Geomagnetic effects on cosmic ray propagation for different conditions

The geomagnetic field (B geo) sets a lower cutoff rigidity (R c) to the entry of cosmic particles to Earth which depends on the geomagnetic activity. From numerical simulations of the trajectory of a proton (performed with the MAGCOS code) in the B geo, we use backtracking to analyze particles arriv...

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Autores principales: Masías-Meza, J.J., Bertou, X., Dass, S.
Formato: Artículo publishedVersion
Publicado: 2011
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Acceso en línea:http://hdl.handle.net/20.500.12110/paper_17439213_v7_nS286_p234_MasiasMeza
https://repositoriouba.sisbi.uba.ar/gsdl/cgi-bin/library.cgi?a=d&c=artiaex&d=paper_17439213_v7_nS286_p234_MasiasMeza_oai
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spelling I28-R145-paper_17439213_v7_nS286_p234_MasiasMeza_oai2024-08-16 Masías-Meza, J.J. Bertou, X. Dass, S. 2011 The geomagnetic field (B geo) sets a lower cutoff rigidity (R c) to the entry of cosmic particles to Earth which depends on the geomagnetic activity. From numerical simulations of the trajectory of a proton (performed with the MAGCOS code) in the B geo, we use backtracking to analyze particles arriving at the Auger Observatory location. We determine the asymptotic trajectories and the values of R c in different incidence directions. Simulations were done using several models of B geo that emulate different geomagnetic conditions. © 2012 International Astronomical Union. application/pdf http://hdl.handle.net/20.500.12110/paper_17439213_v7_nS286_p234_MasiasMeza info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar Proc. Int. Astron. Union 2011;7(S286):234-237 cosmic rays Sun: magnetic fields Geomagnetic effects on cosmic ray propagation for different conditions info:eu-repo/semantics/article info:ar-repo/semantics/artículo info:eu-repo/semantics/publishedVersion https://repositoriouba.sisbi.uba.ar/gsdl/cgi-bin/library.cgi?a=d&c=artiaex&d=paper_17439213_v7_nS286_p234_MasiasMeza_oai
institution Universidad de Buenos Aires
institution_str I-28
repository_str R-145
collection Repositorio Digital de la Universidad de Buenos Aires (UBA)
topic cosmic rays
Sun: magnetic fields
spellingShingle cosmic rays
Sun: magnetic fields
Masías-Meza, J.J.
Bertou, X.
Dass, S.
Geomagnetic effects on cosmic ray propagation for different conditions
topic_facet cosmic rays
Sun: magnetic fields
description The geomagnetic field (B geo) sets a lower cutoff rigidity (R c) to the entry of cosmic particles to Earth which depends on the geomagnetic activity. From numerical simulations of the trajectory of a proton (performed with the MAGCOS code) in the B geo, we use backtracking to analyze particles arriving at the Auger Observatory location. We determine the asymptotic trajectories and the values of R c in different incidence directions. Simulations were done using several models of B geo that emulate different geomagnetic conditions. © 2012 International Astronomical Union.
format Artículo
Artículo
publishedVersion
author Masías-Meza, J.J.
Bertou, X.
Dass, S.
author_facet Masías-Meza, J.J.
Bertou, X.
Dass, S.
author_sort Masías-Meza, J.J.
title Geomagnetic effects on cosmic ray propagation for different conditions
title_short Geomagnetic effects on cosmic ray propagation for different conditions
title_full Geomagnetic effects on cosmic ray propagation for different conditions
title_fullStr Geomagnetic effects on cosmic ray propagation for different conditions
title_full_unstemmed Geomagnetic effects on cosmic ray propagation for different conditions
title_sort geomagnetic effects on cosmic ray propagation for different conditions
publishDate 2011
url http://hdl.handle.net/20.500.12110/paper_17439213_v7_nS286_p234_MasiasMeza
https://repositoriouba.sisbi.uba.ar/gsdl/cgi-bin/library.cgi?a=d&c=artiaex&d=paper_17439213_v7_nS286_p234_MasiasMeza_oai
work_keys_str_mv AT masiasmezajj geomagneticeffectsoncosmicraypropagationfordifferentconditions
AT bertoux geomagneticeffectsoncosmicraypropagationfordifferentconditions
AT dasss geomagneticeffectsoncosmicraypropagationfordifferentconditions
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