<?xml version="1.0" encoding="UTF-8"?>
<!DOCTYPE article PUBLIC "-//NLM//DTD Journal Publishing with OASIS Tables v3.0 20080202//EN" "https://jats.nlm.nih.gov/nlm-dtd/publishing/3.0/journalpub-oasis3.dtd">
<article xmlns:xlink="http://www.w3.org/1999/xlink" xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:oasis="http://docs.oasis-open.org/ns/oasis-exchange/table" xml:lang="en" dtd-version="3.0" article-type="research-article"><?xmltex \bartext{IAHS2022 -- Variability and change across space, time, extremes, and interfaces}?>
  <front>
    <journal-meta><journal-id journal-id-type="publisher">PIAHS</journal-id><journal-title-group>
    <journal-title>Proceedings of IAHS</journal-title>
    <abbrev-journal-title abbrev-type="publisher">PIAHS</abbrev-journal-title><abbrev-journal-title abbrev-type="nlm-ta">Proc. IAHS</abbrev-journal-title>
  </journal-title-group><issn pub-type="epub">2199-899X</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/piahs-385-147-2024</article-id><title-group><article-title>Rainfall data augmentation in Northern Italy through daily extremes and the Hershfield factor</article-title><alt-title>Rainfall data augmentation in Northern Italy</alt-title>
      </title-group><?xmltex \runningtitle{Rainfall data augmentation in Northern Italy}?><?xmltex \runningauthor{P. Mazzoglio et al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes">
          <name><surname>Mazzoglio</surname><given-names>Paola</given-names></name>
          <email>paola.mazzoglio@polito.it</email>
        <ext-link>https://orcid.org/0000-0002-3662-9439</ext-link></contrib>
        <contrib contrib-type="author" corresp="no">
          <name><surname>Butera</surname><given-names>Ilaria</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no">
          <name><surname>Claps</surname><given-names>Pierluigi</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-9624-7408</ext-link></contrib>
        <aff id="aff1"><institution>Department of Environment, Land and Infrastructure Engineering, Politecnico di Torino, Torino, 10129, Italy</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Paola Mazzoglio (paola.mazzoglio@polito.it)</corresp></author-notes><pub-date><day>18</day><month>April</month><year>2024</year></pub-date>
      
      <volume>385</volume>
      <fpage>147</fpage><lpage>153</lpage>
      <history>
        <date date-type="received"><day>28</day><month>May</month><year>2022</year></date>
           <date date-type="rev-recd"><day>26</day><month>January</month><year>2023</year></date>
           <date date-type="accepted"><day>29</day><month>March</month><year>2023</year></date>
      </history>
      <permissions>
        <copyright-statement>Copyright: © 2024 Paola Mazzoglio et al.</copyright-statement>
        <copyright-year>2024</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://piahs.copernicus.org/articles/385/147/2024/piahs-385-147-2024.html">This article is available from https://piahs.copernicus.org/articles/385/147/2024/piahs-385-147-2024.html</self-uri><self-uri xlink:href="https://piahs.copernicus.org/articles/385/147/2024/piahs-385-147-2024.pdf">The full text article is available as a PDF file from https://piahs.copernicus.org/articles/385/147/2024/piahs-385-147-2024.pdf</self-uri>
      <abstract><title>Abstract</title>

      <p id="d1e91">The majority of rainfall measurements in the world is at the daily scale, i.e. related to a specific calendar day and measured over fixed 24 h. On these data, daily annual maximum rainfall depths (<inline-formula><mml:math id="M1" display="inline"><mml:mi>F</mml:mi></mml:math></inline-formula>-maxima) series are easily obtained. On the other hand, 24 h annual maximum rainfall depths (<inline-formula><mml:math id="M2" display="inline"><mml:mi>S</mml:mi></mml:math></inline-formula>-maxima), which refer to a period starting at any instant, are more useful indicators. <inline-formula><mml:math id="M3" display="inline"><mml:mi>S</mml:mi></mml:math></inline-formula>-maxima values cannot be less than the <inline-formula><mml:math id="M4" display="inline"><mml:mi>F</mml:mi></mml:math></inline-formula>-maxima, and are generally higher. The ratio between these extremes, called Hershfield factor (<inline-formula><mml:math id="M5" display="inline"><mml:mi>H</mml:mi></mml:math></inline-formula>), has been studied to move from <inline-formula><mml:math id="M6" display="inline"><mml:mi>F</mml:mi></mml:math></inline-formula>-maxima to <inline-formula><mml:math id="M7" display="inline"><mml:mi>S</mml:mi></mml:math></inline-formula>-maxima, allowing to take advantage of the relevant amount of information included in historical records of daily extremes. For instance, before 1980, in the Italian Hydrological Yearbooks only a subset (<inline-formula><mml:math id="M8" display="inline"><mml:mo lspace="0mm">&lt;</mml:mo></mml:math></inline-formula> 50 %) of the rain gauges was equipped with a recording device, from which annual maxima over 1, 3, 6, 12 and 24 consecutive hours can be derived. In this study we investigate the possibility of using <inline-formula><mml:math id="M9" display="inline"><mml:mi>F</mml:mi></mml:math></inline-formula>-maxima to complement the <inline-formula><mml:math id="M10" display="inline"><mml:mi>S</mml:mi></mml:math></inline-formula>-maxima records related to the Po river basin and the Liguria region (North of Italy). As a first step we retrieved from official databases all the daily rainfall measurements, available over this area, from early 1900 until today and we quality-controlled the measurements. We then computed the annual <inline-formula><mml:math id="M11" display="inline"><mml:mi>H</mml:mi></mml:math></inline-formula> for all the stations and all the years where both the <inline-formula><mml:math id="M12" display="inline"><mml:mi>F</mml:mi></mml:math></inline-formula>- and <inline-formula><mml:math id="M13" display="inline"><mml:mi>S</mml:mi></mml:math></inline-formula>-maxima were available, to obtain data that can be analyzed in their temporal and spatial variability. The spatial distribution of the Hershfield factor shows values similar to the ones suggested in the literature and is related to the geographic position of the stations, allowing the possibility to identify some distinct areas with positive or negative anomalies. The obtained map of the <inline-formula><mml:math id="M14" display="inline"><mml:mi>H</mml:mi></mml:math></inline-formula> factor, with interpolated local anomalies, allows to reconstruct the missing <inline-formula><mml:math id="M15" display="inline"><mml:mi>S</mml:mi></mml:math></inline-formula>-maxima in stations with only <inline-formula><mml:math id="M16" display="inline"><mml:mi>F</mml:mi></mml:math></inline-formula>-maxima, and improve the knowledge of the spatial variability of sub-daily rainfall extremes.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

