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  <front>
    <journal-meta><journal-id journal-id-type="publisher">CP</journal-id><journal-title-group>
    <journal-title>Climate of the Past</journal-title>
    <abbrev-journal-title abbrev-type="publisher">CP</abbrev-journal-title><abbrev-journal-title abbrev-type="nlm-ta">Clim. Past</abbrev-journal-title>
  </journal-title-group><issn pub-type="epub">1814-9332</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/cp-16-1547-2020</article-id><title-group><article-title>Changes in high-intensity precipitation on the northern Apennines (Italy) as
revealed by multidisciplinary data <?xmltex \hack{\break}?>over the last 9000 years</article-title><alt-title>Changes in high-intensity precipitation on the northern Apennines (Italy)</alt-title>
      </title-group><?xmltex \runningtitle{Changes in high-intensity precipitation on the northern Apennines (Italy)}?><?xmltex \runningauthor{S.~Segadelli et al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Segadelli</surname><given-names>Stefano</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="yes" rid="aff2 aff6">
          <name><surname>Grazzini</surname><given-names>Federico</given-names></name>
          <email>fgrazzini@arpae.it</email>
        <ext-link>https://orcid.org/0000-0002-3435-2376</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3">
          <name><surname>Rossi</surname><given-names>Veronica</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Aguzzi</surname><given-names>Margherita</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff4">
          <name><surname>Marvelli</surname><given-names>Silvia</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff4">
          <name><surname>Marchesini</surname><given-names>Marco</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff5">
          <name><surname>Chelli</surname><given-names>Alessandro</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff5">
          <name><surname>Francese</surname><given-names>Roberto</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>De Nardo</surname><given-names>Maria Teresa</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Nanni</surname><given-names>Sandro</given-names></name>
          
        </contrib>
        <aff id="aff1"><label>1</label><institution>Geological, Seismic and Soil Service, Emilia–Romagna Region
Administration, Bologna, Italy</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>Regional Agency for Prevention, Environment and Energy of
Emilia–Romagna, Hydro-Meteo-Climate Service (ARPAE-SIMC), Bologna, Italy</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>Department of Biological, Geological, and Environmental Sciences –
BiGeA,<?xmltex \hack{\break}?> Alma Mater Studiorum University of Bologna, Bologna, Italy</institution>
        </aff>
        <aff id="aff4"><label>4</label><institution>Laboratory of Palynology and Archaeobotany – C.A.A. Giorgio Nicoli,
San Giovanni in Persiceto, Bologna, Italy</institution>
        </aff>
        <aff id="aff5"><label>5</label><institution>Department of Chemistry, Life Sciences and Environmental
Sustainability, University of Parma, Parma, Italy</institution>
        </aff>
        <aff id="aff6"><label>6</label><institution>Ludwig-Maximilians-Universität, Meteorologisches Institut,
Munich, Germany</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Federico Grazzini (fgrazzini@arpae.it)</corresp></author-notes><pub-date><day>19</day><month>August</month><year>2020</year></pub-date>
      
      <volume>16</volume>
      <issue>4</issue>
      <fpage>1547</fpage><lpage>1564</lpage>
      <history>
        <date date-type="received"><day>4</day><month>November</month><year>2019</year></date>
           <date date-type="rev-request"><day>13</day><month>December</month><year>2019</year></date>
           <date date-type="rev-recd"><day>27</day><month>May</month><year>2020</year></date>
           <date date-type="accepted"><day>14</day><month>July</month><year>2020</year></date>
      </history>
      <permissions>
        <copyright-statement>Copyright: © 2020 Stefano Segadelli et al.</copyright-statement>
        <copyright-year>2020</copyright-year>
      <license license-type="open-access"><license-p>This work is licensed under the Creative Commons Attribution 4.0 International License. To view a copy of this licence, visit <ext-link ext-link-type="uri" xlink:href="https://creativecommons.org/licenses/by/4.0/">https://creativecommons.org/licenses/by/4.0/</ext-link></license-p></license></permissions><self-uri xlink:href="https://cp.copernicus.org/articles/16/1547/2020/cp-16-1547-2020.html">This article is available from https://cp.copernicus.org/articles/16/1547/2020/cp-16-1547-2020.html</self-uri><self-uri xlink:href="https://cp.copernicus.org/articles/16/1547/2020/cp-16-1547-2020.pdf">The full text article is available as a PDF file from https://cp.copernicus.org/articles/16/1547/2020/cp-16-1547-2020.pdf</self-uri>
      <abstract><title>Abstract</title>
    <p id="d1e201">Several record-breaking precipitation events have struck the
mountainous area of the Emilia–Romagna region (northern Apennines, Italy) over
the last 10 years. As a consequence, severe geomorphological processes such
as debris avalanches and debris flows, shallow landslides, and overbank
flooding have affected the territory, causing severe damage to human-made
structures. The unusual intensity of these phenomena prompted an
investigation into their frequency in the past, beyond instrumental time. In
the quest for an understanding of whether these phenomena are unprecedented in
the region, peat bog and lake deposits were analyzed to infer the frequency
of extreme precipitation events that may have occurred in the past. We
present the results of a dedicated field campaign performed in summer 2017
at Lake Moo in the northern Apennines, a 0.15 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> peat bog located at
an altitude of 1130 m a.s.l. During the extreme precipitation event of 13–14
September 2015, several debris flows generated by small streams
affected the Lake Moo plain. In such a small drainage basin (<inline-formula><mml:math id="M2" display="inline"><mml:mrow><mml:mi mathvariant="italic">&lt;</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> km<inline-formula><mml:math id="M3" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula>), high-density floods can be triggered only by high-intensity
precipitation events. The sedimentary succession (ca. 13 m thick) was
studied through the drilling of two cores and one trench. The sequence,
characterized by clusters of coarse-grained alluvial deposits interbedded
with organic-rich silty clays and peat layers, was analyzed by combining
sedimentological, pollen, microanthracological and pedological data with
radiocarbon dating (AMS <inline-formula><mml:math id="M4" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi/><mml:mn mathvariant="normal">14</mml:mn></mml:msup><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula>) in an innovative multidisciplinary
approach for this area. Original data acquired during the field campaign
were also correlated with other specific paleoclimatic proxies available in
the literature for the northern Apennines area. We discover that the
increase in extreme paleoflooding, associated with coarse-grained deposits
similar to the ones observed recently, correlates well with the warm phases
of the Holocene Thermal Maximum and with the ongoing warming trend observed
that started at the beginning of the last century.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <label>1</label><title>Introduction</title>
      <p id="d1e253">High-intensity precipitation (HIP) events, also known as torrential
rainstorms for their capacity to generate flash floods in small streams,
represent a significant component of the Mediterranean water cycle. More
than half of the annual precipitation is concentrated in a few major
precipitation events (e.g., Frei and Schär, 1998; Isotta et al., 2014).
Better knowledge of their expected frequency (and maximum intensity)<?pagebreak page1548?> is
crucial for planning adequate hydraulic defenses and sustainable water
resource management in the present and future climate.</p>
      <p id="d1e256">Under the threat of global warming, a growing number of studies have
investigated the link between a temperature rise in air masses and the intensity
of extreme precipitation, highlighting spatial and seasonal differences
across the globe (e.g., Lehmann et al., 2015; Papalexiou and Montanari,
2019). There is a consensus that HIP events are increasing with global
warming, while mean precipitation could decrease in some regions (Berg et
al., 2013). Myhre et al. (2019) show that HIP over Europe
almost doubles per degree of warming due to the combined effect of
increasing frequency (the major driver) and an increase in intensity.</p>
      <p id="d1e259">At the local scale, different responses of weather patterns and limitations
in moisture availability can alter the uniform expected rise in HIP due to
the increase in saturation water vapor pressure (6 % K<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>–7 % K<inline-formula><mml:math id="M6" 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>) (e.g.,
Westra et al., 2014; Prein et al., 2017). For example, in the Swiss Alps
Scherrer et al. (2016) found a significant increase in daily extreme
precipitation indices since the beginning of the last century (i.e., between
1901 and 2014), while Brugnara and Maugeri (2019) documented regional differences
in HIP trends across the whole Alpine area. These results suggest that
instrumental data do not cover a suitable period to infer reliable local
changes in HIP frequency.</p>
      <p id="d1e286">The investigation of sedimentary archives, like peat bogs and lakes, allow
for the verification of the hypothesized linkage between extreme precipitation and
temperatures in the distant past, substantially widening the period during which we
can verify this relationship.</p>
      <p id="d1e290">In the literature there is ample documentation of the use of these
sedimentary archives to infer chronologies of past flood events (Zavala et
al., 2006, 2011; Giguet-Covex et al., 2012; Gilli et al.,
2013; Glur et al., 2013; Stoffel et al., 2013, 2016; Wirth, 2013; Wirth et al.,
2013; Anselmetti et al., 2014; Longman et al., 2017; Schillereff et al.,
2014; Swierczynski et al., 2017; Ahlborn et al., 2018;
Wilhelm et al., 2012, 2018; Zavala and Pan, 2018), alongside others such as
tree rings (Ballesteros-Cánovas et al., 2015), speleothems (Regattieri
et al., 2014; Zanchetta et al., 2011), and torrential fans and cones
(Schneuwly-Bollschweiler et al., 2013).</p>
      <p id="d1e293">Interestingly, over the Alpine area a synchronization between increasing
flood frequency and Holocene cooling periods characterized by cold and wet
summers, like the Little Ice Age (LIA), has been documented by several studies
(e.g., Glur et al., 2013; Henne et al., 2018). Other authors reported that
under warm paleoclimate conditions floods in the Alps became rarer but
stronger in intensity, highlighting the complexity of this issue
(Giguet-Covex et al., 2012; Brönnimann et al., 2018a). Alpine data
mostly derive from lacustrine sedimentary successions that are known to be
influenced by a combination of factors (e.g., precipitation intensity,
duration, seasonality, and changes in atmospheric circulation and land use)
that might overshadow the physically based relationship between temperature
increase and extreme precipitation events (Utsumi et al., 2011;
Brönnimann et al., 2018b).</p>
      <p id="d1e296">In contrast, less attention was paid to the Holocene flood activity in the
northern Apennines area (N Italy in Fig. 1), which has a different
precipitation climatology compared to the inner Alpine region. Indeed, the
link between cold summers and high values of flood frequency appears more
logical for the Alpine region, which shows a precipitation maximum in the
summer. In contrast, in the northern Apennines area, precipitation maxima
occur in autumn, with more than 60 % of the annual total precipitation
concentrated in a few days characterized by severe meteorological events
(Isotta et al., 2014).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1"><?xmltex \currentcnt{1}?><label>Figure 1</label><caption><p id="d1e301"><bold>(a)</bold> Location map of the Lake Moo plain. The area affected by the
extreme precipitation event of 13 and 14 September 2015 is
highlighted by the red rectangle. <bold>(b)</bold> View of the Lake Moo landscape from
the southern side.</p></caption>
        <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://cp.copernicus.org/articles/16/1547/2020/cp-16-1547-2020-f01.png"/>

