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  <front>
    <journal-meta><journal-id journal-id-type="publisher">SE</journal-id><journal-title-group>
    <journal-title>Solid Earth</journal-title>
    <abbrev-journal-title abbrev-type="publisher">SE</abbrev-journal-title><abbrev-journal-title abbrev-type="nlm-ta">Solid Earth</abbrev-journal-title>
  </journal-title-group><issn pub-type="epub">1869-9529</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/se-11-741-2020</article-id><title-group><article-title>Plio-Quaternary tectonic evolution of the southern margin of the Alboran Basin (Western Mediterranean)</article-title><alt-title>Pliocene-Quaternary tectonics of the Alboran Basin</alt-title>
      </title-group><?xmltex \runningtitle{Pliocene-Quaternary tectonics of the Alboran Basin}?><?xmltex \runningauthor{M.~Lafosse et al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes" rid="aff1 aff2">
          <name><surname>Lafosse</surname><given-names>Manfred</given-names></name>
          <email>m.r.lafosse@uu.nl</email>
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>d'Acremont</surname><given-names>Elia</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Rabaute</surname><given-names>Alain</given-names></name>
          
        <ext-link>https://orcid.org/0000-0003-1369-0218</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3">
          <name><surname>Estrada</surname><given-names>Ferran</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-5536-0183</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff4">
          <name><surname>Jollivet-Castelot</surname><given-names>Martin</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff5">
          <name><surname>Vazquez</surname><given-names>Juan Tomas</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-3747-4838</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff6 aff7">
          <name><surname>Galindo-Zaldivar</surname><given-names>Jesus</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3">
          <name><surname>Ercilla</surname><given-names>Gemma</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3">
          <name><surname>Alonso</surname><given-names>Belen</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Smit</surname><given-names>Jeroen</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff8">
          <name><surname>Ammar</surname><given-names>Abdellah</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Gorini</surname><given-names>Christian</given-names></name>
          
        </contrib>
        <aff id="aff1"><label>1</label><institution>Institut des Sciences de la Terre Paris, ISTeP UMR 7193, INSU-CNRS, Sorbonne Université, 75005 Paris, France</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>Tectonic and Structural Geology groups, Department of Earth Sciences, Utrecht University, P.O. Box 80.021, <?xmltex \hack{\break}?>3508 TA Utrecht, the Netherlands</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>Instituto de Ciencias del Mar, ICM-CSIC, Continental Margin Group,
08003 Barcelona, Spain</institution>
        </aff>
        <aff id="aff4"><label>4</label><institution>Labratoire d'Océanologie et de Géosciences (LOG), Univ. Lille, CNRS, Univ. Littoral Côte d'Opale, UMR 8187,
<?xmltex \hack{\break}?> 59000, Lille,
France</institution>
        </aff>
        <aff id="aff5"><label>5</label><institution>Juan-Tomas Vazquez, Instituto Español de Oceanografía, Centro Oceanográfico de Málaga, 29640 Fuengirola, Spain</institution>
        </aff>
        <aff id="aff6"><label>6</label><institution>Dpto. de Geodinámica, Universidad de Granada, Granada, Spain</institution>
        </aff>
        <aff id="aff7"><label>7</label><institution>Instituto Andaluz de Ciencias de la Tierra (CSIC-UGR), Granada,
Spain</institution>
        </aff>
        <aff id="aff8"><label>8</label><institution>Département de Géologie, Faculté des Sciences, Université Mohammed V, Avenue Ibn-Batouta, B. P. 1014, Rabat, Morocco</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Manfred Lafosse (m.r.lafosse@uu.nl)</corresp></author-notes><pub-date><day>30</day><month>April</month><year>2020</year></pub-date>
      
      <volume>11</volume>
      <issue>2</issue>
      <fpage>741</fpage><lpage>765</lpage>
      <history>
        <date date-type="received"><day>19</day><month>July</month><year>2019</year></date>
           <date date-type="rev-request"><day>26</day><month>July</month><year>2019</year></date>
           <date date-type="rev-recd"><day>10</day><month>March</month><year>2020</year></date>
           <date date-type="accepted"><day>11</day><month>March</month><year>2020</year></date>
      </history>
      <permissions>
        <copyright-statement>Copyright: © 2020 </copyright-statement>
        <copyright-year>2020</copyright-year>
      <license license-type="open-access"><license-p>This work is licensed under the Creative Commons Attribution 4.0 International License. To view a copy of this licence, visit <ext-link ext-link-type="uri" xlink:href="https://creativecommons.org/licenses/by/4.0/">https://creativecommons.org/licenses/by/4.0/</ext-link></license-p></license></permissions><self-uri xlink:href="https://se.copernicus.org/articles/.html">This article is available from https://se.copernicus.org/articles/.html</self-uri><self-uri xlink:href="https://se.copernicus.org/articles/.pdf">The full text article is available as a PDF file from https://se.copernicus.org/articles/.pdf</self-uri>
      <abstract><title>Abstract</title>
    <p id="d1e233">Progress in the understanding and dating of the sedimentary record of the Alboran Basin allows us to propose a model of its tectonic evolution since the Pliocene. After a period of extension, the Alboran Basin underwent a progressive tectonic inversion starting around 9–7.5 Ma. The Alboran Ridge is a NE–SW transpressive structure accommodating the shortening in the basin. We mapped its southwestern termination, a Pliocene rhombic structure exhibiting series of folds and thrusts. The active
Al-Idrissi Fault zone (AIF) is a Pleistocene strike-slip structure trending
NNE–SSW. The AIF crosses the Alboran Ridge and connects to the transtensive
Nekor Basin and the Nekor Fault to the south. In the Moroccan shelf and at
the edge of a submerged volcano we dated the inception of the local
subsidence at 1.81–1.12 Ma. The subsidence marks the propagation of the AIF
toward the Nekor Basin. Pliocene thrusts and folds and Quaternary
transtension appear at first sight to act at different tectonic periods but
reflect the long-term evolution of a transpressive system. Despite the
constant direction of Africa–Eurasia convergence since 6 Ma, along the
southern margin of the Alboran Basin, the Pliocene–Quaternary compression
evolves from transpressive to transtensive along the AIF and the Nekor
Basin. This system reflects the logical evolution of the deformation of the
Alboran Basin under the indentation of the African lithosphere.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <label>1</label><title>Introduction</title>
      <p id="d1e245">The Pliocene–Quaternary tectonics of the Alboran Basin and its margins show the superposition of transpressive and transtensive structures that have
been attributed to different mechanisms including changes in far-field stress, slab rollback and mantle delamination (Calvert
et al., 2000; Gutscher et al., 2002; Martínez-García et al., 2013,
2017; Petit et al., 2015; Thurner et al., 2014). At present day, GPS
velocities define an Alboran tectonic domain in between the African and Iberian
rigid blocks (Fig. 1) (Neres et al., 2016; Palano et al., 2013, 2015). Based on the seismicity (Fig. 2), a present-day diffuse plate boundary between Africa and Eurasia was proposed in the Alboran Basin and the Betic–Rif belt (Bird, 2003; Neres et al., 2016; Palano et al., 2015). DeMets et al. (2015) constrained the location of the rotation poles between Eurasia, North America and Africa since the Miocene.<?pagebreak page742?> They show that since 5.2 Ma, the southeastward migration of the rotation pole between Africa and Eurasia results in a roughly constant direction of convergence and an increase in the convergence rate (from <inline-formula><mml:math id="M1" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">3.5</mml:mn></mml:mrow></mml:math></inline-formula> to <inline-formula><mml:math id="M2" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">5.5</mml:mn></mml:mrow></mml:math></inline-formula> mm yr<inline-formula><mml:math id="M3" 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> at 35<inline-formula><mml:math id="M4" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 5<inline-formula><mml:math id="M5" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W). More recently, Spakman et al. (2018) showed
that from 8 Ma to the present day, the Africa–Eurasia absolute convergence
has produced 15 km of relative motion in the NNE–SSW direction. These
reconstructions question the idea of a change in plate kinematics as the
cause for changes in tectonic evolution in the Alboran tectonic domain (Martínez-García et al., 2013). Lithosphere-scale processes and crustal heterogeneities such as mantle and lower crustal delamination have exerted a strong influence on the deformation and the structure of the Alboran Basin (Petit et al., 2015; Thurner et al., 2014). The mechanical coupling between the Alboran Domain and the subsiding lithosphere and/or slab dragging under Africa–Eurasia convergence have caused the extrusion of the Betic–Rif belt toward the southwest (Neres et al., 2016; Perouse et al., 2010; Petit et al., 2015; Spakman et al., 2018; Thurner et al., 2014).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1" specific-use="star"><?xmltex \currentcnt{1}?><label>Figure 1</label><caption><p id="d1e300">Topographic map and principal structural units of the Alboran
region. Structural units in the studied area modified from Chalouan
et al. (2008), Comas et al. (1999), Leblanc and Olivier (1984) and Romagny
et al. (2014). The Trans-Alboran shear zone (TASZ) indicates the motion
inferred for the Late Miocene – Pliocene period. The red faults are the
present-day active Al-Idrissi Fault and its conjugated Averroes Fault. AC:
Alboran Channel; AFZ: Adra Fault zone; AVR: Averroes Fault; ABR: Abubacer
Ridge; CF: Carboneras Fault; CR: central Rif; DJ: Djibouti Plateau; EB:
eastern Betic; EAB: East Alboran Basin; AIF: Al-Idrissi Fault; ER: eastern
Rif; JF: Jebha Fault; NF: Nekor Fault; SAB: South Alboran Basin; SAR: South
Alboran Ridge; SB: Sorbas Basin; NAR: North Alboran Ridge; YF: Yusuf Fault; and
WAB: West Alboran Basin. Inset: hypotheses of plate boundaries between an
Alboran tectonic domain and the African plate from Nocquet (2012).</p></caption>
        <?xmltex \igopts{width=369.885827pt}?><graphic xlink:href="https://se.copernicus.org/articles/11/741/2020/se-11-741-2020-f01.png"/>

