<?xml version="1.0" encoding="UTF-8"?>
<!DOCTYPE article PUBLIC "-//NLM//DTD Journal Publishing with OASIS Tables v3.0 20080202//EN" "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" dtd-version="3.0">
  <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-17-467-2017</article-id><title-group><article-title>Landslides, floods and sinkholes in a karst environment:<?xmltex \hack{\newline}?> the 1–6 September
2014 Gargano event, southern Italy</article-title>
      </title-group><?xmltex \runningtitle{Landslides, floods and sinkholes in a karst environment}?><?xmltex \runningauthor{M.~E.~Martinotti et al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes" rid="aff1">
          <name><surname>Martinotti</surname><given-names>Maria Elena</given-names></name>
          <email>maria.elena.martinotti@irpi.cnr.it</email>
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2 aff6">
          <name><surname>Pisano</surname><given-names>Luca</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Marchesini</surname><given-names>Ivan</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-8342-3134</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Rossi</surname><given-names>Mauro</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-0252-4321</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Peruccacci</surname><given-names>Silvia</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Brunetti</surname><given-names>Maria Teresa</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Melillo</surname><given-names>Massimo</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3">
          <name><surname>Amoruso</surname><given-names>Giuseppe</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3">
          <name><surname>Loiacono</surname><given-names>Pierluigi</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2 aff4">
          <name><surname>Vennari</surname><given-names>Carmela</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-3704-3456</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2 aff5">
          <name><surname>Vessia</surname><given-names>Giovanna</given-names></name>
          
        <ext-link>https://orcid.org/0000-0003-1733-7112</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3">
          <name><surname>Trabace</surname><given-names>Maria</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2 aff7">
          <name><surname>Parise</surname><given-names>Mario</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Guzzetti</surname><given-names>Fausto</given-names></name>
          
        <ext-link>https://orcid.org/0000-0003-4950-6056</ext-link></contrib>
        <aff id="aff1"><label>1</label><institution>Consiglio Nazionale delle Ricerche, Istituto di Ricerca per la
Protezione Idrogeologica, <?xmltex \hack{\newline}?>via Madonna Alta 126, 06128 Perugia, Italy</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>Consiglio Nazionale delle Ricerche, Istituto di Ricerca per la
Protezione Idrogeologica, <?xmltex \hack{\newline}?>via Amendola 122, 70126 Bari, Italy</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>Regione Puglia, Servizio di Protezione Civile, Via delle Magnolie 6/8,
70126 Modugno (Bari), Italy</institution>
        </aff>
        <aff id="aff4"><label>4</label><institution>University of Naples “Federico II”, Naples, Italy</institution>
        </aff>
        <aff id="aff5"><label>5</label><institution>University of Chieti-Pescara “Gabriele D'Annunzio”, Chieti, Italy</institution>
        </aff>
        <aff id="aff6"><label>6</label><institution>University of Molise, Department of Biosciences and Territory,
Contrada Fonte Lappone, Pesche (IS), Italy</institution>
        </aff>
        <aff id="aff7"><label>a</label><institution>present address: University “Aldo Moro”, Department of Earth and
Environmental Sciences, Via Orabona 7,<?xmltex \hack{\newline}?> 70126 Bari, Italy</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Maria Elena Martinotti (maria.elena.martinotti@irpi.cnr.it)</corresp></author-notes><pub-date><day>22</day><month>March</month><year>2017</year></pub-date>
      
      <volume>17</volume>
      <issue>3</issue>
      <fpage>467</fpage><lpage>480</lpage>
      <history>
        <date date-type="received"><day>23</day><month>September</month><year>2016</year></date>
           <date date-type="rev-request"><day>31</day><month>October</month><year>2016</year></date>
           <date date-type="rev-recd"><day>8</day><month>February</month><year>2017</year></date>
           <date date-type="accepted"><day>24</day><month>February</month><year>2017</year></date>
      </history>
      <permissions>
<license license-type="open-access">
<license-p>This work is licensed under a Creative Commons Attribution 3.0 Unported License. To view a copy of this license, visit <ext-link ext-link-type="uri" xlink:href="http://creativecommons.org/licenses/by/3.0/">http://creativecommons.org/licenses/by/3.0/</ext-link></license-p>
</license>
</permissions><self-uri xlink:href="https://nhess.copernicus.org/articles/17/467/2017/nhess-17-467-2017.html">This article is available from https://nhess.copernicus.org/articles/17/467/2017/nhess-17-467-2017.html</self-uri>
<self-uri xlink:href="https://nhess.copernicus.org/articles/17/467/2017/nhess-17-467-2017.pdf">The full text article is available as a PDF file from https://nhess.copernicus.org/articles/17/467/2017/nhess-17-467-2017.pdf</self-uri>


      <abstract>
    <p>In karst environments, heavy rainfall is known to cause
multiple geohydrological hazards, including inundations, flash floods,
landslides and sinkholes. We studied a period of intense rainfall from 1 to
6 September 2014 in the Gargano Promontory, a karst area in Puglia, southern
Italy. In the period, a sequence of torrential rainfall events caused severe
damage and claimed two fatalities. The amount and accuracy of the
geographical and temporal information varied for the different hazards. The
temporal information was most accurate for the inundation caused by a major
river, less accurate for flash floods caused by minor torrents and even
less accurate for landslides. For sinkholes, only generic information on the
period of occurrence of the failures was available. Our analysis revealed
that in the promontory, rainfall-driven hazards occurred in response to
extreme meteorological conditions and that the karst landscape responded to
the torrential rainfall with a threshold behaviour. We exploited the
rainfall and the landslide information to design the new ensemble–non-exceedance probability (E-NEP) algorithm for the quantitative evaluation of
the possible occurrence of rainfall-induced landslides and of related
geohydrological hazards. The ensemble of the metrics produced by the E-NEP
algorithm provided better diagnostics than the single metrics often used for
landslide forecasting, including rainfall duration, cumulated rainfall and
rainfall intensity. We expect that the E-NEP algorithm will be useful for
landslide early warning in karst areas and in other similar environments. We
acknowledge that further tests are needed to evaluate the algorithm in
different meteorological, geological and physiographical settings.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <title>Introduction</title>
      <p>Torrential rainfall is known to cause inundations, flash floods and
different types of landslides, including debris flows, soil slides and rockfalls. Less known is that intense rainfall can cause sinkholes, a subtle
hazard in many karst environments (Parise and Gunn, 2007; De Waele et al.,
2011; Gutierrez et al., 2014; Parise et al., 2015). Here, we describe a
series of rainfall events and their ground effects in the period from 1 to 6
September 2014 in the Gargano Promontory, a karst environment and a popular
tourist area in the Puglia (Apulia) region, southern Italy. In a 6-day period, a
sequence of four heavy rainfall events, separated by periods with little or
no rainfall, caused multiple geohydrological hazards in the promontory,
including landslides, flash floods, widespread inundation and sinkholes.
The death toll amounted to two fatalities, and a number of people were
forced to leave their homes or businesses. Urban areas, tourist resorts,
roads and rails were inundated and damaged, causing severe economic
consequences. We have investigated the spatial–temporal relationships
between the rainfall trigger and the geohydrological hazards, and we have
designed and tested an algorithm for improved early landslide warning.</p>
      <p>The paper is organised as follows. After a brief description of the study
area (Sect. 2), in Sect. 3 we present the main meteorological and
rainfall characteristic of the heavy rainfall period that has resulted in
landslides, flash floods, inundations and sinkholes in the Gargano
Promontory, and we investigate the spatial-temporal relationships between
the intense rainfall and its ground effects. Next, in Sect. 4 we present a
new method to forecast the possible occurrence of rainfall-induced
landslides – and possibly the other associated geohydrological hazards –
based on the continuous monitoring of local rainfall conditions. This is
followed, in Sect. 5, by a discussion of the results obtained, including
general considerations on the effects of intense rainfall in karst
environments and their possible predictability using the new rainfall-based
forecasting method. We conclude (Sect. 6) summarising the lessons learnt.</p>
</sec>
<sec id="Ch1.S2">
  <title>Study area</title>
      <p>The study area covers approximately 1600 km<inline-formula><mml:math id="M1" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula> and encompasses the
Gargano Promontory that extends for a few tens of kilometres into the
Adriatic Sea, in the NE part of the Puglia region, southern Italy (Fig. 1).
The Lesina and Varano coastal lakes separate the northern side of the
promontory from the sea. Elevation in the area ranges from sea level to 1056 m a.s.l.
with a mean value of about 400 m, and morphology is controlled by
E–W- and NW–SE-trending  faults (Funiciello et al., 1988; Brankman and Aydin,
2004). Due to the presence of a well-developed karst environment, surface
hydrography is limited to a few short  ephemeral drainages along the slopes
that bound the elevated central plateau, and to the Candelaro River and
minor drainages in the alluvial and coastal plains surrounding the
promontory. In the area, sedimentary rocks crop out, chiefly carbonate
platform limestone, limited marl and residual “terra rossa” deposits
(Bosellini et al., 1999). Soils, where present, are chromic Cambisols and
Luvisols. Yearly cumulated rainfall ranges between 400 and 1200 mm, and mean
annual air temperature varies from 10 to 17 <inline-formula><mml:math id="M2" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C.
The climate  is Mediterranean to Mediterranean suboceanic. July and August are
dry, and most of the precipitation falls as rainfall from September to
November (Polemio and Lonigro, 2011). The promontory hosts the Gargano
National Park and a number of towns and villages that collectively represent
an important touristic area and a significant economic resource.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1"><caption><p>Panel <bold>(a)</bold> shows the location of the study area (red rectangle) in
Italy. Grey area is the Puglia (Apulia) region. Panel <bold>(b)</bold> shows the
location of 39 rain gauges in the study area and the neighbouring area.
Panel <bold>(c)</bold> shows the main rock types (colours) and place names in the study area.
WGS84/Pseudo Mercator (EPSG: 3857).</p></caption>
        <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/17/467/2017/nhess-17-467-2017-f01.png"/>

      </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2" specific-use="star"><caption><p>Meteorological setting for the period 1–6 September 2014 over
central and southern Italy. Images show Meteosat Second Generation (MSG) –
visible (VIS) 0.6 <inline-formula><mml:math id="M3" display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>m for <bold>(a)</bold> 1 September 2014, 12:00 UTC, <bold>(b)</bold> 2
September 2014, 12:00 UTC, <bold>(c)</bold> 3 September 2014, 12:00 UTC, <bold>(d)</bold> 6 September
2014, 12:00 UTC. Green lines show geopotential height of 500 hPa pressure
level. Black lines show mean sea level pressure. Light brown lines show
geographical boundaries. Source: <uri>http://www.eumetrain.org</uri>.</p></caption>
        <?xmltex \igopts{width=369.885827pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/17/467/2017/nhess-17-467-2017-f02.png"/>