      </fig>

      <p id="d1e315">Focusing the analysis on the Emilia–Romagna region (ER region; Fig. 1), an
increase in the interannual variability of torrential rainfall has been observed
over the last 10 years with marked or even exceptional droughts, such as
those occurring in 2012 and 2017 (Grazzini et al., 2012), followed by years
of record-breaking rainfall (2014 and 2018). Between September 2014 and
September 2015, the ER region was affected by three events of
exceptional intensity with an estimated return period of several centuries
(Grazzini et al., 2016).</p>
      <p id="d1e319">To consolidate HIP trends on the N Apennines area, we analyzed the Holocene
sedimentary succession of a small-sized<?pagebreak page1549?> peat bog (Lake Moo in Fig. 1) through
the application of a multidisciplinary approach that integrates
sedimentological and environmental data (e.g., pollen-derived
paleovegetation patterns) with climatological observations and physical
arguments.</p>
      <p id="d1e322">Lake Moo is in the proximity of the main N Apennines crest that is very
exposed to moist maritime airflow coming from the central Mediterranean Sea.
The dimension of the drainage basin is small (total area <inline-formula><mml:math id="M7" display="inline"><mml:mrow><mml:mi mathvariant="italic">&lt;</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> km<inline-formula><mml:math id="M8" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula>), and the modern anthropogenic impact is low as the site belongs to
the Natura 2000 network (site code and name: IT4020008 – Monte Ragola, Lago
Moo, Lago Bino). Moreover, the activation of debris flows (sensu Hungr et al.,
2014) during a severe flash-flood event occurred on 13–14
September 2015, with an estimated rainfall intensity of 112 mm every 3 h over the
Lake Moo basin (Segadelli et al., 2020; Grazzini et al., 2016), offering the
unique opportunity to use these recent deposits as an archetype of past
events. According to the literature (Milliman and Syvitski, 1992; Mulder and
Syvitski, 1995; Mutti et al., 1996), in such a small drainage basin
high-density floods can be triggered only by HIP events lasting long enough
for the water to infiltrate and mobilize large quantities of debris. All
these geomorphological features make Lake Moo an ideal site to investigate
past changes in HIP events in terms of sedimentary expression, frequency and
forcing factors. This research addresses the following questions.
<list list-type="custom"><list-item><label>a.</label>
      <p id="d1e346">Are the recent events unprecedented on a millennial timescale (i.e., the
Holocene period)?</p></list-item><list-item><label>b.</label>
      <p id="d1e350">Is the frequency of HIP events coupled with (paleo)temperature variations?</p></list-item></list></p>
</sec>
<sec id="Ch1.S2">
  <label>2</label><title>The study area</title>
<sec id="Ch1.S2.SS1">
  <label>2.1</label><title>Geographic and climate context</title>
      <p id="d1e368">The Lake Moo plain (44<inline-formula><mml:math id="M9" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>37<inline-formula><mml:math id="M10" display="inline"><mml:msup><mml:mi/><mml:mo>′</mml:mo></mml:msup></mml:math></inline-formula>29<inline-formula><mml:math id="M11" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>′</mml:mo><mml:mo>′</mml:mo></mml:mrow></mml:msup></mml:math></inline-formula> N, 9<inline-formula><mml:math id="M12" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>32<inline-formula><mml:math id="M13" display="inline"><mml:msup><mml:mi/><mml:mo>′</mml:mo></mml:msup></mml:math></inline-formula>25<inline-formula><mml:math id="M14" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>′</mml:mo><mml:mo>′</mml:mo></mml:mrow></mml:msup></mml:math></inline-formula> E), about
0.15 km<inline-formula><mml:math id="M15" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula> wide, is located near the boundary between the Emilia–Romagna and
Liguria regions (Piacenza province, Italy; Fig. 1a) in the upper valley of
the Nure stream at an altitude of 1130 m above sea level (a.s.l.). A high
tree cover density characterizes the present-day catchment area (i.e., the
total woodland cover is 65.55 %; Corticelli et al., 2011), with a high
richness of plant species and an exceptional concentration of protected
mountain taxa of particular phytogeographical interest. The vegetation
landscape shows the widespread occurrence of <italic>Fagus sylvatica</italic>, locally interrupted by
grazing areas and blueberry moorlands with the presence of rare <italic>Juniperus nana</italic> and <italic>Sorbus chamaemespilus</italic>.
Reforestation of <italic>Pinus nigra</italic> is also documented (Fig. 1b).</p>
      <p id="d1e453">Present-day climate conditions primarily reflect the interaction of the
prevalent atmospheric flow and the mountain range surrounding the Lake Moo
plain. The proximity to the Ligurian Sea (about 40 km SW) makes the location
particularly favorable to orographic precipitation enhancement in the case
of moisture-laden southerly flow. The most precipitation is usually
observed in spring and autumn, with a marked peak in early autumn. In
this period we observe a particular synergy of midlatitude synoptic
disturbances, becoming more frequent towards the cold seasons, and strong
convective systems still developing over the warm Mediterranean Sea at the
end of summer and in autumn (Grazzini et al., 2020); this is a situation very
favorable for the genesis of extreme precipitation events in the area.</p>
</sec>
<sec id="Ch1.S2.SS2">
  <label>2.2</label><title>Geological and geomorphological setting</title>
      <p id="d1e464">The study area mainly consists of extensively fractured serpentinites that
represent the accreted fragments of the Ligure–Piemonte oceanic basin
separating the European and Adria plates during the Middle–Upper Jurassic
(Marroni et al., 2010). The ultramafic rocks are bordered by polygenic breccias
made of blocks of limestones or marly limestones embedded within a
fine-grained matrix (Mt. Ragola Complex, late Santonian–early Campanian;
Elter et al., 1997).</p>
      <p id="d1e467">The geomorphological landscape includes flat areas and steep slopes located
at different altitudes. On the former, marshy environments commonly occur
recording the last filling phases of small lacustrine basins, some of which
still exist as Lake Moo and Lake Bino (Figs. 1–2). However, the
origin of Lake Moo is still a matter of debate as some authors point to a
glacial origin (Elter et al., 1997; Marchetti and Fraccia, 1988; Carton and
Panizza, 1988), while others have interpreted the basin as the expression of
Holocene deep-seated gravitational slope deformations (Geological, Seismic
and Soil Service of the Emilia–Romagna Region, 2012) mainly controlled by
changes in the incision rates of the Nure stream (Elter et al., 1997). The
complexity of past and present morphological processes is likely enhanced
by the superposition of lithological units with strong mechanical contrast,
such as ophiolites and the underlying a predominantly clayey unit (Elter et
al., 1997).</p>
</sec>
</sec>
<sec id="Ch1.S3">
  <label>3</label><title>Data and methods</title>
<sec id="Ch1.S3.SS1">
  <label>3.1</label><title>Field investigation</title>
      <p id="d1e486">Taking into account the criteria indicated by Gilli et al. (2013) and
Schillereff et al. (2014), Lake Moo shares several advantageous
characteristics for the reconstruction of Holocene flood activity:
<list list-type="bullet"><list-item>
      <p id="d1e491">steep slopes (average inclination of 24<inline-formula><mml:math id="M16" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>) composed of deposits
highly susceptible to erosion (i.e., polygenic and monogenic breccias with a
pelitic matrix – the Mt. Ragola Complex; Elter et al., 1997; Fig. 2);</p></list-item><list-item>
      <p id="d1e504">absence of lacustrine basins in the upstream part of the catchment;</p></list-item><list-item>
      <p id="d1e508">small drainage basin area (1.94 km<inline-formula><mml:math id="M17" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula>);</p></list-item><list-item>
      <p id="d1e521">one dominant inflow into the lake;</p></list-item><list-item>
      <p id="d1e525">lack of regulated flow structures; and</p></list-item><list-item>
      <p id="d1e529">lack of natural pre-lake sediment storage zones.</p></list-item></list></p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2" specific-use="star"><?xmltex \currentcnt{2}?><label>Figure 2</label><caption><p id="d1e534">Geomorphological map showing the main geological units and the
hydrological elements of the Lake Moo plain. The detailed mapping of flood
deposits formed during the recent HIP event (13–14 September
2015), the location of the geognostic investigations and the geophysical
survey tracks are also reported. Original data from the field campaign are overlaid
on the geological database of the Emilia–Romagna region.</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://cp.copernicus.org/articles/16/1547/2020/cp-16-1547-2020-f02.png"/>

