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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-9-847-2018</article-id><title-group><article-title>Mechanical models to estimate the paleostress state<?xmltex \hack{\break}?> from igneous intrusions</article-title><alt-title>Mechanical models to estimate the paleostress state from igneous intrusions</alt-title>
      </title-group><?xmltex \runningtitle{Mechanical models to estimate the paleostress state from igneous intrusions}?><?xmltex \runningauthor{T. L. Stephens et al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes" rid="aff1">
          <name><surname>Stephens</surname><given-names>Tara L.</given-names></name>
          <email>tls15@le.ac.uk</email>
        <ext-link>https://orcid.org/0000-0003-1435-5198</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Walker</surname><given-names>Richard J.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Healy</surname><given-names>David</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Bubeck</surname><given-names>Alodie</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>England</surname><given-names>Richard W.</given-names></name>
          
        </contrib>
        <aff id="aff1"><label>1</label><institution>School of Geography, Geology and the Environment, University of Leicester, Leicester, LE1 7RH, UK</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>School of Geosciences, King's College, University of Aberdeen, Aberdeen, AB24 3UE, UK</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Tara L. Stephens (tls15@le.ac.uk)</corresp></author-notes><pub-date><day>9</day><month>July</month><year>2018</year></pub-date>
      
      <volume>9</volume>
      <issue>4</issue>
      <fpage>847</fpage><lpage>858</lpage>
      <history>
        <date date-type="received"><day>4</day><month>March</month><year>2018</year></date>
           <date date-type="rev-request"><day>21</day><month>March</month><year>2018</year></date>
           <date date-type="rev-recd"><day>15</day><month>June</month><year>2018</year></date>
           <date date-type="accepted"><day>21</day><month>June</month><year>2018</year></date>
      </history>
      <permissions>
        
        
      <license license-type="open-access"><license-p>This work is licensed under the Creative Commons Attribution 4.0 International License. To view a copy of this licence, visit <ext-link ext-link-type="uri" xlink:href="https://creativecommons.org/licenses/by/4.0/">https://creativecommons.org/licenses/by/4.0/</ext-link></license-p></license></permissions><self-uri xlink:href="https://se.copernicus.org/articles/.html">This article is available from https://se.copernicus.org/articles/.html</self-uri><self-uri xlink:href="https://se.copernicus.org/articles/.pdf">The full text article is available as a PDF file from https://se.copernicus.org/articles/.pdf</self-uri>
      <abstract>
    <p id="d1e125">Dikes and sills represent an important component of the deformation history
in volcanic systems, but unlike dikes, sills are typically omitted from
traditional paleostress analyses in tectonic studies. The emplacement of
sheet intrusions is commonly associated with Mode I fracturing in a low
deviatoric stress state, in which dilation is perpendicular to the fracture
plane. Many natural examples of sills and dikes, however, are observed to
accommodate minor shear offsets, in addition to a component of dilation. Here
we present mechanical models for sills in the San Rafael subvolcanic field,
Utah, which use field-based measurements of intrusion attitude and opening
angles to constrain the tectonic stress axes during emplacement and the
relative magma pressure for that stress state. The sills display bimodal dips
to the NE and SW and consistent vertical opening directions, despite variable
sill dips. Based on sill attitude and opening angles, we find that the sills
were emplaced during a phase of NE–SW horizontal shortening. Calculated
principal stress axes are consistent (within <inline-formula><mml:math id="M1" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 4<inline-formula><mml:math id="M2" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>) with
paleostress results for penecontemporaneous thrust faults in the area. The
models presented here can be applied to any set of dilational structures,
including dikes, sills, or hydrous veins, and represent a robust method for
characterising the paleostress state in areas where other brittle deformation
structures (e.g. faults) are not present.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <title>Introduction</title>
      <p id="d1e151">Sills and dikes are traditionally treated as extension fractures with a
dilation vector normal to the fracture wall; i.e. they are extension
fractures (Mode I; e.g. Anderson, 1951). This assumption has
important implications for the use of sheet intrusions in constraining
tectonic stress states because the minimum compressive stress (<inline-formula><mml:math id="M3" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>)
is perpendicular to the extension fracture walls; local deflections of the
intrusion attitude are commonly inferred to represent local rotations of the
stress axes. This is most commonly attributed to mechanical layering and the
presence of pre-existing structures (e.g. Rubin, 1995; Gudmundsson, 2002;
2011a; Magee et al., 2016). This model implies that intrusions can locally
propagate out of the regional <inline-formula><mml:math id="M4" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>–<inline-formula><mml:math id="M5" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> plane, via Mode I
failure of intact rock, or through Mode I dilation of pre-existing
structures, producing intrusions that display variable dilation vectors along
a single intrusion. Notably, many field examples of sills and dikes exhibit
near-parallel dilation vectors, regardless of the intrusion attitude (e.g.
Hoek, 1991; Walker, 1993; Airoldi et al., 2011; Martinez-Poza et al., 2014;
Muirhead et al., 2014; Eide et al., 2016; Walker et al., 2017). Intrusions
that demonstrate shear offset of markers across their margins indicate that
during emplacement the dilation vector was inclined from plane normal
(Muirhead et al., 2014; Stephens et al., 2017; Walker et al., 2017); this
obliquity of opening can be characterised by the opening angle (Fig. 1).</p>
      <p id="d1e187">Dilated structures have been studied in detail by Delaney et al. (1986), Baer
et al. (1994), and Jolly and Sanderson (1997), who applied mechanical methods
to estimate paleostress states using sheet intrusion attitudes. These
mechanical models have been adopted for statistical constraints on
paleostress axes, and the paleostress state, from vein or dike data (e.g.
Sato et al., 2013; Yamaji, 2016). Although several methods exist to determine
paleostress axes and a state of paleostress via fault, fracture, or dike
data, subhorizontal sheet intrusions (sills) are typically omitted from<?pagebreak page848?> such
analyses. This is because sill emplacement is commonly associated with a
local rotation of the principal stress axes, as a result of bedding or other
layer heterogeneities, during regional extension or a low-deviatoric stress
state (i.e. where <inline-formula><mml:math id="M6" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mo>≈</mml:mo><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>≈</mml:mo><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>; e.g.
Gudmundsson, 2011a; Magee et al., 2016). Several studies have demonstrated
that sills may also form during tectonic horizontal shortening, in which the
minimum principal stress is vertical (Walker, 2016; Walker et al., 2017;
Stephens et al., 2017); hence sills can be used as paleostress indicators,
provided they are accompanied by detailed kinematic characterisation.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1"><caption><p id="d1e217">Schematic diagrams to show the dilation direction (yellow arrow) and
opening angle (<inline-formula><mml:math id="M7" display="inline"><mml:mi mathvariant="italic">μ</mml:mi></mml:math></inline-formula>) of fractures in different stress regimes:
<bold>(a)</bold> normal-fault regime (where <inline-formula><mml:math id="M8" display="inline"><mml:mrow><mml:msub><mml:mi>S</mml:mi><mml:mi mathvariant="normal">H</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi mathvariant="normal">v</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>);
<bold>(b)</bold> thrust-fault regime (where <inline-formula><mml:math id="M9" display="inline"><mml:mrow><mml:msub><mml:mi>S</mml:mi><mml:mi mathvariant="normal">h</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi mathvariant="normal">v</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>);
the plane attitude is described by <inline-formula><mml:math id="M10" display="inline"><mml:mi mathvariant="italic">θ</mml:mi></mml:math></inline-formula>, the angle between the normal
stress and the maximum stress. <bold>(c)</bold> Example of cross-cutting sills;
the middle sill (outlined in blue) shows a consistent vertical opening
direction: Mode I opening on horizontal planes and extensional-shear opening
on inclined planes. <bold>(d)</bold> Graph showing changes in vertical thickness,
tv, and true thickness, <inline-formula><mml:math id="M11" display="inline"><mml:mi>t</mml:mi></mml:math></inline-formula>, with changes of apparent dip, for the sills
shown in panel <bold>(c)</bold>.</p></caption>
        <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://se.copernicus.org/articles/9/847/2018/se-9-847-2018-f01.pdf"/>