      </fig>

      <p>Although not particularly frequent or abundant compared to other areas in
southern Italy, different geohydrological hazards have been reported in the
Gargano Promontory. In recent historical times, destructive events occurred
on 15 July 1972 (Bissanti, 1972) and 29 July 1976, when the city of
Manfredonia, to the south of the promontory (Fig. 1), suffered inundations, and
on 10–12 September 1982, when the town of San Marco in Lamis was hit by
torrential rain. Landslides were reported in 1931, 1935, 1950, 1952, 1962,
1963, 1972, 1996 and 1997  and floods in 1996, 1997, 1998, 2002, 2007 and
2011. The main landslide types are rockfalls, topples and small disrupted
rock slides that originate primarily from steep rock slopes. Flash floods
and coastal floods occur in response to intense rainfall, but are not very
frequent in the historical record. The karst environment favours the
formation of sinkholes, i.e. karst forms also known as “dolines” (Ford and
Williams, 2007), with a local density of up to 100 dolines per square
kilometre (Castiglioni and Sauro, 2000; Simone and Fiore, 2014). Sinkhole features
in the promontory range in size from small to very small,  extending
a few tens of square metres, to large and deep features including the
“Dolina Pozzatina” with a depth of 100 m and a perimeter of about 1850 m,
and to large polje, including the Sant'Egedio polje, near San Giovanni Rotondo
(Fig. 1).</p>
</sec>
<sec id="Ch1.S3">
  <title>Description of the events</title>
<sec id="Ch1.S3.SS1">
  <title>Meteorological settings</title>
      <p>The meteorological event that brought torrential rainfall in the Gargano
area began on 1 September 2014, when a perturbed nucleus originating from
northern Europe moved to lower latitudes and impacted the Italian peninsula,
starting from the northern and eastern sectors. In the early afternoon of
1 September, the central and southern parts of the Italian peninsula were
first affected (Fig. 2a). Between 2 and 3 September, the low-pressure vortex
moved towards the Ionian Sea and then to the Balkans and the Hellenic
peninsula. The meteorological situation determined an inflow of perturbed
masses of air over most of the Adriatic regions (Fig. 2b, c). The
anticlockwise circulation affected most of central and southern Italy
and persisted until 6 September. Residual perturbed meteorological
conditions remained over the southern Italian regions; in
particular
those facing the Ionian Sea, with isolated minor precipitations until the
late morning of 7 September  (Fig. 2d).</p>
</sec>
<sec id="Ch1.S3.SS2">
  <title>Rainfall events</title>
      <p>The perturbed meteorological conditions over Italy resulted in torrential
precipitation in the Gargano Promontory, with cumulated rainfall exceeding
500 mm in the 6-day period 1–6 September (Fig. 3). To study the intense
rainfall period, we used hourly rainfall records available for 39 rain
gauges pertaining to the national network of rain gauges operated in the
area by the Italian National Department of Civil Protection and the Puglia
Regional Government. Inspection of the rainfall records and of the
geographical distribution of the precipitation (Fig. 3) revealed that (i) heavy
rainfall persisted for the entire observation period, hitting
different parts of the promontory at different times, and that (ii) seven
periods could be singled out, including four rainfall (wet) periods and
three no-rainfall (dry or nearly dry) periods (Fig. 3). The rainfall
periods ranged from 8 to 49 h and were separated by dry periods  lasting between
11 and 19 h (Table 1).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3"><caption><p>Rainfall and hydrological conditions for the period 1–6 September
2014 in the Gargano Promontory. <bold>(a–f)</bold> Hourly rainfall measurements for
six rain gauges in the study area. <bold>(g)</bold> Cumulated rainfall for the same rain
gauges; inset shows location of the rain gauges. <bold>(h)</bold> River water level at
two gauging stations along the Candelaro River; inset shows location of
gauging stations. In the charts, shaded areas are rainfall (wet)  periods
(I, III, V, VII) and white areas are no-rainfall (dry) periods (II, IV,
VI).</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/17/467/2017/nhess-17-467-2017-f03.png"/>

        </fig>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T1" specific-use="star"><caption><p>Characteristics of seven periods in the sequence of rainfall events
that hit the Gargano Promontory between 1 and 6 September 2014. Start and
end times are given in UTC<inline-formula><mml:math id="M4" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>2. Rain/dry lists rainfall, wet (R) and
no-rainfall, dry or nearly dry (D), periods. Rainfall gives the
range (minimum–maximum) of the cumulated rainfall in each period. Intensity
is the average intensity in the period for the maximum cumulated rainfall.
See also Figs. 3 and  7.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="7">
     <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="right"/>
     <oasis:colspec colnum="5" colname="col5" align="left"/>
     <oasis:colspec colnum="6" colname="col6" align="right"/>
     <oasis:colspec colnum="7" colname="col7" align="right"/>
     <oasis:thead>
       <oasis:row>  
         <oasis:entry colname="col1"/>  
         <oasis:entry rowsep="1" colname="col2">Start</oasis:entry>  
         <oasis:entry rowsep="1" colname="col3">End</oasis:entry>  
         <oasis:entry rowsep="1" colname="col4">Length</oasis:entry>  
         <oasis:entry rowsep="1" colname="col5">Rain/dry</oasis:entry>  
         <oasis:entry rowsep="1" colname="col6">Rainfall</oasis:entry>  
         <oasis:entry rowsep="1" colname="col7">Intensity</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">  
         <oasis:entry colname="col1">Period</oasis:entry>  
         <oasis:entry colname="col2">day, hour</oasis:entry>  
         <oasis:entry colname="col3">day, hour</oasis:entry>  
         <oasis:entry colname="col4">hour</oasis:entry>  
         <oasis:entry colname="col5"/>  
         <oasis:entry colname="col6">mm</oasis:entry>  
         <oasis:entry colname="col7">mm h<inline-formula><mml:math id="M5" 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></oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>  
         <oasis:entry colname="col1">I</oasis:entry>  
         <oasis:entry colname="col2">1 Sep, 12:00</oasis:entry>  
         <oasis:entry colname="col3">1 Sep, 20:00</oasis:entry>  
         <oasis:entry colname="col4">8</oasis:entry>  
         <oasis:entry colname="col5">R</oasis:entry>  
         <oasis:entry colname="col6">20–50</oasis:entry>  
         <oasis:entry colname="col7">6.25</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">II</oasis:entry>  
         <oasis:entry colname="col2">1 Sep, 20:00</oasis:entry>  
         <oasis:entry colname="col3">2 Sep, 15:00</oasis:entry>  
         <oasis:entry colname="col4">19</oasis:entry>  
         <oasis:entry colname="col5">D</oasis:entry>  
         <oasis:entry colname="col6">0–6</oasis:entry>  
         <oasis:entry colname="col7">0.31</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">III</oasis:entry>  
         <oasis:entry colname="col2">2 Sep, 15:00</oasis:entry>  
         <oasis:entry colname="col3">4 Sep, 16:00</oasis:entry>  
         <oasis:entry colname="col4">49</oasis:entry>  
         <oasis:entry colname="col5">R</oasis:entry>  
         <oasis:entry colname="col6">50–440</oasis:entry>  
         <oasis:entry colname="col7">8.97</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">IV</oasis:entry>  
         <oasis:entry colname="col2">4 Sep, 16:00</oasis:entry>  
         <oasis:entry colname="col3">5 Sep, 04:00</oasis:entry>  
         <oasis:entry colname="col4">12</oasis:entry>  
         <oasis:entry colname="col5">D</oasis:entry>  
         <oasis:entry colname="col6">0–6</oasis:entry>  
         <oasis:entry colname="col7">0.50</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">V</oasis:entry>  
         <oasis:entry colname="col2">5 Sep, 04:00</oasis:entry>  
         <oasis:entry colname="col3">5 Sep, 16:00</oasis:entry>  
         <oasis:entry colname="col4">12</oasis:entry>  
         <oasis:entry colname="col5">R</oasis:entry>  
         <oasis:entry colname="col6">10–130</oasis:entry>  
         <oasis:entry colname="col7">10.83</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">VI</oasis:entry>  
         <oasis:entry colname="col2">5 Sep, 16:00</oasis:entry>  
         <oasis:entry colname="col3">6 Sep, 03:00</oasis:entry>  
         <oasis:entry colname="col4">11</oasis:entry>  
         <oasis:entry colname="col5">D</oasis:entry>  
         <oasis:entry colname="col6">0–20</oasis:entry>  
         <oasis:entry colname="col7">1.82</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">VII</oasis:entry>  
         <oasis:entry colname="col2">6 Sep, 03:00</oasis:entry>  
         <oasis:entry colname="col3">6 Sep, 14:00</oasis:entry>  
         <oasis:entry colname="col4">11</oasis:entry>  
         <oasis:entry colname="col5">R</oasis:entry>  
         <oasis:entry colname="col6">50–140</oasis:entry>  
         <oasis:entry colname="col7">12.73</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table></table-wrap>

      <p>The first rainfall period (I) lasted 8 h, from 12:00 to 20:00 UTC<inline-formula><mml:math id="M6" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>2 on
1 September. In this wet period, around 50 mm of rain was measured by
most of the rain gauges, for an average rainfall intensity of about 6.25 mm h<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>
(Fig. 3, Table 1). After a period of 19 h without rainfall
(II), the second rainfall period started (III) and was particularly severe
in the SW part of the promontory. About 400 mm was measured at the San
Giovanni Rotondo and the San Marco in Lamis rain gauges, corresponding to an
average intensity exceeding 8.2 mm h<inline-formula><mml:math id="M8" 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>, with peak values exceeding 40 mm h<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>.
Relatively smaller amounts of rainfall were recorded at the
Cagnano Varano (240 mm, most of which between 05:00 and 12:00 UTC<inline-formula><mml:math id="M10" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>2 on
4 September) and the Monte Sant'Angelo (200 mm) rain gauges. The
Vico del Gargano and the Bosco Umbra rain gauges, located in the NE part of
the promontory, recorded approximately 50 mm of rain in the period (Figs. 1,
3).</p>
      <p>Following a dry period of 12 h (IV), rainfall started again on 5
September (V), and this time it was most abundant in the NE part of the
promontory. In this period, the Bosco Umbra and Vico del Gargano rain gauges
measured slightly more and slightly less than 100 mm of rain, respectively,
corresponding to a rainfall intensity exceeding 8.0 mm h<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>. On the
opposite, southern side of the promontory, the San Marco in Lamis rain gauge
recorded only 10 mm of rainfall. In the same period (V), the San Giovanni
Rotondo and Monte Sant'Angelo rain gauges, in the SE part of the promontory,
measured about 50 mm of rainfall. Period V was followed by an 11 h nearly
dry period (VI) which ended at 03:00 UTC<inline-formula><mml:math id="M12" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>2 of 6 September 2014, when
intense rainfall started again. The last rainfall period (VII) lasted until
14:00 UTC<inline-formula><mml:math id="M13" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>2. In the 11 h period all the considered rain gauges measured
more than 50 mm of rain, with the maximum cumulated value recorded by the
Vico del Gargano rain gauge, where 140 mm of rain was  measured,
corresponding to a rainfall intensity exceeding 12.0 mm h<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>.</p>
      <p>A rank analysis of rainfall measurements for six rain gauges in the 7-year
period from April 2009 to April 2016, highlighted the severity of the 6-day
rainfall period (Fig. 4). Except for the Monte Sant'Angelo rain gauge,
located in the southern part of the promontory, the 1–6 September rainfall
period exhibited the highest cumulated rainfall in the observation period.
Adopting the classification proposed by Alpert et al. (2002), the rainfall
was “torrential” in all the considered  rain gauges and, for three of the rain gauges, it was the only torrential event in the (short) record available (Fig. 
4).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4"><caption><p>Rank order analysis of rainfall events in the Gargano Promontory
from April 2009 to April 2016. Coloured bars show cumulated event rainfall
for six rain gauges: <bold>(a)</bold> Bosco Umbra – BU, <bold>(b)</bold> Cagnano Varano – CV,
<bold>(c)</bold> Monte Sant'Angelo – MA, <bold>(d)</bold> San Giovanni Rotondo – SR, <bold>(e)</bold> San Marco in
Lamis – SM and <bold>(f)</bold> Vico del Gargano – VG. Bars arranged from high (left) to
low (right) values. Colours identify six categories of cumulated rainfall
proposed by Alpert et al. (2002). Legend: T is torrential rainfall (minimum 128 mm day<inline-formula><mml:math id="M15" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>,
HT is heavy–torrential (64–128 mm day<inline-formula><mml:math id="M16" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>, H is heavy
(32–64 mm day<inline-formula><mml:math id="M17" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>,
MH is moderate–heavy (16–32 mm day<inline-formula><mml:math id="M18" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> and LM is
light–moderate (4–16 mm day<inline-formula><mml:math id="M19" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>. Black bars with red asterisks show the
1–6 September 2014 period.</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/17/467/2017/nhess-17-467-2017-f04.png"/>

        </fig>

</sec>
<sec id="Ch1.S3.SS3">
  <title>Landslides, floods and sinkholes</title>
      <p>The sequence of intense rainfall events resulted in a number of floods,
flash floods, landslides and sinkholes and caused two flood fatalities at
Peschici and at Carpino (<uri>http://polaris.irpi.cnr.it/</uri>) and severe
socio-economic damage (Fig. 5). Throughout the promontory, the road and
railway networks were interrupted at several sites by inundations (Fig. 6a)
and landslides, and many road underpasses were clogged by debris and
sediments (Fig. 6b). In several towns and dwellings the inhabitants were
evacuated from their homes, and a number of touristic resorts were inundated
by water, mud and debris.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F5"><caption><p>Map showing location of event landslides, floods and sinkholes
triggered by the 1–6 September 2014 intense rainfall event in the Gargano
Promontory. WGS84/Pseudo Mercator (EPSG:3857).</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/17/467/2017/nhess-17-467-2017-f05.png"/>