      </fig>

      <p id="d1e309">Plio-Quaternary changes in stress directions have been demonstrated in the
Betic–Rif belt from field geology (Aït Brahim and Chotin, 1990; Galindo-Zaldívar et al., 1993; Giaconia et al., 2015; Martínez-Díaz and Hernández-Enrile, 2004). The
local changes in horizontal stress directions have led to compression and
uplift of Plio-Quaternary sediments offshore the Palomares Fault on the
Iberian margin (Giaconia et al., 2015). In the Rif,
field studies and paleomagnetic data demonstrated a 15<inline-formula><mml:math id="M6" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> counterclockwise rotation since the Upper Miocene (Crespo-Blanc et al., 2016, and references
therein). At the present time, the direction of shortening seems to be
orthogonal to the offshore NE–SW Trans-Alboran shear zone (TASZ) (Fig. 1)
(Palano et al., 2013). Recent structural mapping has
shown that the offshore distribution of the deformation in the Alboran Sea
has localized during the Quaternary on a set of conjugated strike-slip
faults: the Al-Idrissi Fault (AIF) and the Averroes Fault (Fig. 1) (Estrada
et al., 2018; Galindo-Zaldivar et al., 2018; Lafosse et al., 2017;
Martínez-García et al., 2013, 2017). Along the newly formed
Averroes Fault (Fig. 1), the onset of the strike-slip motion has been
estimated around 1 Ma (Perea et al., 2018). Using a block rotation pinned model, Meghraoui and Pondrelli (2013) have proposed that the oblique convergence led to a rigid-block rotation accommodated by transcurrent faults (e.g., the TASZ, in Fig. 1). However, the timing and mechanism of this structural evolution remains poorly constrained.</p>
      <p id="d1e322">In the present work, we address the Pliocene–Quaternary structural evolution
of the southwestern margin of the Alboran Basin, toward the southern
termination of the Trans-Alboran shear zone. In this poorly studied, yet key
region, we analyze in high-resolution the changes in tectonic and
stratigraphic setting by the means of newly acquired multiresolution 2D
seismic reflection and TOPAS profiles and multibeam data. Based on the
seismic stratigraphic interpretation of our database and on a regional
synthesis of structural data, we propose that the structural evolution of
the Alboran Basin and its southern margin reflects a Pleistocene change in
tectonic style. Our new tectonic model explains the evolution of the
southern margin of the Alboran Basin and the Al-Idrissi Fault zone during
the constant Africa–Eurasia convergence.</p>
<sec id="Ch1.S1.SS1">
  <label>1.1</label><title>Geological and geodynamical settings</title>
      <p id="d1e332">The Alboran Basin developed over a collapsed Tertiary orogen and is limited
onshore by the Betic–Rif belt (Fig. 1) (Comas et al., 1999). The formation of the Alboran Basin has been linked to Early Miocene forearc extension (Booth-Rea et al., 2007; Faccenna et al., 2001; Gómez de la Peña et al., 2018; Jolivet et al., 2008, 2009; Jolivet and Faccenna, 2000). Several Miocene
strike-slip shear zones cut the entire basin from the Iberian to the
Moroccan margins and accommodate the upper-plate deformation that forms a
broad shear zone called the Trans-Alboran shear zone (TASZ; Fig. 1) (Leblanc and Olivier, 1984). Following the westward slab retreat, the TASZ acted as a left-lateral fault zone accommodating the extension of the Alboran Basin. The Africa–Eurasia NW–SE oblique convergence led to a tectonic reorganization during the Late
Miocene (Comas et al., 1999; Do Couto et al., 2016). Due to ongoing Africa–Eurasia convergence, the TASZ underwent an oblique positive inversion starting around 8 Ma in the Sorbas Basin of the Betic margin (Do Couto et al., 2014; Martínez-García et al., 2017). The compression has migrated
westward since approximately 7–8 Ma from the Spanish and Algerian margins to
the Alboran Ridge and since ca. 5 Ma on the Al-Idrissi Fault (Figs. 1 and 2) (Giaconia et al., 2015).</p>

      <?xmltex \floatpos{p}?><fig id="Ch1.F2" specific-use="star"><?xmltex \currentcnt{2}?><label>Figure 2</label><caption><p id="d1e337">Maps showing the distribution of the seismicity along the Neogene tectonic structures in the Alboran Sea. <bold>(a)</bold> Neotectonic map of the Alboran region modified from d'Acremont et al. (2014), Alvarez-Marrón et al. (1999), Chalouan et al. (1997), Estrada et al. (2014), Gràcia et al. (2006, 2012), Lafosse et al. (2017), Martínez-García et al. (2011), Muñoz et al. (2008), Perea et al. (2014), Vázquez et al. (2014) and this study. Seismicity from IGN catalogue 1970–2017
(<uri>http://www.ign.es/</uri>, last access: 1 June 2018); only earthquakes with <inline-formula><mml:math id="M7" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">w</mml:mi></mml:msub><mml:mo>≥</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M8" display="inline"><mml:mrow><mml:mtext>depth</mml:mtext><mml:mo>≥</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> km are figured. <bold>(b)</bold> GPS data from Koulali et al. (2011) and Sh<inline-formula><mml:math id="M9" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">max</mml:mi></mml:msub></mml:math></inline-formula> from Neres et al. (2016). See
Fig. 1 for scale. CF: Carboneras Fault; PF: Palomares Fault; YF: Yusuf
Fault; NF: Nekor Fault; and AIF: Al-Idrissi Fault zone.</p></caption>
          <?xmltex \igopts{width=384.112205pt}?><graphic xlink:href="https://se.copernicus.org/articles/11/741/2020/se-11-741-2020-f02.png"/>

        </fig>

      <p id="d1e392">In the southern margin of the Alboran Sea, the Alboran Ridge corresponds to
a tectonic high that developed since the Late Miocene
(Bourgois et al., 1992; Do Couto, 2014). The Alboran Ridge and the Yusuf Fault divide the Alboran Basin into three different
subbasins: the West (WAB), South (SAB) and East (EAB) Alboran Basin (Fig. 1). Conjugate to the Alboran Ridge, the right-lateral Yusuf Fault zone has been active since the Miocene (Fig. 1) (Martínez-García et al., 2013,
2017). The Al-Idrissi Fault divides the Alboran Ridge into the North (NAR)
and South Alboran (SAR) ridges (Fig. 1). The SAR corresponds to a series of
NE–SW striking submarine highs culminating around <inline-formula><mml:math id="M10" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">110</mml:mn></mml:mrow></mml:math></inline-formula> m (Xauen Bank, Petit Tofiño Bank, Tofiño Bank, Ramon Margalef High, Eurofleet High and Francesc
Pagès Bank in Fig. 3).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3" specific-use="star"><?xmltex \currentcnt{3}?><label>Figure 3</label><caption><p id="d1e408">Bathymetry of the studied area showing the main morpho-structural
features of the studied area. Dark grey and black lines: positions of the
seismic lines used in the study. MTDs: mass transport deposits; WAB: West
Alboran Basin; SAB: South Alboran Basin; BB: Boudinar Basin; BF: Boussekkour
Fault; Bof: Bokoya Fault; BiF: Boudinar Fault; NB: Nekor Basin; NF: Nekor
Fault; AIF: Al-Idrissi Fault zone; TF: Trougout Fault; and AjF:Adjir-Imzouren
Fault.</p></caption>
          <?xmltex \igopts{width=369.885827pt}?><graphic xlink:href="https://se.copernicus.org/articles/11/741/2020/se-11-741-2020-f03.png"/>

