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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-7-1003-2016</article-id><title-group><article-title>Tectonothermal evolution in the core of an arcuate fold and thrust belt: the
south-eastern sector of the Cantabrian Zone<?xmltex \hack{\newline}?> (Variscan belt, north-western Spain)</article-title>
      </title-group><?xmltex \runningtitle{Tectonothermal evolution in the core of an arcuate fold and thrust belt}?><?xmltex \runningauthor{M.~L.~Val\'{\i}n et al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Valín</surname><given-names>María Luz</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>García-López</surname><given-names>Susana</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Brime</surname><given-names>Covadonga</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="yes" rid="aff1">
          <name><surname>Bastida</surname><given-names>Fernando</given-names></name>
          <email>bastida@geol.uniovi.es</email>
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Aller</surname><given-names>Jesús</given-names></name>
          
        </contrib>
        <aff id="aff1"><institution>Departamento de Geología, Universidad de Oviedo, 33005 Oviedo, Spain</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Fernando Bastida (bastida@geol.uniovi.es)</corresp></author-notes><pub-date><day>11</day><month>July</month><year>2016</year></pub-date>
      
      <volume>7</volume>
      <issue>4</issue>
      <fpage>1003</fpage><lpage>1022</lpage>
      <history>
        <date date-type="received"><day>16</day><month>March</month><year>2016</year></date>
           <date date-type="rev-request"><day>4</day><month>April</month><year>2016</year></date>
           <date date-type="rev-recd"><day>10</day><month>June</month><year>2016</year></date>
           <date date-type="accepted"><day>17</day><month>June</month><year>2016</year></date>
      </history>
      <permissions>
<license license-type="open-access">
<license-p>This work is licensed under a Creative Commons Attribution 3.0 Unported License. To view a copy of this license, visit <ext-link ext-link-type="uri" xlink:href="http://creativecommons.org/licenses/by/3.0/">http://creativecommons.org/licenses/by/3.0/</ext-link></license-p>
</license>
</permissions><self-uri xlink:href="https://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>
    <p>The tectonothermal evolution of an area located in the core of the
Ibero-Armorican Arc (Variscan belt) has been determined by using the conodont
colour alteration index (CAI), Kübler index of illite (KI), the Árkai
index of chlorite (AI) and the analysis of clay minerals and rock cleavage.
The area is part of the Cantabrian Zone (CZ), which represents the foreland
fold and thrust belt of the orogen. It has been thrust by several large units
of the CZ, what resulted in the generation of a large number of synorogenic
Carboniferous sediments. CAI, KI and AI values show an irregular distribution
of metamorphic grade, independent of stratigraphic position. Two
tectonothermal events have been distinguished in the area. The first one,
poorly defined, is mainly located in the northern part. It gave rise to very-low-grade metamorphism in some areas and it was associated with a deformation
event that resulted in the emplacement of the last large thrust unit and
development of upright folds and associated cleavage (<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>S</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>. The second
tectonothermal event gave rise to low-grade metamorphism and cleavage
(<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>S</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> crosscutting earlier upright folds in the central, western and
southern parts of the study area. The event continued with the intrusion of
small igneous rock bodies, which gave rise to contact metamorphism and
hydrothermal alteration. This event was linked to an extensional episode due
to a gravitational instability at the end of the Variscan deformation. This
tectonothermal evolution occurred during the Gzhelian–Sakmarian.
Subsequently, several hydrothermal episodes took place and local crenulation
cleavage developed during the Alpine deformation.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <title>Introduction</title>
      <p>The Variscan belt defines an arc in the north-western Iberian Peninsula
(Ibero-Armorican Arc) whose core is formed by the Cantabrian Zone (CZ),
which represents the foreland fold and thrust belt of the orogen (Fig. 1).
This zone consists of Palaeozoic rocks in which two tectonostratigraphic
units have been distinguished (Julivert, 1978; Marcos and Pulgar, 1982),
whose limit is approximately located by the Devonian–Carboniferous boundary.
The pre-orogenic unit is formed of Cambrian to Devonian rocks consisting of
alternating carbonate and siliciclastic formations; they form a wedge that
thins towards the foreland. The synorogenic unit is formed by several clastic
units, also thinning towards the foreland, which filled foredeep basins
generated in the front of the main thrust units of the CZ. In this zone, the
Variscan deformation occurred during the upper Carboniferous and gave rise to
thin-skinned tectonics, with several large thrust units and associated folds
(Fig. 1); the units were emplaced in a sequence towards the foreland. The
deformation occurred under shallow crustal conditions, so that diagenetic
conditions are dominant in the zone and absence of cleavage in the rocks is
also dominant. Nevertheless, there are several areas of the CZ where cleavage
and very-low- or low-grade metamorphism are present. One of these areas is
the south-eastern sector of the CZ. It is a foreland basin that
occupies the core of the Ibero-Armorican Arc and has undergone a complex
history of sedimentation, deformation, metamorphism and, to a lesser extent,
magmatism.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1" specific-use="star"><caption><p>Generalized geological map of the Cantabrian Zone (after Julivert
1971) showing major thrust units and the location of the study area.</p></caption>
        <?xmltex \igopts{width=483.69685pt}?><graphic xlink:href="https://se.copernicus.org/articles/7/1003/2016/se-7-1003-2016-f01.pdf"/>

      </fig>

      <p>The present study aims to present a model of tectonothermal evolution for
the core of the Ibero-Armorican Arc based on conodont colour alteration
index (CAI), the Kübler index (KI) of illite, the Árkai index (AI)
of chlorite (Chl), the analysis of clay minerals and the rock cleavage
development.</p>
</sec>
<sec id="Ch1.S2">
  <title>Geological setting</title>
      <p>The south-eastern sector of the CZ is made up of two units: the
Pisuerga–Carrión unit (PCU) and the Valsurbio unit (VU) (Fig. 1). As a
consequence of its location in the core of the Ibero-Armorican Arc, the PCU
has been thrust over successively by the VU, the Central Coal Basin, the
Ponga unit and the Picos de Europa unit (Fig. 1). Thus, the PCU operated as a
foreland basin during a great part of the history of the Variscan
deformation. This history involved the accumulation of a great thickness of
synorogenic Carboniferous sediments, corresponding to clastic wedges
associated with the exhumation of the thrust units.</p>
      <p>The VU is located to the south of the PCU. Marine facies occur in both units,
but from the Emsian the sediments in the latter unit were deposited in
deeper waters than those in the former unit. The VU represents an extension
of the southern part of the CZ, and the Devonian succession of both is
comparable (Koopmans, 1962). The units within the PCU containing
Silurian–Devonian rocks have been interpreted as transported from internal
areas of the orogenic belt, specifically from the south-eastern extension of
the West Asturian–Leonese Zone, currently hidden under the Mesozoic–Cenozoic
cover of the Douro basin and located to the south of the VU (Frankenfeld,
1983; Marquínez and Marcos, 1984; Rodríguez Fernández and
Heredia, 1987; Rodríguez Fernández, 1994). These units were named
“Palentine nappes” by Rodríguez Fernández and Heredia (1987). The
PCU and the VU are separated by the León fault (also called “Ruesga
fault” in the study area) (Fig. 2) that crosses most of the CZ
and whose meaning is controversial (Alonso et al., 2009 and references
therein).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2" specific-use="star"><caption><p>Geological map of the south-eastern part of the Cantabrian Zone
showing sampled localities (composed from Lobato, 1977; Colmenero et al.,
1982; Ambrose et al., 1984; Julivert and Navarro, 1984; Martínez
García et al., 1984; Lobato et al., 1985; Heredia et al, 1986, 1991,
1997; Rodríguez Fernández, 1994; Rodríguez Fernández et
al., 1994). Devonian and Silurian rocks of the PCU form the Palentine
nappes; cg – conglomerate; l – limestone; m – marl; s – sandstone; sh – shale.
C –
Curavacas–Lechada syncline; I – Pico Iján granodiorite; J. Pico Jano
granodiorite; L – León fault; P – Peña Prieta granodiorite; PU – Ponga
unit; V – Ventaniella fault. Picos de Europa conodont samples after Bastida
et al. (2004); Valsurbio conodont samples after García-López et al. (2013). A–B indicates the location of cross section in Fig. 11.</p></caption>
        <?xmltex \igopts{width=569.055118pt, angle=-90}?><graphic xlink:href="https://se.copernicus.org/articles/7/1003/2016/se-7-1003-2016-f02.pdf"/>