        </fig>

      <p id="d1e543">The field campaign led to the acquisition of two sedimentary cores (S1 and
S2), 14 and 6 m long, respectively, and one trench (T1) to investigate the
sedimentary succession capped by the high-density flood deposits formed
during the recent HIP event (13–14 September 2015). The
location of the cores and the trench benefited from a detailed
geomorphological map (Fig. 2) and a high-resolution reflection seismic
survey (Fig. SUP1 in the Supplement), both originally produced
for this research. The latter provided useful information about the lake-basin-floor morphology and the thickness of the infilling succession.</p>
      <p id="d1e547">The two cores, S1 and S2, were obtained using a continuous drilling system
that guaranteed an undisturbed stratigraphy and a high recovery percentage
(about 90 %). A trench (6 m long, 3 m wide, 2 m deep) was excavated
between the two coring sites, allowing for a detailed analysis of the most recent
deposits.</p>
      <p id="d1e550">We focused our attention on the longest core (S1) that shows the complete
record of the Lake Moo infilling succession, as it reaches the ophiolite
bedrock. Therefore, all the laboratory analyses (grain size, radiocarbon and
palynological analysis) were undertaken on core S1, while the other core
(S2) and the trench were used to support the stratigraphic reconstruction.
Elevation and geographic coordinates of reference core S1 were acquired
using a Garmin eTrex 10 GPS receiver: 1120.2 m a.s.l. and 44<inline-formula><mml:math id="M18" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>37<inline-formula><mml:math id="M19" display="inline"><mml:msup><mml:mi/><mml:mo>′</mml:mo></mml:msup></mml:math></inline-formula>25<inline-formula><mml:math id="M20" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>′</mml:mo><mml:mo>′</mml:mo></mml:mrow></mml:msup></mml:math></inline-formula> N–9<inline-formula><mml:math id="M21" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>32<inline-formula><mml:math id="M22" display="inline"><mml:msup><mml:mi/><mml:mo>′</mml:mo></mml:msup></mml:math></inline-formula>43<inline-formula><mml:math id="M23" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>′</mml:mo><mml:mo>′</mml:mo></mml:mrow></mml:msup></mml:math></inline-formula> E, respectively.</p>
</sec>
<?pagebreak page1550?><sec id="Ch1.S3.SS2">
  <label>3.2</label><title>Facies analysis and chronology</title>
      <p id="d1e622">Facies characterization of the Lake Moo sedimentary succession was mainly
performed by integrating the observable macroscopic physical characteristics
(i.e., grain size, sedimentary structures, Munsell chart color and types of
bounding surfaces) with the grain size data available for the reference core
S1. The interpretation in terms of depositional environments also benefited
from the precise position of the core(s) with respect to the spill point of
Lake Moo and the application of the facies tract concept. The latter
strongly supported the interpretation of the coarse-grained intervals
encountered throughout the studied succession. Specifically, a facies tract
is defined as the association of genetic facies that can be observed within
the flood deposits along with the downslope motion transformation (Lowe,
1982; Mutti, 1992; Mutti et al., 1996). Thus, the application of the facies
tract concept, if framed into the stratigraphy of the core(s), may allow for the
reconstruction of how flood deposits changed through time at a fixed
location (Figs. 3, 4).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3" specific-use="star"><?xmltex \currentcnt{3}?><label>Figure 3</label><caption><p id="d1e627">Sedimentological features and lithofacies characterization of the
reference core S1. Radiocarbon dates, palynological and grain size samples,
and stratigraphic units (described in Sect. 4.2) are also
reported.</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://cp.copernicus.org/articles/16/1547/2020/cp-16-1547-2020-f03.png"/>