        </fig>

      <p><?xmltex \hack{\newpage}?>The consequences of the storm of September 2014 were reported soon after
their occurrence, and a first analysis was carried out immediately in its
aftermath. The collection of information was obtained searching different
sources: (i) field surveys, (ii) technical reports produced by geologists,
and (iii) online national, regional and local newspapers.</p>
      <p>The collected information allowed the geographical
coordinates of each phenomenon, its occurrence date and the type of hazard to be reconstructed.</p>
      <p>No geological and geomorphological details were available for the
landslides, especially when the information was found in newspapers. A
specific landslide catalogue was built and managed in a GIS environment. The
catalogue lists the following items: (i) event identification code, (ii) source
of information, (iii) landslide location (geographic coordinates,
municipality, province), (iv) occurrence date and time (if available), (v) spatial
and temporal accuracy and (vi) landslide type.</p>
      <p>As concerns floods, the main information consisted of the areas of interest, the
reported damage and the extent of the flooded territory. Information on
sinkholes included the occurrence site obtained through field surveys (high
geographical accuracy) and the occurrence time, which was mostly based upon
interviews with local inhabitants (low to medium temporal accuracy).</p>
      <p>Flooding was widespread in the Candelaro catchment that bounds to the SW the
Gargano Promontory (Fig. 5). Two hydrological gauging stations, one located
where the Candelaro River crosses State Road SS 272 (W of the Gargano range)
and one where it crosses the Provincial Road SP 60 near to the outlet in the Manfredonia Gulf (Fig. 5), measured very high water levels. The upstream
gauge along the SS 272 measured a first peak of 5.30 m at 02:00 UTC<inline-formula><mml:math id="M20" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>2 on
4 September, followed by a slightly higher peak of 5.50 m at 06:30 UTC<inline-formula><mml:math id="M21" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>2.
The water level remained very sustained until 09:00 UTC<inline-formula><mml:math id="M22" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>2 and then it
diminished (Fig. 3h). At the downstream gauging station located along SP 60,
about 30 km downstream from the upstream gauge, a peak of 3.77 m was
measured at 16:00 UTC<inline-formula><mml:math id="M23" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>2 on  4 September, about 10 h later than the peak
measured by the upstream gauge. We justify the (significant) time difference
in the peak discharge by the widespread inundation of the Candelaro River
plain (Fig. 6a).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F6"><caption><p>Examples of geohydrological hazards triggered by the 1–6
September 2014 torrential rainfall in the Gargano Promontory. <bold>(a)</bold> Flood
plain inundated by the Candelaro River (photograph: Regione Puglia). <bold>(b)</bold> Inundation
in Rodi Garganico (photograph: Regione Puglia). <bold>(c, f)</bold> Shallow
landslides in the town of San Marco in Lamis. <bold>(d)</bold> Sinkhole in San Marco in
Lamis (photograph: M. Parise). <bold>(e)</bold> Shallow landslide in Cagnano Varano
(photograph: Regione Puglia). <bold>(g)</bold> Sinkhole in Monte Sant'Angelo (photograph: M. Parise).</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/17/467/2017/nhess-17-467-2017-f06.jpg"/>

        </fig>

      <p>Inundations were also severe along the northern coastal area, between Varano Lake and Vieste, and particularly between the towns of Cagnano Varano
and Carpino (Fig. 5). Near Varano Lake, large agricultural areas were
inundated. Along the northern coast of the promontory, flash floods produced
by small torrents occurred mostly on 5–6 September. In the morning of 5 September,
the Macchio Torrent overflowed and inundated Vieste, and several
touristic sites. Overflowing of minor torrents and ditches was reported in
the early hours of 6 September in the towns of Peschici, Vico del Gargano and Rodi Garganico.</p>
      <p>The torrential rain caused a number of landslides, mostly shallow landslides
(Fig. 6c, e, f). Overall, we collected information on 46 landslides,
including 14 earthflows, 14 debris flows, 11 soil slides, 4 rockfalls, 1
mudflow and 2 slope failures of undetermined type. This is a subset of all
the event landslides in the Gargano Promontory. Based on the type of
failures, we hypothesise that all the landslides were from rapid to
extremely rapid. Most of the mapped landslides were in the municipalities of
San Marco in Lamis, Ischitella and Cagnano Varano. Landslides were also
reported near San Giovanni Rotondo, Rignano Garganico and Rodi Garganico
(Fig. 5).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F7" specific-use="star"><caption><p>Analysis of the spatial and temporal distribution of the event
rainfall and of the triggered event landslides. See text for explanation.</p></caption>
          <?xmltex \igopts{width=426.791339pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/17/467/2017/nhess-17-467-2017-f07.png"/>