      </fig>

      <p>The oldest sediments of the study area are Silurian (Wenlock–Pridoli)
sandstones and lutites. The Devonian rocks consist of an alternation of
carbonate and siliciclastic formations with the facies differences cited
above. Mississippian rocks are mainly limestones in the lower part,
especially in the VU; upwards a mostly turbiditic sequences appears
with common olistoliths in the northern sector and some carbonate levels.
The Pennsylvanian succession is dominantly siliciclastic, with a thickness
of several thousand metres and synorogenic character. In relation to this
synorogenic sedimentation, several syntectonic unconformities have been
described, among which the Curavacas unconformity (early Moscovian) can be
highlighted by its structural significance (Van Veen, 1965; Lobato, 1977;
Alonso and Rodríguez Fernández, 1983; Martín-Merino et al.,
2014).</p>
      <p>The first deformation events were pre-Curavacas (prior to or earliest
Moscovian) and involved the emplacement of the Palentine nappes and the VU.
Two generations of thrusts and associated folds occurred during this episode
(Rodríguez Fernández, 1994), which translated sequences northwards.
Further, some back thrusts and normal faults occurred.</p>
      <p>The post-Curavacas deformation events involved the development of several
generations of thrusts and high-angle reverse faults, folds, cleavages and
normal faults. Some thrusts have a trend approximately parallel to the basal
thrust of the Ponga unit and are probably related to the emplacement of this
thrust unit (Rodríguez Fernández and Heredia, 1987), which occurred
during the late Moscovian. In the same episode that involved the emplacement
of the Picos de Europa thrust unit during the Kasimovian–Gzhelian
(Merino-Tomé et al. 2009), N–S shortening occurred in the study area,
involving the development of thrusts, high-angle reverse faults and the
reactivation of older faults with a movement dominantly southward (Maas,
1974). In addition, upright folds with E–W axial trace developed; among
them, the Curavacas–Lechada syncline is remarkable for its notable dimensions
(Savage, 1967; Lobato, 1977; Rodríguez Fernández, 1994).</p>
      <p>Several cleavages have been recognised in the study area. Among them, a
gently dipping cleavage crosscutting folds is the most relevant and has been
described by various authors (Van Veen, 1965; Savage, 1967; Lobato, 1977; Van
der Pluijm et al., 1986; Rodríguez Fernández, 1994; Marín,
1997; García-López et al., 2007; and reference therein).</p>
      <p>A subsequent N–S shortening episode occurred during the Alpine deformation.
It involved tightening of folds, local development of crenulation cleavage
and reactivation of some faults. It is responsible for the dome geometry of
the VU (Marín et al., 1995; Marín, 1997). Another post-Variscan
structure of the study area is the Ventaniella fault, which traverses the
whole CZ in a NW–SE direction. It is essentially a dextral,
strike–slip fault with a net slip of 4–5 km (Julivert et al., 1971) whose
activity began in the Permian and continues to the present
(López-Fernández et al., 2004).</p>
      <p>Outcrops of intrusive igneous rocks are common in the PCU, and their
knowledge is important to understand the tectonothermal evolution of this
unit. Among these rocks, three granodioritic stocks (Pico Iján, Peña
Prieta and Pico Jano; Fig. 2) and many small outcrops can be distinguished.
The latter are mainly concentrated in the southern half of the unit.</p>
      <p>The stocks of Pico Iján, Peña Prieta and Pico Jano dominantly have
granodioritic composition and their intrusion was favoured by the existence
of faults (Suárez and García, 1974; Corretgé and Suárez,
1990), having developed a notable aureole of contact metamorphism in the case
of the Peña Prieta stock. The porphyroblasts in this aureole are
post-tectonic relative to the gently dipping cleavage (Gallastegui et al.,
1990; Rodríguez Fernández, 1994). The U/Pb age of the Peña
Prieta granitoid is Cisuralian (<inline-formula><mml:math display="inline"><mml:mrow><mml:mn>292</mml:mn><mml:mo>+</mml:mo><mml:mn mathvariant="normal">3</mml:mn><mml:mo>/</mml:mo><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> Ma after Valverde-Vaquero et al., 1999), and the Pico Iján
granitoid is nonconformably covered by Lower Triassic rocks. The large number
of small outcrops of igneous rocks that exist in the southern half of the
unit are concentrated in two areas (one in the eastern part and another in
the western part) joined by a band whose outcrops of igneous rocks have been
related to the León fault (Corretgé et al., 1987; Suárez and
Corretgé, 1987; Corretgé and Suárez, 1990). All these southern
outcrops have been, in general, related to fractures and appear as small
stocks, probably apophyses of bigger bodies in depth, and as sills or dikes.
Their composition is varied and ranges from granodioritic to gabbroic. In
some cases, they developed ore bodies close to their contacts
(Martín-Izard et al., 1986).</p>
      <p>Earlier metamorphic studies in the CZ using CAI and/or KI
methods have shown the existence of areas with very-low- or low-grade
metamorphism in the PCU and the VU (Raven and van der Pluijm, 1986; Keller
and Krumm, 1993; Marín et al., 1996; Marín, 1997; Köberle et
al., 1998; García-López et al., 1999, 2007, 2013; Bastida et al.,
2002; Clauer and Weh, 2014, and references therein). Similar results have been obtained
for the southern part of the study area using coal rank and vitrinite
reflectance (Colmenero and Prado, 1993; Llorens et al., 2006; Colmenero et
al., 2008; Clauer and Weh, 2014). This metamorphism has been described as
associated with a late-orogenic extensional event and with the corresponding
cleavage (García-López et al., 1999, 2007, 2013; Bastida et al.,
2002). Analysis of ore deposits and of the tectonothermal evolution in the
neighbouring unit of the Picos de Europa has defined a subsequent
hydrothermal episode during the Permian (Gómez-Fernández et al.,
1993, 2000; Bastida et al., 2004). Brime and Valín (2006) have suggested
a hydrothermal origin for mineral associations with chloritoid (Cld) and
pyrophyllite (Prl) found in samples of pelitic rocks collected in the study area.
K–Ar dating of illite in samples collected in the southern part of the study
area identified four thermal episodes (Clauer and Weh, 2014), namely at (1)
293 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 3 Ma (Cisuralian), (2) 268 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 6 Ma (Guadalupian), (3)
243 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 5 Ma (middle Triassic) and (4) 175 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 6 Ma (early–middle
Jurassic). Low-temperature thermochronology studies by Fillon et al. (2016)
in three samples of Westphalian sandstones collected in the northern and
central parts of the PCU, provided cooling ages below 180 <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C by
37–39 Ma. They inferred Cenozoic erosion of a rock thickness between 6.4
and 8 km (assuming a steady-state geothermal gradient of
25 <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C km<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>.</p>
</sec>
<sec id="Ch1.S3">
  <title>Methods</title>
<sec id="Ch1.S3.SS1">
  <title>X-ray diffraction (XRD)</title>
      <p>A total of 297 mudrocks from various localities (Fig. 2) were studied by
XRD analysis in order to determine their phyllosilicate
mineralogy, KI of illites and AI of
chlorites. Preparation of samples and methods for XRD analysis follow
the methods described in Brime et al. (2003)</p>
      <p>Reaction progress in illitic minerals (sensu Środoń, 1984) has been
widely used to assess the evolution of pelitic lithologies during diagenesis
and low-grade metamorphism. Prograde changes can be identified by use of the
KI technique (illite “crystallinity”; see Guggenheim et
al,. 2002) involving quantification of the width of the 10 Å peak of
illite. This is an indirect measure of lattice reorganisation and thickening
of illite crystals (Kisch, 1983; Merriman and Peacor, 1999) with increasing
grade. The KI is expressed in <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mo>∘</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula>2<inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">θ</mml:mi></mml:math></inline-formula>
to minimise variations caused by differences in recording conditions. For
this study the KI was measured using a laboratory procedure similar to that
outlined by the IGCP 294 working group (Kisch, 1991). The numerical KI value
decreases with improving “crystallinity” and is expressed as small changes
in the Bragg angle <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mo>∘</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula>2<inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">θ</mml:mi></mml:math></inline-formula>, using Cu K<inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">α</mml:mi></mml:math></inline-formula>
radiation.</p>
      <p>The transient zone between diagenesis and metamorphism (the anchizone of
Kübler, 1967) is defined by KI values between 0.42<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> and 0.25
<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mo>∘</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula>2<inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">θ</mml:mi></mml:math></inline-formula> respectively (Kisch, 1991). The values obtained
in our laboratory were correlated with the Kübler scale using a
calibration curve based on data obtained from polished slate standards kindly
provided by H. Kisch. The diagenetic zone has been subdivided in shallow (KI
&gt; 1 <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mo>∘</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula>2<inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="italic">θ</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> and deep
(1.0<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> &gt; KI &gt; 0.42 <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mo>∘</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula>2<inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">θ</mml:mi></mml:math></inline-formula>), using the terms proposed by the IUGS Subcommission on the
Systematics of Metamorphic rocks (Árkai et al., 2007). Following Merriman
and Peacor (1999) we have divided the anchizone into low (0.42 &lt; KI
&lt;0.30 <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mo>∘</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula>2<inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">θ</mml:mi></mml:math></inline-formula>) and high (0.30 &lt; KI
&lt;0.25 <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mo>∘</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula>2<inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">θ</mml:mi></mml:math></inline-formula>).</p>
      <p>Crystallinity index standards (CISs; Warr and Rice, 1994) have also been used
to compare the results thus obtained with other published results using that
scale. KI values obtained in this work could be converted to the CIS scale by
using the calibration reaction:
            <disp-formula id="R1" content-type="numbered reaction"><mml:math display="block"><mml:mrow><mml:msub><mml:mtext>KI</mml:mtext><mml:mtext>CIS</mml:mtext></mml:msub><mml:mo>=</mml:mo><mml:mn>1.505</mml:mn><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msub><mml:mtext>KI</mml:mtext><mml:mtext>this  work</mml:mtext></mml:msub><mml:mo>-</mml:mo><mml:mn>0.046</mml:mn><mml:mo>(</mml:mo><mml:msup><mml:mi>R</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>=</mml:mo><mml:mn>0.996</mml:mn><mml:mo>)</mml:mo><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula>
          For the problems involved in the use of the CIS scale to assess metamorphic
grade, see Brime (1999) and Kisch et al. (2005).</p>
      <p>The KI method does not allow temperature constraints to be placed on the
upper and lower boundaries of the anchizone and it is more likely to be a
measure of reaction progress than of the thermodynamic equilibrium achieved
(Essene and Peacor, 1995). However, this method, in combination with others
such as fluid inclusions or reflectance of carbonaceous material, indicates
that the transition diagenesis–anchizone could be correlated with a
temperature of 230 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 10 <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C, whereas the limit
anchizone–epizone would be at 300 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 10 <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C (Müllis, 1979;
Frey et al., 1980; Frey, 1987; Von Gosen et al., 1991; Müllis et al.,
1995, 2002; Merriman and Frey, 1999; Ferreiro Mählmann et al., 2002).</p>
      <p>The presence of illite/smectite (I/S) and paragonite (Pg) and
paragonite/muscovite (Pg/Ms) hampers determination of KI of many
samples. However, pro-grade changes can also be identified by use of the
AI technique (of chlorite “crystallinity”; see Guggenheim et
al., 2002) involving quantification of the width of the 14 Å or 7 Å
peaks of chlorite (Árkai, 1991; Meunier, 2005). The AI
was determined in the 002 peak using the same instrumental conditions as
those for KI measurements. The anchizone limits have been established using
samples free of I/S and Pg–Pg/Ms in which the KI measured in the air-dried samples has been calibrated with Kisch standards. The AI was measured
in the same samples and the regression line obtained allowed the delimitation
of the upper and lower anchizone limits using chlorite for AI values of 0.234
and 0.135 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">Δ</mml:mi></mml:math></inline-formula><inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>2<inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">θ</mml:mi></mml:math></inline-formula> respectively. It should be noted that
AI values are smaller than the corresponding KI and the method is therefore
slightly less sensitive than KI method.</p>
</sec>
<sec id="Ch1.S3.SS2">
  <title>Conodont colour alteration index</title>
      <p>Colour changes in conodont elements are related to the progressive and
irreversible alteration of the amounts of organic matter within their apatite
composition. The CAI method is based on analysis of the colour changes that
the conodonts undergo in response of the organic matter to a temperature
increase with time. These changes permit construction of a scale of CAI
values with eight units that allows the use of the conodonts as maximum
palaeothermometers for a temperature interval of between 50 and
600 <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C (Epstein et al., 1977; Rejebian et al., 1987). It is used
mainly in carbonate rocks. Besides colour changes, apatite textural
alteration also takes place and can provide complementary information about
the thermal conditions. In the present paper the terminology of Rejebian et
al. (1987) and García-López et al. (1997, 2006) is used for the
textural description of conodonts. In agreement with Rejebian et al. (1987),
well-preserved conodonts and high CAI values with a wide dispersion are
indicative of contact metamorphism. Furthermore, coarse recrystallisation and
corrosion are related to hydrothermal processes.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3"><caption><p>Arrhenius plot to determine palaeotemperature from CAI values (on
the lines) and heating time (from Rejebian et al., 1987). Point A indicates
the minimum temperature necessary to obtain a CAI <inline-formula><mml:math display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 5 for a rock with an
age of 400 Ma. The green area shows the temperatures and heating times
unable to produce CAI <inline-formula><mml:math display="inline"><mml:mo>≥</mml:mo></mml:math></inline-formula> 5 in this rock.</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://se.copernicus.org/articles/7/1003/2016/se-7-1003-2016-f03.pdf"/>

