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<article xmlns:xlink="http://www.w3.org/1999/xlink" xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:oasis="http://docs.oasis-open.org/ns/oasis-exchange/table" xml:lang="en" dtd-version="3.0"><?xmltex \bartext{Stop 2}?>
  <front>
    <journal-meta><journal-id journal-id-type="publisher">DEUQUASP</journal-id><journal-title-group>
    <journal-title>DEUQUA Special Publications</journal-title>
    <abbrev-journal-title abbrev-type="publisher">DEUQUASP</abbrev-journal-title><abbrev-journal-title abbrev-type="nlm-ta">DEUQUA Spec. Pub.</abbrev-journal-title>
  </journal-title-group><issn pub-type="epub">2625-8137</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/deuquasp-2-19-2019</article-id><title-group><article-title>Sea cliff at Kieler Ufer (Pleistocene stripes 11–16) – large-scale
architecture and kinematics of the Jasmund<?xmltex \hack{\break}?> Glacitectonic Complex</article-title><alt-title>Sea cliff at Kieler Ufer (Pleistocene stripes 11–16)</alt-title>
      </title-group><?xmltex \runningtitle{Sea cliff at Kieler Ufer (Pleistocene stripes 11--16)}?><?xmltex \runningauthor{A. Gehrmann et al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes" rid="aff1">
          <name><surname>Gehrmann</surname><given-names>Anna</given-names></name>
          <email>anna.gehrmann@uni-greifswald.de</email>
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Meschede</surname><given-names>Martin</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Hüneke</surname><given-names>Heiko</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-7509-8768</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Pedersen</surname><given-names>Stig A. Schack</given-names></name>
          
        </contrib>
        <aff id="aff1"><label>1</label><institution>Institut für Geographie und Geologie, Universität Greifswald,
Friedrich-Ludwig-Jahn-Str. 17a, 17487 Greifswald, Germany</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>Geological Survey of Denmark and Greenland (GEUS), Øster Voldgade
10, 1350 Copenhagen, Denmark</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Anna Gehrmann (anna.gehrmann@uni-greifswald.de)</corresp></author-notes><pub-date><day>15</day><month>August</month><year>2019</year></pub-date>
      
