FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2329120260> ?p ?o ?g. }

• W2329120260 endingPage "938" @default.
• W2329120260 startingPage "935" @default.
• W2329120260 abstract "Research Article| October 01, 2012 Debris-flow–dependent variation of cosmogenically derived catchment-wide denudation rates F. Kober; F. Kober * 1Institute of Geology, ETH Zürich, 8092 Zürich, Switzerland *E-mail: kober@erdw.ethz.ch. Search for other works by this author on: GSW Google Scholar K. Hippe; K. Hippe 2Institute of Geochemistry and Petrology, ETH Zürich, 8092 Zürich, Switzerland Search for other works by this author on: GSW Google Scholar B. Salcher; B. Salcher 1Institute of Geology, ETH Zürich, 8092 Zürich, Switzerland Search for other works by this author on: GSW Google Scholar S. Ivy-Ochs; S. Ivy-Ochs 3Institute of Ion Beam Physics, ETH Zürich, 8093 Zürich, Switzerland Search for other works by this author on: GSW Google Scholar P.W. Kubik; P.W. Kubik 3Institute of Ion Beam Physics, ETH Zürich, 8093 Zürich, Switzerland Search for other works by this author on: GSW Google Scholar L. Wacker; L. Wacker 3Institute of Ion Beam Physics, ETH Zürich, 8093 Zürich, Switzerland Search for other works by this author on: GSW Google Scholar N. Hählen N. Hählen 4Oberingenieurkreis I, Tiefbauamt des Kantons Bern, 3601 Thun, Switzerland Search for other works by this author on: GSW Google Scholar Author and Article Information F. Kober * 1Institute of Geology, ETH Zürich, 8092 Zürich, Switzerland K. Hippe 2Institute of Geochemistry and Petrology, ETH Zürich, 8092 Zürich, Switzerland B. Salcher 1Institute of Geology, ETH Zürich, 8092 Zürich, Switzerland S. Ivy-Ochs 3Institute of Ion Beam Physics, ETH Zürich, 8093 Zürich, Switzerland P.W. Kubik 3Institute of Ion Beam Physics, ETH Zürich, 8093 Zürich, Switzerland L. Wacker 3Institute of Ion Beam Physics, ETH Zürich, 8093 Zürich, Switzerland N. Hählen 4Oberingenieurkreis I, Tiefbauamt des Kantons Bern, 3601 Thun, Switzerland *E-mail: kober@erdw.ethz.ch. Publisher: Geological Society of America Received: 12 Mar 2012 Revision Received: 19 Apr 2012 Accepted: 24 Apr 2012 First Online: 09 Mar 2017 Online ISSN: 1943-2682 Print ISSN: 0091-7613 © 2012 Geological Society of America Geology (2012) 40 (10): 935–938. https://doi.org/10.1130/G33406.1 Article history Received: 12 Mar 2012 Revision Received: 19 Apr 2012 Accepted: 24 Apr 2012 First Online: 09 Mar 2017 Cite View This Citation Add to Citation Manager Share Icon Share Facebook Twitter LinkedIn MailTo Tools Icon Tools Get Permissions Search Site Citation F. Kober, K. Hippe, B. Salcher, S. Ivy-Ochs, P.W. Kubik, L. Wacker, N. Hählen; Debris-flow–dependent variation of cosmogenically derived catchment-wide denudation rates. Geology 2012;; 40 (10): 935–938. doi: https://doi.org/10.1130/G33406.1 Download citation file: Ris (Zotero) Refmanager EasyBib Bookends Mendeley Papers EndNote RefWorks BibTex toolbar search Search Dropdown Menu toolbar search search input Search input auto suggest filter your search All ContentBy SocietyGeology Search Advanced Search Abstract Catchment-wide denudation rates (CWDRs) obtained from cosmogenic nuclides are an efficient way to determine geomorphic processes quantitatively in alpine mountain ranges over Holocene time scales. These rate estimations assume steady geomorphic processes. Here we use a time series (3 yr) in the Aare catchment (central Swiss Alps) to test the impact of spatially heterogeneous stochastic sediment supply on CWDRs. Our results show that low-frequency, high-magnitude debris-flow events significantly perturb cosmogenic nuclide (10Be, 14C) concentrations and thus CWDRs. The 10Be concentrations decrease by a factor of two following debris-flow events, resulting in a doubling of inferred CWDRs. The variability indicates a clear time and source dependency on sediment supply, with restricted area-weighted mixing of sediment. Accordingly, in transient environments, it is critical to have an understanding of the history of geomorphic processes to derive meaningful CWDRs. We hypothesize that the size of debris flows, their connectivity with the trunk stream, and the ability of the system to sufficiently mix sediment from low- and high-order catchments control the magnitude of CWDR perturbations. We also determined in situ 14C in a few samples. In conjunction with 10Be, these data suggest partial storage for colluvium of a few thousand years within the catchment prior to debris-flow initiation. You do not have access to this content, please speak to your institutional administrator if you feel you should have access." @default.