      
      </body>
    <back><notes notes-type="specialsection"><title>Keywords</title>
    

      <p id="d1e215">UPH 17; field observation; Italy; Po river basin; rainfall; extremes</p>
  </notes>
<sec id="Ch1.S1" sec-type="intro">
  <label>1</label><title>Introduction</title>
      <p id="d1e226">For decades, several hydrological variables as the rainfall depths were measured on a calendar day basis, usually at 09:00 a.m. local time (Morbidelli et al., 2021). In Italy, those daily measurements are published in the Hydrological Yearbooks, a collection of data usually available only in printed format. The availability of shorter duration records was limited by the requirement of continuous monitoring rainfall gauges. After the replacement of the mechanical rain gauges with the automatic ones in the last decades of the 20th century, the reference time for the calendar day rainfall measure was shifted to 00:00 a.m. However, the daily measurement approach was never ended, even if it is widely known that such discretization in time leads to bias when dealing with extreme events (Papalexiou et al., 2016). Considering the vast heritage of measurements and its simplicity, the majority of annual maximum rainfall depths in the world are at the daily scale, i.e. expressed over fixed 24 h (<inline-formula><mml:math id="M17" display="inline"><mml:mi>F</mml:mi></mml:math></inline-formula>-maxima).</p>
      <?pagebreak page148?><p id="d1e236">It is clear, however, that sliding 24 h maxima obtained from continuous measurements (<inline-formula><mml:math id="M18" display="inline"><mml:mi>S</mml:mi></mml:math></inline-formula>-maxima) are more useful values. They refer to 24 h periods starting at any instant and cannot be less than the <inline-formula><mml:math id="M19" display="inline"><mml:mi>F</mml:mi></mml:math></inline-formula>-maxima. An analysis conducted over the United States proved that the <inline-formula><mml:math id="M20" display="inline"><mml:mi>S</mml:mi></mml:math></inline-formula>-maxima statistics like the median, the mean and the standard deviation are higher than those of <inline-formula><mml:math id="M21" display="inline"><mml:mi>F</mml:mi></mml:math></inline-formula>-maxima and have a greater dispersion; the difference between the <inline-formula><mml:math id="M22" display="inline"><mml:mi>F</mml:mi></mml:math></inline-formula>- and <inline-formula><mml:math id="M23" display="inline"><mml:mi>S</mml:mi></mml:math></inline-formula>-maxima statistics increases as the time interval increases and appears to become constant for time scales larger than 36 h (Papalexiou et al., 2016).</p>
      <p id="d1e282">The ratio between <inline-formula><mml:math id="M24" display="inline"><mml:mi>F</mml:mi></mml:math></inline-formula>- and <inline-formula><mml:math id="M25" display="inline"><mml:mi>S</mml:mi></mml:math></inline-formula>-maxima, named Hershfield factor (<inline-formula><mml:math id="M26" display="inline"><mml:mi>H</mml:mi></mml:math></inline-formula>), has been suggested to correct the incongruences induced by the different time discretization, allowing to take advantage of the relevant amount of information included in historical records of <inline-formula><mml:math id="M27" display="inline"><mml:mi>F</mml:mi></mml:math></inline-formula>-maxima (Hershfield, 1961; Harihara Ayyar and Tripathi, 1973; van Montfort, 1990; Dwyer and Reed, 1995; van Montfort, 1997; Papalexiou et al., 2016; Llabrés-Brustenga et al., 2020).</p>