      <volume>2</volume>
      <fpage>19</fpage><lpage>27</lpage>
      
      <permissions>
        <copyright-statement>Copyright: © 2019 Anna Gehrmann et al.</copyright-statement>
        <copyright-year>2019</copyright-year>
      <license license-type="open-access"><license-p>This work is licensed under the Creative Commons Attribution 4.0 International License. To view a copy of this licence, visit <ext-link ext-link-type="uri" xlink:href="https://creativecommons.org/licenses/by/4.0/">https://creativecommons.org/licenses/by/4.0/</ext-link></license-p></license></permissions><self-uri xlink:href="https://deuquasp.copernicus.org/articles/2/19/2019/deuquasp-2-19-2019.html">This article is available from https://deuquasp.copernicus.org/articles/2/19/2019/deuquasp-2-19-2019.html</self-uri><self-uri xlink:href="https://deuquasp.copernicus.org/articles/2/19/2019/deuquasp-2-19-2019.pdf">The full text article is available as a PDF file from https://deuquasp.copernicus.org/articles/2/19/2019/deuquasp-2-19-2019.pdf</self-uri>
      <abstract><title>Abstract</title>
    <p id="d1e105">The Kieler Ufer cliff section is a structural key
location in the late Weichselian thrust-dominated-to-fold–thrust-dominated
glacitectonic complex of Jasmund. Restoration and balancing of geological
cross sections from the eastern coast (southern sub-complex) enabled strain
quantification and the illustration of stress orientation. The entire
horizontal shortening of the Kieler Ufer section is 1280 m (51.6 %) at its
minimum. The thrust faults generally inclined towards south indicate a local
glacier push from the S/SSW, which fits well into the glacio-dynamic model
suggested by Gehrmann and Harding (2018).</p>
  </abstract>
      <custom-meta-group><custom-meta><meta-name>citationstatement</meta-name><meta-value>Gehrmann, A., Meschede, M., Hüneke, H., and Pedersen, S. A. S.: Sea cliff at Kieler Ufer (Pleistocene stripes 11–16) – large-scale
architecture and kinematics of the Jasmund Glacitectonic Complex, DEUQUA Spec. Pub., 2, 19–27, https://doi.org/10.5194/deuquasp-2-19-2019, 2019.</meta-value></custom-meta></custom-meta-group>
    </article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <label>1</label><title>Introduction</title>
      <p id="d1e117">The sea cliff Kieler Ufer (KU) is located on the east coast of Jasmund, and
it is easily accessible via the stairs at the creek Kieler Bach
(54<inline-formula><mml:math id="M1" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>33.165<inline-formula><mml:math id="M2" display="inline"><mml:msup><mml:mi/><mml:mo>′</mml:mo></mml:msup></mml:math></inline-formula> N, 13<inline-formula><mml:math id="M3" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>40.594<inline-formula><mml:math id="M4" display="inline"><mml:msup><mml:mi/><mml:mo>′</mml:mo></mml:msup></mml:math></inline-formula> E), which crosses the
fault boundary between the imbricates S13 and S14 (Fig. 1a). The
abbreviation S used in conjunction with a number stands for “section”, and the section numbers S11 to S16 in
the Kieler Ufer cliff profile have been adapted from the Pleistocene-stripe
annotations given by Jaekel (1917). The horizontal length of the entire
cross section is 1202 m. The highest point of the cliff profile is at the
southernmost top of S15 (64 m a.s.l.).</p>
      <p id="d1e156">The Kieler Ufer section represents a key area in the contractional
fold-and-thrust system of Jasmund's southern structural sub-complex, which
is a large imbricate fan with a number of individual thrust sheets and at
least three duplex stacks (S01 to S23) (Gehrmann, 2018; Gehrmann and
Harding, 2019). The large-scale glacitectonic folds and
associated thrusts deforming both Upper Cretaceous (Maastrichtian) chalk and