      </fig>

      <p id="d1e299">Here, we present mechanical models, based on those of Jolly and
Sanderson (1997), to determine paleostress state using the attitude of
dilated fracture sets; we verify this using the measured opening angle of the
intrusions. The method is applicable to any dilated fracture; here we focus
on the stress state associated with sill emplacement in the San Rafael
subvolcanic field (SRSVF), Utah,  and compare these results to fault data in the same
area to demonstrate the particular importance of subhorizontal igneous
intrusions as records of paleostress.</p>
</sec>
<sec id="Ch1.S2">
  <title>Dilation of pre-existing fractures</title>
      <p id="d1e308">Dilation of a cohesionless pre-existing planar structure occurs when the
fluid pressure (<inline-formula><mml:math id="M12" display="inline"><mml:mrow><mml:msub><mml:mi>P</mml:mi><mml:mi mathvariant="normal">f</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) exceeds the normal stress on the plane
(<inline-formula><mml:math id="M13" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi mathvariant="normal">n</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>; Fig. 1) (Delaney et al., 1986; Jolly and Sanderson,
1997). Normal stress is related to the plane attitude (<inline-formula><mml:math id="M14" display="inline"><mml:mi mathvariant="italic">θ</mml:mi></mml:math></inline-formula>) and the
maximum (<inline-formula><mml:math id="M15" display="inline"><mml:mrow><mml:msub><mml:mi>S</mml:mi><mml:mi mathvariant="normal">H</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) and minimum (<inline-formula><mml:math id="M16" display="inline"><mml:mrow><mml:msub><mml:mi>S</mml:mi><mml:mi mathvariant="normal">h</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) principal stresses
acting on the plane (Jolly and Sanderson, 1997):
          <disp-formula id="Ch1.E1" content-type="numbered"><mml:math id="M17" display="block"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi mathvariant="normal">n</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msub><mml:mi>S</mml:mi><mml:mi mathvariant="normal">H</mml:mi></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi>S</mml:mi><mml:mi mathvariant="normal">h</mml:mi></mml:msub></mml:mrow><mml:mn mathvariant="normal">2</mml:mn></mml:mfrac></mml:mstyle><mml:mo>+</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msub><mml:mi>S</mml:mi><mml:mi mathvariant="normal">H</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi>S</mml:mi><mml:mi mathvariant="normal">h</mml:mi></mml:msub></mml:mrow><mml:mn mathvariant="normal">2</mml:mn></mml:mfrac></mml:mstyle><mml:mi>cos⁡</mml:mi><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="italic">θ</mml:mi><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
        with the range of possible dilatant fracture attitudes controlled by the
stress ratio (<inline-formula><mml:math id="M18" display="inline"><mml:mi mathvariant="italic">φ</mml:mi></mml:math></inline-formula>),
          <disp-formula id="Ch1.E2" content-type="numbered"><mml:math id="M19" display="block"><mml:mrow><mml:mi mathvariant="italic">ϕ</mml:mi><mml:mo>=</mml:mo><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
        and the driving pressure ratio (<inline-formula><mml:math id="M20" display="inline"><mml:mrow><mml:msup><mml:mi>R</mml:mi><mml:mo>′</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula>) (Baer et al., 1994):
          <disp-formula id="Ch1.E3" content-type="numbered"><mml:math id="M21" display="block"><mml:mrow><mml:mi>R</mml:mi><mml:mo>=</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msub><mml:mi>P</mml:mi><mml:mi mathvariant="normal">f</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula>
        The stress ratio, <inline-formula><mml:math id="M22" display="inline"><mml:mrow><mml:mi mathvariant="italic">ϕ</mml:mi><mml:mo>,</mml:mo></mml:mrow></mml:math></inline-formula> is a non-directional value that describes the
relative magnitudes of the principal stresses: <inline-formula><mml:math id="M23" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:mo>≤</mml:mo><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>≤</mml:mo><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> (here, compressive stresses are positive). The
driving pressure ratio <inline-formula><mml:math id="M24" display="inline"><mml:mrow><mml:msup><mml:mi>R</mml:mi><mml:mo>′</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula> describes the relative magnitudes of the fluid
pressure and the remote stress state: when <inline-formula><mml:math id="M25" display="inline"><mml:mrow><mml:msup><mml:mi>R</mml:mi><mml:mo>′</mml:mo></mml:msup><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula> (i.e. <inline-formula><mml:math id="M26" display="inline"><mml:mrow><mml:msub><mml:mi>P</mml:mi><mml:mi mathvariant="normal">f</mml:mi></mml:msub><mml:mo>≤</mml:mo><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>) there is no dilation, and when <inline-formula><mml:math id="M27" display="inline"><mml:mrow><mml:msup><mml:mi>R</mml:mi><mml:mo>′</mml:mo></mml:msup><mml:mo>≥</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula>
(i.e. <inline-formula><mml:math id="M28" display="inline"><mml:mrow><mml:msub><mml:mi>P</mml:mi><mml:mi mathvariant="normal">f</mml:mi></mml:msub><mml:mo>≥</mml:mo><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>) all fracture attitudes could dilate.
This assumes that an intrusion is emplaced during a deviatoric stress state
(i.e. where <inline-formula><mml:math id="M29" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mo>≠</mml:mo><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>≠</mml:mo><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>); if <inline-formula><mml:math id="M30" display="inline"><mml:mrow><mml:msub><mml:mi>P</mml:mi><mml:mi mathvariant="normal">f</mml:mi></mml:msub><mml:mo>&gt;</mml:mo><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> during a non-deviatoric stress state (i.e. where <inline-formula><mml:math id="M31" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mo>=</mml:mo><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>=</mml:mo><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>), all pre-existing
fracture attitudes could dilate.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2"><caption><p id="d1e705">Schematic diagrams to show the relationship between opening mode and
apparent shear. <bold>(a–b)</bold> Initial pre-intrusion geometries with a
marker unit oblique to the fracture/fault plane.
<bold>(c–d)</bold> Extensional-shear dilation of a pre-existing fracture and
fault. <bold>(e–f)</bold> Mode I dilation of a pre-existing fracture and fault,
creating an apparent shear offset. <bold>(g)</bold> Dilation directions and
opening angles along linked segments can be used to infer the true dilation
direction and fluid pressure during intrusion. <inline-formula><mml:math id="M32" display="inline"><mml:mi mathvariant="italic">μ</mml:mi></mml:math></inline-formula> (ap): apparent
opening angle.</p></caption>
        <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://se.copernicus.org/articles/9/847/2018/se-9-847-2018-f02.pdf"/>

      </fig>

      <p id="d1e733">Pre-existing fractures, with poles parallel to the <inline-formula><mml:math id="M33" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> axis, will
show plane-normal dilation (i.e. dilation parallel to the normal stress
vector). Fractures inclined to the plane of <inline-formula><mml:math id="M34" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> resolve a shear
stress on their surface (Delaney et al., 1986). During dilation, shear stress
is reduced to zero through a plane-oblique dilation vector (extensional
shear). The angle between the dilation vector and normal stress is defined as
the opening angle (<inline-formula><mml:math id="M35" display="inline"><mml:mi mathvariant="italic">μ</mml:mi></mml:math></inline-formula>; Fig. 1a–c) and represents the ratio of shear to
dilation (Delaney et al., 1986). Extensional shear therefore acts to reduce
the amount of dilation. For an intrusion comprising inclined and
subhorizontal sections, the inclined sections will therefore be thinner than
subhorizontal sections oriented perpendicular to <inline-formula><mml:math id="M36" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> (e.g. Fig. 1c,
d) for a given fluid pressure, providing the stress state is deviatoric and
<inline-formula><mml:math id="M37" display="inline"><mml:mrow><mml:mn mathvariant="normal">0</mml:mn><mml:mo>&lt;</mml:mo><mml:msup><mml:mi>R</mml:mi><mml:mo>′</mml:mo></mml:msup><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> (England, 1988). The dilation vector can be measured using
traditional compass techniques in the field based on offset piercing points
or unique contact geometries, such as recognisable corners in the intrusion
walls<?pagebreak page849?> (e.g. Figs. 1c, 2a, b). True offsets result from extensional-shear
opening (Fig. 2c, d); however apparent shear offset can be produced by marker
units that are oriented at an oblique angle to the intrusion plane (Fig. 2e)
or via dilation of pre-existing faults, which produce a larger-than-expected
opening angle (Fig. 2f). To determine whether offset and the opening angle
are true or apparent, multiple manual measurements of opening angle and
intrusion thickness must be made along strike of an intrusion (Figs. 1c, 2g).
The opening angle (<inline-formula><mml:math id="M38" display="inline"><mml:mi mathvariant="italic">μ</mml:mi></mml:math></inline-formula>) of a dilated fracture can be calculated as the
inverse cosine of the true thickness (<inline-formula><mml:math id="M39" display="inline"><mml:mi>t</mml:mi></mml:math></inline-formula>, normal to the plane) and the
vertical thickness (tv, parallel to the dilation vector; Fig. 1c):

              <disp-formula id="Ch1.E4" content-type="numbered"><mml:math id="M40" display="block"><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:mi mathvariant="italic">μ</mml:mi><mml:mo>=</mml:mo><mml:msup><mml:mi>cos⁡</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>/</mml:mo><mml:mtext>tv</mml:mtext><mml:mo>)</mml:mo><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula>