      <p id="d1e313"><inline-formula><mml:math id="M28" display="inline"><mml:mi>H</mml:mi></mml:math></inline-formula> acts as a multiplier that aims at correcting the underestimation caused by the daily time sampling. Hershfield itself suggested to use a value equal to 1.13 after an analysis carried out using data covering the United States (Hershfield, 1961). In a recent analysis in the United States, Papalexiou et al. (2016) obtained a value equal to 1.14. An application over India suggested a value equal to 1.15 (Harihara Ayyar and Tripathi, 1973). Over China, van Montfort (1997) obtained values in the range 1.04–1.17. Dwyer and Reed (1995) suggested a mean value of 1.16, while proposing differences according to different regimes: a correction factor of 1.15 for rainfall regimes with more frequent short-duration concentrated events, and 1.17 for sites with rainfall regimes with more frequent longer events, such as those produced by large frontal systems. Llabrés-Brustenga et al. (2020) obtained a mean value of 1.125 over Catalonia (Spain) and highlighted considerable variations within the year: summer is the season in which lower <inline-formula><mml:math id="M29" display="inline"><mml:mi>H</mml:mi></mml:math></inline-formula> (1.093) was obtained, justified by the fact that rainfall is often raised by the influence of the diurnal cycle and the <inline-formula><mml:math id="M30" display="inline"><mml:mi>S</mml:mi></mml:math></inline-formula>-maxima are not usually split by daily measuring in the morning; in spring, a higher <inline-formula><mml:math id="M31" display="inline"><mml:mi>H</mml:mi></mml:math></inline-formula> (1.161) was obtained, possibly determined by the fact that rainfall events are more often split when <inline-formula><mml:math id="M32" display="inline"><mml:mi>F</mml:mi></mml:math></inline-formula>-maxima measurements are taken at 08:00 a.m.</p>
      <p id="d1e351">All these studies (except Papalexiou et al., 2016 and Llabrés-Brustenga et al., 2020) are based on old records. In our study, we investigated the possibility of using <inline-formula><mml:math id="M33" display="inline"><mml:mrow><mml:mo>≈</mml:mo><mml:mn mathvariant="normal">1000</mml:mn></mml:mrow></mml:math></inline-formula> stations with at least 10 years of both <inline-formula><mml:math id="M34" display="inline"><mml:mi>F</mml:mi></mml:math></inline-formula>- and <inline-formula><mml:math id="M35" display="inline"><mml:mi>S</mml:mi></mml:math></inline-formula>-maxima for the same years, covering the period from early 1900 until today, to enrich the availability of <inline-formula><mml:math id="M36" display="inline"><mml:mi>S</mml:mi></mml:math></inline-formula>-maxima rainfall measurements, by selecting the data-rich Po river basin and the Liguria region (North of Italy) as a case study. The objective is to obtain mean values of <inline-formula><mml:math id="M37" display="inline"><mml:mi>H</mml:mi></mml:math></inline-formula> for the stations where both <inline-formula><mml:math id="M38" display="inline"><mml:mi>F</mml:mi></mml:math></inline-formula>- and <inline-formula><mml:math id="M39" display="inline"><mml:mi>S</mml:mi></mml:math></inline-formula>-maxima data are available and make these value available, through spatial interpolation, to <inline-formula><mml:math id="M40" display="inline"><mml:mi>F</mml:mi></mml:math></inline-formula>-maxima stations where <inline-formula><mml:math id="M41" display="inline"><mml:mi>S</mml:mi></mml:math></inline-formula>-maxima data are unavailable.</p>
</sec>
<sec id="Ch1.S2">
  <label>2</label><title>Data management and quality-control</title>
<sec id="Ch1.S2.SS1">
  <label>2.1</label><title>Area of interest</title>
      <p id="d1e436">In this study we analysed an area of about 90 000 km<inline-formula><mml:math id="M42" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula> extent located in the North of Italy, that coincides with the Po river basin and the Liguria region. The different administrative regions included in this area and the elevation data are represented in Fig. 1.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1"><?xmltex \currentcnt{1}?><?xmltex \def\figurename{Figure}?><label>Figure 1</label><caption><p id="d1e450">Elevation data with borders and names of the administrative regions. Source: Shuttle Radar Topography Mission (Farr et al., 2007).</p></caption>
        <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://piahs.copernicus.org/articles/385/147/2024/piahs-385-147-2024-f01.png"/>

