Deciphering the evolution of the Bleis Marscha rock glacier (Val d'Err, eastern Switzerland) with cosmogenic nuclide exposure dating, aerial image correlation, and finite element modeling

<p>We constrain the Holocene development of the active Bleis Marscha rock glacier (Err–Julier area, eastern Swiss Alps) with 15 cosmogenic nuclide exposure ages (<span class="inline-formula"><sup>10</sup></span>Be, <span class="inline-formula">...

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Main Authors: D. Amschwand, S. Ivy-Ochs, M. Frehner, O. Steinemann, M. Christl, C. Vockenhuber
Format: Article
Language:English
Published: Copernicus Publications 2021-04-01
Series:The Cryosphere
Online Access:https://tc.copernicus.org/articles/15/2057/2021/tc-15-2057-2021.pdf
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spelling doaj-47d936874e1344e0a28f409567055d052021-04-26T11:27:07ZengCopernicus PublicationsThe Cryosphere1994-04161994-04242021-04-01152057208110.5194/tc-15-2057-2021Deciphering the evolution of the Bleis Marscha rock glacier (Val d'Err, eastern Switzerland) with cosmogenic nuclide exposure dating, aerial image correlation, and finite element modelingD. Amschwand0D. Amschwand1S. Ivy-Ochs2S. Ivy-Ochs3M. Frehner4O. Steinemann5M. Christl6C. Vockenhuber7Department of Earth Sciences, ETH Zurich, 8092, Zurich, Switzerlandnow at: Department of Geosciences, University of Fribourg, 1700, Fribourg, SwitzerlandDepartment of Earth Sciences, ETH Zurich, 8092, Zurich, SwitzerlandLaboratory of Ion Beam Physics, ETH Zurich, 8093, Zurich, SwitzerlandDepartment of Earth Sciences, ETH Zurich, 8092, Zurich, SwitzerlandLaboratory of Ion Beam Physics, ETH Zurich, 8093, Zurich, SwitzerlandLaboratory of Ion Beam Physics, ETH Zurich, 8093, Zurich, SwitzerlandLaboratory of Ion Beam Physics, ETH Zurich, 8093, Zurich, Switzerland<p>We constrain the Holocene development of the active Bleis Marscha rock glacier (Err–Julier area, eastern Swiss Alps) with 15 cosmogenic nuclide exposure ages (<span class="inline-formula"><sup>10</sup></span>Be, <span class="inline-formula"><sup>36</sup></span>Cl), horizontal surface creep rate quantification by correlating two orthophotos from 2003 and 2012, and finite element modeling. We used the latter to separate the control on surface movement exerted by topography and material properties. Bleis Marscha is a stack of three overriding lobes whose formation phases are separated by time gaps expressed morphologically as over-steepened terrain steps and kinematically as a sharp downslope decrease in surface movement. The three discrete formation phases appear to be correlated to major Holocene climate shifts: Early Holocene low-elevation lobes (<span class="inline-formula">∼8.9</span>–8.0 ka, after the Younger Dryas), Middle Holocene lobe (<span class="inline-formula">∼5.2</span>–4.8 ka, after the Middle Holocene warm period), and Late Holocene high-elevation lobes (active since <span class="inline-formula">∼2.8</span> ka, intermittently coexisting with oscillating Bleis Marscha cirque glacierets). The formation phases appear to be controlled in the source area by the climate-sensitive accumulation of an ice-debris mixture in proportions susceptible to rock glacier creep. The ongoing cohesive movement of the older generations requires ice at a depth which is possibly as old as its Early–Middle Holocene debris mantle. Permafrost degradation is attenuated by “thermal filtering” of the coarse debris boulder mantle and implies that the dynamics of the Bleis Marscha lobes that once formed persisted over millennia are less sensitive to climate. The cosmogenic radionuclide inventories of boulders on a moving rock glacier ideally record time since deposition on the rock glacier root but are stochastically altered by boulder instabilities and erosional processes. This work contributes to deciphering the long-term development and the past to quasi-present climate sensitivity of rock glaciers.</p>https://tc.copernicus.org/articles/15/2057/2021/tc-15-2057-2021.pdf
collection DOAJ
language English
format Article
sources DOAJ
author D. Amschwand
