dc.contributor.author
Schaar, Konstantin
dc.date.accessioned
2024-02-01T14:13:06Z
dc.date.available
2024-02-01T14:13:06Z
dc.identifier.uri
https://refubium.fu-berlin.de/handle/fub188/41586
dc.identifier.uri
http://dx.doi.org/10.17169/refubium-41306
dc.description.abstract
The data contains the model output (.nc-data) used in our paper "The Role of Deposition of Cosmogenic 10Be for the Detectability of Solar Proton Events". Our simulations were carried out with the chemistry-climate model ECHAM/MESSy Atmospheric Chemistry (EMAC) (Jöckel et al., 2016), which is based on the European Centre for Medium-Range Weather Forecast Hamburg general circulation model 5 (ECHAM5) (Roeckner et al., 2006) and the modular earth submodel system (MESSy) model version 2.55. The simulations were conducted using a horizontal/vertical resolution of T42L47MA corresponding to a Gaussian grid of 2.8 by 2.8° in latitude and longitude, 47 layers in height, with the model top at 0.01 hPa (~80 km), and pre-industrial conditions (time slice 1850), with fixed sea surface temperatures and no interactive chemistry. The data contains e.g, data on the depostion flux and mole ratio of different 10Be tracers from galactic cosmic rays and solar energetic particles as well as some general meterological model output like precipitation, wind speed and surface temperatures.
dc.publisher
Freie Universität Berlin
dc.rights.uri
https://creativecommons.org/public-domain/cc0/
dc.subject
Cosmogenic isotopes
en
dc.subject
Atmospheric dynamics
en
dc.subject.ddc
500 Naturwissenschaften und Mathematik::550 Geowissenschaften, Geologie::550 Geowissenschaften
dc.title
The Role of deposition of cosmogenic 10Be for the detectability of solar proton events
refubium.affiliation
Geowissenschaften
refubium.affiliation.other
Institut für Meteorologie
refubium.funding.funder
other
refubium.note.author
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dcterms.accessRights.openaire
open access