        </fig>

      <p>Samples were collected from the Pisuerga–Carrión and Valsurbio units. CAI
values are based on 5 kg samples of limestone that were treated with 6 %
acetic acid solution. Unfortunately, recovery of conodonts from Carboniferous
rocks was hindered in some areas by their dominantly siliciclastic character.
Sampling was complemented with specimens from collections housed at the
University of Oviedo (Spain) and those of the National Museum of Natural
History at Leiden (Netherlands) and Institut und Museum für Geologie und
Paläontologie in Göttingen (Germany) (Fig. 2); 213 positive samples,
corresponding to an age interval from the Pridoli to Gzhelian, were analysed
for CAI determination (Supplement 1 in the supplementary material).</p>
      <p>The methodology involved in CAI determination can be found in
García-López et al. (1997) and Bastida et al. (1999). Several CAI
values were obtained from most samples and the mean of CAI values has been
determined for each of them in order to tentatively contour CAI values.
Samples with a range higher than 1.5 have not been used to obtain mean CAI
values and temperatures. The interpretation of the results is mainly based on
the analysis of the CAI isograds and their relationship to the stratigraphic
contacts and the main structures of the study area.</p>
      <p>For the metamorphic zonation from CAI data, we use the terminology described
by García-López et al. (2001) that involves a division in
diacaizone (CAI &lt; 4), ancaizone (4 <inline-formula><mml:math display="inline"><mml:mo>≤</mml:mo></mml:math></inline-formula> CAI <inline-formula><mml:math display="inline"><mml:mo>≤</mml:mo></mml:math></inline-formula> 5.5) and
epicaizone (CAI &gt; 5.5).</p>
      <p>Temperature ranges of the CAI values were obtained from the Arrhenius plot
presented by Epstein et al. (1977) and Rejebian et al. (1987). The maximum
possible heating time is the age of the rock. Nevertheless, it is possible to
place greater limits on this maximum time (García-López et al.,
2013). According to the Arrhenius plot a minimum temperature is required to
obtain a specific CAI value. For example, in a rock with an age of 400 Ma
(Devonian), development of CAI <inline-formula><mml:math display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 5 requires at least 290 <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C
(point A in Fig. 3). Then, it can be assumed that a
temperature &lt; 290 <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C does not contribute to the generation of a
CAI <inline-formula><mml:math display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 5. Hence, to produce a given CAI, the maximum time of heating
begins when the rock reaches the minimum temperature necessary to produce
that CAI, and it ends when the rock cools down and the temperature becomes
lower than this minimum value. Although the heating time can be slightly
different depending on the geological location of the samples, we consider
that the main heating time corresponds to a late-Variscan period that began
at the boundary Kasimovian–Gzhelian and ended at the beginning of the
Triassic (heating time of about 50 Ma); this agrees with the age of the
metamorphism analysed below and the igneous rocks. The hydrothermal
post-Variscan episodes described by Clauer and Weh (2014) probably involved
lower temperatures than those reached in the late-Variscan event, in which
magmatism and cleavage development are more intense. It must be taken into
account that, in rocks undergoing more than one heating period, the period to
be considered for the development of the CAI is the one which generated
higher temperatures. In any case, due to the geometry of the CAI curves in the
Arrhenius plot, for heating intervals such as those involved in the present
case, an error of a few Ma in the maximum time of heating has little
influence on the results. According to Patrick et al. (1985) and Rejebian et
al. (1987), the minimum time of heating assumed here is  1 Ma.</p>
</sec>
<sec id="Ch1.S3.SS3">
  <title>Cleavage</title>
      <p>Development of cleavage requires mineralogical and microstructural changes
due to ductile deformation, involving mechanisms, such as pressure solution,
that require a minimum temperature of about 200 <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C for cleavage
development in pelitic rocks and 175 <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C in limestones (Groshong et
al. 1984). Thus widespread presence of cleavage occurs below a certain
crustal level (minimum overburden of 5–7 km; Engelder and Marshak, 1985).
Furthermore, the relations between folds and cleavages and the overprinting
relations between cleavages play an important role in defining deformation
events (Passchier and Trouw, 2005). In addition, cleavage is also a key
structure to establish chronological relations between metamorphic
crystallisation and deformation.</p>
      <p>In the context of the study area, we refer to a tectonothermal event as a
deformational event with cleavage development and associated metamorphic
conditions, and we use the term thermal event for metamorphic conditions
without cleavage development.</p>
</sec>
</sec>
<sec id="Ch1.S4">
  <title>Results and interpretation</title>
      <p>In order to facilitate description, the samples have been mainly grouped in
the following areas, namely Liébana, Valdeón, Yuso–Carrión,
Pisuerga, Riaño–Cervera and Valsurbio (Fig. 4) (cf. Martín-Merino et
al., 2014).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4"><caption><p>Diagrammatic map indicating the areas in which the study units have
been subdivided, following Martín-Merino et al. (2014).</p></caption>
        <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://se.copernicus.org/articles/7/1003/2016/se-7-1003-2016-f04.pdf"/>

      </fig>

<sec id="Ch1.S4.SS1">
  <title>Clay minerals</title>
<sec id="Ch1.S4.SS1.SSS1">
  <title>Clay mineral assemblages</title>
      <p>Mineralogical analysis of the &lt; 2 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>m fractions shows that
dioctahedral K-rich mica-like structures (referred to as illite or muscovite) is present in all the samples with the majority also containing
Chl (Fig. 5). Chlorites have poorly developed 14 Å peaks,
indicating high iron content suggestive of chamositic compositions (Moore and
Reynolds, 1997). Other phases such as ordered illite/smectite (I/S) or
Pg and mixed layers Pg/Ms are also
common. Asymmetry of peaks and sample behaviour after glycolation indicate
the presence of ordered illite/smectite (I/S). Absence of random
I/S indicate that zone 3 of Eberl (1993) has been reached, suggesting
that temperatures exceeded 100 <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C. Kaolinite (Kln) and pyrophyllite
may also be present in some samples and are abundant in a few samples.
In addition, Cld is also present and widespread in the study
area. However, it is more abundant in samples close to the intrusions and/or
faults in which case is found together with chlorite and Pg <inline-formula><mml:math display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> Pg/Ms.
Only in samples to the east (Pisuerga Area), where it is not as abundant, may it
be associated with Prl, Kln or I/S. Finally, chlorite/vermiculite mixed
layer(C/V) and stilpnomelane (Stp) have been found, in small amounts,
in a few samples and are restricted to samples to the eastern Pisuerga and
eastern Yuso–Carrión areas.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F5" specific-use="star"><caption><p>Distribution of clay minerals in the study area. All the samples
contain illite and therefore this phase has not been considered in the plot.
Presence of a certain phase in the sample is indicated by the colour in the
corresponding square. I – Pico Iján granodiorite; P – Peña Prieta
granodiorite. For legend see Fig. 8.</p></caption>
            <?xmltex \igopts{width=597.507874pt, angle=-90}?><graphic xlink:href="https://se.copernicus.org/articles/7/1003/2016/se-7-1003-2016-f05.png"/>