      </fig>

</sec>
<sec id="Ch1.S2.SS2">
  <label>2.2</label><?xmltex \opttitle{Validated $S$- and $F$-maxima datasets}?><title>Validated <inline-formula><mml:math id="M43" display="inline"><mml:mi>S</mml:mi></mml:math></inline-formula>- and <inline-formula><mml:math id="M44" display="inline"><mml:mi>F</mml:mi></mml:math></inline-formula>-maxima datasets</title>
      <p id="d1e482">Annual maximum rainfall depths related to a 24 h time interval (i.e., the <inline-formula><mml:math id="M45" display="inline"><mml:mi>S</mml:mi></mml:math></inline-formula>-maxima) are derived from the Improved Italian – Rainfall Extreme Dataset (I<inline-formula><mml:math id="M46" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula>-RED; Mazzoglio et al., 2020), a collection of rainfall extremes recorded since 1916 by more than 5200 rain gauges installed all over Italy. In this analysis we used only the time series of the 1713 rain gauges installed in the study area.</p>
      <p id="d1e501">A set of validated <inline-formula><mml:math id="M47" display="inline"><mml:mi>F</mml:mi></mml:math></inline-formula>-maxima (i.e., quality-controlled daily annual maxima published in a dedicated table of annual maxima) is available in digital format from: ARPA Piemonte for the years 1988–2018 (ARPA Piemonte, 2022), the Functional Center of the Autonomous Aosta Valley Region for the years 1994–2016 (Centro Funzionale Regione Autonoma Valle d'Aosta, 2022), the VAPI Piemonte project for the years 1913–1986 (Villani, 2003), Meteotrentino for the years 1921–2009 (Meteotrentino, 2022) and ARPA Veneto for the years 1984–2021 (ARPA Veneto, 2022).</p>
</sec>
<sec id="Ch1.S2.SS3">
  <label>2.3</label><title>Continuous time series datasets</title>
      <p id="d1e519">The spatio-temporal coverage of the validated datasets (Fig. 2) is very limited with respect to the spatio-temporal coverage of the printed version of the Hydrological Yearbooks. The digitization of the Yearbooks tables containing validated <inline-formula><mml:math id="M48" display="inline"><mml:mi>F</mml:mi></mml:math></inline-formula>-maxima would require a massive effort, out of the scope of this work. To fill the spatio-temporal gaps caused<?pagebreak page149?> by missing validated data, we resorted to available historical continuous daily rainfall time series, available in digital format, that are partially uncontrolled. The main data source that we used is the SCIA database (ISPRA, 2022). It has been integrated with few daily time series, coming from: ARPA Piemonte for 1988 onwards (ARPA Piemonte, 2022), the “Banca dati meteoclimatica” of Liguria Region (Regione Liguria and ARPAL, 2022), the “Atlante climatico della Liguria” for the years 1960–2010 (Agrillo and Bonati, 2013) and the Dext3r webapp (ARPAE-SIMC, 2022).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2"><?xmltex \currentcnt{2}?><?xmltex \def\figurename{Figure}?><label>Figure 2</label><caption><p id="d1e531">Spatio-temporal availability of the validated <inline-formula><mml:math id="M49" display="inline"><mml:mi>F</mml:mi></mml:math></inline-formula>-maxima. Grey colour indicates areas where a database of daily annual maxima in digital format is not available.</p></caption>
        <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://piahs.copernicus.org/articles/385/147/2024/piahs-385-147-2024-f02.png"/>

      </fig>

      <p id="d1e547">In this study we did not consider the influence of the change of the time of the daily measurements, because precise and extensive information on the years in which the hydrological agencies started to record the daily measurement at 00:00 a.m. is not available. However, it should be noted that Llabrés-Brustenga et al. (2020) pointed out that very high <inline-formula><mml:math id="M50" display="inline"><mml:mi>H</mml:mi></mml:math></inline-formula> is obtained only in the case of <inline-formula><mml:math id="M51" display="inline"><mml:mi>F</mml:mi></mml:math></inline-formula>-maxima taken with starting time in the afternoon. They also argue that <inline-formula><mml:math id="M52" display="inline"><mml:mi>F</mml:mi></mml:math></inline-formula>-maxima is usually more precise if sampled at 00:00 a.m., even though 08:00 a.m. can be considered as a good sampling time.</p>
      <p id="d1e572">All the continuous daily time series of the datasets mentioned before were merged into a unique dataset. The SCIA database was found lacking some of the most relevant daily maxima recorded in recent years in the Liguria region: a manual gap-filling procedure was thus performed after having identified the time series that contains only 1 missing daily data (i.e., the actual <inline-formula><mml:math id="M53" display="inline"><mml:mi>F</mml:mi></mml:math></inline-formula>-maxima). In this case, the missing measurement (that was probably removed by too strict quality-control procedure applied while building the SCIA dataset) was retrieved from the printed version of the Hydrological Yearbooks or from ARPA Liguria website. Afterwards, to verify the correctness of the continuous daily data, high precipitation values (greater than 500 mm) were manually controlled, to verify if they were realistic. In a few cases, these high values were removed, because caused by a mistake with decimals in the table.</p>
      <p id="d1e582">After this merging and control operations, only continuous time series with at least 330 out of 365 daily measurements were used to compute the annual <inline-formula><mml:math id="M54" display="inline"><mml:mi>F</mml:mi></mml:math></inline-formula>-maxima. These were integrated with the already validated <inline-formula><mml:math id="M55" display="inline"><mml:mi>F</mml:mi></mml:math></inline-formula>-maxima.</p>
</sec>
<sec id="Ch1.S2.SS4">
  <label>2.4</label><title>Final datasets</title>
      <p id="d1e607">The data merging procedure allowed us to reach a total of about 1000 stations with at least 10 years of both <inline-formula><mml:math id="M56" display="inline"><mml:mi>F</mml:mi></mml:math></inline-formula>- and <inline-formula><mml:math id="M57" display="inline"><mml:mi>S</mml:mi></mml:math></inline-formula>-maxima for the same years. Nevertheless, the total number of <inline-formula><mml:math id="M58" display="inline"><mml:mi>F</mml:mi></mml:math></inline-formula>-stations is significantly higher: in this region, 2149 stations with <inline-formula><mml:math id="M59" display="inline"><mml:mi>F</mml:mi></mml:math></inline-formula>-maxima are available, allowing to have a data density of 1 rain gauge every 42 km<inline-formula><mml:math id="M60" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula> (the data density of the sub-daily time series is of 1 rain gauge every 53 km<inline-formula><mml:math id="M61" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula>). In Fig. 3 it is possible to observe the spatial distribution of the <inline-formula><mml:math id="M62" display="inline"><mml:mi>F</mml:mi></mml:math></inline-formula>- and <inline-formula><mml:math id="M63" display="inline"><mml:mi>S</mml:mi></mml:math></inline-formula>-maxima. From the figure one can realize that the data density is not uniform: even including the <inline-formula><mml:math id="M64" display="inline"><mml:mi>F</mml:mi></mml:math></inline-formula>-maxima, several locations in the lowlands or at high elevations are still poorly sampled.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3"><?xmltex \currentcnt{3}?><?xmltex \def\figurename{Figure}?><label>Figure 3</label><caption><p id="d1e680">Spatial distribution of the sub-daily and daily records. Source: I<inline-formula><mml:math id="M65" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula>-RED data (Mazzoglio et al., 2020).</p></caption>
        <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://piahs.copernicus.org/articles/385/147/2024/piahs-385-147-2024-f03.png"/>