        </fig>

      <p>We searched information on the time or  period of occurrence of the
landslides. However, for most of the landslides the time or period of
occurrence remains unknown or suffers from very large uncertainty. For only
nine landslides we obtained reasonably accurate information on the period of
occurrence of the slope failures. On 3–4 September, four landslides
occurred near San Marco in Lamis, along SS 272, most probably in the 3 h
period between 23:00 and 02:00 UTC<inline-formula><mml:math id="M24" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>2. We consider these landslides
representative of a larger cluster in the same area (cluster A). On 4
September, a landslide occurred between 05:00 and 16:00 UTC<inline-formula><mml:math id="M25" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>2 near Cagnano
Varano (cluster B). In the same day, a single landslide occurred in the
municipality of San Giovanni Rotondo at an undetermined time between 14:00
and 21:00 UTC<inline-formula><mml:math id="M26" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>2 (cluster C). Lastly, three landslides occurred in the
night between 5 and 6 September and most probably between 23:00 and 05:00 UTC<inline-formula><mml:math id="M27" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>2,
in the municipalities of Ischitella and Rodi Garganico (cluster D).
We attribute the scarce temporal information and the poor accuracy of the
information on the time of occurrence of the failures to the difficulty  of
reaching some of the places where the landslides occurred and to the fact that
many landslides occurred in the evening or during the night and were
reported only several hours after the event.</p>
      <p>The torrential rainfall also caused sinkholes. We mapped 10  small
sinkholes near the villages of San Marco in Lamis and Monte Sant'Angelo
(Fig. 5). Based on their morphology and shape, the sinkholes were classified
as collapse or cover-collapse sinkholes (Gutiérrez et al., 2008, 2014).
At San Marco in Lamis, four sinkholes affected the lower part of a
pre-existing karst depression. The deepest sinkhole was about 6 m deep, 5 m
wide and exposed limestone and residual terra rossa deposits that
represent the upper part of the epikarst (Williams, 2008) (Fig. 6d). Other
sinkholes were less developed and were detected and mapped locally only
based upon morphological considerations. Due to the remote areas where the
sinkholes occurred, their limited sizes (Fig. 6g) and the difficulty of
detecting them, no accurate information is available on the time or period of
occurrence of the sinkholes.</p>
</sec>
<sec id="Ch1.S3.SS4">
  <title>Spatial and temporal distributions of rainfall and geohydrological
hazards</title>
      <p>To help investigate  the effect of the changing spatial and temporal
distribution of the rainfall on the location of the landslides, floods and
sinkholes, we prepared Fig. 7,   which portrays, for each period in the sequence
of rainfall events (Sect. 3.2), maps showing the spatial distributions of
the mean rainfall intensity (in mm h<inline-formula><mml:math id="M28" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>, the cumulated rainfall for the
single period and from the beginning of the event (in mm) and the location
of the landslides that occurred in each period and in previous periods.</p>
      <p>An inspection of Fig. 7 reveals that the total cumulated rainfall, exceeding
100 mm in large parts of the promontory, was the result of separate rainfall
events that hit different parts of the promontory at different times. The
first rainy period (I) was more widespread but characterised by an overall
moderate cumulated rainfall not exceeding 50 mm and rainfall intensity not
exceeding 6.2 mm h<inline-formula><mml:math id="M29" 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>. No landslides or floods were reported during the
first rainy period. The second (III) and the third (V) rainy periods were
more localised; the second was in the central part of the promontory (San Marco
in Lamis and San Giovanni Rotondo) and the third was in the NE sector of the
promontory (Ischitella, Vico del Gargano and Vieste), and were both
characterised by high values of cumulated rainfall (exceeding 400 mm in the
second and 130 mm in the third period) and of rainfall intensity (
exceeded 8.5 mm h<inline-formula><mml:math id="M30" 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> for the second period and 10.5 mm h<inline-formula><mml:math id="M31" 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> for the
third period, respectively). Landslides were reported in the central
(cluster A) and in the northern (cluster B) parts of the promontory during
the second rainfall period (III). In the same period the upstream
hydrological gauging station along the Candelaro River measured high water
flows exceeding 5.0 m (Fig. 2), about 2 h after the maximum hourly
rainfall measured at the San Marco in Lamis rain gauge, at 24:00 UTC<inline-formula><mml:math id="M32" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>2 on
3 September. The landslides occurred in areas where the total event
cumulated rainfall exceeded 400 mm (for cluster A) and 200 mm (for cluster B).</p>
      <p>In the central part of the promontory, landslides were also reported
(cluster C) during the second dry period (IV). Given the poor temporal
accuracy of these landslides (i.e. between 14:00 and 21:00 UTC<inline-formula><mml:math id="M33" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>2 on 4 September),
we cannot exclude that the failures occurred during the last few
hours of the previous rainfall period (III). The hypothesis is supported by
the fact that the San Giovanni Rotondo rain gauge measured rainfall until
15:00 UTC<inline-formula><mml:math id="M34" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>2 on 4 September (Fig. 2). The last rainfall period (VII) was
again characterised by widespread rainfall throughout most of the promontory
with a distinct peak in the NE sector exceeding 130 mm. Where rainfall
intensity was particularly intense (&gt; 11 mm h<inline-formula><mml:math id="M35" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> in the NE
part of the promontory, between Rodi Garganico and Peschici, landslides were
also reported (cluster D).</p>
</sec>
</sec>
<sec id="Ch1.S4">
  <title>Geohydrological hazards forecasting algorithm</title>
      <p>We used the rainfall records and hazard information available for the
Gargano event to design and test an algorithm for the possible operational
forecasting of rainfall-induced landslides and other geohydrological
hazards, including flash floods and sinkholes</p>
<sec id="Ch1.S4.SS1">
  <title>The E-NEP algorithm</title>
      <p>The ensemble–non-exceedance probability (E-NEP) algorithm exploits a
standard rainfall record obtained by a rain gauge to trace in time the
probability of possible landslide occurrence and of related
geohydrological hazards. For the purpose, for each time <inline-formula><mml:math id="M36" display="inline"><mml:mrow><mml:msub><mml:mi>t</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, E-NEP
calculates the event rainfall duration <inline-formula><mml:math id="M37" display="inline"><mml:mi>D</mml:mi></mml:math></inline-formula>, and the corresponding event
cumulated rainfall <inline-formula><mml:math id="M38" display="inline"><mml:mi>E</mml:mi></mml:math></inline-formula>, for increasing antecedent periods before <inline-formula><mml:math id="M39" display="inline"><mml:mrow><mml:msub><mml:mi>t</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, from
<inline-formula><mml:math id="M40" display="inline"><mml:mrow><mml:msub><mml:mi>t</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> to <inline-formula><mml:math id="M41" display="inline"><mml:mrow><mml:msub><mml:mi>t</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mo>+</mml:mo><mml:mi>T</mml:mi></mml:mrow></mml:math></inline-formula>, in <inline-formula><mml:math id="M42" display="inline"><mml:mi>d</mml:mi></mml:math></inline-formula> time steps, with <inline-formula><mml:math id="M43" display="inline"><mml:mi>T</mml:mi></mml:math></inline-formula> the maximum length of the
considered antecedent rainfall period and <inline-formula><mml:math id="M44" display="inline"><mml:mi>d</mml:mi></mml:math></inline-formula> the time step used to increment
the duration of the antecedent rainfall period. For each
rainfall-duration–event-cumulated-rainfall pair the corresponding
non-exceedance probability (NEP) <inline-formula><mml:math id="M45" display="inline"><mml:mrow><mml:mi>p</mml:mi><mml:mo>(</mml:mo><mml:mi>D</mml:mi><mml:mo>,</mml:mo><mml:mi>E</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> is obtained using the probabilistic
approach proposed by Brunetti et al. (2010) and modified by Peruccacci
et al. (2012) for the definition of empirical rainfall thresholds for possible
landslide occurrence (Guzzetti et al., 2007). The set of the NEP values
(i.e. <inline-formula><mml:math id="M46" display="inline"><mml:mo mathvariant="italic">{</mml:mo></mml:math></inline-formula>NEP<inline-formula><mml:math id="M47" display="inline"><mml:mo mathvariant="italic">}</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M48" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M49" display="inline"><mml:mrow><mml:mo mathvariant="italic">{</mml:mo><mml:mi>p</mml:mi><mml:mo>(</mml:mo><mml:mi>D</mml:mi><mml:mo>,</mml:mo><mml:mi>E</mml:mi><mml:mo>)</mml:mo><mml:mo mathvariant="italic">}</mml:mo></mml:mrow></mml:math></inline-formula>) is then used to determine an ensemble of metrics,
including the maximum value of the NEP (NEP<inline-formula><mml:math id="M50" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mi mathvariant="normal">max</mml:mi></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>, the 10th, 25th, 50th,
75th and 90th percentiles (NEP<inline-formula><mml:math id="M51" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">10</mml:mn></mml:msub></mml:math></inline-formula>, NEP<inline-formula><mml:math id="M52" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">25</mml:mn></mml:msub></mml:math></inline-formula>, NEP<inline-formula><mml:math id="M53" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">50</mml:mn></mml:msub></mml:math></inline-formula>, NEP<inline-formula><mml:math id="M54" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">75</mml:mn></mml:msub></mml:math></inline-formula>,
NEP<inline-formula><mml:math id="M55" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">90</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>, and the rainfall duration (<inline-formula><mml:math id="M56" display="inline"><mml:mrow><mml:msub><mml:mi>D</mml:mi><mml:mi mathvariant="normal">NEPmax</mml:mi></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> associated with
NEP<inline-formula><mml:math id="M57" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">max</mml:mi></mml:msub></mml:math></inline-formula>, that collectively are exploited for landslide forecasting. The
process is repeated at regular time intervals (<inline-formula><mml:math id="M58" display="inline"><mml:mi>z</mml:mi></mml:math></inline-formula>, where <inline-formula><mml:math id="M59" display="inline"><mml:mrow><mml:msub><mml:mi>t</mml:mi><mml:mrow><mml:mi>i</mml:mi><mml:mo>+</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msub><mml:mo>=</mml:mo></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M60" display="inline"><mml:mrow><mml:msub><mml:mi>t</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mo>+</mml:mo><mml:mi>z</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>,
allowing the temporal evolution of the probability
of possible occurrence of rainfall-induced landslides and of related
geohydrological hazards to be followed.</p>
      <p>Figure 8 portrays the logical schema for the E-NEP algorithm, which consists
of two nested loops. First, the maximum length of the considered rainfall period, <inline-formula><mml:math id="M61" display="inline"><mml:mi>T</mml:mi></mml:math></inline-formula> (in hours),
the time step to increment the duration of the considered antecedent rainfall, d (in hours)
and the time interval before the next set of (<inline-formula><mml:math id="M62" display="inline"><mml:mrow><mml:mi>D</mml:mi><mml:mo>,</mml:mo><mml:mi>E</mml:mi></mml:mrow></mml:math></inline-formula>) pairs is computed, <inline-formula><mml:math id="M63" display="inline"><mml:mi>z</mml:mi></mml:math></inline-formula> (in hours),
are set to user-defined values. We stress that the three time (duration) variables are independent,
with the only constraint that <inline-formula><mml:math id="M64" display="inline"><mml:mrow><mml:mi>d</mml:mi><mml:mo>≤</mml:mo><mml:mi>T</mml:mi></mml:mrow></mml:math></inline-formula>. Next, the external loop (cyan in Fig. 8)
starts, the rainfall duration <inline-formula><mml:math id="M65" display="inline"><mml:mi>D</mml:mi></mml:math></inline-formula> is set to <inline-formula><mml:math id="M66" display="inline"><mml:mi>d</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M67" display="inline"><mml:mo mathvariant="italic">{</mml:mo></mml:math></inline-formula>NEP<inline-formula><mml:math id="M68" display="inline"><mml:mo mathvariant="italic">}</mml:mo></mml:math></inline-formula>
is set to null (an empty set). Next, the internal loop
(orange in Fig. 8) starts and for the given rainfall duration <inline-formula><mml:math id="M69" display="inline"><mml:mi>D</mml:mi></mml:math></inline-formula>, the
corresponding cumulated rainfall <inline-formula><mml:math id="M70" display="inline"><mml:mi>E</mml:mi></mml:math></inline-formula> is determined, and the probability of
landslide occurrence <inline-formula><mml:math id="M71" display="inline"><mml:mrow><mml:mi>p</mml:mi><mml:mo>(</mml:mo><mml:mi>D</mml:mi><mml:mo>,</mml:mo><mml:mi>E</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> is computed adopting the method proposed by
Brunetti et al. (2010) and Peruccacci et al. (2012) and stored in
<inline-formula><mml:math id="M72" display="inline"><mml:mo mathvariant="italic">{</mml:mo></mml:math></inline-formula>NEP<inline-formula><mml:math id="M73" display="inline"><mml:mo mathvariant="italic">}</mml:mo></mml:math></inline-formula>. The rainfall duration <inline-formula><mml:math id="M74" display="inline"><mml:mi>D</mml:mi></mml:math></inline-formula> is then
incremented (<inline-formula><mml:math id="M75" display="inline"><mml:mrow><mml:mi>D</mml:mi><mml:mo>=</mml:mo><mml:mi>D</mml:mi><mml:mo>+</mml:mo><mml:mi>d</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> and tested to verify whether  it is larger than <inline-formula><mml:math id="M76" display="inline"><mml:mi>T</mml:mi></mml:math></inline-formula>. If <inline-formula><mml:math id="M77" display="inline"><mml:mrow><mml:mi>D</mml:mi><mml:mo>≤</mml:mo><mml:mi>T</mml:mi></mml:mrow></mml:math></inline-formula>,
the internal loop is repeated using the current value of <inline-formula><mml:math id="M78" display="inline"><mml:mi>D</mml:mi></mml:math></inline-formula> and the
corresponding <inline-formula><mml:math id="M79" display="inline"><mml:mi>E</mml:mi></mml:math></inline-formula>; otherwise (<inline-formula><mml:math id="M80" display="inline"><mml:mi>D</mml:mi></mml:math></inline-formula> &gt; <inline-formula><mml:math id="M81" display="inline"><mml:mi>T</mml:mi></mml:math></inline-formula>) the loop ends, and the ensemble of metrics of
<inline-formula><mml:math id="M82" display="inline"><mml:mo mathvariant="italic">{</mml:mo></mml:math></inline-formula>NEP<inline-formula><mml:math id="M83" display="inline"><mml:mo mathvariant="italic">}</mml:mo></mml:math></inline-formula> (NEP<inline-formula><mml:math id="M84" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">10</mml:mn></mml:msub></mml:math></inline-formula>, NEP<inline-formula><mml:math id="M85" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">25</mml:mn></mml:msub></mml:math></inline-formula>, NEP<inline-formula><mml:math id="M86" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">50</mml:mn></mml:msub></mml:math></inline-formula>,
NEP<inline-formula><mml:math id="M87" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">75</mml:mn></mml:msub></mml:math></inline-formula>, NEP<inline-formula><mml:math id="M88" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">90</mml:mn></mml:msub></mml:math></inline-formula>, NEP<inline-formula><mml:math id="M89" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mi mathvariant="normal">max</mml:mi></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> and the value of <inline-formula><mml:math id="M90" display="inline"><mml:mrow><mml:msub><mml:mi>D</mml:mi><mml:mi mathvariant="normal">NEPmax</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> are
calculated. The external loop is then repeated after the user-defined time
interval of <inline-formula><mml:math id="M91" display="inline"><mml:mi>z</mml:mi></mml:math></inline-formula> hours.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F8"><caption><p>Logical scheme for the E-NEP algorithm.  <inline-formula><mml:math id="M92" display="inline"><mml:mi>D</mml:mi></mml:math></inline-formula> is rainfall duration in
hours. <inline-formula><mml:math id="M93" display="inline"><mml:mi>E</mml:mi></mml:math></inline-formula> is cumulated rainfall in milimetres. <inline-formula><mml:math id="M94" display="inline"><mml:mi>T</mml:mi></mml:math></inline-formula> is maximum length of the considered
rainfall period in hours. <inline-formula><mml:math id="M95" display="inline"><mml:mi>d</mml:mi></mml:math></inline-formula> is the time step used to increment the duration of the
rainfall period, up to <inline-formula><mml:math id="M96" display="inline"><mml:mi>T</mml:mi></mml:math></inline-formula> in hours. <inline-formula><mml:math id="M97" display="inline"><mml:mi>z</mml:mi></mml:math></inline-formula> is the time interval before the next set of
(<inline-formula><mml:math id="M98" display="inline"><mml:mrow><mml:mi>D</mml:mi><mml:mo>,</mml:mo><mml:mi>E</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> pairs is computed, in hours. <inline-formula><mml:math id="M99" display="inline"><mml:mo mathvariant="italic">{</mml:mo></mml:math></inline-formula>NEP<inline-formula><mml:math id="M100" display="inline"><mml:mo mathvariant="italic">}</mml:mo></mml:math></inline-formula> is the set of
non-exceedance probability (NEP) values obtained for each (<inline-formula><mml:math id="M101" display="inline"><mml:mrow><mml:mi>D</mml:mi><mml:mo>,</mml:mo><mml:mi>E</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> pair adopting
the method proposed by Brunetti et al. (2010) and Peruccacci et al. (2012).
Statistics of <inline-formula><mml:math id="M102" display="inline"><mml:mo mathvariant="italic">{</mml:mo></mml:math></inline-formula>NEP<inline-formula><mml:math id="M103" display="inline"><mml:mo mathvariant="italic">}</mml:mo></mml:math></inline-formula> are 10th, 25th, 50th, 75th and 90th percentiles. and NEP<inline-formula><mml:math id="M104" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">max</mml:mi></mml:msub></mml:math></inline-formula> is the maximum value of NEP.
<inline-formula><mml:math id="M105" display="inline"><mml:mrow><mml:msub><mml:mi>D</mml:mi><mml:mi mathvariant="normal">NEPmax</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, event rainfall duration corresponding to NEP<inline-formula><mml:math id="M106" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">max</mml:mi></mml:msub></mml:math></inline-formula>. External
(blue) loop is run every <inline-formula><mml:math id="M107" display="inline"><mml:mi>z</mml:mi></mml:math></inline-formula> hours or fraction of hour. Internal (orange) loop
runs from <inline-formula><mml:math id="M108" display="inline"><mml:mi>d</mml:mi></mml:math></inline-formula> to <inline-formula><mml:math id="M109" display="inline"><mml:mi>T</mml:mi></mml:math></inline-formula>, in <inline-formula><mml:math id="M110" display="inline"><mml:mi>d</mml:mi></mml:math></inline-formula> time steps. In Figs. 9, 10 <inline-formula><mml:math id="M111" display="inline"><mml:mi>z</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M112" display="inline"><mml:mi>d</mml:mi></mml:math></inline-formula> were set to 1 h and
<inline-formula><mml:math id="M113" display="inline"><mml:mi>T</mml:mi></mml:math></inline-formula> to 96 h. See text for explanation.</p></caption>
          <?xmltex \igopts{width=142.26378pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/17/467/2017/nhess-17-467-2017-f08.png"/>