        </fig>

      <?pagebreak page745?><p id="d1e417">Sedimentary processes, volcanism and tectonics shaped the morphology of the
Alboran Ridge. Above the Messinian Erosional Surface (MES) (Estrada et al., 2011; Garcia-Castellanos et al., 2011), the deep sedimentation in the Alboran Sea is driven by contouritic processes that has also shaped the seafloor since 5.33 Ma) (Ercilla et al., 2016; Juan et al., 2016). On both flanks of the Alboran Ridge,
contourite deposits produce significant thickness variations in the
Quaternary depositional units that are pinched and thinned toward the foot
of the submarines highs
(Juan et al., 2016). Submarine erosion can occur at the moat of the contouritic
systems, generally at the foot of the slopes, whereas deposition occurs at
deepest locations (Ercilla et al., 2016; Juan et al., 2016). The 70 km long SAR corresponds to a series of faults and folds and to volcanoes affecting the Pliocene–Quaternary depositional sequences (Fig. 3) (Bourgois
et al., 1992; Chalouan et al., 1997; Gensous et al., 1986;
Martínez-García et al., 2013; Muñoz et al., 2008; Tesson et
al., 1987). To the south, the SAR flanks a NE–SW syncline called the South
Alboran Trough and to the north, the Alboran Channel and the WAB (Fig. 3).
The SAR marks the southward transition from thinned to thickened continental
crust (Díaz et al., 2016). It is an
inherited Early Miocene extensional structure that has undergone compressive
deformation since 8 Ma (Fig. 1) (Do Couto et al., 2016). In the WAB, a syn-rift sequence is dated late Aquitanian–Burdigalian
to Langhian (Do Couto et al., 2016). At the base
of the sedimentary column of the SAR, the seismic reflection data show Early
to mid-Miocene under-compacted shales deposited during the extensional
period (Do Couto, 2014; Do Couto et al., 2016; Soto et al., 2008). Pre-Messinian deposits are exposed at the seafloor in the cores of the anticlines of the Alboran Ridge (Chalouan et al., 2008; Do Couto et al., 2016; Juan et al., 2016; Tesson et al., 1987). Local occurrences of volcanism in the Francesc Pagès Bank and the
Ras Tarf are of Miocene and Pliocene age (Figs. 1 and 3). The volcanism in
the Francesc Pagès Bank is not accurately dated (Gill et al., 2004). Basaltic rocks are dated
between 9.6 and 8.7 Ma in the same area by Duggen et al. (2004). In the Ras Tarf (Fig. 3), the volcanism ends around 9 Ma (El Azzouzi et al., 2014). Samples of the Ibn Batouta Seamount contain 5 Ma old gabbro (Duggen et al., 2008).</p>
      <p id="d1e420">Since the Late Miocene, deformation has migrated from the eastern Betic
margin toward the SAR in the southwest (Fig. 1) Giaconia et al. (2015). The SAR has been inverted during the Plio-Quaternary along NE–SW trending faults (Fig. 1) (Chalouan et al., 1997). Seismic reflection
profiles and well data show that the folding continued until the Quaternary
in the Francesc Pagès Bank and highlight several erosion periods during
Pliocene–Quaternary time (Galindo-Zaldivar et al., 2018; Tesson et al., 1987). Unconformities and increasing
accumulation rates indicate three tectonic phases: phase 1 dated from
5.33 to 4.57 Ma, phase 2 from 3.28 to 2.45 Ma and phase 3 between
1.81 and 1.19 Ma (Martínez-García et al., 2013). More recently, Martínez-García et al. (2017) suggested that the uplift along the Alboran Ridge culminated around 2.45 Ma in response to shortening.</p>
      <p id="d1e423">The most recent deformation involves NNW–SSE sinistral transtension from the
frontal indentation of the northern part of the Alboran Ridge to the
transtensive Nekor Basin via the AIF, across the NAR and the SAR at the NE
tip of the Francesc Pagès Bank (Dillon et al., 1980; Estrada et al., 2018; Lafosse et al., 2017). The Nekor Basin accommodates the present-day deformation of the southern Alboran margin
(Figs. 2 and 3). Bathymetric and seismic reflection data show that the
deformation along the AIF is accommodated by a series of sinistral NNE–SSW
strike-slip faults segments (Figs. 1 and 2) (Ballesteros et al., 2008;
Martínez-García et al., 2011). The AIF propagated southward during
the Quaternary (Ballesteros et al., 2008;<?pagebreak page746?> Gràcia et al., 2006; Martínez-García et al., 2011, 2013), connecting to the NNE–SSW active strike-slip Boussekkour–Bokoya Fault zone (Fig. 3) (d'Acremont et al., 2014; Calvert et al., 1997; Lafosse et al., 2017).</p>
      <p id="d1e426">East of the TASZ, the SAB and the Oriental External Rif behave as the
African block (Koulali et al., 2011; Vernant et al., 2010). GPS kinematics show a WNW–ESE convergence rate of 4.6 mm yr<inline-formula><mml:math id="M11" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> between the Africa and Eurasia plates (Nocquet and Calais, 2004). Maximum present-day extrusion rates of 5.5–6 mm yr<inline-formula><mml:math id="M12" 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> in the Alboran
tectonic domain are measured between the Jebha and Nekor faults and indicate
a southwestward lateral escape (Fig. 2b) (Koulali et al., 2011; Vernant et al., 2010).</p>
      <p id="d1e453">The Nekor Basin, SAR and AIF are affected by significant crustal seismicity
(Bezzeghoud and Buforn, 1999; Stich et al., 2005). The focal mechanisms of three main regional earthquakes show subvertical nodal planes and a left-lateral displacement (Fig. 4) (Bezzeghoud and Buforn, 1999; Biggs et al., 2006; Calvert et al., 1997; El Alami et al., 1998; Hatzfeld et al., 1993; Stich et al., 2005, 2006). At the northern border
of the Nekor Basin, earthquakes with <inline-formula><mml:math id="M13" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">w</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">6.3</mml:mn></mml:mrow></mml:math></inline-formula> and 5.9 occurred in 1994 and 2004, respectively (Fig. 4) (Custódio et al., 2016). The NNE–SSW fault tracks identified at the seafloor, in the vicinity of the epicenters, can correspond to the active fault planes deduced from seismological data (d'Acremont et al., 2014; Calvert et al., 1997; Lafosse et al., 2017). On 25 January  2016, a <inline-formula><mml:math id="M14" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">w</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">6.3</mml:mn></mml:mrow></mml:math></inline-formula> earthquake occurred in the vicinity of the AIF (Buforn et al., 2017; Medina and Cherkaoui, 2017; Galindo-Zaldivar et al., 2018). In the deep basin, the earthquake
sequence indicates a strike-slip mode of the AIF, with mainly NNE–SSW
left-lateral motion (Ballesteros et al., 2008; Buforn et al., 2017; Galindo-Zaldivar et al., 2018; Martínez-García et al., 2011; Medina and Cherkaoui, 2017). Several compressional events with NE–SW nodal planes parallel to the Alboran Ridge indicate that the Alboran Ridge is locally reactivated (Fig. 4). In the Nekor Basin, the deformation is partitioned into a normal component in the center of the basin and a left-lateral component on its borders (Fig. 4) (Lafosse et al., 2017). In the SAR, the
style of the deformation is unclear, with focal mechanisms showing
strike-slip or normal components indiscriminately (Stich et al., 2010). Below the WAB, deep earthquakes occur at <inline-formula><mml:math id="M15" display="inline"><mml:mrow><mml:mtext>depths</mml:mtext><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">60</mml:mn></mml:mrow></mml:math></inline-formula> km (Fig. 2a) and are associated with the ongoing necking of sinking lithospheric material (Fig. 2a)
(Bezada et al., 2013; Ruiz-Constán et al., 2011; Sun and Bezada, 2020; Thurner et al., 2014). This distributed lithospheric tear could have propagate from the Betic to the WAB (Heit et al., 2017; Mancilla et al., 2015), yet the timing and the effect of this tear on the local tectonic is still poorly understood.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4" specific-use="star"><?xmltex \currentcnt{4}?><label>Figure 4</label><caption><p id="d1e501">Map of the distribution of the present-day deformation showing strike-slip and compressive deformation along the northern part of the studied area and extensional and strike-slip structures along the southern part. Focal mechanism till 2014 period from the compilation of Custódio et al. (2016) and for the year 2016 from GCMT project (<uri>http://www.globalcmt.org/</uri>, last access: 1 June 2018, Dziewonski et al., 1981 and Ekström et al., 2012). The size of the focal mechanisms corresponds to the magnitude values (from <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:mo>=</mml:mo><mml:mn mathvariant="normal">2.3</mml:mn></mml:mrow></mml:math></inline-formula> to 6.4). Structural data compiled from Ballesteros et al. (2008), Biggs et al. (2006), Buforn et al. (2017), Chalouan et al. (1997), Lafosse et al. (2017) and Martínez-García et al. (2011). BF: Boudinar Fault; WAB: West Alboran Basin; SAB: South Alboran Basin; and NF: Nekor Fault.</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://se.copernicus.org/articles/11/741/2020/se-11-741-2020-f04.png"/>