      </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4"><?xmltex \currentcnt{4}?><?xmltex \def\figurename{Figure}?><label>Figure 4</label><caption><p id="d1e700">Time history of the number of active rain gauges.</p></caption>
        <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://piahs.copernicus.org/articles/385/147/2024/piahs-385-147-2024-f04.png"/>

      </fig>

      <?pagebreak page150?><p id="d1e710">In Fig. 4 it is possible to see the time history of the available stations. From this figure it clearly emerges that, for instance, before 1980 only a subset (<inline-formula><mml:math id="M66" display="inline"><mml:mrow><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">50</mml:mn></mml:mrow></mml:math></inline-formula> %) of the rain gauges was equipped with a continuous recording device.</p>
</sec>
</sec>
<sec id="Ch1.S3">
  <label>3</label><title>Evaluation of the Hershfield factor</title>
      <p id="d1e732">For all the stations and all the years where both the <inline-formula><mml:math id="M67" display="inline"><mml:mi>F</mml:mi></mml:math></inline-formula>-maxima and <inline-formula><mml:math id="M68" display="inline"><mml:mi>S</mml:mi></mml:math></inline-formula>-maxima are available, the Hershfield factor was computed according to its definition:
        <disp-formula id="Ch1.E1" content-type="numbered"><label>1</label><mml:math id="M69" display="block"><mml:mrow><mml:mi>H</mml:mi><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msub><mml:mi>h</mml:mi><mml:mn mathvariant="normal">24</mml:mn></mml:msub></mml:mrow><mml:mrow><mml:msub><mml:mi>h</mml:mi><mml:mi mathvariant="normal">g</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="M70" display="inline"><mml:mrow><mml:msub><mml:mi>h</mml:mi><mml:mn mathvariant="normal">24</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> is the 24 h annual maximum and <inline-formula><mml:math id="M71" display="inline"><mml:mrow><mml:msub><mml:mi>h</mml:mi><mml:mi mathvariant="normal">g</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the daily maximum in a given year.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F5"><?xmltex \currentcnt{5}?><?xmltex \def\figurename{Figure}?><label>Figure 5</label><caption><p id="d1e799">Box plot of the yearly Hershfield factors computed using the validated data <bold>(a)</bold> and from the merged dataset <bold>(b)</bold>. Each box plot displays the following information: the median, the lower and upper quartiles (blue box), any outlier (values that are more than 1.5 times the interquartile range, depicted as a blue circle), and the minimum and maximum values that are not outliers (black whiskers).</p></caption>
      <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://piahs.copernicus.org/articles/385/147/2024/piahs-385-147-2024-f05.png"/>