        </fig>

      <p>Figure 9 exemplifies the application of the E-NEP algorithm to a specific
rainfall record, at a given time <inline-formula><mml:math id="M114" display="inline"><mml:mrow><mml:msub><mml:mi>t</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> (i.e. the application of the orange
internal loop of Fig. 8), for an antecedent period <inline-formula><mml:math id="M115" display="inline"><mml:mrow><mml:mi>T</mml:mi><mml:mo>=</mml:mo></mml:mrow></mml:math></inline-formula> 96 h, with <inline-formula><mml:math id="M116" display="inline"><mml:mrow><mml:mi>d</mml:mi><mml:mo>=</mml:mo></mml:mrow></mml:math></inline-formula> 1 h. E-NEP calculates the cumulated event rainfall <inline-formula><mml:math id="M117" display="inline"><mml:mi>E</mml:mi></mml:math></inline-formula> for increasing
durations <inline-formula><mml:math id="M118" display="inline"><mml:mi>D</mml:mi></mml:math></inline-formula> from 1 (<inline-formula><mml:math id="M119" display="inline"><mml:mrow><mml:msub><mml:mi>t</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula>) to 96 h (<inline-formula><mml:math id="M120" display="inline"><mml:mrow><mml:msub><mml:mi>t</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:mn mathvariant="normal">96</mml:mn></mml:mrow></mml:math></inline-formula>), every hour (time step <inline-formula><mml:math id="M121" display="inline"><mml:mrow><mml:mi>d</mml:mi><mml:mo>=</mml:mo></mml:mrow></mml:math></inline-formula> 1).
The individual (<inline-formula><mml:math id="M122" display="inline"><mml:mrow><mml:mi>D</mml:mi><mml:mo>,</mml:mo><mml:mi>E</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> pairs are plotted as grey dots in Fig. 9d. For each pair,
the corresponding NEP, the non-exceedance probability of possible landslide occurrence, was calculated and is shown by the blue squares in Fig. 9d. To further clarify the operations performed by the E-NEP algorithm,
the bar charts in Fig. 9a, b, c show, for the same time <inline-formula><mml:math id="M123" display="inline"><mml:mrow><mml:msub><mml:mi>t</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, three
antecedent rainfall periods corresponding to durations of <inline-formula><mml:math id="M124" display="inline"><mml:mrow><mml:mi>D</mml:mi><mml:mo>=</mml:mo></mml:mrow></mml:math></inline-formula> 6 h (red
bars), <inline-formula><mml:math id="M125" display="inline"><mml:mrow><mml:mi>D</mml:mi><mml:mo>=</mml:mo></mml:mrow></mml:math></inline-formula> 16 h (green bars) and <inline-formula><mml:math id="M126" display="inline"><mml:mrow><mml:mi>D</mml:mi><mml:mo>=</mml:mo></mml:mrow></mml:math></inline-formula> 44 h (yellow bars). The
corresponding cumulated event rainfall (red, green, yellow circles) and the
associated non-exceedance probability values (red, green, yellow squares)
are  shown in Fig. 9d. Lastly, the box plot to the right of Fig. 9d portrays
(i) the ensemble of metrics of <inline-formula><mml:math id="M127" display="inline"><mml:mo mathvariant="italic">{</mml:mo></mml:math></inline-formula>NEP<inline-formula><mml:math id="M128" display="inline"><mml:mo mathvariant="italic">}</mml:mo></mml:math></inline-formula>:
NEP<inline-formula><mml:math id="M129" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">10</mml:mn></mml:msub></mml:math></inline-formula>, NEP<inline-formula><mml:math id="M130" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">25</mml:mn></mml:msub></mml:math></inline-formula>, NEP<inline-formula><mml:math id="M131" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">50</mml:mn></mml:msub></mml:math></inline-formula>, NEP<inline-formula><mml:math id="M132" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">75</mml:mn></mml:msub></mml:math></inline-formula> and NEP<inline-formula><mml:math id="M133" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">90</mml:mn></mml:msub></mml:math></inline-formula> and the
maximum value of the non-exceedance probability, NEP<inline-formula><mml:math id="M134" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">max</mml:mi></mml:msub></mml:math></inline-formula>. In Fig. 9d,
the green square identifies NEP<inline-formula><mml:math id="M135" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">max</mml:mi></mml:msub></mml:math></inline-formula>, i.e. the non-exceedance probability
corresponding to the most critical rainfall condition for possible landslide
occurrence in the considered rainfall period. The corresponding duration
(<inline-formula><mml:math id="M136" display="inline"><mml:mrow><mml:mi>D</mml:mi><mml:mo>=</mml:mo></mml:mrow></mml:math></inline-formula> 16 h) represents the <inline-formula><mml:math id="M137" display="inline"><mml:mrow><mml:msub><mml:mi>D</mml:mi><mml:mi mathvariant="normal">NEPmax</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> value.</p>
</sec>
<sec id="Ch1.S4.SS2">
  <title>Application and discussion of the E-NEP algorithm</title>
      <p>We applied the E-NEP algorithm to the 13-day period between 31 August and
12 September,
which encompasses the entire series of rainfall events that hit the
Gargano Promontory. We applied the algorithm to synthetic hourly rainfall
records reconstructed for the locations of the four spatial-temporal
landslide clusters identified in the study area (Fig. 7). To reconstruct the
synthetic rainfall records, we interpolated the hourly rainfall measurements
obtained by 39 rain gauges in the Gargano Promontory and the surrounding
regions at the landslide locations. For that purpose, we used a standard
inverse weighted distance (IDW) spatial interpolator (Shepard, 1968) to
obtain hourly rainfall values on a regular 500 m <inline-formula><mml:math id="M138" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 500 m grid.
Next, the hourly rainfall grids were sampled at the grid cells selected to
represent the four landslide clusters A, B, C and D, and the synthetic
hourly rainfall time series were reconstructed for each landslide cluster.</p>
      <p>For our analysis, and for each landslide cluster, <inline-formula><mml:math id="M139" display="inline"><mml:mrow><mml:msub><mml:mi>t</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> ranged from 31
August, 00:00 UTC<inline-formula><mml:math id="M140" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>2 to 11 September, 24:00 UTC<inline-formula><mml:math id="M141" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>2, in regular 1 h time
intervals (<inline-formula><mml:math id="M142" display="inline"><mml:mrow><mml:mi>z</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>, corresponding to a total of 288 time intervals. For each
<inline-formula><mml:math id="M143" display="inline"><mml:mrow><mml:msub><mml:mi>t</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, E-NEP computed the NEP<inline-formula><mml:math id="M144" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">10</mml:mn></mml:msub></mml:math></inline-formula>, NEP<inline-formula><mml:math id="M145" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">25</mml:mn></mml:msub></mml:math></inline-formula>, NEP<inline-formula><mml:math id="M146" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">50</mml:mn></mml:msub></mml:math></inline-formula>, NEP<inline-formula><mml:math id="M147" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">75</mml:mn></mml:msub></mml:math></inline-formula> and NEP<inline-formula><mml:math id="M148" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">90</mml:mn></mml:msub></mml:math></inline-formula> percentiles, the NEP<inline-formula><mml:math id="M149" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">max</mml:mi></mml:msub></mml:math></inline-formula> and the corresponding
<inline-formula><mml:math id="M150" display="inline"><mml:mrow><mml:msub><mml:mi>D</mml:mi><mml:mi mathvariant="normal">NEPmax</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>.</p>
      <p>Results of the analysis of the four landslide
clusters are shown in Fig. 10, in which  the single plots show, from top to bottom, the temporal
evolution of (i) the measured and the cumulated rainfall, (ii) the
NEP<inline-formula><mml:math id="M151" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">10</mml:mn></mml:msub></mml:math></inline-formula>, NEP<inline-formula><mml:math id="M152" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">25</mml:mn></mml:msub></mml:math></inline-formula>, NEP<inline-formula><mml:math id="M153" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">50</mml:mn></mml:msub></mml:math></inline-formula>, NEP<inline-formula><mml:math id="M154" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">75</mml:mn></mml:msub></mml:math></inline-formula>, NEP<inline-formula><mml:math id="M155" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">90</mml:mn></mml:msub></mml:math></inline-formula> percentiles
(shown in ranges, by two different shades of blue and by the thick blue
line) and NEP<inline-formula><mml:math id="M156" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">max</mml:mi></mml:msub></mml:math></inline-formula> (purple line) and (iii) the corresponding
<inline-formula><mml:math id="M157" display="inline"><mml:mrow><mml:msub><mml:mi>D</mml:mi><mml:mi mathvariant="normal">NEPmax</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> (green line). Figure 10 also shows (i) with grey areas, the
possible period of occurrence of the landslides, a measure of the
uncertainty in the failure occurrence time and (ii) with a vertical blue
line the time of the high peak measured by the Candelaro gauge along SS 272
(Fig. 10a, Fig. 3).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F9"><caption><p>Exemplification of the E-NEP algorithm used to provide a
non-exceedance probability (NEP) of possible landslide occurrence. Panels <bold>(a)</bold>,
<bold>(b)</bold> and
<bold>(c)</bold> show the same rainfall record and three antecedent conditions
corresponding to durations of <bold>(a)</bold> <inline-formula><mml:math id="M158" display="inline"><mml:mrow><mml:mi>D</mml:mi><mml:mo>=</mml:mo></mml:mrow></mml:math></inline-formula> 6 h (red bars), <bold>(b)</bold> <inline-formula><mml:math id="M159" display="inline"><mml:mrow><mml:mi>D</mml:mi><mml:mo>=</mml:mo></mml:mrow></mml:math></inline-formula> 16 h
(green bars) and <bold>(c)</bold> <inline-formula><mml:math id="M160" display="inline"><mml:mrow><mml:mi>D</mml:mi><mml:mo>=</mml:mo></mml:mrow></mml:math></inline-formula> 44 h (yellow bars). Panel <bold>(d)</bold> shows rainfall
(<inline-formula><mml:math id="M161" display="inline"><mml:mrow><mml:mi>D</mml:mi><mml:mo>,</mml:mo><mml:mi>E</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> pairs (grey dots); red, green and yellow dots represent the (<inline-formula><mml:math id="M162" display="inline"><mml:mrow><mml:mi>D</mml:mi><mml:mo>,</mml:mo><mml:mi>E</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> pairs
corresponding to the conditions shown in <bold>(a)</bold>, <bold>(b)</bold> and <bold>(c)</bold>. Blue squares
show the corresponding non-exceedance probabilities (NEP). Green square
represents NEP<inline-formula><mml:math id="M163" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">max</mml:mi></mml:msub></mml:math></inline-formula>. See text for explanation.</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/17/467/2017/nhess-17-467-2017-f09.png"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F10" specific-use="star"><caption><p>Results of the application of the E-NEP algorithm to synthetic
rainfall records reconstructed for the locations of four landslide
clusters.
<bold>(a)</bold> Landslide cluster A, <bold>(b)</bold> landslide cluster B, <bold>(c)</bold> landslide cluster
C, <bold>(d)</bold> landslide cluster D. Each panel shows, from top to bottom, (1) hourly
rainfall record (blue bars) and cumulated event rainfall (red line); (2)
median, E-NEP<inline-formula><mml:math id="M164" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">50</mml:mn></mml:msub></mml:math></inline-formula> (orange line) and maximum, E-NEP<inline-formula><mml:math id="M165" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">max</mml:mi></mml:msub></mml:math></inline-formula> (purple line)
values of the non-exceedance probability with ranges E-NEP<inline-formula><mml:math id="M166" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">25</mml:mn></mml:msub></mml:math></inline-formula>–E-NEP<inline-formula><mml:math id="M167" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">75</mml:mn></mml:msub></mml:math></inline-formula>
(dark blue shade) and E-NEP<inline-formula><mml:math id="M168" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">10</mml:mn></mml:msub></mml:math></inline-formula>–E-NEP<inline-formula><mml:math id="M169" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">90</mml:mn></mml:msub></mml:math></inline-formula> (light blue
shade); (3) rainfall duration corresponding to the most critical rainfall
condition, D-NEP<inline-formula><mml:math id="M170" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">max</mml:mi></mml:msub></mml:math></inline-formula> (green line). The period of occurrence of the
landslides (identified by the landslide road sign) is shown by a grey shaded
area. The occurrence time (and the associated uncertainty) of nine
landslides (cf. Sect. 3.3) is used to define the landslide occurrence
period of the four clusters. The time of occurrence of peak flow (identified
by the flood road sign) is shown by the vertical blue line. See text for
explanation.</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/17/467/2017/nhess-17-467-2017-f10.png"/>

