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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-24-1135-2024</article-id><title-group><article-title>Surface rupture kinematics of the 2020 <inline-formula><mml:math id="M1" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">w</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> 6.6 Masbate (Philippines) earthquake determined from optical and radar data</article-title><alt-title>Surface rupture kinematics of the 2020 <inline-formula><mml:math id="M2" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">w</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> 6.6 Masbate earthquake</alt-title>
      </title-group><?xmltex \runningtitle{Surface rupture kinematics of the 2020 $M_{\mathrm{w}}$\,6.6 Masbate earthquake}?><?xmltex \runningauthor{K.~S.~Sta.~Rita et al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes" rid="aff1">
          <name><surname>Sta. Rita</surname><given-names>Khelly Shan</given-names></name>
          <email>kcstarita@up.edu.ph</email>
        <ext-link>https://orcid.org/0000-0001-5329-8806</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Valkaniotis</surname><given-names>Sotiris</given-names></name>
          
        <ext-link>https://orcid.org/0000-0003-0003-2902</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff3">
          <name><surname>Lagmay</surname><given-names>Alfredo Mahar Francisco</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-9672-9389</ext-link></contrib>
        <aff id="aff1"><label>1</label><institution>National Institute of Geological Sciences, University of the Philippines, Diliman, 1101 Quezon City, Philippines</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>Department of Civil Engineering, Democritus University of Thrace, 67100 Xanthi, Greece</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>UP Resilience Institute, University of the Philippines, Diliman, 1101 Quezon City, Philippines</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Khelly Shan Sta. Rita (kcstarita@up.edu.ph)</corresp></author-notes><pub-date><day>3</day><month>April</month><year>2024</year></pub-date>
      
      <volume>24</volume>
      <issue>4</issue>
      <fpage>1135</fpage><lpage>1161</lpage>
      <history>
        <date date-type="received"><day>11</day><month>May</month><year>2023</year></date>
           <date date-type="rev-request"><day>22</day><month>June</month><year>2023</year></date>
           <date date-type="rev-recd"><day>8</day><month>January</month><year>2024</year></date>
           <date date-type="accepted"><day>26</day><month>February</month><year>2024</year></date>
      </history>
      <permissions>
        <copyright-statement>Copyright: © 2024 </copyright-statement>
        <copyright-year>2024</copyright-year>
      <license license-type="open-access"><license-p>This work is licensed under the Creative Commons Attribution 4.0 International License. To view a copy of this licence, visit <ext-link ext-link-type="uri" xlink:href="https://creativecommons.org/licenses/by/4.0/">https://creativecommons.org/licenses/by/4.0/</ext-link></license-p></license></permissions><self-uri xlink:href="https://nhess.copernicus.org/articles/.html">This article is available from https://nhess.copernicus.org/articles/.html</self-uri><self-uri xlink:href="https://nhess.copernicus.org/articles/.pdf">The full text article is available as a PDF file from https://nhess.copernicus.org/articles/.pdf</self-uri>
      <abstract><title>Abstract</title>

      <p id="d1e133">Optical correlation, interferometry, and field investigation of laterally offset features were undertaken to analyze the kinematics of the 2020 <inline-formula><mml:math id="M3" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">w</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> 6.6 Masbate earthquake. Ground displacement fields show a peak left-lateral offset of 0.6 m corresponding to <inline-formula><mml:math id="M4" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">w</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> 6.6 geodetic moment magnitude, with an average 0.4 m left-lateral slip. The slip distributions also indicate a single asperity located <inline-formula><mml:math id="M5" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">200</mml:mn></mml:mrow></mml:math></inline-formula> m SE of the centroid. Post-seismic deformation estimates from interferometry highlight an at least 0.14 m left-lateral offset consistent with a <inline-formula><mml:math id="M6" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">w</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> 6.2 post-seismic moment magnitude. The total and post-seismic slip distributions coincide with each other, with both peaks adjacent to the centroid. Slip measurements and the <inline-formula><mml:math id="M7" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">28.2</mml:mn></mml:mrow></mml:math></inline-formula>–41 km rupture length estimates from field and remote sensing datasets characterize the Masbate segment as capable of producing long ruptures with significant offsets despite the presence of interseismic creep. Post-seismic interferograms resolved the rupture far better than optical correlation, which was degraded due to high-amplitude noise from sensor and environmental sources. Nevertheless, this review of the 2020 <inline-formula><mml:math id="M8" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">w</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> 6.6 Masbate earthquake provides a comprehensive slip measurement of the surface rupture and demonstrates the presence of two transtensional basins in the Masbate province, revealing new insights into the seismic hazard and seismotectonic setting of the central Philippines.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <label>1</label><title>Introduction</title>
      <p id="d1e210">Philippine earthquake geodesy traditionally relies on interferometry, a global navigation satellite system (GNSS), waveform modeling, and field investigation <xref ref-type="bibr" rid="bib1.bibx93 bib1.bibx102" id="paren.1"/>. The techniques have been used to investigate the rupture kinematics of significant earthquakes in the Philippines. Earthquake kinematics describes the three-dimensional motion of the ground surface during an earthquake event and is characterized by the spatial distribution of ground displacements along the fault rupture. It is crucial in seismic hazard assessments since it can be used in estimating the possible ground shaking intensity and fault rupture potential of a particular location <xref ref-type="bibr" rid="bib1.bibx65" id="paren.2"/>.</p>
      <p id="d1e219">A <inline-formula><mml:math id="M9" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">w</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> 6.6 earthquake jolted the island of Masbate on 18 August 2020 and was followed by a <inline-formula><mml:math id="M10" display="inline"><mml:mi>M</mml:mi></mml:math></inline-formula> 5.7 aftershock in about 10 min <xref ref-type="bibr" rid="bib1.bibx11" id="paren.3"/>. In the span of 32 h after the mainshock, 244 aftershocks were recorded ranging from <inline-formula><mml:math id="M11" display="inline"><mml:mi>M</mml:mi></mml:math></inline-formula> 1.6 to <inline-formula><mml:math id="M12" display="inline"><mml:mi>M</mml:mi></mml:math></inline-formula> 5.1 <xref ref-type="bibr" rid="bib1.bibx70" id="paren.4"/>. The focal mechanism solution of the mainshock illustrates a strike-slip movement with hypocenter at 7 km S29° E of Cataingan and a depth of 21 km <xref ref-type="bibr" rid="bib1.bibx70" id="paren.5"/>. The earthquake resulted in devastating losses in terms of human lives and properties <xref ref-type="bibr" rid="bib1.bibx66" id="paren.6"/>. The heavy impacts of the earthquake warrant a thorough evaluation of the event to support the assessment of seismic hazards to mitigate losses and damages for the next earthquakes on the island of Masbate.</p>
      <?pagebreak page1136?><p id="d1e267">Preliminary assessments using Sentinel-1 interferograms showed butterfly-shaped fringes and phase shifts between 3 and 30 cm along the descending track line of sight (LOS) <xref ref-type="bibr" rid="bib1.bibx70" id="paren.7"/> and <inline-formula><mml:math id="M13" display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">15</mml:mn></mml:mrow></mml:math></inline-formula> cm LOS ground deformation along the ascending track <xref ref-type="bibr" rid="bib1.bibx84" id="paren.8"/>. The ascending interferograms used a 12 d (15–27 August 2020) temporal baseline, resulting in low phase coherence of the InSAR pairs. Spectral analysis of seismic waveforms <xref ref-type="bibr" rid="bib1.bibx82" id="paren.9"/> outlined a 3.0 km s<inline-formula><mml:math id="M14" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> rupture velocity beginning on a shallow region of the southern fault plane with peak ground displacements <inline-formula><mml:math id="M15" display="inline"><mml:mo>≥</mml:mo></mml:math></inline-formula> 1.0 m.</p>
      <p id="d1e309">We introduce the application of optical image correlation (OIC) in the Philippines to highlight its importance when used alongside interferometry. The simultaneous application of OIC and InSAR provides complementary information on the decorrelated portions of the coseismic interferogram to improve the understanding of the 2020 <inline-formula><mml:math id="M16" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">w</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> 6.6 Masbate earthquake since the event is still relatively unstudied compared with the 2003 <inline-formula><mml:math id="M17" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> 6.2 event that occurred on the same fault segment <xref ref-type="bibr" rid="bib1.bibx18 bib1.bibx52 bib1.bibx88 bib1.bibx89" id="paren.10"/>.</p>
      <p id="d1e338">This study presents first-order ground displacements and post-seismic slip from the Masbate segment of the Philippine Fault (PF). The resulting slip distributions and surface rupture parameters refine our understanding of the Masbate segment, shed light on the relationship of rupture initiation with mesoscale structures, topography, and bedrock lithology, as well as provide insights into the underlying faulting mechanisms. The accompanying morphological interpretations of surface ruptures highlight the known stress regime in Masbate, expanding upon our understanding of the structural characteristics of the central Philippines. These findings contribute to the enhancement of earthquake models for use in seismic hazard assessments in the region.</p>
</sec>
<sec id="Ch1.S2">
  <label>2</label><title>Geologic setting and tectonic framework</title>
      <p id="d1e349">The Philippines is a region of active tectonics and volcanism arising from the interaction of the Sunda block of the Eurasian plate with the Philippine Sea Plate (Fig. <xref ref-type="fig" rid="Ch1.F1"/>a) <xref ref-type="bibr" rid="bib1.bibx5 bib1.bibx20" id="paren.11"/>. Oppositely dipping subduction margins flank the archipelago: the east-dipping Manila, Sulu, Negros, and Cotabato trenches in the west; and the west-dipping Philippine Trench and East Luzon Trough in the east <xref ref-type="bibr" rid="bib1.bibx5 bib1.bibx16" id="paren.12"/>. The eastern margin accommodates the northwesterly advance of the Philippine Sea Plate at a rate of 3–9 cm yr<inline-formula><mml:math id="M18" 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> relative to the Eurasian plate <xref ref-type="bibr" rid="bib1.bibx81" id="paren.13"/>, while the western end consumes the subducting Sunda block moving at a rate of 1 cm yr<inline-formula><mml:math id="M19" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> eastward relative to the Eurasian plate <xref ref-type="bibr" rid="bib1.bibx26" id="paren.14"/>. The interaction and oblique convergence of the tectonic plates that bind the country resulted in the formation of the approximately 1200 km-long left-lateral Philippine Fault in the Middle Miocene <xref ref-type="bibr" rid="bib1.bibx2 bib1.bibx39 bib1.bibx89 bib1.bibx71" id="paren.15"/> as the Philippine Sea Plate's motion shifted counterclockwise from northward to a northwestward direction <xref ref-type="bibr" rid="bib1.bibx5" id="paren.16"/>. An Association of Southeast Asian Nations (ASEAN)-wide GPS network assessment <xref ref-type="bibr" rid="bib1.bibx10 bib1.bibx4 bib1.bibx6 bib1.bibx75" id="paren.17"/> measured a 2–3 cm yr<inline-formula><mml:math id="M20" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> current slip rate throughout the fault zone. An approximately 580 m curved section of the PF traverses the central Philippines from the southeastern portion of Quezon Province to Leyte Island (Fig. <xref ref-type="fig" rid="Ch1.F1"/>b). Coined the Philippine Fault Bend, the deformation zone in the midsection of the PF is characterized by a N50° W fault strike and forms a releasing bend structure relative to the approximately N20° W general strike north and south of the central section <xref ref-type="bibr" rid="bib1.bibx51" id="paren.18"/>.</p>

      <?xmltex \floatpos{p}?><fig id="Ch1.F1" specific-use="star"><?xmltex \currentcnt{1}?><?xmltex \def\figurename{Figure}?><label>Figure 1</label><caption><p id="d1e420">Panel <bold>(a)</bold> shows the regional geologic setting of the Philippine archipelago with the adjacent Philippine Sea Plate (PSP) and Eurasian plate (EU). The large-scale tectonic features are also depicted, including the east-dipping subduction zones – the Manila Trench (MT), Negros Trench (NT), Cotabato Trench (CT), and Sulu Trench (ST) – on the western side; west-dipping trenches – East Luzon Trough (ELT) and Philippine Trench (PT) – on the eastern side; and the resultant Philippine Fault running across the archipelago. The white arrow indicates the movement direction of the Philippine Sea Plate. Panel <bold>(b)</bold> shows the major structural features directly affecting Masbate including the central Philippine Fault Zone (Guinayangan, Masbate, and Leyte segments), their approximate offshore projections, the Legaspi Lineament, and the Sibuyan Sea Fault. Panel <bold>(c)</bold> shows the southeastern Masbate area with the involved lithologic units and traces of the Philippine Fault and Uson Fault. The black–white boundary box highlights the primary region of interest. (Lithology adapted from <xref ref-type="bibr" rid="bib1.bibx57" id="altparen.19"/>; trace of active structural features adapted from PHIVOLCS.) Panel <bold>(d)</bold> shows the historical seismicity of Masbate Island from 1917 to 2022 with the moderate earthquakes (<inline-formula><mml:math id="M21" display="inline"><mml:mi>M</mml:mi></mml:math></inline-formula> 4–6.6) with focal mechanism solutions of the February 2003 and August 2020 events. (Background topography and bathymetry from GEBCO; earthquake data acquired from USGS-NEIC; focal mechanism solutions sourced from GlobalCMT.)</p></caption>
        <?xmltex \igopts{width=426.791339pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/24/1135/2024/nhess-24-1135-2024-f01.jpg"/>

