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  <front>
    <journal-meta><journal-id journal-id-type="publisher">NHESS</journal-id><journal-title-group>
    <journal-title>Natural Hazards and Earth System Sciences</journal-title>
    <abbrev-journal-title abbrev-type="publisher">NHESS</abbrev-journal-title><abbrev-journal-title abbrev-type="nlm-ta">Nat. Hazards Earth Syst. Sci.</abbrev-journal-title>
  </journal-title-group><issn pub-type="epub">1684-9981</issn><publisher>
    <publisher-name>Copernicus Publications</publisher-name>
    <publisher-loc>Göttingen, Germany</publisher-loc>
  </publisher></journal-meta>
    <article-meta>
      <article-id pub-id-type="doi">10.5194/nhess-21-2881-2021</article-id><title-group><article-title>UAV survey method to monitor and analyze geological <?xmltex \hack{\break}?> hazards: the case study of the mud volcano of <?xmltex \hack{\break}?> Villaggio Santa Barbara, Caltanissetta (Sicily)</article-title><alt-title>UAV survey method to monitor and analyze geological hazards</alt-title>
      </title-group><?xmltex \runningtitle{UAV survey method to monitor and analyze geological hazards}?><?xmltex \runningauthor{F. Brighenti et al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Brighenti</surname><given-names>Fabio</given-names></name>
          
        <ext-link>https://orcid.org/0000-0003-3292-9335</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Carnemolla</surname><given-names>Francesco</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-8403-5187</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3">
          <name><surname>Messina</surname><given-names>Danilo</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="yes" rid="aff1 aff2">
          <name><surname>De Guidi</surname><given-names>Giorgio</given-names></name>
          <email>deguidi@unict.it</email>
        </contrib>
        <aff id="aff1"><label>1</label><institution>Department of Biological, Geological and Environmental Sciences,
<?xmltex \hack{\break}?> University of Catania, Corso Italia 55–57, Catania, 95129, Italy</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>CRUST – Interuniversity Center for 3D Seismotectonics with
territorial applications – UR-UniCT, <?xmltex \hack{\break}?>Corso Italia 55–57, Catania, 95129, Italy</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>independent researcher: INGV-Osservatorio Etneo, Piazza Roma 2, Catania, 95125, Italy</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Giorgio De Guidi (deguidi@unict.it)</corresp></author-notes><pub-date><day>28</day><month>September</month><year>2021</year></pub-date>
      
      <volume>21</volume>
      <issue>9</issue>
      <fpage>2881</fpage><lpage>2898</lpage>
      <history>
        <date date-type="received"><day>16</day><month>November</month><year>2020</year></date>
           <date date-type="rev-request"><day>3</day><month>December</month><year>2020</year></date>
           <date date-type="rev-recd"><day>5</day><month>August</month><year>2021</year></date>
           <date date-type="accepted"><day>24</day><month>August</month><year>2021</year></date>
      </history>
      <permissions>
        <copyright-statement>Copyright: © 2021 Fabio Brighenti et al.</copyright-statement>
        <copyright-year>2021</copyright-year>
      <license license-type="open-access"><license-p>This work is licensed under the Creative Commons Attribution 4.0 International License. To view a copy of this licence, visit <ext-link ext-link-type="uri" xlink:href="https://creativecommons.org/licenses/by/4.0/">https://creativecommons.org/licenses/by/4.0/</ext-link></license-p></license></permissions><self-uri xlink:href="https://nhess.copernicus.org/articles/21/2881/2021/nhess-21-2881-2021.html">This article is available from https://nhess.copernicus.org/articles/21/2881/2021/nhess-21-2881-2021.html</self-uri><self-uri xlink:href="https://nhess.copernicus.org/articles/21/2881/2021/nhess-21-2881-2021.pdf">The full text article is available as a PDF file from https://nhess.copernicus.org/articles/21/2881/2021/nhess-21-2881-2021.pdf</self-uri>
      <abstract><title>Abstract</title>
    <p id="d1e130">Active geological processes often generate a ground surface response such as uplift, subsidence and faulting/fracturing. Nowadays remote sensing represents a key tool for the evaluation and monitoring of natural hazards. The use of unmanned aerial vehicles (UAVs) in relation to observations of natural hazards encompasses three main stages: pre- and post-event data acquisition, monitoring, and risk assessment. The mud volcano of Santa Barbara (Municipality of Caltanissetta, Italy) represents a dangerous site because on 11 August 2008 a paroxysmal event caused serious damage to infrastructures within a range of about 2 km. The main precursors to mud volcano paroxysmal events are uplift and the development of structural features with dimensions ranging from centimeters to decimeters. Here we present a methodology for monitoring deformation processes that may be precursory to paroxysmal events at the Santa Barbara mud volcano. This methodology is based on (i) the data collection, (ii) the structure from motion (SfM) processing chain and (iii) the M3C2-PM algorithm for the comparison between point clouds and uncertainty analysis with a statistical approach. The objective of this methodology is to detect precursory activity by monitoring deformation processes with centimeter-scale precision and a temporal frequency of 1–2 months.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <label>1</label><title>Introduction</title>
      <p id="d1e142">In recent decades, both high-resolution digital photographs and structure
from motion (SfM) software have enabled the generation of high-quality
topographic information. In geosciences many studies have been dedicated to
morphological processes (Castillo et al., 2012; James and Robson, 2012;
James and Varley, 2012; Amici et al., 2013b; Casella et al., 2014;
Gomez-Gutierrez et al., 2014; James and Robson, 2014; Lucieer et al., 2014;
Ryan et al., 2015; Westoby et al., 2015; Woodget et al., 2015; Eltner et
al., 2015; Dietrich, 2016b; Smith et al., 2016; Javernick et al., 2016;
Walter et al., 2018; Deng et al., 2019; Johnson et al., 2014). Applications include runoff laboratory trials (Morgan et al., 2017), applied geology (Niethammer et al., 2012; Russell, 2016; Saito et al., 2018), geomorphology (Bemis et al., 2014; Javernick et al., 2014; Snapir et al., 2014; Dietrich, 2014; Smith and Vericat, 2015; Bakker and Lane, 2015; Dietrich, 2016a, b; Mercer and Westbrook, 2016; Pearson et al., 2017; Prosdocimi et al., 2017; Marteau et al., 2016; Balaguer-Puig et al., 2017; Vinci et al., 2017; Heindel et al., 2018; Seitz et al., 2018), glaciology (Immerzeel et al., 2017; Piermattei et al., 2016), coastal morphology (James and Robson, 2012; Casella et al., 2016; Brunier et al., 2016), volcanology (James and Robson, 2012; Bretar et al., 2013; Müller et al., 2017; Giordan et al., 2017, 2018; Carr et al., 2018; Favalli et al., 2018; Witt et al., 2018; Andaru and Rau, 2019; Bonali et al., 2019; De Beni et al., 2019) and geophysics (Amici et al., 2013a; Greco<?pagebreak page2882?> et al., 2016; Di Felice et al., 2018; Zahorec et al., 2018; Federico et al., 2019). SfM is commonly used in the cultural heritage field for 3D reconstruction (Sapirstein, 2016, 2018; Sapirstein and Murray, 2017; Jalandoni et al., 2018). The monitoring of active geological processes is a preventive action in risk mitigation (Stöcker et al., 2017; Turner et al., 2017b; Diefenbach et al., 2018; Rosa et al., 2018; Deng et al., 2019). Disasters occur when two factors – hazard and vulnerability – coincide. The risk is proportional to the magnitude of the hazards and the vulnerability of the affected population. Among the deformation monitoring systems, the photogrammetry technique from unmanned aerial vehicles (UAVs) is becoming more widely used thanks to the high efficiency in data acquisition, the low cost compared to traditional techniques and the acquisition of high-resolution images (Harwin and Lucieer, 2012; James and Robson, 2012; Westoby et al., 2012; Fonstad et al., 2013; Javernick et al., 2014; Johnson et al., 2014; James et al., 2017a, b, 2020). This technique is important for studying catastrophic natural events such as floods, earthquakes, landslides, etc. Different acquisition methods and the ability to obtain high spatial (centimeter) and temporal resolution (hours or days) (Boccardo et al., 2015) enable the acquisition of detailed information on the evolution of the landscape; therefore UAVs are an effective and complementary tool for field
investigations. Furthermore, UAVs have other advantages including (i) the
ability to fly at low altitudes, (ii) the ability to reach remote locations,
(iii) the ability to host multiple sensors (cameras, lidar, thermal imaging
cameras, navigation/inertial sensors, etc.), (iv) the ability to capture
images at different angles and (v) the flexibility to carry out monitoring
operations on a small, medium and large scale (Jordan et al., 2018). Ground
control points (GCPs) are used to improve the accuracy of the resulting
data. Therefore, recognizable points in the UAV imagery are measured with a
high-precision surveying device to georeference the data. In this process a
correct number of GCPs is required which leads to a greater accuracy of the
resulting data (point clouds, 3D grid, orthomosaic or digital surface model, DSM). The precision of the resulting data is also controlled by other
variables, such as the focal distance of the camera, flight path and flight
altitude, the orientation of the camera, the picture quality, the processing
chain, and the category of UAV system (fixed or rotary wings).</p>
      <p id="d1e145">In this paper, we present the results and analysis of the surface
deformation monitoring of the mud volcano of Santa Barbara (Caltanissetta,
central Sicily) (Fig. 1). We have applied the statistical analysis of
significant changes with a level of detection at 95 % confidence  (LoD<inline-formula><mml:math id="M1" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">95</mml:mn><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="italic">%</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula>). In detail, we used precision maps and the M3C2-PM (Lague et al., 2013; James et al., 2017b) algorithm to determine the surface variations. The statistical analysis allows us to verify (i) the uncertainty between the different surveys, (ii) the spatial variability in the accuracy in the surveys (James et al., 2017b) and (iii) the quality of the georeferencing of the surveys based on the number of GCPs.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1"><?xmltex \currentcnt{1}?><?xmltex \def\figurename{Figure}?><label>Figure 1</label><caption><p id="d1e163">Aerial view of the Santa Barbara mud volcano. Photo taken by the
UAV from the west side of the mud volcano.</p></caption>
        <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/21/2881/2021/nhess-21-2881-2021-f01.jpg"/>