        </fig>

      <p id="d1e636">The abundance of wood remains and peaty layers within the sedimentary
succession under examination supported the development of a robust
chronological framework. A total of 12 samples were selected from the reference
core S1 and radiocarbon dated at the CEDAD Laboratory of the University of
Salento (Italy). The data are available in Table TS1 (in the Supplement), and the conventional <inline-formula><mml:math id="M24" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi/><mml:mn mathvariant="normal">14</mml:mn></mml:msup><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> ages were converted into calendar
years using the OxCal software version 3.10 (Reimer et al., 2013).</p>
      <p id="d1e652">An age–depth model was also constructed using linear interpolation.
Coarse-grained intervals were not excluded from the processing because of
the difficulty to evaluate the exact thickness of the deposits interpretable
as instantaneous events. Indeed, the upper limit of coarse-grained intervals
commonly appears transitional toward finer sediments, and, in a few cases, some
intervals for a total thickness of 107 cm were not recovered.</p>
</sec>
<sec id="Ch1.S3.SS3">
  <label>3.3</label><title>Pollen and microanthracological analysis</title>
      <p id="d1e663">In order to refine facies characterization and highlight past vegetation
changes at the study site, pollen analyses were carried out on 14 samples
collected from the core S1. We focused the analyses on two key stratigraphic
intervals formed during periods of well-known different paleoclimate (and
paleotemperature) conditions: (i) Interval 1 (ca. 10.5–9 m of core depth),
covering the period between ca. 9600 and 7300 cal yr BP, thus centered on the
Holocene Thermal Maximum – HTM (Renssen et al., 2012), and (ii) Interval 2 (ca.
5.5–4.5 m of core depth), recording the final stages of HTM and the following
cooling period between ca. 5500 and 3800 cal yr BP. In these two stratigraphic
intervals, samples were collected from fine-grained layers following a mean
sampling resolution of ca. 30 cm.</p>
      <p id="d1e666">A standard methodology already tested for pollen substrates was applied with
some minor modifications (Lowe et al., 1996). The method includes a series
of laboratory treatments: about 8–10 g of sample was treated in 10 %
Na pyrophosphate to deflocculate the sediment matrix; a <italic>Lycopodium</italic> tablet
was added to calculate the pollen concentration (expressed as pollen grains per
gram),  the sediment residue was subsequently washed through a 7 <inline-formula><mml:math id="M25" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>m sieve. The sample was resuspended in HCl 10 % to remove calcareous
material and subjected to Erdtman acetolysis; a heavy liquid separation method
was then introduced using Na metatungstate hydrate with a specific gravity of 2.0 and
centrifugation at 2000 rpm for 20 min. Following this procedure, the
retained fractions were treated with 40 % hydrogen fluoride for 24 h, and then the
sediment residue was washed in distilled water and after in ethanol with
glycerol; the final residue was desiccated and mounted on slides using
glycerol jelly and finally sealed with paraffin.</p>
      <p id="d1e680">Identification of the samples was performed at <inline-formula><mml:math id="M26" display="inline"><mml:mrow><mml:mo>×</mml:mo><mml:mn mathvariant="normal">400</mml:mn></mml:mrow></mml:math></inline-formula> magnification, and only
difficult pollen, such as <italic>Triticum</italic>, <italic>Avena</italic> or <italic>Hordeum</italic> types, was observed at <inline-formula><mml:math id="M27" display="inline"><mml:mrow><mml:mo>×</mml:mo><mml:mn mathvariant="normal">1000</mml:mn></mml:mrow></mml:math></inline-formula> magnification.</p>
      <?pagebreak page1551?><p id="d1e712">Determination of pollen grains was based on the Palinoteca of the “Centro
Agricoltura Ambiente – CAA G. Nicoli” laboratory (Italy), atlases and a
vast amount of specific morpho-palynological literature. Names of the
families, genus and species of plants conform to the classifications of
Italian Flora proposed by Pignatti (2017–2019) and European Flora (Tutin et
al., 1964–1993). The pollen terminology was based on Berglund and
Ralska-Jasiewiczowa (1986), Faegri and Iversen (1989), and Moore et al. (1991) with slight modifications that tend to simplify plant nomenclature.
The term “taxa” is used in a broad sense to indicate both the systematic
categories and the pollen morphological types (Beug, 2004). For each sample,
at least 500 pollen grains were counted, and the identified taxa have been
expressed as percentages of the total pollen sum that includes only
terrestrial pollen, no fern spores and no aquatic plants.</p>
      <?pagebreak page1552?><p id="d1e716">On the basis of vegetational and ecological characteristics, the following
main pollen groups were identified: conifers (<italic>Pinus–Abies alba</italic>), deciduous trees (this group
includes quercetum taxa – <italic>Quercus, Carpinus betulus, Corylus avellana, Fraxinus, Ostrya carpinifolia, Tilia</italic> and <italic>Ulmus</italic> <inline-formula><mml:math id="M28" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> other deciduous trees), meadow (this
group mainly comprises <italic>Fabaceae</italic> and <italic>Asteroideae</italic>, <italic>Caryophyllaceae</italic>, <italic>Cichorioideae</italic> and<italic> Poaceae</italic>), anthropogenic indicators (e.g.,
<italic>Cerealia, Chenopodium, Convolvulus arvensis, Plantago, Urtica</italic>) and “alia”, which includes all taxa excluded from previous groups. The group
of hygro <inline-formula><mml:math id="M29" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> aquatic plants was also distinguished. It includes hygrophilous
herbs (e.g., <italic>Cyperaceae</italic>), helophytes and hydrophytes (i.e., <italic>Lemna, Junchus, Nymphaea, Phragmites, Potamogeton</italic> and <italic>Sparganium</italic>), which are
considered a good proxy for humid conditions typical of wetlands.</p>
      <?pagebreak page1553?><p id="d1e771">The 14 samples prepared for pollen analysis were also investigated for the
identification of microcharcoals. Microanthracological analysis has been
used to track past changes in fire history, likely connected to
anthropogenic activities (Vescovi et al., 2010). A point-count estimation of
microscopic charcoal abundance was carried out, and charcoal fragments
encountered during pollen counting were recorded in four size classes based
on the long axis length: 10–50, 50–125, 125–250, <inline-formula><mml:math id="M30" display="inline"><mml:mrow><mml:mi mathvariant="italic">&gt;</mml:mi><mml:mn mathvariant="normal">250</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M31" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>m
(Whitlock and Millspaugh, 1996; Clark, 1982; Patterson et al., 1987; Whitlock
and Larsen, 2001; Fisinger et al., 2008). The former two classes were
interpreted to be windblown transported, hence giving information about
regional fire events, whereas the latter two were considered the result of
local vegetation burning (Vittori Antisari et al., 2015).</p>
      <p id="d1e792">Pollen and microcharcoal results are presented in Sect. 5 to support
facies stratigraphy and to discuss controlling factors on flood activation.</p>
</sec>
<sec id="Ch1.S3.SS4">
  <label>3.4</label><title>Temperature reconstruction and modern climatological dataset</title>
      <p id="d1e803">Central to our study is the availability of a reliable (paleo)temperature
dataset for the chronological period recorded by the Lake Moo sedimentary
succession. In this respect, the Holocene paleoclimate reconstruction
conducted by Samartin et al. (2017) on the nearby Lake Verdarolo represents
a very important reference. The Lake Verdarolo site is located at 1390 m a.s.l., 270 m higher and 54 km SE from Lake Moo (Fig. 1), in a very similar
climatic context. The authors reconstructed the mean July air temperature
using a chironomid-based inference model developed through a combination of
data extracted from more than 200 lakes in Norway and the Swiss Alps (Heiri et
al., 2011). This vegetation-independent paleotemperature reconstruction is
the first for the northern Apennines, and it agrees with that of Gemini
Lake (1350 m a.s.l. elevation and 48 km SE from Lake Moo) as well as several
other records coming from central Italy (Samartin et al., 2017).</p>
      <p id="d1e806">Modern temperature and precipitation time series (1961–2018) at Lake
Verdarolo and Lake Moo were derived from the gridded high-resolution dataset
of Emilia–Romagna (Eraclito4), described in Antolini et al. (2016). Trend
estimation and a Mann–Kendall significance trend test were computed with the
pyMannKendall package (Hussain et al., 2019).</p>
</sec>
</sec>
<sec id="Ch1.S4">
  <label>4</label><title>Results</title>
<sec id="Ch1.S4.SS1">
  <label>4.1</label><title>Holocene stratigraphy</title>
<sec id="Ch1.S4.SS1.SSS1">
  <label>4.1.1</label><title>Sedimentary facies</title>
      <p id="d1e832">A total of 14 lithofacies (LM1 to LM14) have been identified within the infilling
succession of the Lake Moo basin. A detailed lithological description of each
lithofacies is reported below.
<list list-type="bullet"><list-item>
      <p id="d1e837">LM1 to LM2 includes a clast-supported deposit with a thickness ranging between 5 and 15 cm. Fine boulders to coarse cobbles with abundant coarse- to fine-grained
sand matrix, showing a low degree of sorting, occur. Polygenic clasts have
low sphericity and a very angular shape. Wood fragments locally occur. The
basal and top contacts are sharp, and the basal one occasionally shows evidence
of erosion.</p></list-item><list-item>
      <p id="d1e841">LM3 to LM4 includes a clast-supported deposit with a thickness ranging between 5 and 15 cm. It is composed of fine cobbles to coarse pebbles with a very fine sand
to silt matrix. Polygenic clasts have low sphericity and a subangular shape.
Scraps of wood are encountered. The basal and top contacts are sharp, and the
basal one occasionally shows evidence of erosion.</p></list-item><list-item>
      <p id="d1e845">LM5 is a massive matrix-supported deposit composed of medium pebbles to granules
embedded within a very fine sand to silt matrix. Polygenic clasts have low
sphericity and a subangular shape. Scraps of wood are encountered. The basal
and top contacts are sharp, and the basal one occasionally shows evidence of
erosion.</p></list-item><list-item>
      <p id="d1e849">LM6 to LM8 is generally a clast-supported, poorly sorted deposit with a
thickness ranging between 10 and 30 cm. Polygenic clasts and massive or crudely
graded angular to subangular fine pebbles to very fine granules occur.
Crudely horizontal laminae are locally recorded on top. Fragments of wood can
be encountered at the base of the layers. The basal contact is sharp and
occasionally shows evidence of erosion; the upper boundary is transitional.</p></list-item><list-item>
      <p id="d1e853">LM9 to LM10 shows massive or crudely fining-upward graded very coarse to fine
sands with a low degree of sorting. The total thickness ranges between
5 and 20 cm. Evidence of a planar lamination and scattered wood fragments is found
close to the upper boundary, which is transitional. The basal contact is
sharp.</p></list-item><list-item>
      <p id="d1e857">LM11 is fine sandy loam to clayey loam, showing a dark grayish brown color
(10YR 4/2 or 10YR 3/2). Polygenic fine to medium pebbles aligned with low
sphericity and a very angular shape occur. Both basal and top contacts are
sharp.</p></list-item><list-item>
      <p id="d1e861">LM12 is a silty deposit of dark color (10YR 3/1) with a high content of
decomposed organic matter. Occasional fine to medium pebbles aligned with
low sphericity and very angular shape occasionally occur.</p></list-item><list-item>
      <p id="d1e865">LM13 is a loam to silty clay deposit showing a coarse angular blocky structure
and dark olive gray color (5Y3/2), with yellowish brown (10YR5/6) due to the
presence of iron oxides. The deposit is deprived of calcium carbonate, and a
field pH 5.5 value was recorded.</p></list-item><list-item>
      <p id="d1e869">LM14 includes massive clayey silts with a low amount of decomposed organic matter
and a dark greenish gray color (5G 4<inline-formula><mml:math id="M32" display="inline"><mml:mo>\</mml:mo></mml:math></inline-formula>1). Scattered polygenic
clasts (fine pebbles) with low sphericity and a very angular shape are
recorded. Both basal and top contacts are sharp.</p></list-item></list></p>
      <p id="d1e879">In terms of sedimentary processes, the coarse-grained LM1–LM10 lithofacies
have been interpreted as flood deposits triggered by HIP events in the
catchment area (Milliman and Syvitski, 1992; Mulder and Syvitski, 1995;
Mutti et al., 1996). Particularly, the identified lithofacies were grouped
according to their features (i.e., grain size, color, sedimentary
structures) and the facies tract concept (Lowe, 1982; Mutti, 1992; Mutti et
al., 1996), distinguishing three main depositional settings along an
idealized transect (Fig. 4): subaerial (LM1 to LM4), marginal (LM5) and
subaqueous–lacustrine (LM6 to LM10).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4" specific-use="star"><?xmltex \currentcnt{4}?><label>Figure 4</label><caption><p id="d1e884">Idealized genetic facies tract showing the 14 lithofacies
(LM1–LM14) identified within the reference core S1, whose stratigraphy is
reported in Fig. 3.</p></caption>
            <?xmltex \igopts{width=398.338583pt}?><graphic xlink:href="https://cp.copernicus.org/articles/16/1547/2020/cp-16-1547-2020-f04.png"/>