Pleistocene glacial deposits were formed in the Pomeranian W2 phase of the
late Weichselian (see Kenzler and Hüneke, 2019). The
detailed stratigraphy of the Maastrichtian chalk outlined by the flint-band
numbers has been adapted from Steinich (1972). The Pleistocene sediments lie
paraconformably on the chalk, parallel to this major lithostratigraphical
boundary. The older glacial sediments (older than Pomeranian W2 phase) are
subdivided into the tills/diamictons M1 and M2 that are separated and
overlain by the units I1 and partly I2 with interbedded gravel, sand, and
clay (e.g. Steinich, 1972; Panzig, 1995; Müller and Obst, 2006; Kenzler
et al., 2015, 2016). These glacial deposits are cut by thrust faults at the
trailing end of each imbricate in the SSW, below the large hanging-wall
anticlines of the<?pagebreak page20?> southerly adjoining thrust sheets. The youngest M3
sediment complex (Pomeranian W2 phase/Mecklenburg W3 phase) lies
unconformably upon a major erosion surface, which truncates the underlying
glacitectonised sequence (chalk, M1, I1, M2, I2) (e.g. Steinich, 1972;
Panzig, 1995; Müller and Obst, 2006; Niedermeyer et al., 2010). At the
top of the Kieler Ufer cliff the M3 complex is only exposed in small
patches. The tectonic setting at the Kieler Ufer shows an imbricate fan with
six major thrust sheets subjected to fault-bend folding (Fig. 1b).
The six thrust sheets S11 to S16 strike SSW–NNE and are exposed by the
N–S-trending sea cliff at high angle.</p>
      <p id="d1e159">Cross-section restoration and balancing is an increasingly applied
kinematic-analysis technique in glacial environments. This was well
demonstrated for instance by Croot (1987), Pedersen (2005), and Benediktsson
et al. (2010). The restoration of the Kieler Ufer section has been performed
on the single imbricates of the cliff profile in several experiments using
different algorithms and bedding geometries until the best-fit
interpretation could be used for shortening calculations and further
interpretation (software: Move and the supplementary module 2-D Kinematic
Modelling). The tectonic model, which best explains the geometry of the six
thrust sheets at the Kieler Ufer is shown in Fig. 1. Regarding
the structural evolution of classic fold-and-thrust belts, the restoration
worked backwards from the distal to the proximal deformation area (see
Pedersen, 2005). Thus, the youngest sheet S16 (closest to the foreland of
the southern structural sub-complex) was first restored, and the oldest sheet
S11 (closest to the hinterland) was restored in the end. Within the scope of the
restoration, the individual thrust sheets (S11 to S16) have been renamed
(KU1, KU2, KU3d1, KU3d2, KU3d3, KU4) according to the chronology of
re-deformation (see Figs. 1 and 5). The orientation values of
beds and faults were adapted from the best-fit model of the Kieler Ufer
section, and they have been compared with those given by Steinich (1972).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1" specific-use="star"><?xmltex \currentcnt{1}?><label>Figure 1</label><caption><p id="d1e165">Structural conditions of the Kieler Ufer section (S11 to S16). <bold>(a)</bold> Overview of the thrust sheets S11 to S16 at the cliff coast. The red/yellow
lines indicate thrust faults. The black dashed lines show the sedimentary
boundary between Cretaceous chalk and Pleistocene glacigenic deposits. <bold>(b)</bold> Projected and interpreted cross section (simplified). Architectural surfaces
are marked by numbers 1 to 3. Transparent fields represent approximate
interpretations.</p></caption>
        <?xmltex \igopts{width=483.69685pt}?><graphic xlink:href="https://deuquasp.copernicus.org/articles/2/19/2019/deuquasp-2-19-2019-f01.png"/>