      </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2"><?xmltex \currentcnt{2}?><?xmltex \def\figurename{Figure}?><label>Figure 2</label><caption><p id="d1e175">Cartographic extract with the location of the major fractures (in
red) detected on the ground and the damaged structures (in yellow) related
to the paroxysmal event of 2008. In green are fractures detected in 2002. The
base map is Carta Tecnica Regionale 2008 (CTR). The reference system is WGS
84/UTM zone 33N.</p></caption>
        <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/21/2881/2021/nhess-21-2881-2021-f02.png"/>

      </fig>

      <p id="d1e184"><?xmltex \hack{\newpage}?>The mud volcano of Santa Barbara is located within the Caltanissetta
foredeep basin of the Apennines–Maghrebian collisional chain which developed
from the late Miocene to the Quaternary along the border of the converging
Eurasia–Nubia plate (Catalano et al., 2008; Dewey et al., 1989; Serpelloni
et al., 2007). This structural domain is formed by a foreland fold and
thrust belt involving the deposition of clastic sediments which were
gradually deformed from the late Miocene to the Pleistocene (Monaco and
Tortorici, 1996; Lickorish et al., 1999, and references therein).</p>
      <?pagebreak page2883?><p id="d1e188"><?xmltex \hack{\newpage}?>According to Madonia et al. (2011) mud volcanoes are most of the time in
stasis, but they represent a preferential way for rising fluids rich in
methane and sludge; therefore they can be considered a risk to urbanized
areas or sites with an economy dedicated to natural attractions.</p>
      <p id="d1e192">At several mud volcanoes (e.g., Ayaz-Akhtarma and Khara Zira island mud
volcanoes in Azerbaijan), certain geomorphic and/or structural features have been
observed within the year preceding a paroxysmal event (Antonielli  et al.,
2014; Madonia et al., 2011). The area of the Santa Barbara volcano was also
affected in 2008 by a paroxysmal mud eruption which was preceded by
deformation features (Fig. 2). Moreover, the surface of the mud volcanic cone
is incised by a drainage system (Fig. 1) characterized by hydrographic basins
with elongated dendritic geometry arranged for a centrifugal development from
the areas of the summit craters towards the lower slopes of the volcano
complex. The higher order of the thalwegs presents deep recessed meanders
(landscape rejuvenation process). This morphometric structure is typical of
uplifting areas and therefore relative decrease in the base level. This
suggests an inflection process of the volcano ground surface induced by an
increase in fluid pressure inside of a shallower stagnation chamber which is
located at a depth of about 30 m (Imposa et al., 2018). The stagnation
chamber has a “sill-like” geometry, a radius of about 50 m and a thickness
of about 30 m. This morphostructural configuration supported by geophysical
data configures the active geological structure as a high potential
geological hazard.</p>
      <p id="d1e195">On the surface, fractures and shear lineaments extend outside the erupted
mud area (Madonia et al., 2011; Bonini et al., 2012; INGV, 2008; Regione
Siciliana, 2008), and they highlight the high stress and strain environment
induced by the mud volcano (Fig. 2). Such structures have been detected in
2002 and 2008, and we speculate that they are still active (Fig. 2). This
development has often been a precursor of paroxysmal events such as the 11 August 2008 event (INGV, 2008; Regione Siciliana, 2008).</p>
</sec>
<sec id="Ch1.S2">
  <label>2</label><title>Methods</title>
<sec id="Ch1.S2.SS1">
  <label>2.1</label><title>Local network</title>
      <p id="d1e213">In order to monitor active deformation in the mud volcano area, a local global navigation satellite system (GNSS)
network was created according to the criteria described by De Guidi et al. (2017), in particular ensuring (i) the basic requirement of spatial and
temporal stability, (ii) absence of possible gravitational instabilities in
both static and dynamic conditions at sites, and (iii) a panoramic and
elevated position for the theodolite total station (TST).</p>
      <p id="d1e216">According to these criteria two GNSS benchmarks were created, CTN0 and CTN1,
located on the roof of a building in the northern sector of the studied area
(Fig. 3).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3"><?xmltex \currentcnt{3}?><?xmltex \def\figurename{Figure}?><label>Figure 3</label><caption><p id="d1e221">Chorography of the eastern periphery of the inhabited area of
Caltanissetta (Santa Barbara Village). The base map is Carta Tecnica
Regionale 2008 (CTR). The reference system is WGS 84/UTM zone 33N.</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/21/2881/2021/nhess-21-2881-2021-f03.png"/>