      </fig>

<sec id="Ch1.S2.SS1">
  <label>2.1</label><title>Geology of Masbate</title>
      <p id="d1e459">The PF and Sibuyan Sea Fault (SSF) are the prominent structural features of Masbate Island <xref ref-type="bibr" rid="bib1.bibx70 bib1.bibx89" id="paren.20"/> (Fig. <xref ref-type="fig" rid="Ch1.F1"/>b). The Masbate segment of the PF extends from Burias and Ticao islands in the north, and strikes N40° W as it crosses the southeastern tip of the mainland <xref ref-type="bibr" rid="bib1.bibx9" id="paren.21"/>. In terms of morphology, it spans approximately 30 km along a linear trough parallel to the coastline <xref ref-type="bibr" rid="bib1.bibx70 bib1.bibx89" id="paren.22"/>. Complexities in the fault geometry include a fault complexity between 12°08<inline-formula><mml:math id="M22" display="inline"><mml:msup><mml:mi/><mml:mo>′</mml:mo></mml:msup></mml:math></inline-formula> N and 12°06<inline-formula><mml:math id="M23" display="inline"><mml:msup><mml:mi/><mml:mo>′</mml:mo></mml:msup></mml:math></inline-formula> N latitude, and a bifurcation around 12°03<inline-formula><mml:math id="M24" display="inline"><mml:msup><mml:mi/><mml:mo>′</mml:mo></mml:msup></mml:math></inline-formula> N. The northeastern leg of the bifurcated structure is curved at 12° N and connects to the Leyte segment, whereas the southwestern leg strikes at N20° W and appears to terminate at Cataingan Bay <xref ref-type="bibr" rid="bib1.bibx69" id="paren.23"/>. Offshore seismic profiling in the bay <xref ref-type="bibr" rid="bib1.bibx56" id="paren.24"/> shows left-stepping faults and negative flower structures that denote transtensional deformation in the region.</p>
      <p id="d1e507">The SSF is another left-lateral strike-slip fault with a normal component <xref ref-type="bibr" rid="bib1.bibx9 bib1.bibx21" id="paren.25"/>. It runs parallel to the PF in mainland Masbate and then deflects westward into the Sibuyan Sea (Fig. <xref ref-type="fig" rid="Ch1.F1"/>b). The extensional component associated with the SSF is represented by tilted blocks formed from normal faulting and bathymetric depressions in the Sibuyan Sea <xref ref-type="bibr" rid="bib1.bibx22" id="paren.26"/>. The SSF influences the local stress regime expressed by alternating extensive and compressive structures, due to its interaction with the PF <xref ref-type="bibr" rid="bib1.bibx10" id="paren.27"/>. The SSF was also described as separate from the PF and is a manifestation of the transtensional deformation with the <inline-formula><mml:math id="M25" display="inline"><mml:mrow><mml:mn mathvariant="normal">3</mml:mn><mml:mi mathvariant="italic">σ</mml:mi></mml:mrow></mml:math></inline-formula> oriented perpendicular to the PF <xref ref-type="bibr" rid="bib1.bibx3 bib1.bibx9" id="paren.28"/>. GPS measurements further substantiate this regime on the local scale <xref ref-type="bibr" rid="bib1.bibx13 bib1.bibx33" id="paren.29"/>.</p>
      <?pagebreak page1138?><p id="d1e538">Ophiolites comprise the basement complex of Masbate Island and are unconformably overlain by a series of sedimentary and igneous units (Fig. <xref ref-type="fig" rid="Ch1.F1"/>c). The Cretaceous Panguiranan Chert represents the pelagic cover of the ophiolite sequence <xref ref-type="bibr" rid="bib1.bibx8" id="paren.30"/>. The Late Oligocene Nabangig Formation is the oldest lithologic unit underlying the area of interest and is composed of a clastic sequence with recrystallized limestone. The Middle Miocene Lanang Formation lies unconformably over the Nabangig Formation and consists of highly deformed sedimentary rocks ranging from conglomerates to mudstones <xref ref-type="bibr" rid="bib1.bibx57" id="paren.31"/>. The majority of the study area is underlain by the Miocene–Pliocene Buyag Formation. It overlies the Lanang Formation and is composed of conglomerates with fine-grained igneous clasts and interbedded shale and siliceous sediments. The largely coralline Pleistocene Port Barrera Limestone is the youngest stratigraphic unit in the province <xref ref-type="bibr" rid="bib1.bibx73" id="paren.32"/>.</p>
</sec>
<sec id="Ch1.S2.SS2">
  <label>2.2</label><title>Seismotectonics of the Masbate segment</title>
      <p id="d1e561"><xref ref-type="bibr" rid="bib1.bibx13" id="text.33"/> and <xref ref-type="bibr" rid="bib1.bibx52" id="text.34"/> described the Masbate segment as the transition zone between the northern and southern segments of the central PF. Historical earthquake information revealed recurrence intervals from as short as 5 years <xref ref-type="bibr" rid="bib1.bibx18" id="paren.35"/> for moderate magnitude (<inline-formula><mml:math id="M26" display="inline"><mml:mi>M</mml:mi></mml:math></inline-formula> 5.5–6.2) earthquakes to as much as 238 years using slip deficit rates between the 2003 event and interseismic velocities <xref ref-type="bibr" rid="bib1.bibx52" id="paren.36"/>. A marked absence of strong events beyond <inline-formula><mml:math id="M27" display="inline"><mml:mrow><mml:mi>M</mml:mi><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">7.0</mml:mn></mml:mrow></mml:math></inline-formula> in the past four centuries is also apparent <xref ref-type="bibr" rid="bib1.bibx17 bib1.bibx80" id="paren.37"/>. A map (Fig. <xref ref-type="fig" rid="Ch1.F1"/>d) of moderate seismicity between 1917 and 2022 culled from the United States Geological Survey – National Earthquake Information Center (USGS-NEIC) <xref ref-type="bibr" rid="bib1.bibx92" id="paren.38"/> highlights the earthquake epicenters related to the Masbate segment and the SSF during this period. Observations and discussions on the 2003 event led <xref ref-type="bibr" rid="bib1.bibx18" id="text.39"/> to characterize the seismic activity of the segment as capable of generating moderate to large events that produce ruptures larger than expected and can be succeeded by post-seismic deformation or creep.</p>
      <p id="d1e606">The 2003 <inline-formula><mml:math id="M28" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> 6.2 event is the previous notable earthquake in the province that produced an approximately 20 km-long rupture with the epicenter in the northern portion of the Masbate segment. It was accompanied by either post-seismic deformation or a slow creep component <xref ref-type="bibr" rid="bib1.bibx18 bib1.bibx52 bib1.bibx88 bib1.bibx89" id="paren.40"/>. Kinematic offsets were measured at a maximum of 47–50 cm, which is beyond the expected peak offsets for a <inline-formula><mml:math id="M29" display="inline"><mml:mi>M</mml:mi></mml:math></inline-formula> 6.2 earthquake, based on empirical magnitude scaling equations <xref ref-type="bibr" rid="bib1.bibx98" id="paren.41"/>. <xref ref-type="bibr" rid="bib1.bibx52" id="text.42"/> attributed the post-seismic deformation to the significant excess moment released by the earthquake. Aftershock analysis of earthquakes within 2 months of the 2003 temblor showed a cluster of <inline-formula><mml:math id="M30" display="inline"><mml:mi>M</mml:mi></mml:math></inline-formula> 5.0–6.0 epicenters at the southern portion of the fault. The aftershocks were accompanied by the development of hairline fractures near Cataingan that expanded to as much as 8 mm <xref ref-type="bibr" rid="bib1.bibx18" id="paren.43"/>. In addition, <xref ref-type="bibr" rid="bib1.bibx14" id="text.44"/> recorded 10 cm GPS deviations within 6 months after the mainshock, supporting observations of post-seismic deformation. Coulomb stress transfer (CST) analysis showed that the 2003 event raised the stress in the southern part of Masbate by approximately 0.3–1 bar <xref ref-type="bibr" rid="bib1.bibx53" id="paren.45"/>, which is presumed to have reduced the time elapsed before the 2020 earthquake.</p>
      <p id="d1e653">The apparent absence of strong earthquakes (<inline-formula><mml:math id="M31" display="inline"><mml:mrow><mml:mi>M</mml:mi><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">7.0</mml:mn></mml:mrow></mml:math></inline-formula>) in the Masbate segment can be explained by the presence of creep <xref ref-type="bibr" rid="bib1.bibx79" id="paren.46"/>. Aseismic slip during interseismic periods was measured at <inline-formula><mml:math id="M32" display="inline"><mml:mrow><mml:mn mathvariant="normal">2.3</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">1.1</mml:mn></mml:mrow></mml:math></inline-formula> cm yr<inline-formula><mml:math id="M33" 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> through GPS <xref ref-type="bibr" rid="bib1.bibx14" id="paren.47"/> and 0.7–1.7 cm 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> through alignment arrays <xref ref-type="bibr" rid="bib1.bibx90" id="paren.48"/>. A moderate background seismicity can be observed along the Masbate segment (Fig. <xref ref-type="fig" rid="Ch1.F1"/>d) and is further described in PHIVOLCS reports <xref ref-type="bibr" rid="bib1.bibx68" id="paren.49"/>.</p>
</sec>
</sec>
<sec id="Ch1.S3">
  <label>3</label><title>Data and methods</title>
      <p id="d1e728">The surface displacement components of the Masbate earthquake were measured using optical and radar satellite data. Pixel offset tracking on PlanetLabs image pairs with 3.125 m resolution was accomplished using the <monospace>mm2dpossism</monospace> binary of the MicMac program <xref ref-type="bibr" rid="bib1.bibx77" id="paren.50"/> for the horizontal ground displacements. Interferometric Synthetic Aperture Radar (InSAR) was done using the European Space Agency's (ESA) Sentinel-1A/B radar data with a 6 d temporal baseline (14–21 August 2020) for the coseismic slip and a 31 d (20 August to 20 September 2020) time series after the mainshock for the post-seismic deformation following the rapid aftershock decay duration.</p>
<sec id="Ch1.S3.SS1">
  <label>3.1</label><title>Spatiotemporal seismicity analysis</title>
      <p id="d1e744">Earthquake data from 2019 to 2021 with magnitudes <inline-formula><mml:math id="M35" display="inline"><mml:mrow><mml:mi>M</mml:mi><mml:mo>≥</mml:mo><mml:mn mathvariant="normal">1.0</mml:mn></mml:mrow></mml:math></inline-formula> were gathered from the PHIVOLCS online earthquake archive (Sect. S3 in the Supplement). Foreshock and aftershock patterns were analyzed by plotting the distribution of both magnitude and frequency in time and space. All seismicity information was primarily used to define the earthquake periods <xref ref-type="bibr" rid="bib1.bibx38 bib1.bibx64" id="paren.51"/> related to the 2020 Masbate event. Focal mechanism solutions acquired from PHIVOLCS, USGS, and GlobalCMT were used for the analysis of the nodal planes present in the double couple as a seismological basis of the sense of movement of the fault plane responsible for the mainshock.</p>
</sec>
<sec id="Ch1.S3.SS2">
  <label>3.2</label><title>Optical image correlation</title>
      <p id="d1e770">PlanetScope satellite imagery <xref ref-type="bibr" rid="bib1.bibx72" id="paren.52"/> was the primary dataset due to the daily data acquisition and high spatial resolution of the available products. Images with the least cloud cover covering the region of interest (Fig. <xref ref-type="fig" rid="Ch1.F1"/>c) with a maximum 15 % obstruction threshold were selected. Ortho Tile products with a 3.125 m ground resolution, processed at level 3A and corrected for surface reflectance (SR), were utilized. When Ortho Tile products were unavailable, we used Ortho Scene products downsampled to 3.125 m ground resolution and corrected for top-of-atmosphere (TOA) reflectance.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2" specific-use="star"><?xmltex \currentcnt{2}?><?xmltex \def\figurename{Figure}?><label>Figure 2</label><caption><p id="d1e780">Two classes of PlanetScope satellite imagery pairs evaluated through optical correlation. Panel <bold>(a)</bold> shows short-term pairs taken within the same year as the Masbate earthquake ranging from 5 to 9 months apart and as close to the event as possible. Panel <bold>(b)</bold> shows approximately annual span pairs acquired at about 365 d apart where environmental interference is expected to be at a minimum <xref ref-type="bibr" rid="bib1.bibx34" id="paren.53"/>.</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/24/1135/2024/nhess-24-1135-2024-f02.png"/>

        </fig>

      <p id="d1e798">We realize the necessity for the shortest temporal baseline to properly delimit the slip components. However, no workable Planet datasets in terms of cloud cover, ROI coverage, or compatibility of acquisition parameters were available that more closely bracketed the earthquake. To observe the influence of time on the quality of the output offset rasters, two sets of temporal ranges were tested for the Masbate event (Fig. <xref ref-type="fig" rid="Ch1.F2"/>). Five short-term pairs were selected from<?pagebreak page1139?> visually feasible images sampled months apart in 2020, whereas 10 <italic>annual</italic> pairs were roughly 1 year apart (Table <xref ref-type="table" rid="Ch1.T1"/>). This was done to minimize the effect of environmental variables following the approach of <xref ref-type="bibr" rid="bib1.bibx34" id="text.54"/>.</p>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T1"><?xmltex \currentcnt{1}?><label>Table 1</label><caption><p id="d1e815">Satellite geometry and acquisition parameters of the PlanetScope data used in the study. Values of the satellite azimuth (satAzi) are unavailable for the older images in the table. Available tiles for 23 June 2020 are merged to create a single mosaic to maximize the extent. The two datasets for 2 April 2020 are analyzed separately. Time zone is UTC.</p></caption><oasis:table frame="topbot"><?xmltex \begin{scaleboxenv}{.88}[.88]?><oasis:tgroup cols="6">
     <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="center"/>
     <oasis:thead>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">Acquisition</oasis:entry>
         <oasis:entry colname="col2">satID</oasis:entry>
         <oasis:entry colname="col3">satAzi</oasis:entry>
         <oasis:entry colname="col4">view<inline-formula><mml:math id="M36" display="inline"><mml:mi mathvariant="normal">∠</mml:mi></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col5">sunAzi</oasis:entry>
         <oasis:entry colname="col6">sunElev</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>
         <oasis:entry colname="col1">2019-11-28T01:53:43</oasis:entry>
         <oasis:entry colname="col2">103e</oasis:entry>
         <oasis:entry colname="col3">–</oasis:entry>
         <oasis:entry colname="col4">1.2</oasis:entry>
         <oasis:entry colname="col5">143.9</oasis:entry>
         <oasis:entry colname="col6">48.7</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">2020-04-09T00:33:57</oasis:entry>
         <oasis:entry colname="col2">100d</oasis:entry>
         <oasis:entry colname="col3">–</oasis:entry>
         <oasis:entry colname="col4">0</oasis:entry>
         <oasis:entry colname="col5">90.3</oasis:entry>
         <oasis:entry colname="col6">42.7</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">2020-04-17T02:35:36</oasis:entry>
         <oasis:entry colname="col2">106e</oasis:entry>
         <oasis:entry colname="col3">–</oasis:entry>
         <oasis:entry colname="col4">2.1</oasis:entry>
         <oasis:entry colname="col5">92.5</oasis:entry>
         <oasis:entry colname="col6">73.1</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">2020-06-06T00:26:15</oasis:entry>
         <oasis:entry colname="col2">0f32</oasis:entry>
         <oasis:entry colname="col3">–</oasis:entry>
         <oasis:entry colname="col4">3</oasis:entry>
         <oasis:entry colname="col5">69.9</oasis:entry>
         <oasis:entry colname="col6">41.8</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">2020-06-23T01:29:47</oasis:entry>
         <oasis:entry colname="col2">2263</oasis:entry>
         <oasis:entry colname="col3">272.7</oasis:entry>
         <oasis:entry colname="col4">2</oasis:entry>
         <oasis:entry colname="col5">66.4</oasis:entry>
         <oasis:entry colname="col6">55.4</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">2020-06-23T01:54:27</oasis:entry>
         <oasis:entry colname="col2">100a</oasis:entry>
         <oasis:entry colname="col3">102.6</oasis:entry>
         <oasis:entry colname="col4">1</oasis:entry>
         <oasis:entry colname="col5">63.2</oasis:entry>
         <oasis:entry colname="col6">61.1</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">2020-07-07T00:19:38</oasis:entry>
         <oasis:entry colname="col2">1048</oasis:entry>
         <oasis:entry colname="col3">204.5</oasis:entry>
         <oasis:entry colname="col4">0.1</oasis:entry>
         <oasis:entry colname="col5">70.4</oasis:entry>
         <oasis:entry colname="col6">39.2</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">2020-11-18T02:03:10</oasis:entry>
         <oasis:entry colname="col2">105c</oasis:entry>
         <oasis:entry colname="col3">98.7</oasis:entry>
         <oasis:entry colname="col4">5</oasis:entry>
         <oasis:entry colname="col5">146.2</oasis:entry>
         <oasis:entry colname="col6">52.6</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">2020-11-29T01:51:59</oasis:entry>
         <oasis:entry colname="col2">1010</oasis:entry>
         <oasis:entry colname="col3">98.0</oasis:entry>
         <oasis:entry colname="col4">5</oasis:entry>
         <oasis:entry colname="col5">143.8</oasis:entry>
         <oasis:entry colname="col6">48.8</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">2020-12-24T02:21:12</oasis:entry>
         <oasis:entry colname="col2">1069</oasis:entry>
         <oasis:entry colname="col3">261.0</oasis:entry>
         <oasis:entry colname="col4">3</oasis:entry>
         <oasis:entry colname="col5">149.9</oasis:entry>
         <oasis:entry colname="col6">49.4</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">2021-04-01T02:16:14</oasis:entry>
         <oasis:entry colname="col2">241c</oasis:entry>
         <oasis:entry colname="col3">99.1</oasis:entry>
         <oasis:entry colname="col4">2</oasis:entry>
         <oasis:entry colname="col5">106.1</oasis:entry>
         <oasis:entry colname="col6">66.2</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">2021-04-02T02:13:12</oasis:entry>
         <oasis:entry colname="col2">1105</oasis:entry>
         <oasis:entry colname="col3">168.7</oasis:entry>
         <oasis:entry colname="col4">0.1</oasis:entry>
         <oasis:entry colname="col5">104.3</oasis:entry>
         <oasis:entry colname="col6">65.6</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">2021-04-02T01:54:40</oasis:entry>
         <oasis:entry colname="col2">1013</oasis:entry>
         <oasis:entry colname="col3">276.8</oasis:entry>
         <oasis:entry colname="col4">5</oasis:entry>
         <oasis:entry colname="col5">101.2</oasis:entry>
         <oasis:entry colname="col6">60.8</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">2021-04-11T01:33:11</oasis:entry>
         <oasis:entry colname="col2">2276</oasis:entry>
         <oasis:entry colname="col3">98.6</oasis:entry>
         <oasis:entry colname="col4">4.1</oasis:entry>
         <oasis:entry colname="col5">93.2</oasis:entry>
         <oasis:entry colname="col6">57.7</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">2021-04-12T02:15:35</oasis:entry>
         <oasis:entry colname="col2">227c</oasis:entry>
         <oasis:entry colname="col3">98.4</oasis:entry>
         <oasis:entry colname="col4">4.9</oasis:entry>
         <oasis:entry colname="col5">96.1</oasis:entry>
         <oasis:entry colname="col6">68.1</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">2021-06-05T01:51:14</oasis:entry>
         <oasis:entry colname="col2">1038</oasis:entry>
         <oasis:entry colname="col3">98.2</oasis:entry>
         <oasis:entry colname="col4">4.9</oasis:entry>
         <oasis:entry colname="col5">63.9</oasis:entry>
         <oasis:entry colname="col6">61.7</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">2021-06-10T23:23:03</oasis:entry>
         <oasis:entry colname="col2">1049</oasis:entry>
         <oasis:entry colname="col3">84.5</oasis:entry>
         <oasis:entry colname="col4">3</oasis:entry>
         <oasis:entry colname="col5">70</oasis:entry>
         <oasis:entry colname="col6">27.5</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">2021-07-08T02:15:18</oasis:entry>
         <oasis:entry colname="col2">2274</oasis:entry>
         <oasis:entry colname="col3">12.8</oasis:entry>
         <oasis:entry colname="col4">0.2</oasis:entry>
         <oasis:entry colname="col5">61.7</oasis:entry>
         <oasis:entry colname="col6">65.1</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">2021-07-11T01:26:43</oasis:entry>
         <oasis:entry colname="col2">2434</oasis:entry>
         <oasis:entry colname="col3">277.1</oasis:entry>
         <oasis:entry colname="col4">5</oasis:entry>
         <oasis:entry colname="col5">68.8</oasis:entry>
         <oasis:entry colname="col6">54.1</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup><?xmltex \end{scaleboxenv}?></oasis:table><?xmltex \gdef\@currentlabel{1}?></table-wrap>