        Alternatively, <inline-formula><mml:math id="M41" display="inline"><mml:mi mathvariant="italic">μ</mml:mi></mml:math></inline-formula> can be measured as a rake of the obtuse angle between
the intrusion contact and the dilation vector, minus 90<inline-formula><mml:math id="M42" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>.
Importantly, this measurement only accounts for the opening angle in two
dimensions; movement in or out of the face will not be recorded; therefore
dip-parallel sections should ideally be used.</p>
      <p id="d1e857">The opening angle is related to the shear stress (<inline-formula><mml:math id="M43" display="inline"><mml:mi mathvariant="italic">τ</mml:mi></mml:math></inline-formula>), normal stress
(<inline-formula><mml:math id="M44" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi mathvariant="normal">n</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>), and fluid pressure (<inline-formula><mml:math id="M45" display="inline"><mml:mrow><mml:msub><mml:mi>P</mml:mi><mml:mi mathvariant="normal">f</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) acting on that
plane at the time of intrusion (Delaney et al., 1986; Jolly and Sanderson,
1997):
          <disp-formula id="Ch1.E5" content-type="numbered"><mml:math id="M46" display="block"><mml:mrow><mml:mi mathvariant="italic">μ</mml:mi><mml:mo>=</mml:mo><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">tan</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup><mml:mfenced close=")" open="("><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mi mathvariant="italic">τ</mml:mi><mml:mrow><mml:msub><mml:mi>P</mml:mi><mml:mi mathvariant="normal">f</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi mathvariant="normal">n</mml:mi></mml:msub></mml:mrow></mml:mfrac></mml:mstyle></mml:mfenced><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula>
        Equation (5) shows that if the fluid overpressure (<inline-formula><mml:math id="M47" display="inline"><mml:mrow><mml:msub><mml:mi>P</mml:mi><mml:mi mathvariant="normal">f</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>–<inline-formula><mml:math id="M48" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi mathvariant="normal">n</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) is equal to the shear stress, the opening angle is 45<inline-formula><mml:math id="M49" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>,
and the shear-to-dilation ratio is unity. If the overpressure is greater than
the shear stress, the opening angle is less than 45<inline-formula><mml:math id="M50" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>, and the
fracture will show a greater component of dilation to shear. When <inline-formula><mml:math id="M51" display="inline"><mml:mi mathvariant="italic">μ</mml:mi></mml:math></inline-formula> is
negative, the fracture will remain closed as the fluid pressure did not
exceed the normal stress. An intrusive segment, however, may inflate against
a closed fracture (where <inline-formula><mml:math id="M52" display="inline"><mml:mrow><mml:msub><mml:mi>P</mml:mi><mml:mi mathvariant="normal">f</mml:mi></mml:msub><mml:mo>&lt;</mml:mo><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi mathvariant="normal">n</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>), causing a local
contractional shear and a blunt intrusion tip (e.g. Fig. 2g).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3" specific-use="star"><caption><p id="d1e997">Mechanical models showing contoured fracture-opening angles for
various stress and fluid pressure conditions, using the equation from Delaney
et al. (1986), projected onto lower-hemisphere, equal-area stereonets and
Mohr circles (colour scheme from Thyng et al., 2016). The dashed line on the
Mohr circles indicates the fluid pressure magnitude. Five increments of fluid
pressure <bold>(a</bold><inline-formula><mml:math id="M53" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mi mathvariant="bold">i</mml:mi><mml:mtext mathvariant="bold">–</mml:mtext><mml:mi mathvariant="bold">v</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula><bold>)</bold> have been
modelled with three stress states: <bold>(b)</bold> thrust-fault regime
(<inline-formula><mml:math id="M54" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi mathvariant="normal">v</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>), <bold>(c)</bold> strike-slip regime
(<inline-formula><mml:math id="M55" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi mathvariant="normal">v</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>), and <bold>(d)</bold> normal-fault regime
(<inline-formula><mml:math id="M56" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi mathvariant="normal">v</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>). Colour contours correspond to
pole-to-plane values. Poles that plot in the yellow zone (where <inline-formula><mml:math id="M57" display="inline"><mml:mrow><mml:mi mathvariant="italic">μ</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula>–10<inline-formula><mml:math id="M58" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>) will display approximately plane-normal opening; poles with
larger opening angles will display extensional-shear dilation and have a
smaller true thickness than adjoining segments that plot in the yellow zone.</p></caption>
        <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://se.copernicus.org/articles/9/847/2018/se-9-847-2018-f03.pdf"/>

      </fig>

</sec>
<sec id="Ch1.S3">
  <title>Mechanical models for fracture dilation and opening angle</title>
      <p id="d1e1115">Equation (5) can be represented in three-dimensional (3-D) space, for any
given stress state, stress ratio, and fluid pressure: Fig. 3 shows the opening
angle (<inline-formula><mml:math id="M59" display="inline"><mml:mi mathvariant="italic">μ</mml:mi></mml:math></inline-formula>) of all possible fracture planes in 3-D space, plotted as
colour-contoured pole-to-plane values of <inline-formula><mml:math id="M60" display="inline"><mml:mi mathvariant="italic">μ</mml:mi></mml:math></inline-formula>, on equal-area lower-hemisphere stereographic projections and on 3-D Mohr diagrams. Fluid pressure
was calculated at five equal intervals,
which are expressed as <inline-formula><mml:math id="M61" display="inline"><mml:mrow><mml:msup><mml:mi>R</mml:mi><mml:mo>′</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula> values (Fig. 3a), relative to the ambient stress state. Figure 3 shows plots of opening
angles for three tectonic regimes in which <inline-formula><mml:math id="M62" display="inline"><mml:mi mathvariant="italic">ϕ</mml:mi></mml:math></inline-formula> is 0.5: (1) a thrust-fault
regime (<inline-formula><mml:math id="M63" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi mathvariant="normal">v</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>) (Fig. 3b), (2) a strike-slip regime
(<inline-formula><mml:math id="M64" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi mathvariant="normal">v</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>) (Fig. 3c), and (3) a normal-fault regime
(<inline-formula><mml:math id="M65" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi mathvariant="normal">v</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>) (Fig. 3d). The principal stress attitudes
are constant in all models, with the azimuth for the maximum horizontal
stress (<inline-formula><mml:math id="M66" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi mathvariant="normal">H</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) trending E–W. All planes are modelled as
cohesionless surfaces.</p>
      <p id="d1e1216">The models complement the results of Jolly and Sanderson (1997) and
demonstrate that within a given stress state, increasing the fluid pressure
increases the range of pre-existing fracture attitudes that can dilate,
provided the dilated fracture is linked to the magmatic source. The models
also show that for any given fracture, increasing <inline-formula><mml:math id="M67" display="inline"><mml:mrow><mml:msub><mml:mi>P</mml:mi><mml:mi mathvariant="normal">f</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> decreases
<inline-formula><mml:math id="M68" display="inline"><mml:mi mathvariant="italic">μ</mml:mi></mml:math></inline-formula>. Where <inline-formula><mml:math id="M69" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:mo>&lt;</mml:mo><mml:msub><mml:mi>P</mml:mi><mml:mi mathvariant="normal">f</mml:mi></mml:msub><mml:mo>≤</mml:mo><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> (Fig. 3b–d, i–ii),
the dilation zone, delineating the poles to fractures that are predicted to
dilate forms an ellipse about the <inline-formula><mml:math id="M70" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> axis and is elongate in the
direction of the intermediate stress (<inline-formula><mml:math id="M71" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>); only fractures with
poles parallel to the <inline-formula><mml:math id="M72" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> axis show Mode I opening. If <inline-formula><mml:math id="M73" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>&lt;</mml:mo><mml:msub><mml:mi>P</mml:mi><mml:mi mathvariant="normal">f</mml:mi></mml:msub><mml:mo>&lt;</mml:mo><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> (Fig. 3b<inline-formula><mml:math id="M74" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">iii</mml:mi></mml:msub></mml:math></inline-formula>–d<inline-formula><mml:math id="M75" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">iii</mml:mi></mml:msub></mml:math></inline-formula>) the
dilation zone forms a girdle parallel to the axis of <inline-formula><mml:math id="M76" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, with two
defined zones of near-Mode I opening (0–10<inline-formula><mml:math id="M77" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>) surrounding the
<inline-formula><mml:math id="M78" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M79" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> poles. Fractures of all attitudes can dilate if
P<inline-formula><mml:math id="M80" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mi mathvariant="normal">f</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> (Fig. 3b<inline-formula><mml:math id="M81" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">iv</mml:mi></mml:msub></mml:math></inline-formula>–d<inline-formula><mml:math id="M82" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">iv</mml:mi></mml:msub></mml:math></inline-formula>). The
models suggest that Mode I opening of pre-existing fractures should only be
common if the fluid pressure exceeds <inline-formula><mml:math id="M83" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> (e.g.
Fig. 3b<inline-formula><mml:math id="M84" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">v</mml:mi></mml:msub></mml:math></inline-formula>–d<inline-formula><mml:math id="M85" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">v</mml:mi></mml:msub></mml:math></inline-formula>). For dilation of misoriented
cohesionless fractures, with planes oriented at a high angle to <inline-formula><mml:math id="M86" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, a higher<?pagebreak page850?> fluid pressure is required to overcome the normal stress
acting on their surface (e.g. Gaffney et al., 2007). Importantly, if
misoriented planes do not become linked to the fluid network, high fluid
overpressures will be relaxed by dilation of preferentially oriented
pre-existing structures, or via failure of intact rock (e.g. Sibson, 2012).
Dilational fracture data should therefore plot stereographically with the
greatest density of poles to planes about the <inline-formula><mml:math id="M87" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> axis (Jolly and
Sanderson, 1997; Yamaji et al., 2010). Propagating intrusions may cut across
or terminate against misoriented structures, which plot in the zone of no
dilation (white areas on the Mohr circles and stereonets; Fig. 3), as the
normal stress acting on these planes exceeds the fluid pressure, preventing
dilation (e.g. Gaffney et al., 2007; Gudmundsson, 2011a). Terminated
intrusions may inflate against closed fractures if magma supply continues;
dilation will be accommodated by local shear along the closed fracture,
producing a blunt intrusion tip (Baer, 1991; Stephens et al., 2017). Through
measurement of the opening angles of veins or intrusions, and determining the
distribution of fracture attitudes that are in contact with intrusions, but
not dilated, it is therefore possible to constrain the fluid pressure
relative to the ambient stress state.</p>
      <p id="d1e1469">In addition to changes in fluid pressure, fracture dilation is also sensitive
to changes in remote stress, particularly at lower <inline-formula><mml:math id="M88" display="inline"><mml:mrow><mml:msub><mml:mi>P</mml:mi><mml:mi mathvariant="normal">f</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>. For
instance, where <inline-formula><mml:math id="M89" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:mo>&lt;</mml:mo><mml:msub><mml:mi>P</mml:mi><mml:mi mathvariant="normal">f</mml:mi></mml:msub><mml:mo>≤</mml:mo><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> (Fig. 3b–d, i–ii)
each stress regime is defined by a particular range of fracture attitudes,
with a unique opening angle pattern. Where <inline-formula><mml:math id="M90" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>&lt;</mml:mo><mml:msub><mml:mi>P</mml:mi><mml:mi mathvariant="normal">f</mml:mi></mml:msub><mml:mo>≤</mml:mo><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> (Fig. 3b–d, iii–iv), the thrust-fault regime
(Fig. 3b<inline-formula><mml:math id="M91" display="inline"><mml:msub><mml:mi/><mml:mtext>iii–iv</mml:mtext></mml:msub></mml:math></inline-formula>) and strike-slip regime (Fig. 3c<inline-formula><mml:math id="M92" display="inline"><mml:msub><mml:mi/><mml:mtext>iii–iv</mml:mtext></mml:msub></mml:math></inline-formula>)
have<?pagebreak page851?> similar opening angle patterns, whereas the distribution of attitudes
and opening angles for the normal-fault regime (Fig. 3d<inline-formula><mml:math id="M93" display="inline"><mml:msub><mml:mi/><mml:mtext>iii–iv</mml:mtext></mml:msub></mml:math></inline-formula>) is
unique. Applied carefully, using detailed kinematic field analyses of sills,
and their associated deformation, the method has the potential to
discriminate among intrusions related to
different remote stress states. Here, we have applied this method to igneous
sills in the SRSVF in Utah.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4" specific-use="star"><caption><p id="d1e1563">Location maps for the San Rafael subvolcanic field in Utah amended
from Walker et al. (2017). <bold>(a)</bold> Digital elevation model for Utah,
showing major structural and depositional areas of the Colorado Plateau.
Solid black line shows province boundaries. Dashed black line is a region of
lower-crustal delamination and crustal thinning detailed in Levander et
al. (2011); dashed white line is their outline of a downwelling body at
200 km depth, estimated from body wave tomography. <bold>(b)</bold> Aerial
imagery for the San Rafael subvolcanic field (SRSVF) highlighting location
and distribution of intrusive bodies; the white star marks the Cedar Mountain
sill studied by Richardson et al. (2015). <bold>(c)</bold> Hillshaded digital
elevation models for thick sills in the southern SRSVF, coloured to show
extrapolated elevation data for sill top contacts (modified from Walker et
al., 2017). <bold>(d)</bold> Field photograph of the Last Chance sills, which
transgress through the stratigraphy; the upper sill cuts across the
Carmel–Entrada Formation boundary. <bold>(e)</bold> Sills cut dike and cut and
abut against subvertical fractures (sills outlined in black, dike in white).
<bold>(f)</bold> Lower-hemisphere stereographic projections show sill top contact
polygon attitudes (extrapolated from panel <bold>c</bold>) as great circles, and
poles to planes for each sill system (data from Walker et al., 2017).</p></caption>
        <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://se.copernicus.org/articles/9/847/2018/se-9-847-2018-f04.pdf"/>