        </fig>

      <p id="d1e231"><?xmltex \hack{\newpage}?>The benchmarks were surveyed using double frequency (L1/L2) receivers
(Topcon HiPer V and HiPer SR) in static mode. Once the stability of the
benchmarks has been assessed, we surveyed CTN0 and CTN1 five and two times,
respectively.</p>
      <p id="d1e235">Post-processing of GNSS data was carried out by AUSPOS online service
(Geoscience Australia, 2011; Jia  et al., 2014).</p>
      <p id="d1e238">To process the CTN0 data of the 28 February 2018 survey, AUSPOS used 15 International GNSS Service (IGS) stations
to compute the baselines – ANKR, BOR1, BRUX, BUCU, GANP, GRAS, GRAZ, LROC,
MAT1, MEDI, SOFI, TLSE, VILL, YEBE and ZIM2 – with an average ambiguity
resolution of 90.0 %; position uncertainties (95 % C.L., confidence level) are respectively
0.005, 0.005 and 0.016 m for east, north and ellipsoidal height.</p>
      <p id="d1e241">To process the CTN1 data of the 26 November 2018  survey, AUSPOS used 15 IGS stations
to compute the baselines – ANKR, BOR1, BRUX, BUCU, GANP, GRAS, GRAZ, LROC,
MAT1, MEDI, SOFI, TLSE, VILL, YEBE and ZIM2 – with an average ambiguity
resolution of 84.5 %; position uncertainties (95 % C.L.) are respectively 0.007, 0.007 and 0.024 m for east, north and ellipsoidal height.</p>
      <p id="d1e244">Finally, the optimal ITRF2014-UTM33N coordinates have been definitively
assigned to CTN0 and CTN1.</p>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T1" specific-use="star"><?xmltex \currentcnt{1}?><label>Table 1</label><caption><p id="d1e251">Average RMSE of GCPs obtained for each survey and for each
technique used to determinate the GCPs coordinates: <inline-formula><mml:math id="M2" display="inline"><mml:mi>X</mml:mi></mml:math></inline-formula> (easting), <inline-formula><mml:math id="M3" display="inline"><mml:mi>Y</mml:mi></mml:math></inline-formula>
(northing), <inline-formula><mml:math id="M4" display="inline"><mml:mi>Z</mml:mi></mml:math></inline-formula> (altitude) and the total error. The image residual (“Img error” in the table) is shown.</p></caption><oasis:table frame="topbot"><?xmltex \begin{scaleboxenv}{.95}[.95]?><oasis:tgroup cols="8">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="left"/>
     <oasis:colspec colnum="3" colname="col3" align="right"/>
     <oasis:colspec colnum="4" colname="col4" align="right"/>
     <oasis:colspec colnum="5" colname="col5" align="right"/>
     <oasis:colspec colnum="6" colname="col6" align="right"/>
     <oasis:colspec colnum="7" colname="col7" align="right"/>
     <oasis:colspec colnum="8" colname="col8" align="right"/>
     <oasis:thead>
       <oasis:row>
         <oasis:entry colname="col1">Date</oasis:entry>
         <oasis:entry colname="col2">Method of</oasis:entry>
         <oasis:entry colname="col3">GCP</oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M5" display="inline"><mml:mi>X</mml:mi></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M6" display="inline"><mml:mi>Y</mml:mi></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col6"><inline-formula><mml:math id="M7" display="inline"><mml:mi>Z</mml:mi></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col7">Total</oasis:entry>
         <oasis:entry colname="col8">Img</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">(yyyy/mm/dd)</oasis:entry>
         <oasis:entry colname="col2">survey</oasis:entry>
         <oasis:entry colname="col3">number</oasis:entry>
         <oasis:entry colname="col4">error (CM)</oasis:entry>
         <oasis:entry colname="col5">error (CM)</oasis:entry>
         <oasis:entry colname="col6">error (CM)</oasis:entry>
         <oasis:entry colname="col7">error (CM)</oasis:entry>
         <oasis:entry colname="col8">error (PIX)</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>
         <oasis:entry colname="col1">2018/02/28</oasis:entry>
         <oasis:entry colname="col2">Static ultra rapid</oasis:entry>
         <oasis:entry colname="col3">6</oasis:entry>
         <oasis:entry colname="col4">12.06</oasis:entry>
         <oasis:entry colname="col5">8.85</oasis:entry>
         <oasis:entry colname="col6">10.02</oasis:entry>
         <oasis:entry colname="col7">18.01</oasis:entry>
         <oasis:entry colname="col8">0.587</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">2018/04/16</oasis:entry>
         <oasis:entry colname="col2">RTK</oasis:entry>
         <oasis:entry colname="col3">6</oasis:entry>
         <oasis:entry colname="col4">2.18</oasis:entry>
         <oasis:entry colname="col5">1.79</oasis:entry>
         <oasis:entry colname="col6">3.34</oasis:entry>
         <oasis:entry colname="col7">4.29</oasis:entry>
         <oasis:entry colname="col8">0.326</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">2018/04/16</oasis:entry>
         <oasis:entry colname="col2">TST</oasis:entry>
         <oasis:entry colname="col3">6</oasis:entry>
         <oasis:entry colname="col4">2.04</oasis:entry>
         <oasis:entry colname="col5">1.39</oasis:entry>
         <oasis:entry colname="col6">1.68</oasis:entry>
         <oasis:entry colname="col7">2.99</oasis:entry>
         <oasis:entry colname="col8">0.325</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">2019/07/29</oasis:entry>
         <oasis:entry colname="col2">TST</oasis:entry>
         <oasis:entry colname="col3">29</oasis:entry>
         <oasis:entry colname="col4">0.78</oasis:entry>
         <oasis:entry colname="col5">0.95</oasis:entry>
         <oasis:entry colname="col6">0.72</oasis:entry>
         <oasis:entry colname="col7">1.43</oasis:entry>
         <oasis:entry colname="col8">0.244</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">2019/09/13</oasis:entry>
         <oasis:entry colname="col2">TST</oasis:entry>
         <oasis:entry colname="col3">30</oasis:entry>
         <oasis:entry colname="col4">0.79</oasis:entry>
         <oasis:entry colname="col5">0.84</oasis:entry>
         <oasis:entry colname="col6">0.86</oasis:entry>
         <oasis:entry colname="col7">1.45</oasis:entry>
         <oasis:entry colname="col8">0.316</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">2019/10/14</oasis:entry>
         <oasis:entry colname="col2">TST</oasis:entry>
         <oasis:entry colname="col3">31</oasis:entry>
         <oasis:entry colname="col4">0.78</oasis:entry>
         <oasis:entry colname="col5">0.66</oasis:entry>
         <oasis:entry colname="col6">0.78</oasis:entry>
         <oasis:entry colname="col7">1.29</oasis:entry>
         <oasis:entry colname="col8">0.311</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">2020/01/13</oasis:entry>
         <oasis:entry colname="col2">TST</oasis:entry>
         <oasis:entry colname="col3">31</oasis:entry>
         <oasis:entry colname="col4">0.95</oasis:entry>
         <oasis:entry colname="col5">0.82</oasis:entry>
         <oasis:entry colname="col6">0.77</oasis:entry>
         <oasis:entry colname="col7">1.48</oasis:entry>
         <oasis:entry colname="col8">0.237</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">2020/06/15</oasis:entry>
         <oasis:entry colname="col2">TST</oasis:entry>
         <oasis:entry colname="col3">26</oasis:entry>
         <oasis:entry colname="col4">0.43</oasis:entry>
         <oasis:entry colname="col5">0.39</oasis:entry>
         <oasis:entry colname="col6">0.45</oasis:entry>
         <oasis:entry colname="col7">0.73</oasis:entry>
         <oasis:entry colname="col8">0.249</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup><?xmltex \end{scaleboxenv}?></oasis:table></table-wrap>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4" specific-use="star"><?xmltex \currentcnt{4}?><?xmltex \def\figurename{Figure}?><label>Figure 4</label><caption><p id="d1e601">GCPs locations and error estimates. <inline-formula><mml:math id="M8" display="inline"><mml:mi>Z</mml:mi></mml:math></inline-formula> error is represented by the
color of the ellipse. <inline-formula><mml:math id="M9" display="inline"><mml:mi>X</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M10" display="inline"><mml:mi>Y</mml:mi></mml:math></inline-formula> errors are represented by ellipse shape. GCP
locations are marked with a dot. Note that the different scale of the error
ellipse in green: in the left image the ellipse in <inline-formula><mml:math id="M11" display="inline"><mml:mi>X</mml:mi></mml:math></inline-formula> direction is enlarged
60 times, and in the right image it is enlarged 500 times. The reference system
is WGS 84/UTM zone 33N.</p></caption>
          <?xmltex \igopts{width=426.791339pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/21/2881/2021/nhess-21-2881-2021-f04.png"/>