        </fig>

      <p>For cluster A, encompassing landslides occurred along State Road SS 272 and
SP 48 near San Marco in Lamis; a short rainfall burst hit the landslide area
at 12:00 UTC<inline-formula><mml:math id="M171" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> on 1 September and stopped shortly afterward (Fig. 10a1, I in Fig. 3). In this period, the NEP<inline-formula><mml:math id="M172" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">max</mml:mi></mml:msub></mml:math></inline-formula> increased rapidly to 0.15
and decreased immediately afterwards due to  a lack of rainfall (Fig. 10 a2).
Next, following a dry period of 19 h (II in Fig. 3), the main rainfall
event started at 16:00 UTC<inline-formula><mml:math id="M173" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>2 on 2 September (Fig. 10a1, III in Fig. 3).
As a result of this second, intense rainfall event all the NEP percentiles
increased abruptly and significantly (Fig. 10a2), with NEP<inline-formula><mml:math id="M174" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">max</mml:mi></mml:msub></mml:math></inline-formula>
exceeding 0.99 at 23:00 UTC<inline-formula><mml:math id="M175" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>2 on 3 September. The landslides of cluster A
followed shortly afterward.</p>
      <p>Following the landslide occurrence, all the NEP values remained high for 12 h. When the rainfall stopped, at 14:00 UTC<inline-formula><mml:math id="M176" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>2 on 4 September, the NEP
percentiles decreased, beginning with NEP10 and continuing with the other
(larger) percentiles. NEP<inline-formula><mml:math id="M177" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">max</mml:mi></mml:msub></mml:math></inline-formula> decreased below 0.25 at 21:00 UTC<inline-formula><mml:math id="M178" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>2 on
8 September. The analysis of the temporal trend of <inline-formula><mml:math id="M179" display="inline"><mml:mrow><mml:msub><mml:mi>D</mml:mi><mml:mi mathvariant="normal">NEPmax</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> (Fig. 10a3),
the rainfall duration corresponding to largest NEP, is of interest.
<inline-formula><mml:math id="M180" display="inline"><mml:mrow><mml:msub><mml:mi>D</mml:mi><mml:mi mathvariant="normal">NEPmax</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> (i) increased in response to the first rainfall period (I in
Fig. 3), (ii) kept rising during the first dry period (II in Fig. 3), (iii) dropped
to zero during the second (main) rainfall period and precisely when
the rainfall intensity reached a maximum value of 7 mm h<inline-formula><mml:math id="M181" 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> (III in Fig. 3),
(iv) increased steadily for 94 h and (iv) remained high until
almost the end of the considered period.</p>
      <p>We observe that landslides in cluster A occurred when the NEP<inline-formula><mml:math id="M182" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">max</mml:mi></mml:msub></mml:math></inline-formula> was
close to its maximum possible value (NEP<inline-formula><mml:math id="M183" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mi mathvariant="normal">max</mml:mi></mml:msub><mml:mo>=</mml:mo></mml:mrow></mml:math></inline-formula> 1), a very critical
condition for possible landslide initiation (Brunetti et al., 2010;
Peruccacci et al., 2012).  Just before the landslide occurrence (i) NEP<inline-formula><mml:math id="M184" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">50</mml:mn></mml:msub></mml:math></inline-formula>
was close to NEP<inline-formula><mml:math id="M185" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">max</mml:mi></mml:msub></mml:math></inline-formula>; i.e. the median value was close to the
maximum value of the non-exceedance probability, (ii) the inter-percentile
ranges NEP<inline-formula><mml:math id="M186" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">10</mml:mn></mml:msub></mml:math></inline-formula>–NEP<inline-formula><mml:math id="M187" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">90</mml:mn></mml:msub></mml:math></inline-formula> and NEP<inline-formula><mml:math id="M188" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">25</mml:mn></mml:msub></mml:math></inline-formula>–NEP<inline-formula><mml:math id="M189" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">75</mml:mn></mml:msub></mml:math></inline-formula> were narrow and
(iii) there was a sudden increase of all NEP values, particularly of the
lower percentiles (i.e. NEP<inline-formula><mml:math id="M190" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">10</mml:mn></mml:msub></mml:math></inline-formula>, NEP<inline-formula><mml:math id="M191" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">25</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> (Fig. 10a2). We further
observe that landslides in this cluster occurred after <inline-formula><mml:math id="M192" display="inline"><mml:mrow><mml:msub><mml:mi>D</mml:mi><mml:mi mathvariant="normal">NEPmax</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>
began to rise following a sudden drop (Fig. 10a3).</p>
      <p>Inspection of the other plots in Fig. 10 reveals significant similarities
in the temporal evolution of the metrics computed by the E-NEP algorithm for
the other three landslide clusters, when compared to the same metrics
computed for cluster A. Specifically, (i) all landslides occurred when the
NEPmax was close to its maximum value, and immediately before landslide
occurrence
(ii) NEP50 was close to NEPmax, (iii) the range NEP25-NEP75 was narrow, (iv) there was a sudden increase of all NEP percentiles (Fig. 10a2) except NEP10
(Fig. 10c2) and (v) the landslides occurred after the DNEPmax had started to rise following a previous sudden drop. We consider these observations diagnostic of the
rainfall conditions that have resulted in landslides (and other
geohydrological hazards) in the Gargano Promontory in the period 1–6 September
2014.</p>
</sec>
</sec>
<sec id="Ch1.S5">
  <title>Discussion</title>
      <p>The analysis of the rainfall records and the geohydrological hazard
information available for the Gargano Promontory rainfall events between 1
and 6 September 2014 (Sect. 3) and their application to test the ensemble–non-exceedance probability (E-NEP) algorithm (Sect. 4) allows for
general and specific considerations.</p>
      <p>We first observe that landslides in the four examined clusters occurred for
different levels of the cumulated event rainfall, <inline-formula><mml:math id="M193" display="inline"><mml:mi>E</mml:mi></mml:math></inline-formula> (Fig. 7, Table 1). We
also observe that rainfall intensity was very high in the period of the
failures or immediately before it, but also that periods of high rainfall
intensity were not associated with  (known) landslides (see e.g. clusters C
and D; Fig. 10b, c). We conclude that, in the case of the investigated
rainfall events, single metrics like the event cumulated rainfall <inline-formula><mml:math id="M194" display="inline"><mml:mi>E</mml:mi></mml:math></inline-formula> and the
rainfall intensity <inline-formula><mml:math id="M195" display="inline"><mml:mi>I</mml:mi></mml:math></inline-formula>, on their own, were not singularly diagnostic of the
rainfall conditions that have resulted in the known landslides.</p>
      <p>As discussed in Sect. 4.2, a number of potentially diagnostic observations
drawn from the ensemble of metrics produced by the E-NEP algorithm were
common to all the examined landslide clusters, including the facts that (i) all
the landslides occurred when NEP<inline-formula><mml:math id="M196" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">max</mml:mi></mml:msub></mml:math></inline-formula> was close to its maximum
possible value, and that (ii) shortly before landslide occurrence there was
a sudden increase in all NEP percentiles (except NEP<inline-formula><mml:math id="M197" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">10</mml:mn></mml:msub></mml:math></inline-formula> locally, Fig. 10c2),
NEP<inline-formula><mml:math id="M198" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">50</mml:mn></mml:msub></mml:math></inline-formula> was close to NEP<inline-formula><mml:math id="M199" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">max</mml:mi></mml:msub></mml:math></inline-formula>, and the interquartile range
NEP<inline-formula><mml:math id="M200" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">25</mml:mn></mml:msub></mml:math></inline-formula>–NEP<inline-formula><mml:math id="M201" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">75</mml:mn></mml:msub></mml:math></inline-formula> was narrow. Following landslides occurrence,
NEP<inline-formula><mml:math id="M202" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">max</mml:mi></mml:msub></mml:math></inline-formula> remained typically sustained for long periods, but the NEP
percentiles dropped more or less rapidly, even when additional rainfall
fell in the area. We observe that no information on landslide occurrence was
reported when NEP<inline-formula><mml:math id="M203" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">50</mml:mn></mml:msub></mml:math></inline-formula> was low or very low. A further observation is that
landslides occurred shortly after the <inline-formula><mml:math id="M204" display="inline"><mml:mrow><mml:msub><mml:mi>D</mml:mi><mml:mi mathvariant="normal">NEPmax</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> had started to rise
following a previous drop. A sudden drop of <inline-formula><mml:math id="M205" display="inline"><mml:mrow><mml:msub><mml:mi>D</mml:mi><mml:mi mathvariant="normal">NEPmax</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is always related
to an increase in NEP<inline-formula><mml:math id="M206" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">max</mml:mi></mml:msub></mml:math></inline-formula> that is determined by an increase in the
rainfall intensity. However, a small increase in rainfall intensity may not
be sufficient to cause <inline-formula><mml:math id="M207" display="inline"><mml:mrow><mml:msub><mml:mi>D</mml:mi><mml:mi mathvariant="normal">NEPmax</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> to drop. We argue that visual analysis
of the temporal evolution of <inline-formula><mml:math id="M208" display="inline"><mml:mrow><mml:msub><mml:mi>D</mml:mi><mml:mi mathvariant="normal">NEPmax</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> can be exploited to provide
indications of the rapid change of the possible critical rainfall conditions
that may lead to slope failures shortly afterwards.</p>
      <p>We conclude that the ensemble of the metrics produced by the E-NEP algorithm
provides better diagnostic results than the single metrics often used for
landslide forecasting, including rainfall duration, cumulated event
rainfall and rainfall intensity (Guzzetti et al., 2007). This is visually
portrayed in Fig. 10, where the temporal trend of the cumulated rainfall is
less diagnostic than the corresponding trends of the NEP<inline-formula><mml:math id="M209" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">max</mml:mi></mml:msub></mml:math></inline-formula> or the
<inline-formula><mml:math id="M210" display="inline"><mml:mrow><mml:msub><mml:mi>D</mml:mi><mml:mi mathvariant="normal">NEPmax</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> in forecasting the periods of landslide occurrence.</p>
      <p>We maintain that the E-NEP algorithm is potentially useful for near-real-time  landslide warning, but we acknowledge that more investigations are
required to test the algorithm in different meteorological, geological and
physiographical settings. The sequences of closely spaced rainfall events in
the Gargano Promontory covered a long period (6 days), and this made it
particularly well suited for the design and testing of the E-NEP algorithm.
The sequence of rainfall events was also the result of a relatively simple
meteorological setting. More tests are needed to evaluate the performance of
the E-NEP algorithm for shorter and longer rainfall periods, and in
different and more complex meteorological conditions.</p>
      <p>We stress that the E-NEP algorithm was designed to attempt to forecast
rainfall conditions for the possible occurrence of landslides that react
rapidly to a rainfall input. These are typically shallow landslides,
including soil slides and debris flows. E-NEP was not designed to attempt to
evaluate other landslides that react slowly or very slowly to a rainfall
input, including, for example, deep-seated landslides, shallow landslides in stiff
clay. Also, E-NEP was not designed to attempt to predict landslides caused
by meteorological triggers other than intense rainfall, including, for
example, rain-on-snow events or rapid snow-melt events. However, we expect that E-NEP
can be adapted to forecast shallow landslides caused by intense rainfall
even in specific, local conditions (e.g. in areas burnt by wildfires;
Cannon et al., 2010; De Graff et al., 2013; Moody et al., 2013), provided
that sufficient information is available to apply the method proposed by
Brunetti et al. (2010) and Peruccacci et al. (2012).</p>
      <p>Analysis of the rainfall conditions that have resulted in landslides, flash
floods, inundation and sinkholes in the investigated period in the Gargano
Promontory revealed that the geohydrological hazards occurred in response
to extreme rainfall conditions. This is confirmed by the fact that (i) rainfall
was torrential (Alpert et al., 2002) (Fig. 4) and (ii) the
geohazards – and particularly the landslides – occurred when all the NEP
percentiles were close to the possible maximum value of the non-exceedance
probability of possible landslide occurrence (Fig. 10), which represent very
severe rainfall conditions. The available record of historical landslides
and floods indicates that these are not very frequent or abundant compared
to other areas in southern Italy. We conclude that in the Gargano Promontory
meteorologically driven  hazards occur in response to extreme (i.e. rare)
meteorological conditions. For rainfall-driven hazards, the landscape in the
Gargano Promontory exhibits a threshold behaviour that can be modelled
conceptually by a Heaviside step function (Abramowitz and Stegun, 1972). For
light to heavy rainfall events (Alpert et al., 2002) geohydrological
hazards do not occur or are rare and minor, whereas for heavy–torrential to
torrential rainfall events they are abundant and particularly disruptive. We
attribute the threshold-based behaviour to the karst environment that
dominates the landscape in the promontory.</p>
      <p>In the karst environment of the promontory, rainfall infiltration is
efficient even for high-intensity rainfall rates. This limits the occurrence
of landslides, except for very intense (i.e. extreme) rainfall events.
On the other hand, the arrival of a great amount of rainfall in a setting
typically characterised by water infiltrating within the rock mass through
the network of conduits and joints highly facilitates the formation of
flash floods, particularly in small catchments, as has been frequently
registered also in other parts of Puglia (Parise, 2003; Mossa, 2007).
Further, karst aquifers have very poor retention capacity. These and other
characteristics allow the flash floods to be identified as one of the
main hazards in karst terrains (Fleury et al., 2013; Gutierrez et al., 2014;
Parise et al., 2015).</p>
      <p>In the sinkholes, the presence of residual soils varies largely, depending
on the location, size and depth of the sinkholes. Where the infiltration is
reduced, partial or total inundation of the sinkholes occurs. These local
inundations are difficult to detect because they last only for short
periods and because they often go unnoticed in the rural, scarcely
populated landscape of the promontory.</p>
      <p>The torrential rainfall has triggered sinkholes in the Gargano Promontory
(Fig. 6d, g). Accurate information on the time or period of occurrence of the
sinkholes is not available, and even the simple detection of the sinkholes
was hampered by their small size and the remote location of the events.
However, sinkholes represent a subtle and serious hazard in the promontory and in other karst areas (Parise and Gunn, 2007; Gutierrez et al., 2014;
Parise et al., 2015), and establishing methods and procedures for their
possible forecasting is of primary interest in karst environments. Based on
the analysis of the 1–6 September 2014 Gargano rainfall period, we confirm
that in the promontory, and in similar karst areas, torrential rainfall can
trigger sinkholes, and we hypothesise that approaches based on the
near-real-time monitoring of rainfall (e.g. the E-NEP algorithm) can be
used to forecast the possible occurrence of rainfall-induced sinkholes. We
acknowledge that an analysis of a larger number of events is required to
test this hypothesis.</p>
</sec>
<sec id="Ch1.S6" sec-type="conclusions">
  <title>Conclusions</title>
      <p>We studied a period of torrential rain between 1 and 6 September 2014 in the
Gargano Promontory, Puglia, southern Italy, which caused a variety of
geohydrological hazards, including landslides, flash floods, inundations and sinkholes. We obtained information on the location of the events through
field surveys and the analysis of anecdotal information obtained from
various sources. The temporal information varied among the hazards. For
inundations the time or period of occurrence were known from gauge data
(Fig. 3h), and for flash floods from anecdotal sources (Fig. 6a, b). For
landslides, the period of occurrence was inferred from anecdotal sources for
only nine (out of 46) slope failures and with significant uncertainty. No
information on the time or period of occurrence was available for the
sinkholes. We conclude that the ability to obtain accurate temporal
information for the different hazards, which is important for establishing
and validating early warning systems, depended on the extent and the location
of the different hazards. The temporal information was most accurate for
flooding along the Candelaro River (Fig. 3h), followed by flash floods and
landslides (Fig. 3), and was not available for the sinkholes.</p>
      <p>We used the rainfall and the landslide information available to us to design
and test the new ensemble–non-exceedance probability (E-NEP) algorithm
for the quantitative evaluation of the probability of possible occurrence of
rainfall-induced landslides and of related geohydrological hazards (e.g.
flash floods, sinkholes). For the investigated rainfall events, the ensemble
of the metrics produced by the E-NEP algorithm provided better diagnostics
than the single metrics often used for landslide forecasting, including
rainfall duration, cumulated rainfall and rainfall intensity (Guzzetti et
al., 2007; Brunetti et al., 2010; Peruccacci et al., 2012). We maintain that
the E-NEP algorithm is potentially useful for landslide early warning, but
we acknowledge that more work is needed to test the algorithm in different
meteorological, geological and physiographical settings.</p>
      <p>Our analysis revealed that in the Gargano Promontory meteorologically driven
hazards occur in response to extreme (i.e. rare) meteorological conditions,
and the karst landscape responds to torrential rainfall with a threshold
behaviour. For light to heavy rainfall events (Alpert et al., 2002)
landslides, floods and sinkholes do not occur or are rare and minor,
whereas for heavy–torrential to torrential rainfall events they are abundant
and particularly disruptive, as for the case for the 1–6 September 2014
event. We maintain that this information is useful for landslide early warning systems (and for other
geohydrological hazards).</p>
</sec>