          </fig>

      <p>The I/S is more abundant to the north and east (Valdeón, Liébana, and
eastern part of the Pisuerga and Yuso–Carrión areas) and the presence of Kln is
almost restricted to samples to the east (Pisuerga and eastern part of the
Yuso–Carrión areas). Prl is common in samples from the central and
north-eastern parts (Liébana and Pisuerga areas and eastern part of the
Yuso–Carrión area) (Fig. 5). Quartz, calcite, feldspars and goethite were
accessory phases recognised in some samples.</p>
      <p>In general the assemblages found are, in order of abundance of the most
frequent phase besides illite (<inline-formula><mml:math display="inline"><mml:mrow><mml:mi>n</mml:mi><mml:mo>=</mml:mo><mml:mn>291</mml:mn></mml:mrow></mml:math></inline-formula>),
              <disp-formula id="Ch1.Ex1"><mml:math display="block"><mml:mrow><?xmltex \hack{\hbox\bgroup\fontsize{7.0}{7.0}\selectfont$\displaystyle}?><mml:mtable class="array" rowspacing="5.690551pt 5.690551pt 5.690551pt 5.690551pt 5.690551pt 5.690551pt" columnalign="left"><mml:mtr><mml:mtd><mml:mrow><mml:mrow class="chem"><mml:mi mathvariant="normal">I</mml:mi></mml:mrow><mml:mo>+</mml:mo><mml:mi mathvariant="bold">Chl</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mo>(</mml:mo><mml:mi>n</mml:mi><mml:mo>=</mml:mo><mml:mn>215</mml:mn><mml:mo>)</mml:mo><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mo>±</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mrow class="chem"><mml:mi mathvariant="normal">Pg</mml:mi></mml:mrow><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mo>±</mml:mo><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mrow class="chem"><mml:mi mathvariant="normal">Pg</mml:mi></mml:mrow><mml:mo>/</mml:mo><mml:mrow class="chem"><mml:mi mathvariant="normal">Ms</mml:mi></mml:mrow><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mo>±</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mrow class="chem"><mml:mi mathvariant="normal">Cld</mml:mi></mml:mrow><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mo>±</mml:mo><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mrow class="chem"><mml:mi mathvariant="normal">I</mml:mi></mml:mrow><mml:mo>/</mml:mo><mml:mrow class="chem"><mml:mi mathvariant="normal">S</mml:mi></mml:mrow><mml:mo>±</mml:mo><mml:mo>[</mml:mo><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi></mml:mrow><mml:mo>/</mml:mo><mml:mrow class="chem"><mml:mi mathvariant="normal">V</mml:mi></mml:mrow><mml:mo>]</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mo>±</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mo>[</mml:mo><mml:mrow class="chem"><mml:mi mathvariant="normal">Prl</mml:mi></mml:mrow><mml:mo>]</mml:mo><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mo>±</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mo>[</mml:mo><mml:mrow class="chem"><mml:mi mathvariant="normal">Kln</mml:mi></mml:mrow><mml:mo>]</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mo>±</mml:mo><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mo>[</mml:mo><mml:mrow class="chem"><mml:mi mathvariant="normal">Stp</mml:mi></mml:mrow><mml:mo>]</mml:mo></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mrow><mml:mrow class="chem"><mml:mi mathvariant="normal">I</mml:mi></mml:mrow><mml:mo>+</mml:mo><mml:mi mathvariant="bold">Pg</mml:mi><mml:mo>+</mml:mo><mml:mi mathvariant="bold">Pg</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="bold">Ms</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mo>(</mml:mo><mml:mi>n</mml:mi><mml:mo>=</mml:mo><mml:mn>162</mml:mn><mml:mo>)</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mo>±</mml:mo><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mrow class="chem"><mml:mi mathvariant="normal">Chl</mml:mi></mml:mrow><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mo>±</mml:mo><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mrow class="chem"><mml:mi mathvariant="normal">Cld</mml:mi></mml:mrow><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mo>±</mml:mo><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mo>[</mml:mo><mml:mrow class="chem"><mml:mi mathvariant="normal">I</mml:mi></mml:mrow><mml:mo>/</mml:mo><mml:mrow class="chem"><mml:mi mathvariant="normal">S</mml:mi></mml:mrow><mml:mo>]</mml:mo><mml:mo>±</mml:mo><mml:mo>[</mml:mo><mml:mrow class="chem"><mml:mi mathvariant="normal">Prl</mml:mi></mml:mrow><mml:mo>]</mml:mo><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mo>±</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mo>[</mml:mo><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi></mml:mrow><mml:mo>/</mml:mo><mml:mrow class="chem"><mml:mi mathvariant="normal">V</mml:mi></mml:mrow><mml:mo>]</mml:mo><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mo>±</mml:mo><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mo>[</mml:mo><mml:mrow class="chem"><mml:mi mathvariant="normal">Kln</mml:mi></mml:mrow><mml:mo>]</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mo>±</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mo>[</mml:mo><mml:mrow class="chem"><mml:mi mathvariant="normal">Stp</mml:mi></mml:mrow><mml:mo>]</mml:mo></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mrow><mml:mrow class="chem"><mml:mi mathvariant="normal">I</mml:mi></mml:mrow><mml:mo>+</mml:mo><mml:mi mathvariant="bold">I</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="bold">S</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mo>(</mml:mo><mml:mi>n</mml:mi><mml:mo>=</mml:mo><mml:mn>112</mml:mn><mml:mo>)</mml:mo><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mo>±</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mrow class="chem"><mml:mi mathvariant="normal">Chl</mml:mi></mml:mrow><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mo>±</mml:mo><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mrow class="chem"><mml:mi mathvariant="normal">Kln</mml:mi></mml:mrow><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mo>±</mml:mo><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mrow class="chem"><mml:mi mathvariant="normal">Prl</mml:mi></mml:mrow><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mo>±</mml:mo><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi></mml:mrow><mml:mo>/</mml:mo><mml:mrow class="chem"><mml:mi mathvariant="normal">V</mml:mi></mml:mrow><mml:mo>±</mml:mo><mml:mrow class="chem"><mml:mi mathvariant="normal">Pg</mml:mi></mml:mrow><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mo>±</mml:mo><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mrow class="chem"><mml:mi mathvariant="normal">Pg</mml:mi></mml:mrow><mml:mo>/</mml:mo><mml:mrow class="chem"><mml:mi mathvariant="normal">Ms</mml:mi></mml:mrow><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mo>±</mml:mo><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi></mml:mrow><mml:mo>/</mml:mo><mml:mrow class="chem"><mml:mi mathvariant="normal">V</mml:mi></mml:mrow><mml:mo>±</mml:mo><mml:mo>[</mml:mo><mml:mrow class="chem"><mml:mi mathvariant="normal">Cld</mml:mi></mml:mrow><mml:mo>]</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mo>±</mml:mo><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mo>[</mml:mo><mml:mrow class="chem"><mml:mi mathvariant="normal">Stp</mml:mi></mml:mrow><mml:mo>]</mml:mo></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mrow><mml:mrow class="chem"><mml:mi mathvariant="normal">I</mml:mi></mml:mrow><mml:mo>+</mml:mo><mml:mi mathvariant="bold">Cld</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mo>(</mml:mo><mml:mi>n</mml:mi><mml:mo>=</mml:mo><mml:mn>93</mml:mn><mml:mo>)</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mo>±</mml:mo><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mrow class="chem"><mml:mi mathvariant="normal">Chl</mml:mi></mml:mrow><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mo>±</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mrow class="chem"><mml:mi mathvariant="normal">Pg</mml:mi></mml:mrow><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mo>±</mml:mo><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mrow class="chem"><mml:mi mathvariant="normal">Pg</mml:mi></mml:mrow><mml:mo>/</mml:mo><mml:mrow class="chem"><mml:mi mathvariant="normal">Ms</mml:mi></mml:mrow><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mo>±</mml:mo><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mrow class="chem"><mml:mi mathvariant="normal">I</mml:mi></mml:mrow><mml:mo>/</mml:mo><mml:mrow class="chem"><mml:mi mathvariant="normal">S</mml:mi></mml:mrow><mml:mo>±</mml:mo><mml:mo>[</mml:mo><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi></mml:mrow><mml:mo>/</mml:mo><mml:mrow class="chem"><mml:mi mathvariant="normal">V</mml:mi></mml:mrow><mml:mo>]</mml:mo><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mo>±</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mo>[</mml:mo><mml:mrow