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  STEIN - Stochastic erosion in-situ cosmogenic nuclide model

Dennis, D., Scherler, D. (2022): STEIN - Stochastic erosion in-situ cosmogenic nuclide model.
https://doi.org/10.5880/GFZ.3.3.2022.001

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 Creators:
Dennis, Donovan1, Author              
Scherler, Dirk1, Author              
Affiliations:
13.3 Earth Surface Geochemistry, 3.0 Geochemistry, Departments, GFZ Publication Database, Deutsches GeoForschungsZentrum, ou_146037              

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Free keywords: cosmogenic nuclides, stochastic erosion, rockfalls, hillslopes processes, alpine permafrost, Beryllium-10, Carbon-14, Helium-3
 Abstract: The stochastic erosion in-situ cosmogenic nuclide model is a 1D numerical model that simulates the evolution of the concentrations of in situ-produced Be-10, C-14, and He-3 alongside the bedrock thermal field in the shallow Earth surface. It is useful for evaluating cosmogenic nuclide data derived from field samples, in order to determine the erosion rate, erosion style, as well as the time-integrated bedrock thermal history. The model simulates erosion in four styles: no erosion, uniform (steady-state) erosion, episodic erosion, and stochastic erosion. It is particularly useful for evaluating the time-temperature evolution of bedrock hillslopes in mountainous regions.

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Language(s): eng - English
 Dates: 20222022
 Publication Status: Finally published
 Pages: -
 Publishing info: Potsdam : GFZ Data Services
 Table of Contents: -
 Rev. Type: -
 Identifiers: DOI: 10.5880/GFZ.3.3.2022.001
GFZPOF: p4 T5 Future Landscapes
 Degree: -

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