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

      <p>The authors declare that they have no conflict of interest.</p>
  </notes><ack><title>Acknowledgements</title><p>Work performed in the framework of projects supported by the Italian
National Department for Civil Protection (DPC), and the Puglia (Apulia)
Regional Government (PRG). Maria Elena Martinotti and Massimo Melillo were
supported by two grants of DPC. Luca Pisano was supported by a grant of PRG.<?xmltex \hack{\newline}?><?xmltex \hack{\newline}?>
Edited by: A. Günther <?xmltex \hack{\newline}?>
Reviewed by: J. De Waele and one anonymous referee</p></ack><ref-list>
    <title>References</title>

      <ref id="bib1.bib1"><label>1</label><mixed-citation>
Abramowitz, M. and Stegun, I. A. (Eds): Handbook of Mathematical Functions with
Formulas, Graphs, and Mathematical Tables, 9th printing, New York, 1972.</mixed-citation></ref>
      <ref id="bib1.bib2"><label>2</label><mixed-citation>Alpert, P., Ben-Gai, T., Baharan, A., Benjamini, Y., Yekutieli, D.,
Colacino, M., Diodato, L., Ramis, C., Homar, V., Romero, R., Michaelides,
S., and Manes, A.: The paradoxical increase of Mediterranean extreme daily
rainfall in spite of decrease in total values, Geophy. Res. Lett.,
29, 31-1–31-4, <ext-link xlink:href="http://dx.doi.org/10.1029/2001GL013554" ext-link-type="DOI">10.1029/2001GL013554</ext-link>, 2002.</mixed-citation></ref>
      <ref id="bib1.bib3"><label>3</label><mixed-citation>
Bissanti, A. A.: L'alluvione del luglio 1972 a Manfredonia, Mem Ist Geogr Fac
Econ Comm Università Bari, 5–73, 1972.</mixed-citation></ref>
      <ref id="bib1.bib4"><label>4</label><mixed-citation>
Bosellini, A., Morsilli, M., and Neri, C.: Long-term event stratigraphy of the
Apulia platform margin (Upper Jurassic to Eocene; Gargano, southern Italy),
J. Sediment. Res., 69, 1241–1252, 1999.</mixed-citation></ref>
      <ref id="bib1.bib5"><label>5</label><mixed-citation>
Brankman, C. M. and Aydin, A.: Uplift and contractional deformation along a
segmented strike-slip fault system: the Gargano Promontory, southern Italy,
J. Struct. Geol., 26, 807–824, 2004.</mixed-citation></ref>
      <ref id="bib1.bib6"><label>6</label><mixed-citation>Brunetti, M. T., Peruccacci, S., Rossi, M., Luciani, S., Valigi, D., and
Guzzetti, F.: Rainfall thresholds for the possible occurrence of landslides
in Italy, Nat. Hazards Earth Syst. Sci., 10, 447–458,
<ext-link xlink:href="http://dx.doi.org/10.5194/nhess-10-447-2010" ext-link-type="DOI">10.5194/nhess-10-447-2010</ext-link>, 2010.</mixed-citation></ref>
      <ref id="bib1.bib7"><label>7</label><mixed-citation>
Cannon, S. H., Gartner, J. E., Rupert, M. G., Michael, J. A., Rea, A. H., and
Parrett, C.: Predicting the probability and volume of post wildfire debris
flows in the intermountain western United States, Geol. Soc. Am. Bull., 122,
127–144, 2010.</mixed-citation></ref>
      <ref id="bib1.bib8"><label>8</label><mixed-citation>
Castiglioni, B. and Sauro, U.: Large collapse dolines in Puglia (southern
Italy): the cases of “Dolina Pozzatina” in the Gargano plateau and of
“puli” in the Murge, Acta Carsologica, 29, 83–93, 2000.</mixed-citation></ref>
      <ref id="bib1.bib9"><label>9</label><mixed-citation>
De Graff, J. V., Cannon, S. H., and Parise, M.: Limiting the immediate and
subsequent hazards associated with wildfires, in: Landslide science and
practice, volume 4, Global Environmental Change, Springer, 199–209, 2013.</mixed-citation></ref>
      <ref id="bib1.bib10"><label>10</label><mixed-citation>
De Waele, J., Gutiérrez, F., Parise, M., and Plan, L.: Geomorphology and
natural hazards in karst areas: A review, Geomorphology, 134, 1–8, 2011.</mixed-citation></ref>
      <ref id="bib1.bib11"><label>11</label><mixed-citation>Fleury, P., Maréchal, J. C., and Ladouche, B.: Karst flash-flood
forecasting in the city of Nîmes (southern France), Eng. Geol., 164,
26–35, <ext-link xlink:href="http://dx.doi.org/10.1016/j.enggeo.2013.06.007" ext-link-type="DOI">10.1016/j.enggeo.2013.06.007</ext-link>, 2013.</mixed-citation></ref>
      <ref id="bib1.bib12"><label>12</label><mixed-citation>
Ford, D. C. and Williams, P.: Karst Hydrogeology and Geomorphology, Wiley,
Chichester, 562 pp., 2007.</mixed-citation></ref>
      <ref id="bib1.bib13"><label>13</label><mixed-citation>
Funiciello, R., Montone, P., Salvini, F., and Tozzi, M.: Caratteri
strutturali del promontorio del Gargano, Mem. Soc. Geol. It., 41, 1235–1243,
1988.</mixed-citation></ref>
      <ref id="bib1.bib14"><label>14</label><mixed-citation>
Gutiérrez, F., Guerrero, J., and Lucha, P.: A genetic classification of
sinkholes illustrated from evaporite paleokarst exposures in Spain, Environ.
Geol., 53, 993–1006, 2008.</mixed-citation></ref>
      <ref id="bib1.bib15"><label>15</label><mixed-citation>
Gutiérrez, F., Parise, M., De Waele, J., and Jourde, H.: A review on
natural and human-induced geohazards and impacts in karst, Earth-Sci. Rev.,
138, 61–88, 2014.</mixed-citation></ref>
      <ref id="bib1.bib16"><label>16</label><mixed-citation>Guzzetti, F., Peruccacci, S., Rossi, M., and Stark, C. P.: Rainfall
thresholds for the initiation of landslides in central and southern Europe,
Meteorol. Atmos. Phys., 98, 239–267, <ext-link xlink:href="http://dx.doi.org/10.1007/s00703-007-0262-7" ext-link-type="DOI">10.1007/s00703-007-0262-7</ext-link>, 2007.</mixed-citation></ref>
      <ref id="bib1.bib17"><label>17</label><mixed-citation>Moody, J. A., Shakesby, R. A., Robichaud, P. R., Cannon, S. H., and Martin,
D. A.: Current research issues related to post-wildfire runoff and erosion
processes, Earth-Sci. Rev., 122, 10–37, <ext-link xlink:href="http://dx.doi.org/10.1016/j.earscirev.2013.03.004" ext-link-type="DOI">10.1016/j.earscirev.2013.03.004</ext-link>,
2013.</mixed-citation></ref>
      <ref id="bib1.bib18"><label>18</label><mixed-citation>
Mossa, M.: The floods in Bari: what history should have taught, J. Hydraul.
Res., 45, 579–594, 2007.</mixed-citation></ref>
      <ref id="bib1.bib19"><label>19</label><mixed-citation>Parise, M.: Flood history in the karst environment of Castellana-Grotte
(Apulia, southern Italy), Nat. Hazards Earth Syst. Sci., 3, 593–604,
<ext-link xlink:href="http://dx.doi.org/10.5194/nhess-3-593-2003" ext-link-type="DOI">10.5194/nhess-3-593-2003</ext-link>, 2003.</mixed-citation></ref>
      <ref id="bib1.bib20"><label>20</label><mixed-citation>
Parise, M. and Gunn, J. (Eds.): Natural and anthropogenic hazards in karst
areas: Recognition, Analysis and Mitigation, Geological Society, Special
Publication 279, London, 2007.</mixed-citation></ref>
      <ref id="bib1.bib21"><label>21</label><mixed-citation>Parise, M., Ravbar, N., Živanovic, V., Mikszewski, A., Kresic, N.,
Mádl-Szonyi, J., and Kukuric, N.: Hazards in Karst and Managing Water
Resources Quality, in: Karst Aquifers – Characterization and Engineering,
Professional Practice in Earth Sciences, edited by: Stevanovic, Z., Springer,
601–687, <ext-link xlink:href="http://dx.doi.org/10.1007/978-3-319-12850-4_17" ext-link-type="DOI">10.1007/978-3-319-12850-4_17</ext-link>, 2015.</mixed-citation></ref>
      <ref id="bib1.bib22"><label>22</label><mixed-citation>
Peruccacci, S., Brunetti, M. T., Luciani, S., Vennari, C., and Guzzetti, F.:
Lithological and seasonal control on rainfall thresholds for the possible
initiation of landslides in central Italy, Geomorphology, 139–140, 79–90,
2012.</mixed-citation></ref>
      <ref id="bib1.bib23"><label>23</label><mixed-citation>Polemio, M. and Lonigro, T.: Variabilità climatica e ricorrenza delle
calamità idrogeologiche in Puglia, in: Le modificazioni climatiche e i
rischi naturali, edited by: Polemio, M., CNR IRPI, Bari, 13–16, 2011.
 </mixed-citation></ref><?xmltex \hack{\newpage}?>
      <ref id="bib1.bib24"><label>24</label><mixed-citation>
Shepard, D.: A two-dimensional interpolation function for irregularly-spaced
data, in: Proceedings of the 1968 23rd ACM national conference, ACM, New
York, 517–524, 1968.</mixed-citation></ref>
      <ref id="bib1.bib25"><label>25</label><mixed-citation>
Simone, O. and Fiore, A.: Five Large Collapse Dolines in Apulia (Southern
Italy) – the Dolina Pozzatina and the Murgian Puli, Geoheritage, 6,
291–303, 2014.</mixed-citation></ref>
      <ref id="bib1.bib26"><label>26</label><mixed-citation>
Williams, P. W.: The role of the epikarst in karst and cave hydrogeology: a
review, Int. J. Speleol., 37, 1–10, 2008.</mixed-citation></ref>