class="chem"><mml:mi mathvariant="normal">Prl</mml:mi></mml:mrow><mml:mo>]</mml:mo><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mo>±</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mo>[</mml:mo><mml:mrow class="chem"><mml:mi mathvariant="normal">Kln</mml:mi></mml:mrow><mml:mo>]</mml:mo><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mo>±</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mo>[</mml:mo><mml:mrow class="chem"><mml:mi mathvariant="normal">Stp</mml:mi></mml:mrow><mml:mo>]</mml:mo></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mrow><mml:mrow class="chem"><mml:mi mathvariant="normal">I</mml:mi></mml:mrow><mml:mo>+</mml:mo><mml:mi mathvariant="bold">Prl</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mo>(</mml:mo><mml:mi>n</mml:mi><mml:mo>=</mml:mo><mml:mn>56</mml:mn><mml:mo>)</mml:mo><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mo>±</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mrow class="chem"><mml:mi mathvariant="normal">I</mml:mi></mml:mrow><mml:mo>/</mml:mo><mml:mrow class="chem"><mml:mi mathvariant="normal">S</mml:mi></mml:mrow><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mo>±</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mrow class="chem"><mml:mi mathvariant="normal">Chl</mml:mi></mml:mrow><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mo>±</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mrow class="chem"><mml:mi mathvariant="normal">Pg</mml:mi></mml:mrow><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mo>±</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mrow class="chem"><mml:mi mathvariant="normal">Pg</mml:mi></mml:mrow><mml:mo>/</mml:mo><mml:mrow class="chem"><mml:mi mathvariant="normal">Ms</mml:mi></mml:mrow><mml:mo>±</mml:mo><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi></mml:mrow><mml:mo>/</mml:mo><mml:mrow class="chem"><mml:mi mathvariant="normal">V</mml:mi></mml:mrow><mml:mo>±</mml:mo><mml:mo>[</mml:mo><mml:mrow class="chem"><mml:mi mathvariant="normal">Cld</mml:mi></mml:mrow><mml:mo>]</mml:mo><mml:mo>±</mml:mo><mml:mo>[</mml:mo><mml:mrow class="chem"><mml:mi mathvariant="normal">Kln</mml:mi></mml:mrow><mml:mo>]</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mo>±</mml:mo><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mo>[</mml:mo><mml:mrow class="chem"><mml:mi mathvariant="normal">Stp</mml:mi></mml:mrow><mml:mo>]</mml:mo></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mrow><mml:mrow class="chem"><mml:mi mathvariant="normal">I</mml:mi></mml:mrow><mml:mo>+</mml:mo><mml:mi mathvariant="bold">C</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="bold">V</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mo>(</mml:mo><mml:mi>n</mml:mi><mml:mo>=</mml:mo><mml:mn>48</mml:mn><mml:mo>)</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mo>±</mml:mo><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mrow class="chem"><mml:mi mathvariant="normal">I</mml:mi></mml:mrow><mml:mo>/</mml:mo><mml:mrow class="chem"><mml:mi mathvariant="normal">S</mml:mi></mml:mrow><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mo>±</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mrow class="chem"><mml:mi mathvariant="normal">Chl</mml:mi></mml:mrow><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mo>±</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mrow class="chem"><mml:mi mathvariant="normal">Pg</mml:mi></mml:mrow><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mo>±</mml:mo><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mrow class="chem"><mml:mi mathvariant="normal">Pg</mml:mi></mml:mrow><mml:mo>/</mml:mo><mml:mrow class="chem"><mml:mi mathvariant="normal">Ms</mml:mi></mml:mrow><mml:mo>±</mml:mo><mml:mrow class="chem"><mml:mi mathvariant="normal">Kln</mml:mi></mml:mrow><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mo>±</mml:mo><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mrow class="chem"><mml:mi mathvariant="normal">Prl</mml:mi></mml:mrow><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mo>±</mml:mo><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mrow class="chem"><mml:mi mathvariant="normal">Cld</mml:mi></mml:mrow><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mo>±</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mo>[</mml:mo><mml:mrow class="chem"><mml:mi mathvariant="normal">Stp</mml:mi></mml:mrow><mml:mo>]</mml:mo></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mrow><mml:mrow class="chem"><mml:mi mathvariant="normal">I</mml:mi></mml:mrow><mml:mo>+</mml:mo><mml:mi mathvariant="bold">Kln</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mo>(</mml:mo><mml:mi>n</mml:mi><mml:mo>=</mml:mo><mml:mn>39</mml:mn><mml:mo>)</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mo>±</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mrow class="chem"><mml:mi mathvariant="normal">I</mml:mi></mml:mrow><mml:mo>/</mml:mo><mml:mrow class="chem"><mml:mi mathvariant="normal">S</mml:mi></mml:mrow><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mo>±</mml:mo><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mrow class="chem"><mml:mi mathvariant="normal">Chl</mml:mi></mml:mrow><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mo>±</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi></mml:mrow><mml:mo>/</mml:mo><mml:mrow class="chem"><mml:mi mathvariant="normal">V</mml:mi></mml:mrow><mml:mo>±</mml:mo><mml:mo>[</mml:mo><mml:mrow class="chem"><mml:mi mathvariant="normal">Prl</mml:mi></mml:mrow><mml:mo>]</mml:mo><mml:mo>±</mml:mo><mml:mo>[</mml:mo><mml:mrow class="chem"><mml:mi mathvariant="normal">Cld</mml:mi></mml:mrow><mml:mo>]</mml:mo><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mo>±</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mo>[</mml:mo><mml:mrow class="chem"><mml:mi mathvariant="normal">Pg</mml:mi></mml:mrow><mml:mo>]</mml:mo><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mo>±</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mo>[</mml:mo><mml:mrow class="chem"><mml:mi mathvariant="normal">Pg</mml:mi></mml:mrow><mml:mo>/</mml:mo><mml:mrow class="chem"><mml:mi mathvariant="normal">Ms</mml:mi></mml:mrow><mml:mo>]</mml:mo><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mo>±</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mo>[</mml:mo><mml:mrow class="chem"><mml:mi mathvariant="normal">Stp</mml:mi></mml:mrow><mml:mo>]</mml:mo><mml:mo>.</mml:mo></mml:mrow></mml:mtd></mml:mtr></mml:mtable><?xmltex \hack{$\egroup}?></mml:mrow></mml:math></disp-formula></p>
</sec>
<sec id="Ch1.S4.SS1.SSS2">
  <?xmltex \opttitle{K\"{u}bler index}?><title>Kübler index</title>
      <p>As mentioned above, determination of KI has been hampered by the presence in
some samples of certain types of I/S and big amounts of Pg or Prl, in
relation to the amount of illite, that interfere with the 001 peak of illite,
therefore rendering their KI values useless for grade determination using KI,
even in the glycolated state. As a result, 23 (indicated in italic
in Supplement 2) of the 291 samples studied
yielded doubtful KI values (Figs. 6, 7; Supplement 2). They are included, nevertheless, as they indicate maximum value of
the KI.</p>
      <p>Grade ranges from deep diagenetic to epizonal, but deep diagenetic and
mainly low anchizonal metapelites are predominant in most of the areas
(Figs. 6 and 7). Expandability of the 10 Å peak is only lost at the high
anchizone to epizone boundary. Deep diagenetic areas can be found to the
north (Liébana and Valdeón areas). The Riaño–Cervera area is
mainly low anchizonal with a few samples being diagenetic or deep
anchizonal. In the Pisuerga area, the grade ranges from deep diagenetic to
low anchizonal (Figs. 6, 7). Higher-grade (epizonal) samples may appear in
any formation and they are more abundant in the western part of the
Yuso–Carrión area, where the Peña Prieta granodiorite is located,
and in the Devonian of the Valsurbio area (Fig. 7). In both cases, it is in
those high-grade samples where chloritoid is more abundant (Fig. 6).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F6" specific-use="star"><caption><p>Map showing the location of Kübler index (KI) values
(<inline-formula><mml:math display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula>100) (Kübler scale). Upper value, in red, is the air-dried sample;
lower value, in green, is the sample treated with ethylene glycol. Árkai index
(AI) is indicated by the colour of the sampling point. Values corresponding
to samples with significant amounts of I/S, Prl and/or Pg–Pg/Ms
have not been highlighted with grade colours. For legend see Fig. 8.</p></caption>
            <?xmltex \igopts{width=597.507874pt, angle=-90}?><graphic xlink:href="https://se.copernicus.org/articles/7/1003/2016/se-7-1003-2016-f06.png"/>

