<?xml version="1.0" encoding="UTF-8"?>
<!DOCTYPE article PUBLIC "-//NLM//DTD Journal Publishing with OASIS Tables v3.0 20080202//EN" "journalpub-oasis3.dtd">
<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{Express report}?>
  <front>
    <journal-meta><journal-id journal-id-type="publisher">EGQSJ</journal-id><journal-title-group>
    <journal-title>E&amp;G Quaternary Science Journal</journal-title>
    <abbrev-journal-title abbrev-type="publisher">EGQSJ</abbrev-journal-title><abbrev-journal-title abbrev-type="nlm-ta">E&amp;G Quaternary Sci. J.</abbrev-journal-title>
  </journal-title-group><issn pub-type="epub">2199-9090</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/egqsj-67-17-2018</article-id><title-group><article-title>Reconsidering the origin of the Sedrun fans<?xmltex \hack{\break}?> (Graubünden, Switzerland)</article-title><alt-title>Reconsidering the origin of the Sedrun fans</alt-title>
      </title-group><?xmltex \runningtitle{Reconsidering the origin of the Sedrun fans}?><?xmltex \runningauthor{C. Dieleman et al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Dieleman</surname><given-names>Catharina</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="yes" rid="aff2">
          <name><surname>Ivy-Ochs</surname><given-names>Susan</given-names></name>
          <email>ivy@phys.ethz.ch</email>
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Hippe</surname><given-names>Kristina</given-names></name>
          
        <ext-link>https://orcid.org/0000-0003-0946-9772</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Kronig</surname><given-names>Olivia</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3">
          <name><surname>Kober</surname><given-names>Florian</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Christl</surname><given-names>Marcus</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-3131-6652</ext-link></contrib>
        <aff id="aff1"><label>1</label><institution>Institute of Geology, ETH Zurich, 8093 Zurich, Switzerland</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>Laboratory of Ion Beam Physics, ETH Zurich, 8092 Zurich, Switzerland</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>NAGRA, Hardstrasse 73, 5430 Wettingen, Switzerland</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Susan Ivy-Ochs (ivy@phys.ethz.ch)</corresp></author-notes><pub-date><day>20</day><month>April</month><year>2018</year></pub-date>
      
      <volume>67</volume>
      <issue>1</issue>
      <fpage>17</fpage><lpage>23</lpage>
      
      <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://egqsj.copernicus.org/articles/67/17/2018/egqsj-67-17-2018.html">This article is available from https://egqsj.copernicus.org/articles/67/17/2018/egqsj-67-17-2018.html</self-uri><self-uri xlink:href="https://egqsj.copernicus.org/articles/67/17/2018/egqsj-67-17-2018.pdf">The full text article is available as a PDF file from https://egqsj.copernicus.org/articles/67/17/2018/egqsj-67-17-2018.pdf</self-uri>
      <custom-meta-group><custom-meta><meta-name>citationstatement</meta-name><meta-value>Dieleman, C., Ivy-Ochs, S., Hippe, K., Kronig, O., Kober, F., and Christl, M.: Reconsidering the origin of the Sedrun fans (Graubünden, Switzerland), E&amp;G Quaternary Sci. J., 67, 17–23, https://doi.org/10.5194/egqsj-67-17-2018, 2018.</meta-value></custom-meta></custom-meta-group>
    </article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <title>Introduction</title>
      <p id="d1e137">Four alluvial fans, Pulanera, L'Ondadusa, Drun and Bugnei, located near the
town of Sedrun in the upper Vorderrhein Valley (Fig. 1), are striking in that
they have a common aggradation surface (<inline-formula><mml:math id="M1" display="inline"><mml:mo lspace="0mm">∼</mml:mo></mml:math></inline-formula> 1<inline-formula><mml:math id="M2" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> slope oriented
along the main valley axis) and distinct coterminous cut-off toes. Similar
coalesced fans with marked incised toes occur just downstream at Disentis
(Fig. 2a). These geomorphological characteristics suggest that the fans built
up for a limited period of time and then were abruptly incised by the
Vorderrhein River. Switching between aggradation, fan abandonment and channel
entrenchment can be a response to (1) variation in discharge due to climate
changes or extreme precipitation events, (2) decreases in sediment supply
reflecting waning (e.g. paraglacial) sediment availability, (3) tectonic
uplift, or (4) changes in base level (Harvey et al., 2005; Hornung et al.,
2010, and references therein). Inside a mountain range, change in local base
level can be caused by large-scale downstream blockage by a glacier, a
landslide or a man-made dam (Korup and Tweed, 2007).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1" specific-use="star"><caption><p id="d1e158">Panorama photograph (looking E) showing the coalesced-fan surface
and the distinct cut-off toes of the fans in the upper Vorderrhein area near
Sedrun. Fans and associated catchments are labelled P, Pulanera;
O, L'Ondadusa; D, Drun; and B, Bugnei.</p></caption>
        <?xmltex \igopts{width=398.338583pt}?><graphic xlink:href="https://egqsj.copernicus.org/articles/67/17/2018/egqsj-67-17-2018-f01.jpg"/>