      </fig>

</sec>
<sec id="Ch1.S2">
  <label>2</label><title>The Kieler Ufer section as representative part of Jasmund's southern
structural sub-complex</title>
      <p id="d1e188">There are generally three individual thrust sheets: S16, S15, and S11 (KU1,
KU2, and KU4). A duplex stack consisting of S14, S13, and S12 (KU3d1, KU3d2,
and KU3d3) and the lowermost part of the thrust sheet S15 (KU2) are
subject to debate. The highest point of the interpreted cross section is the
hanging-wall anticline of S14 (166 m a.s.l.). Three different
architectural surfaces occur between S11 and S16 (sensu stricto Pedersen, 2014)
(Fig. 1b). The top of the cliff and minor zones, where the base-M3
unconformity occurs (mainly S12 and S16), are first-order surfaces. Another
first-order surface is the décollement zone at ca. 120 m b.s.l. The
ramps and upper flats between the sections are second-order surfaces.
Considering the duplex stack, the intermediate flat at ca. 92 m b.s.l.
(KU3d3) also belongs to the second-order surfaces. The bedding outlining
the hanging-wall anticlines and the footwall syncline in S13 belong to the
third order.</p>
      <p id="d1e191">The Kieler Ufer section contains at least five satellite faults, which may
have formed during the glacitectonic thrusting (Fig. 1b). Their age
(post-, pre-, syn-tectonic) is difficult to determine, as they are truncated
by the erosional unconformity at the cliff top. However, the interpretation
can be related to the best-fit model using Move and the supplementary module
2-D Kinematic Modelling as well as comparisons with the faults in the
surrounding sections. The reverse satellite fault in S16 dips steeply
towards the SW, 235/70 (dip direction/dip), and shows an offset of at least 6 m.
The satellite fault in S15 (presumably 250/47, 250/56) forms a vertical
splay at a branch point about 7 m a.s.l. The offset at the main fault is
about 10 m in the lowermost part. Above the branch point, the offset is less
strong with ca. 3 to 4 m at each fault. The satellite fault in S13 may be
moderately to steeply inclined towards the S (190/61), which is similar to that
in S12. The northerly reverse fault in thrust sheet S11 is also assumed to
have formed during glacitectonism of the southern structural sub-complex. It
dips towards the SW by 72<inline-formula><mml:math id="M5" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>. The southern reverse fault (205/80), on
contrary, can certainly be interpreted as a pre-Quaternary structure, since
it does not displace the chalk top and the Pleistocene beds above
(Fig. 1b).</p>
<sec id="Ch1.S2.SS1">
  <label>2.1</label><title>The youngest thrust sheets S16 (KU1) and S15 (KU2)</title>
      <p id="d1e210">The footwall-ramp panel of the thrust sheet S16 contains flint bands and
Pleistocene beds, which are gently inclined to the SSW (Fig. 2a). The
beds steepen towards the centre of the tight hanging-wall anticline in the
northern part. The Pleistocene deposits reach the cliff bottom, since their
trend corresponds to the geometry of the moderately inclined footwall ramp
below S16 and they are cut by the S15/S16 thrust fault only at or even
closely below the cliff bottom (Figs. 1 and 2a). The frontal thrust
fault of the Kieler Ufer section below S16 starts at the décollement at
120 m b.s.l. with a gentle-to-moderate inclination (210/38), and it becomes
nearly vertical to the top of the cliff (210/79 and 210/80 following Steinich,
1972). The thrust plane is interpreted to have a slight listric shape.</p>
      <p id="d1e213">The thrust sheet S15 is characterised by an open folded geometry both in the
footwall-ramp panel and in the hanging-wall anticline (Figs. 1 and
2b). The beds of the southern anticline limb dip towards the SSW by
30<inline-formula><mml:math id="M6" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> on average (210/30). Thus, they are more gently inclined than
the beds in S16 (205/45). However, the thrust fault between S14 and S15 is
much steeper between 0 and 51 m a.s.l. than the frontal thrust below S16,
and therefore it truncates the Pleistocene beds at a higher level than in
S16 (Fig. 2). Thus, the Pleistocene unit does not reach the beach
level. The thrust fault between S15 and S16 is steeply inclined to the SSW
(205/65), and<?pagebreak page21?> at a hinge point ca. 15 m above the cliff base it turns into a
moderately inclined thrust fault (205/38). In fact, this part represents an
upper flat, since it is parallel to the bedding in the S16 thrust sheet
below. The inclinations from the best-fit model correspond well to the
orientation 205/35 given by Steinich (1972).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2" specific-use="star"><?xmltex \currentcnt{2}?><label>Figure 2</label><caption><p id="d1e227">Detailed 2-D cross sections of the two youngest thrust sheets. <bold>(a)</bold> S16 with a horizontal length of 175 m at the cliff base but 294 m from its
SSW to its NNE end. The thickness of the Cretaceous unit (flint bands F01 to
F54) is 98 to 89 m, while the Pleistocene unit (M1, I1, and M2) is 24 m
thick. <bold>(b)</bold> S15 with a horizontal length of 138 m at the cliff base and a
total length of 427 m (max 477 m). The maximum thickness of the beds down to
F01 is 128 m. The Pleistocene unit (M1 and I1) is ca. 21 to 12 m, while the
chalk unit (F01 to F54) is at least 107 m. The coloured lines represent the
flint bands of the chalk as well as horizons of the Pleistocene beds; the
red lines are faults. The cross sections constructed by Steinich (1972) are
shown in the background of each model.</p></caption>
          <?xmltex \igopts{width=483.69685pt}?><graphic xlink:href="https://deuquasp.copernicus.org/articles/2/19/2019/deuquasp-2-19-2019-f02.png"/>