          </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F7" specific-use="star"><caption><p>Plot of Kübler index (KI) measured on air-dried (AD) vs. KI
measured on ethylene glycol solvated samples (EG), standardised at Kübler
scale. DD – shallow diagenesis; LA – low anchizone; HA – high anchizone; Ep – epizone. Samples are plotted according to the areas outlined in Fig. 4 and
have been grouped following the divisions of Fig. 2: A – Silurian; B –
Devonian; C – Tournaisian–Visean; D – Prioro Group; E – Pando Group; F –
Viorna Group; G – Campollo–Remoña Group. Samples with significant
amounts of I/S, Prl and/or Pg–Pg/Ms are indicated as NA (not
applicable). Minerals absent in each of the areas are indicated in red.</p></caption>
            <?xmltex \igopts{width=483.69685pt}?><graphic xlink:href="https://se.copernicus.org/articles/7/1003/2016/se-7-1003-2016-f07.png"/>

          </fig>

      <p>Work in progress on the variation of the chemical composition of the
phyllosilicates of the study area allowed estimation of temperatures using
Battaglia's (2004) approach based in the variation in the chemical
composition of illites. Temperatures obtained are in the range
230–280 <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C, consistent with the anchizonal KI values of the analysed
samples. The observed deficit in layer charge (Brime and Valín, 2006) is
characteristic of anchizonal K white mica (Hunziker et al., 1986; Livi et
al., 1997; Merriman and Peacor, 1999; Árkai, 2002; Árkai et al.,
2003).</p>
</sec>
<sec id="Ch1.S4.SS1.SSS3">
  <?xmltex \opttitle{\'{A}rkai index}?><title>Árkai index</title>
      <p>The AI has been measured in 118 samples, most, if not all of
them, containing various amounts of I/S and/or Pg–Pg/Ms. Of
them, 40 yielded diagenetic values, 63 low anchizonal values, 14 high
anchizonal values and just 1 epizonal value. Distribution of these values
can be seen in Fig. 6. In those cases in which KI and AI have been
determined, the correlation of the grade indicated by both indices is good (<inline-formula><mml:math display="inline"><mml:mrow><mml:mi>r</mml:mi><mml:mo>=</mml:mo><mml:mn>0.65</mml:mn></mml:mrow></mml:math></inline-formula>; significance level 0.1 % <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>r</mml:mi><mml:mn>60</mml:mn></mml:msub><mml:mo>=</mml:mo><mml:mn>0.41</mml:mn></mml:mrow></mml:math></inline-formula>), suggesting that
both phases were formed under the same conditions and supporting the
reliability of the AI as indicator of grade in those cases in which it is the
only index available (Árkai et al., 1995).</p>
      <p>The existence of some discrepancies between KI and AI may be caused by the
presence of small amounts of I/S or Pg that alter the width of the
illite peaks. However, those discrepancies are always small and are usually
in samples at the boundary between metamorphic-grade zones (Supplement 2).</p>
</sec>
<sec id="Ch1.S4.SS1.SSS4">
  <title>Mineral distribution in relation with grade</title>
      <p>Kaolinite is present in deep diagenetic samples and also in some low
anchizonal ones. Maximum stability temperature of Kln is 270 <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C,
according to laboratory experiments (Velde, 1992), and therefore in agreement
with its presence in the anchizonal samples. Paragonite, apart from its
presence in deep diagenetic samples, is more frequently present in the
anchizone and some epizonal samples (Figs. 5 and 6). Pyrophyllite is more
abundant in samples from the anchizone but it can also be present in
diagenetic samples.</p>
      <p>The widespread occurrence of Kln and quartz in the diagenetic rock samples
may provide the starting material for the formation of Prl by the reaction
              <disp-formula id="R2" content-type="numbered reaction"><mml:math display="block"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mtext>kaolinite</mml:mtext><mml:mo>+</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mtext>quartz</mml:mtext><mml:mo>→</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mtext>pyrophyllite</mml:mtext><mml:mo>+</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mi mathvariant="normal">O</mml:mi></mml:mrow><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
            as suggested in the Glarus Alps by Frey (1978), who considered Prl an
indicator of anchizonal regional conditions. In fact of the 53 samples in
which Prl is present, Kln is found, and in very small amounts, in only 8 of
them. However, the stability field of Prl is strongly influenced by water
activity, and thus the formation temperature could be notably lower
(Thompson, 1970; Winkler, 1979; Hemley et al., 1980). Its presence in
diagenetic samples is not uncommon and could be due to the influence of
magmatic fluids (Hosterman et al., 1970; Kisch, 1987). According to Kisch (1987), Prl appears in regional terrains only in the anchizone but in areas
of intrusive activity it may appear in lower-grade zones. Therefore, the presence
of Prl in samples with diagenetic KI <inline-formula><mml:math display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> AI values, as in the eastern part of
the Liébana and Yuso–Carrión areas, could be regarded as evidence
for high geothermal gradients or magmatic heating.</p>
      <p>Chloritoid is abundant in samples from the high anchizone to epizone
(south-eastern Valsurbio area and western Yuso–Carrión area), but it can
also be present, in smaller amounts, in low anchizonal (1, 3W, 4E, 4W, 5E,
5W) and even diagenetic samples (eastern Liébana, Pisuerga and
Riaño–Cervera areas). Cld is Fe rich. The average Mg <inline-formula><mml:math display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> (Fe <inline-formula><mml:math display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> Mg)
found is &lt; 0.12 (Brime and Valín, 2006), similar to that of
pelites subjected to intermediate <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>P</mml:mi><mml:mo>/</mml:mo><mml:mi>T</mml:mi></mml:mrow></mml:math></inline-formula> conditions. It is noteworthy that
when this phase is present in the samples (a total of 93 samples have Cld),
Prl is absent, or in very minor amounts in a few samples (10 in total),
indicating that it could have been formed according to the reaction
originally proposed by Zen (1960), which is generally accepted for the
formation of Cld during metamorphism of aluminous pelites (Theye et al.,
1992):
              <disp-formula id="R3" content-type="numbered reaction"><mml:math display="block"><mml:mrow><mml:mtext>Pyrophyllite</mml:mtext><mml:mo>+</mml:mo><mml:mtext>chlorite</mml:mtext><mml:mo>→</mml:mo><mml:mtext>chloritoid</mml:mtext><mml:mo>+</mml:mo><mml:mtext>quartz</mml:mtext><mml:mo>+</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mi mathvariant="normal">O</mml:mi></mml:mrow><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula>
            The absence of Cld in the eastern part of the Yuso–Carrión area where
Prl is abundant, together with Chl, could indicate that the temperature
required for its formation by Reaction (R3) has not been reached.</p>
      <p>Presence of some Fe oxides has been detected in samples from the study area.
Therefore more Cld could be produced by the reaction suggested by Bucher and
Frey (1994):
              <disp-formula id="R4" content-type="numbered reaction"><mml:math display="block"><mml:mrow><mml:mtext>Chl</mml:mtext><mml:mo>+</mml:mo><mml:mn mathvariant="normal">4</mml:mn><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mtext>hematite</mml:mtext><mml:mo>=</mml:mo><mml:mtext>Cld</mml:mtext><mml:mo>+</mml:mo><mml:mn mathvariant="normal">4</mml:mn><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mtext>magnetite</mml:mtext><mml:mo>+</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mtext>Qtz</mml:mtext><mml:mo>+</mml:mo><mml:mn mathvariant="normal">3</mml:mn><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mi mathvariant="normal">O</mml:mi></mml:mrow><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula>
            However, it has been observed in thin sections that occurrence of Prl is
almost restricted to veins and fracture zones, suggesting that Cld could
have been formed during the hydrothermal alteration of the pelites following
the reaction proposed by Phillips (1988):
              <disp-formula id="R5" content-type="numbered reaction"><mml:math display="block"><mml:mrow><?xmltex \hack{\hbox\bgroup\fontsize{9.5}{9.5}\selectfont$\displaystyle}?><mml:mtext mathvariant="normal">Chlorite</mml:mtext><mml:mo>→</mml:mo><mml:mtext>chloritoid</mml:mtext><mml:mo>+</mml:mo><mml:mtext>Fe-rich  phase</mml:mtext><mml:mo>+</mml:mo><mml:mtext>quartz</mml:mtext><mml:mo>+</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mi mathvariant="normal">O</mml:mi></mml:mrow><mml:mo>.</mml:mo><?xmltex \hack{$\egroup}?></mml:mrow></mml:math></disp-formula>
            Presence of Cld in the anchizone has been discussed by Kisch (1983), who
concluded that Cld cannot unequivocally be regarded as an indicator of the
beginning of the epizone, as previously suggested, because there are
occurrences in the anchizone (Árkai et al., 1981). In the study area, Cld
is more abundant in the epizonal samples of the Valsurbio (6) and western
Yuso–Carrión (3W) areas, but it is also present in low anchizonal and a few
deep diagenetic samples from the Riaño–Cervera (5E), Pisuerga (4E) or
Valdeón (2) areas, thus corroborating the conclusion of Kisch (1983).</p>
      <p>Cld and Prl are widespread in virtually all rock types and grade
conditions (Supplement 2). This occurrence could
be related to basin-wide alteration by infiltrating hydrothermal fluids
(Phillips, 1988; Brime and Valín, 2006). Late- to post-Variscan fluid
flow events have been described in the other areas of the CZ
(Ayllón et al., 2003; Gasparrini et al., 2003) and some of them have been related to a more
general Variscan event (Boni et al., 2000).</p>
</sec>
</sec>
<sec id="Ch1.S4.SS2">
  <title>Conodont colour alteration index</title>
      <p>The CAI values are in general independent of the stratigraphic position of
the samples (Figs. 8 and 9). The Kasimovian–Gzhelian rocks show lower values,
but the small number of samples makes this result insignificant. CAI values
vary widely, ranging from 1.5 to 7.5, corresponding respectively to intervals
of temperatures of &lt; 40–60 and 550–590 <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C (see
Supplement 1). However, values equal to or lower than 2 are unusual, being
limited to the south-eastern sector of the Pisuerga–Carrión unit. Some
samples with conodonts having high CAI values and a range of one and a half
units, or more, are indicative of contact metamorphism and/or hydrothermal
processes. Values <inline-formula><mml:math display="inline"><mml:mo>≥</mml:mo></mml:math></inline-formula> 6 are usually found close to outcrops of igneous
rocks. The upper boundary of the ancaizone (CAI <inline-formula><mml:math display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 4) corresponds to a
temperature range of 190–225 <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C, while the lower limit
(CAI <inline-formula><mml:math display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 5.5) corresponds to the range of 340–375 <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F8" specific-use="star"><caption><p>Map with location of CAI values and delimitation of CAI isograds.
Picos de Europa CAI data after Bastida et al. (2004); Valsurbio CAI data
after García-López et al. (2013). Symbols of the CAI samples as in
Fig. 2.</p></caption>
          <?xmltex \igopts{width=625.96063pt, angle=-90}?><graphic xlink:href="https://se.copernicus.org/articles/7/1003/2016/se-7-1003-2016-f08.png"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F9"><caption><p>Diagram showing the distribution of CAI values in the different
stratigraphic levels. The small vertical straight segments represent the
mean value and the horizontal segments the CAI range. N – number of data; s – standard deviation. (1) Silurian–Devonian; (2) Tournaisian to lowermost
Serpukhovian; (3) lower Serpukhovian to lowermost Moscovian (Prioro Group);
(4) lower–upper Moscovian (Pando Group); (5) Kasimovian–Gzhelian.</p></caption>
          <?xmltex \igopts{width=170.716535pt}?><graphic xlink:href="https://se.copernicus.org/articles/7/1003/2016/se-7-1003-2016-f09.pdf"/>

