Diffusion and drift of cosmic rays in highly turbulent magnetic fields
- Autores
- Candia, Julián Marcelo; Roulet, Esteban
- Año de publicación
- 2004
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- We determine numerically the parallel, perpendicular, and antisymmetric diffusion coefficients for charged particles propagating in highly turbulent magnetic fields, by means of extensive Monte Carlo simulations. We propose simple expressions, given in terms of a small set of fitting parameters, to account for the diffusion coefficients as functions of magnetic rigidity and turbulence level, and corresponding to different kinds of turbulence spectra. The results obtained satisfy scaling relations, which make them useful for describing the cosmic ray origin and transport in a variety of different astrophysical environments.
Instituto de Física La Plata - Materia
-
Astronomía
cosmic rays
magnetic fields - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- http://creativecommons.org/licenses/by/3.0/
- Repositorio
.jpg)
- Institución
- Universidad Nacional de La Plata
- OAI Identificador
- oai:sedici.unlp.edu.ar:10915/128618
Ver los metadatos del registro completo
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Diffusion and drift of cosmic rays in highly turbulent magnetic fieldsCandia, Julián MarceloRoulet, EstebanAstronomíacosmic raysmagnetic fieldsWe determine numerically the parallel, perpendicular, and antisymmetric diffusion coefficients for charged particles propagating in highly turbulent magnetic fields, by means of extensive Monte Carlo simulations. We propose simple expressions, given in terms of a small set of fitting parameters, to account for the diffusion coefficients as functions of magnetic rigidity and turbulence level, and corresponding to different kinds of turbulence spectra. The results obtained satisfy scaling relations, which make them useful for describing the cosmic ray origin and transport in a variety of different astrophysical environments.Instituto de Física La Plata2004-10-08info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfhttp://sedici.unlp.edu.ar/handle/10915/128618enginfo:eu-repo/semantics/altIdentifier/issn/1475-7516info:eu-repo/semantics/altIdentifier/arxiv/astro-ph/0408054info:eu-repo/semantics/altIdentifier/doi/10.1088/1475-7516/2004/10/007info:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by/3.0/Creative Commons Attribution 3.0 Unported (CC BY 3.0)reponame:SEDICI (UNLP)instname:Universidad Nacional de La Platainstacron:UNLP2025-09-29T11:31:17Zoai:sedici.unlp.edu.ar:10915/128618Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-09-29 11:31:17.714SEDICI (UNLP) - Universidad Nacional de La Platafalse |
| dc.title.none.fl_str_mv |
Diffusion and drift of cosmic rays in highly turbulent magnetic fields |
| title |
Diffusion and drift of cosmic rays in highly turbulent magnetic fields |
| spellingShingle |
Diffusion and drift of cosmic rays in highly turbulent magnetic fields Candia, Julián Marcelo Astronomía cosmic rays magnetic fields |
| title_short |
Diffusion and drift of cosmic rays in highly turbulent magnetic fields |
| title_full |
Diffusion and drift of cosmic rays in highly turbulent magnetic fields |
| title_fullStr |
Diffusion and drift of cosmic rays in highly turbulent magnetic fields |
| title_full_unstemmed |
Diffusion and drift of cosmic rays in highly turbulent magnetic fields |
| title_sort |
Diffusion and drift of cosmic rays in highly turbulent magnetic fields |
| dc.creator.none.fl_str_mv |
Candia, Julián Marcelo Roulet, Esteban |
| author |
Candia, Julián Marcelo |
| author_facet |
Candia, Julián Marcelo Roulet, Esteban |
| author_role |
author |
| author2 |
Roulet, Esteban |
| author2_role |
author |
| dc.subject.none.fl_str_mv |
Astronomía cosmic rays magnetic fields |
| topic |
Astronomía cosmic rays magnetic fields |
| dc.description.none.fl_txt_mv |
We determine numerically the parallel, perpendicular, and antisymmetric diffusion coefficients for charged particles propagating in highly turbulent magnetic fields, by means of extensive Monte Carlo simulations. We propose simple expressions, given in terms of a small set of fitting parameters, to account for the diffusion coefficients as functions of magnetic rigidity and turbulence level, and corresponding to different kinds of turbulence spectra. The results obtained satisfy scaling relations, which make them useful for describing the cosmic ray origin and transport in a variety of different astrophysical environments. Instituto de Física La Plata |
| description |
We determine numerically the parallel, perpendicular, and antisymmetric diffusion coefficients for charged particles propagating in highly turbulent magnetic fields, by means of extensive Monte Carlo simulations. We propose simple expressions, given in terms of a small set of fitting parameters, to account for the diffusion coefficients as functions of magnetic rigidity and turbulence level, and corresponding to different kinds of turbulence spectra. The results obtained satisfy scaling relations, which make them useful for describing the cosmic ray origin and transport in a variety of different astrophysical environments. |
| publishDate |
2004 |
| dc.date.none.fl_str_mv |
2004-10-08 |
| dc.type.none.fl_str_mv |
info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion Articulo http://purl.org/coar/resource_type/c_6501 info:ar-repo/semantics/articulo |
| format |
article |
| status_str |
publishedVersion |
| dc.identifier.none.fl_str_mv |
http://sedici.unlp.edu.ar/handle/10915/128618 |
| url |
http://sedici.unlp.edu.ar/handle/10915/128618 |
| dc.language.none.fl_str_mv |
eng |
| language |
eng |
| dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/issn/1475-7516 info:eu-repo/semantics/altIdentifier/arxiv/astro-ph/0408054 info:eu-repo/semantics/altIdentifier/doi/10.1088/1475-7516/2004/10/007 |
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info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/3.0/ Creative Commons Attribution 3.0 Unported (CC BY 3.0) |
| eu_rights_str_mv |
openAccess |
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http://creativecommons.org/licenses/by/3.0/ Creative Commons Attribution 3.0 Unported (CC BY 3.0) |
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application/pdf |
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