        </fig>

<?xmltex \hack{\newpage}?>
</sec>
<?pagebreak page2884?><sec id="Ch1.S2.SS2">
  <label>2.2</label><title>Ground control points (GCPs)</title>
      <p id="d1e648">Various acquisition methods of ground control points (GCPs) were tested in
order to define the most suitable one. The main function of GCPs is to
georeference outcomes from SfM.</p>
      <p id="d1e651">Initially (2016–2018) we used only GNSS receivers in different
configurations: real-time kinematics (RTK) and static ultra rapid. The GCPs
were made of 50 cm <inline-formula><mml:math id="M12" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 50 cm alveolar polypropylene square targets. Using
these configurations (Table 1), errors ranging from centimeters to decimeters
were recorded. In these early phases, errors were only computed by the SfM
software PhotoScan (v 1.4.5.7554).</p>
      <p id="d1e661">PhotoScan provides different types of error estimation: <inline-formula><mml:math id="M13" display="inline"><mml:mrow><mml:mi>X</mml:mi><mml:mi>Y</mml:mi></mml:mrow></mml:math></inline-formula> error (m) – root
mean square error for horizontal coordinates for a GCP location; <inline-formula><mml:math id="M14" display="inline"><mml:mi>Z</mml:mi></mml:math></inline-formula> error (m)
– error for elevation coordinate for a GCP location; error <inline-formula><mml:math id="M15" display="inline"><mml:mi>X</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math id="M16" display="inline"><mml:mi>Y</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M17" display="inline"><mml:mi>Z</mml:mi></mml:math></inline-formula> (m) –
root mean square error for <inline-formula><mml:math id="M18" display="inline"><mml:mi>X</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math id="M19" display="inline"><mml:mi>Y</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M20" display="inline"><mml:mi>Z</mml:mi></mml:math></inline-formula> coordinates for a GCP location; error img
(pix) – root mean square error for <inline-formula><mml:math id="M21" display="inline"><mml:mi>X</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M22" display="inline"><mml:mi>Y</mml:mi></mml:math></inline-formula> coordinates on an image for a GCP
location averaged over all the images; and total error (m) – implies averaging
over all the GCP locations.</p>
      <p id="d1e738">Using static ultra rapid mode, the total error was about 18 cm, whereas
using the RTK configuration the total error was reduced to approximately 4 cm  (Brighenti et al., 2018).</p>
      <p id="d1e742">From 2018 the use of the Topcon DS-103 TST was introduced, obtaining lower
values for the GCP errors than those measured with the GNSS technique
(Table 1). With this measurement technique the total error has been reduced to
about 3 cm. On the first three campaigns, we used six GCPs to georeference the
cloud points (Fig. 4). In the following section, these first three campaigns will not
be considered in the computation of the significant changes for their
incomparability with the last campaigns. Since 2019, we preferred to use<?pagebreak page2885?> only the
TST for the GCP survey, and, according to Tahar et al. (2013), the number of
GCPs has been increased (Table 1). Considering these two improvements, the
total error has been reduced to about 1.4 cm and in the last campaign about
0.7 cm.</p>
      <p id="d1e745">In the last two campaigns we used the TST to obtain
the coordinates of the GCPs. The TST was positioned on the CTN0 point of the
local network (Fig. 3) which coincides with the roof of the nearby private
houses in the northern part (Fig. 5a). A classic celerimetric survey was
carried out.</p>
      <p id="d1e748">The measurements of the GCPs were carried out with a surveying ranging rod
equipped with a reflecting prism (offset of <inline-formula><mml:math id="M23" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">30</mml:mn></mml:mrow></mml:math></inline-formula> mm) assisted by a tripod
with a spirit level (Fig. 5b) to ensure the upright and stability of the
measurement.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F5"><?xmltex \currentcnt{5}?><?xmltex \def\figurename{Figure}?><label>Figure 5</label><caption><p id="d1e763"><bold>(a)</bold> TST DS 103 placed on the fixed metal base in coincidence with
point CTN0. <bold>(b)</bold> Surveying ranging rod on the mud volcano during the survey
phase.</p></caption>
          <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/21/2881/2021/nhess-21-2881-2021-f05.jpg"/>

        </fig>

      <p id="d1e777">We assumed a “marker accuracy” on PhotoScan of 5 mm due to the
instrumental error. This value has been assumed due to the uncertainty of
the CTN0 and CTN1 point coordinates, obtained through GNSS measurements,
considering that the uncertainty derived from the TST is negligible.</p>
      <p id="d1e781">To validate GCP data we performed an analysis using the python script
“Monte_Carlo_BA.py”, with a statistical
iterative approach (Monte Carlo approach) (James et al., 2017a). For
clarity, the following terminology will be used in the text:
<list list-type="bullet"><list-item>
      <p id="d1e786">GCPs are the points measured in the field. They can be used as control points or check points within the bundle adjustment (James et al., 2017a).</p></list-item><list-item>
      <p id="d1e790">Control points are GCPs when they are tied to the model in the bundle
adjustment.</p></list-item><list-item>
      <p id="d1e794">Check points are GCPs when they are not tied to the model in the bundle adjustment.</p></list-item></list></p>
      <p id="d1e797">This script modifies the percentage of GCPs which are used as check points
or control points and applies to the check points random variations (James
et al., 2017a). To be more precise values ranging from 10 % up to 80 %
of GCPs have been set.</p>
</sec>
<sec id="Ch1.S2.SS3">
  <label>2.3</label><title>Photo acquisition</title>
      <p id="d1e808">We have performed five measurement campaigns in approximately 1 year. The
same flight plan was used for all five of them. The AOI (area of interest)
was captured by a DJI Phantom 4 Standard, a quadcopter UAV, at a flight
height of 33 m above the ground. The sensor size of the UAV's digital camera
is 6.17 mm by 4.55 mm, capable of shooting images with a resolution of 12 MP
(4000 <inline-formula><mml:math id="M24" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 3000 pixels) with a mechanical shutter. Each flight
planning was carried out with the Pix4D Mapper software, adopting a frontal
and side overlapping of 80 % and 70 %, respectively. The camera was
set up in a nadir orientation to capture vertical imagery. The flight was
carried out in a single grid (simple geometric flight patterns without
intersections). An average of 280 images for each survey were acquired with
about 1.1 cm ground sampling distance (GSD).</p>
</sec>
<sec id="Ch1.S2.SS4">
  <label>2.4</label><title>Data processing through structure from motion (SfM) techniques</title>
      <p id="d1e826">The photogrammetric processing was performed using the commercial software
Agisoft PhotoScan. The photogrammetric processing is based on the workflow
formulated by the USGS (2017). Steps of the processing chain regarding tie
point accuracy and marker accuracy have been performed according to James (2017a) (Fig. 6).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F6" specific-use="star"><?xmltex \currentcnt{6}?><?xmltex \def\figurename{Figure}?><label>Figure 6</label><caption><p id="d1e831">Simplified block diagram of the photogrammetric processing chain.</p></caption>
          <?xmltex \igopts{width=398.338583pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/21/2881/2021/nhess-21-2881-2021-f06.png"/>