      </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2" specific-use="star"><caption><p id="d1e169"><bold>(a)</bold> Slope map based on 2 <inline-formula><mml:math id="M3" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.5 m resolution DEM
(swissAlti3D, swisstopo JA100120) of the oversize fans near Sedrun and
Disentis. Catchments (encircled with dashed line) connected to the Sedrun
fans are labelled P, Pulanera; O, L'Ondadusa; D, Drun; and B, Bugnei. The
14 March 2016 debris avalanche release and deposit area are shown. Squares
indicate locations of Fig. 2b and c. <bold>(b)</bold> Close-up of the moraines in
Val Giuv with <inline-formula><mml:math id="M4" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">10</mml:mn></mml:msup></mml:math></inline-formula>Be-dated boulder locations (dates shown in Fig. 4).
<bold>(c)</bold> Close-up of the aspect map of the upper Drun fan. Note
morphology of debris-flow levees on
upper fan surface; arrow points to left-lateral moraines of the Val Strem
paleoglacier that are partly buried by the upper Drun fan sediment.</p></caption>
        <?xmltex \igopts{width=384.112205pt}?><graphic xlink:href="https://egqsj.copernicus.org/articles/67/17/2018/egqsj-67-17-2018-f02.jpg"/>

      </fig>

      <p id="d1e203">Previous work in the study area was focused on the bedrock (Huber, 1948),
especially for characterization of the NEAT Gotthard basis tunnel site below
Sedrun (Schneider, 1992, and references therein). In the northern tributary
valleys (Val Giuv, Val Mila, Val Strem; Fig. 2a) Aar granite dominates,
while strongly sheared metamorphic rocks of the Tavetscher Zwischenmassif
underlie the Vorderrhein Valley itself. Along the trough shoulder,
especially at Cuolm da Vi (Fig. 2a), active deep-seated slope degradation is
present as evidenced by abundant trenches and uphill facing scarps (Amann et
al., 2006).</p>
      <p id="d1e206">The aim of this study is to determine what caused this abrupt and apparently
brief period of fan aggradation in the upper Vorderrhein. Previous
researchers have interpreted the Sedrun and Disentis fans as kame terraces
(Scapozza, 2012) or as Lateglacial outwash fans (Hantke,
1983). For the latter to be true the valley fill at Sedrun would have to be
dominated by tributary valley sediment rather than Vorderrhein fluvial
sediments. Both of these hypotheses require that the fans formed between
about 17 and 11.7 kyr ago.</p>
</sec>
<sec id="Ch1.S2">
  <title>Methods</title>
      <p id="d1e215">To decipher the evolution of the upper Vorderrhein region and the origin of
the Sedrun fans, we did detailed geomorphologic mapping supported by ArcGIS
landscape analysis, as well as cosmogenic <inline-formula><mml:math id="M5" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">10</mml:mn></mml:msup></mml:math></inline-formula>Be exposure dating of
boulders on moraines at the mouths of the three tributary valleys. No
boulders suitable for exposure dating were found on any of the fan surfaces.
Debris-flow sediments of the fans bury several of these moraines; thus the
moraine dates<?pagebreak page18?> provide maximum ages for aggradation of the fans. Sampling,
sample preparation and age calculations for <inline-formula><mml:math id="M6" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">10</mml:mn></mml:msup></mml:math></inline-formula>Be exposure dating
followed established procedures (Ivy-Ochs and Kober, 2008). Based on the
mapped lateral and frontal moraines, paleoglaciers were reconstructed and
the associated equilibrium line altitudes (ELAs) were calculated using the
ArcGIS GlaRe tool (Pellitero et al., 2015, 2016). Knowledge of the ELA
depression with respect to the Little Ice Age ELA is another means of
estimating the timing of the glacier advance and associated moraine
construction. We reconstructed the sedimentary fill of the upper Vorderrhein
Valley based on our own outcrop descriptions combined with the information
gleaned from the published NEAT core logs (Schneider, 1992).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3" specific-use="star"><caption><p id="d1e238"><bold>(a)</bold> Sediment of the upper Drun fan exposed in the Drun
stream incision just south of Valtgeva (location shown in Fig. 2a). The
outcrop is dominated by debris-flow deposits made up of crudely bedded,
angular to subangular gneiss and schist cobbles and boulders (in part
imbricated) in a silty, sandy matrix. Close to the top of the section,
<inline-formula><mml:math id="M7" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 0.75 m of interbedded laminated sands is visible, which is in turn
overlain by another block layer. <bold>(b)</bold> View up into Val Giuv along the
dated inner left-lateral moraine. Boulder Giuv1 is in the right foreground
(age 10 880 <inline-formula><mml:math id="M8" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 430 years).</p></caption>
        <?xmltex \igopts{width=355.659449pt}?><graphic xlink:href="https://egqsj.copernicus.org/articles/67/17/2018/egqsj-67-17-2018-f03.jpg"/>