          </fig>

      <p id="d1e894">The fine-grained facies (LM11-LM14 in Figs. 3, 4) also form two main groups.
The first group includes LM11 and LM13 (paleosol) that are characterized by
features indicative of subaerial conditions; the second group consists of
LM12 (i.e., peaty deposits) and LM14, deposited along the marginal zone of
the (paleo)lake under low-energy conditions and different degrees of
organic matter enrichment.</p>
</sec>
<?pagebreak page1554?><sec id="Ch1.S4.SS1.SSS2">
  <label>4.1.2</label><title>Stratigraphic units</title>
      <p id="d1e905">Above the ophiolite bedrock, five informal stratigraphic units have been
distinguished within core S1 and are described as follows (Fig. 3). Each
unit is interpreted in terms of depositional environment.</p>
      <p id="d1e908"><italic>Unit 1</italic> (12.25–11.30 m). This 95 cm thick unit is exclusively represented by
the LM13 lithofacies that is, in turn, composed of two main horizons
indicative of a mature paleosol. The lowermost horizon (Bw), recorded
between 12.25 and 11.60 m, corresponds to weathered deposits overlain by a 30 cm thick slickensides horizon (Bss). This unit is interpreted as a residual
pedogenized colluvium marking the base of a structural depression produced
by gravitational block sliding.</p>
      <p id="d1e913"><italic>Unit 2</italic> (11.30–4.4 m). This ca. 7 m thick unit is characterized by the
presence of several very coarse intervals (LM6–LM8) showing a thickness of
about 10–30 cm locally capped by sandy layers (LM9–LM10). Silty deposits
with a variable organic matter content, accompanied by a scarce (LM12) or
moderate (LM5) occurrence of pebbles and granules, separate the coarse-grained
intervals. This unit, which is capped by a marked unconformity surface, is
interpreted as a relatively shallow lacustrine environment subjected to
several flood events of remarkable intensity.</p>
      <p id="d1e918"><italic>Unit 3</italic> (4.4–2.3 m). This unit, ca. 2 m thick, shows sharp boundaries and the
occurrence of two subunits (3a and 3b). The lowermost subunit 3a, ranging
between 4.4 and 3.2 m, is exclusively represented by silty deposits with
scattered pebbles and granules, several wood fragments, and a mottled-like
appearance corresponding to the LM5 lithofacies. These deposits are
attributed to a marginal lacustrine environment subject to sporadic floods.
Upwards, marginal lacustrine clayey deposits (LM14) capped the sequence
(subunit 3b), documenting a period of apparent flood inactivity.</p>
      <p id="d1e924"><italic>Unit 4</italic> (2.3–0.9 m). This 1.4 m thick unit is composed of alternating coarse-grained
(LM3–LM4) and fine-grained deposits (LM12 and LM11) that record the following:
<list list-type="bullet"><list-item>
      <p id="d1e931">the disappearance  of truly lacustrine deposits that are replaced by
subaerial ones through an erosional surface that marks the lower boundary of
Unit 4 (the stratigraphic depth of this boundary is in accordance with
the altitude of the spill point of Lake Moo at 1116 m a.s.l.); and</p></list-item><list-item>
      <p id="d1e935">the return of several centimeter-thick flood deposits (LM3–LM4).</p></list-item></list></p>
      <p id="d1e938"><italic>Unit 5</italic> (0.9–0 m). This unit is characterized by the presence of several
layers of very coarse sediments (LM1–LM2) separated by finer deposits
(LM11). An erosional contact separates Unit 4 from Unit 5, which includes
the flood deposits produced by the rainfall event that occurred on
13 and 14  September 2015 (Figs. 3, 5).</p>
      <p id="d1e943">As a whole, we interpret the lacustrine succession as an infill of a
structural depression produced by gravitational block sliding that was
induced by post-glacial fluvial incision (Elter et al., 1997).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F5"><?xmltex \currentcnt{5}?><label>Figure 5</label><caption><p id="d1e948">Representative photograph of the trench (see Fig. 2 for location),
showing the uppermost 50 cm thick sedimentary succession. Though the
exposure is quite small, the graded pebble–sand couplets belonging to
Unit 5 can be interpreted as a sheet-flood deposit.</p></caption>
            <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://cp.copernicus.org/articles/16/1547/2020/cp-16-1547-2020-f05.jpg"/>

          </fig>

</sec>
</sec>
<sec id="Ch1.S4.SS2">
  <label>4.2</label><title>Age–depth model</title>
      <p id="d1e966">The age–depth model, based on 8 out of 12 <inline-formula><mml:math id="M33" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi/><mml:mn mathvariant="normal">14</mml:mn></mml:msup><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> dates available
for the S1 core (Table TS1 in the Supplement), indicates that
the sedimentary succession above the bedrock encompasses almost all of the
Holocene period (about the last 10 kyr; Fig. 6). Three ages (at 9.60,
3.10 and 2.40 m of core depth) were excluded as they show evidence of
contamination (i.e., ages younger than 1950 CE), while one sample collected
at 2.35 m was not datable due to a very low organic matter content. The
selected calibrated ages are stratigraphically coherent and mainly derived
from wood fragments and peaty deposits. In order to reduce the potential
bias due to long-lived plants and reworking processes, small twigs were
selected (Oswald et al., 2005) from fine-grained deposits and identified
when possible (e.g., <italic>Pinus</italic> and <italic>Abies alba</italic>). Due to the small dimension of the basin and the
ophiolite prevalence in the drainage area (Fig. 2), we consider
the hard-water effect on peats negligible.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F6" specific-use="star"><?xmltex \currentcnt{6}?><label>Figure 6</label><caption><p id="d1e989">S1 core stratigraphy and the age–depth model obtained from
radiocarbon dates. Red and orange lines represent the 2-sigma probability
envelope.</p></caption>
          <?xmltex \igopts{width=398.338583pt}?><graphic xlink:href="https://cp.copernicus.org/articles/16/1547/2020/cp-16-1547-2020-f06.png"/>

        </fig>

      <?pagebreak page1555?><p id="d1e998">The resulting age–depth model suggests the occurrence of four main
stratigraphic intervals in terms of sedimentation rates. The lowermost
interval (about 9.5–7.3 cal kyr BP) denotes a mean accumulation rate of ca.
0.50 mm yr<inline-formula><mml:math id="M34" 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>  that increases up to ca. 2.38 mm yr<inline-formula><mml:math id="M35" 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> within the overlying section
dated around 7.3–5.5 cal kyr BP. A change in the accumulation rate occurs
at around 5 m with a drop to ca. 0.3 mm yr<inline-formula><mml:math id="M36" 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> between the 5.5 and 4.0 cal kyr BP
interval. Between ca. 4.5 and 3 m, the deposit shows an uncertain chronology due
to the lack of reliable radiocarbon dates and the occurrence of an
unconformity surface at around 4.5 m, at the contact between Units 2 and 3 (Figs. 3, 6). During recent times (the last 146–14 cal yr BP), the accumulation
rate has increased, reaching ca. 12 mm yr<inline-formula><mml:math id="M37" 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>
</sec>
</sec>
<sec id="Ch1.S5">
  <label>5</label><title>Discussion</title>
      <p id="d1e1059">As a basis for discussion we assemble, and temporally synchronize, the Lake
Moo data with the most relevant paleoclimate proxy available from
the literature, focusing on the N Apennines paleoarchives (Figs. 1, 7). As a
whole, the Holocene infilling succession of the lacustrine basin (i.e.,
Units 2–3) is composed of an alternation of centimeters- to meters-thick,
coarse-grained flood deposits and silts characterized by a variable amount
of organic matter (Sect. 4.1. and 4.2.; Figs. 3, 4, 7). The coarse
intervals are particularly well-developed and frequent within the portion of
stratigraphic Unit 2, which is chronologically correspondent to the HTM
(Holocene Thermal Optimum), constrained between ca. 9 and 5 kyr cal BP in the
nearby Lake Verdarolo (Samartin et al., 2017, in Fig. 7a; Sect. 3.4).
Interestingly, stable oxygen isotope records from the nearby Apuan Alps
(Corchia caves; Fig. 1) document that, within the same time interval, the
wettest conditions were observed (I and II humid periods in Fig. 7b) with a
peak between ca. 8500 and 7500 cal yr BP (I humid period; Regattieri et al.,
2014; Zanchetta et al., 2011). This precipitation peak is in phase with a
clastic layer dated to 8.2 and 7.1 cal kyr BP, indicative of a period of
enhanced cave flooding triggered by high-magnitude precipitation events
(Zhornyak et al., 2011). The authors attribute this maximum fluvial activity
to an increase in strong convective episodes like the one that affected the
Versilia region in 1996 (see Cacciamani et al., 2000, for a description of
the Versilia flood event).</p>