        </fig>

</sec>
</sec>
<sec id="Ch1.S2">
  <label>2</label><title>Material and methods</title>
      <p id="d1e537">The data used in this study consist of multichannel seismic, sparker and
TOPAS profiles and multibeam bathymetry, acquired during four oceanographic
surveys (Fig. 3). The seismic reflection data were acquired with a
12-channel streamer during the 2011 Marlboro-1 survey, as eight NNW–SSE
parallel lines crossing the W–E folds of the SAR and two WSW–ENE parallel
lines in the southern domain (Fig. 3). The 2012 SARAS survey focused on the
acquisition of shallow data, SPARKER and TOPAS profiles, multibeam
bathymetry, and acoustic reflectivity at a 25 m per pixel resolution of the deep
submarine seafloor (Rodriguez et al., 2017). During the Marlboro-2 survey in 2012 (d'Acremont et al., 2014; Lafosse et al., 2017), SPARKER profiles and shallow multibeam bathymetry at a 5 m per pixel resolution were acquired. The bathymetric data from the 2016 INCRISIS survey were also used (Galindo-Zaldivar et al., 2018). In addition, we used a digital elevation model downloaded from the EMODNET data set (<uri>http://www.emodnet.eu/</uri>, last access: 1 June 2018) to fill the missing parts of our dataset.</p>
      <p id="d1e543">We used the seismic reflection and TOPAS data interpretation for the
tectonic analysis of the subsurface. At the seafloor, we made a visual
recognition of fault scarps using the multibeam bathymetry and the curvature
maps. The curvature is known as a relevant parameter to track the fault
offsets on 3D seismic section (e.g., Roberts, 2001) and at the seafloor  (e.g., Paulatto et al., 2014). The sum of the plan-curvature values was made with the help of ArcGis V10.2 using the focal statistics tool to smoothen the noise at depths below <inline-formula><mml:math id="M17" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">150</mml:mn></mml:mrow></mml:math></inline-formula> m. The seismic–stratigraphic analysis of the Pliocene–Quaternary sequences is based on the stratigraphy defined by Juan
et al. (2016) (Fig. 5). The chronology of the seismic stratigraphic
boundaries was defined based on age calibration of data from scientific
wells DSDP 121 and ODP 976, 977, 978 and 979 (Figs. 1 and 5) (Ercilla
et al., 2016; Juan et al., 2016). Using the velocity analysis for the ODP
well 976 (Soto et al., 2012), we assume an average P-wave velocity of 1750 m s<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> for the Pliocene–Quaternary pelagic sediments. We
propose seismic and sequential stratigraphy interpretations of depositional
units based on the nomenclature and general principles presented in the
literature (Catuneanu, 2007; Catuneanu et al., 2011). All seismic lines shown in the present article are presented uninterpreted in the supplementary material (Figs. S1 to S8 in the Supplement).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F5" specific-use="star"><?xmltex \currentcnt{5}?><label>Figure 5</label><caption><p id="d1e570">Well log correlation to the seismic section, seismic line crossing the location of the ODP 979 site, vertical stacking of the Pliocene and Quaternary units, and available <inline-formula><mml:math id="M19" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup><mml:mi mathvariant="normal">O</mml:mi></mml:mrow></mml:math></inline-formula> curve from Lisiecki and Raymo (2005). The colors of the stratigraphic surfaces are the same as in the following seismic lines.</p></caption>
        <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://se.copernicus.org/articles/11/741/2020/se-11-741-2020-f05.png"/>

      </fig>

</sec>
<sec id="Ch1.S3">
  <label>3</label><title>Results</title>
<sec id="Ch1.S3.SS1">
  <label>3.1</label><title>Pliocene–Quaternary seismic stratigraphy</title>
      <p id="d1e607">The Pliocene–Quaternary sedimentary sequence of the southern Alboran margin has
been divided into three Pliocene (Pl1, Pl2 and Pl3) and four Quaternary
(Qt1 to<?pagebreak page747?> Qt4) seismic units (Fig. 5). These units are limited at the base by
discontinuity surfaces, with M, P0 and P1 for the Pliocene units and BQD and Q0 to
Q2 for the Quaternary units. These discontinuity surfaces are mostly
defined by onlap and erosive surfaces; locally, downlap surfaces are
identified (Figs. 6 and 7). Subparallel, parallel, oblique and wavy
stratified reflections characterize the Pliocene units. Pl1, Pl2 and Pl3
units are pinching toward the structural highs and show aggrading wedge
geometries. The Quaternary seismic units (QT1 to QT4) show an aggradational
geometry and pinch on the older tilted Pliocene deposits (Figs. 6 and 7) (Juan et al., 2016).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F6" specific-use="star"><?xmltex \currentcnt{6}?><label>Figure 6</label><caption><p id="d1e612">Multichannel seismic lines showing the Plio-Quaternary stratigraphy and structural features. Dashed and colored lines are the stratigraphic surface defined in Fig. 5. Black reflectors, pre-MSC reflectors. The seismic section <bold>(a–f)</bold> are ordered from east to west. WAB, South Alboran Basin; SAT, South Alboran Trough; AIF, Al-Idrissi Fault zone.</p></caption>
          <?xmltex \igopts{width=426.791339pt}?><graphic xlink:href="https://se.copernicus.org/articles/11/741/2020/se-11-741-2020-f06.png"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F7" specific-use="star"><?xmltex \currentcnt{7}?><label>Figure 7</label><caption><p id="d1e626">Seismic unconformities at the foot slope of the northern flank of
the South Alboran Ridge. <bold>(a)</bold> Seismic line at the foot of the Francesc Pagès Bank. <bold>(b)</bold> Seismic line at the foot of the Ramon Margalef High. The seismic lines show the diachronism of the deformation affecting the SAR during the Pliocene. After 2.6 Ma, the moats of the contourites pinch at the feet of the folds.</p></caption>
          <?xmltex \igopts{width=426.791339pt}?><graphic xlink:href="https://se.copernicus.org/articles/11/741/2020/se-11-741-2020-f07.png"/>

        </fig>

      <?pagebreak page748?><p id="d1e642">Contouritic deposits and associated sedimentary features, mass transport deposits (MTDs) and volcanic
deposits constitute the Pliocene–Quaternary deposits. The plastered drift
type is dominant and contributes to cover the structural highs (Juan
et al., 2016). Truncations at the foot of topographic highs corresponds to
contourite moats and channels on seismic lines (Fig. 7). Sediments show
local intercalations of lenticular chaotic or transparent facies that are
interpreted as mass-flow deposits, corresponding to scars on the bathymetry
(Fig. 3) (Rodriguez et al., 2017). Regarding the volcanic deposits, two buried volcanic edifices are identified on seismic reflection, the Big Al-Idrissi Volcano (Figs. 3 and 8) and the Small Al-Idrissi Volcano
(Figs. 3, 6 and  9). Acoustically, they correspond to a seismic facies of
poorly continuous, high-amplitude reflectors (Figs. 6, 8 and 9). Pliocene to
Quaternary reflectors onlaps onto these seismic bodies (Figs. 8 and 9). They
trend NE–SW following the trend of South Alboran Trough (Fig. 10).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F8" specific-use="star"><?xmltex \currentcnt{8}?><label>Figure 8</label><caption><p id="d1e647">Multichannel seismic profile showing the transgression of marine
sediment (in green) over the prograding shelf to the edges of the Big
Al-Idrissi Volcano (in pink) crossing the Ras Tarf promontory and the Big
Al-Idrissi Volcano. Dashed black reflector: multiple of the seafloor. Red
points: offlap break (paleoshoreline) marking the concave up trajectories
of the offlap breaks and progradation of the shelf and the first
transgression before 1.81 Ma. The red surface is a maximum regressive surface in the sense of Catuneanu et al. (2011). The seismic line shows the
transgression of marine sediment (in green) over the Pliocene to Quaternary
prograding shelf to the edges of the Big Al-Idrissi Volcano (in pink). Older
depositional units are colored in blue, and the acoustic basement is in grey.</p></caption>
          <?xmltex \igopts{width=426.791339pt}?><graphic xlink:href="https://se.copernicus.org/articles/11/741/2020/se-11-741-2020-f08.png"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F9" specific-use="star"><?xmltex \currentcnt{9}?><label>Figure 9</label><caption><p id="d1e658">Multichannel seismic profile showing seismic stratigraphy and the main structural elements along a portion of the South Alboran Trough located between N145<inline-formula><mml:math id="M20" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> striking faults and the AIF. Line track on Fig. 3.
<bold>(a)</bold> Raw seismic line. <bold>(b)</bold> Interpreted seismic line. Red crosses in <bold>(b)</bold> represent a seismic body made of poorly continuous high-amplitude reflectors interpreted as volcano-clastic deposits.</p></caption>
          <?xmltex \igopts{width=426.791339pt}?><graphic xlink:href="https://se.copernicus.org/articles/11/741/2020/se-11-741-2020-f09.png"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F10" specific-use="star"><?xmltex \currentcnt{10}?><label>Figure 10</label><caption><p id="d1e687">Structural map of Plio-Quaternary faults and folds overlying the map of depths of the Messinian unconformity. Active faults correspond to the faults affecting the seafloor. BF: Boussekkour Fault; Bof: Bokoya Fault; and RF: Rouadi Fault. The two-way travel time (twtt) is in millimeters per second.</p></caption>
          <?xmltex \igopts{width=426.791339pt}?><graphic xlink:href="https://se.copernicus.org/articles/11/741/2020/se-11-741-2020-f10.png"/>

        </fig>

      <p id="d1e697">The Big Al-Idrissi Volcano corresponds to a conic structure located to the
north of the Ras Tarf (Figs. 3 and 8) that has been interpreted as an N–S
volcanic ridge (Bourgois et al., 1992). The top of this seismic body merges with the M reflector (Fig. 8). Above, Pliocene–Quaternary seismic units bury this volcano and show prograding to aggrading sigmoid reflectors that characterize the growth of a continental shelf (Fig. 8). On the west side of this seamount, the trajectory of the offlap breaks is concave up, indicating that the rate of progradation decreases progressively with time. Reflectors onlap on the bottomsets and foresets of the prograding seismic units, marking the beginning of a retrogradation after 1.81 Ma (Fig. 8). West-dipping normal faults offset the depositional unit of prograding sigmoid reflectors (Fig. 8). These normal faults correspond to scarps at the seafloor (Figs. 8 and 11). Toward the top
of the sequence, a unit of flat-lying reflectors corresponds to the
bottomsets of the Late Pleistocene Moroccan shelf offshore of the Ras Tarf
(Fig. 8). The flat top of the Big Al-Idrissi Volcano culminates at an
approximate depth of 150–200 m below the present-day sea level and
corresponds to a toplap surface (Fig. 8).</p>
      <?pagebreak page749?><p id="d1e700">In the South Alboran Trough, the Small Al-Idrissi Volcano has a 4–5 km wide
conic structure and trends roughly NNE–SSW (Figs. 9, 10 and 11). This seismic
body intercalated within the Pl1 seismic unit pinches abruptly toward the
west (Fig. 9). This body corresponds to a rounded high at the seafloor (Fig. 11). The top of the Pl1 seismic unit rests unconformably on
this seismic body indicating an Early Pliocene age (Fig. 9). In the Francesc
Pagès Bank, a seismic body with similar facies is present at the core of
an NNE–SSW striking anticline (Fig. 6), truncated by the M reflector (Fig. 6).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F11" specific-use="star"><?xmltex \currentcnt{11}?><label>Figure 11</label><caption><p id="d1e705">Active structures around the roughly NNE–SSW AIF and adjacent
submarine highs. The AIF bends to the north, where it follows the trends of
the NAR. High values of curvatures in the Francesc Pagès Bank and the
northeast corner of the map underline the linear features at the seafloor,
which corresponds to the truncated Miocene–Pliocene layers. Extreme positive
values in red represent concave topography at the seafloor; extreme negative
values in blue represent convex topography. <bold>(a)</bold> Profile curvature map textured above the shaded bathymetry; dashed purple lines: fault tracks at the seafloor; dashed black lines: positions of the seismic line in <bold>(b)</bold> and in Figs. 8, 9 and 13. <bold>(b)</bold> TOPAS profile showing active N145<inline-formula><mml:math id="M21" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> normal faults. Red lines: active faults; red arrows: positions of the fault traces in <bold>(a)</bold>.</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://se.copernicus.org/articles/11/741/2020/se-11-741-2020-f11.png"/>