      </fig>

</sec>
<?pagebreak page19?><sec id="Ch1.S3">
  <title>Geomorphology of the upper Vorderrhein Valley</title>
<sec id="Ch1.S3.SS1">
  <title>Fan morphology and valley fill</title>
      <p id="d1e277">The four fans studied here have a common, coalesced aggradation surface
(<inline-formula><mml:math id="M9" display="inline"><mml:mo lspace="0mm">∼</mml:mo></mml:math></inline-formula> 1380 m a.s.l.) that once must have extended all the way
across the valley to the southern slope. Although the Pulanera fan is
located at the mouth of Val Mila, the fan emanates from the small
erosional-collapse catchment named Val Pulanera (Fig. 2a). At the toe of the
Pulanera fan, incision by the Vorderrhein created a sequence of nine
terraces. Riser height of the oldest terrace is 20 m. The most recent
terrace is 1 m above today's active channel. Just to the west at Val
Giuv numerous lateral and frontal moraines mark past glacier positions (Fig. 2b), but there is very little outwash downstream of the moraines and no fan,
and the Giuv stream enters a bedrock canyon before joining the Vorderrhein.
The lower part of the canyon is filled with and draped by sediment of the
neighbouring Pulanera fan. The L'Ondadusa fan is built up of material from
the small catchment L'Ondadusa, which lies between Val Mila and Val Strem.
Both the Pulanera and L'Ondadusa fans are largely inactive with little
material being delivered to the fan today. Only tiny streams, which lack
incised channels, traverse the two fans. The erosion escarpment along the
Vorderrhein is about 50 m at L'Ondadusa and 70 m at the toe of the Drun fan.
The Strem torrent, which separates the L'Ondadusa and Drun fans (Fig. 2a),
has incised about 30 m into the topographically contiguous fan surface.</p>
      <p id="d1e287">The Drun fan, which lies at the mouth of Val Strem, consists of a lower main
fan and an upper fan to the northeast. Surface morphology shows that the fan
itself does not emanate from Val Strem, but instead the upper fan sediment is
sourced in the Drun catchment (Fig. 2c). The fan is a ski area and both the
lower and upper fans were cleaned of large boulders. The upper Drun fan bears
scattered boulders (&lt; 0.5 m in height) and faint levees of
abandoned channels. Outcrops of the upper fan deposit along the incised Drun
channel (<inline-formula><mml:math id="M10" display="inline"><mml:mo lspace="0mm">∼</mml:mo></mml:math></inline-formula> 35 m) near Valtgeva reveal several-metre-thick,
matrix-supported block layers with infrequent interbedded laminated sands
(Fig. 3a). The former are dominated by angular to
subangular schist and gneiss blocks
in a matrix of silty sand. The Drun catchment lies at the foot of the Cuolm
da Vi, the site of active gravitational collapse and toppling with reported
movement rates of some tens of centimetres per year (Amann et al., 2006). Several-metre-thick debris-flow
deposits within the channel itself attest to recent deposition by the Drun
torrent. Left lateral moraines present in Val Strem at Valtgeva are partially
buried by the debris-flow sediments
of the upper Drun fan (Fig. 2c). The most upvalley moraine was buried in part
by the 14 March 2016 Val Strem debris avalanche (Fig. 2a). During this event
the western flank of Cuolm da Vi collapsed and <inline-formula><mml:math id="M11" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 200 000 m<inline-formula><mml:math id="M12" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:math></inline-formula> of
rock debris mixed with snow detached and ran up tens of metres on the
opposite valley slope to eventually form a <inline-formula><mml:math id="M13" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 1 km debris tongue
(<ext-link xlink:href="https://www.nzz.ch/panorama/ungluecksfaelle-und-verbrechen/felssturz-in-sedrun-geroell-verschuettet-wasser-und-stromversorgung-1.18712845">https://www.nzz.ch/panorama/ungluecksfaelle-und-verbrechen/felssturz-in-sedrun-geroell-verschuettet-wasser–und-stromversorgung-1.18712845</ext-link>,