      <?xmltex \floatpos{p}?><fig id="Ch1.F7" specific-use="star"><?xmltex \currentcnt{7}?><label>Figure 7</label><caption><p id="d1e1064">Stratigraphy of core S1, main palynological features and
microcharcoal content. Relative abundances of the pollen groups that are explained in the
text (Sect. 3.3) are reported along with the frequencies of
hygrophilous herbs and aquatics. Asterisks point to samples containing
coprophilous fungi and other spores like<italic> Sporormiella</italic>, <italic>Dicrocoelium</italic> and <italic>Ascaris</italic>. These data are compared
with the most relevant paleoclimate reconstructions available from
the literature for the area of interest. <bold>(a)</bold> Reconstructed mean July air
temperature from Lake Verdarolo (from Samartin et al., 2017); <bold>(b)</bold>
<inline-formula><mml:math id="M38" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O speleothem records and reconstructed precipitation trends
(mean anomaly time series) from Corchia cave (slightly modified from
Combourieu et al., 2013; Zanchetta et al., 2011; Zhornyak et al., 2011); and
<bold>(c)</bold> June (red)  to December (blue) insolation values reported for
45<inline-formula><mml:math id="M39" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N (from Samartin et al., 2017). Main Holocene climate
phases and events are also shown (Regattieri et al., 2014). Available
radiocarbon ages are reported as calibrated years BP.</p></caption>
        <?xmltex \igopts{width=554.82874pt, angle=90}?><graphic xlink:href="https://cp.copernicus.org/articles/16/1547/2020/cp-16-1547-2020-f07.png"/>

      </fig>

      <p id="d1e1112">Climatic simulations (monthly temperature and precipitation) for the
mid-Holocene climatic conditions (Tinner et al., 2013) show higher
precipitation in autumn over the northern Apennines. We speculate that the
precipitation increases, also reflected in high-frequency flood activity,
could have occurred during a phase of a progressive reduction in the Hadley
cell, paralleled by a reduction in subtropical high pressure after the
insolation peak (Fig. 7c). This would lead to enhanced meteorological
activity over the Mediterranean area due to the midlatitude weather
systems, especially at the transition towards the cold season. Although in
decline, the presence of the African monsoon (Skinner and Poulsen, 2016)
could also have contributed to enriching subtropical air masses in the water
vapor potentially extractable<?pagebreak page1556?> by midlatitude synoptic disturbances.
Accordingly, Krichak et al. (2015) documented how this mechanism is relevant
for modern extremes in precipitation in the Mediterranean; moreover, the
events occurring in the autumn months are characterized by a greater
transport of water vapor from the subtropical Atlantic, even across North
Africa.</p>
      <p id="d1e1116">With the end of the HTM, a drastic decrease in flood activity is documented
at Lake Moo, as the coarse intervals are abruptly reduced in number and thickness
within the uppermost portion of Unit 2 (ca. 5.5–3.8 kyr BP). This
stratigraphic trend is reasonably interpreted as the expression of a
decrease in the frequency of HIP events over the study area under cooler and
less humid climate conditions (Fig. 7). The limit between Unit 2 and Unit 3
corresponds to an unconformity that marks the passage to a marginal
lacustrine succession of uncertain age, at least for the lowermost portion
(subunit 3a). This interpretation is supported by palynological data, which
show high values of herbaceous hygrophytes (mainly Cyperaceae) and aquatic
species.</p>
      <p id="d1e1119">The upper subunit 3b, dated around 146–14 cal yr BP, is almost deprived of
coarse materials, documenting a period of apparent flood inactivity at Lake
Moo (Figs. 3, 7). This is followed by a reactivation of flood processes from
ca. 1800 CE (i.e., coarse-grained flood deposits within Units 4–5; Figs. 3,
7) with a minimum of 5 events to a maximum of 12 events every 100 years, as the confidence range associated with the calibrated age at 2.80 m
is rather wide (146–14 cal yr BP; Fig. 7). Despite the low degree of
precision affecting radiocarbon ages younger than 200 years, this renewed
increase in flood activity fits well with the instrumental record that
points to a significant increase in record-breaking (from 3 to 24 h
accumulations) precipitation events in the northern Apennines (Libertino et
al., 2019) starting from the second half of the last century. These phenomena
seem to be responsible for the replacement of lake deposits by subaerial
ones through an erosional contact (Unit 4 lower boundary).</p>
      <?pagebreak page1558?><p id="d1e1122">To compare the most recent stratigraphic units (Units 4–5) with quantitative
climate data, the instrumental temperature values, available since the
second half of the last century from the Eraclito ER dataset, has been added
to the Verdarolo curve. The overlap with the latest part of the Verdarolo curve
confirms the good accuracy of the reconstruction technique in this region
(Fig. 8). The recent sharp temperature increase is striking if compared with
the whole Holocene, and the current July temperature is comparable with the
maximum temperature reached at HTM over the study area. The actual trend of
July temperature, estimated over the period 1961–2018 from monthly mean
values, is <inline-formula><mml:math id="M40" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">4.3</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M41" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C in 100 years. The trend is statistically
significant, with <inline-formula><mml:math id="M42" display="inline"><mml:mi>p</mml:mi></mml:math></inline-formula> value <inline-formula><mml:math id="M43" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 0.0004 (see Sect. 3.4), and more than
double the maximum temperature gradient found in the Verdarolo curve at
<inline-formula><mml:math id="M44" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>2 <inline-formula><mml:math id="M45" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C per 100 years at the end of the Little Ice Age (1850–1900).
From Figs. 6 and 7, we observe flood intensification corresponding to periods
of rising temperatures. This is testified by the exceptionally high
accumulation rate estimated on the recent period for Units 4–5 (Fig. 6;
Sect. 4.3), a rate of about 1 m per 100 years calculated since ca. 1800 CE.
The recent increase in flood activity is also supported by instrumental
data, wherein we also observe an emerging trend (not yet significant) of
precipitation intensity increase (as both a daily maximum and monthly
cumulative values) in the autumn months (Fig. 9).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F8"><?xmltex \currentcnt{8}?><label>Figure 8</label><caption><p id="d1e1177">Comparison of current data and reconstructed July mean temperature
at the Lake Verdarolo site (see Fig. 1 for location). The blue line is the
reconstructed temperature, and the shaded area is the sample-specific
estimated standard error associated with the temperature reconstruction
based on the chironomid assemblage from Samartin et al. (2017). The orange line
represents the July mean temperature (1961–2018) retrieved for the grid cell
of Lake Verdarolo from the Emilia–Romagna climate reanalysis Eraclito (11-year
running average). The shaded orange area is <inline-formula><mml:math id="M46" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 1 standard deviation.
The full available period is reported on the left, while a zoom into the most
recent period (since 1600 CE) is shown on the right.</p></caption>
        <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://cp.copernicus.org/articles/16/1547/2020/cp-16-1547-2020-f08.png"/>