        </fig>

      <p id="d1e735">North of the Nekor Basin, the shelf records an Early Quaternary regression
(Fig. 12). We follow the Q1 surface northeastward toward the top of the
submerged shelf surrounding the Big Al-Idrissi Volcano (Fig. 8). The Q0
reflector corresponds to an unconformity at the bottom of prograding oblique
reflectors. This depositional unit displays the geometry of continental
shelf deposits. The most distal offlap break shows the maximum extent of the
Pleistocene continental shelf north of the Nekor Basin. It indicates that
the retrogradation of the shoreline starts before 1.12 Ma and<?pagebreak page750?> after 1.81 Ma
(Q1 reflector, Fig. 12). The most distal offlap break near Al Hoceima is
located around <inline-formula><mml:math id="M22" display="inline"><mml:mrow><mml:mn mathvariant="normal">312</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">30</mml:mn></mml:mrow></mml:math></inline-formula> mstwt (milliseconds two-way travel time), corresponding
to a depth of <inline-formula><mml:math id="M23" display="inline"><mml:mrow><mml:mn mathvariant="normal">188</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">5</mml:mn></mml:mrow></mml:math></inline-formula> m below sea level (Fig. 12). In the distal part
of the shelf, we interpret a seismic body of poorly continuous wavy
reflectors deposited above an erosional surface as a local mass transport
complex, which could mark an early-Quaternary destabilization of the shelf.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F12" specific-use="star"><?xmltex \currentcnt{12}?><label>Figure 12</label><caption><p id="d1e764">SPARKER seismic line showing the transgression of marine sediment
(in green) over the prograding shelf of the Nekor Basin (in pink). Oldest
depositional units (Pliocene) are colored in blue, and the acoustic basement is
in grey. The Maximum Regressive Surface (MRS) is in red.</p></caption>
          <?xmltex \igopts{width=369.885827pt}?><graphic xlink:href="https://se.copernicus.org/articles/11/741/2020/se-11-741-2020-f12.png"/>

        </fig>

</sec>
<?pagebreak page752?><sec id="Ch1.S3.SS2">
  <label>3.2</label><title>Tectonic structures</title>
<sec id="Ch1.S3.SS2.SSS1">
  <label>3.2.1</label><title>Folded structures in the South Alboran Ridge (SAR)</title>
      <p id="d1e788">The shortening in the SAR is distributed from east to west over a 10 to 25 km wide folding structure, composed of series of two to four 4 km wavelength
anticlines (Figs. 6 and 10). Northward-verging anticlines characterize the
northern deformation front (Fig. 6). In the eastern part of the SAR, the
Francesc Pagès and the Eurofleet highs correspond to a south-verging
10 km wide antiformal stack of pinched anticlines (MAB16 and 14; Fig. 6).
Several southward and northward dipping blind thrusts affect the M reflector
(Fig. 6). From east to west and above the thrust faults, a series<?pagebreak page753?> of
anticlines and synclines draw a sigmoidal pattern (Fig. 10). Azimuths of the
hinge lines trend toward a mean N085<inline-formula><mml:math id="M24" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> direction at the center of
the folds and toward a N070<inline-formula><mml:math id="M25" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> direction toward the tips of the
folds. The orientation of the most western tip of the SAR changes from NE–SW
to E–W (Fig. 6). The azimuths of the Pliocene folds in the southern
termination of the NAR trend N058<inline-formula><mml:math id="M26" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> (Fig. 10).</p>
      <p id="d1e818">Below the M surface, truncated Miocene seismic units show local folding
(Fig. 6f). Along the northern flank of the SAR, P0 to BQD unconformities
show the growth of the contouritic drift deposits during tectonic tilting
(Fig. 7). Within the Pliocene sequence, the folding appears to be
progressive and diachronic from east to west. At the foot of the Francesc
Pagès Bank, P1 reflectors are unconformably lying on the P0 reflector
(Fig. 7a). At the foot of the Ramon Margalef High, Pliocene reflectors older
than P1 show a more even geometry with constant thicknesses, and P0 is
conformable (Fig. 7b).</p>
      <p id="d1e821">Parallel to the SAR, the South Alboran Trough corresponds to a syncline that
narrows from east to west (Fig. 6). Its northern flank is steeper than the
southern one (Fig. 6). The local thickness variations reveal the
non-cylindrical folding of the syncline (Figs. 6 and 10). The progressive
tilt of the QT1 to QT4 units and internal growth strata reveal a more
continuous Quaternary to Pleistocene folding of the South Alboran Trough
near the Al-Idrissi Fault zone (Figs. 6 and 9).</p>
</sec>
<sec id="Ch1.S3.SS2.SSS2">
  <label>3.2.2</label><title>The Al-Idrissi Fault zone</title>
      <p id="d1e832">At present day, the AIF is a NNE–SSW fault zone composed of several segments
that locally follow the older NE–SW trend of the Alboran Ridge (Figs. 10 and 11). The AIF forms a clear positive flower structure across the eastern end
of the Francesc Pagès Bank and the western end of the NAR (Fig. 13). The
AIF here corresponds to a left-lateral restraining bend, connecting the
northern and southern segments.<?pagebreak page754?> This structure partially reactivates NE–SW
Pliocene thrusts of the Alboran Ridge and affects the most recent Quaternary
sediments (Figs. 11 and 13). The location of the left-lateral restraining
bend is highlighted in the present day by the cluster of compressive focal
mechanisms (Fig. 4) (Stich et al., 2010). Locally, some Pliocene thrusts appear to be abandoned during the Quaternary (Fig. 13b). The Messinian unconformity is deeper at the western tip of the Alboran Ridge than at the Francesc Pages Bank (Fig. 10), indicating differential
uplift/subsidence across the AIF.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F13" specific-use="star"><?xmltex \currentcnt{13}?><label>Figure 13</label><caption><p id="d1e837">Multichannel seismic lines across the left-lateral restraining
bend of the Al-Idrissi Fault zone showing lateral evolution of the tectonic
structures in North Alboran Ridge and in the left-lateral restraining bend.
<bold>(a)</bold> The Al-Idrissi Fault zone is a positive flower structure following the front of the Alboran Ridge. <bold>(b)</bold> The Al-Idrissi Fault zone is a positive flower structure distinct from the Pliocene thrusts and folds.</p></caption>
            <?xmltex \igopts{width=369.885827pt}?><graphic xlink:href="https://se.copernicus.org/articles/11/741/2020/se-11-741-2020-f13.png"/>

          </fig>

      <p id="d1e852">At the southern tip of the AIF, NNE–SSW active fault segments correspond to the
splay faults distributing the deformation that affect present-day deposits
(Figs. 9 and 11). At the seafloor, the fault traces are clear toward the
southwest where they offset the Small Al-Idrissi Volcano and link to the
Bokoya Fault (Figs. 10 and 11). Below the volcanic facies, poor acoustic
penetration prohibits the interpretation of tectonic structures (Fig. 9).</p>
      <p id="d1e856">On the north-dipping flank of the South Alboran Ridge, we observe
N145<inline-formula><mml:math id="M27" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> trending lineaments at the seafloor that correspond to
normal faults (Figs. 11 and 14). The fault network forms a 10–12 km wide shear zone (Fig. 14). The recognition of pockmarks at the seafloor and signal
attenuation near the faults on the seismic reflection data suggest fluid
seepages along active faults (Fig. 14) (e.g., Judd and Hovland, 2009). Northward, the faults disappear below the seafloor under the
present-day contourite drift. These faults affect Q1 and Q2 surfaces
demonstrating Late Pleistocene activity (Fig. 14b). Southward, the fault
traces disappear against the hinge axis of the Francesc Pagès Bank.
Similar NW–SE striking faults affect the seafloor at the southwestern flank
of the Francesc Pagès Bank (Fig. 11a). These N145<inline-formula><mml:math id="M28" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> lineaments
correspond to the normal faults highlighted in red on the TOPAS profile
(Fig. 11b) that uplift the western block. Despite reduced expression at the
seafloor, this fault zone continues southeast, where it affects the whole
Plio-Quaternary sequence (Fig. 9). Along the AIF, the vertical offset of the
P1 surface is around 100 m (Fig. 9). Between the N145<inline-formula><mml:math id="M29" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> faults and
the AIF, several fault segments affect the subsurface, highlighting the
distributed deformation between the N145<inline-formula><mml:math id="M30" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> faults and the AIF with
a higher apparent vertical offset along the AIF (Fig. 9).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F14" specific-use="star"><?xmltex \currentcnt{14}?><label>Figure 14</label><caption><p id="d1e897">Active structures affecting the northern flank of Francesc
Pagès and Ramon Margalef highs. <bold>(a)</bold> Plan curvature map overlying the shaded bathymetry; red arrows: pockmarks on the seafloor; dashed black lines: seismic lines in the figures <bold>(b, c)</bold>; and dashed red lines: positions of the fault tracks. <bold>(b)</bold> SPARKER seismic reflection line showing the northward continuity of 145<inline-formula><mml:math id="M31" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N fault (red line). <bold>(c)</bold> TOPAS seismic line showing the subsurface of the seafloor. Red arrows: positions of the faults drawn in <bold>(a)</bold>.</p></caption>
            <?xmltex \igopts{width=426.791339pt}?><graphic xlink:href="https://se.copernicus.org/articles/11/741/2020/se-11-741-2020-f14.png"/>