last access: 17 January 2018).</p>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T1" specific-use="star"><caption><p id="d1e326">Sample information, measured <inline-formula><mml:math id="M14" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">10</mml:mn></mml:msup></mml:math></inline-formula>Be concentrations and calculated
surface exposure ages; all errors are 1<inline-formula><mml:math id="M15" display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula>.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="8">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="right"/>
     <oasis:colspec colnum="3" colname="col3" align="right"/>
     <oasis:colspec colnum="4" colname="col4" align="right"/>
     <oasis:colspec colnum="5" colname="col5" align="right"/>
     <oasis:colspec colnum="6" colname="col6" align="right"/>
     <oasis:colspec colnum="7" colname="col7" align="right"/>
     <oasis:colspec colnum="8" colname="col8" align="right"/>
     <oasis:thead>
       <oasis:row>
         <oasis:entry colname="col1">Sample</oasis:entry>
         <oasis:entry colname="col2">Latitude</oasis:entry>
         <oasis:entry colname="col3">Longitude</oasis:entry>
         <oasis:entry colname="col4">Elevation</oasis:entry>
         <oasis:entry colname="col5">Sample</oasis:entry>
         <oasis:entry colname="col6">Topographic</oasis:entry>
         <oasis:entry colname="col7"><inline-formula><mml:math id="M22" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">10</mml:mn></mml:msup></mml:math></inline-formula>Be concentration</oasis:entry>
         <oasis:entry colname="col8">Exposure</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">ID</oasis:entry>
         <oasis:entry colname="col2"/>
         <oasis:entry colname="col3"/>
         <oasis:entry colname="col4">(m a.s.l.)</oasis:entry>
         <oasis:entry colname="col5">thickness (cm)</oasis:entry>
         <oasis:entry colname="col6">shielding factor</oasis:entry>
         <oasis:entry colname="col7">(10<inline-formula><mml:math id="M23" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msup></mml:math></inline-formula> at g<inline-formula><mml:math id="M24" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>)<inline-formula><mml:math id="M25" display="inline"><mml:msup><mml:mi/><mml:mi mathvariant="normal">a</mml:mi></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col8">age<inline-formula><mml:math id="M26" display="inline"><mml:msup><mml:mi/><mml:mi mathvariant="normal">b</mml:mi></mml:msup></mml:math></inline-formula></oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>
         <oasis:entry colname="col1">Mila1</oasis:entry>
         <oasis:entry colname="col2">46.6835</oasis:entry>
         <oasis:entry colname="col3">8.7412</oasis:entry>
         <oasis:entry colname="col4">1672</oasis:entry>
         <oasis:entry colname="col5">2.0</oasis:entry>
         <oasis:entry colname="col6">0.966</oasis:entry>
         <oasis:entry colname="col7">15.36 <inline-formula><mml:math id="M27" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.67</oasis:entry>
         <oasis:entry colname="col8">10 120 <inline-formula><mml:math id="M28" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 440</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Mila2</oasis:entry>
         <oasis:entry colname="col2">46.6782</oasis:entry>
         <oasis:entry colname="col3">8.7472</oasis:entry>
         <oasis:entry colname="col4">1532</oasis:entry>
         <oasis:entry colname="col5">2.3</oasis:entry>
         <oasis:entry colname="col6">0.985</oasis:entry>
         <oasis:entry colname="col7">18.64 <inline-formula><mml:math id="M29" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.93</oasis:entry>