      </fig>

<sec id="Ch1.S5.SS1">
  <label>5.1</label><title>Holocene flood activity, paleotemperature changes and HIP events</title>
      <p id="d1e1200">A positive link emerges correlating Holocene (July) paleotemperatures,
precipitation intensity reconstructions and flood history (Fig. 7) at the
study site, as the stratigraphic units showing the highest frequency of
coarse-grained flood deposits (i.e., Units 2, 4 and 5) invariably fall into
periods of higher temperatures (i.e., HTM and the post-LIA time). This
strongly supports the hypothesis that greater warmth favors the occurrence
of extreme precipitation events, probably more frequently at the end of the
summer–autumn as already reported by other authors (e.g., Marcott et al.,
2013; Giguet-Covex et al., 2012). Although the process attribution and the
geographical uniformity of the HTM wet phase are still a matter of debate, the
abundance of coarse-grained flood deposits within the Lake Moo record around
9.5–5.5 kyr BP suggests a precipitation increase also identified in other
sites of the central and southern Mediterranean (Magny et al., 2012b).</p>
      <p id="d1e1203">However, local factors such as changes in vegetation cover (i.e., tree cover
percentage) due to human disturbance and fires could have significantly
contributed to enhancing slope erosion and then influenced the Lake Moo
sedimentary record, partly weakening our reconstruction of the
temperature–HIP–flood activity relationship at the Holocene scale. In order
to overcome this issue, we explored and compared the pollen and
microcharcoal content of two key intervals (I<inline-formula><mml:math id="M47" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:math></inline-formula> and I<inline-formula><mml:math id="M48" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> in Figs. 7,
10) that are characterized by a different flood record (high versus low flood
activity) formed during consecutive periods of distinct climate conditions:
the HTM and the following cooling. The difference in mean temperature
between I<inline-formula><mml:math id="M49" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:math></inline-formula> and I<inline-formula><mml:math id="M50" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, obtained by averaging the corresponding
chronological intervals in the Verdarolo paleotemperature curve, is
<inline-formula><mml:math id="M51" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>1.3 <inline-formula><mml:math id="M52" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C, while the maximum difference reaches <inline-formula><mml:math id="M53" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>3.1 <inline-formula><mml:math id="M54" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C
(Fig. 8).</p>
      <p id="d1e1275">For the post-LIA interval, in particular since 1950 CE, no significant contribution to debris mobilization can be attributed to
vegetation landscape changes along the slopes as Lake Moo is a protected
area characterized by dense forests (Corticelli et al., 2011; Sect. 2.1).
Consistently, the most recent pollen sample (P14 yielding an age of 146–14 cal yr BP; Fig. 7) shows a tree cover of about 80 %.</p>
      <p id="d1e1278">The main considerations arising from the in-depth analysis of I<inline-formula><mml:math id="M55" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:math></inline-formula> and
I<inline-formula><mml:math id="M56" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> are the following.
<list list-type="bullet"><list-item>
      <p id="d1e1301">For I<inline-formula><mml:math id="M57" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:math></inline-formula> (ca. 9.5–7 kyr BP; 10.5–9 m of core depth), the woody component (i.e.,
tree cover percent) is invariably higher than the herbaceous one, and it shows a
value of 80 % on average. The conifers, mainly represented by pines and
silver fir, are dominant with respect to the deciduous trees (e.g., <italic>Corylus avellana</italic> and
<italic>Quercus</italic>), reaching a maximum of 95 % within the P4 sample dated between 9.3 and 9.1 cal kyr BP. Interestingly, <italic>Abies alba</italic> shows the highest percentages (ca. 15 %–55 %)
within the chronological interval that corresponds to the warmest period of
the HTM (Figs. 7, 10; Samartin et al., 2017). Moreover, <italic>A. alba</italic> reaches the peak of
ca. 55 % during the HTM wettest conditions (around 7.5–7.3 cal kyr BP;
I<inline-formula><mml:math id="M58" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:math></inline-formula> humid period in Fig. 7), as reconstructed by several authors
(Regatieri et al., 2014; Zanchetta et al., 2011; Zhornyak et al., 2011) from
the Apuan Alps speleothems. This trend is consistent with the fact that <italic>A. alba</italic> is
a warm-temperature tree with a preference for high moisture availability
(Tinner et al., 2013), as clearly documented within the nearby Lake Greppo
record (Vescovi et al., 2010, confirming higher rainfall accumulation
already highlighted by lake-level dynamics from the Jura Mountains and
central–northern Italy; Magny et al., 2004, 2009, 2012b). Although no
specific inferences can be made on past water levels of Lake Moo, it is
interesting to note that the low amount of hygrophytes and aquatics (Fig. 7)
is fully consistent with highstand conditions. Anthropogenic indicator taxa
(Fig. 7), as well as the anthropogenic index (AI; Fig. 10), show very low
values throughout the interval, documenting a negligible human impact on the
area in accordance with the extremely low content of microcharcoals
(0.01–0.13 mm<inline-formula><mml:math id="M59" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula> g<inline-formula><mml:math id="M60" 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. 10). Besides, the coarser microcharcoals
(<inline-formula><mml:math id="M61" display="inline"><mml:mrow><mml:mi mathvariant="italic">&gt;</mml:mi><mml:mn mathvariant="normal">125</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M62" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>m) are not recorded, suggesting no significant local
fires. A slightly higher amount of anthropogenic indicator taxa occurs
within sample P6, dated between 8070 and 7880 ca yr BP; this<?pagebreak page1559?> is interpreted
as an effect of categorization difficulties about spontaneous taxa such as
<italic>Artemisia vulgaris</italic> type, <italic>Chenopodium</italic>, <italic>Plantago</italic> and <italic>Urtica</italic>.</p>
      <p id="d1e1390">Palynological data, combined with the stratigraphic interpretation of the S1
core, support our hypothesis that warmer and wetter conditions typical of
the HTM led to a high amount of HIP and then high flood activity in the
basin, independently of local factors. The presence of an extensive
vegetation cover along the slopes implies the need for even more intense
rainfall to trigger a debris mobilization that leads to the deposition of
thick, coarse-grained layers containing pebbles with remarkable diameters (LM6,
LM7 and LM8 in Fig. 10).</p></list-item><list-item>
      <p id="d1e1394">For I<inline-formula><mml:math id="M63" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> (ca. 5.5–3.8 kyr BP.; 5.5–4.5 m of core depth), tree cover reduction
(ranging between ca. 87.4 % and 45.1 %; Figs. 7, 9), in favor of grassland
expansion, characterizes this interval that sees a fall in <italic>A. alba</italic> percentages
(commonly less than 10 %) and a high amount of meadow taxa (mainly
<italic>Poaceae</italic>, <italic>Cichorioideae</italic> and <italic>Asteroideae</italic>; Fig. 7). The growth in hygrophytes and aquatics (up to ca.
18.2 %) is consistent with a marginal lacustrine environment and then a
relative lowering of the water level. Both anthropogenic indicator taxa and
AI increase, up to ca. 7.3 % and 16.2 %, respectively (Figs. 7, 9),
suggesting a moderate degree of human impact on the vegetation cover (i.e.,
tree cover changes). This impact is probably due to pastoral activities
more than agriculture as few cereal grains are locally encountered (less
than 4 %). Accordingly, the meadow (pasture) taxa are abundant, and
coprophilous fungi and others spores (<italic>Sporormiella</italic>, <italic>Dicrocoelium</italic> and <italic>Ascaris</italic>; Figs. 7, 9) are sporadically
found. By contrast, microcharcoal remains very low in amount, pointing to
little fire activity.</p>
      <p id="d1e1428">Although pollen-derived vegetation features (i.e., decrease in tree cover
and a moderate degree of human impact) document local conditions more
favorable for debris flow activation with respect to those
characterizing I<inline-formula><mml:math id="M64" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:math></inline-formula>, this interval shows low flood activity with few and
thin (<inline-formula><mml:math id="M65" display="inline"><mml:mrow><mml:mi mathvariant="italic">&lt;</mml:mi><mml:mn mathvariant="normal">5</mml:mn></mml:mrow></mml:math></inline-formula> cm) sandy deposits (LM9 to LM10 in Fig. 10). Integrating
the I<inline-formula><mml:math id="M66" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> stratigraphic record with pollen data, such low flood activity
most likely reflects a low frequency (and intensity) of HIP events during a
cooler and less humid period (Figs. 7, 9).</p></list-item></list></p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F9" specific-use="star"><?xmltex \currentcnt{9}?><label>Figure 9</label><caption><p id="d1e1462">Monthly mean 2 m temperature <bold>(a)</bold>, accumulated precipitation <bold>(b)</bold> and
maximum daily precipitation <bold>(c)</bold> for 1961–1990 (blue) and 1991–2018 (green)
computed over the Lake Moo site grid cell of the Eraclito reanalysis (grid cell 258,
Ferriere Municipality). Confidence intervals at 95 % significance (black
vertical segments) are computed with a bootstrapping method (1000
iterations) as part of the Seaborn Python library.</p></caption>
          <?xmltex \igopts{width=369.885827pt}?><graphic xlink:href="https://cp.copernicus.org/articles/16/1547/2020/cp-16-1547-2020-f09.png"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F10" specific-use="star"><?xmltex \currentcnt{10}?><label>Figure 10</label><caption><p id="d1e1482">Sedimentological and palynological features of two key
stratigraphic intervals (Intervals 1 and 2) from the reference core S1.
These features are compared with the most relevant paleoclimate data
available from the literature for the area of interest (for references, please
see Fig. 7). The anthropogenic index (AI) has been calculated as
(anthropogenic indicator <inline-formula><mml:math id="M67" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> tree percentage)<inline-formula><mml:math id="M68" display="inline"><mml:mo>⋅</mml:mo></mml:math></inline-formula>100 following Accorsi et al. (1999). Asterisks point to samples containing coprophilous fungi and other
spores like <italic>Sporormiella</italic>, <italic>Dicrocoelium</italic> and <italic>Ascaris</italic>. Core S1 sample ages derive from the age–depth model
reported in Fig. 6. P samples correspond to the pollen samples; LM labels
refer to the lithofacies explained in the text (Sect. 4.1) and in Figs. 3–4; dmax corresponds to the maximum diameter.</p></caption>
          <?xmltex \igopts{width=497.923228pt}?><graphic xlink:href="https://cp.copernicus.org/articles/16/1547/2020/cp-16-1547-2020-f10.png"/>