        </fig>

</sec>
<sec id="Ch1.S2.SS2">
  <label>2.2</label><title>Duplex stack S14–S13–S12 (KU3d1, KU3d2, KU3d3)</title>
      <p id="d1e250">S14 is a long sheet with an open hanging-wall anticline (Figs. 1 and
3a). It is the lowermost element of the central duplex stack in the Kieler
Ufer section and shows an S-type duplex segment (see inset in Fig. 3a). The flint bands gently dip towards the SSW (220/19), but the inclination
increases towards the anticline core in the SSW (220/60). The thrust faults
bounding S14 in the SSW and NNE are relatively steep in the cliff section,
but they are more gently inclined below the cliff bottom, regarding the
best-fit model. The frontal ramp starts at the décollement with an
initially gentle inclination towards the SSW (210/21). At the hinge point at 37 m b.s.l. the inclination steepens (210/61). At another hinge point 53 m a.s.l., the thrust fault again turns into a gently inclined fault (210/24).</p>
      <p id="d1e253">S13 is the very small central element of the duplex stack (Fig. 3b). It is also an S-type element. The bedding shows a gentle-to-moderate
inclination (Fig. 3b). The upper flint bands of the chalk unit and
the Pleistocene beds were dragged along the footwall ramp of S12 so that
they form a slight footwall syncline in the trailing edge. The base of the
thrust sheet is not the décollement or another flat. It is a gently
inclined footwall ramp (220/12), which grows steeper at ca. 53 m b.s.l.
(220/53). At 21 m a.s.l. the ramp may pass into the upper flat.</p>
      <p id="d1e256">S12 is the upper segment of the duplex stack, also indicating an S-type
element (Fig. 3c). The bedding of S12 shows a gentle inclination
(225/07) until it exhibits a kink-like geometry at about section metre 360
(Fig. 3c). Northeast of this area the inclination is 225/53.
Northeast of the satellite fault, the flint bands of the hanging-wall
anticline show a succession of two smaller anticlines and a syncline in
between, which may point to a thrust-fault geometry exhibiting a double ramp
between section metre 445 and 500 rather than the simplified fault shown in
Fig. 3c. S12 does not reach the décollement surface at 120 m b.s.l., but it reaches the intermediate flat at ca. 92 m b.s.l. At section metre
323 it turns into the actual footwall ramp of S13, which is gently inclined
towards the SSW. The footwall ramp of S12 starts at section metre 349. It has a
moderate inclination towards the S (190/45).</p>

      <?xmltex \floatpos{p}?><fig id="Ch1.F3" specific-use="star"><?xmltex \currentcnt{3}?><label>Figure 3</label><caption><p id="d1e262">Detailed 2-D cross sections of the three duplex-stack elements. The
schematic illustration of a duplex stack including the three different
elements (L-, S-, and G-type) is given in <bold>(a)</bold> (modified following Pedersen, 2005). <bold>(a)</bold> S14 with a horizontal length of 178 m at the beach level but an entire
horizontal length from the SSW end to the NNE end of ca. 820 m. The
Cretaceous beds (F01 to F54) are 89 m thick at maximum. The thickness of the
Pleistocene unit (M1, I1, and M2) is 22 m. <bold>(b)</bold> S13; the horizontal length is
131 m at the cliff base but 315 m from its SSW end to its NNE end. The
chalk unit (F01 to F54) has a maximum thickness of 94 m. The Pleistocene
deposits (M1, I1, and M2) are up to 14 m. <bold>(c)</bold> S12 with a horizontal length of
184 m at the cliff base. The entire horizontal length is 506 m. The entire
bed thickness in the thrust sheet is 106 m from the F01 flint band to the
topmost bed in the Pleistocene sequence. However, the bed thickness from the
thrust-sheet base to the top is 131 m. The Cretaceous unit has a thickness
of 81 m (F01 to F54/chalk top) but a of maximum 106 m. The Pleistocene sequence
is ca. 25 m. The coloured lines represent the flint bands of the chalk as
well as horizons of the Pleistocene beds; the red lines are faults. A
detailed legend for the horizons and faults can be found in Fig. 2. The
cross sections constructed by Steinich (1972) are shown in the background
of each model.</p></caption>
          <?xmltex \igopts{width=421.100787pt}?><graphic xlink:href="https://deuquasp.copernicus.org/articles/2/19/2019/deuquasp-2-19-2019-f03.jpg"/>