    </fig>

      <p id="d1e814">As a general rule, <inline-formula><mml:math id="M72" display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>≤</mml:mo><mml:mi>H</mml:mi><mml:mo>≤</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> (van Montfort, 1997). It can be equal to 1 if the <inline-formula><mml:math id="M73" display="inline"><mml:mi>S</mml:mi></mml:math></inline-formula>-maxima occurred inside the same calendar day, while it can be equal to 2 if the extreme event is equally divided into two days.</p>
      <p id="d1e841">In a first step, we analysed <inline-formula><mml:math id="M74" display="inline"><mml:mi>H</mml:mi></mml:math></inline-formula> using only the validated data, whatever the record length, to obtain reliable results that would be compared to those obtained using the entire dataset.</p>
      <p id="d1e851">Even in validated data we found cases in which <inline-formula><mml:math id="M75" display="inline"><mml:mi>F</mml:mi></mml:math></inline-formula>-maxima were higher than <inline-formula><mml:math id="M76" display="inline"><mml:mi>S</mml:mi></mml:math></inline-formula>-maxima. This inconsistency is not unusual, and can be attributed to errors in the digitization, due to the manual daily recording. These occurrences, and the others in which we found <inline-formula><mml:math id="M77" display="inline"><mml:mrow><mml:mi>H</mml:mi><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula>, were removed. Figure 5a shows the box plot of the individual <inline-formula><mml:math id="M78" display="inline"><mml:mi>H</mml:mi></mml:math></inline-formula> values obtained year by year: the overall median <inline-formula><mml:math id="M79" display="inline"><mml:mi>H</mml:mi></mml:math></inline-formula> is 1.112, while the whiskers ends are, respectively, 1 and 1.585. The overall mean value obtained for <inline-formula><mml:math id="M80" display="inline"><mml:mi>H</mml:mi></mml:math></inline-formula> is 1.170, somewhat higher than those in the literature.</p>
      <p id="d1e902">Having removed only the undeniable anomalies (<inline-formula><mml:math id="M81" display="inline"><mml:mrow><mml:mi>H</mml:mi><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> or <inline-formula><mml:math id="M82" display="inline"><mml:mrow><mml:mi>H</mml:mi><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula>) does not exclude the possibility that other anomalies may have occurred. We then used the limits of the box plot to filter out possible outliers in the process of extending the computation to the entire dataset. Therefore, when computing the <inline-formula><mml:math id="M83" display="inline"><mml:mi>H</mml:mi></mml:math></inline-formula> values for all the stations using the entire dataset, made of validated and not validated data, we used series with at least 10 years of data and we used the whiskers ends of the validated data (1 and 1.585) as thresholds to remove the outliers. After this computation, the median <inline-formula><mml:math id="M84" display="inline"><mml:mi>H</mml:mi></mml:math></inline-formula> resulted of 1.144 and the mean resulted equal to 1.146, which are in line with the values reported in the literature. By increasing the minimum record length to 20 years we obtained an average of <inline-formula><mml:math id="M85" display="inline"><mml:mi>H</mml:mi></mml:math></inline-formula> equal to 1.142, and a median equal to 1.141, suggesting that even a time series of only 10 years could provide reliable estimates.</p>
      <p id="d1e950">Examinig the box plots in Fig. 5 one can recognize that the variability of the <inline-formula><mml:math id="M86" display="inline"><mml:mi>H</mml:mi></mml:math></inline-formula> computed from the entire dataset turns out to be similar to the one of the validated data, despite a higher number of outliers. This evidence confirms the suitability of using also non-validated data to guarantee an higher spatio-temporal coverage of <inline-formula><mml:math id="M87" display="inline"><mml:mi>F</mml:mi></mml:math></inline-formula>-maxima.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F6"><?xmltex \currentcnt{6}?><?xmltex \def\figurename{Figure}?><label>Figure 6</label><caption><p id="d1e969">Spatial distribution of the Hershfield factor obtained by applying and Ordinary Kriging with spherical variogram.</p></caption>
      <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://piahs.copernicus.org/articles/385/147/2024/piahs-385-147-2024-f06.png"/>

    </fig>

      <p id="d1e979">After the computation and validation of the <inline-formula><mml:math id="M88" display="inline"><mml:mi>H</mml:mi></mml:math></inline-formula> values in the so-reached <inline-formula><mml:math id="M89" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 1000 stations, we proceeded to a spatial interpolation at 1 km resolution of the mean <inline-formula><mml:math id="M90" display="inline"><mml:mi>H</mml:mi></mml:math></inline-formula>. This procedure was realized using the Ordinary Kriging (Fig. 6). By analyzing the spatial distribution of the interpolated Hershfield factor within the study area, we found variability patterns similar to those available in the literature, i.e. the mean (at station) <inline-formula><mml:math id="M91" display="inline"><mml:mi>H</mml:mi></mml:math></inline-formula> values turn out to be non uniform over the space. They seem influenced by the geographic position of the stations, and the patterns entail the possibility to identify some<?pagebreak page151?> distinct areas with a positive or negative anomaly with respect to the spatial average. More specifically, higher values emerge in the Northern part of the examined region, mainly in Piedmont and Lombardy. The Aosta Valley, despite its location in the northern parts, shows different anomalies. This difference could probably be addressed to different prevailing rainfall mechanisms occurring in the Aosta Valley, possibly due to the presence of high peaks at the borders between Piedmont and the Aosta Valley, which act as a barrier. An influence of the geographic position was also pointed out over Catalonia (Spain) by Llabrés-Brustenga et al. (2020), and over China, where van Montfort (1997) analyzed monthly <inline-formula><mml:math id="M92" display="inline"><mml:mi>H</mml:mi></mml:math></inline-formula> values in relation to the location of the station, the autocorrelation within its daily measurements and the fraction of wet days.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F7"><?xmltex \currentcnt{7}?><?xmltex \def\figurename{Figure}?><label>Figure 7</label><caption><p id="d1e1019">Spatial distribution of the Hershfield factor before <bold>(a)</bold> and after <bold>(b)</bold> the site-specific data-cleaning operation. Focus over the Eastern part of Lombardy region.</p></caption>
      <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://piahs.copernicus.org/articles/385/147/2024/piahs-385-147-2024-f07.png"/>