      <p id="d1e1291">The image pairs were coregistered to a Sentinel-2 basemap using the global coregistration function of the Automated and Robust Open-Source Image Co-Registration Software (AROSICS) <xref ref-type="bibr" rid="bib1.bibx78" id="paren.55"/> to increase the registration accuracy while preserving the deformation signal. The pairs were clipped to their overlapping extents with a Universal Transverse Mercator (UTM) projection and either an 8- or a 16-bit integer pixel data type as required by MicMac. Manual cloud masking was accomplished using the <monospace>saisiemasqQT</monospace> binary of MicMac for precision masking.</p>
      <p id="d1e1300">Correlations in the spatial domain were performed with MicMac on the prepared image pairs using the following parameters: <list list-type="bullet"><list-item>
      <p id="d1e1305"><inline-formula><mml:math id="M37" display="inline"><mml:mrow><mml:mn mathvariant="normal">7</mml:mn><mml:mo>×</mml:mo><mml:mn mathvariant="normal">7</mml:mn></mml:mrow></mml:math></inline-formula> window size (SzW <inline-formula><mml:math id="M38" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 3) for a 21.875 m search grid on each side to compensate for feature-related noise and expected displacement,</p></list-item><list-item>
      <?pagebreak page1140?><p id="d1e1327">0.5 regularization factor (Reg <inline-formula><mml:math id="M39" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 0.5) to provide distance-based correlation weights on the neighboring pixels within the window for noise reduction, and, <?xmltex \hack{\newpage}?></p></list-item><list-item>
      <p id="d1e1339">pixel subsampling parameter of 2 (SsResolOpt <inline-formula><mml:math id="M40" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 2) as recommended by <xref ref-type="bibr" rid="bib1.bibx25" id="text.56"/> for earthquake events to resolve displacement fields close to the ground resolution of the source imagery.</p></list-item></list></p>
      <p id="d1e1352">The resulting output files were georeferenced using <monospace>gdal_translate</monospace> with the <monospace>-a_ullr</monospace> flag <xref ref-type="bibr" rid="bib1.bibx41" id="paren.57"/> to ensure a <inline-formula><mml:math id="M41" display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>:</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> alignment with the input image pairs without warping the rasters. To retain most deformation signals, the correlation threshold was set to 50 %. A non-local median (NLM) filter with a low H-noise value was applied to prevent flattening real ground deformation signals while improving the signal-to-noise ratio (SNR). The outputs were then translated into the spatial domain by multiplying the rasters with the ground resolution of the input files. The rasters chosen to extract profiles and calculate fault-parallel offsets were selected based on noise levels, atmospheric obstruction, pre-processing accuracy, ROI coverage, and quality of slip visualization (Sect. S1.1 in the Supplement).</p>
      <p id="d1e1376">The post-processed data generated coherent pixel offset maps along the N–S (<inline-formula><mml:math id="M42" display="inline"><mml:mrow><mml:msub><mml:mi>D</mml:mi><mml:mrow><mml:msub><mml:mi mathvariant="normal">N</mml:mi><mml:mi mathvariant="normal">OIC</mml:mi></mml:msub></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>) and E–W (<inline-formula><mml:math id="M43" display="inline"><mml:mrow><mml:msub><mml:mi>D</mml:mi><mml:mrow><mml:msub><mml:mi mathvariant="normal">E</mml:mi><mml:mi mathvariant="normal">OIC</mml:mi></mml:msub></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>) horizontal axes with a 3.125 m pixel resolution. Slip measurements with respect to the general fault strike azimuth (<inline-formula><mml:math id="M44" display="inline"><mml:mrow><mml:mi mathvariant="italic">θ</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">325</mml:mn></mml:mrow></mml:math></inline-formula>°) of the Masbate segment were acquired by transposing the N–S and E–W slip into fault-oriented components using the following equations <xref ref-type="bibr" rid="bib1.bibx34" id="paren.58"/>:

                <disp-formula specific-use="align" content-type="numbered"><mml:math id="M45" display="block"><mml:mtable displaystyle="true"><mml:mlabeledtr id="Ch1.E1"><mml:mtd><mml:mtext>1</mml:mtext></mml:mtd><mml:mtd><mml:mstyle displaystyle="true" class="stylechange"/></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:msub><mml:mi>D</mml:mi><mml:mo>∥</mml:mo></mml:msub><mml:mo>=</mml:mo><mml:msub><mml:mi>D</mml:mi><mml:mrow><mml:msub><mml:mi mathvariant="normal">N</mml:mi><mml:mi mathvariant="normal">OIC</mml:mi></mml:msub></mml:mrow></mml:msub><mml:mo>⋅</mml:mo><mml:mi>cos⁡</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="italic">θ</mml:mi><mml:mo>)</mml:mo><mml:mo>+</mml:mo><mml:msub><mml:mi>D</mml:mi><mml:mrow><mml:msub><mml:mi mathvariant="normal">E</mml:mi><mml:mi mathvariant="normal">OIC</mml:mi></mml:msub></mml:mrow></mml:msub><mml:mo>⋅</mml:mo><mml:mi>sin⁡</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="italic">θ</mml:mi><mml:mo>)</mml:mo><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E2"><mml:mtd><mml:mtext>2</mml:mtext></mml:mtd><mml:mtd><mml:mstyle class="stylechange" displaystyle="true"/></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:msub><mml:mi>D</mml:mi><mml:mo>⟂</mml:mo></mml:msub><mml:mo>=</mml:mo><mml:msub><mml:mi>D</mml:mi><mml:mrow><mml:msub><mml:mi mathvariant="normal">N</mml:mi><mml:mi mathvariant="normal">OIC</mml:mi></mml:msub></mml:mrow></mml:msub><mml:mo>⋅</mml:mo><mml:mi>sin⁡</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="italic">θ</mml:mi><mml:mo>)</mml:mo><mml:mo>-</mml:mo><mml:msub><mml:mi>D</mml:mi><mml:mrow><mml:msub><mml:mi mathvariant="normal">E</mml:mi><mml:mi mathvariant="normal">OIC</mml:mi></mml:msub></mml:mrow></mml:msub><mml:mo>⋅</mml:mo><mml:mi>cos⁡</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="italic">θ</mml:mi><mml:mo>)</mml:mo><mml:mo>.</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr></mml:mtable></mml:math></disp-formula>

            Measurements were acquired by taking profiles of the pixel offset data across the fault to determine the net fault-parallel offset (Sect. S1.2). The fault-parallel (<inline-formula><mml:math id="M46" display="inline"><mml:mrow><mml:msub><mml:mi>D</mml:mi><mml:mo>∥</mml:mo></mml:msub></mml:mrow></mml:math></inline-formula>) direction refers to movements parallel to the fault trace represented by laterally offset features on the field. This component was the sole subject of profiling due to the stronger horizontal offset signal in the field. The tension–compression (<inline-formula><mml:math id="M47" display="inline"><mml:mrow><mml:msub><mml:mi>D</mml:mi><mml:mo>⟂</mml:mo></mml:msub></mml:mrow></mml:math></inline-formula>) aspect detectable from the fault-normal component was not analyzed due to the minimal deformation along the vertical axis, further complicated by high noise amplitudes.</p>
      <p id="d1e1571">Wide swath profiles (<inline-formula><mml:math id="M48" display="inline"><mml:mrow><mml:mn mathvariant="normal">321</mml:mn><mml:mo>×</mml:mo><mml:mn mathvariant="normal">161</mml:mn></mml:mrow></mml:math></inline-formula> px, roughly <inline-formula><mml:math id="M49" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">1.0</mml:mn><mml:mo>×</mml:mo><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">0.5</mml:mn></mml:mrow></mml:math></inline-formula> km) along the fault trace were acquired with StackProf <xref ref-type="bibr" rid="bib1.bibx74" id="paren.59"/> developed for the MicMac project. The slip values from profiles aided in the measurement of the near-fault slip distribution for comparison with offsets measured in the field. The displacements were calculated from the intercepts of the regression of weighted median offsets across the fault trace. We used the coherence values to remove zero correlation pixels to highlight the genuine earthquake slip in the arctangent model. We selected the regression limits by hand to exclude areas of decorrelation, apparent noise signals, and obvious spurious pixel offset data that remained after filtering. As a result, most regression lines were limited to 300–600 m across the fault trace. Validated slip data were plotted along the fault strike to show the spatial trends.</p>
      <p id="d1e1606"><?xmltex \hack{\newpage}?>Absolute standard deviations (<inline-formula><mml:math id="M50" display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mi mathvariant="italic">σ</mml:mi></mml:mrow></mml:math></inline-formula>) from the weighted median values across the transect indicate the measurement uncertainties in individual box profiles. The individual slip uncertainties are the sum of the standard errors of intercepts of the regression of the eastern and western blocks <xref ref-type="bibr" rid="bib1.bibx74" id="paren.60"/>. The displacement curve was calculated using a robust weighted moving mean approach with minimal smoothing (<inline-formula><mml:math id="M51" display="inline"><mml:mrow><mml:mi>q</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.15</mml:mn></mml:mrow></mml:math></inline-formula>) to prevent the removal of small deviations along the strike.</p>
</sec>
<sec id="Ch1.S3.SS3">
  <label>3.3</label><title>Small baseline subset interferometry</title>
      <p id="d1e1643">Coseismic and post-seismic interferograms were processed with NASA's Alaska Satellite Facility Distributed Active Archive Center (ASF DAAC) Hybrid Pluggable Processing Pipeline (HyP3) <xref ref-type="bibr" rid="bib1.bibx49" id="paren.61"/>. Sentinel-1A/B single look complex (SLC) C-band radar data acquired through the interferometric wide (IW) swath mode were used. Data with 6–12 d intervals from paths 61 (descending track) and 69 (ascending track) (Fig. <xref ref-type="fig" rid="Ch1.F1"/>d) imaged from 14 to 21 August 2020 for the coseismic slip and 20 August to 20 September 2020 for the afterslip were multilooked by 20 in the azimuth direction and 4 in the range resulting in a pixel size of <inline-formula><mml:math id="M52" display="inline"><mml:mrow><mml:mn mathvariant="normal">80</mml:mn><mml:mo>×</mml:mo><mml:mn mathvariant="normal">80</mml:mn></mml:mrow></mml:math></inline-formula> m to minimize the effect of land cover (Table <xref ref-type="table" rid="Ch1.T2"/>).</p>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T2" specific-use="star"><?xmltex \currentcnt{2}?><label>Table 2</label><caption><p id="d1e1668">Summary of reference and secondary scenes processed within Alaska Satellite Facility's Hyp3 processor to create interferograms.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="8">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="center"/>
     <oasis:colspec colnum="3" colname="col3" align="right"/>
     <oasis:colspec colnum="4" colname="col4" align="center"/>
     <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="left"/>
     <oasis:thead>
       <oasis:row>
         <oasis:entry colname="col1">Track</oasis:entry>
         <oasis:entry colname="col2">Reference</oasis:entry>
         <oasis:entry colname="col3">Path/frame 1</oasis:entry>
         <oasis:entry colname="col4">Secondary</oasis:entry>
         <oasis:entry colname="col5">Path/frame 2</oasis:entry>
         <oasis:entry colname="col6">Perp.</oasis:entry>
         <oasis:entry colname="col7">Interval</oasis:entry>
         <oasis:entry colname="col8">Seismic</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2"/>
         <oasis:entry colname="col3"/>
         <oasis:entry colname="col4"/>
         <oasis:entry colname="col5"/>
         <oasis:entry colname="col6">baseline</oasis:entry>
         <oasis:entry colname="col7">(days)</oasis:entry>
         <oasis:entry colname="col8">stage</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2"/>
         <oasis:entry colname="col3"/>
         <oasis:entry colname="col4"/>
         <oasis:entry colname="col5"/>
         <oasis:entry colname="col6">(m)</oasis:entry>
         <oasis:entry colname="col7"/>
         <oasis:entry colname="col8"/>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>
         <oasis:entry colname="col1">Desc</oasis:entry>
         <oasis:entry colname="col2">20200814</oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M53" display="inline"><mml:mrow><mml:mn mathvariant="normal">61</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">551</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4">20200820</oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M54" display="inline"><mml:mrow><mml:mn mathvariant="normal">61</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">54</mml:mn></mml:mrow></mml:math></inline-formula>9</oasis:entry>
         <oasis:entry colname="col6"><inline-formula><mml:math id="M55" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">76.4</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col7">6</oasis:entry>
         <oasis:entry colname="col8">Co</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Asc</oasis:entry>
         <oasis:entry colname="col2">20200815</oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M56" display="inline"><mml:mrow><mml:mn mathvariant="normal">69</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">32</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4">20200821</oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M57" display="inline"><mml:mrow><mml:mn mathvariant="normal">69</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">34</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col6">107.1</oasis:entry>
         <oasis:entry colname="col7">6</oasis:entry>
         <oasis:entry colname="col8">Co</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Desc</oasis:entry>
         <oasis:entry colname="col2">20200820</oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M58" display="inline"><mml:mrow><mml:mn mathvariant="normal">61</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">549</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4">20200901</oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M59" display="inline"><mml:mrow><mml:mn mathvariant="normal">61</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">549</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col6">50.4</oasis:entry>
         <oasis:entry colname="col7">12</oasis:entry>
         <oasis:entry colname="col8">Post</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Asc</oasis:entry>
         <oasis:entry colname="col2">20200821</oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M60" display="inline"><mml:mrow><mml:mn mathvariant="normal">69</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">34</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4">20200827</oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M61" display="inline"><mml:mrow><mml:mn mathvariant="normal">69</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">32</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col6"><inline-formula><mml:math id="M62" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">173.3</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col7">6</oasis:entry>
         <oasis:entry colname="col8">Post</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Desc</oasis:entry>
         <oasis:entry colname="col2">20200826</oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M63" display="inline"><mml:mrow><mml:mn mathvariant="normal">61</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">551</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4">20200901</oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M64" display="inline"><mml:mrow><mml:mn mathvariant="normal">61</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">549</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col6"><inline-formula><mml:math id="M65" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">76.4</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col7">6</oasis:entry>
         <oasis:entry colname="col8">Post</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Asc</oasis:entry>
         <oasis:entry colname="col2">20200827</oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M66" display="inline"><mml:mrow><mml:mn mathvariant="normal">69</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">32</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4">20200902</oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M67" display="inline"><mml:mrow><mml:mn mathvariant="normal">69</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">34</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col6">126.0</oasis:entry>
         <oasis:entry colname="col7">6</oasis:entry>
         <oasis:entry colname="col8">Post</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Asc</oasis:entry>
         <oasis:entry colname="col2">20200827</oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M68" display="inline"><mml:mrow><mml:mn mathvariant="normal">69</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">32</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4">20200908</oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M69" display="inline"><mml:mrow><mml:mn mathvariant="normal">69</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">32</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col6">42.6</oasis:entry>
         <oasis:entry colname="col7">12</oasis:entry>
         <oasis:entry colname="col8">Post</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Desc</oasis:entry>
         <oasis:entry colname="col2">20200901</oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M70" display="inline"><mml:mrow><mml:mn mathvariant="normal">61</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">549</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4">20200907</oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M71" display="inline"><mml:mrow><mml:mn mathvariant="normal">61</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">551</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col6">49.6</oasis:entry>
         <oasis:entry colname="col7">6</oasis:entry>
         <oasis:entry colname="col8">Post</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Desc</oasis:entry>
         <oasis:entry colname="col2">20200901</oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M72" display="inline"><mml:mrow><mml:mn mathvariant="normal">61</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">549</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4">20200913</oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M73" display="inline"><mml:mrow><mml:mn mathvariant="normal">61</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">549</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col6">68.5</oasis:entry>
         <oasis:entry colname="col7">12</oasis:entry>
         <oasis:entry colname="col8">Post</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Asc</oasis:entry>
         <oasis:entry colname="col2">20200902</oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M74" display="inline"><mml:mrow><mml:mn mathvariant="normal">69</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">34</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4">20200908</oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M75" display="inline"><mml:mrow><mml:mn mathvariant="normal">69</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">32</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col6"><inline-formula><mml:math id="M76" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">83.1</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col7">6</oasis:entry>
         <oasis:entry colname="col8">Post</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Asc</oasis:entry>
         <oasis:entry colname="col2">20200908</oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M77" display="inline"><mml:mrow><mml:mn mathvariant="normal">69</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">32</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4">20200920</oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M78" display="inline"><mml:mrow><mml:mn mathvariant="normal">69</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">32</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col6">49.9</oasis:entry>
         <oasis:entry colname="col7">12</oasis:entry>
         <oasis:entry colname="col8">Post</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Desc</oasis:entry>
         <oasis:entry colname="col2">20200913</oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M79" display="inline"><mml:mrow><mml:mn mathvariant="normal">61</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">549</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4">20200919</oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M80" display="inline"><mml:mrow><mml:mn mathvariant="normal">61</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">551</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col6"><inline-formula><mml:math id="M81" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">39.4</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col7">6</oasis:entry>
         <oasis:entry colname="col8">Post</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table><?xmltex \gdef\@currentlabel{2}?></table-wrap>