        </fig>

      <p id="d1e840">The procedure above is conventional, but we modified some parameters during
the cleaning procedure of the sparse point cloud. We adopted the optimal
values defined on the workflow (Fig. 6) of “reconstruction uncertain” and
“projection accuracy” in the “gradual selection” option in PhotoScan. The
“reconstruction uncertain” improves the geometric reconstruction of the
cloud point. The “projection accuracy” improves pixel mismatches in
images.</p>
      <p id="d1e844">Thus, the obtained cleaned sparse cloud point was tied to the GCPs in order
to georeference it.</p>
      <p id="d1e847">We perform the “gradual selection” option, adjusting the “reprojection
error” values to reduce the residual pixel errors (Fig. 6) (USGS, 2017).</p>
      <p id="d1e850">Furthermore, appropriate pixel values of tie point accuracy and marker
accuracy are set following the suggestions of James et al. (2017b).</p>
      <p id="d1e853">We applied the “precision_estimate.py” script (James  et
al., 2017b). The script operates by an interactive Monte Carlo approach to
estimate the accuracy of SfM surveys through photogrammetric and
georeferencing parameters, which are then used to provide spatially variable
confidence limits for the detection of surface variations.</p>
      <p id="d1e856">The precision estimates are calculated through multiple “bundle adjustments”
(“optimize camera alignment” in<?pagebreak page2886?> PhotoScan) with different pseudo-random
offsets (in this case 4000 pseudo-random offsets) (Fig. 7) applied to each
image and checkpoint. The pseudo-random offsets are derived from normal
distributions with standard deviations representative of the appropriate
accuracy within the survey (James et al., 2017b).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F7"><?xmltex \currentcnt{7}?><?xmltex \def\figurename{Figure}?><label>Figure 7</label><caption><p id="d1e862">Example of the iterative approach in the 29 July 2020 survey.
Estimates of uncertainties on <inline-formula><mml:math id="M25" display="inline"><mml:mi>X</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math id="M26" display="inline"><mml:mi>Y</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M27" display="inline"><mml:mi>Z</mml:mi></mml:math></inline-formula> improve as the number of iterations
increase.</p></caption>
          <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/21/2881/2021/nhess-21-2881-2021-f07.png"/>

        </fig>

      <p id="d1e892">The SfM-Georef software (James and Robson, 2012) reads the output given by
the Monte Carlo python script, setting to each point of the sparse cloud
different values of precision on the three spatial components. The results
of the script, read by SfM-Georef, are estimates of the error of the
individual points of the sparse cloud point in the three different spatial
dimensions (Fig. 8).</p>

      <?xmltex \floatpos{p}?><fig id="Ch1.F8" specific-use="star"><?xmltex \currentcnt{8}?><?xmltex \def\figurename{Figure}?><label>Figure 8</label><caption><p id="d1e897">3D error estimates of each point of the sparse cloud of the 13 September 2019  survey. The error (sX, sY, sZ) is in millimeters. <bold>(a)</bold> and <bold>(b)</bold> The horizontal
errors (<inline-formula><mml:math id="M28" display="inline"><mml:mi>X</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M29" display="inline"><mml:mi>Y</mml:mi></mml:math></inline-formula> component) are shown. <bold>(c)</bold> The vertical errors (<inline-formula><mml:math id="M30" display="inline"><mml:mi>Z</mml:mi></mml:math></inline-formula> component)
are shown. The reference system is WGS 84/UTM zone 33N.</p></caption>
          <?xmltex \igopts{width=426.791339pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/21/2881/2021/nhess-21-2881-2021-f08.png"/>

        </fig>

      <?xmltex \floatpos{p}?><fig id="Ch1.F9" specific-use="star"><?xmltex \currentcnt{9}?><?xmltex \def\figurename{Figure}?><label>Figure 9</label><caption><p id="d1e939">Estimates of the 3D error of the dense point cloud obtained by
interpolation with the sparse cloud of the 13 September 2019 survey. The error (sX,
sY, sZ) is in millimeters. <bold>(a)</bold> and <bold>(b)</bold> The horizontal errors (<inline-formula><mml:math id="M31" display="inline"><mml:mi>X</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M32" display="inline"><mml:mi>Y</mml:mi></mml:math></inline-formula> component) are
shown. <bold>(c)</bold> The vertical errors (<inline-formula><mml:math id="M33" display="inline"><mml:mi>Z</mml:mi></mml:math></inline-formula> component) are shown. The reference system
is WGS 84/UTM zone 33N.</p></caption>
          <?xmltex \igopts{width=426.791339pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/21/2881/2021/nhess-21-2881-2021-f09.png"/>

        </fig>

      <?xmltex \floatpos{p}?><fig id="Ch1.F10" specific-use="star"><?xmltex \currentcnt{10}?><?xmltex \def\figurename{Figure}?><label>Figure 10</label><caption><p id="d1e982">Point clouds resulting from M3C2-PM processing – comparison
between 29 July 2019 and 15 June 2020: <bold>(a)</bold> significant changes between the two
point clouds with LOD<inline-formula><mml:math id="M34" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mi mathvariant="italic">%</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mn mathvariant="normal">95</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula>, <bold>(b)</bold> distances between the two point clouds and
<bold>(c)</bold> uncertainty of the distance between the two point clouds. The reference
system is WGS 84/UTM zone 33N.</p></caption>
          <?xmltex \igopts{width=426.791339pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/21/2881/2021/nhess-21-2881-2021-f10.png"/>

        </fig>

      <p id="d1e1013">The 3D topographic change is usually detected from sparse point clouds that
have been cleaned to exclude the vegetation that interferes with the
comparison techniques. The next step is to link those points to the
precision estimates of the sparse cloud; this has been done in CloudCompare
v. 2.11 (<uri>http://www.cloudcompare.org/</uri>, last access: 15 October 2019).</p>
      <p id="d1e1019">Through CloudCompare the sparse cloud is interpolated (with the relative
precision values on the 3D components) with the dense point
cloud. In this phase we decide which<?pagebreak page2887?> interpolation technique is the most
suitable; in this case we chose the “nearest neighbors” that are the
three closest points to the sparse cloud, using the median value (better
outlier mitigation) to assign the error values to the dense point clouds
(Fig. 9). This methodology has been chosen due to the heterogeneous
distribution of the points in the sparse cloud, avoiding points with null
values.</p>
      <p id="d1e1022">Once the precise dense point cloud and their error have been obtained, it is
possible to compare the surveys in order to determine the changes between
them. Comparisons between the surveys were performed on CloudCompare by the
M3C2-PM plugin (James et al., 2017b; Lague et al., 2013) that identifies a
statistically significant change where the topographical differences exceed
a value of spatially variable uncertainty. According to James et al. (2017b), the M3C2-PM is particularly suited for point clouds derived from SfM. The M3C2-PM (James et al., 2017b) uses estimates of the precision of the coordinates of points (3D precision map) that we have previously calculated.</p>
      <p id="d1e1025">The outputs of M3C2-PM are scalar values applied to the cloud:
<list list-type="bullet"><list-item>
      <p id="d1e1030">significant change (Fig. 10a)</p></list-item><list-item>
      <p id="d1e1034">M3C2 distance (Fig. 10b)</p></list-item><list-item>
      <p id="d1e1038">distance uncertainty (Fig. 10c).</p></list-item></list></p>
      <p id="d1e1041"><?xmltex \hack{\newpage}?>The first output (Fig. 10a) shows the changes which exceed the uncertainty
values in both point clouds. It represents a confidence interval constrained
by values with a level of detection at 95 % confidence (LoD<inline-formula><mml:math id="M35" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">95</mml:mn><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="italic">%</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula>) which are
spatially variable. This is applicable in any morphological setting,
providing a reliable 3D analysis of topographical change.</p>
      <p id="d1e1059">The second output (Fig. 10b) shows the calculated distances between the two
clouds.</p>
      <p id="d1e1062">The third output (Fig. 10c) shows the uncertainty values of the distances and
their spatial variation between the two clouds. Once the uncertainty value
is defined, the changes are significant when they overtake the value of the
uncertainty.</p>
      <p id="d1e1065">In the 15 June 2020 survey, we used callipers to test and validate the method
of the measurements. Five numbered callipers, with steps of increasing
height of about 2 cm, were positioned on the mud dome. The heights are 2, 4,
6, 8 and 10 cm.</p>
      <p id="d1e1068">These were used to obtain an instrumental sensitivity of the measures
(Fig. 11). All callipers are detected, and we show as an example the smallest
(Fig. 11).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F11" specific-use="star"><?xmltex \currentcnt{11}?><?xmltex \def\figurename{Figure}?><label>Figure 11</label><caption><p id="d1e1073">In the upper part of the figure, the dense point clouds of the two
surveys of the same area carried out on 29 July 2019 (left) and 15 June 2020
(right) are shown. In the lower part are the clouds with the significant change
(left) and the M3C2 distance (right). The arrows indicate the significant
changes between the surveys. The calculated changes between the two clouds
estimate an altitude increase of about 6.3 cm for the fragment of rock used
to maintain the target in position and an increase in height of about 2.5 cm
for the calliper which is 2 cm thick. The reference system is WGS 84/UTM
zone 33N.</p></caption>
          <?xmltex \igopts{width=426.791339pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/21/2881/2021/nhess-21-2881-2021-f11.png"/>