    </fig>

      <p id="d1e1034">The exam of the spatial distribution of <inline-formula><mml:math id="M93" display="inline"><mml:mi>H</mml:mi></mml:math></inline-formula> has suggested the necessity to perform an additional data control, as some suspicious isolated anomalies clearly emerged (Fig. 7a). This happened especially in areas where official and quality-controlled annual maxima were not available, so that <inline-formula><mml:math id="M94" display="inline"><mml:mi>F</mml:mi></mml:math></inline-formula>-maxima were computed from continuous daily records. For these isolated “peaks” of <inline-formula><mml:math id="M95" display="inline"><mml:mi>H</mml:mi></mml:math></inline-formula>, the <inline-formula><mml:math id="M96" display="inline"><mml:mi>F</mml:mi></mml:math></inline-formula>-maxima time series of the rain gauges have been checked and the incorrect <inline-formula><mml:math id="M97" display="inline"><mml:mi>F</mml:mi></mml:math></inline-formula>-maxima data have been replaced using the values reported in the printed version of the Hydrological Yearbooks, as depicted in Fig. 7b. Note that Fig. 6 already report the fully corrected version of the map.</p>
</sec>
<sec id="Ch1.S4">
  <label>4</label><title>Discussion</title>
      <p id="d1e1081">To increase the spatial detail of the extremes of precipitation over the North of Italy, a consistent database including daily precipitation (<inline-formula><mml:math id="M98" display="inline"><mml:mi>F</mml:mi></mml:math></inline-formula>-maxima) can be used. The analysis of the ratio between 24 h and daily extremes (Hershfield factor) throughout the investigated area can allow to estimate annual <inline-formula><mml:math id="M99" display="inline"><mml:mi>S</mml:mi></mml:math></inline-formula>-maxima (i.e. over 24 h) in the stations that lack this information. In some areas (mountain regions and the lowlands between Piedmont and Lombardy) the increase in detail is noteworthy, and can provide important improvement over the spatial analysis of 24 h extremes.</p>
      <p id="d1e1098">Before proceeding with the use of these reconstructed data, some care must be exerted about the reliability of these newly-computed maxima. In these terms, it is worth mentioning that Koutsoyiannis and Iliopoulou (2022) pointed out that there is no theoretical basis behind the “inflation” through the Hershfield factor, even though it can represent an acceptable estimate from an engineering point of view. The authors pointed out that all realizations are stochastically equivalent and there is no theoretical basis for their correction. By correcting the series, its stochastic properties can be distorted.</p>
      <p id="d1e1101">In terms of series properties, indeed, Papalexiou et al. (2016) had previously noted that the ratios between the mean values of <inline-formula><mml:math id="M100" display="inline"><mml:mi>F</mml:mi></mml:math></inline-formula>- and <inline-formula><mml:math id="M101" display="inline"><mml:mi>S</mml:mi></mml:math></inline-formula>-maxima deviate from the standard deviation ratios: this implies that the application of the <inline-formula><mml:math id="M102" display="inline"><mml:mi>H</mml:mi></mml:math></inline-formula> factor cannot appropriately preserve the standard deviation of the <inline-formula><mml:math id="M103" display="inline"><mml:mi>F</mml:mi></mml:math></inline-formula>-maxima. These authors have then introduced an approach that simultaneously correct both the mean and the standard deviation errors.</p>
      <p id="d1e1132">Despite the caveats, however, we cannot ignore that the possibility to include data recorded in decades at the beginning of the past century (see Fig. 4) can produce relevant benefit in the spatial detail of the process. This suggests us to proceed with the application of the <inline-formula><mml:math id="M104" display="inline"><mml:mi>H</mml:mi></mml:math></inline-formula> factor to include the <inline-formula><mml:math id="M105" display="inline"><mml:mi>F</mml:mi></mml:math></inline-formula>-maxima in the existing 24 h records.</p>
      <p id="d1e1150">On the other hand, when looking for trends in the data, to protect the reconstructed data from the distortion mentioned by Koutsoyiannis and Iliopoulou (2022) robust methods can be used, as Sen's method, the non-parametric Mann-Kendall test and the Spearman rank correlation test that all exhibit negligible sensitivity to data distortion (Morbidelli et al., 2021).</p>
      <p id="d1e1153">In this work and in all the other ones cited in this paper the <inline-formula><mml:math id="M106" display="inline"><mml:mi>H</mml:mi></mml:math></inline-formula> values were considered as constant over time. Nevertheless, future works could be directed to investigate if the variations observed all over Italy in the 24 h extremes (Mazzoglio et al., 2022) can be detected also in the <inline-formula><mml:math id="M107" display="inline"><mml:mi>H</mml:mi></mml:math></inline-formula> values.</p>
</sec>
<sec id="Ch1.S5" sec-type="conclusions">
  <label>5</label><title>Conclusions</title>
      <p id="d1e1178">In this study we performed a complex data merging operation to recover all the <inline-formula><mml:math id="M108" display="inline"><mml:mi>F</mml:mi></mml:math></inline-formula>-maxima recorded starting from the 20th century by 2149 stations. This dataset was then used to evaluate the Hershfield factor, that is a coefficient computed as the ratio between the <inline-formula><mml:math id="M109" display="inline"><mml:mi>S</mml:mi></mml:math></inline-formula>-maxima and the <inline-formula><mml:math id="M110" display="inline"><mml:mi>F</mml:mi></mml:math></inline-formula>-maxima that can be relevant for the reconstruction of missing sub-daily annual maxima. The interpolation realized, reported with a map in Fig. 6, allows to reconstruct the missing <inline-formula><mml:math id="M111" display="inline"><mml:mi>S</mml:mi></mml:math></inline-formula>-maxima in stations with only <inline-formula><mml:math id="M112" display="inline"><mml:mi>F</mml:mi></mml:math></inline-formula>-maxima, and improves the knowledge of the spatial variability of sub-daily rainfall extremes.</p>
      <?pagebreak page152?><p id="d1e1216">In view of the extension of this data-recovering procedure to the entire Italy, further investigations are to be directed to the correction of distortion effects noted in the statistical properties of the reconstructed series. In that sense, it is important to consider the trade-off between the increase of uncertainty on the 24 h series properties and the increase in the spatial detail of <inline-formula><mml:math id="M113" display="inline"><mml:mi>S</mml:mi></mml:math></inline-formula>-maxima in data-scarce regions.</p>
</sec><notes notes-type="dataavailability"><title>Data availability</title>