         <oasis:entry colname="col8">13 430 <inline-formula><mml:math id="M30" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 670</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">Mila3</oasis:entry>
         <oasis:entry colname="col2">46.6790</oasis:entry>
         <oasis:entry colname="col3">8.7509</oasis:entry>
         <oasis:entry colname="col4">1512</oasis:entry>
         <oasis:entry colname="col5">2.4</oasis:entry>
         <oasis:entry colname="col6">0.987</oasis:entry>
         <oasis:entry colname="col7">18.62 <inline-formula><mml:math id="M31" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.79</oasis:entry>
         <oasis:entry colname="col8">13 600 <inline-formula><mml:math id="M32" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 580</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Giuv1</oasis:entry>
         <oasis:entry colname="col2">46.6741</oasis:entry>
         <oasis:entry colname="col3">8.7209</oasis:entry>
         <oasis:entry colname="col4">1841</oasis:entry>
         <oasis:entry colname="col5">4.0</oasis:entry>
         <oasis:entry colname="col6">0.979</oasis:entry>
         <oasis:entry colname="col7">18.64 <inline-formula><mml:math id="M33" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.73</oasis:entry>
         <oasis:entry colname="col8">10 880 <inline-formula><mml:math id="M34" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 430</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Giuv2</oasis:entry>
         <oasis:entry colname="col2">46.6738</oasis:entry>
         <oasis:entry colname="col3">8.7213</oasis:entry>
         <oasis:entry colname="col4">1831</oasis:entry>
         <oasis:entry colname="col5">3.5</oasis:entry>
         <oasis:entry colname="col6">0.980</oasis:entry>
         <oasis:entry colname="col7">33.45 <inline-formula><mml:math id="M35" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 1.43</oasis:entry>
         <oasis:entry colname="col8">19 610 <inline-formula><mml:math id="M36" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 840</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Giuv3</oasis:entry>
         <oasis:entry colname="col2">46.6734</oasis:entry>
         <oasis:entry colname="col3">8.7227</oasis:entry>
         <oasis:entry colname="col4">1795</oasis:entry>
         <oasis:entry colname="col5">2.5</oasis:entry>
         <oasis:entry colname="col6">0.982</oasis:entry>
         <oasis:entry colname="col7">20.31 <inline-formula><mml:math id="M37" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.76</oasis:entry>
         <oasis:entry colname="col8">12 070 <inline-formula><mml:math id="M38" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 450</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table><table-wrap-foot><p id="d1e345"><inline-formula><mml:math id="M16" display="inline"><mml:msup><mml:mi/><mml:mi mathvariant="normal">a</mml:mi></mml:msup></mml:math></inline-formula> Analyses were normalized to the ETH AMS
(accelerator mass spectrometry) standard S2007N (Christl et al., 2013).
<inline-formula><mml:math id="M17" display="inline"><mml:msup><mml:mi/><mml:mi mathvariant="normal">b</mml:mi></mml:msup></mml:math></inline-formula> Calculated with the online calculator of Balco et al. (2008)
using the northeast North America calibration data set, a rock density of
2.65 g cm<inline-formula><mml:math id="M18" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>, and no erosion. Errors include the statistical
uncertainties of the AMS measurement and the error on the subtracted blank
(3.5 <inline-formula><mml:math id="M19" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 2.5 <inline-formula><mml:math id="M20" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<inline-formula><mml:math id="M21" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">15</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>).</p></table-wrap-foot></table-wrap>