        </fig>

</sec>
</sec>
<sec id="Ch1.S3">
  <label>3</label><title>Results</title>
      <p id="d1e1091">As illustrated in Sect. 2.2, the results show that using between 40 % and 60 % of the GCPs (as control points) the RMSE value has minimal variation.
Thus, the optimal minimum number of GPCs is between 12 and 18. When the
threshold of 60 % is exceeded, there are no significant improvements
(Fig. 12). This result has been confirmed in all campaigns.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F12" specific-use="star"><?xmltex \currentcnt{12}?><?xmltex \def\figurename{Figure}?><label>Figure 12</label><caption><p id="d1e1096">The boxes represent the distribution of the RMSE of GCPs
(13 September 2019 survey) on the three components: magnitude (3D), horizontal and
vertical according to the percentage of the GCPs used as control points. RMSE is
calculated on 50 self-calibrating bundle adjustments for each percentage of GCPs
used as control points. The GCPs are randomly selected for each
self-calibrating bundle adjustment. The central bars indicate the median
RMSE values, which are included in the boxes that extend from the 25th to 75th
percentile, and the outliers are indicated by the <inline-formula><mml:math id="M36" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> symbols.</p></caption>
        <?xmltex \igopts{width=398.338583pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/21/2881/2021/nhess-21-2881-2021-f12.png"/>

      </fig>

      <p id="d1e1112">The results obtained from the photogrammetric comparisons supported by
geodetic topographic survey have an average uncertainty of about 6.4 cm,
with a minimum of about 2 cm and a maximum of about 12 cm, relative to an
area of 42 700 m<inline-formula><mml:math id="M37" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula> (Fig. 13a). The uncertainty of the central
area has an average value of about 3.9 cm, with a minimum of about 2 cm and
maximum of 10 cm, on an extension of 360 m<inline-formula><mml:math id="M38" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula> (Fig. 13b).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F13" specific-use="star"><?xmltex \currentcnt{13}?><?xmltex \def\figurename{Figure}?><label>Figure 13</label><caption><p id="d1e1136">Point clouds with uncertainty distance values between 29 July 2019
and 15 June 2020 (right). On the left, <bold>(a)</bold> the Gaussian distribution of the
distance uncertainty over the whole area is shown; the mean is about 6.4 cm,
and the standard deviation is about 2.5 cm.  <bold>(b)</bold> The Gaussian distribution of
the distance uncertainty of the central emission area is shown; the mean is
about 3.9 cm, and the standard deviation is about 1.4 cm. The reference
system is WGS 84/UTM zone 33N.</p></caption>
        <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/21/2881/2021/nhess-21-2881-2021-f13.png"/>

      </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F14" specific-use="star"><?xmltex \currentcnt{14}?><?xmltex \def\figurename{Figure}?><label>Figure 14</label><caption><p id="d1e1153">Enlargement of the comparison between the point clouds of the
13 September 2019 and 14 October 2019 campaigns with significant changes. Two significant
changes (<bold>a</bold> and <bold>b</bold>) are shown, which highlight an anthropogenic action, i.e.,
the movement of a wooden platform about 15 cm high. (<bold>a</bold>, upper part) A lowering of an average height of 16 cm is detected, and the Gaussian
distribution of the M3C2-PM distances with the mean and the standard
deviation is shown. (<bold>a</bold>, lower part) The distance uncertainty varies spatially
with an average value of about 5 cm, and the Gaussian distribution of the
M3C2-PM distances with the mean and the standard deviation is shown. (<bold>b</bold>,
upper part) An increase in height of 14 cm is recorded, and the Gaussian
distribution of the M3C2-PM distances with the mean and the standard
deviation is shown. (<bold>b</bold>, lower part) The distance uncertainty has an average
value of about 3 cm, and the Gaussian distribution of the M3C2-PM distances with
the mean and the standard deviation is shown. The reference system is WGS
84/UTM zone 33N.</p></caption>
        <?xmltex \igopts{width=369.885827pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/21/2881/2021/nhess-21-2881-2021-f14.png"/>

      </fig>

      <p id="d1e1181">During the monitoring period, in addition to natural changes, we recorded
anthropogenic action due to the relocation of objects (garbage) in the area
after unauthorized access. These changes have a decimetric order of
magnitude and are easily detected by the technique used (Fig. 14).</p>
      <p id="d1e1184">Two types of analysis were carried out: semi-quantitative and quantitative.
The surveys on 29 July 2019 and 15 June 2020 (time interval of about 1 year) were
chosen to perform the semi-quantitative analysis. This analysis was carried
out on the whole mud volcano area, and the objective is to detect significant
deformations (on the order of decimeters). In order to visualize this
deformation (Fig. 15), the values of M3C2 distance ranging between <inline-formula><mml:math id="M39" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> and 2 cm
were excluded according to the minimum value of distance uncertainty. This
range was verified instrumentally with the use of callipers.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F15"><?xmltex \currentcnt{15}?><?xmltex \def\figurename{Figure}?><label>Figure 15</label><caption><p id="d1e1199">Orthophoto with M3C2 distance. The distance scale has been
adjusted to exclude values between <inline-formula><mml:math id="M40" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>2 and <inline-formula><mml:math id="M41" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>2 cm. The positive distances,
observed at the margin of the mud dome, are interpreted as mud flow or
sediment deposition coming from peripheral griffon vent eruptions or
erosion of summit area. The reference system is WGS 84/UTM zone 33N.</p></caption>
        <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/21/2881/2021/nhess-21-2881-2021-f15.png"/>