      </fig>

      <p id="d1e1595">Dilated fractures, created during the same dilational event, will produce a
unique distribution of opening angles when plotted stereographically as poles
to planes (e.g. Jolly and Sanderson, 1997; Yamaji et al., 2010; Sato et al.,
2013). Whether this is a tight cluster or a distributed set of poles, the
pattern is usually interpreted to represent a single event, governed by one
fluid pressure (e.g. Jolly and Sanderson, 1997); however, it is possible that
the data represent multiple events caused by fluid pressure pulses of
varying magnitude (Yamaji et al., 2010). As the opening angle represents the
ratio of shear to dilation (Delaney et al., 1986), magmatic events of varying
magnitude within the same governing stress state could produce
cross-cutting intrusions with similar geometries but different opening
angles (e.g. Fig. 3). The attitude and opening angle of dilated fractures,
along with cross-cutting relationships, can therefore be used to identify
whether a network of dilated fractures represents one, or multiple, fluid
pressure pulses and the stress state during each pulse.</p>
</sec>
<sec id="Ch1.S4">
  <title>Stress state model for sill emplacement: San Rafael subvolcanic
field</title>
      <p id="d1e1604">The SRSVF is located in the north-western Colorado Plateau, central Utah
(Fig. 4a), and comprises numerous sills, dikes, and volcanic breccia bodies
(Fig. 4b, c). The close spatial association of these different intrusive bodies has been suggested to
reflect emplacement during a low deviatoric stress state (Delaney and
Gartner, 1997; Richardson et al., 2015). No crustal magma chambers have been
identified as the source for the intrusive complex (Delaney and Gartner,
1997). The exposed intrusive system was emplaced at <inline-formula><mml:math id="M94" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 1 km depth,
within the Middle Jurassic sedimentary rocks of the San Rafael Group, which
comprises four formations: the Carmel Formation (siltstone and shale),
Entrada Sandstone (interbedded sandstone, siltstone, and claystone), Curtis
Formation (interbedded glauconitic sandstone, and siltstone), and the
Summerville Formation (siltstone, sandstone, and shale) (Gartner, 1986;
Richardson et al., 2015). The sequence represents a paralic environment, with
near-shore and shallow marine deposits (Gartner, 1986; Peterson, 1988). The
sills are mainly emplaced within the Entrada Sandstone; however they also cut
across formation boundaries to intrude the Carmel and Summerville formations
(e.g. Fig. 4d; Walker et al., 2017). Richardson et al. (2015) highlighted an
example of a dike-to-sill transition for the Cedar Mountain sills (Fig. 4b).
Our study focuses on sills in the southern SRSVF (Fig. 4b), and we cannot
confirm that relationship here. In our study area, sills and dikes display
mutual cross-cutting relationships (e.g. Fig. 4e; Gartner, 1986; Walker et
al., 2017), and we have observed no dike–sill transitions for the major
sills (e.g. Fig. 4c). Delaney and Gartner (1997) determined ages of dike
emplacement between 4.6 and 3.7 Ma; the field relationships therefore
constrain sill emplacement to a <inline-formula><mml:math id="M95" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 1 Myr interval.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F5" specific-use="star"><caption><p id="d1e1623">Sill geometry and paleostress analyses of deformation structures in
the San Rafael subvolcanic field. <bold>(a)</bold> Kilometre-scale segmented sills show en-echelon
stepping consistent with conjugate faults (sills shaded red). Inset shows
schematic interpretation. <bold>(b)</bold> The 100 m scale sills showing NE and SW
dips (sills outlined in black). <bold>(c)</bold> The <inline-formula><mml:math id="M96" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> 100 m scale sills with
bimodal dips (sills outlined in black). <bold>(d)</bold> Deformation bands and
low-angle fractures parallel to gypsum veins. <bold>(e)</bold> Gypsum veins with
conjugate geometries. <bold>(f)</bold> Sill intruding and cut by a thrust fault
and low-angle fractures (sills outlined in black). <bold>(g–i)</bold> Lower-hemisphere equal-area projections showing <bold>(g)</bold> gypsum veins and
fractures, <bold>(h)</bold> thrust faults, and <bold>(i)</bold> deformation band
data; principal stress axes calculated for panels <bold>(h)</bold> and
<bold>(i)</bold> using the right dihedra method (Delvaux and Sperner, 2003).
Calculated stress axes given as plunge–trend measurements; <inline-formula><mml:math id="M97" display="inline"><mml:mi mathvariant="italic">ϕ</mml:mi></mml:math></inline-formula> value is
the stress ratio (<inline-formula><mml:math id="M98" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>–<inline-formula><mml:math id="M99" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:mo>/</mml:mo><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>–<inline-formula><mml:math id="M100" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>).</p></caption>
        <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://se.copernicus.org/articles/9/847/2018/se-9-847-2018-f05.pdf"/>