      <p id="d1e783">Two of the NEAT cores (Schneider, 1992) were taken close to the middle of the
valley (locations shown in Fig. 2a). Examination of the published core log
data allowed us a glimpse into the valley fill beneath the L'Ondadusa and
Drun fans. Core SBA at 1342 m a.s.l. (2701381/1170326) lies in the
Vorderrhein channel, while core SBB at 1358 m a.s.l. (2701314/1170165) lies
in the Strem channel <inline-formula><mml:math id="M39" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 240 m north of the Vorderrhein. Both cores
traversed bedrock (Schneider, 1992), in SBA at 55 m depth (1288 m a.s.l.)
and in SBB at 89 m depth (1269 m a.s.l.). This reach of the Vorderrhein
Valley is overdeepened as shown by
the top bedrock surface at 1269 m a.s.l. (core SBB),
which is tens of metres lower than
the bedrock threshold in the canyon near Bugnei at 1340 m a.s.l. The first
5–10 m of sediment on top of bedrock was interpreted by Schneider (1992)<?pagebreak page20?> as
subglacial till (overconsolidated diamicton). This is overlain by
glaciofluvial gravels, rare interbedded glacigenic sediments (“tills”) and
lake sediments. The glaciofluvial deposits contain a broad spectrum of
lithologies attesting to both local and Vorderrhein contributions. Starting
at an elevation of about 1300 m a.s.l., Vorderrhein gravels with
well-rounded clasts begin to dominate both cores. Schneider (1992)
interpreted this as signalling the onset of the Holocene. No <inline-formula><mml:math id="M40" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:math></inline-formula>C dates
are reported for any of the NEAT cores in the valley. In core SBB, the
presence of clean, well-sorted and at times cross-bedded sands between
elevations of 1330 and 1340 m a.s.l. was interpreted to indicate the
presence of a lake (Schneider, 1992). Starting at elevation 1350 m a.s.l.
and continuing to the top of core SBB poorly sorted, locally sourced
debris-flow sediments with subangular gneiss blocks ranging up to 1 m<inline-formula><mml:math id="M41" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:math></inline-formula>
in diameter were logged. The elevation of the (abandoned) Drun fan surface
just adjacent to core SBB is at 1385–1390 m a.s.l., allowing
35–40 m of debris-flow sediments, which comprise the fan topography visible
today.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4" specific-use="star"><caption><p id="d1e814">Reconstructed paleoglaciers in the three tributary valleys. Pink
lines show the AAR ELAs calculated with the ArcGIS tool GlaRe (Pellitero et
al., 2015, 2016). Yellow dots indicate the locations of <inline-formula><mml:math id="M42" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">10</mml:mn></mml:msup></mml:math></inline-formula>Be-dated
boulders. The corresponding <inline-formula><mml:math id="M43" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">10</mml:mn></mml:msup></mml:math></inline-formula>Be ages and their uncertainties are given.
The coherence of the ELAs and <inline-formula><mml:math id="M44" display="inline"><mml:mi mathvariant="normal">Δ</mml:mi></mml:math></inline-formula>ELAs with respect to the Little Ice
Age ELAs (see text) in concert with the <inline-formula><mml:math id="M45" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">10</mml:mn></mml:msup></mml:math></inline-formula>Be ages suggest that these
glaciers advanced during the Alpine Lateglacial Egesen stadial.</p></caption>
          <?xmltex \igopts{width=355.659449pt}?><graphic xlink:href="https://egqsj.copernicus.org/articles/67/17/2018/egqsj-67-17-2018-f04.jpg"/>