      <p id="d1e2390">Small baseline time series analysis (SBAS) was employed using MintPy <xref ref-type="bibr" rid="bib1.bibx103" id="paren.62"/> to quantify the post-seismic deformation in the aftershock observation period. Atmospheric corrections were not applied, since the study area is highly localized relative to the global dataset implemented in available databases. Furthermore, the unwrapping reference point was set to a common high coherence pixel for both tracks. The ascending (<inline-formula><mml:math id="M82" display="inline"><mml:mrow><mml:msub><mml:mi>V</mml:mi><mml:mi mathvariant="normal">A</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) and descending (<inline-formula><mml:math id="M83" display="inline"><mml:mrow><mml:msub><mml:mi>V</mml:mi><mml:mi mathvariant="normal">D</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) LOS velocities were projected into the azimuthal fault strike (<inline-formula><mml:math id="M84" display="inline"><mml:mrow><mml:mi mathvariant="italic">θ</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">325</mml:mn></mml:mrow></mml:math></inline-formula>°) <xref ref-type="bibr" rid="bib1.bibx32 bib1.bibx55 bib1.bibx91" id="paren.63"/> to estimate the fault-parallel (<inline-formula><mml:math id="M85" display="inline"><mml:mrow><mml:msub><mml:mi>V</mml:mi><mml:mrow><mml:mo>|</mml:mo><mml:mo>|</mml:mo></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>) and vertical (<inline-formula><mml:math id="M86" display="inline"><mml:mrow><mml:msub><mml:mi>V</mml:mi><mml:mi>Z</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) post-seismic velocities. The approach assumes a zero third component acceptable for areas of relatively simple faulting. Equation (<xref ref-type="disp-formula" rid="Ch1.E3"/>) was used to derive the fault-oriented afterslip LOS velocities within the <monospace>asc_desc2horz_vert</monospace> script in MintPy. The pixel unit vector directed to the satellite was decomposed into <inline-formula><mml:math id="M87" display="inline"><mml:mi>e</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math id="M88" display="inline"><mml:mi>n</mml:mi></mml:math></inline-formula>, and <inline-formula><mml:math id="M89" display="inline"><mml:mi>u</mml:mi></mml:math></inline-formula> representing the east, north, and upward directions of both tracks, respectively:
            <disp-formula id="Ch1.E3" content-type="numbered"><label>3</label><mml:math id="M90" display="block"><mml:mrow><mml:mfenced open="[" close="]"><mml:mtable class="matrix" columnalign="center" framespacing="0em"><mml:mtr><mml:mtd><mml:mrow><mml:msub><mml:mi>V</mml:mi><mml:mi mathvariant="normal">A</mml:mi></mml:msub></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mrow><mml:msub><mml:mi>V</mml:mi><mml:mi mathvariant="normal">D</mml:mi></mml:msub></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:mfenced><mml:mo>=</mml:mo><mml:mfenced open="[" close="]"><mml:mtable class="matrix" columnalign="center center" framespacing="0em"><mml:mtr><mml:mtd><mml:mrow><mml:msub><mml:mi>e</mml:mi><mml:mi mathvariant="normal">A</mml:mi></mml:msub><mml:mi>sin⁡</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="italic">θ</mml:mi><mml:mo>)</mml:mo><mml:mo>+</mml:mo><mml:msub><mml:mi>n</mml:mi><mml:mi mathvariant="normal">A</mml:mi></mml:msub><mml:mi>cos⁡</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="italic">θ</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:msub><mml:mi>u</mml:mi><mml:mi mathvariant="normal">A</mml:mi></mml:msub></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mrow><mml:msub><mml:mi>e</mml:mi><mml:mi mathvariant="normal">D</mml:mi></mml:msub><mml:mi>sin⁡</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="italic">θ</mml:mi><mml:mo>)</mml:mo><mml:mo>+</mml:mo><mml:msub><mml:mi>n</mml:mi><mml:mi mathvariant="normal">D</mml:mi></mml:msub><mml:mi>cos⁡</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="italic">θ</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:msub><mml:mi>u</mml:mi><mml:mi mathvariant="normal">D</mml:mi></mml:msub></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:mfenced><mml:mfenced close="]" open="["><mml:mtable class="matrix" columnalign="center" framespacing="0em"><mml:mtr><mml:mtd><mml:mrow><mml:msub><mml:mi>V</mml:mi><mml:mo>∥</mml:mo></mml:msub></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mrow><mml:msub><mml:mi>V</mml:mi><mml:mi>Z</mml:mi></mml:msub></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:mfenced><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula>
          The total afterslip was obtained by multiplying the fault-parallel component with the temporal range of the time series, and the data were smoothed using an NLM filter to arrest pixel outliers. Swath profiles <xref ref-type="bibr" rid="bib1.bibx50" id="paren.64"/> were taken at 0.5 km intervals with a 3.5 km swath width across the fault strike (Sect. S4.1). We determined the across-fault <inline-formula><mml:math id="M91" display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mi mathvariant="italic">σ</mml:mi></mml:mrow></mml:math></inline-formula> uncertainties from the absolute deviation from the weighted median in each swath. Slip uncertainty estimates come from the sum of the standard error of regression intercepts of the<?pagebreak page1141?> eastern and western blocks, following the StackProf approach <xref ref-type="bibr" rid="bib1.bibx74" id="paren.65"/>. Similar to optical correlation, the regression lines for the eastern and western blocks were manually delimited in order to exclude the remaining phase unwrapping artifacts and other noise signals.</p>
      <p id="d1e2627">The spatial distribution of the afterslip along the strike was evaluated using a smoothed moving mean displacement curve (<inline-formula><mml:math id="M92" display="inline"><mml:mrow><mml:mi>q</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.15</mml:mn></mml:mrow></mml:math></inline-formula>). The vertical post-seismic displacement was not investigated due to the primarily horizontal ground movement. The coseismic interferogram was limited to qualitative comparisons with optical correlation. No quantifiable comparisons can be made since slip is unresolved in the near-fault region as a result of decorrelation due to high magnitudes of coseismic slip.</p>
</sec>
<sec id="Ch1.S3.SS4">
  <label>3.4</label><title>Ground truthing</title>
      <p id="d1e2651">Field investigation was conducted from 18 to 21 May 2022 to identify and measure the horizontal offsets across the ground rupture. Locations of known ground rupture (Ronald dela Cruz, personal communication, 2022) were complemented by points of interest identified from the image correlation outputs and InSAR. Due to the 2-year interval between the earthquake and fieldwork, geomorphic or human modifications of offset features may have occurred. Additionally, many offsets and evidence of surface rupture may have been erased given the small magnitude of surface slip. The significance of these changes can be assessed by correlating field data with other measurement techniques to determine the slip.</p>
      <p id="d1e2654">We selected points of interest for field checking based on the pixel offset rasters, prioritizing locations with significant contrast along the approximate and certain fault traces. Field offsets were measured with a steel tape and structural orientations were determined with a base plate compass. Measurements of on-fault offsets were limited to individual rupture strands. Due to the scarcity of remnant ruptures, most sites had a single measurement. Uncertainty was estimated by comparing values at these locations to earlier measurements acquired a week after the earthquake <xref ref-type="bibr" rid="bib1.bibx70 bib1.bibx63" id="paren.66"/>. In areas with complex, closely spaced ruptures, multiple measurements were acquired and statistically assessed to estimate the uncertainty.</p>
      <p id="d1e2660">Observation points with measurable feature offset and ruptures were plotted along the strike to show the attitude and slip distribution along the fault (Sect. S2). The measured horizontal offsets were used to validate the results of the remote sensing analysis. Finally, the maximum and average displacements, as well as the surface rupture length were derived from the conjoined remote sensing outputs and field data to estimate the seismic moment.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3" specific-use="star"><?xmltex \currentcnt{3}?><?xmltex \def\figurename{Figure}?><label>Figure 3</label><caption><p id="d1e2666">Panel <bold>(a)</bold> is an earthquake probability density subplot showing the normalized population of earthquakes per day, highlighting the contrast between the periods of the earthquake sequence. Panel <bold>(b)</bold> is a plot showing the number of earthquakes with magnitudes <inline-formula><mml:math id="M93" display="inline"><mml:mrow><mml:mi>M</mml:mi><mml:mo>≥</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> related to the Masbate segment and their temporal distribution relative to the 18 August 2020 mainshock.</p></caption>
          <?xmltex \igopts{width=398.338583pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/24/1135/2024/nhess-24-1135-2024-f03.png"/>

        </fig>

</sec>
</sec>
<sec id="Ch1.S4">
  <label>4</label><title>Results</title>
<sec id="Ch1.S4.SS1">
  <label>4.1</label><title>Seismicity</title>
<sec id="Ch1.S4.SS1.SSS1">
  <label>4.1.1</label><title>Earthquake frequency and temporal relationships</title>
      <p id="d1e2716">The frequency–time distribution of earthquakes between 25 August 2019 and 18 August 2021 shows the immediate seismicity related to the 18 August 2020 <inline-formula><mml:math id="M94" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">w</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> 6.6 event (Fig. <xref ref-type="fig" rid="Ch1.F3"/>). The foreshocks, mainshock, and aftershocks are identifiable in the probability density subplot (Fig. <xref ref-type="fig" rid="Ch1.F3"/>a) as a distinct bell-shaped curve relative to the generally quiescent background activity. The island of Masbate typically experiences less than 10 earthquakes per day, corresponding to a moderate background seismicity. An increase in earthquake frequency defines the foreshock sequence <xref ref-type="bibr" rid="bib1.bibx38" id="paren.67"/> at around 32 d before the mainshock, as shown by the distinct trend increase in the probability density subplot. The peaks of the frequency plots (Fig. <xref ref-type="fig" rid="Ch1.F3"/>a and b)<?pagebreak page1142?> correspond to 141 earthquakes which were mostly aftershocks on 18 August 2020. A negative slope in the probability density subplot depicts the aftershock sequence. The decaying earthquake frequency is initially symmetrical to the foreshock trend with an inflection point around 30 d after the mainshock, which transitioned to a more gradual decrease. The aftershocks persisted for 166 d or up to 31 January 2021. The succeeding return to background levels saw a similar seismic activity to the previous background activity from 2019 to early 2020.</p>
</sec>
<sec id="Ch1.S4.SS1.SSS2">
  <label>4.1.2</label><title>Spatiotemporal earthquake distribution</title>
      <p id="d1e2747">In general, the background seismicity (<inline-formula><mml:math id="M95" display="inline"><mml:mrow><mml:mi>M</mml:mi><mml:mo>≤</mml:mo><mml:mn mathvariant="normal">4</mml:mn></mml:mrow></mml:math></inline-formula>) is well distributed throughout the overall length of the Masbate segment of the PF traversing the islands of Ticao and Burias, as well as the provincial mainland (Fig. <xref ref-type="fig" rid="Ch1.F4"/>a). However, an absence of seismic activity is noticeable in the northern portion of the fault in mainland Masbate during this period. On the contrary, an earthquake cluster occurred near the location of the mainshock. Foreshock activity is concentrated in southeastern Masbate adjacent to the mainshock and is composed of mostly weak (<inline-formula><mml:math id="M96" display="inline"><mml:mi>M</mml:mi></mml:math></inline-formula> 2–3) and shallow hypocenters peaking at <inline-formula><mml:math id="M97" display="inline"><mml:mi>M</mml:mi></mml:math></inline-formula> 4.9 (Fig. <xref ref-type="fig" rid="Ch1.F4"/>b).</p>

      <?xmltex \floatpos{p}?><fig id="Ch1.F4" specific-use="star"><?xmltex \currentcnt{4}?><?xmltex \def\figurename{Figure}?><label>Figure 4</label><caption><p id="d1e2782">Spatiotemporal earthquake distribution for the Masbate segment: <bold>(a)</bold> background seismicity between 25 August 2019 and 10 July 2020; <bold>(b)</bold> foreshocks from 19 July to 17 August 2020; <bold>(c)</bold> moment tensors of the mainshock from GlobalCMT, PHIVOLCS, and USGS; <bold>(d)</bold> same-day aftershocks; <bold>(e)</bold> first-month aftershocks from 19 August to 17 September 2020; <bold>(f)</bold> second-month aftershocks from 18 September to 17 October 2020; <bold>(g)</bold> third-month aftershocks from 19 October to 16 November 2020; <bold>(h)</bold> fourth-month aftershocks from 18 November to 14 December 2020; <bold>(i)</bold> last aftershocks from 22 December 2020 to 31 January 2021; and <bold>(j)</bold> return to background seismicity covering 9 February to 18 August 2021.</p></caption>
            <?xmltex \igopts{width=426.791339pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/24/1135/2024/nhess-24-1135-2024-f04.png"/>

          </fig>

      <p id="d1e2822">Three moment tensor solutions from GlobalCMT, PHIVOLCS, and USGS highlight the mainshock's dominant left-lateral strike-slip movement (Fig. <xref ref-type="fig" rid="Ch1.F4"/>c). The solutions of PHIVOLCS and USGS show a noticeable, albeit minimal, dip-slip component toward the NNE. The epicentral location of the mainshock from GlobalCMT and PHIVOLCS coincided with the fault trace, while USGS' focal mechanism solution deviated to the northeast of the fault.</p>
      <p id="d1e2828">Aftershocks that transpired on the same day as the mainshock (Fig. <xref ref-type="fig" rid="Ch1.F4"/>d) are shallow (1–30 km) and densely grouped in the southeastern offshore extension of the segment and deepen (10–50 km) as they taper toward the onshore portion. The aftershocks have weak magnitudes ranging from <inline-formula><mml:math id="M98" display="inline"><mml:mi>M</mml:mi></mml:math></inline-formula> 2.0 to <inline-formula><mml:math id="M99" display="inline"><mml:mi>M</mml:mi></mml:math></inline-formula> 4.4. Succeeding first-month aftershocks are weak to moderate, with a wide range of magnitudes between <inline-formula><mml:math id="M100" display="inline"><mml:mi>M</mml:mi></mml:math></inline-formula> 1.7 and <inline-formula><mml:math id="M101" display="inline"><mml:mi>M</mml:mi></mml:math></inline-formula> 5.1, mostly occurring at depths above 30 km. A monthly progressive dispersal of hypocenters in space is also observed, with the first month showing a dense cluster in the southeastern section that tapers to the northwest (Fig. <xref ref-type="fig" rid="Ch1.F4"/>e). The pattern and geographic extent of the first-month aftershocks appear to be an expansion of the same-day aftershocks. The succession of the aftershock patterns in the following months continued to scatter along the Masbate segment and the SSF while retaining a perceptible concentration in the offshore southeastern extension of the causative fault segment (Fig. <xref ref-type="fig" rid="Ch1.F4"/>f–i). The last 2 months of aftershock activity (Fig. <xref ref-type="fig" rid="Ch1.F4"/>h and i) feature the least number of hypocenters throughout the aftershock sequence.</p>
      <p id="d1e2868">Background levels returned on 2 February 2021 defined by the well-distributed hypocenters on the fault segments with moderate magnitudes (Fig. <xref ref-type="fig" rid="Ch1.F4"/>j) similar to the pre-event seismicity in 2019 (Fig. <xref ref-type="fig" rid="Ch1.F4"/>a). The frequency and distribution of earthquakes in time and space enabled the distinction of various stages of the earthquake sequence relative to the 2020 Masbate event.</p>
</sec>
</sec>
<?pagebreak page1144?><sec id="Ch1.S4.SS2">
  <label>4.2</label><title>Optical image correlation</title>
<sec id="Ch1.S4.SS2.SSS1">
  <label>4.2.1</label><title>Long and short temporal baseline</title>
      <p id="d1e2891">The acquired pixel offset maps (Fig. <xref ref-type="fig" rid="Ch1.F5"/>) illustrate the fault rupture and the known left-lateral movement of the Masbate segment, despite the presence of noise that obscures portions of the rupture. Only one of the eight image pairs from the short time span spaced months apart (Fig. <xref ref-type="fig" rid="Ch1.F2"/>a) produced outputs with perceptible rupture due to the low SNR. Annual time-span pairs resolved the rupture more clearly compared with the short time-span image pairs. The north–south slip components show better representations of the rupture, whereas the east–west components tend to be noisier. Nevertheless, the valid image pairs (Sect. S1.1) with resolvable slip and subjected to stack profiling exhibit reliable estimates of the slip in the near-field region.</p>