          </fig>

</sec>
</sec>
</sec>
<sec id="Ch1.S4">
  <label>4</label><title>Discussion</title>
      <p id="d1e941">Our results show at least two phases of tectonic activity from the Early
Pliocene to the present day. Based on a literature synthesis (Fig. 15) and
our new data, we show that the Al-Idrissi Fault zone is a young feature
(<inline-formula><mml:math id="M32" display="inline"><mml:mrow><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">1.8</mml:mn></mml:mrow></mml:math></inline-formula> Ma) that profoundly affects regional deformation. The first
phase of transpressive deformation started probably during the Tortonian and
ends during the Early Quaternary, with the local occurrence of volcanism.
The second phase clearly started after 1.8 Ma and continues today. It
corresponds to a transtensive tectonic regime. Both phases evidence the
overall oblique convergence and control by deep structures, which we detail
thereafter.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F15" specific-use="star"><?xmltex \currentcnt{15}?><label>Figure 15</label><caption><p id="d1e956">Synthesis of the tectonic events in the Alboran Basin and the
Rif from the literature and the present study. <inline-formula><mml:math id="M33" display="inline"><mml:msup><mml:mi/><mml:mo>*</mml:mo></mml:msup></mml:math></inline-formula> this study; (1) Benmakhlouf et al. (2012); (2) Romagny et al. (2014); (3) Aït
Brahim and Chotin (1990), (4) Lafosse et al. (2017); (5) Azdimousa et
al. (2006); (6) Galindo-Zaldivar et al. (2018); (7) Juan et al. (2016);
(8) Martínez-García et al. (2013); (9) Martínez-García et al. (2017); (10) Gràcia et al. (2019); (11) Perea et al. (2018); and (12) Giaconia et al. (2015). The main tectonic events are in green. Green arrows and question marks indicate the age uncertainties of the main tectonic events.</p></caption>
        <?xmltex \igopts{width=497.923228pt}?><graphic xlink:href="https://se.copernicus.org/articles/11/741/2020/se-11-741-2020-f15.png"/>

      </fig>

<sec id="Ch1.S4.SS1">
  <label>4.1</label><title>Miocene–Pliocene to Early Quaternary strain partitioning</title>
      <p id="d1e981">Truncated folds (Fig. 6f) indicate that shortening started in the South
Alboran Ridge before the Messinian Salinity Crisis (MSC) (Do Couto et al., 2016). The lateral and vertical stratal pattern of the Plio-Quaternary units shows that the shortening occurs mostly during the Pliocene. The overall geometry of deformation in the SAR shows the development of a N065<inline-formula><mml:math id="M34" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> shear zone that partitioned the deformation in imbricated folds and thrusts and left-lateral shear (Fig. 6). The change in stacking pattern of the Pliocene deposits along the folds suggests a diachronous growth during the Pliocene with lateral variation in the uplift rates (Figs. 6 and 7). The intra-Pliocene unconformities, the tilting of the Pliocene units and the aggradation of Quaternary contourite deposits indicate a relative quiescence of the folding during the Quaternary after 2.6 Ma (Juan et al., 2016).</p>
      <p id="d1e993">The Pliocene deformation is locally contemporaneous with volcanism. The
lateral continuity of the highly reflective facies from west to east
suggests that the Small and Big Al-Idrissi volcanoes are part of a volcanic
structure that is offset by local extensional faults during the Pleistocene
(Figs. 8 and 10). This highly reflective material triggers the acoustic
masking of the reflections below (Fig. 9), as observed in debris-avalanche
deposits elsewhere (Le Friant et al., 2002, 2009). The intercalation of this volcanic material toward the top of the Pl1 unit dates the Small Al-Idrissi Volcano between 4.5 and 5.33 Ma (Fig. 9). The NE–SW distribution of the volcanic material suggests a syn-folding
infill of the syncline of the South Alboran Trough (Fig. 10). The local
volcanism is contemporaneous with the volcanic activity occurring to the north
of the Alboran Ridge, dated between 6 and 4.5 Ma (Duggen et al., 2008). This volcanism occurred above
a thinned continental lithosphere (Duggen et al., 2008). The local volcanism suggests that the SAR could have accommodated
westward thinning of the crust in the West Alboran Basin from Late Miocene
to Pliocene. This extension could be linked to the transition from slab
rollback to delamination as proposed in Petit al. (2015).</p>
      <p id="d1e996">NE–SW thrust faults distribute the deformation between the Nekor and Jebha
Fault and the Alboran Ridge and accommodate the strike-slip motion during
the Pliocene. The 20<inline-formula><mml:math id="M35" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> angle between the N065<inline-formula><mml:math id="M36" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> trend of
the SAR and the N085<inline-formula><mml:math id="M37" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> trend of internal folds evidence a N–S
maximum horizontal shortening direction in the SAR (in the present-day
structural framework) and indicates left-lateral transpression during the
Pliocene folding (e.g., Fossen et al., 1994; Fossen and Tikoff, 1998). It reflects the oblique shortening direction relative to the NE–SW basement faults during the Pliocene. In the SAR, the Pliocene folds show a left-lateral deflection of their hinge lines from the E–W to NE–SW, drawing an<?pagebreak page755?> overall sigmoidal shape (Figs. 6 and 10). Comparison of
the structures in the SAR with analogue models of fold-and-thrust belt
(e.g., ter Borgh et al., 2011; Koyi et al., 2016; Storti et al., 2007) suggests
reactivation of basement faults and vertical-axis rotation of the faults
(Fig. 16a–c). The development of E–W faults and thickness variation in the sedimentary cover, resulting in non-cylindrical thrust wedges, lateral escape of frontal thrust sheets and
vertical-axis block rotations demonstrate the influence of a viscous layer.
In the SAR, such a weak layer corresponds to the Early Miocene,
under-compacted shales at the base of the sedimentary cover (Soto et al., 2008, 2012). Such a weak layer can explain why the deformation is distributed in the SAR, whereas it appears to be more localized in the NAR.</p>
      <p id="d1e1026">As the direction of relative plate motion between Africa–Eurasia has been
approximatively constant since 6 Ma (DeMets et al., 2015), left-lateral transpression in the SAR in the present-day framework is unlikely. Instead, it suggests a progressive rotation of
basement faults relative to the regional shortening direction since the
Pliocene and a progressive change from left-lateral transpressive to more
purely compressive deformation (Fig. 16a and b). This model is in
accordance with the bookshelf model, which assumes 2–3<inline-formula><mml:math id="M38" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> Ma<inline-formula><mml:math id="M39" 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>
progressive vertical-axis rotation of basement faults since the Pliocene (Meghraoui and Pondrelli, 2013).</p>
      <p id="d1e1051">The offshore Pliocene oblique compression is equivalent to transpressive
tectonics in the Rif onshore (Fig. 15), where the area between the Nekor and
Jebha Fault accommodates distributed deformation (Fig. 16a). The passive
infilling of paleo-rias indicates relatively low vertical motion (Romagny et al., 2014) (Fig. 15). After 3.8 Ma, a transition from compression to radial extension (Benmakhlouf et al., 2012) causes NE–SW normal faulting and
tectonic tilting of the Moroccan margin (Fig. 16b) (Romagny et al., 2014). Toward the southeast, the Nekor Fault has acted as a transpressive fault zone accommodating the shortening (Ait Brahim et al., 2002; Aït Brahim and Chotin, 1990). The offshore extensional faults
prolonging the Nekor Fault were sealed by Pliocene deposits and inverted as
blind thrust faults during the Plio-Quaternary (Watts et al., 1993). In the
external Rif, in the southwestward continuity of the Nekor Fault, field
studies demonstrate NE–SW compression (Roldán et al., 2014). Interpretation of 2D seismic reflection lines indicates thick-skin tectonic from Tortonian–early Messinian to Pliocene times, causing the uplift of
intra-mountainous basins around the Nekor Fault (Fig. 16a) (Capella et al., 2016).</p>