        </fig>

</sec>
<sec id="Ch1.S2.SS3">
  <label>2.3</label><title>The oldest thrust sheet S11 (KU4)</title>
      <p id="d1e292">The southernmost and oldest thrust sheet of the Kieler Ufer section is S11,
which is an individual thrust sheet SSW of the<?pagebreak page22?> duplex stack (Fig. 1). Due to
the step-like geometry of the thrust fault between S11 and S12, the bedding
also shows a kinking geometry (Fig. 4). In the SSW of S11, the beds
are moderately inclined to the SSW (205/45), while the central beds are gently
inclined (205/18). Farther north, the inclination gets steeper again to form
the southern limb of the hanging-wall anticline. The hanging-wall anticline
is characterised by two smaller anticlines comparable to the frontal edge of
S12. This is a hint to a double-ramp configuration of the frontal thrust
fault (Fig. 4). Below this structure, the ramp steeply dips to the SW
(225/61). At a hinge point 57 m b.s.l. the ramp is only gently inclined
(225/13). In its lowermost part, it forms the moderately inclined ramp
between the décollement surface and the intermediate flat, on which S12
and S13 were translated.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4" specific-use="star"><?xmltex \currentcnt{4}?><label>Figure 4</label><caption><p id="d1e297">Detailed 2-D cross section of the oldest thrust sheet S11 in the
Kieler Ufer section. The horizontal length is about 162 m. The entire thrust
sheet has a horizontal length of 478 m from the southernmost to the
northernmost end. The chalk deposits (F01 to F54) are about 100 m thick; the
Pleistocene unit (M1 and I1) is at least 16 m. The coloured lines represent
the flint bands of the chalk as well as horizons of the Pleistocene beds;
the red lines are faults. A detailed legend for the horizons and faults can
be found in Fig. 2. The cross sections constructed by Steinich (1972) are
shown in the background of each model.</p></caption>
          <?xmltex \igopts{width=483.69685pt}?><graphic xlink:href="https://deuquasp.copernicus.org/articles/2/19/2019/deuquasp-2-19-2019-f04.png"/>

        </fig>

</sec>
</sec>
<sec id="Ch1.S3">
  <label>3</label><title>The restored cross section: key to understanding Jasmund's glacitectonic
evolution and kinematics</title>
      <?pagebreak page24?><p id="d1e315">The kinematic analysis of the Kieler Ufer section led to strain
quantification and the illustration of stress orientation. It includes
strain partitioning and, hence, the separation of the shortening amount into
folding and faulting. Cross-section restoration and balancing of the
imbricate fans of the southern structural sub-complex revealed that the
Kieler Ufer section had an initial length of at least 2482 m before its
glacitectonic imbrication. Thus, the entire horizontal shortening of the
Kieler Ufer section is 1280 m (51.6 %) at its minimum. This includes both
folding and the translation along the flats and ramps. The process of
folding constitutes only 20.5 % (263 m) of the entire deformation, while
the translation part is even 79.5 % (1017 m). The amount of displacement
along the individual thrust faults is 206 m (KU1), 164 m (KU2), 328 m
(KU3d1), 521 m (KU3d2), 438 m (KU3d3), and 243 m (KU4). The stress was
directed from the SSW to NNE. The orientation fits well into the glacio-dynamic
model suggested by Gehrmann and Harding (2018). The glacier with a
piedmont-type lobe mainly moved from the SE to NW in the second evolutionary
stage and induced local stress in all sides due to the radial propagation in
the unconfined ice-marginal zone (see e.g. Ó Cofaigh et al., 2003;
Jónsson et al., 2014). This induced a local orientation change of the
thrust faults from a dip to the SE in the inland zone of the southern
sub-complex to the S/SW at the eastern cliff.</p>
      <p id="d1e318">The final cross section of the Kieler Ufer section cannot be completely
balanced. There are smaller restoration gaps in the northern parts of the
restored sheets KU1, KU2, and KU3d1 (S16, S15, S14) (Fig. 5). A
large gap can be seen in the northern end of KU3d2 (S13). Projection of the
cliff sections has been considered in the modelling process to reduce such
errors. The azimuth of the final large track of the Kieler Ufer section is
210<inline-formula><mml:math id="M7" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>, adapted from the main orientation of the thrust faults or
individually of the flint bands. The projection has been performed normal to
the sections. However, the gaps represent volume loss during deformation
rather than construction errors. Tectonic erosion may have occurred at the
ramps, when the single sheets were thrust up, leading to small gaps in the
frontal edge of the thrust sheets in the restored cross section. In
addition, it has to be taken into account that the restored cross section
only shows a 2-D interpretation. In particular, the large restoration gap in
KU3d2 (S13) may point to a very complicated bedding and deformation history
in the area of the Kieler Ufer section, which is highly likely related to
interference between the northern and southern structural sub-complex. The
specific complexity is confirmed by the high amount of shortening (51.6 %) and the duplex stack in the centre of the Kieler Ufer section.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F5" specific-use="star"><?xmltex \currentcnt{5}?><label>Figure 5</label><caption><p id="d1e332">Interpretation and restoration of the Kieler Ufer section (S11 to
S16) with horizontal-shortening results. <bold>(a)</bold> Cross section interpreted above
and below the cliff boundaries (simplified). <bold>(b)</bold> Restored cross section
indicating the configuration before the glacitectonic deformation of the
southern structural sub-complex. The restored thrust sheets are additionally
labelled with the new abbreviations KU1 to KU4, which represent the
chronology of the restoration process.</p></caption>
        <?xmltex \igopts{width=483.69685pt}?><graphic xlink:href="https://deuquasp.copernicus.org/articles/2/19/2019/deuquasp-2-19-2019-f05.png"/>