        </fig>

      <p id="d1e857">Topographically, the abandoned Drun fan surface continues to the east to
coalesce with the Bugnei fan, where the Vorderrhein has incised more than 120 m at the fan toe. Fan outcrops along the northern canyon wall indicate the
presence of a pre-existing canyon that was filled by Bugnei debris. The
canyon is contiguous with the Cavorgia bedrock canyon that separates the
Sedrun fan surface from the Disentis fan surface (Fig. 2a). The rather
uniform 7<inline-formula><mml:math id="M46" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> radial angle of the Bugnei fan surface on both the west
and east side underscores the idea that during fan aggradation the (former)
Cavorgia canyon must have been already completely filled up.</p>
</sec>
<sec id="Ch1.S3.SS2">
  <title>Moraines and paleoglacier reconstruction</title>
      <p id="d1e875">Results of <inline-formula><mml:math id="M47" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">10</mml:mn></mml:msup></mml:math></inline-formula>Be exposure dating of moraine boulders are given in Table 1 and shown in Fig. 4. In Val Giuv, the prominent left-lateral moraine
(Fig. 2b) is an accretionary moraine with the outermost left-lateral moraine
(age 12 070 <inline-formula><mml:math id="M48" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 450 years, Giuv3) having been partially buried by the
larger more prominent inner left-lateral moraine (age 10 880 <inline-formula><mml:math id="M49" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 430 years,
Giuv1, Fig. 3b). The apparently too old age of Giuv2 19 610 <inline-formula><mml:math id="M50" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 840 years
(also on outermost moraine) reflects cosmogenic nuclide inheritance and is
not discussed further. Sub-parallel latero-frontal moraines at the mouth of
Val Mila indicate that, 13 430 <inline-formula><mml:math id="M51" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 670 years ago (Mila2), the local
glacier had just reached the main valley. The upvalley left-lateral moraine
records stabilization of the glacier at a recessional position 10 120 <inline-formula><mml:math id="M52" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 440 years ago (Mila1). From a boulder on the left flank of the
Vorderrhein Valley an age of 13 600 <inline-formula><mml:math id="M53" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 580 years (Mila3) was obtained.
This gives a minimum age for the timing of an ice-free main valley. Pollen
data indicate ice-free conditions around Sedrun by the beginning of the
Bølling interstadial (ca. 14.6 kyr ago; Burga, 1987).</p>
      <p id="d1e930">Comparison of the ELAs of the paleoglaciers
provides an independent means of assessing contemporaneity of moraine
formation in the three tributary valleys. Determined ELAs for the
reconstructed paleoglaciers are 2300, 2230, and 2240 m a.s.l. (accumulation
area ratio, AAR) for Val Giuv, Mila and Strem, respectively (Fig. 4). All
three valleys hosted glaciers during the Little Ice Age. ELA depressions
with respect to the Little Ice Age ELAs, which were 2700, 2570 and 2650 m a.s.l. (Maisch, 1992), are 400, 340 and 410 m, respectively. ELA depression
during the Egesen stadial across the Alps varies between 250 and 350 m
(Ivy-Ochs, 2015, and references therein). Both the <inline-formula><mml:math id="M54" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">10</mml:mn></mml:msup></mml:math></inline-formula>Be ages and ELA
depressions support the hypothesis that the studied moraines record advance
of Val Giuv, Mila, and Strem glaciers during the Egesen stadial, which was
between about 13 and 11.5 kyr ago (Ivy-Ochs, 2015).</p>
</sec>
</sec>
<sec id="Ch1.S4" sec-type="conclusions">
  <title>Discussion and conclusions</title>
      <?pagebreak page21?><p id="d1e949">The dated left-lateral moraine at the mouth of Val Mila (Mila2) is buried
along its downstream end by fan sediments sourced in the small basin Val
Pulanera. In Val Strem three left-lateral moraines are partially buried by
the Drun upper fan deposits (Fig. 2c). Although those moraines are undated,
the similarity of the paleoglacier ELAs and <inline-formula><mml:math id="M55" display="inline"><mml:mi mathvariant="normal">Δ</mml:mi></mml:math></inline-formula>ELAs with respect to
Little Ice Age ELAs point to contemporaneity of moraine formation with the
dated moraines in Val Giuv (12.9–10.9 kyr ago). As the footprint of the
paleoglacier snout associated with the dated moraines (Fig. 4) was downstream
of the Drun–Strem confluence, debris-flow activity post-dates the Egesen
stadial. Similarly, the core data show that only the top 35–40 m of valley
fill is actually debris-flow sediments; most is fluvial and glaciofluvial
deposits of the Vorderrhein River, which accumulated in the overdeepening
upstream of Bugnei. In sum, our data indicate that fan sediments built up
after the end of the Lateglacial and that aggradation only took place for a
few tens to at most hundreds of years (deposit thickness 30–40 m), when one
considers that tens of metres of debris-flow
sediment can accumulate in a single event (Harvey et al., 2005).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F5" specific-use="star"><caption><p id="d1e961">Coloured elevation overlain on hillshade map of the area between
Disentis and Flims (swisstopo JA100120). The dark grey area represents the
Flims landslide deposits. The black thick dashed line indicates the location
of the blockage of the Vorderrhein River by the landslide dam (von
Poschinger, 2005). The proposed Ilanzersee shoreline at an elevation of
1150 m a.s.l. (Wassmer et al., 2004) is outlined in grey dots. This
reconstruction shows that a lake with surface at 1150 m a.s.l would have
overflowed the landslide dam at several points both north and south of the
location of the blockage and subsequent final breach. The white and light
blue areas show extents of Ilanzersee with shorelines of 940 and
830 m a.s.l., respectively, as proposed by von Poschinger (2005). Lower
panel: longitudinal ESE–WNW profile along the Vorderrhein River down to the
Flims landslide deposits. The two lake levels, 940 and 830 m a.s.l., are
shown. In the background the mountain peaks to the north are illustrated.
Vertical exaggeration 2.5<inline-formula><mml:math id="M56" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula>.</p></caption>
        <?xmltex \igopts{width=398.338583pt}?><graphic xlink:href="https://egqsj.copernicus.org/articles/67/17/2018/egqsj-67-17-2018-f05.jpg"/>