        </fig>

      <p>The lack of carbonate rocks prevents in some areas the construction of a
complete map of CAI isograds; however, it is possible to observe that they
crosscut the trend of the Variscan structures. CAI data allow the
distinguishing of the following sectors in the study area (Fig. 8).
<list list-type="custom"><list-item><label>(a)</label><p>Northern sector (Liébana and Valdeón areas): this is an ancaizonal
area that passes without thermal discontinuity through the basal thrust of
the Picos de Europa unit. Inside this unit, the boundary
ancaizone/diacaizone appears and the CAI decreases northwards (Bastida et
al., 2004; Blanco-Ferrera et al., 2011).</p></list-item><list-item><label>(b)</label><p>Central-eastern sector (eastern part of the Yuso–Carrión area) with
dominance of ancaizonal conditions: in the areas where CAI data exist
a remarkable homogeneity of CAI values appears, mainly in the Devonian rocks
of the area located to the east of the Curavacas–Lechada syncline.</p></list-item><list-item><label>(c)</label><p>Central and western sectors (western part of the Yuso–Carrión and
Riaño–Cervera areas): the limited CAI data available indicate that
epicaizonal areas coexist with ancaizonal areas.</p></list-item><list-item><label>(d)</label><p>Southern sector: corresponds to the VU and presents a wide area with
epicaizonal conditions (García-López et al., 2013).</p></list-item><list-item><label>(e)</label><p>South-eastern sector (eastern part of the Yuso–Carrión and Pisuerga
areas): diacaizonal conditions are dominant, but ancaizonal
and epicaizonal areas also appear. The latter areas appear adjacent to
outcrops of igneous rocks. The greater variation of CAI values is found in
this area, with a range from 1.5 to 7.</p></list-item></list></p>
      <p>The apparently chaotic distribution of CAI isograds could be due to a heat
from subsurface intrusions at depth resulting in isotherms having complex
geometry. This pattern may be related to a crustal thinning during an
extensional episode and to the subsequent intrusion of igneous bodies that
emplaced at different levels, generating contact metamorphism and
hydrothermal fluids.</p>
      <p>In general, conodonts of the study area are undeformed and well preserved.
Most of them have granular texture due to apatite recrystallisation under
high temperature. The apatite crystals do not show preferential orientation
and their size increases with temperature. The granular texture is commonly
incipient for CAI values between 4 and 4.5 and is widespread for CAI values
<inline-formula><mml:math display="inline"><mml:mo>≥</mml:mo></mml:math></inline-formula> 5. Furthermore, some conodonts with CAI values between 6 and 7 have
coarse recrystallisation, corrosion and loss of ornamentation, so that in a
few cases they have lost their original morphology (“ghost conodonts”).
These alterations of conodonts with CAI values <inline-formula><mml:math display="inline"><mml:mo>≥</mml:mo></mml:math></inline-formula> 5 are indicative of
contact metamorphism and hydrothermal processes. Some conodonts with CAI <inline-formula><mml:math display="inline"><mml:mo>≥</mml:mo></mml:math></inline-formula> 4.5 present sets of parallel microfissures, probably related to the rock
cleavage. Conodonts with CAI <inline-formula><mml:math display="inline"><mml:mo>≤</mml:mo></mml:math></inline-formula> 4 have occasionally unaltered surfaces,
but most of them present a sugary texture (dull, frosted or pitted surfaces).
The surfaces of these conodonts show several types of overgrowth of apatite
crystals, mainly developed in the diacaizone, irrespective of the thermal
conditions inside this zone; they were usually a result of apatite solution
and crystallisation processes (Blanco-Ferrera et al., 2011).</p>
</sec>
<sec id="Ch1.S4.SS3">
  <title>Cleavage development and tectonothermal evolution</title>
      <p>Two main cleavages have been found in the study area (Fig. 10). Cleavage
<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>S</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> is a rough foliation associated with upright folds and trends
approximately E–W; it appears mainly in the northern half of the study area.
This cleavage affects the latest Carboniferous rocks (Kasimovian–Gzhelian age).
Cleavage <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>S</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> dips gently, crosscuts earlier upright folds and is
associated with the development of metre-scale open cascade folds. It is
especially well developed in the Curavacas–Lechada syncline (Fig. 11) and in
the VU. Both cleavages appear in different areas and have not been observed
superimposed. The existence of two cleavages with different age suggests that
two tectonothermal events took place in the south-eastern sector of the CZ.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F10" specific-use="star"><caption><p><bold>(a)</bold> <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>S</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> cleavage associated with a nearly upright fold
(eastern part of the Liébana area; north to the right). <bold>(b)</bold> <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>S</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>
cleavage dipping less than bedding in a normal stratigraphic succession
(Pando Group; Curavacas–Lechada syncline; north to the left).</p></caption>
          <?xmltex \igopts{width=483.69685pt}?><graphic xlink:href="https://se.copernicus.org/articles/7/1003/2016/se-7-1003-2016-f10.jpg"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F11" specific-use="star"><caption><p>Cross section of the Curavacas–Lechada syncline showing the
distribution of <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>S</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> cleavage and crenulation cleavage. Location in
Fig. 2.</p></caption>
          <?xmltex \igopts{width=483.69685pt}?><graphic xlink:href="https://se.copernicus.org/articles/7/1003/2016/se-7-1003-2016-f11.pdf"/>

        </fig>

      <p>The first event, associated with the <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>S</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> cleavage (sub-vertical), is not
well defined, since it developed in an area where presence of I/S and
Kln and KI and AI values indicate deep diagenesis or low anchizonal
conditions, and CAI values dominantly show ancaizonal conditions. According
to the age of the latest rocks affected, this event probably occurred during
the late Gzhelian. It resulted in crustal thickening produced by the N–S
shortening that gave rise to the emplacement of the Picos de Europa unit, the
last major Variscan thrust unit that was generated in the foreland fold and
thrust belt, and to the development of other thrusts and folds to the south
of this unit.</p>
      <p>The second event produced cleavage <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>S</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> that crosscuts the upright folds
in the southern part of the study area (Curavacas–Lechada syncline and the
VU). Under the microscope, this cleavage shows evidences of pressure solution
and crystallisation of oriented muscovite and chlorite with formation of
chlorite–muscovite porphyroblasts. XRD indicates that the rocks
affected by this cleavage present Chl <inline-formula><mml:math display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> Pg–Pg/Ms assemblages; KI
and AI values indicate high anchizonal to epizonal conditions and CAI values
indicate similar conditions. The gently dipping attitude of <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>S</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> suggests
that this event was associated with an extensional deformation. The event
culminated with the intrusion of igneous rocks that pierced the rocks with
cleavage and generated a contact metamorphism associated with hydrothermal
processes, as indicated by (1) the widespread presence of Cld and Prl
(Fig. 5; Brime and Valín, 2006) and low KI and AI values, (2)
recrystallisation in conodonts (granular texture), (3) high CAI values in
samples close to outcrops of intrusive rocks, (4) a wide range of CAI in some
samples and (5) irregular variation of the CAI through the area and strong
corrosion in some conodonts. The cleavage <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>S</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> developed earlier than the
porphyroblasts (biotite, andalusite and chloritoid) formed during the contact
metamorphism associated with the granodioritic stock of Peña Prieta
(Gallastegui et al., 1990; Rodríguez Fernández, 1994), whose age is
Cisuralian (<inline-formula><mml:math display="inline"><mml:mrow><mml:mn>292</mml:mn><mml:mo>+</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:mo>/</mml:mo><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:math></inline-formula> Ma after Valverde-Vaquero et al., 1999). These data
suggest the development of a thermal event that took place near the boundary
Carboniferous–Permian and that progressed during the Cisuralian with the
intrusion of many small igneous bodies that rose along faults (Suárez and
García, 1974; Corretgé and Suárez, 1990).</p>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T1" specific-use="star"><caption><p>Tectonothermal evolution of the south-eastern sector of the
Cantabrian Zone.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="2">
     <oasis:colspec colnum="1" colname="col1" align="justify" colwidth="142.26378pt"/>
     <oasis:colspec colnum="2" colname="col2" align="justify" colwidth="256.074803pt"/>
     <oasis:thead>
       <oasis:row rowsep="1">  
         <oasis:entry colname="col1">Variscan deformation</oasis:entry>  
         <oasis:entry colname="col2">Emplacement of north-directed Palentine nappes (prior or earliest Moscovian) and the adjacent western Cantabrian nappes (late Moscovian) with associated thrusts in the PCU</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row rowsep="1">  
         <oasis:entry colname="col1">Variscan deformation (cont.)</oasis:entry>  
         <oasis:entry colname="col2">Emplacement of the south-directed Picos de Europa unit; thrusts and folds in the PCU (Kasimovian–Gzhelian)</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">  
         <oasis:entry colname="col1">(N–S shortening)</oasis:entry>  
         <oasis:entry colname="col2">Upright folds and axial plane cleavage (<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>S</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>; first tectonothermal event with deep diagenetic – low anchizonal and ancaizonal areas in the northern part of the PCU (late Gzhelian)</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">  
         <oasis:entry colname="col1">Late-Variscan gravitational<?xmltex \hack{\hfill\break}?>readjustment; extensional event</oasis:entry>  
         <oasis:entry colname="col2">Gently dipping cleavage (<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>S</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> associated with crosscutting folds; second tectonothermal event; very-low- or low-grade metamorphism (high anchizone–epizone, and ancaizone–epicaizone) in the Curavacas–Lechada syncline and the VU. Normal faults (late-most Gzhelian to early Cisuralian)</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">  
         <oasis:entry colname="col1"/>  
         <oasis:entry colname="col2">Intrusion of igneous rocks, contact metamorphism and wide development of hydrothermal processes (Cisuralian)</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">  
         <oasis:entry colname="col1">Extension linked to the<?xmltex \hack{\hfill\break}?>Basque–Cantabrian basin</oasis:entry>  
         <oasis:entry colname="col2">Permian and Mesozoic hydrothermal episodes</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">Alpine deformation</oasis:entry>  
         <oasis:entry colname="col2">N–S shortening, tightening of gentle folds, local crenulation cleavage and tilting of rocks northwards (Cenozoic).</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table></table-wrap>