      <?xmltex \floatpos{p}?><fig id="Ch1.F5" specific-use="star"><?xmltex \currentcnt{5}?><?xmltex \def\figurename{Figure}?><label>Figure 5</label><caption><p id="d1e2900">Optical correlation results showing the representative data from the 9 April 2020 and 2 April 2021 image pair. Blue lines in <bold>(e)</bold> and <bold>(g)</bold> are the absolute median fault-parallel values across the profile box. Gray shaded region in <bold>(e)</bold> and <bold>(g)</bold> feature the <inline-formula><mml:math id="M102" display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mi mathvariant="italic">σ</mml:mi></mml:mrow></mml:math></inline-formula> absolute standard deviation of the fault-parallel values across the fault in each box. Panel <bold>(a)</bold> shows the N–S component. Blue refers to southward movement and yellow refers to northward motion. Panel <bold>(b)</bold> shows the E–W component. Blue refers to westward movement and yellow refers to eastward motion. Panel <bold>(c)</bold> shows the fault-parallel component. Pink refers to movements toward the NW and blue denotes motion toward the SE. Panel <bold>(d)</bold> is a closer view of box 32 showing the fault-parallel offset. Panel <bold>(e)</bold> shows a swath profile of box 32 highlighting the 43 cm slip. Lower regression intercept of the western block relative to the eastern block indicates left-lateral movement. Panel <bold>(f)</bold> is a closer view of box 47 displaying the fault-parallel offset in Cataingan. Panel <bold>(g)</bold> shows a swath profile of box 47 exhibiting the peak 59.2 cm left-lateral offset in this particular image pair.</p></caption>
            <?xmltex \igopts{width=426.791339pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/24/1135/2024/nhess-24-1135-2024-f05.jpg"/>

          </fig>

</sec>
<sec id="Ch1.S4.SS2.SSS2">
  <label>4.2.2</label><title>Horizontal ground displacements</title>
      <p id="d1e2962">A generalized fault trace (yellow line in Fig. <xref ref-type="fig" rid="Ch1.F5"/>) was delineated from the valid pixel offset rasters and the known fault trace, which served as the baseline for slip profiling. The fault trace is mostly straight, except for an apparent northeasterly strike rotation toward the north, where it follows the piedmont of a topographic high in Dimasalang. No measurements were acquired in the area due to anomalously high values, which are probably terrain residuals. Topographic artifacts and decreasing slip away from the epicenter posed difficulties in delineating the northern rupture section near Naro Bay. In the southwestern section,the offset rasters show a new splay striking NW–SE that bisects the previously recognized bifurcation in Cataingan. The rupture traverses the deltaic area and possibly continues southward across Cataingan Bay, then resurfaces on the opposite side of the bay. Smaller fractures and minute rupture components are not visible due to ubiquitous noise.</p>
      <p id="d1e2967">Left-lateral offsets were quantified along the <inline-formula><mml:math id="M103" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">25</mml:mn></mml:mrow></mml:math></inline-formula> km onshore length of the fault from Dimasalang to Cataingan, given the inland spatial extents and continuity where optical correlation was feasible. Edge artifacts and the obscured western block in the south of the bay hindered the acquisition of slip profiles.</p>
      <p id="d1e2980">A total of 51 wide swath profile boxes were generated throughout the fault rupture, with the first box in Dimasalang and the last in Cataingan to determine the along-strike-slip distribution (Fig. <xref ref-type="fig" rid="Ch1.F6"/>). The optical correlation results generated a total of 126 left-lateral measurements over six image pairs (Sect. S1.2). Using a 325° general strike azimuth of the Masbate segment, the east–west and north–south displacement components (Fig. <xref ref-type="fig" rid="Ch1.F5"/>a and b) were transposed into the fault-parallel direction (Fig. <xref ref-type="fig" rid="Ch1.F5"/>c).</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="d1e2992">Along-strike distribution of the fault-parallel offsets from 126 profile boxes across six image pairs. Error bars refer to the <inline-formula><mml:math id="M104" display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mi mathvariant="italic">σ</mml:mi></mml:mrow></mml:math></inline-formula> sum of standard errors of the intercepts of regressions of the eastern and western blocks providing slip uncertainty estimates.</p></caption>
            <?xmltex \igopts{width=455.244094pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/24/1135/2024/nhess-24-1135-2024-f06.png"/>

          </fig>

      <p id="d1e3011">The 9 April 2020 to 2 April  2021 pair was selected as the representative dataset due to its wide spatial extent and reliable representation of the fault rupture. The north–south component (Fig. <xref ref-type="fig" rid="Ch1.F5"/>a) shows a continuous linear rupture trace from Dimasalang to the deltaic area in Cataingan, although the Dimasalang area and its border with Palanas exhibited unusually high values due to topographic artifacts. The east–west component (Fig. <xref ref-type="fig" rid="Ch1.F5"/>b) is less coherent, likely due to smaller ground movements in this direction or overprinted data from the noise. The outputs show noise from both artificial and environmental sources, represented by topographic artifacts in the southwestern block, an apparent seamline, and reduced coherence due to differences in land cover between the images. Nevertheless, the fault-parallel component (Fig. <xref ref-type="fig" rid="Ch1.F5"/>c) shows good estimates of the left-lateral slip, further supported by the near-field offset models.</p>
      <p id="d1e3020">Box 32 (Fig. <xref ref-type="fig" rid="Ch1.F5"/>d), located <inline-formula><mml:math id="M105" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">6</mml:mn></mml:mrow></mml:math></inline-formula> km north of the GlobalCMT surface projection, shows a 43 cm slip in the near field (Fig. <xref ref-type="fig" rid="Ch1.F5"/>e). Pixel offset values increase in the far field for the western block, which may either represent noise or distributed deformation. Box 47, situated <inline-formula><mml:math id="M106" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">1.5</mml:mn></mml:mrow></mml:math></inline-formula> km south of the GlobalCMT epicenter, exhibits a 59.2 cm left-lateral offset. The box represents the peak offset in this image pair and displays a clear contrast between the eastern and western blocks.</p>
      <p id="d1e3047">The plot of the slip distribution along strike (Fig. <xref ref-type="fig" rid="Ch1.F6"/>) displays the 126 left-lateral offsets compiled from the valid offset rasters to characterize the displacement field. The slip minima ranges from 6 to 9 cm, located 4.5 km from the northern shoreline in Dimasalang. The displacement increased to <inline-formula><mml:math id="M107" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">50</mml:mn></mml:mrow></mml:math></inline-formula> cm around the vicinity of the GlobalCMT projection of the centroid. Slip values remained constant within a <inline-formula><mml:math id="M108" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">5</mml:mn></mml:mrow></mml:math></inline-formula> km span in Cataingan and increased to a peak <inline-formula><mml:math id="M109" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">60</mml:mn></mml:mrow></mml:math></inline-formula> cm at around <inline-formula><mml:math id="M110" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> km southeast of the centroid. South of the peak value, the displacement declines toward the shoreline. The skewed semi-elliptical weighted moving mean curve (solid gray line in Fig. <xref ref-type="fig" rid="Ch1.F6"/>) shows the average left-lateral offset of <inline-formula><mml:math id="M111" display="inline"><mml:mrow><mml:mn mathvariant="normal">37.7</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">10</mml:mn></mml:mrow></mml:math></inline-formula> cm, while the individual measurements indicate a peak <inline-formula><mml:math id="M112" display="inline"><mml:mrow><mml:mn mathvariant="normal">60.6</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">9.8</mml:mn></mml:mrow></mml:math></inline-formula> cm offset adjacent to the surface projection of the centroid in Cataingan.</p>
</sec>
</sec>
<sec id="Ch1.S4.SS3">
  <label>4.3</label><title>Interferometry</title>
<sec id="Ch1.S4.SS3.SSS1">
  <label>4.3.1</label><title>Coseismic interferograms</title>
      <p id="d1e3135">The Sentinel-1 coseismic wrapped interferograms in the ascending and descending tracks (Fig. <xref ref-type="fig" rid="Ch1.F7"/>a and c) show the butterfly-shaped fringe patterns and oppositely verging LOS displacements, both of which are typical of strike-slip events. The fringe lobe patterns illustrate a range increase from the ascending track and a range decrease from the descending track for the western side of the fault. Since the orbit of the ascending track is subparallel to the regional fault strike, the left-lateral movement is indicated with a possible subsidence component. This is consistent with the moment tensor solutions (Fig. <xref ref-type="fig" rid="Ch1.F4"/>c) and agrees with the sense of movement shown by the optical correlation outputs and field observations.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F7" specific-use="star"><?xmltex \currentcnt{7}?><?xmltex \def\figurename{Figure}?><label>Figure 7</label><caption><p id="d1e3144">Sentinel-1 coseismic interferograms in ascending and descending tracks: <bold>(a)</bold> wrapped ascending interferogram, <bold>(b)</bold> unwrapped LOS displacement in the ascending track, <bold>(c)</bold> wrapped descending track interferogram, and <bold>(d)</bold> unwrapped LOS displacement in the descending track.</p></caption>
            <?xmltex \igopts{width=398.338583pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/24/1135/2024/nhess-24-1135-2024-f07.jpg"/>

          </fig>

      <?pagebreak page1147?><p id="d1e3165">Low phase coherence persists in the near-fault region. Widespread decorrelation leads to mostly unusable information upon phase unwrapping due to the likelihood of creating unwrapping errors. Noise is similarly dominant and overprints most of the deformation signals in an approximately 18 km-wide region across the fault trace, hence, the lack of near-fault information in preliminary published interferograms <xref ref-type="bibr" rid="bib1.bibx70 bib1.bibx84" id="paren.68"/>. In addition, the rupture is unresolved upon phase unwrapping (Fig. <xref ref-type="fig" rid="Ch1.F7"/>b and d) due to decorrelation. This loss of resolvable information in the near field ultimately hinders slip measurements in the coseismic interferograms.</p>
</sec>
<sec id="Ch1.S4.SS3.SSS2">
  <label>4.3.2</label><title>Post-seismic deformation estimates</title>
      <p id="d1e3181">Post-seismic interferograms capture an improved overall manifestation of the fault rupture compared with the coseismic ones (Fig. <xref ref-type="fig" rid="Ch1.F8"/>). This is a consequence of the expected smaller afterslip values relative to the coseismic slip, which decreases the number of fringes and increases the coherence. The temporal coverage of the interferogram stack allows us to quantify afterslip to complement the estimated coseismic slip from optical correlation. However, the first post-earthquake Sentinel-1 revisit occurred 2 d after the mainshock, resulting in all measurements to be lower-bound estimates of the afterslip.</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="d1e3188">Post-seismic deformation between 20 August and 20 September 2020. Panel <bold>(a)</bold> is the ascending track time series showing range increase (yellow) and decrease (blue) for the eastern and western blocks, respectively. Panel <bold>(b)</bold> is the descending track time series showing range decrease (blue) and increase (yellow) for the eastern and western blocks, respectively. Panel <bold>(c)</bold> shows the projected fault-parallel post-seismic deformation field. Panel <bold>(d)</bold> shows the fault-parallel afterslip for box 4 in Dimasalang indicating the 5.4 cm left-lateral afterslip. Lower regression intercept of the western block relative to the eastern block indicates left-lateral movement. Median afterslip value is shown by the blue line. Gray background exhibits the <inline-formula><mml:math id="M113" display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mi mathvariant="italic">σ</mml:mi></mml:mrow></mml:math></inline-formula> uncertainty across the box. Panel <bold>(e)</bold> shows the swath profile of box 13 indicating an 8.4 cm left-lateral afterslip around the Dimasalang–Palanas boundary. Panel <bold>(f)</bold> is the swath profile of box 25 showing a 6.9 cm afterslip in Palanas. Panel <bold>(g)</bold> is the swath profile of box 39 in Cataingan showing a 12.0 cm left-lateral afterslip.</p></caption>
            <?xmltex \igopts{width=455.244094pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/24/1135/2024/nhess-24-1135-2024-f08.jpg"/>

          </fig>

      <p id="d1e3229">Unwrapping errors are less frequent on the ascending and descending track interferograms and are further minimized upon time-series stacking. The remaining phase unwrapping errors upon stacking and filtering were manually excluded in profiling. These unwrapping errors occur as significant high amplitude phase shifts and polarity reversals, noticeable in the Dimasalang and Palanas areas.</p>
      <p id="d1e3233">The fault-parallel afterslip deformation field (Fig. <xref ref-type="fig" rid="Ch1.F8"/>c) shows a strongly linear and simple fault trace that accommodated the post-seismic deformation. Deviations from the regional fault strike are observed around 5–13 km from Naro Bay in the north, represented by multiple short NNE–SSW oriented (<inline-formula><mml:math id="M114" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">290</mml:mn></mml:mrow></mml:math></inline-formula>–300° azimuth) bends which are adjacent to and coincide with the narrow stepover in the Palanas–Dimasalang area. However, the noticeable unwrapping errors and low ground resolution (80 m) precludes the validity and recognition of these rupture complexities.</p>
      <p id="d1e3248">The afterslip is resolved from Naro Bay in the north toward Cataingan Bay in the south along the <inline-formula><mml:math id="M115" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">25</mml:mn></mml:mrow></mml:math></inline-formula> km simplified fault trace (Sect. S4.1). A total of 49 swath profile boxes were generated along this trace. Individual measurements reveal centimetric fault-parallel afterslip with minimal across-fault variability and minor <inline-formula><mml:math id="M116" display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mi mathvariant="italic">σ</mml:mi></mml:mrow></mml:math></inline-formula> uncertainties, except where the boxes overlap with the phase unwrapping error patches. The deformation was detected up to the far-field extents of the profiles from most swath boxes.</p>
      <p id="d1e3271">Boxes 4, 13, 25, and 39 (Fig. <xref ref-type="fig" rid="Ch1.F8"/>d–g) illustrate select wide swath profiles roughly equidistant from each other. Box 4, situated in Dimasalang, shows a 5.4 cm left-lateral fault-parallel afterslip and reasonably low variability across the fault. Unwrapping errors in the far field at 1.5 km from the fault on both sides caused irregularities in the profile. Box 13, located around the boundary of Palanas and Dimasalang, depicts an 8.4 cm fault-parallel slip. Both sides of the fault exhibit exceedingly even slip across the fault, except for a noticeable dip in the eastern edge. The dip is likely due to data loss since the box overlapped with the water body to the east. The profile also appears to be offset by about <inline-formula><mml:math id="M117" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">100</mml:mn></mml:mrow></mml:math></inline-formula> m to the west, which corresponds to one of the abovementioned bends that may be an unwrapping artifact. Still, the measured slip from the arctangent model remains valid. Box 25 shows a 6.9 cm afterslip in Palanas, located at the southern edge of the fault complexity. Multiple across-fault deviations are visible around 200 and 500 m east of the fault, as well as in the western far field. The eastern anomalies could either be unwrapping or topography related, while the western patch comes from unwrapping issues. Box 39 in Cataingan displays a 12.0 cm left-lateral afterslip with good symmetry and even across-fault distribution.</p>
      <p id="d1e3286">The along-strike afterslip distribution graph (Fig. <xref ref-type="fig" rid="Ch1.F9"/>) depicts the computed fault-parallel offsets from north to south on the mainland. The smallest value is measured in Dimasalang, adjacent to Naro Bay, amounting to 4.3 cm of left-lateral afterslip. The ground offsets exhibit a generally increasing trend to around <inline-formula><mml:math id="M118" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">5</mml:mn></mml:mrow></mml:math></inline-formula> km from the north. Fluctuating values are observed between 6.1 to 13.8 km from the north in Dimasalang and Palanas. The measured displacements oscillate between 5.0 and 9.6 cm in this span. The increasing trend continued to a <inline-formula><mml:math id="M119" display="inline"><mml:mrow><mml:mn mathvariant="normal">14.3</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">0.9</mml:mn></mml:mrow></mml:math></inline-formula> cm peak value in Cataingan, located 24 km from Naro Bay and <inline-formula><mml:math id="M120" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:math></inline-formula> km southwest of the GlobalCMT surface projection. The displacements decrease from the largest value to 11.5 cm on the shoreline of Cataingan Bay. The weighted moving mean curve (solid blue line in Fig. <xref ref-type="fig" rid="Ch1.F9"/>) indicates a mean left-lateral afterslip of at least <inline-formula><mml:math id="M121" display="inline"><mml:mrow><mml:mn mathvariant="normal">8.8</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">0.7</mml:mn></mml:mrow></mml:math></inline-formula> cm.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F9" specific-use="star"><?xmltex \currentcnt{9}?><?xmltex \def\figurename{Figure}?><label>Figure 9</label><caption><p id="d1e3340">Along-strike distribution of the fault-parallel afterslip formed by the 49 profile boxes. Error bars refer to the <inline-formula><mml:math id="M122" display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mi mathvariant="italic">σ</mml:mi></mml:mrow></mml:math></inline-formula> standard errors of the intercepts of regressions of the eastern and western blocks. Solid blue line shows the weighted moving mean afterslip curve.</p></caption>
            <?xmltex \igopts{width=455.244094pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/24/1135/2024/nhess-24-1135-2024-f09.png"/>