      </fig>

      <p id="d1e977">If the fans did not build up due to evacuation of Lateglacial glacial
deposits from the tributary valleys, then why did they aggrade and why did
aggradation stop and give way to toe incision so abruptly? We propose that
the build-up of the Sedrun and Disentis fans was related to the damming of
the Vorderrhein River by the Flims landslide. The Flims landslide (volume
9–12 km<inline-formula><mml:math id="M57" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> has been dated to 9400 cal yr BP with radiocarbon
(Deplazes et al., 2007) and 8900 <inline-formula><mml:math id="M58" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 700 years with cosmogenic <inline-formula><mml:math id="M59" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">10</mml:mn></mml:msup></mml:math></inline-formula>Be
and <inline-formula><mml:math id="M60" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">36</mml:mn></mml:msup></mml:math></inline-formula>Cl (Ivy-Ochs et al., 2009). The Vorderrhein was completely blocked
by a more than 600 m-thick landslide dam and a lake, Ilanzersee, formed
upstream (Wassmer et al., 2004; von Poschinger, 2005). This would have led to
marked upstream aggradation for as long as the lake existed. Interestingly,
in 1882 Heim mentioned that the Flims landslide-dammed lake had an impact on
the landscape all the way up to Disentis, without giving details (Heim,
1882). The highest elevation of the lake is difficult to assess, especially
as it may not have been at that elevation for very long. Wassmer et
al. (2004) suggest a lake level of 1150 m a.s.l. but geomorphological
evidence shows that a lake that high would have overflowed the landslide at
numerous locations (cf. von Poschinger, 2005). It seems that the lake could
have attained a level of around 940 m a.s.l. without overflowing (Fig. 5).
Von Poschinger (2005) estimated a highest level of 936 m a.s.l. and a level
that was held for fairly long at about 830 m a.s.l. As soon as the lake had
filled with water (taking many years, disregarding seepage), a new higher
local base level for all torrents upstream of the lake was established. The
marked flattening of the river gradient and reduction in stream power led to
immediate and rapid aggradation upstream. First to aggrade were the fans near
Disentis whose fan toes were closest to the western end of the lake. At
present, there is no evidence that the Disentis fans were deltas. As these
fans grew they blocked the Cavorgia canyon (Fig. 2). Vorderrhein sediment
choked the canyon and the Bugnei fan began to build up. This led to formation
of accommodation space around Sedrun. As shown by the core data, first a lake
formed west of Bugnei (recorded by sand layers between 1330 and
1340 m a.s.l. in core SBB), then the three fans, Pulanera, L'Ondadusa and
Drun, aggraded and coalesced to form a continuous surface with an elevation
of about 1380 m a.s.l. Ilanzersee never filled completely with sediment but
emptied (likely stepwise) due to breaches in the landslide deposit where the
present Vorderrhein channel is. The uniformity of the marked cut-off toes of
the Disentis and<?pagebreak page22?> Sedrun fans suggests coherent response to an abrupt
downstream change in base level, which we suggest was the draining of
Ilanzersee. As the lake level decreased suddenly, the Vorderrhein was able to
clear out the Cavorgia canyon (there is no evidence for formation of a new
bedrock canyon epigenetically), base level dropped and fan aggradation
ceased. The fan toes were incised. The associated knickpoint is now located
near the outlet of the Drun torrent just west of the Bugnei fan, as attested
by the bedrock outcrops in the channel at elevation 1340 m a.s.l. This is
also the approximate elevation of the present floodplain upstream of this
point. The broad floodplain (200 m wide) and the nine cut terraces reflect
meandering of the Vorderrhein near Pulanera and point to the river being in a
stable state at present along this reach.</p>
</sec>

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

      <p id="d1e1022">All primary data for this paper are given in the tables.
Data are archived in the expage database (<uri>http://expage.github.io/</uri>,
last access: 17 April 2018).</p>
  </notes><notes notes-type="competinginterests">

      <p id="d1e1031">The authors declare that they have no conflict of
interest.</p>
  </notes><ack><title>Acknowledgements</title><p id="d1e1037">AlpTransit Gotthard AG and swisstopo are thanked for allowing access to drill
core data for the Gotthard basis tunnel site. We are grateful for support of
fieldwork, sample preparation and AMS measurements provided by the Ion Beam
Physics group at ETH Zurich. Constructive reviews and comments by an
anonymous reviewer and Christopher Lüthgens helped us to improve the
manuscript.</p></ack><ref-list>
    <title>References</title>

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