      </fig>

      <p id="d1e1724">Walker et al. (2017) interpret the sills in the SRSVF as low-angle conjugate
intrusions, and concluded that the sills record a phase of horizontal
tectonic shortening, rather than relating to local deflections due to
material layering. The sills range from <inline-formula><mml:math id="M101" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> 10 cm to <inline-formula><mml:math id="M102" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 30 m thick
and are discordant to bedding, with dips of 1–25<inline-formula><mml:math id="M103" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> (Fig. 4d, f).
Based on sill attitude measurements over kilometre-scale outcrops, Walker et
al. (2017) showed that sill poles cluster about a near-vertical axis with two
defined clusters: a NW- and SE-dipping set in the northern SRSVF and a NE- and
SW-dipping set in the southern SRSVF. This study focuses on the NE- and SW-dipping sills in the southern SRSVF (Fig. 4b, c).</p>
      <p id="d1e1750">Across all scales, we find mutual cross-cutting relationships between sills
with bimodal dips (e.g. Figs. 1c, 5a–c), and en-echelon sill segments which
define low-angle (<inline-formula><mml:math id="M104" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 20<inline-formula><mml:math id="M105" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> dip) conjugate sets (Fig. 5a).
Deformation bands and gypsum veins have comparable attitudes to sills and
thrust faults in the field area and define low-angle conjugate sets with NE
and SW dips (Fig. 5d–i). Sills intruded and have been cut by low-angle
fractures, thrust faults, and reverse faults (all referred to as thrust
faults henceforth) and either cut or abut against sub-vertical fractures
(Figs. 4d, 5f; Walker et al., 2017). A constant near-vertical opening
direction is noted across all sill segment attitudes (Figs. 6, 7a). Local
sill contact data display a range of dips from 4 to 87<inline-formula><mml:math id="M106" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> with
horizontal to subhorizontal sill segments (0–20<inline-formula><mml:math id="M107" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> dip) showing
plane-normal (Mode I) and extensional-shear dilation
(<inline-formula><mml:math id="M108" display="inline"><mml:mi mathvariant="italic">μ</mml:mi></mml:math></inline-formula> <inline-formula><mml:math id="M109" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 0–20<inline-formula><mml:math id="M110" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>), respectively (Figs. 6a, 7a). Inclined segments
(20–56<inline-formula><mml:math id="M111" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> dip) are consistently thinner than adjoining horizontal
segments and display reverse-sense shear offset of piercing points
(<inline-formula><mml:math id="M112" display="inline"><mml:mrow><mml:mn mathvariant="normal">20</mml:mn><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mo>&lt;</mml:mo><mml:mi mathvariant="italic">μ</mml:mi><mml:mo>≤</mml:mo><mml:mn mathvariant="normal">75</mml:mn><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula>; Fig. 7a).
Subvertical to vertical fractures (<inline-formula><mml:math id="M113" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> 70<inline-formula><mml:math id="M114" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> dip) were not intruded
(Fig. 7a), suggesting that fluid pressure was less than the normal stress on
those planes during intrusion, and the opening angle was <inline-formula><mml:math id="M115" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> 0<inline-formula><mml:math id="M116" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F6"><caption><p id="d1e1880">Sill–sill cross-cutting relationships. <bold>(a)</bold> Younger
horizontal sill maintains a constant thickness when cutting older sill.
<bold>(b–c)</bold> Inclined sill sections are thinner than horizontal sections.
All sills show near-vertical opening directions, regardless of attitude.</p></caption>
        <?xmltex \igopts{width=199.169291pt}?><graphic xlink:href="https://se.copernicus.org/articles/9/847/2018/se-9-847-2018-f06.pdf"/>

      </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F7" specific-use="star"><caption><p id="d1e1897">The opening-angle mechanical model. <bold>(a)</bold> Field example of
thin sills (<inline-formula><mml:math id="M117" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> 1 m thick) displaying a range of local contact dips and a
consistent vertical opening. <bold>(b)</bold> Lower-hemisphere, equal-area
stereonet with local sill contacts plotted as poles to planes, coloured
relative to their opening angle, with Mode I and total dilational ellipses
constructed. <bold>(c)</bold> Determination of principal stress axes and <inline-formula><mml:math id="M118" display="inline"><mml:mi mathvariant="italic">θ</mml:mi></mml:math></inline-formula> angles. <bold>(d)</bold> Mechanical model results using the stress ratio and
driving pressure (<inline-formula><mml:math id="M119" display="inline"><mml:mrow><mml:mi mathvariant="italic">ϕ</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula>.77, <inline-formula><mml:math id="M120" display="inline"><mml:mrow><mml:msup><mml:mi>R</mml:mi><mml:mo>′</mml:mo></mml:msup><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula>.68; see text for details) derived from
panel <bold>(c)</bold>. <bold>(e)</bold> 3-D Mohr circle showing how <inline-formula><mml:math id="M121" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">θ</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and
<inline-formula><mml:math id="M122" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">θ</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> can be used to calculate relative fluid pressure; the Mohr circle is
colour contoured for values of <inline-formula><mml:math id="M123" display="inline"><mml:mi mathvariant="italic">μ</mml:mi></mml:math></inline-formula>; local sill contacts are plotted as
poles and coloured by their opening angle.</p></caption>
        <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://se.copernicus.org/articles/9/847/2018/se-9-847-2018-f07.pdf"/>