      </fig>

      <?pagebreak page2889?><p id="d1e1223"><?xmltex \hack{\newpage}?>Comparing the 29 July 2019 and 15 June 2020 surveys (Fig. 15), we observe that
the surface of the volcanic cone is not affected by deformations. Only
morphological changes in the volcanic structures can be underlined, such as
small eruptive cones, gryphons, sauces and mud pools.</p>
      <p id="d1e1227">The quantitative analysis was performed on small central portions of the mud
volcano. The aim of the quantitative analysis is to estimate the trend and
evolution of the deformation. To assess the deformation and the local
morphostructural evolution, two temporal series have been developed in two
areas: <inline-formula><mml:math id="M42" display="inline"><mml:mrow><mml:mi>Z</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> (collapse zone) and <inline-formula><mml:math id="M43" display="inline"><mml:mrow><mml:mi>Z</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> (uplifting zone) (Figs. 16 and 17). The
zones were chosen in relation to the significant change. For the selected zone,
the average distances between points with significant change were computed
by M3C2-PM. <inline-formula><mml:math id="M44" display="inline"><mml:mrow><mml:mi>Z</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> has an extension of 1 m<inline-formula><mml:math id="M45" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula> (Fig. 16), and <inline-formula><mml:math id="M46" display="inline"><mml:mrow><mml:mi>Z</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> has
an extension of 0.84 m<inline-formula><mml:math id="M47" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula> (Fig. 17).</p>
      <?pagebreak page2891?><p id="d1e1289"><?xmltex \hack{\newpage}?>The campaign of 29 July 2019 (<inline-formula><mml:math id="M48" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>) was chosen as the master (Table 2).</p>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T2"><?xmltex \currentcnt{2}?><label>Table 2</label><caption><p id="d1e1307">Surveys used to generate the time series. Dates are given in yyyy/mm/dd.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="2">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="left"/>
     <oasis:tbody>
       <oasis:row>
         <oasis:entry colname="col1"><inline-formula><mml:math id="M49" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col2">2019/07/29</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"><inline-formula><mml:math id="M50" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col2">2019/09/13</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"><inline-formula><mml:math id="M51" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col2">2019/10/14</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"><inline-formula><mml:math id="M52" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col2">2020/01/13</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"><inline-formula><mml:math id="M53" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col2">2020/06/15</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table></table-wrap>

      <?xmltex \floatpos{t}?><fig id="Ch1.F16" specific-use="star"><?xmltex \currentcnt{16}?><?xmltex \def\figurename{Figure}?><label>Figure 16</label><caption><p id="d1e1414"><bold>(a)</bold> M3C2 distance (29 July 2019 vs. 15 June 2020) of <inline-formula><mml:math id="M54" display="inline"><mml:mrow><mml:mi>Z</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula>; the area used
to create the time series is delimited with a dashed line (selected by
significant change). <bold>(a')</bold> Orthophoto of 29 July 2019 with the gryphon border
in red. <bold>(b)</bold> The orthophoto of 13 September 2019 highlights the expansion of the
gryphon border in blue. <bold>(c)</bold> Orthophotos of 15 June 2020 showing the gryphon during the
quiescence phase and the split of the channel in yellow. Below, the time
series with a decreasing trend is shown. The reference system is WGS 84/UTM zone 33N.</p></caption>
        <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/21/2881/2021/nhess-21-2881-2021-f16.png"/>

      </fig>

      <p id="d1e1445">In Fig. 16, the subsidence (about 10 cm per 60 d) of gryphon is
represented by the southwest migration of the mud pool edge. In Fig. 17,
the uplift (about 4 cm per 60 d) of a blind gryphon is represented by the
development of radial fractures on the cone surface. Close to the growing
gryphon, another indication of deformation is the deviation of a mudslide
flowing in the north–south direction towards the southern sector of the analyzed
area. Finally, the sudden appearance of the gryphon is well highlighted in
the orthophoto of the last survey (Fig. 17).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F17" specific-use="star"><?xmltex \currentcnt{17}?><?xmltex \def\figurename{Figure}?><label>Figure 17</label><caption><p id="d1e1450"><bold>(a)</bold> M3C2 distance (29 July 2019 vs. 15 June 2020) of the <inline-formula><mml:math id="M55" display="inline"><mml:mrow><mml:mi>Z</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula>; the area
used to create the time series is delimited with a dashed line (selected by
significant change). <bold>(a')</bold> Orthophoto of 29 July 2019, the margin of the
deflected flow in green and the radial fractures in red. <bold>(b)</bold> Orthophoto
of 14 October 2019, formation of a new emission gryphon in red and the previous
flow in green. <bold>(c)</bold> Orthophoto of 15 June 2020, formation of a new emission
gryphon in red. Below, the time series with upward trend is shown. The
reference system is WGS 84/UTM zone 33N.</p></caption>
        <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/21/2881/2021/nhess-21-2881-2021-f17.png"/>

      </fig>

<?xmltex \hack{\newpage}?>
</sec>
<sec id="Ch1.S4">
  <label>4</label><title>Discussion</title>
      <p id="d1e1490">UAV technology combined with SfM is a valuable tool in geological risk
assessment and monitoring; however, some issues must be considered.</p>
      <p id="d1e1493">The first is the quantity and quality of the acquired GCPs. According to the
results, the minimum optimal number for georeferencing is 12 GCPs. A slight
improvement is observable up to 18 GCPs, while no appraisable improvement is
detected for a higher number of GCPs (Fig. 12). In addition, the method of
acquiring GCPs reduces their error by using the total station theodolite
(Table 1). The combined use of high-precision topographic instruments with an
optimal number of GCPs improves the reliability of the datasets.</p>
      <p id="d1e1496">The second aspect to be considered is the evaluation of distance uncertainty
when two surveys are compared. The distance uncertainty between two datasets (surveys) can be considered as an estimate of the sensitivity of the
methods to detect measurable topographic changes. The results of the M3C2-PM
show that the average distance uncertainty between the first and the last
surveys is about 6.5 cm over the whole area at the 95 % confidence level
(Fig. 13a). Furthermore, considering a smaller portion of the area, the
uncertainty decreases to about 3.9 cm at the 95 % confidence level
(Fig. 13b). This allows us to analyze certain morphological changes and
anthropogenic activity on the mud surface (Fig. 14). The anthropogenic
activity determined a height decrease of about 16 cm where a wood platform
was previously located. Moreover, a height increase of about 14 cm is
recorded at the place where the wood platform has been relocated. The values
recorded are consistent with the real thickness of the object detected,
differing by 2 cm (Fig. 14). The callipers show that it is possible to
measure changes of at least 2 cm (Fig. 11).</p>
      <p id="d1e1499">After the uncertainty and sensitivity of the surveys were computed, the time
series were made. Considering the significant changes and their errors, we
computed the trend of deformation of two areas in order to reconstruct the
evolution of the phenomena which generated these changes (Figs. 16 and
17).</p>
      <p id="d1e1503">Considering the results obtained by SfM, we propose a monitoring system of the
Santa Barbara mud volcano based on a semi-quantitative approach. We defined
three states by setting a space-time range:
<list list-type="bullet"><list-item>
      <p id="d1e1508">normal state if the deformation value does not exceed 5 cm in the range
between 1 and 2 months</p></list-item><list-item>
      <p id="d1e1512">pre-alert state if the deformation value is between 5 cm and 10 cm during a
period of between 1 and 2 months</p></list-item><list-item>
      <p id="d1e1516">alert state if the deformation value exceeds 10 cm in the range between 1 and
2 months.</p></list-item></list></p>
      <p id="d1e1519">To define the state of the activity of the mud volcano, the area affected by
deformation must be a significant area of<?pagebreak page2892?> the total surface of the volcano.
The definition of the activity is an important aspect of the monitoring of
hazard because there are many natural phenomena that can produce
deformation in a small area (like a gryphon) or in a larger portion (like
the sedimentation occurring at the border of the mud volcano). The
significant area affected by deformation must be correctly defined by an
operator (public agency, university, institute of research or Dipartimento
della Protezione Civile) which really knows the natural phenomena that can
occur on the Santa Barbara mud volcano.</p>
      <p id="d1e1522">The methodological approach is valuable and efficient from the point of view
of quantity and quality of data collected in relation to the work and time
spent. This monitoring technique is a useful tool to detect the early
unrest phase of the mud volcano usually induced by changes in pressure and
volume of fluid rising from the stagnation chamber.</p>
      <p id="d1e1525">The pre-eruptive deformation consists of a marked uplift and occasional
small subsidence which are probably related to the redistribution of the
subsoil of the pressurized fluids (Antonelli et al., 2014). According to
Antonelli et al. (2014), soil uplift can occur up to a year before the
eruption.</p><?xmltex \hack{\newpage}?>
</sec>
<sec id="Ch1.S5" sec-type="conclusions">
  <label>5</label><title>Conclusion</title>
      <p id="d1e1538">In hazard management, the SfM technique (Gomez and Purdie, 2016; Kaab, 2000;
Fugazza et al., 2018; Giordan et al., 2017, 2018) is starting to be widely used
by the scientific community. In the monitoring of potentially dangerous
active sites, the UAVs are very advantageous because they are not used only
as a support in the post-disaster events (Rokhmana and Andaru, 2017;
Hisbaron et al., 2018) but also for the pre-event monitoring.</p>
      <p id="d1e1541">According to Kopf (2002), Antonielli  et al. (2014), Madonia et al. (2011),
INGV (2008), and Regione Siciliana (2008), the deformations of the surface
shell of mud volcanoes can occur up to 1 year before the paroxysmal event
with doming and the development of structural lineaments with an order of magnitude from centimeters to decimeters.</p>
      <p id="d1e1544">The results allow us to define the criteria for monitoring and analyzing the
study area. For the mud volcano of Santa Barbara, the monitoring criteria
are as follows:</p>
      <p id="d1e1547"><list list-type="bullet">
          <list-item>