        </fig>

      <p id="d1e1514">The paleoenvironmental–paleovegetation features characterizing the Interval
2 persists up-core, in correspondence to Unit 3 that records apparent flood
inactivity (Figs. 3, 7). The uppermost sample P14 likely tracks a strong
increment of <italic>A. alba</italic>.</p><?xmltex \hack{\newpage}?>
</sec>
</sec>
<sec id="Ch1.S6" sec-type="conclusions">
  <label>6</label><title>Conclusions</title>
      <p id="d1e1530">Placing present climate conditions into a geological perspective, beyond the
instrumental era, is essential for understanding changes in the hydrological
cycle induced by anthropogenic climate warming, complementing projections of
model simulations. Physical reasons and regional climate reconstructions are
consistently pointing to an increase in precipitation intensity when water
vapor is not limited. In the last decade, record-breaking rainfall events
have frequently occurred around the world. This trend is emerging with
variable strength in different areas. Therefore, in the attempt to
build confidence in the extreme precipitation trend, we extended
our analysis, passing from the instrumental to the geological timescale
(i.e., the Holocene period). This choice implies a robust multidisciplinary
approach, which includes, in addition to climate and meteorological data,
proxy and expertise coming from the geological, geomorphological,
stratigraphic and palynological–microanthracological area.</p>
      <p id="d1e1533">The major outcomes of our work can be summarized as follows.
<list list-type="order"><list-item>
      <p id="d1e1538">The matching of instrumental temperature data and paleoenvironmental data
allow us to affirm that current summer temperature is comparable with the
temperature recorded in the northern Apennines during the HTM. The current
temperature trend computed from the monthly values of July temperature at
the Lake Verdarolo site over the period 1961–2018 is <inline-formula><mml:math id="M69" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">4.3</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M70" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C per 100 years (highly statistically significant), and it is likely to be one of the highest
recorded in the Holocene.</p></list-item><list-item>
      <p id="d1e1561">The stratigraphic units showing a high frequency of coarse-grained flood
deposits are Unit 2, deposited in the HTM, and Units 4 and 5, which belong
to the post-LIA time. Both periods are characterized by higher temperatures.
The human impact is almost absent in the HTM and very low in the post-LIA
time, especially in the last part of the 20th century. This strongly
supports the hypothesis that greater warmth favors the occurrence of
extreme precipitation events. In particular, the recent sedimentation rate
computed since ca. 1800 CE (post-LIA) is at least 1 m per 100 years. This high
value of the sedimentation rate has to be correlated with the presence of
numerous coarse-grained levels within Units 4 and 5, after a period of
absence of flood deposits in subunit 3b. This difference in flood layers must
be linked to an increase in HIP over the Lake Moo basin since we could not
attribute it to any other changes in physiographic or vegetation dynamics
(i.e., tree cover). During the HTM and current time, the forested area coverage
around Lake Moo has persisted at high values, and this factor is considered
disadvantageous for debris mobilization. On the contrary, during about 6–4 kyr BP we did not find any increase in coarse-grained layers from<?pagebreak page1560?> flood
events, even though the forested area declined significantly and the
anthropogenic impact increased.</p></list-item><list-item>
      <p id="d1e1565">HIP increase in response to higher temperature is already detectable in
observation series. We found evidence that this also occurred in the past,
especially during the HTM, as testified by the higher deposition of coarse-grained
levels. A comparison with the past helps to understand future projections for
the area. However, we are aware that past evolution cannot be taken as a
perfect analogy for the future due to the<?pagebreak page1561?> different forcing and consequent
response of the climate system (D'Agostino et al., 2019). As temperature
will continue to increase in the Mediterranean area, precipitation intensity
would keep increasing over the northern Apennines. We hypothesize that
precipitation intensity increase will be more evident in months with cooler
and moist air masses, like in autumn and in winter, when moisture
availability is not limited. An increase in precipitation maxima in autumn
months is already emerging on the northern Apennines.</p></list-item></list></p>
      <p id="d1e1568">The Lake Moo basin proves to be an ideal study area to achieve a reconstruction
between high-intensity precipitation and debris flow due to its position relative to
the dominant atmospheric flow and favorable geological, geomorphological
and vegetation characteristics. Further investigations, in association with
other analogous sites along the northern Apennines crest, are planned to
provide a multi-site assessment of the dynamics of past extreme precipitation
events.</p>
</sec>

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

      <p id="d1e1575">Original data acquired during the field campaign (including pollen counts, radiocarbon analysis and photos) are
available on the open data repository of ARPAE Emilia–Romagna
(<uri>https://arpaeprv.datamb.it/dataset/lake-moo</uri>, Grazzini et al., 2019).</p>
  </notes><app-group>
        <supplementary-material position="anchor"><p id="d1e1581">The supplement related to this article is available online at: <inline-supplementary-material xlink:href="https://doi.org/10.5194/cp-16-1547-2020-supplement" xlink:title="pdf">https://doi.org/10.5194/cp-16-1547-2020-supplement</inline-supplementary-material>.</p></supplementary-material>
        </app-group><notes notes-type="authorcontribution"><title>Author contributions</title>

      <p id="d1e1590">SS and FG developed the idea and the research activity
planning and execution. SN, MA and MTDN have taken care of the administrative
aspects. All authors, except for SN and MTDN, contributed to field
activity. Granulometric analysis was conducted by AC. Pollen analysis
was conducted by SM and MM; data elaboration and figures were
created by VR, SM and MM. SS, FG and VR prepared the paper with
contributions from all co-authors. FG provided management and coordination.</p>
  </notes><notes notes-type="competinginterests"><title>Competing interests</title>

      <p id="d1e1596">The authors declare that they have no conflict of interest.</p>
  </notes><ack><title>Acknowledgements</title><p id="d1e1602">We are very grateful for all comments received in the public
discussion; in particular, we thank reviewers Picotti and Tinner for
their useful suggestions. Finally, we thank Francesca Staffilani
(Geological, Seismic and Soil Service, Emilia–Romagna region) for the
pedological data interpretation.</p></ack><notes notes-type="financialsupport"><title>Financial support</title>

      <p id="d1e1607">This research has been supported by the Regional
Agency of Civil Protection and the
Geological, Seismic and Soil Survey of the Emilia-Romagna Region
in the framework of the cooperation agreement with ARPAE-SIMC.</p>
  </notes><?xmltex \hack{\newpage}?><notes notes-type="reviewstatement"><title>Review statement</title>

      <p id="d1e1615">This paper was edited by Keely Mills and reviewed by Vincenzo Picotti and Willy Tinner.</p>
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    <!--<article-title-html>Changes in high-intensity precipitation on the northern Apennines (Italy) as revealed by multidisciplinary data over the last 9000 years</article-title-html>
<abstract-html><p>Several record-breaking precipitation events have struck the
mountainous area of the Emilia–Romagna region (northern Apennines, Italy) over
the last 10 years. As a consequence, severe geomorphological processes such
as debris avalanches and debris flows, shallow landslides, and overbank
flooding have affected the territory, causing severe damage to human-made
structures. The unusual intensity of these phenomena prompted an
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of extreme precipitation events that may have occurred in the past. We
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September 2015, several debris flows generated by small streams
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precipitation events. The sedimentary succession (ca. 13&thinsp;m thick) was
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with organic-rich silty clays and peat layers, was analyzed by combining
sedimentological, pollen, microanthracological and pedological data with
radiocarbon dating (AMS <sup>14</sup>C) in an innovative multidisciplinary
approach for this area. Original data acquired during the field campaign
were also correlated with other specific paleoclimatic proxies available in
the literature for the northern Apennines area. We discover that the
increase in extreme paleoflooding, associated with coarse-grained deposits
similar to the ones observed recently, correlates well with the warm phases
of the Holocene Thermal Maximum and with the ongoing warming trend observed
that started at the beginning of the last century.</p></abstract-html>
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