      <?xmltex \floatpos{p}?><fig id="Ch1.F16" specific-use="star"><?xmltex \currentcnt{16}?><label>Figure 16</label><caption><p id="d1e1056">Palinspastic maps of the SAR and the Rif from 5 Ma to the
present day are using 14<inline-formula><mml:math id="M40" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> clockwise rotation of the Alboran
tectonic domain from <bold>(a)</bold> to <bold>(c)</bold>. Dashed blue line: approximate coastline; continuous blue line: present-day coastline; dark yellow: Miocene–Pliocene onshore basins; light yellow: Pliocene and Quaternary onshore basins; and grey patch: position of the slab remaining approximatively constant below the Alboran Basin during the Plio-Quaternary. Thick grey arrows in <bold>(c)</bold> indicate the direction and relative amount of extrusion in the central Rif considering a fixed Eurasia. The shortening is accommodated through compressive structures in <bold>(a)</bold>. The initiation of subsidence along the Big Al-Idrissi Volcano and the Moroccan shelf corresponds to <bold>(b)</bold>, and the present–day partitioning of the deformation corresponds to <bold>(c)</bold>. CR: central Rif; JF: Jebha Fault; NF: Nekor Fault; and AIF: Al-Idrissi Fault zone.</p></caption>
          <?xmltex \igopts{width=184.942913pt}?><graphic xlink:href="https://se.copernicus.org/articles/11/741/2020/se-11-741-2020-f16.png"/>

        </fig>

</sec>
<sec id="Ch1.S4.SS2">
  <label>4.2</label><title>Quaternary to present-day strain partitioning</title>
<sec id="Ch1.S4.SS2.SSS1">
  <label>4.2.1</label><title>Evidence of Quaternary tectonic subsidence</title>
      <p id="d1e1109">In contrast to the South Alboran Ridge, the recorded uplift increases
through time in the North Alboran Ridge until it reaches a maximum around
2.45 Ma, related to the development of a popup structure (Martínez-García et al., 2017) (Fig. 15). This
contrast could be linked to the incipient activity of the AIF and suggests
that the AIF progressively decouples the deformation between the NAR and the
SAR from 2.6<?pagebreak page756?> to 2.45 Ma (Fig. 16). Before 1.8 Ma, basinward motion of the
shelf along the Big Al-Idrissi Volcano and the normal regressive geometry
of the shelf wedges support the argument for progradation driven by sediment supply. It may
indicate positive accommodation at the coastline (Catuneanu et al., 2011).</p>
      <p id="d1e1112">After 1.8 Ma, the later Pleistocene transgression is linked to the normal
faulting along N–S faults (Figs. 8 and 12). Including the onshore Trougout
and Boudinar faults, we interpret the N–S fault network as an en échelon
right-stepping set of normal faults (Figs. 10 and 16). Focal mechanism and
microstructural studies demonstrate that this fault network is likely to be
active with a normal and a sinistral component (Fig. 4) (Poujol et al., 2014). The local stratigraphy recorded the start of the activity of this
tectonic structure during the Pleistocene. The depth of the Pleistocene
offlap breaks and the geometry of the shelves indicate evident tectonic
subsidence contemporaneous with the northward tilting of the margin
(Ammar et al., 2007). The Moroccan shelf underwent a local transgression and flooding characterized by the building of transgressive
wedges on top of prograding clinoforms (Figs. 8 and 10). The retrogradation
of the shoreline started between 1.8 and 1.12 Ma on the margins of the
Nekor Basin and the Big Al-Idrissi Volcano (Fig. 16). The depth of the
offlap breaks is significantly lower than the maximum depths reached by the
sea-level falls at Gibraltar during the Quaternary (Figs. 8 and 12) (Rohling
et al., 2014) and proves the tectonic subsidence.</p>
</sec>
<sec id="Ch1.S4.SS2.SSS2">
  <label>4.2.2</label><title>Evolution and localization of the Al-Idrissi Fault zone</title>
      <p id="d1e1123">The beginning of the transgression of the shelf around the Big Al-Idrissi
Volcano and the Nekor Basin is approximately synchronous with the last
shortening event along the North Alboran Ridge (1.8 to 1.12 Ma) (Fig. 15).
The AIF has progressively propagated southward, activating the<?pagebreak page757?> N–S
right-stepping normal fault towards the Boudinar and Nekor Basins (Fig. 16b). The transgression of the shelf of the Big Al-Idrissi Volcano and the
subsidence of the Nekor Basin indicate the localization of deformation on a
releasing bend activating these N–S faults.</p>
      <p id="d1e1126">The apparent small lateral offset and the localization of deformation on the
left-lateral Boussekkour–Bokoya Fault zone after 0.8 Ma suggest that the
localization of the deformation along the AIF is a recent feature (Figs. 15
and 16c) (Lafosse et al., 2017). In this context, the normal faults in the
Nekor Basin are equivalent to antithetic faults within a horsetail splay
that connect to the Trougout Fault and the Nekor faults (Fig. 16b). Such
structures are probably related to a relay ramp, like the one proposed in
other strike-slip contexts such as the Paleogene Bowey Basin
(Peacock and Sanderson, 1995). It denotes a progressive localization of the deformation along the AIF and westward migration of the deformation as proposed in Lafosse et al. (2017) and Galindo-Zaldivar
et al. (2018) (Fig. 16c).</p>
      <p id="d1e1129">The left-lateral restraining bend in the northern part of the AIF affects
the seafloor and was active during the recent seismic crisis (Buforn
et al., 2017; Galindo-Zaldívar et al., 2015). In the eastern part of
the SAR, the N145<inline-formula><mml:math id="M41" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> normal faults are active with an orientation
similar to the N140<inline-formula><mml:math id="M42" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> normal faults in the Nekor Basin (Figs. 10, 11
and 14) (Lafosse et al., 2017). The local direction of the maximum horizontal stress field and focal mechanisms (Figs. 2b and 4) (Neres et al., 2016)
indicate that the fault zone is transtensive with a right-lateral motion.
This fault zone may act as the conjugate to the present-day left-lateral
AIF or be an extensional structure related to the southern fault tip in the
horsetail splay (Fig. 16c).</p>
      <?pagebreak page759?><p id="d1e1150">The inception of the southern Al-Idrissi Fault zone after 1.8Ma is coherent
with similar ages found for the inception of strike-slip tectonics to the
north of the NAR where the set of conjugated Al-Idrissi and Averroes
strike-slip faults is dated around 1–1.1 Ma (Figs. 1, 15 and 16) (Estrada et al., 2018; Gràcia et al., 2019; Perea et al., 2018). The AIF decouples the deformation in the SAR and the NAR and acts as a transfer fault that
connects the shortening north of the Alboran Ridge (Estrada et al., 2018) and the Rifian extrusion along the Nekor Fault. The localization of the deformation along the AIF could be controlled by a Miocene pre-existing structure, as proposed in Martínez-García et al. (2017). At a
crustal-scale, geophysical studies show a <inline-formula><mml:math id="M43" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">20</mml:mn></mml:mrow></mml:math></inline-formula>–30 km crustal
thickness variation in the Al Hoceima region (Diaz et al., 2016). The crustal thickness contrasts are a consequence of Miocene oblique collision (Booth-Rea et al., 2012), lower crustal doming during the Miocene transtension (Le Pourhiet et al., 2014) or removal of lower crust associated with delamination
processes (Bezada et al., 2014; Petit et al., 2015). The localization of the deformation on crustal heterogeneities has been evidenced in numerical models, for example, in the cratonic lithosphere (Burov et
al., 1998). Similarly, the localization of the AIF evidences the control of
the crustal thickness variations.</p>
</sec>
</sec>
<sec id="Ch1.S4.SS3">
  <label>4.3</label><title>Evolution of the southeastern limit of the Alboran tectonic domain</title>
      <p id="d1e1172">The Late Miocene–Early Pliocene period in the Rif Belt matches the uplift of
the Miocene intra-mountainous basin along the Nekor Fault under compression
and left-lateral displacement (Fig. 16a) (Capella et al., 2016). The uplift of those basins corresponds to the change from thin-skin to thick-skin deformation in the external Rif during the inversion of the deep Mesozoic extensional structures (Capella et al., 2016; Martínez-García et al., 2017). Our preferred tectonic scenario consists of a progressive mechanical coupling between the African margin and the Alboran Domain, locking the Nekor Fault in its eastern segment (Fig. 16). This scenario is supported by paleomagnetic data from the External Rif
that indicate at least 15<inline-formula><mml:math id="M44" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> of counterclockwise rotation since the
Upper Miocene (Crespo-Blanc et al., 2016, and references therein). Progressive vertical-axis rotation associated with the shortening of the Alboran Basin decreases the left-lateral shear and
increases the compressive deformation along the Alboran Ridge (Fig. 16b).
Eventually, the deformation localized on the AIF during the Early
Quaternary and has been decoupling the deformation between the NAR and the SAR with a
developing transtensive regime since 1.81 Ma (Fig. 16c). This evolution
induced a change in strain partitioning along the TASZ illustrated by the
transition from a Pliocene left-lateral shearing and folding of the SAR to a
transtensive Quaternary deformation localized on the AIF and the Nekor Basin
(Fig. 16). Since 6 Ma, the relative direction of Africa–Eurasia convergence
has remained constant (DeMets et al., 2015), with a NNE–SSW direction in an absolute reference frame (Spakman et al., 2018). This prohibits changes in the direction of far-field forces as the cause for changes in tectonic style in the Alboran Basin as suggested by Martínez-García et al. (2013).</p>
      <p id="d1e1184">Other scenarios consider that delamination has occurred in the Rif since 6 Ma,
explaining the structural pattern and extension in the Nekor basin (Bezada et al., 2013; Petit et al., 2015). Extension in the Nekor Basin and strike-slip tectonics along the Al-Idrissi Fault since 1.8–1.12 Ma would then correspond to a reappraisal of mantle delamination. However, this process corresponds to a long-term convective removal of the African lithosphere (Petit et al., 2015). To explain the progressive tectonic reorganization during the Plio-Quaternary, we do not favor this last hypothesis because we do not observe an increase in widespread long-wavelength (<inline-formula><mml:math id="M45" display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">100</mml:mn></mml:mrow></mml:math></inline-formula> km) subsidence that is usually associated with convective thinning of the lithosphere in
thermomechanical models (e.g., Le Pourhiet et al., 2006; Valera et al., 2011).</p>
      <p id="d1e1197">Recent papers (Heit et al., 2017; Mancilla et al., 2015; Sun and Bezada, 2020) suggest that a slab tear propagates from the Betic to the western tip of the Alboran Ridge, with a lithospheric necking distributed from north to south below the West Alboran Basin (Sun and Bezada, 2020). It is unclear how fast this slab tear propagates from the Betic to the study area and how it
controls the Plio-Quaternary deformation. Slow uplift and
extension since 4 Ma are recorded in the central Rif (Fig. 15) (Romagny et al., 2014) and might mark the
inception of the lithospheric necking. Since 1.8–1.12 Ma, vertical motion
has been local, however, and associated with the activity of the AIF. The timing is
of primordial importance as demonstrated by thermomechanical models. These
models show that slab detachment is a fast process that can occur in less
than 1 Ma, causing a high-amplitude topographic response (Duretz et al., 2011, 2012). It indicates that the vertical pull due to the sinking
lithosphere must be constant during the Plio-Quaternary. It suggests that
the necking of the sinking lithosphere is a slow process or is very recent
with yet indiscernible effects on the shallower structures in the upper
plate.</p>
      <p id="d1e1200">In this framework, normal strike-slip faulting observed to the north of the
NAR (Fig. 1) (Estrada et al., 2018; Giaconia et al., 2015; Gràcia et al., 2012; Grevemeyer et al., 2015) provides additional evidence of indentation by the Africa plate into the Alboran tectonic domain (Estrada et al., 2018; Palano et al., 2015). This indentation is accommodated through the
left-lateral AIF and the right-lateral Averroes Yusuf Fault zone (Figs. 1 and 16) in a way similar to that the Palomares Fault zone, transferring the
orthogonal shortening of the Iberian margin toward the Carboneras Fault zone
and the central Alboran Sea (Estrada et al., 2018; Giaconia et al., 2015). In the SAR and the Nekor Basin, the present-day deformation under the transtensional regime (NNW–SSE to N–S extensional network and NNE–SSW strike-slip faults; Figs. 4 and 16) is limited to the east by the Al-Idrissi Fault. The deformation in the NAR is on the contrary clearly compressive  (Estrada et al., 2018; Martínez-García et al., 2017), and the geodetic data indicate similar displacements in the EAB and in the Rifian units east of the Boudinar Basin (Koulali et al., 2011; Vernant et al., 2010). Such a difference in behavior suggests that the AIF may represent the present-day plate boundary between Africa and Alboran Domain.</p>
</sec>
</sec>
<sec id="Ch1.S5" sec-type="conclusions">
  <label>5</label><title>Conclusion</title>
      <p id="d1e1213">This study focused on the tectonic evolution of the southern margin of the
Alboran Sea during the Plio-Quaternary, particularly the distinct
structural evolutions and interactions of the AIF and the Alboran Ridge and
the mechanisms associated with their formation. The analysis of the seismic
stratigraphy and the comparison between onshore and offshore tectonic
structures led to the following tectonic framework:
<list list-type="custom"><list-item><label>1.</label>
      <p id="d1e1218">The Trans-Alboran shear zone, in particular the Alboran Ridge, localized the deformation between the Miocene and the Early Quaternary. Its orientation favors a<?pagebreak page760?> strike-slip movement during its oblique shortening. The folded structures of the South Alboran Ridge underwent significant left-lateral displacement during the Pliocene.</p></list-item><list-item><label>2.</label>
      <p id="d1e1222">Under the indentation of African lithosphere, vertical-axis block rotations led to a progressive compression on the Alboran Ridge and a Pleistocene activation of the Al-Idrissi Fault. The subsidence of both the Nekor Basin and the Big Al-Idrissi Volcano marks the start of the transtensive deformation between 1.8 and 1.12 Ma.</p></list-item><list-item><label>3.</label>
      <p id="d1e1226">The area between the South Alboran Ridge and the Nekor Fault is being progressively extruded southwestward, whereas east of the Al-Idrissi Fault, the African lithosphere indents the Alboran tectonic domain. The Al-Idrissi Fault transfers this indentation to the Nekor Basin and has represented an incipient plate boundary since 1.8 Ma.</p></list-item></list></p>
      <p id="d1e1229">Our findings demonstrate that at the scale of the basin, strike-slip shear
zones evolve not only in response to far-field forces but also in response to the
local evolution of the Al-Idrissi Fault zone. This evolution is fast, being
achieved in less than 2 Ma, and might be related to lithospheric necking
below the West Alboran Basin or mantle delamination below the Rif. In our
opinion, the indentation of the African lithosphere into the Alboran
tectonic domain explains better the scale and timing of the deformation in
the Al-Idrissi Fault. Additional modeling could help to better understand
the different processes. Further research is needed to better understand
what drives the evolution of such large scale-strike slip structures.</p>
</sec>