          </fig>

</sec>
</sec>
<sec id="Ch1.S4.SS4">
  <label>4.4</label><title>Ground truthing</title>
<sec id="Ch1.S4.SS4.SSS1">
  <label>4.4.1</label><title>Observed surface ruptures</title>
      <p id="d1e3375">Remnant effects after about 2 years post-earthquake were observed on laterally offset cultural and geomorphic features from Dimasalang to Cataingan following the known fault trace (Sect. S2). Assisted by the remote sensing data, the observed ground manifestation of the earthquake from 57 stations (Fig. <xref ref-type="fig" rid="Ch1.F10"/>a and b) include fractures, reported earthquake-induced landslides (EIL), indications of liquefaction features and lateral spreading, secondary gravitational features, and ruptures with quantifiable displacements. Earthquake effects recorded during the field activity include reported ground shaking from interviews with locals.</p>

      <?xmltex \floatpos{p}?><fig id="Ch1.F10" specific-use="star"><?xmltex \currentcnt{10}?><?xmltex \def\figurename{Figure}?><label>Figure 10</label><caption><p id="d1e3382">Compiled ground-truthing data: <bold>(a)</bold> earthquake hazards aside from ruptures, <bold>(b)</bold> ruptures symbolized by size showing the amount of slip, <bold>(c)</bold> rupture orientations, <bold>(d)</bold> ruptured tree showing cumulative 87 cm slip from 2003 and 2020 events with estimated <inline-formula><mml:math id="M123" display="inline"><mml:mrow><mml:mn mathvariant="normal">27</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">10</mml:mn></mml:mrow></mml:math></inline-formula> cm offset from the 2020 earthquake, <bold>(e)</bold> soil mound cut by the fault highlighting a <inline-formula><mml:math id="M124" display="inline"><mml:mrow><mml:mn mathvariant="normal">48</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:math></inline-formula> cm left-lateral offset, <bold>(f)</bold> rice field embankment traversed by fault showing <inline-formula><mml:math id="M125" display="inline"><mml:mrow><mml:mn mathvariant="normal">60</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">15</mml:mn></mml:mrow></mml:math></inline-formula> cm displacement, <bold>(g)</bold> ruptured fishpond dike recording a <inline-formula><mml:math id="M126" display="inline"><mml:mrow><mml:mn mathvariant="normal">34</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">5</mml:mn></mml:mrow></mml:math></inline-formula> cm offset, and <bold>(h)</bold> abandoned septic tank showing a 30 cm displacement south of Cataingan Bay.</p></caption>
            <?xmltex \igopts{width=398.338583pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/24/1135/2024/nhess-24-1135-2024-f10.jpg"/>

          </fig>

      <?pagebreak page1149?><p id="d1e3465">The observed rupture zone of the 2020 Masbate earthquake persisted from Dimasalang to Cataingan and crossed Cataingan Bay. Measured surface ruptures strike at a low angle with respect to the regional fault trace (Fig. <xref ref-type="fig" rid="Ch1.F10"/>c) with a mean strike azimuth of 313°. Our northernmost resolvable ground offset was observed on a road in Dimasalang, around <inline-formula><mml:math id="M127" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:math></inline-formula> km from Naro Bay. An apparent 0.5 cm offset fracture oriented parallel to the fault trace was recorded in this point, possibly representing the minimum northward constraint of the field rupture. A 2–5 cm displacement oriented 325° NW occurring on a residential structure on top of the fault was observed on the border between Dimasalang and Palanas. The rupture displacement increased further south <inline-formula><mml:math id="M128" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">7</mml:mn></mml:mrow></mml:math></inline-formula> km from the northern shoreline, where a 7 cm left-lateral offset was seen coupled with spreading of the road pavement. The fault bisected a coconut tree at the southern limit of the fault complexity in Palanas (Fig. <xref ref-type="fig" rid="Ch1.F10"/>d) <xref ref-type="bibr" rid="bib1.bibx7" id="paren.69"/>, resulting in a cumulative 87 cm opening from the 2003 and 2020 events. The newer slip is estimated at <inline-formula><mml:math id="M129" display="inline"><mml:mrow><mml:mn mathvariant="normal">27</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">10</mml:mn></mml:mrow></mml:math></inline-formula> cm on a 275° W-oriented rupture. Right-stepping en echelon fractures occurred adjacent to the coconut tree, most of which were eroded at the time of visit.</p>
      <p id="d1e3509">The rupture is continuous southward, up to 4 km from the GlobalCMT centroid projection. The fault rupture traversed an abandoned house and deflected its wall by roughly <inline-formula><mml:math id="M130" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">50</mml:mn></mml:mrow></mml:math></inline-formula> cm. A soil mound at the base of the wall (Fig. <xref ref-type="fig" rid="Ch1.F10"/>e) shows a 297° W-oriented rupture with a <inline-formula><mml:math id="M131" display="inline"><mml:mrow><mml:mn mathvariant="normal">48</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:math></inline-formula> cm left-lateral offset. Residents reported a <inline-formula><mml:math id="M132" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">200</mml:mn></mml:mrow></mml:math></inline-formula> m-long rupture in the area, which was already mostly eroded. Nevertheless, the remnant right-stepping en echelon fractures formed a linear rupture zone connected to the displaced wall. A 30 cm offset oriented 279° E on a road in Cataingan likely represents the northern indication of the rupture bisecting the bifurcation in Cataingan. The rupture continued to an agricultural area (Fig. <xref ref-type="fig" rid="Ch1.F10"/>f), where the embankments are displaced by <inline-formula><mml:math id="M133" display="inline"><mml:mrow><mml:mn mathvariant="normal">60</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">15</mml:mn></mml:mrow></mml:math></inline-formula> cm, representing the peak field offset measurements. Long, continuous ruptures were observed on the rice fields immediately after the event but were erased by the time of the field investigation. Another southerly continuation was identified, where a 341° NW-oriented rupture displaced fishpond levees (Fig. <xref ref-type="fig" rid="Ch1.F10"/>g) by about <inline-formula><mml:math id="M134" display="inline"><mml:mrow><mml:mn mathvariant="normal">34</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">5</mml:mn></mml:mrow></mml:math></inline-formula> cm. Locals stated that the visible rupture appeared lengthy and continuous in the deltaic areas immediately after the earthquake. The rupture was evident again south of Cataingan Bay, manifested on a collinear set of points through several residential structures. A septic tank diagonally cut by a 279° NW-oriented rupture shows a 30 cm left-lateral displacement (Fig. <xref ref-type="fig" rid="Ch1.F10"/>h). Offset measurements adjacent to the septic tank vary from 5 to 30 cm.</p>
</sec>
<sec id="Ch1.S4.SS4.SSS2">
  <label>4.4.2</label><title>Left-lateral offset distribution</title>
      <p id="d1e3585">The plot of offset features along the fault strike (Fig. <xref ref-type="fig" rid="Ch1.F11"/>) and shows the minimum 0.5 cm left-lateral displacement <inline-formula><mml:math id="M135" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:math></inline-formula> km from Naro Bay in Dimasalang. This point corresponds to the northernmost resolvable ground offset. The measurements continually increased to 50 cm beginning at 17 km from Naro Bay, around the boundary of Palanas and Cataingan. The offset measurements remained constant for a <inline-formula><mml:math id="M136" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">4</mml:mn></mml:mrow></mml:math></inline-formula> km span followed by an abrupt dip to 30 cm, which increased again to the peak 60 cm offset. The local 30 cm minimum was measured on a ruptured road. This single discordant measurement could be due to off-fault displacement, physical reduction due to post-earthquake repairs, or an inaccurate measurement from a cultural feature. The displacement tapered to 30 cm near the shoreline of Cataingan Bay. Spatially coincident offsets ranging from 5 to 30 cm resulted in a wide range of uncertainties at the southeastern limitation of the plot. The weighted moving mean curve of the slip distribution (broken red line in Fig. <xref ref-type="fig" rid="Ch1.F11"/>) for the 2020 Masbate event indicates a 25.3 cm mean left-lateral displacement, while the individual observations denote the maximum of 60 cm displacement near the GlobalCMT centroid projection.</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="d1e3614">Along-strike distribution of measured field offsets acquired in May 2022.</p></caption>
            <?xmltex \igopts{width=455.244094pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/24/1135/2024/nhess-24-1135-2024-f11.png"/>

          </fig>

<?xmltex \hack{\newpage}?>
</sec>
</sec>
</sec>
<?pagebreak page1151?><sec id="Ch1.S5">
  <label>5</label><title>Discussion</title>
<sec id="Ch1.S5.SS1">
  <label>5.1</label><title>Comparison of optical correlation and InSAR</title>
<sec id="Ch1.S5.SS1.SSS1">
  <label>5.1.1</label><title>Displacement threshold</title>
      <p id="d1e3650">Independently applying optical correlation and interferometry to analyze the 2020 Masbate event provided a basis to assess the technical capabilities and shortcomings of the methods in a tropical setting. Peak displacements of the Masbate earthquake amount to <inline-formula><mml:math id="M137" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">60</mml:mn></mml:mrow></mml:math></inline-formula> cm, denoting a high interferometric phase gradient for Sentinel-1. SAR interferograms lose coherence when offsets exceed half the interferometric fringe per pixel <xref ref-type="bibr" rid="bib1.bibx60" id="paren.70"/>, highlighting the effectiveness of the method for small deformations on millimeter and centimeter scales <xref ref-type="bibr" rid="bib1.bibx87" id="paren.71"/>. The LOS measurements of <xref ref-type="bibr" rid="bib1.bibx70" id="text.72"/> and <xref ref-type="bibr" rid="bib1.bibx84" id="text.73"/> from coseismic interferograms are likely underestimated due to data loss because of the high phase gradients and near-field decorrelation on the coseismic interferograms (Fig. <xref ref-type="fig" rid="Ch1.F7"/>).</p>
      <p id="d1e3678">The ability of InSAR to detect centimetric displacements was evident when comparing the post-seismic and coseismic interferograms. The rupture trace is conspicuous and the offset is observable in both the near field and far field of the post-seismic interferograms. Left-lateral afterslip measurements are at least 4–14 cm with an average 1<inline-formula><mml:math id="M138" display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula> uncertainty of 1.5 cm. Millimeter-scale offsets were not detected given the coarse 80 m pixel resolution and noise of the resultant interferograms.</p>
      <p id="d1e3688">Optical correlation is useful to assess the near-field region <xref ref-type="bibr" rid="bib1.bibx12" id="paren.74"/> and larger displacements equivalent to at least one-tenth of the pixel resolution <xref ref-type="bibr" rid="bib1.bibx35 bib1.bibx54" id="paren.75"/>. Results show that near-field displacements are resolved (Figs. <xref ref-type="fig" rid="Ch1.F5"/> and <xref ref-type="fig" rid="Ch1.F6"/>) despite noticeable high noise levels. OIC, using PlanetScope data with 3.125 m pixel resolution, was able to detect left-lateral offsets between 7 and 60 cm in the near field but with a larger 19.9 cm <inline-formula><mml:math id="M139" display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mi mathvariant="italic">σ</mml:mi></mml:mrow></mml:math></inline-formula> average uncertainty than InSAR due to noise. Thus, careful interpretation of swath profiles is crucial to identify valid measurements because noise easily overprints tectonic signals. Noise signals are amplified by misaligned acquisition geometry, unequal solar illumination angle, and insufficient geometric corrections <xref ref-type="bibr" rid="bib1.bibx35 bib1.bibx83" id="paren.76"/>. The representative 9 April 2020 to 2 April 2021 (satellite ID 1105) images had decent illumination and acquisition geometry agreement (Table <xref ref-type="table" rid="Ch1.T1"/>), and support the validity of the measurements.</p>
</sec>
<sec id="Ch1.S5.SS1.SSS2">
  <label>5.1.2</label><title>Temporal baseline</title>
      <p id="d1e3725">The pair classes of PlanetScope orthoimages used in the study showed that images roughly 1 year apart resolved the rupture far better than those imaged months apart primarily due to the contrasting vegetative cover. Satellite images from the same seasons are critical for optical correlation because feature similarity helps the algorithm match features more accurately <xref ref-type="bibr" rid="bib1.bibx34" id="paren.77"/>. Feature matching in agricultural and developing areas can be difficult in the subpixel domain given the difference in crop patterns and rapid anthropogenic development, leading to differing pixel intensity values in the pre-event and post-event images <xref ref-type="bibr" rid="bib1.bibx15" id="paren.78"/>.</p>
      <p id="d1e3734">Images that are 1 d apart generate deformation fields with minimal seasonal and anthropogenic artifacts. However, this may have exceptions such that correlations for the 2016 Fukushima earthquake using 1 d interval drone images resulted in noisy deformation fields with low correlation (Sotiris Valkaniotis, personal communication, 2021). Single-day intervals were not tested in Masbate due to the lack of usable orthoimagery in terms of study area coverage, compatible acquisition parameters, and cloud cover.</p>
      <?pagebreak page1152?><p id="d1e3737">DInSAR relies on coherence to resolve the deformation along the LOS direction, which is controlled by the similarity of point scatterers between the acquisitions. Good coherence in urban areas and dry deserts that remain constant throughout several years produce quality interferograms <xref ref-type="bibr" rid="bib1.bibx94 bib1.bibx97" id="paren.79"/>, which indicate the capability of interferometry to function for longer periods. However, in other types of surface cover, such as vegetation and snow, coherence has an inverse relationship with temporal 6 d revisit of Sentinel-1 conveniently dictating the pre-event and post-event radar data pairing in areas affected by sub-optimal land cover. The baseline can be increased for L-band satellites, such as ALOS-2, for they can detect the bare ground irrespective of surface cover. Interferograms with severe unwrapping errors are manually excluded in the time-series analysis <xref ref-type="bibr" rid="bib1.bibx103" id="paren.80"/>, effectively limiting the temporal baseline range to 6–12 d.</p>
</sec>
</sec>
<sec id="Ch1.S5.SS2">
  <label>5.2</label><title>Accuracy of optical correlation</title>
      <p id="d1e3755">The slip distribution from optical correlation agrees with the offset feature measurements from the field survey (Fig. <xref ref-type="fig" rid="Ch1.F12"/>a). The weighted moving mean of the pixel offset measurements unifies the six valid pairs to compensate for data gaps that particular pairs are unable to resolve. The variance between the pixel offsets and field measures is typically <inline-formula><mml:math id="M140" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> cm with a maximum <inline-formula><mml:math id="M141" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">17</mml:mn></mml:mrow></mml:math></inline-formula> cm. The larger difference is interpreted to be a local variation or measurement error since the specific point was taken on a repaired road section, which the remote sensing approach may have missed as it generally detects the overall deformation and is less sensitive to local slip.</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="d1e3782">Combined slip distribution plots: <bold>(a)</bold> solid gray line shows the weighted moving mean of the six valid optical correlation pairs, dashed red line represents the weighted moving mean of the field measurements, and blue line as well as markers represent the afterslip from InSAR placed in a secondary axis; <bold>(b)</bold> residual curves of the weighted moving mean pixel offsets and field measurements with InSAR to estimate the coseismic slip.</p></caption>
          <?xmltex \igopts{width=455.244094pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/24/1135/2024/nhess-24-1135-2024-f12.png"/>