  </ref-list><app-group content-type="float"><app><title/>

    </app></app-group></back>
    <!--<article-title-html>Landslides, floods and sinkholes in a karst environment: the 1–6 September 2014 Gargano event, southern Italy</article-title-html>
<abstract-html><p class="p">In karst environments, heavy rainfall is known to cause
multiple geohydrological hazards, including inundations, flash floods,
landslides and sinkholes. We studied a period of intense rainfall from 1 to
6 September 2014 in the Gargano Promontory, a karst area in Puglia, southern
Italy. In the period, a sequence of torrential rainfall events caused severe
damage and claimed two fatalities. The amount and accuracy of the
geographical and temporal information varied for the different hazards. The
temporal information was most accurate for the inundation caused by a major
river, less accurate for flash floods caused by minor torrents and even
less accurate for landslides. For sinkholes, only generic information on the
period of occurrence of the failures was available. Our analysis revealed
that in the promontory, rainfall-driven hazards occurred in response to
extreme meteorological conditions and that the karst landscape responded to
the torrential rainfall with a threshold behaviour. We exploited the
rainfall and the landslide information to design the new ensemble–non-exceedance probability (E-NEP) algorithm for the quantitative evaluation of
the possible occurrence of rainfall-induced landslides and of related
geohydrological hazards. The ensemble of the metrics produced by the E-NEP
algorithm provided better diagnostics than the single metrics often used for
landslide forecasting, including rainfall duration, cumulated rainfall and
rainfall intensity. We expect that the E-NEP algorithm will be useful for
landslide early warning in karst areas and in other similar environments. We
acknowledge that further tests are needed to evaluate the algorithm in
different meteorological, geological and physiographical settings.</p></abstract-html>
<ref-html id="bib1.bib1"><label>1</label><mixed-citation>
Abramowitz, M. and Stegun, I. A. (Eds): Handbook of Mathematical Functions with
Formulas, Graphs, and Mathematical Tables, 9th printing, New York, 1972.
</mixed-citation></ref-html>
<ref-html id="bib1.bib2"><label>2</label><mixed-citation>
Alpert, P., Ben-Gai, T., Baharan, A., Benjamini, Y., Yekutieli, D.,
Colacino, M., Diodato, L., Ramis, C., Homar, V., Romero, R., Michaelides,
S., and Manes, A.: The paradoxical increase of Mediterranean extreme daily
rainfall in spite of decrease in total values, Geophy. Res. Lett.,
29, 31-1–31-4, <a href="http://dx.doi.org/10.1029/2001GL013554" target="_blank">doi:10.1029/2001GL013554</a>, 2002.
</mixed-citation></ref-html>
<ref-html id="bib1.bib3"><label>3</label><mixed-citation>
Bissanti, A. A.: L'alluvione del luglio 1972 a Manfredonia, Mem Ist Geogr Fac
Econ Comm Università Bari, 5–73, 1972.
</mixed-citation></ref-html>
<ref-html id="bib1.bib4"><label>4</label><mixed-citation>
Bosellini, A., Morsilli, M., and Neri, C.: Long-term event stratigraphy of the
Apulia platform margin (Upper Jurassic to Eocene; Gargano, southern Italy),
J. Sediment. Res., 69, 1241–1252, 1999.
</mixed-citation></ref-html>
<ref-html id="bib1.bib5"><label>5</label><mixed-citation>
Brankman, C. M. and Aydin, A.: Uplift and contractional deformation along a
segmented strike-slip fault system: the Gargano Promontory, southern Italy,
J. Struct. Geol., 26, 807–824, 2004.
</mixed-citation></ref-html>
<ref-html id="bib1.bib6"><label>6</label><mixed-citation>
Brunetti, M. T., Peruccacci, S., Rossi, M., Luciani, S., Valigi, D., and
Guzzetti, F.: Rainfall thresholds for the possible occurrence of landslides
in Italy, Nat. Hazards Earth Syst. Sci., 10, 447–458,
<a href="http://dx.doi.org/10.5194/nhess-10-447-2010" target="_blank">doi:10.5194/nhess-10-447-2010</a>, 2010.
</mixed-citation></ref-html>
<ref-html id="bib1.bib7"><label>7</label><mixed-citation>
Cannon, S. H., Gartner, J. E., Rupert, M. G., Michael, J. A., Rea, A. H., and
Parrett, C.: Predicting the probability and volume of post wildfire debris
flows in the intermountain western United States, Geol. Soc. Am. Bull., 122,
127–144, 2010.
</mixed-citation></ref-html>
<ref-html id="bib1.bib8"><label>8</label><mixed-citation>
Castiglioni, B. and Sauro, U.: Large collapse dolines in Puglia (southern
Italy): the cases of “Dolina Pozzatina” in the Gargano plateau and of
“puli” in the Murge, Acta Carsologica, 29, 83–93, 2000.
</mixed-citation></ref-html>
<ref-html id="bib1.bib9"><label>9</label><mixed-citation>
De Graff, J. V., Cannon, S. H., and Parise, M.: Limiting the immediate and
subsequent hazards associated with wildfires, in: Landslide science and
practice, volume 4, Global Environmental Change, Springer, 199–209, 2013.
</mixed-citation></ref-html>
<ref-html id="bib1.bib10"><label>10</label><mixed-citation>
De Waele, J., Gutiérrez, F., Parise, M., and Plan, L.: Geomorphology and
natural hazards in karst areas: A review, Geomorphology, 134, 1–8, 2011.
</mixed-citation></ref-html>
<ref-html id="bib1.bib11"><label>11</label><mixed-citation>
Fleury, P., Maréchal, J. C., and Ladouche, B.: Karst flash-flood
forecasting in the city of Nîmes (southern France), Eng. Geol., 164,
26–35, <a href="http://dx.doi.org/10.1016/j.enggeo.2013.06.007" target="_blank">doi:10.1016/j.enggeo.2013.06.007</a>, 2013.
</mixed-citation></ref-html>
<ref-html id="bib1.bib12"><label>12</label><mixed-citation>
Ford, D. C. and Williams, P.: Karst Hydrogeology and Geomorphology, Wiley,
Chichester, 562 pp., 2007.
</mixed-citation></ref-html>
<ref-html id="bib1.bib13"><label>13</label><mixed-citation>
Funiciello, R., Montone, P., Salvini, F., and Tozzi, M.: Caratteri
strutturali del promontorio del Gargano, Mem. Soc. Geol. It., 41, 1235–1243,
1988.
</mixed-citation></ref-html>
<ref-html id="bib1.bib14"><label>14</label><mixed-citation>
Gutiérrez, F., Guerrero, J., and Lucha, P.: A genetic classification of
sinkholes illustrated from evaporite paleokarst exposures in Spain, Environ.
Geol., 53, 993–1006, 2008.
</mixed-citation></ref-html>
<ref-html id="bib1.bib15"><label>15</label><mixed-citation>
Gutiérrez, F., Parise, M., De Waele, J., and Jourde, H.: A review on
natural and human-induced geohazards and impacts in karst, Earth-Sci. Rev.,
138, 61–88, 2014.
</mixed-citation></ref-html>
<ref-html id="bib1.bib16"><label>16</label><mixed-citation>
Guzzetti, F., Peruccacci, S., Rossi, M., and Stark, C. P.: Rainfall
thresholds for the initiation of landslides in central and southern Europe,
Meteorol. Atmos. Phys., 98, 239–267, <a href="http://dx.doi.org/10.1007/s00703-007-0262-7" target="_blank">doi:10.1007/s00703-007-0262-7</a>, 2007.
</mixed-citation></ref-html>
<ref-html id="bib1.bib17"><label>17</label><mixed-citation>
Moody, J. A., Shakesby, R. A., Robichaud, P. R., Cannon, S. H., and Martin,
D. A.: Current research issues related to post-wildfire runoff and erosion
processes, Earth-Sci. Rev., 122, 10–37, <a href="http://dx.doi.org/10.1016/j.earscirev.2013.03.004" target="_blank">doi:10.1016/j.earscirev.2013.03.004</a>,
2013.
</mixed-citation></ref-html>
<ref-html id="bib1.bib18"><label>18</label><mixed-citation>
Mossa, M.: The floods in Bari: what history should have taught, J. Hydraul.
Res., 45, 579–594, 2007.
</mixed-citation></ref-html>
<ref-html id="bib1.bib19"><label>19</label><mixed-citation>
Parise, M.: Flood history in the karst environment of Castellana-Grotte
(Apulia, southern Italy), Nat. Hazards Earth Syst. Sci., 3, 593–604,
<a href="http://dx.doi.org/10.5194/nhess-3-593-2003" target="_blank">doi:10.5194/nhess-3-593-2003</a>, 2003.
</mixed-citation></ref-html>
<ref-html id="bib1.bib20"><label>20</label><mixed-citation>
Parise, M. and Gunn, J. (Eds.): Natural and anthropogenic hazards in karst
areas: Recognition, Analysis and Mitigation, Geological Society, Special
Publication 279, London, 2007.
</mixed-citation></ref-html>
<ref-html id="bib1.bib21"><label>21</label><mixed-citation>
Parise, M., Ravbar, N., Živanovic, V., Mikszewski, A., Kresic, N.,
Mádl-Szonyi, J., and Kukuric, N.: Hazards in Karst and Managing Water
Resources Quality, in: Karst Aquifers – Characterization and Engineering,
Professional Practice in Earth Sciences, edited by: Stevanovic, Z., Springer,
601–687, <a href="http://dx.doi.org/10.1007/978-3-319-12850-4_17" target="_blank">doi:10.1007/978-3-319-12850-4_17</a>, 2015.
</mixed-citation></ref-html>
<ref-html id="bib1.bib22"><label>22</label><mixed-citation>
Peruccacci, S., Brunetti, M. T., Luciani, S., Vennari, C., and Guzzetti, F.:
Lithological and seasonal control on rainfall thresholds for the possible
initiation of landslides in central Italy, Geomorphology, 139–140, 79–90,
2012.
</mixed-citation></ref-html>
<ref-html id="bib1.bib23"><label>23</label><mixed-citation>
Polemio, M. and Lonigro, T.: Variabilità climatica e ricorrenza delle
calamità idrogeologiche in Puglia, in: Le modificazioni climatiche e i
rischi naturali, edited by: Polemio, M., CNR IRPI, Bari, 13–16, 2011.

</mixed-citation></ref-html>
<ref-html id="bib1.bib24"><label>24</label><mixed-citation>
Shepard, D.: A two-dimensional interpolation function for irregularly-spaced
data, in: Proceedings of the 1968 23rd ACM national conference, ACM, New
York, 517–524, 1968.
</mixed-citation></ref-html>
<ref-html id="bib1.bib25"><label>25</label><mixed-citation>
Simone, O. and Fiore, A.: Five Large Collapse Dolines in Apulia (Southern
Italy) – the Dolina Pozzatina and the Murgian Puli, Geoheritage, 6,
291–303, 2014.
</mixed-citation></ref-html>
<ref-html id="bib1.bib26"><label>26</label><mixed-citation>
Williams, P. W.: The role of the epikarst in karst and cave hydrogeology: a
review, Int. J. Speleol., 37, 1–10, 2008.
</mixed-citation></ref-html>--></article>