      <p>In some locations, <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>S</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> is gently folded with local development of
crenulation cleavage. This may be a result of the Alpine deformation, which
is the only post-Variscan compressional deformation described in the area
(Gallastegui, 2000 and references therein), and involved a ductile
deformation that required a moderate temperature and gave rise to a dome
shape in the VU (Marín, 1997).</p>
      <p>The features described above refer to penetrative structures or to the
thermal history developed during the last stages of the Variscan evolution.
However, this evolution does not preclude the development of other thermal
episodes subsequently, such as the hydrothermal post-Variscan episodes
described by Boni et al. (2000), Muchez et al. (2005), Gasparrini et
al. (2006) and Clauer and Weh (2014).</p>
</sec>
</sec>
<sec id="Ch1.S5">
  <title>Discussion</title>
      <p>The distribution of the different grade indicators used in the study area
shows, in general, an acceptable correlation between them, although some
discrepancies have been observed. All methods coincide in pointing out the
location of the areas with higher metamorphic grade, being the CAI and the AI
the indicators that tend to give the highest and the lowest grade
respectively. All indices point to an irregular distribution of the areas
with very-low-grade metamorphism. Diacaizonal areas are limited to the
south-eastern sector. A discrepancy is observed in the eastern
Yuso–Carrión area between clay mineral and CAI data; a notable number of
CAI values systematically indicates ancaizonal conditions, whereas clay
assemblages with abundant I/S and Kln, KI and AI indicate diagenetic
conditions.</p>
      <p>The correlation among the different indicators that can be used to establish
the metamorhic grade is challenging due to several factors, such as the
different kinetics of the processes that modify the colour of the conodonts
and the transformation of the clay minerals and the different influence of
fluids in limestones and pelitic rocks. These processes could explain the
discrepancies observed.</p>
      <p>In the context of the CZ, the low-grade extensional metamorphism
of the PCU extends westwards and allows an elongated area to be defined that
can be followed up to the Central Coal Basin (Fig. 1) (Aller, 1981, 1986;
Brime, 1985; Aller et al., 1987, 2005; García-López et al., 2007).
The biggest width of this zone is in the study area, coinciding with the core
of the Ibero-Armorican Arc, where a special evolution occurred in the context
of the CZ. The last stages of arc tightening gave rise to strong shortening
with formation of folds and cleavage (<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>S</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> in the core of the arc, and
the corresponding crustal thickening and heating (late Gzhelian).
Subsequently, a gravitational instability in this core produced an
extensional episode during which low-grade metamorphism and subhorizontal
cleavage (<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>S</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> crosscutting previous folds developed in some areas. This
evolution continued during the Cisuralian with the intrusion of igneous
bodies and associated contact metamorphism whose minerals post-date the
<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>S</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> cleavage. The existence of a crustal thickening followed by a
gravitational instability in the core of the Ibero-Armorican Arc has also
been proposed by other authors (Gutiérrez-Alonso et al., 2004, 2011). In
the Central Coal Basin, the metamorphism associated with subhorizontal
cleavage and crosscutting folds has been related to the possible existence of
igneous bodies in depth (Aller, 1986) or to the rise of fluids along faults,
especially the León fault (Aller et al., 2005). In the metamorphic
southern part of the study area (VU), the metamorphism disappears westward,
so that the adjacent western unit of the Esla nappe region is not metamorphic
(García-López et al., 2013; Valín and Brime, unpublished data).</p>
      <p>The existence of hydrothermal alteration has been suggested by Brime and
Valín (2006) and Clauer and Weh (2014). The common occurrence of Cld and
Prl and the irregular distribution of CAI values, the wide range in the high
CAI values in some samples and textural alterations of conodonts agree with
the occurrence of hydrothermal fluids and possible subsurface igneous bodies.
As for the thermal events dated by Clauer and Weh (illite K–Ar; 2014), the
first has an age (293 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 3 Ma), comparable to that of the Peña
Prieta granitoid, and the others (Guadalupian, middle Triassic and
early–middle Jurassic) are probably related to the crustal extension
associated with the Basque–Cantabrian basin. Specific structural evidences of
these three later events have not been found and their temperatures were
probably lower than those of the late-Variscan extensional episode, which,
being related to igneous intrusions, probably gave rise to the palaeothermal
peak.</p>
      <p>The zircon (U–Th) <inline-formula><mml:math display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> He ages obtained by Fillon et al. (2016) in three
samples from our study area indicate that they had probably a temperature
above 180 <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C before exhumation started by 37–39 Ma ago (Eocene).
This is consistent with the local occurrence of crenulation cleavage
associated with Alpine ductile deformation.</p>
      <p>The proposed tectonothermal evolution of the studied region from Variscan up
to Alpine times is summarised in Table 1.</p>
</sec>
<sec id="Ch1.S6" sec-type="conclusions">
  <title>Conclusions</title>
      <p>Study of the low-grade metamorphic rocks and associated structures in the
south-eastern sector of the CZ has allowed a model for the tectonothermal
evolution of the core of an arcuate orogenic belt to be developed. This core,
although  a part of a foreland fold and thrust belt where diagenetic
conditions are dominant, portrays a complex evolution due to its special
location inside the belt. It was thrust during the Carboniferous by large
units from south, west and north, which resulted in a great accumulation of
syntectonic sediments and development of unconformities and structures. The
latter arose as a result of compression in different directions that also
generated a crustal thickening. The emplacement of the last thrust unit
(Picos de Europa unit) produced a N–S shortening that generated thrusts and
associated folds. Shortly afterwards, upright folds with E–W trend and
associated cleavage (<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>S</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> developed, mainly in the northern part of the
sector. The ductile deformation occurred under thermal conditions which
reached the anchizone and the ancaizone in some areas. This represents the
first tectonothermal event registered in the south-eastern sector of the CZ.</p>
      <p>At the end of the Variscan deformation, gravitational instability gave rise
to an extensional episode and the corresponding crustal thinning. During this
event an increase in the thermal gradient enabled ductile deformation and
low-grade metamorphism to take place in some areas (second tectonothermal
event), mainly in the central part (Curavacas–Lechada syncline) and the
southern part (Valsurbio unit) of the sector. The ductile deformation
produced gently dipping cleavage (<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>S</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> crosscutting earlier upright
<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>F</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> folds. Some small, open cascade folds were also produced. The
metamorphism reached epizonal and epicaizonal conditions during this event.
The process culminated in the Cisuralian with the intrusion of igneous rocks
and the development of contact metamorphism around the larger igneous bodies.
In the case of Peña Prieta granodiorite, post-<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>S</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> andalusite
porphyroblasts developed. Hydrothermal fluids were common during this
extensional episode, resulting in the development of Prl and Cld,
textural alteration and high CAI dispersions in conodont samples.</p>
      <p>As a whole, the metamorphic grade is independent of the stratigraphic
location of the samples and the trend of the main structures, indicating the
late-orogenic character of the tectonothermal events. The thermal level
decreases progressively northwards inside the adjacent Picos de Europa unit.
However, the metamorphism associated with the extensional episode
in the PCU is extended westwards as an elongated area whose development was
probably favoured by the rise of fluids along faults, especially along the
León fault.</p>
<sec id="Ch1.S6.SSx1" specific-use="unnumbered">
  <title>Information about the Supplement</title>
      <p>Supplement 1 contains conodont CAI values and temperatures
inferred from the CAI Arrhenius plot (Epstein et al., 1977; Rejebian et al.,
1987). (V: Valsurbio samples; P: Pisuerga-Carrión samples; Po: Ponga
samples; Pe: Picos de Europa samples).
Supplement 2 contains the following.
<list list-type="order"><list-item><p>Values of KI measured on air-dried vs. KI measured
on ethylene glycol solvated samples, standardised at Kübler scale.
Samples are grouped according to the areas outlined in Fig. 4. Samples with
significant amounts of I/S and Pg–Pg/Ms that have not been
plotted in Figs 6 and 7 are indicated with Roman letter type of smaller size.</p></list-item><list-item><p>AI  measured on air-dried samples.</p></list-item><list-item><p>Clay minerals present in the samples. Capitals and bold type indicate
more abundance of the phase.</p></list-item></list></p>
</sec>
</sec>

      
      </body>
    <back><app-group>
        <supplementary-material position="anchor"><p><bold>The Supplement related to this article is available online at <inline-supplementary-material xlink:href="http://dx.doi.org/10.5194/se-7-1003-2016-supplement" xlink:title="pdf">doi:10.5194/se-7-1003-2016-supplement</inline-supplementary-material>.</bold></p></supplementary-material>
        </app-group><ack><title>Acknowledgements</title><p>This paper is dedicated to the memory of Andrés
Pérez Estaún in recognition to his major contribution to the study
the geology of the Variscan belt in Spain and his pioneer work on the
low-grade metamorphism of the area and in gratitude for fruitful cooperation
over a period of many years. The present paper has been supported by the
CGL2015-66997-R project funded by the Ministerio de Economía y
Competitividad of Spain. The authors acknowledge Dr. Robin Offler, who read an
earlier version of this paper and suggested improvements. Susana
García-López acknowledges the cooperation of C. F. Winkler Prins
from the National Museum of Natural History (Leiden, Netherlands) and H.
Jahnke from the Institut und Museum für Geologie und Paläontologie
(Göttingen, Germany) for providing access to the Cantabrian conodont
collections of these institutions. We thank Joaquina Álvarez-Marrón,
Tom Blenkinsop, Josep Poblet and an anonymous referee for useful suggestions
for improving the manuscript.
<?xmltex \hack{\newline}?><?xmltex \hack{\newline}?>
Edited by: J. Alvarez-Marron</p></ack><ref-list>
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    <!--<article-title-html>Tectonothermal evolution in the core of an arcuate fold and thrust belt: the
south-eastern sector of the Cantabrian Zone (Variscan belt, north-western Spain)</article-title-html>
<abstract-html><p class="p">The tectonothermal evolution of an area located in the core of the
Ibero-Armorican Arc (Variscan belt) has been determined by using the conodont
colour alteration index (CAI), Kübler index of illite (KI), the Árkai
index of chlorite (AI) and the analysis of clay minerals and rock cleavage.
The area is part of the Cantabrian Zone (CZ), which represents the foreland
fold and thrust belt of the orogen. It has been thrust by several large units
of the CZ, what resulted in the generation of a large number of synorogenic
Carboniferous sediments. CAI, KI and AI values show an irregular distribution
of metamorphic grade, independent of stratigraphic position. Two
tectonothermal events have been distinguished in the area. The first one,
poorly defined, is mainly located in the northern part. It gave rise to very-low-grade metamorphism in some areas and it was associated with a deformation
event that resulted in the emplacement of the last large thrust unit and
development of upright folds and associated cleavage (<i>S</i><sub>1</sub>). The second
tectonothermal event gave rise to low-grade metamorphism and cleavage
(<i>S</i><sub>2</sub>) crosscutting earlier upright folds in the central, western and
southern parts of the study area. The event continued with the intrusion of
small igneous rock bodies, which gave rise to contact metamorphism and
hydrothermal alteration. This event was linked to an extensional episode due
to a gravitational instability at the end of the Variscan deformation. This
tectonothermal evolution occurred during the Gzhelian–Sakmarian.
Subsequently, several hydrothermal episodes took place and local crenulation
cleavage developed during the Alpine deformation.</p></abstract-html>
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