      </fig>

</sec>
<sec id="Ch1.S4" sec-type="conclusions">
  <label>4</label><title>The southern sub-complex of Jasmund in the context of glacitectonic-complex
models</title>
      <p id="d1e355">The Kieler Ufer section represents a structural key location in the
thrust-dominated-to-fold–thrust-dominated glacitectonic complex of Jasmund
(see Boulton et al., 1999). The specific geometric features of the
constructed and restored cross section led to major information on the
kinematics and deformation history, including the relationship between the
northern and southern structural sub-complex of Jasmund.</p>
      <p id="d1e358">The southern sub-complex exhibits a realistic décollement depth at
mainly 120 m b.s.l., because the deformation in ancient glacitectonic
complexes can extend to a depth of a few tens of metres up to 200 m (e.g.
Aber et al., 1989; van der Wateren, 2003; Huuse and Lykke-Andersen, 2000;
Vaughan-Hirsch and Phillips, 2017). Modern structurally<?pagebreak page25?> similar
glacitectonic landforms are generally smaller, with décollement depths of
about 5 to 30 m (e.g. Boulton et al., 1999; Benediktsson et al., 2010).</p>
      <p id="d1e361">Considering the classic separation of glacitectonic complexes into a
proximal, central, and distal zone (e.g. Boulton et al., 1999; Pedersen,
2000), the Kieler Ufer section is part of the central zone, which is
characterised by a highly complicated structural framework of duplex stacks
and steeply dipping thrust faults implying a high-strain area with intensive
thrusting and shortening. The Kieler Ufer section has the highest amount of
horizontal shortening (51.6 %) compared to the other sections of the
southern sub-complex. The highest elevations of the modelled southern
structural sub-complex are at the hanging-wall anticlines of the central
zone (e.g. S14: 166 m a.s.l.), which may confirm the intensive deformation
and compression. Boulton et al. (1999) also described the more intensive
folding and thrusting for the centre of the modern glacitectonic complex in
front of Holmstrømbreen on Svalbard.</p>
      <p id="d1e364">There are also substantial differences between Jasmund and previously
described glacitectonic complexes when the entire southern sub-complex is
considered. While most glacitectonic complexes indicate a significant strain
decrease from the proximal to the distal end, the Jasmund Glacitectonic
Complex is characterised by a constantly high strain. Normally, the length
of the thrust sheets increases towards the foreland, which implies a greater
degree of shortening towards the proposed ice margin (e.g. Pedersen, 2005;
Vaughan-Hirsch and Phillips, 2017). However, such a
trend cannot be seen in the southern sub-complex of Jasmund. Typically, the angle of the
thrust faults and the offsets decrease towards the foreland (Dixon and Liu,
1992; Pedersen, 2005; Vaughan-Hirsch and Phillips, 2017). This is also not
the case in the Jasmund Glacitectonic Complex. Even though the steepest
thrust sheets are situated in the most proximal zone, there are still
steeply to moderately inclined faults in the central and distal zone. This
phenomenon can be explained with the complex relationship between the
northern and southern structural sub-complex of Jasmund. Since the northern
sub-complex was formed first by an earlier glacitectonically effective
glacier in the SW Baltic Sea region, there already existed the structural
framework of a glacitectonic complex in the north of the southern structural
sub-complex. Thus, an obstacle in front of the deformation area has
controlled the imbrication during the second stage (see Gehrmann and
Harding, 2018). These circumstances intensively affected the deformation
process of the southern sub-complex as well as its internal structure. There
was no possibility to form gently inclined thrust faults in the distal
foreland during the final deformation, as the northern sub-complex acted as
a resistance. The stress induced by both the glacier and the northern
sub-complex led to the documented highly complex architecture, which
represents an exception from classic glacitectonic-complex models
(unconfined). The structural configuration of Jasmund can be used as a model
characteristic of confined glacitectonic complexes. It is all the more so an
example of<?pagebreak page26?> various and intensive superimpositions in a multi-stage structural
evolution (see Pedersen, 2000).</p>
</sec>

