
Research Council), whose 3D-Var extension to the assimilation of radar
reflectivity factor is shown in this paper for the first time.</p><p>Results for the two cases show that the assimilation of lightning and radar
reflectivity factor, especially when used together, have a significant and
positive impact on the precipitation forecast. For specific time intervals,
the data assimilation is of practical importance for civil protection
purposes because it changes a missed forecast of intense precipitation ( ≥ 40&thinsp;mm in 3&thinsp;h) to a correct one.</p><p>While there is an improvement of the rainfall VSF thanks to the lightning
and radar reflectivity factor data assimilation, its usefulness is partially
reduced by the increase in false alarms, especially when both datasets
are assimilated.</p></abstract-html>
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