      </fig>

      <p id="d1e1996">Since the range of dilated sill attitudes is known, we can determine the
relative stress and fluid pressure using the parameters <inline-formula><mml:math id="M124" display="inline"><mml:mi mathvariant="italic">ϕ</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M125" display="inline"><mml:mrow><mml:msup><mml:mi>R</mml:mi><mml:mo>′</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula>. We
calculate these parameters stereographically, using an adapted method from
Jolly and Sanderson (1997). The local sill contact data are plotted as poles
to planes and coloured by their <inline-formula><mml:math id="M126" display="inline"><mml:mi mathvariant="italic">μ</mml:mi></mml:math></inline-formula> value; the pole cluster showing Mode I
opening (<inline-formula><mml:math id="M127" display="inline"><mml:mrow><mml:mi mathvariant="italic">μ</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula>–10<inline-formula><mml:math id="M128" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>) is fitted with an ellipse (Fig. 7b). For data
with a clustered distribution, this ellipse geometry provides a guide for the
total range of dilated fractures, for which blunt tips define the limit of
fracture<?pagebreak page852?> attitudes able to dilate; beyond this is the zone of no opening
(where <inline-formula><mml:math id="M129" display="inline"><mml:mrow><mml:mi mathvariant="italic">μ</mml:mi><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula><inline-formula><mml:math id="M130" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>; Fig. 7b). The minimum compressive stress
(<inline-formula><mml:math id="M131" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>) plots in the centre of the Mode I ellipse (which likely
coincides with the centre of the data cluster); <inline-formula><mml:math id="M132" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M133" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>
are mutually orthogonal to this (Fig. 7c). If the data have a girdled
distribution, the 0–10<inline-formula><mml:math id="M134" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> ellipse should be used as an approximation
for the geometry of the zone of no opening. In these cases, there will be two
clusters of poles where <inline-formula><mml:math id="M135" display="inline"><mml:mrow><mml:mi mathvariant="italic">μ</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula>–10<inline-formula><mml:math id="M136" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> (see
Fig. 3b<inline-formula><mml:math id="M137" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">iii</mml:mi></mml:msub></mml:math></inline-formula>–d<inline-formula><mml:math id="M138" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">iii</mml:mi></mml:msub></mml:math></inline-formula>); the larger ellipse signifies the
location of <inline-formula><mml:math id="M139" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>. A distributed set of dilated fractures may contain
several zones of Mode I opening (<inline-formula><mml:math id="M140" display="inline"><mml:mrow><mml:mi mathvariant="italic">μ</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula>–10<inline-formula><mml:math id="M141" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>; see Fig. 3):
<inline-formula><mml:math id="M142" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> will plot in the larger of these ellipses and <inline-formula><mml:math id="M143" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> in
the zone of highest opening angle, or the smallest Mode I ellipse when
<inline-formula><mml:math id="M144" display="inline"><mml:mrow><mml:msub><mml:mi>P</mml:mi><mml:mi mathvariant="normal">f</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> exceeds <inline-formula><mml:math id="M145" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> (see
Fig. 3b<inline-formula><mml:math id="M146" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">v</mml:mi></mml:msub></mml:math></inline-formula>–b<inline-formula><mml:math id="M147" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">v</mml:mi></mml:msub></mml:math></inline-formula>).</p>
      <?pagebreak page853?><p id="d1e2244">Field data for sills in the SRSVF can be fitted to an elliptical region on
the stereonet with a NW–SE long axis (Fig. 7b), giving horizontal NE–SW
maximum compression where <inline-formula><mml:math id="M148" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> plunges 3<inline-formula><mml:math id="M149" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> towards
068<inline-formula><mml:math id="M150" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>; <inline-formula><mml:math id="M151" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> is vertical, plunging 87<inline-formula><mml:math id="M152" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> towards
265<inline-formula><mml:math id="M153" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>; and <inline-formula><mml:math id="M154" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> is horizontal, plunging 1<inline-formula><mml:math id="M155" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> towards
158<inline-formula><mml:math id="M156" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> (Fig. 7c). Using the stereonet data in Fig. 7c, we derive the
angles <inline-formula><mml:math id="M157" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">θ</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M158" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">θ</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, which are used to calculate the stress
ratio (<inline-formula><mml:math id="M159" display="inline"><mml:mi mathvariant="italic">ϕ</mml:mi></mml:math></inline-formula>) and driving pressure ratio (<inline-formula><mml:math id="M160" display="inline"><mml:mrow><mml:msup><mml:mi>R</mml:mi><mml:mo>′</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula>) by Jolly and
Sanderson (1997):
          <disp-formula id="Ch1.E6" content-type="numbered"><mml:math id="M161" display="block"><mml:mrow><mml:mi mathvariant="italic">ϕ</mml:mi><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>+</mml:mo><mml:mi>cos⁡</mml:mi><mml:mo>(</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:msub><mml:mi mathvariant="italic">θ</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>+</mml:mo><mml:mi>cos⁡</mml:mi><mml:mo>(</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:msub><mml:mi mathvariant="italic">θ</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:mfrac></mml:mstyle><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
        and
          <disp-formula id="Ch1.E7" content-type="numbered"><mml:math id="M162" display="block"><mml:mrow><mml:msup><mml:mi>R</mml:mi><mml:mo>′</mml:mo></mml:msup><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>+</mml:mo><mml:mi mathvariant="normal">cos</mml:mi><mml:mo>(</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:msub><mml:mi mathvariant="italic">θ</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow><mml:mn mathvariant="normal">2</mml:mn></mml:mfrac></mml:mstyle><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
        where <inline-formula><mml:math id="M163" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">θ</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> is the angle between the <inline-formula><mml:math id="M164" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> axis and the
perimeter of the dilational ellipse and <inline-formula><mml:math id="M165" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">θ</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> is the angle between the
<inline-formula><mml:math id="M166" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> axis and the dilational ellipse (Jolly and Sanderson, 1997).
When an ellipse can only be fitted to the zone of no dilation, Jolly and
Sanderson (1997) provide an alternative method for calculating <inline-formula><mml:math id="M167" display="inline"><mml:mi mathvariant="italic">ϕ</mml:mi></mml:math></inline-formula>. The
<inline-formula><mml:math id="M168" display="inline"><mml:mrow><mml:msup><mml:mi>R</mml:mi><mml:mo>′</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula> value is two-dimensional (2-D); it does not take into account the
magnitude of <inline-formula><mml:math id="M169" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>. The three-dimensional relationship between the
fluid pressure and all principal stresses is illustrated by the ellipse
geometry on the stereonet (Fig. 7c, d), and can also be visualised through
construction of a 3-D Mohr circle (Fig. 7e).</p>
      <p id="d1e2539">The calculated <inline-formula><mml:math id="M170" display="inline"><mml:mi mathvariant="italic">ϕ</mml:mi></mml:math></inline-formula> (0.77) and <inline-formula><mml:math id="M171" display="inline"><mml:mrow><mml:msup><mml:mi>R</mml:mi><mml:mo>′</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula> (0.68) values define the stress ratio
and driving stress used to create the opening angle mechanical model
(Fig. 7d). For the model, we assigned a minimum vertical stress of 25 MPa
to simulate a <inline-formula><mml:math id="M172" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 1 km emplacement depth (Gartner, 1986). Development of
extensional-shear fractures requires a low differential stress (<inline-formula><mml:math id="M173" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi mathvariant="normal">D</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>: <inline-formula><mml:math id="M174" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>–<inline-formula><mml:math id="M175" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>): 4<inline-formula><mml:math id="M176" display="inline"><mml:mrow><mml:mi>T</mml:mi><mml:mo>&lt;</mml:mo><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi mathvariant="normal">D</mml:mi></mml:msub><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">5.66</mml:mn><mml:mi>T</mml:mi></mml:mrow></mml:math></inline-formula>;
compressional shear faults require that <inline-formula><mml:math id="M177" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi mathvariant="normal">D</mml:mi></mml:msub><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">5.66</mml:mn><mml:mi>T</mml:mi></mml:mrow></mml:math></inline-formula> (<inline-formula><mml:math id="M178" display="inline"><mml:mi>T</mml:mi></mml:math></inline-formula> is
the host rock tensile strength; Sibson, 2003). Due to the bimodal (conjugate)
dip distribution of the sills, their consistent near-vertical opening
direction, and the mutual cross-cutting and intrusive relationship between
thrust faults and sills, we estimated that <inline-formula><mml:math id="M179" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi mathvariant="normal">D</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">6</mml:mn><mml:mi>T</mml:mi></mml:mrow></mml:math></inline-formula>. We
estimate the tensile strength of the host rock at 1 km depth to be 3 MPa,
giving <inline-formula><mml:math id="M180" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi mathvariant="normal">D</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">18</mml:mn></mml:mrow></mml:math></inline-formula> MPa. It should be noted, however, that due
to the nature of the model, providing all parameters are scaled relative to
<inline-formula><mml:math id="M181" display="inline"><mml:mi>T</mml:mi></mml:math></inline-formula>, the value of <inline-formula><mml:math id="M182" display="inline"><mml:mi>T</mml:mi></mml:math></inline-formula> does not change the resulting opening angle pattern,
only the magnitudes of the principal stresses and fluid pressure. <inline-formula><mml:math id="M183" display="inline"><mml:mi mathvariant="italic">ϕ</mml:mi></mml:math></inline-formula>
(0.77) and <inline-formula><mml:math id="M184" display="inline"><mml:mrow><mml:msup><mml:mi>R</mml:mi><mml:mo>′</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula> (0.68) derived in the model indicate a mild horizontal radial
compression during emplacement, with fluid pressure less than <inline-formula><mml:math id="M185" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>
(Fig. 7d, e).</p>
      <p id="d1e2723">The measured opening angles of the studied sills fit with the contouring of a
single ellipse (Fig. 7d), suggesting that during the intrusion of sills in
the study area, the fluid pressure and stress state remained relatively
constant. However, we acknowledge that a broader study across the SRSVF may
reveal spatio-temporal fluctuations in either the stress regime or magma
pressure.</p>
</sec>
<?pagebreak page854?><sec id="Ch1.S5">
  <title>Discussion</title>
<sec id="Ch1.S5.SS1">
  <title>Sill geometry as a record of far-field stress</title>
      <p id="d1e2738">Sills in the SRSVF are mildly transgressive, in that although they have
intruded parallel to bedding at a local scale (e.g. Fig. 5b, c, f), at the
field-scale they cut across the stratigraphy at a low angle (Figs. 4d and
5a–b; Walker et al., 2017). Transgressive sill geometries are typically
inferred to represent either the peripheral section of a saucer-shaped sill
(e.g. Malthe-Sørenssen et al., 2004) or a low-angle cone sheet emanating
from a magma chamber (e.g. Gudmundsson, 2006; Martí and Geyer,
2009). In either case, the transgressive
segments should have an overall centripetal dip distribution. No magma
chamber has been identified in the SRSVF, and the sills do not dip towards a
central source, nor do they have a saucer-shaped geometry. Sills in the SRSVF
show consistent bimodal dip patterns, with mutual cross-cutting
relationships, at the outcrop to field scale (i.e. for sills that are
centimetres to tens of metres thick). We infer, as noted by Walker et
al. (2017), that the bimodal sill geometry is representative of low-angle
conjugate faults, which required a deviatoric stress state
(<inline-formula><mml:math id="M186" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi mathvariant="normal">D</mml:mi></mml:msub><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">5.66</mml:mn><mml:mi>T</mml:mi></mml:mrow></mml:math></inline-formula>; Sibson, 2003) during emplacement.</p>
      <p id="d1e2758">At the local (centimetre–metre) scale, the SRSVF sills display a range of
attitudes with consistent vertical opening directions and attitude-dependent
thickness variations. In a low-deviatoric stress state, local variations in
intrusion attitude are traditionally inferred to represent rotations of the
principal stress axes, which may be caused by the effects of mechanical
layering (e.g. Gudmundsson, 2011a), or pre-existing faults and fractures
(e.g. Fossen, 2010; Magee et al., 2013). Local stress rotations would
therefore cause intrusions of any attitude to dilate in a Mode I sense,
producing a polymodal distribution of opening directions across an intrusive
suite. In that case, the aperture (true thickness) of the segment would be
dominantly controlled by the host rock elastic properties (mainly Young's
modulus, <inline-formula><mml:math id="M187" display="inline"><mml:mi>E</mml:mi></mml:math></inline-formula>) (e.g. Brenner and Gudmundsson, 2004). Units with low <inline-formula><mml:math id="M188" display="inline"><mml:mi>E</mml:mi></mml:math></inline-formula> are
less stiff than those with high <inline-formula><mml:math id="M189" display="inline"><mml:mi>E</mml:mi></mml:math></inline-formula>; i.e. a low <inline-formula><mml:math id="M190" display="inline"><mml:mi>E</mml:mi></mml:math></inline-formula> material will accrue more
strain for a given stress. Accordingly, when a fluid-filled fracture, with
constant fluid pressure, cross-cuts units with varying elastic properties, it
will have a larger aperture in units with low <inline-formula><mml:math id="M191" display="inline"><mml:mi>E</mml:mi></mml:math></inline-formula> and a smaller aperture in
units with higher <inline-formula><mml:math id="M192" display="inline"><mml:mi>E</mml:mi></mml:math></inline-formula> (Brenner and Gudmundsson, 2004; Gudmundsson, 2011b).
Local attitude variations in the SRSVF sills do not correspond solely to
bedding interfaces. Although we infer that the inclined sill sections are
dilated pre-existing fractures, the consistent vertical opening directions
suggest that inclined fractures were subject to extensional
shear rather than Mode I
dilation. This is supported by the attitude-dependant (rather than
lithology-dependent) thickness variations; horizontal sill segments are
consistently thicker than adjoining inclined segments, regardless of the
hosting lithology.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F8" specific-use="star"><caption><p id="d1e2806">Sill geometry and paleostress analyses of deformation structures in
the San Rafael subvolcanic field. <bold>(a)</bold> Field example for comparison
between sill and thrust-fault geometry. <bold>(b–d)</bold> Lower-hemisphere
equal-area projections with calculated stress axes given as plunge–trend
measurements. <bold>(b)</bold> Local sill–host rock contact data; Bingham
analysis (Yamaji, 2016) used to calculate principal stress axes, shown with
95 % confidence regions and density contours (shaded region).
Panels <bold>(c)</bold> and <bold>(d)</bold> are mechanical models contoured for slip
tendency (<inline-formula><mml:math id="M193" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) and dilation tendency (<inline-formula><mml:math id="M194" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>),
respectively.</p></caption>
          <?xmltex \igopts{width=398.338583pt}?><graphic xlink:href="https://se.copernicus.org/articles/9/847/2018/se-9-847-2018-f08.pdf"/>