        </fig>

      <p id="d1e3797">Previous studies show varying degrees of misfit between field offsets and remote sensing data <xref ref-type="bibr" rid="bib1.bibx27 bib1.bibx42" id="paren.81"/>. These misfits were attributed to diffuse displacement, secondary faulting, and shallow fault complexities. Our measurements, however, show consistency and minimal short wavelength variability. This may be a consequence of the 2-year interval between the earthquake event and the field survey as most surface traces have been modified by active surface processes. Furthermore, ruptures on unconsolidated overburden are easily erased due to active weathering and erosion, leaving only the most prominent traces to remain. Similarly, abundant vegetation, challenging surface conditions, and relatively small tectonic displacements compromise the clarity of the resolved rupture and efficacy of optical correlation. Nevertheless, OIC outputs indicate that the remote sensing results accurately capture ground displacements and provide greater along-strike coverage.</p>
      <p id="d1e3804">The extent of detectable rupture is another fundamental difference between optical correlation outputs and field measurements. The northern rupture terminations are situated 4.6 and 3.2 km from Naro Bay for optical correlation and field survey, respectively. To the south, OIC measurements cease at the shore of Cataingan Bay since no slip measurements are attainable on the opposite side of the water body, where the field survey revealed more ruptures as the fault resurfaced therein. Neither method can resolve slip on submerged fault segments, requiring the use of complementary marine survey techniques and datasets that cover the ocean floor.</p><?xmltex \hack{\newpage}?>
</sec>
<sec id="Ch1.S5.SS3">
  <label>5.3</label><title>Surface rupture kinematics</title>
<sec id="Ch1.S5.SS3.SSS1">
  <label>5.3.1</label><title>Constraining the coseismic slip</title>
      <p id="d1e3823">The temporal range of the pixel offset rasters and field investigation date implies the presence of both coseismic and post-seismic slip components in the optical correlation measurements and field measurements. To estimate the peak coseismic offsets, we subtracted the largest afterslip value from the peak pixel offsets and field measures. The average values were derived from the mean of residuals of the moving mean curves of the two total slip measures with InSAR (Fig. <xref ref-type="fig" rid="Ch1.F12"/>b). From this, the estimated peak coseismic slip amounts to <inline-formula><mml:math id="M142" display="inline"><mml:mrow><mml:mn mathvariant="normal">46.3</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">10.7</mml:mn></mml:mrow></mml:math></inline-formula> cm from the optical correlation and <inline-formula><mml:math id="M143" display="inline"><mml:mrow><mml:mn mathvariant="normal">45.7</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">15.9</mml:mn></mml:mrow></mml:math></inline-formula> cm from the field measure residuals. The average values are 27.7 and 24.3 cm from pixel offsets and field measures, respectively.</p>
</sec>
<sec id="Ch1.S5.SS3.SSS2">
  <label>5.3.2</label><title>Coseismic offsets</title>
      <p id="d1e3860">The amount of coseismic slip is a key factor in the assessment of seismic moment, rupture mechanism, and degree of seismic hazard. The results of this study show a unimodal curve with a characteristic long wavelength and isolated short wavelength variability for the regional slip distribution (Fig. <xref ref-type="fig" rid="Ch1.F12"/>). The pattern suggests a low generalized resolution due to temporally influenced smoothing and noise. In addition, the long wavelength trend can also indicate fault maturity <xref ref-type="bibr" rid="bib1.bibx1" id="paren.82"/>, which is a credible interpretation for the Masbate segment of the PF given its Middle Miocene initiation and rate of activity <xref ref-type="bibr" rid="bib1.bibx39 bib1.bibx89 bib1.bibx71" id="paren.83"/>. Moreover, the known fault trace in Masbate is morphologically linear, supporting the general maturity estimate <xref ref-type="bibr" rid="bib1.bibx58" id="paren.84"/>.</p>
      <p id="d1e3874">Slip distributions can give clues into the fault complexity and mechanical properties of the fault plane <xref ref-type="bibr" rid="bib1.bibx1 bib1.bibx23 bib1.bibx67" id="paren.85"/>. This suggests that the observed unimodal slip distribution with a singular peak implies a relatively simple fault zone at depth, subject to validation through geodetic inversion. Such peaks usually define the location of the ruptured asperity <xref ref-type="bibr" rid="bib1.bibx48" id="paren.86"/> where the highest stress drop occurs due to peak moment release from the accumulated potential energy <xref ref-type="bibr" rid="bib1.bibx40" id="paren.87"/>.</p>
      <p id="d1e3886">Our seismotectonic interpretations (Sect. 5.4) imply a variable slip distribution on the submerged sections of the Masbate segment of the PF since it represents the primary depression of the identified transtensional basin. This inferred slip trend may portray a complex shallow fault structure in this section as the slip is distributed on multiple fault segments <xref ref-type="bibr" rid="bib1.bibx12 bib1.bibx1 bib1.bibx96" id="paren.88"/>. Moreover, recent marine geophysical surveys in the vicinity of Cataingan Bay <xref ref-type="bibr" rid="bib1.bibx56" id="paren.89"/> revealed the<?pagebreak page1153?> geometric complexity of the fault, which supports our interpretation.</p>
      <p id="d1e3895">Offset values gradually decay to zero toward the northwest. The smooth slip trend, devoid of short wavelength variation, suggests a systematic rupture <xref ref-type="bibr" rid="bib1.bibx86" id="paren.90"/> on a relatively simple sub-vertical fault plane <xref ref-type="bibr" rid="bib1.bibx1 bib1.bibx28" id="paren.91"/>. Tapering and deepening aftershock patterns along with the focal mechanism solutions could support this observation.</p>
</sec>
<sec id="Ch1.S5.SS3.SSS3">
  <label>5.3.3</label><title>Post-seismic offsets</title>
      <p id="d1e3912">Our interferometry results denote a 14 cm largest afterslip, which accounts for at least 30 % of the estimated peak coseismic displacement over the rapid aftershock decay interval. This lower-limit estimate is a consequence of the 6 d revisit cycle of Sentinel-1, resulting in incomplete data since the first radar image in the time-series stack was from 20 August 2020, and does not include the earliest post-seismic deformation immediately after the 18 August 2020 mainshock.</p>
      <p id="d1e3915">The distribution of afterslip (Fig. <xref ref-type="fig" rid="Ch1.F12"/>) along the fault demonstrates a general slip increase southwards, which can be divided into two distinct sections. The northern <inline-formula><mml:math id="M144" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">15</mml:mn></mml:mrow></mml:math></inline-formula> km section is characterized by short wavelength variations and average left-lateral offsets of 5–6 cm, whereas the southern section includes the peak afterslip without distinctive variability. The northern trend may indicate the occurrence of diffuse afterslip on a wide zone, which may or may not have breached the surface. <xref ref-type="bibr" rid="bib1.bibx28" id="text.92"/> suggested an increased relative friction such that the released post-seismic moment is typically less compared with the mainshock, resulting in heterogeneous loading. However, we cannot exclude the possibility that variability may stem from surface complexities or data processing artifacts, as indicated by the observed unwrapping errors and the lack of data from the earliest post-seismic period.</p>
      <p id="d1e3933">Post-seismic deformation usually occurs outside the regions of peak coseismic slip as the shear stress is transferred by the mainshock and causes stress loading at the locations of incomplete rupture and unruptured sections <xref ref-type="bibr" rid="bib1.bibx47 bib1.bibx24" id="paren.93"/>. Our results reflect the coincidence of the post-seismic and coseismic slip distributions on the surface, whose maxima are aligned and equidistant from<?pagebreak page1154?> the centroid, accompanied by a gradual slip recession northwards (Fig. <xref ref-type="fig" rid="Ch1.F12"/>). This is similar to the 1999 Izmit <xref ref-type="bibr" rid="bib1.bibx76" id="paren.94"/>, 1996 Biak <xref ref-type="bibr" rid="bib1.bibx30" id="paren.95"/>, 2011 Maduo <xref ref-type="bibr" rid="bib1.bibx95" id="paren.96"/>, and 2014 South Napa <xref ref-type="bibr" rid="bib1.bibx31" id="paren.97"/> earthquakes, which also exhibit spatially overlapping coseismic and post-seismic slip distributions. We interpret this overlap of the slip distributions to indicate a vertical stress migration along the fault surface to either deeper or shallower sections of the fault.</p>
      <p id="d1e3954">Aseismic afterslip, viscoelastic relaxation, and poroelastic rebound are the common mechanisms of post-seismic deformation <xref ref-type="bibr" rid="bib1.bibx44 bib1.bibx85" id="paren.98"/>. The existence of resolvable afterslip is a clear indication of post-seismic activity as the stress is released by the mainshock. Our observed coincidence of the coseismic and post-seismic slip distributions probably indicates a localized stress transfer to the adjacent velocity strengthening vicinity of the primary asperity in accordance with the rate-and-state friction model <xref ref-type="bibr" rid="bib1.bibx59" id="paren.99"/>. This would suggest that the post-seismic deformation is likely stress driven <xref ref-type="bibr" rid="bib1.bibx44" id="paren.100"/> and operated as aseismic afterslip <xref ref-type="bibr" rid="bib1.bibx47" id="paren.101"/> to accommodate the excess coseismic stress. This also agrees with the hypothesized vertical migration of stress along the fault plane.</p>
      <p id="d1e3970">We recognize that the data are limited to surface measurements and more information is required to accurately describe the occurrence of the afterslip along the fault plane. Determining the mechanics of the superposed slip character of the 2020 Masbate earthquake event is of interest and warrants investigation into potential factors such as non-steady-state friction <xref ref-type="bibr" rid="bib1.bibx45" id="paren.102"/>, residual stress heterogeneity <xref ref-type="bibr" rid="bib1.bibx95" id="paren.103"/>, stress reorganization, or shallow material redistribution <xref ref-type="bibr" rid="bib1.bibx44" id="paren.104"/>. Additionally, the contribution of known interseismic creep associated with the Masbate segment to the slip distributions merits further investigation.</p>
</sec>
<sec id="Ch1.S5.SS3.SSS4">
  <label>5.3.4</label><title>Surface rupture length</title>
      <p id="d1e3990">Surface rupture length estimates from remote sensing data were assumed to be symmetrical about the peak displacement zone (Table <xref ref-type="table" rid="Ch1.T3"/>). The ground displacement distributions from optical correlation and field survey (Fig. <xref ref-type="fig" rid="Ch1.F12"/>) imply that the northern rupture terminus is located approximately 3.2 km from the northern shoreline, with peak slip values occurring between 17.3 and 23.5 km, resulting in rupture length estimates ranging from 28.2 to 41 km. The absence of offset measurements in the submerged portions of the fault necessitated the use of interpolation. Given the asymmetrical nature of strike-slip distributions, which can take on either elliptical or triangular forms <xref ref-type="bibr" rid="bib1.bibx67" id="paren.105"/>, caution is critical when interpreting the interpolated values. The rupture lengths are also measured from the total length of the field survey and its extension toward the stepover in Cataingan Bay <xref ref-type="bibr" rid="bib1.bibx56" id="paren.106"/> resulting in 25 and 35.6 km rupture lengths, respectively.</p>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T3"><?xmltex \currentcnt{3}?><label>Table 3</label><caption><p id="d1e4006">Measured rupture parameters with corresponding moment magnitude <xref ref-type="bibr" rid="bib1.bibx98" id="paren.107"/> and seismic moment <xref ref-type="bibr" rid="bib1.bibx43" id="paren.108"/>.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="4">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="left"/>
     <oasis:colspec colnum="3" colname="col3" align="center"/>
     <oasis:colspec colnum="4" colname="col4" align="center"/>
     <oasis:thead>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">Parameter</oasis:entry>
         <oasis:entry colname="col2">Value</oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M161" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">w</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M162" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">o</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> (<inline-formula><mml:math id="M163" display="inline"><mml:mrow><mml:mi>N</mml:mi><mml:mo>⋅</mml:mo><mml:mi>m</mml:mi></mml:mrow></mml:math></inline-formula>)</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>
         <oasis:entry colname="col1">Surface rupture length</oasis:entry>
         <oasis:entry colname="col2">34.4 km<inline-formula><mml:math id="M164" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">1</mml:mn></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">6.9</oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M165" display="inline"><mml:mrow><mml:mn mathvariant="normal">2.6</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mn mathvariant="normal">19</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2">28.2 km<inline-formula><mml:math id="M166" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">6.8</oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M167" display="inline"><mml:mrow><mml:mn mathvariant="normal">1.9</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mn mathvariant="normal">19</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2">41.0 km<inline-formula><mml:math id="M168" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">7.0</oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M169" display="inline"><mml:mrow><mml:mn mathvariant="normal">3.5</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mn mathvariant="normal">19</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2">39.5 km<inline-formula><mml:math id="M170" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">6.9</oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M171" display="inline"><mml:mrow><mml:mn mathvariant="normal">3.3</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mn mathvariant="normal">19</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2">25.0 km<inline-formula><mml:math id="M172" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">5</mml:mn></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">6.7</oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M173" display="inline"><mml:mrow><mml:mn mathvariant="normal">1.5</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mn mathvariant="normal">19</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2">35.6 km<inline-formula><mml:math id="M174" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">6</mml:mn></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">6.9</oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M175" display="inline"><mml:mrow><mml:mn mathvariant="normal">2.8</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mn mathvariant="normal">19</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Maximum displacement</oasis:entry>
         <oasis:entry colname="col2">0.6 m<inline-formula><mml:math id="M176" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">7</mml:mn></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">6.6</oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M177" display="inline"><mml:mrow><mml:mn mathvariant="normal">1.2</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mn mathvariant="normal">19</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2">0.6 m<inline-formula><mml:math id="M178" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">8</mml:mn></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">6.6</oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M179" display="inline"><mml:mrow><mml:mn mathvariant="normal">1.1</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mn mathvariant="normal">19</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Average displacement</oasis:entry>
         <oasis:entry colname="col2">0.4 m<inline-formula><mml:math id="M180" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">9</mml:mn></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">6.7</oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M181" display="inline"><mml:mrow><mml:mn mathvariant="normal">1.2</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mn mathvariant="normal">19</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2">0.3 m<inline-formula><mml:math id="M182" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">10</mml:mn></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">6.5</oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M183" display="inline"><mml:mrow><mml:mn mathvariant="normal">7.3</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mn mathvariant="normal">18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">Largest afterslip</oasis:entry>
         <oasis:entry colname="col2">0.14 m<inline-formula><mml:math id="M184" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">11</mml:mn></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">6.2</oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M185" display="inline"><mml:mrow><mml:mn mathvariant="normal">2.1</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mn mathvariant="normal">18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">Average afterslip</oasis:entry>
         <oasis:entry colname="col2">0.09 m<inline-formula><mml:math id="M186" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">12</mml:mn></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">6.1</oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M187" display="inline"><mml:mrow><mml:mn mathvariant="normal">1.8</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mn mathvariant="normal">18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Est. peak coseismic offset</oasis:entry>
         <oasis:entry colname="col2">0.5 m<inline-formula><mml:math id="M188" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">6.5</oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M189" display="inline"><mml:mrow><mml:mn mathvariant="normal">8.4</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mn mathvariant="normal">18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2">0.4 m<inline-formula><mml:math id="M190" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">6.5</oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M191" display="inline"><mml:mrow><mml:mn mathvariant="normal">8.3</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mn mathvariant="normal">18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Est. average coseismic offset</oasis:entry>
         <oasis:entry colname="col2">0.3 m<inline-formula><mml:math id="M192" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">6.5</oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M193" display="inline"><mml:mrow><mml:mn mathvariant="normal">8.2</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mn mathvariant="normal">18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2">0.2 m<inline-formula><mml:math id="M194" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">16</mml:mn></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">6.5</oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M195" display="inline"><mml:mrow><mml:mn mathvariant="normal">6.9</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mn mathvariant="normal">18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula></oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table><table-wrap-foot><p id="d1e4015"><inline-formula><mml:math id="M145" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">1</mml:mn></mml:msup></mml:math></inline-formula> Symmetrical about the midpoint of the zone of peak displacement. <inline-formula><mml:math id="M146" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula> Symmetrical about the lower limit of the zone of peak displacement. <inline-formula><mml:math id="M147" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:math></inline-formula> Symmetrical about the upper limit of the zone of peak displacement. <inline-formula><mml:math id="M148" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msup></mml:math></inline-formula> Symmetrical about the peak displacement. <inline-formula><mml:math id="M149" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">5</mml:mn></mml:msup></mml:math></inline-formula> Cumulative rupture length from the field survey. <inline-formula><mml:math id="M150" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">6</mml:mn></mml:msup></mml:math></inline-formula> Cumulative rupture length from the field survey extended to the onshore stepover identified by <xref ref-type="bibr" rid="bib1.bibx56" id="text.109"/>. <inline-formula><mml:math id="M151" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">7</mml:mn></mml:msup></mml:math></inline-formula> From optical correlation. <inline-formula><mml:math id="M152" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">8</mml:mn></mml:msup></mml:math></inline-formula> From field survey. <inline-formula><mml:math id="M153" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">9</mml:mn></mml:msup></mml:math></inline-formula> From the weighted moving mean curve of optical correlation outputs. <inline-formula><mml:math id="M154" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">10</mml:mn></mml:msup></mml:math></inline-formula> From the weighted moving mean curve of field measurements. <inline-formula><mml:math id="M155" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">11</mml:mn></mml:msup></mml:math></inline-formula> Highest individual measurement from InSAR. <inline-formula><mml:math id="M156" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">12</mml:mn></mml:msup></mml:math></inline-formula> From the weighted moving mean curve of InSAR. <inline-formula><mml:math id="M157" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:math></inline-formula> Peak optical correlation value minus peak InSAR value. <inline-formula><mml:math id="M158" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:math></inline-formula> Peak field measurement minus peak InSAR value. <inline-formula><mml:math id="M159" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:math></inline-formula> Average of the residuals between the weighted moving mean curves of optical correlation and InSAR. <inline-formula><mml:math id="M160" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">16</mml:mn></mml:msup></mml:math></inline-formula> Average of the residuals between the weighted moving mean curves of field measurements and InSAR.</p></table-wrap-foot><?xmltex \gdef\@currentlabel{3}?></table-wrap>