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

      <p id="d1e1236">Seismic profiles presented in this article are provided in the Supplement. The bathymetry of the seafloor provided in this article is not publicly available.</p>
  </notes><app-group>
        <supplementary-material position="anchor"><p id="d1e1239">The supplement related to this article is available online at: <inline-supplementary-material xlink:href="https://doi.org/10.5194/se-11-741-2020-supplement" xlink:title="pdf">https://doi.org/10.5194/se-11-741-2020-supplement</inline-supplementary-material>.</p></supplementary-material>
        </app-group><notes notes-type="authorcontribution"><title>Author contributions</title>

      <p id="d1e1248">ML wrote the paper and conducted the study.  Ed'A and CG led the oceanic surveys Marlboro-1, 2 and SARAS. They contributed to the study and to the redaction of the present paper. AR contributed to the data acquisition and processing and the redaction of the present paper. JS contributed to the redaction of the present paper. FE contributed to the data acquisition and processing. MJC contributed to the stratigraphic interpretation. JTV contributed to the data acquisition and processing.
JGZ and GE contributed to the data acquisition and processing. They are the PIs of the INCRISIS survey. GE also contributed to the stratigraphic correlations and interpretations. BA contributed to the stratigraphic correlations and interpretations. AA contributed to the data acquisition.</p>
  </notes><notes notes-type="competinginterests"><title>Competing interests</title>

      <p id="d1e1254">The authors declare that they have no conflict of interest.</p>
  </notes><ack><title>Acknowledgements</title><p id="d1e1260">We thank the members of the SARAS and Marlboro cruises in 2011 and 2012. We
thank Emanuele Lodolo, Jacques Déverchère, Guillermo Booth-Rea for their helpful comments and discussion. We also thank the editor, Federico Rossetti, for the attention provided to this article. This work was funded by the French program Actions Marges, the EUROFLEETS program (FP7/2007-2013; no. 228344) and project FICTS-2011-03-01. The French program ANR-17-CE03-0004 also supported this work. Seismic reflection data were processed using the Seismic UNIX SU and Geovecteur software. The processed seismic data were interpreted using Kingdom IHS Suite© software.
This work also benefited from the Fauces Project (Ref CTM2015-65461-C2-R;
MINCIU/FEDER) financed by Ministerio de Economía y Competitividad y al
Fondo Europeo de Desarrollo Regiona (FEDER).</p></ack><notes notes-type="financialsupport"><title>Financial support</title>

      <p id="d1e1265">This research has been supported by the CNRS-INSU-TOTAL-BRGM-IFREMER Actions Marges program, EUROFLEETS program FP7/2007-2013 (grant no. 228344), EU Regional Structural Fund (grant no. FICTS-2011-03-01) and DAMAGE Project (project no. FEDER/CGL2016-80687-R AEI), Fauces Project (project no. FEDER/CTM2015-65461-C2-R; MINCI), ALBAMAR Project (project no. ANR/ANR-17-CE03-0004).</p>
  </notes><notes notes-type="reviewstatement"><title>Review statement</title>

      <p id="d1e1271">This paper was edited by Federico Rossetti and reviewed by Emanuele Lodolo, Jacques Déverchère, and Guillermo Booth-Rea.</p>
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<abstract-html><p>Progress in the understanding and dating of the sedimentary record of the Alboran Basin allows us to propose a model of its tectonic evolution since the Pliocene. After a period of extension, the Alboran Basin underwent a progressive tectonic inversion starting around 9–7.5&thinsp;Ma. The Alboran Ridge is a NE–SW transpressive structure accommodating the shortening in the basin. We mapped its southwestern termination, a Pliocene rhombic structure exhibiting series of folds and thrusts. The active
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evolves from transpressive to transtensive along the AIF and the Nekor
Basin. This system reflects the logical evolution of the deformation of the
Alboran Basin under the indentation of the African lithosphere.</p></abstract-html>
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