• W2329120260 created "2016-06-24" @default.
• W2329120260 creator A5005926508 @default.
• W2329120260 creator A5014196437 @default.
• W2329120260 creator A5053554134 @default.
• W2329120260 creator A5054358077 @default.
• W2329120260 creator A5084656266 @default.
• W2329120260 creator A5084975117 @default.
• W2329120260 creator A5086709204 @default.
• W2329120260 date "2012-10-01" @default.
• W2329120260 modified "2023-10-06" @default.
• W2329120260 title "Debris-flow–dependent variation of cosmogenically derived catchment-wide denudation rates" @default.
• W2329120260 cites W1942985662 @default.
• W2329120260 cites W1968993853 @default.
• W2329120260 cites W1969970441 @default.
• W2329120260 cites W1976972127 @default.
• W2329120260 cites W1987334540 @default.
• W2329120260 cites W1995035032 @default.
• W2329120260 cites W2010036448 @default.
• W2329120260 cites W2048535129 @default.
• W2329120260 cites W2085615677 @default.
• W2329120260 cites W2093570562 @default.
• W2329120260 cites W2098797024 @default.
• W2329120260 cites W2101165942 @default.
• W2329120260 cites W2116292804 @default.
• W2329120260 cites W2144560571 @default.
• W2329120260 doi "https://doi.org/10.1130/g33406.1" @default.
• W2329120260 hasPublicationYear "2012" @default.
• W2329120260 type Work @default.
• W2329120260 sameAs 2329120260 @default.
• W2329120260 citedByCount "59" @default.
• W2329120260 countsByYear W23291202602013 @default.
• W2329120260 countsByYear W23291202602014 @default.
• W2329120260 countsByYear W23291202602015 @default.
• W2329120260 countsByYear W23291202602016 @default.
• W2329120260 countsByYear W23291202602017 @default.
• W2329120260 countsByYear W23291202602018 @default.
• W2329120260 countsByYear W23291202602019 @default.
• W2329120260 countsByYear W23291202602020 @default.
• W2329120260 countsByYear W23291202602022 @default.
• W2329120260 crossrefType "journal-article" @default.
• W2329120260 hasAuthorship W2329120260A5005926508 @default.
• W2329120260 hasAuthorship W2329120260A5014196437 @default.
• W2329120260 hasAuthorship W2329120260A5053554134 @default.
• W2329120260 hasAuthorship W2329120260A5054358077 @default.
• W2329120260 hasAuthorship W2329120260A5084656266 @default.
• W2329120260 hasAuthorship W2329120260A5084975117 @default.
• W2329120260 hasAuthorship W2329120260A5086709204 @default.
• W2329120260 hasConcept C121332964 @default.
• W2329120260 hasConcept C127313418 @default.
• W2329120260 hasConcept C151730666 @default.
• W2329120260 hasConcept C77928131 @default.
• W2329120260 hasConcept C87432785 @default.
• W2329120260 hasConceptScore W2329120260C121332964 @default.
• W2329120260 hasConceptScore W2329120260C127313418 @default.
• W2329120260 hasConceptScore W2329120260C151730666 @default.
• W2329120260 hasConceptScore W2329120260C77928131 @default.
• W2329120260 hasConceptScore W2329120260C87432785 @default.
• W2329120260 hasIssue "10" @default.
• W2329120260 hasLocation W23291202601 @default.
• W2329120260 hasOpenAccess W2329120260 @default.
• W2329120260 hasPrimaryLocation W23291202601 @default.
• W2329120260 hasRelatedWork W2045075746 @default.
• W2329120260 hasRelatedWork W2146702900 @default.
• W2329120260 hasRelatedWork W2329748349 @default.
• W2329120260 hasRelatedWork W2391363624 @default.
• W2329120260 hasRelatedWork W2530194962 @default.
• W2329120260 hasRelatedWork W2792858061 @default.
• W2329120260 hasRelatedWork W2799505156 @default.
• W2329120260 hasRelatedWork W3120001605 @default.
• W2329120260 hasRelatedWork W4220959611 @default.
• W2329120260 hasRelatedWork W4295677999 @default.
• W2329120260 hasVolume "40" @default.
• W2329120260 isParatext "false" @default.
• W2329120260 isRetracted "false" @default.
• W2329120260 magId "2329120260" @default.
• W2329120260 workType "article" @default.