      <p id="d1e1229">The daily time series can be downloaded from the original repositories. Full credits are reported in Sect. 2.</p>

      <p id="d1e1232">The 24 h rainfall data were obtained from the I<inline-formula><mml:math id="M114" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula>-RED database. Although Italian law requires an open-source policy for all public data, this right has not yet been implemented by all the Italian agencies involved in the management of the rain gauge network. The agreements we signed with some of these agencies, aimed at monitoring the correct use of the data, restricted their use to the aims of the authors' project. As a result of these legal restrictions, a complete version of I<inline-formula><mml:math id="M115" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula>-RED can only be provided to two groups of people: members of the authors' research group (who are already fully authorized to use the data) and people who can prove they have received clearance from the regional authorities. The entire quality-controlled database is available on Zenodo (<ext-link xlink:href="https://doi.org/10.5281/zenodo.4269509" ext-link-type="DOI">10.5281/zenodo.4269509</ext-link>, Mazzoglio et al., 2020), albeit with restricted access. The data can be used by third parties, for an indefinite timeframe, upon having completed an agreement with the authors and with the regional agencies involved in the data collection. The raw data availability depends on the region: a complete description of how to access these data is reported in Mazzoglio et al. (2020).</p>
  </notes><notes notes-type="authorcontribution"><title>Author contributions</title>

      <p id="d1e1259">PC, IB and PM designed the experiments and PM carried them out. PM performed the data merging operation and developed the code. PM prepared the manuscript with contributions from all co-authors.</p>
  </notes><notes notes-type="competinginterests"><title>Competing interests</title>

      <p id="d1e1265">The contact author has declared that none of the authors has any competing interests.</p>
  </notes><notes notes-type="disclaimer"><title>Disclaimer</title>

      <p id="d1e1271">Publisher’s note: Copernicus Publications remains neutral with regard to jurisdictional claims in published maps and institutional affiliations.</p>
  </notes><notes notes-type="sistatement"><title>Special issue statement</title>

      <p id="d1e1277">This article is part of the special issue “IAHS2022 – Hydrological sciences in the Anthropocene: Variability and change across space, time, extremes, and interfaces”. It is a result of the XIth Scientific Assembly of the International Association of Hydrological Sciences (IAHS 2022), Montpellier, France, 29 May–3 June 2022.</p>
  </notes><ack><title>Acknowledgements</title><p id="d1e1283">The authors acknowledge the regional agencies involved in the management of the rain gauge networks that provided the rainfall measurements included in I<inline-formula><mml:math id="M116" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula>-RED. Full credits are reported in Mazzoglio et al. (2020).</p></ack><notes notes-type="reviewstatement"><title>Review statement</title>

      <p id="d1e1297">This paper was edited by Christophe Cudennec and reviewed by two anonymous referees.</p>
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