<?xmltex \hack{\newpage}?>
</sec>
<sec id="Ch1.S5.SS3.SSS5">
  <label>5.3.5</label><title>Seismic moment estimates</title>
      <p id="d1e4812">Moment magnitude (<inline-formula><mml:math id="M196" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">w</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) and seismic moment (<inline-formula><mml:math id="M197" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">o</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) estimates for the 2020 Masbate event were calculated from the surface rupture parameters (Table <xref ref-type="table" rid="Ch1.T3"/>). <inline-formula><mml:math id="M198" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">w</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> calculations used the corresponding empirical equations from regression of rupture parameters and moment magnitudes <xref ref-type="bibr" rid="bib1.bibx98" id="paren.110"/>. The <inline-formula><mml:math id="M199" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">o</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> was derived as a function of <inline-formula><mml:math id="M200" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">w</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> from scaling relationships <xref ref-type="bibr" rid="bib1.bibx43" id="paren.111"/>. This approach was preferred over directly calculating the <inline-formula><mml:math id="M201" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">o</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> from the rupture area and material rigidity due to the lack of reliable estimates of rupture width and subsurface fault rupture parameters.</p>
      <?pagebreak page1155?><p id="d1e4890">The <inline-formula><mml:math id="M202" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">w</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> estimates from the maximum and average displacements range between <inline-formula><mml:math id="M203" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">w</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> 6.5 and <inline-formula><mml:math id="M204" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">w</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> 6.7. The estimated maximum and average coseismic offsets all equate to <inline-formula><mml:math id="M205" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">w</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> 6.5. The values closely fit the instrumental 6.6 moment magnitude. All rupture length estimates returned high <inline-formula><mml:math id="M206" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">w</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> values between <inline-formula><mml:math id="M207" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">w</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> 6.7 and <inline-formula><mml:math id="M208" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">w</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> 7.0 which agrees with the 2003 earthquake observations, wherein the fault rupture is longer than expected relative to the magnitude. However, a downward counterfactual approach <xref ref-type="bibr" rid="bib1.bibx100 bib1.bibx99" id="paren.112"/>, given the fault uncertainties at depth, suggests the probability of the larger <inline-formula><mml:math id="M209" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">w</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> estimates. Nevertheless, the estimated coseismic displacements reasonably fit with the instrumental seismic moment of the mainshock. The calculated <inline-formula><mml:math id="M210" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">w</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> 6.5 value from the estimated coseismic slip parameter is consistent with a seismic moment of <inline-formula><mml:math id="M211" display="inline"><mml:mrow><mml:mn mathvariant="normal">8.4</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mn mathvariant="normal">18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M212" display="inline"><mml:mrow><mml:mi>N</mml:mi><mml:mo>⋅</mml:mo><mml:mi>m</mml:mi></mml:mrow></mml:math></inline-formula>.</p>
      <p id="d1e5024">The lower limit of the post-seismic moment was assessed using the largest and average afterslip values (Table <xref ref-type="table" rid="Ch1.T3"/>). The largest afterslip, which measured 0.14 m, corresponds to <inline-formula><mml:math id="M213" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">w</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> 6.2, while the average afterslip of 0.09 m is consistent with <inline-formula><mml:math id="M214" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">w</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> 6.1. By comparing the largest afterslip value (<inline-formula><mml:math id="M215" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">o</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">2.1</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mn mathvariant="normal">18</mml:mn></mml:msup><mml:mi>N</mml:mi><mml:mo>⋅</mml:mo><mml:mi>m</mml:mi></mml:mrow></mml:math></inline-formula>) with the peak coseismic moment, we estimate that the afterslip resulted in the release of energy equal to at least 25 % of the mainshock.</p>
</sec>
</sec>
<sec id="Ch1.S5.SS4">
  <label>5.4</label><title>Seismotectonic implications</title>
<sec id="Ch1.S5.SS4.SSS1">
  <label>5.4.1</label><title>Surface rupture morphology</title>
      <p id="d1e5095">The fault geomorphology (Fig. <xref ref-type="fig" rid="Ch1.F10"/>c) and geodetic observations (Figs. <xref ref-type="fig" rid="Ch1.F5"/> and <xref ref-type="fig" rid="Ch1.F8"/>) highlight the linearity of the Masbate segment. However, the fault complexity <xref ref-type="bibr" rid="bib1.bibx89" id="paren.113"/> around 12°07'N was not clearly defined due to unwrapping errors in interferometry and high-amplitude noise in optical correlations.</p>
      <p id="d1e5107">The ruptures in Palanas form a right-stepping Riedel shear zone, with the ruptures occurring at a low angle with respect to the regional fault strike. Furthermore, a possible new splay was observed to the south, which potentially represents the primary fault plane, cutting across the bifurcating trace and traversing Cataingan Bay. Antithetic shears were observed at the bifurcation point and along the cross-cutting splay.</p>
      <p id="d1e5110">Topography and bedrock geology may also control the rupture <xref ref-type="bibr" rid="bib1.bibx48" id="paren.114"/> such that the southwestern rupture termination is observed on an alluvial plain, succeeded by rugged topography northwards. The fault complexity in Palanas and the bifurcation point in Cataingan coincide with the stratigraphic contacts of the Late Oligocene Nabangig and Miocene–Pliocene Buyag formations. The previously identified fault complexities in this area may reflect the rheological contrast between the clastic limestones of the Nabangig Formation and the conglomeratic Buyag Formation.</p>
</sec>
<sec id="Ch1.S5.SS4.SSS2">
  <label>5.4.2</label><title>Developing transtensional basins</title>
      <p id="d1e5124">The morphology of mainland Masbate following the 2020 event (Fig. <xref ref-type="fig" rid="Ch1.F13"/>) was the basis for assigning a late relative development stage in a modeled transtensional basin development sequence <xref ref-type="bibr" rid="bib1.bibx101" id="paren.115"/>. The basin boundary is characterized by floodplains surrounded by topographic highs. Apparent asymmetrical depocenters were recognized, with the shallower depocenter occurring on the floodplain and the nearshore section of Cataingan Bay, while the second one extends further southwest.</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="d1e5134">Morphology of the transtensional basins linked by a right-stepping shear zone. Solid line indicates the regional fault and lines with hachures indicate the basin sidewall boundary.</p></caption>
            <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://nhess.copernicus.org/articles/24/1135/2024/nhess-24-1135-2024-f13.png"/>

          </fig>

      <p id="d1e5143">A separate transtensional basin is discernible in Dimasalang given the topography, rupture occurrence, and extensional structures in north Masbate <xref ref-type="bibr" rid="bib1.bibx22" id="paren.116"/>. The northern and southern basins appear to be linked by the Riedel shear zone in Palanas. Fault complexities in the principal deformation zone of a pull-apart basin <xref ref-type="bibr" rid="bib1.bibx101" id="paren.117"/> impede rupture propagation <xref ref-type="bibr" rid="bib1.bibx19" id="paren.118"/> in line with the implications of the observed decreasing coseismic and post-seismic slip toward the north. However, the scarcity of observed ruptures inhibits further analysis of the northern transtensional basin.</p>
      <p id="d1e5156">Fitting the development stage of the southern basin is constrained by the absence of information regarding local strain partitioning. Nonetheless, the expressed fault maturity and identified negative flower structures <xref ref-type="bibr" rid="bib1.bibx22 bib1.bibx56" id="paren.119"/> in the northern and southern bays highlight the presence of oblique extensional stress bounding the Masbate mainland. The orientation of the regional fault implies a WNW–ESE-oriented <inline-formula><mml:math id="M216" display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mi mathvariant="italic">σ</mml:mi></mml:mrow></mml:math></inline-formula>. However, real-world conditions are more complex compared with the simplified parameters in analog models.</p>
</sec>
</sec>
</sec>
<sec id="Ch1.S6" sec-type="conclusions">
  <label>6</label><title>Conclusions</title>
      <p id="d1e5182">The necessity of coupling optical correlation and interferometry is demonstrated by investigating the surface rupture of the 2020 <inline-formula><mml:math id="M217" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">w</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> 6.6 Masbate earthquake along the Masbate segment of the Philippine Fault. Seismicity data showed that foreshocks began 32 d prior to the mainshock on 18 August 2020. The first 30 d of subsequent aftershocks are characterized by a rapid decrease in earthquake frequency, followed by a transition to a gradual decay until 31 January 2021.</p>
      <p id="d1e5196">Optical correlation and InSAR are directly compared through the corresponding generated offset maps. Measuring the ground offset from the near-field region of the interferogram is hindered by decorrelation, whereas the far field suffers because of the submerged northeastern block. The optical correlation method revealed an average <inline-formula><mml:math id="M218" display="inline"><mml:mrow><mml:mn mathvariant="normal">37.7</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">10</mml:mn></mml:mrow></mml:math></inline-formula> cm displacement and <inline-formula><mml:math id="M219" display="inline"><mml:mrow><mml:mn mathvariant="normal">60.6</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">9.8</mml:mn></mml:mrow></mml:math></inline-formula> cm peak left-lateral offset in the near field of the onshore fault segments. Estimates of the peak left-lateral coseismic slip from the total slip and afterslip are consistent with a geodetic moment magnitude of <inline-formula><mml:math id="M220" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">w</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> 6.5 (<inline-formula><mml:math id="M221" display="inline"><mml:mrow><mml:mn mathvariant="normal">8.4</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mn mathvariant="normal">18</mml:mn></mml:msup><mml:mi>N</mml:mi><mml:mo>⋅</mml:mo><mml:mi>m</mml:mi></mml:mrow></mml:math></inline-formula>).</p>
      <p id="d1e5255">The capacity of InSAR to detect smaller displacement amplitudes is highlighted by the post-seismic interferograms. The SBAS time-series stack outlined at least <inline-formula><mml:math id="M222" display="inline"><mml:mrow><mml:mn mathvariant="normal">14.3</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">0.9</mml:mn></mml:mrow></mml:math></inline-formula> cm largest afterslip and <inline-formula><mml:math id="M223" display="inline"><mml:mrow><mml:mn mathvariant="normal">8.8</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">0.7</mml:mn></mml:mrow></mml:math></inline-formula> cm average left-lateral afterslip. The measurements correspond to a <inline-formula><mml:math id="M224" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">w</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> 6.2 (<inline-formula><mml:math id="M225" display="inline"><mml:mrow><mml:mn mathvariant="normal">2.1</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mn mathvariant="normal">18</mml:mn></mml:msup><mml:mi>N</mml:mi><mml:mo>⋅</mml:mo><mml:mi>m</mml:mi></mml:mrow></mml:math></inline-formula>) energy release equivalent to at least 25 % of the coseismic moment estimate. The resolved rupture from interferometry is clearer relative to optical correlation. Multimodal rupture<?pagebreak page1156?> length estimates translate to overestimated moment magnitude values. Hence, the Masbate segment is characterized as capable of producing significant slip and ruptures that are longer than expected, despite the short interval and continuous aseismic stress release during interseismic periods.</p>
      <p id="d1e5314">Our optical correlation data agree with the laterally offset features from field investigation, highlighting the capacity of the method to accurately capture ground displacements despite the difficult tropical terrain. We view this as a consequence of the time interval between the 2020 Masbate earthquake and the 2022 field investigation. Weathering and erosion of fine ruptures had transpired, possibly influencing the field offset distribution.</p>
      <p id="d1e5318">The coseismic slip distribution shows the presence of a single asperity adjacent to the GlobalCMT centroid. In conjunction, the surface distribution of the afterslip coincides with the coseismic slip distribution. Based on the stress transfer theorem and the rate-and-state friction model, we infer that the involved post-seismic deformation is fundamentally stress driven and migrated vertically in either the downdip or updip direction along the sub-vertical fault plane.</p>
      <p id="d1e5321">The surface rupture of the 2020 Masbate event cut across the extant bifurcating trace of the Philippine Fault on the island, possibly reflecting the primary fault plane. Comparing the rupture morphology with analog models reveals the presence of two transtensional basins in Cataingan and Dimasalang, located in the south and north, respectively. The low-angle orientation of ruptures in the midsection corresponds to a Riedel shear zone, which is interpreted to link the identified transtensional basins. Recognition of this structure adds valuable insights into zones vulnerable to future deformation, informing targeted land-use planning and mitigation strategies.</p>
      <p id="d1e5324">The findings and the methods we used for this study in Masbate lead us and future scientists to further analyze the geometry, kinematics, mechanics, and dynamics of fault movement in the area for improved seismic hazard mitigation. Specifically, the comprehensive slip data and observed unusually long rupture lengths along the fault measured through the optical correlation method agree with previous characterizations by <xref ref-type="bibr" rid="bib1.bibx18" id="text.120"/>, indicating significant movement despite the presence of creep. This challenges current seismic hazard models of Masbate and underscores the need to reevaluate potential earthquake magnitudes and ground shaking intensities in the region.</p>
      <p id="d1e5330">Our use of optical correlation alongside interferometry provides high-resolution surface displacement measurements that can aid in the assessment of earthquake hazards to assist the development of mitigation strategies. We recommend the widespread adoption of these methods in studying other active faults in the Philippines. Future studies could incorporate other datasets, such as UAVs, and explore the method for other surface processes. By reevaluating existing hazard models, refinement of the geologic characterization, and scrutinizing slip estimates, we can gain a deeper understanding of the region's seismotectonic configuration and enhance earthquake preparedness in the region.</p>
</sec>

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

      <p id="d1e5337">MicMac is available from <uri>https://github.com/micmacIGN/micmac</uri> <xref ref-type="bibr" rid="bib1.bibx61" id="paren.121"/>. StackProf is available from <uri>https://github.com/micmacIGN/stackprof</uri> <xref ref-type="bibr" rid="bib1.bibx62" id="paren.122"/>. MintPy is available from <uri>https://github.com/insarlab/MintPy</uri> <xref ref-type="bibr" rid="bib1.bibx46" id="paren.123"/>.</p>
  </notes><notes notes-type="dataavailability"><title>Data availability</title>

      <p id="d1e5362">Sentinel-2 datasets are accessed from ESA/EC Copernicus Sentinels Scientific Data Hub and various repositories. The dataset in this study is retrievable from <uri>https://www.esa.int/Applications/Observing_the_Earth/Copernicus/Sentinel-2</uri> <xref ref-type="bibr" rid="bib1.bibx36" id="paren.124"/>. Sentinel-1A/B radar data and cloud interferogram processing are available at <uri>https://sentinel.esa.int/web/sentinel/missions/sentinel-1</uri> <xref ref-type="bibr" rid="bib1.bibx37" id="paren.125"/>. PlanetLabs data are not openly accessible, but academic/scientific access can be requested. Outputs were rendered with Scientific Colour Maps available from <ext-link xlink:href="https://doi.org/10.5281/zenodo.5501399" ext-link-type="DOI">10.5281/zenodo.5501399</ext-link> <xref ref-type="bibr" rid="bib1.bibx29" id="paren.126"/>.</p>
  </notes><?xmltex \hack{\newpage}?><app-group>
        <supplementary-material position="anchor"><p id="d1e5385">The supplement related to this article is available online at: <inline-supplementary-material xlink:href="https://doi.org/10.5194/nhess-24-1135-2024-supplement" xlink:title="pdf">https://doi.org/10.5194/nhess-24-1135-2024-supplement</inline-supplementary-material>.</p></supplementary-material>
        </app-group><notes notes-type="authorcontribution"><title>Author contributions</title>

      <p id="d1e5394">KSCSR: conceptualization, data curation, formal analysis, investigation, methodology, project administration, resources, software, validation, visualization, and writing – original draft, review, and editing. SNV: formal analysis, resources, software, supervision, methodology, and writing – review and editing. AMFAL: conceptualization, funding acquisition, resources, supervision, and writing – review and editing.</p>
  </notes><notes notes-type="competinginterests"><title>Competing interests</title>

      <p id="d1e5400">The contact author has declared that none of the authors has any competing interests.</p>
  </notes><notes notes-type="disclaimer"><title>Disclaimer</title>

      <p id="d1e5406">Publisher's note: Copernicus Publications remains neutral with regard to jurisdictional claims made in the text, published maps, institutional affiliations, or any other geographical representation in this paper. While Copernicus Publications makes every effort to include appropriate place names, the final responsibility lies with the authors.</p>
  </notes><ack><title>Acknowledgements</title><p id="d1e5413">We extend our wholehearted appreciation to Arturo Daag, Allan Gil Fernando, Mario Aurelio, and John Dale Dianala for their suggestions and comments. We appreciate the UPRI staff for their administrative and technical assistance and support. We thank the National Mapping and Resource Information Authority for providing the elevation data. We also thank the Philippine Institute of Volcanology and Seismology and the Disaster Risk Management Office of Dimasalang, Masbate, for their contributions to the field investigation. We are also grateful for the comments of Austin Elliot, Gordon Woo, Brianna Corsa, and the anonymous reviewers for their input and contributions toward improving this work.</p></ack><notes notes-type="reviewstatement"><title>Review statement</title>

      <p id="d1e5418">This paper was edited by Veronica Pazzi and reviewed by Austin Elliott, Brianna Corsa, and three anonymous referees.</p>
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