      <?pagebreak page2893?><p id="d1e1552">Monitoring interval is between 1 and 2 months.
<?xmltex \hack{\newpage}?></p>
          </list-item>
          <list-item>

      <p id="d1e1559">The optimal number of GCPs is between 12 and 18.</p>
          </list-item>
          <list-item>

      <p id="d1e1565">Acquisition of GCPs is by high-precision topographical instrumentation (TST).</p>
          </list-item>
          <list-item>

      <p id="d1e1571">The processing chain of the sparse point cloud according to workflow of USGS (2017) was enhanced by the correct value of “tie point accuracy” and
“marker accuracy” as suggested by James (2017a).</p>
          </list-item>
          <list-item>

      <p id="d1e1577">An assessment of the state of activity of the mud volcano is based on a
semi-quantitative approach.</p>
          </list-item>
        </list></p>
      <p id="d1e1583">The frequency of the campaigns depends on the status of activity, while the
other criteria depend on the object/structure of the monitoring.</p>
      <p id="d1e1586">These criteria allow us to detect events with deformation of at least 2 cm.
In the case of anomalous values detected, the monitoring campaigns must be
improved. This involves extensive monitoring, such as (i) developing time
series localized in key areas and (ii) combining different methodologies,
e.g., micro-seismicity monitoring and 3D geophysical
prospecting (Imposa et al., 2016), to improve the monitoring system of the
active geological process.</p>
</sec>

      
      </body>
    <back><notes notes-type="codeavailability"><title>Code availability</title>

      <p id="d1e1593">The codes used in this paper are provided by authors cited in the text. The links to these codes or software are as follows:
Precision_estimates.py: <uri>https://www.lancaster.ac.uk/staff/jamesm/software/python/pe_1.4.0/precision_estimates.pySfm_georef</uri> (James, 2018), <uri>http://www.lancaster.ac.uk/staff/jamesm/software/sfm_georef.htmMonte_Carlo_BA.p</uri> (James, 2017b), <uri>https://www.lancaster.ac.uk/staff/jamesm/software/python/gcp_1.3.0/Monte_Carlo_BA.py</uri> (James, 2016).</p>
  </notes><notes notes-type="dataavailability"><title>Data availability</title>

      <p id="d1e1608">The data are available on request by email to the corresponding author (giorgio.deguidi@unict.it) and to Fabio Brighenti (fabio.brighenti@unict.it).</p>
  </notes><notes notes-type="authorcontribution"><title>Author contributions</title>

      <p id="d1e1614">FB conducted the photogrammetric processing and all the statistical analysis of the point clouds. DM and GDG<?pagebreak page2894?> conducted the UAV flight campaigns. FB, FC, DM and GDG conducted the topographic and geodetic surveys. FC conducted the GNSS processing and analysis. FB and FC conducted the topographic processing and analysis. FB, FC and GDG wrote the paper. FB produced the figures. GDG was the supervisor. All the authors were involved in the conceptualization, discussion of the results and editing of the manuscript.</p>
  </notes><notes notes-type="competinginterests"><title>Competing interests</title>

      <p id="d1e1620">The authors declare that they have no conflict of interest.</p>
  </notes><notes notes-type="disclaimer"><title>Disclaimer</title>

      <p id="d1e1626">Publisher’s note: Copernicus Publications remains neutral with regard to jurisdictional claims in published maps and institutional affiliations.</p>
  </notes><notes notes-type="sistatement"><title>Special issue statement</title>

      <p id="d1e1632">This article is part of the special issue “Remote sensing and Earth observation data in natural hazard and risk studies”. It is not associated with a conference.</p>
  </notes><ack><title>Acknowledgements</title><p id="d1e1638">We thank Silvia Rita Popolo for her valuable support. Finally, we are gratefull to the two anonymous referees and to Elena Russo who helped us to enhance the clarity and structure of the content of this manuscript.</p></ack><notes notes-type="financialsupport"><title>Financial support</title>

      <p id="d1e1643">This research has been supported by the Presidenza del Consiglio dei Ministri (Project Code E98D19000000001, Monitoraggio e Studio dei Processi di 10 Deformazione Superficiale Connessi al Vulcanismo-Sedimentario delle Maccalube di Santa Barbara (Caltanisetta) within the DPCM 25 May 2016 – Riqualificazione Urbana e la Sicurezza delle Periferie delle Città Metropolitane, dei Comuni Capoluogo e delle Città di Aosta; scientific supervisor: Giorgio De Guidi). Moreover, the publication of the paper has been supported by the PhD in Earth and Environmental Sciences fund (PhD coordinator Agata Di Stefano), the PIAno di inCEntivi per la RIcerca di Ateneo (PIACERI 2020/2022) (fund manager Giorgio De Guidi) and UPC Piano Della Ricerca (fund manager Carmelo Monaco).</p>
  </notes><notes notes-type="reviewstatement"><title>Review statement</title>

      <p id="d1e1649">This paper was edited by Michelle Parks and reviewed by Elena Russo and two anonymous referees.</p>
  </notes><?xmltex \hack{\newpage}?><ref-list>
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    <!--<article-title-html>UAV survey method to monitor and analyze geological  hazards: the case study of the mud volcano of  Villaggio Santa Barbara, Caltanissetta (Sicily)</article-title-html>
<abstract-html><p>Active geological processes often generate a ground surface response such as uplift, subsidence and faulting/fracturing. Nowadays remote sensing represents a key tool for the evaluation and monitoring of natural hazards. The use of unmanned aerial vehicles (UAVs) in relation to observations of natural hazards encompasses three main stages: pre- and post-event data acquisition, monitoring, and risk assessment. The mud volcano of Santa Barbara (Municipality of Caltanissetta, Italy) represents a dangerous site because on 11 August 2008 a paroxysmal event caused serious damage to infrastructures within a range of about 2 km. The main precursors to mud volcano paroxysmal events are uplift and the development of structural features with dimensions ranging from centimeters to decimeters. Here we present a methodology for monitoring deformation processes that may be precursory to paroxysmal events at the Santa Barbara mud volcano. This methodology is based on (i) the data collection, (ii) the structure from motion (SfM) processing chain and (iii) the M3C2-PM algorithm for the comparison between point clouds and uncertainty analysis with a statistical approach. The objective of this methodology is to detect precursory activity by monitoring deformation processes with centimeter-scale precision and a temporal frequency of 1–2 months.</p></abstract-html>
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