D. Amschwand
S. Ivy-Ochs
S. Ivy-Ochs
M. Frehner
O. Steinemann
M. Christl
C. Vockenhuber
spellingShingle D. Amschwand
D. Amschwand
S. Ivy-Ochs
S. Ivy-Ochs
M. Frehner
O. Steinemann
M. Christl
C. Vockenhuber
Deciphering the evolution of the Bleis Marscha rock glacier (Val d'Err, eastern Switzerland) with cosmogenic nuclide exposure dating, aerial image correlation, and finite element modeling
The Cryosphere
author_facet D. Amschwand
D. Amschwand
S. Ivy-Ochs
S. Ivy-Ochs
M. Frehner
O. Steinemann
M. Christl
C. Vockenhuber
author_sort D. Amschwand
title Deciphering the evolution of the Bleis Marscha rock glacier (Val d'Err, eastern Switzerland) with cosmogenic nuclide exposure dating, aerial image correlation, and finite element modeling
title_short Deciphering the evolution of the Bleis Marscha rock glacier (Val d'Err, eastern Switzerland) with cosmogenic nuclide exposure dating, aerial image correlation, and finite element modeling
title_full Deciphering the evolution of the Bleis Marscha rock glacier (Val d'Err, eastern Switzerland) with cosmogenic nuclide exposure dating, aerial image correlation, and finite element modeling
title_fullStr Deciphering the evolution of the Bleis Marscha rock glacier (Val d'Err, eastern Switzerland) with cosmogenic nuclide exposure dating, aerial image correlation, and finite element modeling
title_full_unstemmed Deciphering the evolution of the Bleis Marscha rock glacier (Val d'Err, eastern Switzerland) with cosmogenic nuclide exposure dating, aerial image correlation, and finite element modeling
title_sort deciphering the evolution of the bleis marscha rock glacier (val d'err, eastern switzerland) with cosmogenic nuclide exposure dating, aerial image correlation, and finite element modeling
publisher Copernicus Publications
series The Cryosphere
issn 1994-0416
1994-0424
publishDate 2021-04-01
description <p>We constrain the Holocene development of the active Bleis Marscha rock glacier (Err–Julier area, eastern Swiss Alps) with 15 cosmogenic nuclide exposure ages (<span class="inline-formula"><sup>10</sup></span>Be, <span class="inline-formula"><sup>36</sup></span>Cl), horizontal surface creep rate quantification by correlating two orthophotos from 2003 and 2012, and finite element modeling. We used the latter to separate the control on surface movement exerted by topography and material properties. Bleis Marscha is a stack of three overriding lobes whose formation phases are separated by time gaps expressed morphologically as over-steepened terrain steps and kinematically as a sharp downslope decrease in surface movement. The three discrete formation phases appear to be correlated to major Holocene climate shifts: Early Holocene low-elevation lobes (<span class="inline-formula">∼8.9</span>–8.0 ka, after the Younger Dryas), Middle Holocene lobe (<span class="inline-formula">∼5.2</span>–4.8 ka, after the Middle Holocene warm period), and Late Holocene high-elevation lobes (active since <span class="inline-formula">∼2.8</span> ka, intermittently coexisting with oscillating Bleis Marscha cirque glacierets). The formation phases appear to be controlled in the source area by the climate-sensitive accumulation of an ice-debris mixture in proportions susceptible to rock glacier creep. The ongoing cohesive movement of the older generations requires ice at a depth which is possibly as old as its Early–Middle Holocene debris mantle. Permafrost degradation is attenuated by “thermal filtering” of the coarse debris boulder mantle and implies that the dynamics of the Bleis Marscha lobes that once formed persisted over millennia are less sensitive to climate. The cosmogenic radionuclide inventories of boulders on a moving rock glacier ideally record time since deposition on the rock glacier root but are stochastically altered by boulder instabilities and erosional processes. This work contributes to deciphering the long-term development and the past to quasi-present climate sensitivity of rock glaciers.</p>
url https://tc.copernicus.org/articles/15/2057/2021/tc-15-2057-2021.pdf
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