        </fig>

      <p id="d1e2853">Areas that host several intrusion sets, with different attitudes, are
commonly interpreted to represent discrete and separate intrusive events
(e.g. Delaney and Gartner, 1997; Walker, 1993). Our study, however, suggests
that the observed range of sill attitudes is indicative of magmatism during
a deviatoric far-field stress state (e.g. Walker, 2016; Walker et al.,
2017). The sills may, therefore, be equivalent to reverse faults in the
area, accommodating horizontal shortening and vertical thickening.</p>
</sec>
<sec id="Ch1.S5.SS2">
  <title>Accommodation of shortening: comparing sills and reverse faults in
the San Rafael subvolcanic field</title>
      <p id="d1e2862">The SRSVF is host to dikes and sills; the sills cut, and are cut by, thrust
(and reverse) faults that dip to the NE and SW (Figs. 5f, 8a; Walker et al.,
2017). Thrusts, deformation bands, and gypsum veins in the region form
conjugate sets (Fig. 5d–i), which record a coaxial horizontal shortening and
vertical thickening (Walker et al., 2017). Right dihedra paleostress analysis
(using the method of Delvaux and Sperner, 2003) of the thrust faults and
deformation bands in the San Rafael show a close correlation with the
calculated stress state results for sills, with an angular mismatch
among the maximum principal stress axes of <inline-formula><mml:math id="M195" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 4<inline-formula><mml:math id="M196" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>; <inline-formula><mml:math id="M197" display="inline"><mml:mi mathvariant="italic">ϕ</mml:mi></mml:math></inline-formula> values calculated for the faults are lower than for the sills, at
0.53–0.56 (Fig. 5h, i). For comparison, Bingham analyses (Yamaji, 2016) of
the local sill contact data derive an average <inline-formula><mml:math id="M198" display="inline"><mml:mi mathvariant="italic">ϕ</mml:mi></mml:math></inline-formula> value of 0.63 and
principal stress axes creating a 6<inline-formula><mml:math id="M199" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> angular mismatch with the opening
angle and right dihedra models (Fig. 8b). To further constrain the<?pagebreak page855?> stress
ratio, and the relationship between intrusions and contractional shear
structures, we input the thrust fault, deformation band, gypsum vein, and
overall sill geometry pole data into mechanical models of normalised slip
tendency (<inline-formula><mml:math id="M200" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>; Fig. 8c) and dilation tendency (<inline-formula><mml:math id="M201" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>;
Fig. 8d). Although typically used to assess the reactivation potential of
pre-existing structures in a present-day stress state (e.g. Ferrill et al.,
1999), the models can also be used to fit a paleostress state to field data
(e.g. Stephens et al., 2017). Normalised slip tendency (<inline-formula><mml:math id="M202" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mo>(</mml:mo><mml:mi mathvariant="italic">τ</mml:mi><mml:mo>/</mml:mo><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi mathvariant="normal">n</mml:mi></mml:msub><mml:mo>)</mml:mo><mml:mo>/</mml:mo><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub><mml:mo>max⁡</mml:mo></mml:mrow></mml:math></inline-formula>; Morris et al., 1996) and dilation
tendency (<inline-formula><mml:math id="M203" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>–<inline-formula><mml:math id="M204" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi mathvariant="normal">n</mml:mi></mml:msub><mml:mo>)</mml:mo><mml:mo>/</mml:mo><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>–<inline-formula><mml:math id="M205" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>); Ferrill et al., 1999) are calculated from the
stresses acting on a plane, or potential plane. This can be used to predict
the attitude of both potential failure planes and pre-existing fractures that
are susceptible to reactivation in a given stress state. Notably, the zone of
high <inline-formula><mml:math id="M206" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> (0.8–1.0) overlaps with the zone of high <inline-formula><mml:math id="M207" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>
(0.8–1.0), suggesting a zone of potential extensional shear. To enable
conjugate shear failure, we used the same differential stress of 6<inline-formula><mml:math id="M208" display="inline"><mml:mi>T</mml:mi></mml:math></inline-formula>, where
<inline-formula><mml:math id="M209" display="inline"><mml:mrow><mml:mi>T</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:math></inline-formula> MPa, as used previously. By fitting the zones of high slip tendency
to the combined thrust-fault and deformation band data, and zones of high
dilation tendency to the overall sill geometry and gypsum vein data, we were
able to derive a best-fit <inline-formula><mml:math id="M210" display="inline"><mml:mi mathvariant="italic">ϕ</mml:mi></mml:math></inline-formula> value of 0.65, with a horizontal NE–SW
<inline-formula><mml:math id="M211" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> that plots within the 6<inline-formula><mml:math id="M212" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> angular mismatch. The <inline-formula><mml:math id="M213" display="inline"><mml:mi mathvariant="italic">ϕ</mml:mi></mml:math></inline-formula> value is consistent with the right dihedra (<inline-formula><mml:math id="M214" display="inline"><mml:mrow><mml:mi mathvariant="italic">ϕ</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula>.53; Fig. 5h, i),
Bingham analysis (<inline-formula><mml:math id="M215" display="inline"><mml:mrow><mml:mi mathvariant="italic">ϕ</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula>.63; Fig. 8a), and our opening angle models (<inline-formula><mml:math id="M216" display="inline"><mml:mrow><mml:mi mathvariant="italic">ϕ</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula>.77; Fig. 7). The field observations combined with the paleostress
analyses suggest that sill emplacement took place during a state of mild
horizontal radial compression.</p>
      <p id="d1e3128">A key difference between the strains recorded by sills and thrusts is the
dominance of dilation during sill emplacement and compressional shear during
thrusting. The range of local dips, and consistent vertical opening, suggests
that the sills were emplaced by a combination of brittle failure and dilation
of pre-existing structures (including thrust faults), in which the fluid
overpressure accommodates both shear and dilation. Consistent with the
interpretation of Walker<?pagebreak page856?> et al. (2017), our field observations and mechanical
model results suggest that the sills represent conjugate intrusions, which
record the continuity of horizontal shortening during periods of elevated
magmatic pressure.</p>
      <p id="d1e3131">While the opening angle of dilated fractures has been used here to
characterise the paleostress state during dilation of pre-existing
cohesionless fractures, we envisage that it could also be applied to
extension or extensional-shear fractures, formed via failure of intact rock.
In these cases, we would expect the fracture network to resemble a mesh
structure (e.g. Sibson, 1996), which comprises predominantly parallel
(Mode I) and bimodal (conjugate extensional-shear) fractures, which dip at a
low angle to <inline-formula><mml:math id="M217" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, with opening angles of <inline-formula><mml:math id="M218" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> 20<inline-formula><mml:math id="M219" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> (e.g.
Hancock, 1985; Ramsey and Chester, 2004). Importantly, the models presented
in this study can be used to determine whether intrusive suites record
changes in the tectonic stress state, or to identify fluid pressure pulses of
varying magnitude in a single governing far-field stress state. These
attributes have significant implications for improving our understanding of
the development of past and present-day magmatic systems.</p>
</sec>
</sec>
<sec id="Ch1.S6" sec-type="conclusions">
  <title>Conclusions</title>
      <p id="d1e3168">Our mechanical models build upon the work of Delaney et al. (1986) and Jolly
and Sanderson (1997) to use fracture geometry and opening angles to derive
the principal stress axes during sill emplacement and provide crucial new
constraints on the stress state and fluid pressure, applicable to dikes,
sills, and veins. The geometry of sills in the SRSVF records a continuous
horizontal shortening that is otherwise accommodated by contractional faults
in the area. Contoured regions on stereonets for opening angles suggest that
in a high deviatoric stress state, it should be relatively rare for
intrusions to be purely Mode I structures. In such settings, it should be
commonplace for intrusions to accommodate a component of shear during their
emplacement. Our opening angle model is particularly useful in determining
paleostress states for regions where there is little brittle deformation
(i.e. faulting), other than intrusions, and it may therefore present a useful
and important tool in tectonic and magmatic studies.</p>
</sec>

