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STEIN - Stochastic erosion in-situ cosmogenic nuclide model

Authors
/persons/resource/dennis

Dennis,  Donovan
3.3 Earth Surface Geochemistry, 3.0 Geochemistry, Departments, GFZ Publication Database, Deutsches GeoForschungsZentrum;

/persons/resource/scherler

Scherler,  Dirk
3.3 Earth Surface Geochemistry, 3.0 Geochemistry, Departments, GFZ Publication Database, Deutsches GeoForschungsZentrum;

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Citation

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


Cite as: https://gfzpublic.gfz-potsdam.de/pubman/item/item_5011812
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.