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

      <p id="d1e372">The data are publicly available via the thesis
Gehrmann (2018) and the references therein online at
<uri>https://nbn-resolving.org/urn:nbn:de:gbv:9-opus-24751</uri> (last access: 22 July 2019).</p>
  </notes><notes notes-type="authorcontribution"><title>Author contributions</title>

      <p id="d1e381">AG designed the methodology, performed the
analysis, and prepared the manuscript with contributions from all
co-authors.</p>
  </notes><notes notes-type="competinginterests"><title>Competing interests</title>

      <p id="d1e387">The authors declare that they have no conflict of interest.</p>
  </notes><ack><title>Acknowledgements</title><p id="d1e393">We acknowledge granting of software licences
(Move<sup>™</sup> suite) from Midland Valley Exploration Ltd for the years 2014 to 2018. Ralf-Otto Niedermeyer is thanked for his constructive review. We acknowledge support for the article processing charge from the DFG (no. 393148499) and the Open Access Publication Fund of the University of Greifswald.</p></ack><notes notes-type="financialsupport"><title>Financial support</title>

      <p id="d1e401">This research has been supported by the DFG (German Research Foundation, grant no. 393148499) and the Open Access Publication Fund of the University of Greifswald.</p>
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    <!--<article-title-html>Sea cliff at Kieler Ufer (Pleistocene stripes 11–16) – large-scale architecture and kinematics of the Jasmund Glacitectonic Complex</article-title-html>
<abstract-html><p>The Kieler Ufer cliff section is a structural key
location in the late Weichselian thrust-dominated-to-fold–thrust-dominated
glacitectonic complex of Jasmund. Restoration and balancing of geological
cross sections from the eastern coast (southern sub-complex) enabled strain
quantification and the illustration of stress orientation. The entire
horizontal shortening of the Kieler Ufer section is 1280&thinsp;m (51.6&thinsp;%) at its
minimum. The thrust faults generally inclined towards south indicate a local
glacier push from the S/SSW, which fits well into the glacio-dynamic model
suggested by Gehrmann and Harding (2018).</p></abstract-html>
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Iceland: a re-assessment of a classic glaciotectonic locality, Quaternary
Sci. Rev., 29, 484–506, <a href="https://doi.org/10.1016/j.quascirev.2009.10.004" target="_blank">https://doi.org/10.1016/j.quascirev.2009.10.004</a>, 2010.
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complex: Holmstrømbreen, Spitsbergen, Quaternary Sci. Rev., 18,
339–371, 1999.
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Croot, D. G.: Glacio-tectonic structures: a mesoscale model of thin-skinned
thrust sheets?, J. Struct. Geol., 9, 797–808, 1987.
</mixed-citation></ref-html>
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faults, in: Thrust Tectonics, edited by: McClay, K. R., Chapman &amp; Hall,
London, 53–70, 1992.
</mixed-citation></ref-html>
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Greifswald, Germany, 2018.
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<a href="https://doi.org/10.3390/geosciences8060208" target="_blank">https://doi.org/10.3390/geosciences8060208</a>, 2018.
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