      
      </body>
    <back><notes notes-type="codeavailability">

      <p id="d1e3175">The <italic>FracTend</italic> MATLAB code will be made publically
available via GitHub in due course. The code is currently being prepared for
upload; in the meantime, the code is available upon request from David Healy
(d.healy@abdn.ac.uk).</p>
  </notes><notes notes-type="dataavailability">

      <p id="d1e3184">Field locations can be found in Fig. 4. The overall sill
geometry data used in Fig. 4 are from Walker et al. (2017). The structural
field data are available in the Supplement of this work.</p>
  </notes><app-group>
        <supplementary-material position="anchor"><p id="d1e3187"><bold>The Supplement related to this article is available online at <inline-supplementary-material xlink:href="https://doi.org/10.5194/se-9-847-2018-supplement" xlink:title="zip">https://doi.org/10.5194/se-9-847-2018-supplement</inline-supplementary-material>.</bold></p></supplementary-material>
        </app-group><notes notes-type="authorcontribution">

      <p id="d1e3193">Field data were collected by TLS, AB, and RJW. RJW and AB provided valuable
discussions in the field, as well as during paper preparation, along
with RWE and DH. DH developed the <italic>FracTend</italic> MATLAB code. TLS prepared
the paper with contributions from all co-authors.</p>
  </notes><?xmltex \hack{\newpage}?><notes notes-type="competinginterests">

      <p id="d1e3203">The authors declare that they have no conflict of
interest.</p>
  </notes><ack><title>Acknowledgements</title><p id="d1e3209">This work was undertaken during Tara L. Stephens's PhD studentship, supported
by the Central England Natural Environmental Research Council (NERC) Training
Alliance (CENTA) (award reference: 1503848). The authors would like to thank
Nicolas Le Corvec and the anonymous reviewer for their helpful comments during
the reviewing process. Additionally we would like to thank Craig Magee,
Atsushi Yamaji, and an anonymous reviewer for their constructive reviews on
an earlier version of the paper.<?xmltex \hack{\newline}?><?xmltex \hack{\newline}?>
Edited by: Gwenn Peron-Pinvidic <?xmltex \hack{\newline}?>
Reviewed by: Nicolas Le Corvec and one anonymous referee</p></ack><ref-list>
    <title>References</title>

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  </ref-list></back>
    <!--<article-title-html>Mechanical models to estimate the paleostress state from igneous intrusions</article-title-html>
<abstract-html><p>Dikes and sills represent an important component of the deformation history
in volcanic systems, but unlike dikes, sills are typically omitted from
traditional paleostress analyses in tectonic studies. The emplacement of
sheet intrusions is commonly associated with Mode I fracturing in a low
deviatoric stress state, in which dilation is perpendicular to the fracture
plane. Many natural examples of sills and dikes, however, are observed to
accommodate minor shear offsets, in addition to a component of dilation. Here
we present mechanical models for sills in the San Rafael subvolcanic field,
Utah, which use field-based measurements of intrusion attitude and opening
angles to constrain the tectonic stress axes during emplacement and the
relative magma pressure for that stress state. The sills display bimodal dips
to the NE and SW and consistent vertical opening directions, despite variable
sill dips. Based on sill attitude and opening angles, we find that the sills
were emplaced during a phase of NE–SW horizontal shortening. Calculated
principal stress axes are consistent (within  ∼  4°) with
paleostress results for penecontemporaneous thrust faults in the area. The
models presented here can be applied to any set of dilational structures,
including dikes, sills, or hydrous veins, and represent a robust method for
characterising the paleostress state in areas where other brittle deformation
structures (e.g. faults) are not present.</p></abstract-html>
<ref-html id="bib1.bib1"><label>1</label><mixed-citation>
Airoldi, G., Muirhead, J. D., White, J. D. L., and Rowland, J.: Emplacement
of magma at shallow depth: insights from field relationships at Allan Hills,
south Victoria Land, East Antarctica, Antarct. Sci., 23, 281–296,
<a href="https://doi.org/10.1017/s0954102011000095" target="_blank">https://doi.org/10.1017/s0954102011000095</a>, 2011.
</mixed-citation></ref-html>
<ref-html id="bib1.bib2"><label>2</label><mixed-citation>Anderson, E. M.: The dynamics of faulting and dike formation with
applications to Britain, Oliver and Boyd, Edinburgh, UK, 1951.
</mixed-citation></ref-html>
<ref-html id="bib1.bib3"><label>3</label><mixed-citation>Baer, G.: Mechanisms of dike propagation in layered rocks and in massive,
porous sedimentary rocks, J. Geophys. Res., 96, 11911, <a href="https://doi.org/10.1029/91JB00844" target="_blank">https://doi.org/10.1029/91JB00844</a>,
1991.
</mixed-citation></ref-html>
<ref-html id="bib1.bib4"><label>4</label><mixed-citation>Baer, G., Beyth, M., and Reches, Z. E.: Dikes emplaced into fractured
basement, Timna Igneous Complex, Israel, J. Geophys. Res.-Sol. Ea., 99,
24039–24050, <a href="https://doi.org/10.1029/94JB02161" target="_blank">https://doi.org/10.1029/94JB02161</a>, 1994.
</mixed-citation></ref-html>
<ref-html id="bib1.bib5"><label>5</label><mixed-citation>Brenner, S. L. and Gudmundsson, A: Arrest and aperture variation of
hydrofractures in layered reservoirs, Geol. Soc. London Spec. Publ., 231,
117–128, 2004.
</mixed-citation></ref-html>
<ref-html id="bib1.bib6"><label>6</label><mixed-citation>Delaney, P. T.  and Gartner, A. E.: Physical processes of shallow mafic dike
emplacement near the San Rafael Swell, Utah, Geol. Soc. Am. Bull., 109,
1177–1192, <a href="https://doi.org/10.1130/0016-7606(1997)109&lt;1177:pposmd&gt;2.3.co;2" target="_blank">https://doi.org/10.1130/0016-7606(1997)109&lt;1177:pposmd&gt;2.3.co;2</a>, 1997.
</mixed-citation></ref-html>
<ref-html id="bib1.bib7"><label>7</label><mixed-citation>Delaney, P. T., Pollard, D. D., Ziony, J. I., and McKee, E. H.: Field
relations between dikes and joints: Emplacement processes and paleostress
analysis, J. Geophys. Res., 91, 4920, <a href="https://doi.org/10.1029/JB091iB05p04920" target="_blank">https://doi.org/10.1029/JB091iB05p04920</a>, 1986.
</mixed-citation></ref-html>
<ref-html id="bib1.bib8"><label>8</label><mixed-citation>Delvaux, D. and Sperner, B.: New aspects of tectonic stress inversion with
reference to the TENSOR program, Geol. Soc. London Spec. Publ., 212, 75–100,
<a href="https://doi.org/10.1144/gsl.sp.2003.212.01.06" target="_blank">https://doi.org/10.1144/gsl.sp.2003.212.01.06</a>, 2003.
</mixed-citation></ref-html>
<ref-html id="bib1.bib9"><label>9</label><mixed-citation>Eide, C. H., Schofield, N., Jerram, D. A., and Howell, J. A.: Basin-scale
architecture of deeply emplaced sill complexes: Jameson Land, East Greenland,
J. Geol. Soc., 174, 23–40, <a href="https://doi.org/10.1144/jgs2016-018" target="_blank">https://doi.org/10.1144/jgs2016-018</a>, 2016.
</mixed-citation></ref-html>
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from the patterns of volcanic activity, Geol. Soc. London Spec. Publ., 39,
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</mixed-citation></ref-html>
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Armstrong, A., and Morris, A. P.: Stressed Rock Strains Groundwater at Yucca
Mountain, Nevada, GSA Today, 9, 1–8, 1999.
</mixed-citation></ref-html>
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Fossen, H.: Structural Geology, Cambridge University Press, New York, USA,
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Gaffney, E. S., Damjanac, B., and Valentine, G. A.: Localization of volcanic
activity: 2. Effects of pre-existing structure, Earth Planet. Sc. Lett., 263,
323–338, <a href="https://doi.org/10.1016/j.epsl.2007.09.002" target="_blank">https://doi.org/10.1016/j.epsl.2007.09.002</a>, 2007.
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