The role of alpha particles in the emission of plasma waves inside solar ejecta

The enhancement of the resonant instability of right-hand polarized electromagnetic ion cyclotron waves by alpha particles for physical parameters corresponding to coronal mass ejections is studied. We focus on the effects of alpha thermal anisotropy and relative He++/H+ abundance on growth and abso...

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Autores principales: Dasso, S., Gratton, F.T., Farrugia, C.J.
Formato: Artículo publishedVersion
Lenguaje:Inglés
Publicado: 2002
Acceso en línea:http://hdl.handle.net/20.500.12110/paper_01039733_v32_n2B_p632_Dasso
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spelling paperaa:paper_01039733_v32_n2B_p632_Dasso2023-06-12T16:46:27Z The role of alpha particles in the emission of plasma waves inside solar ejecta Braz. J. Phys. 2002;32(2 B):632-635 Dasso, S. Gratton, F.T. Farrugia, C.J. The enhancement of the resonant instability of right-hand polarized electromagnetic ion cyclotron waves by alpha particles for physical parameters corresponding to coronal mass ejections is studied. We focus on the effects of alpha thermal anisotropy and relative He++/H+ abundance on growth and absorption rates. The first parameter governs directly wave emission, while the second modifies also the wave speed and indirectly enhances the wave excitation. Fil:Dasso, S. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. Fil:Gratton, F.T. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. 2002 info:eu-repo/semantics/article info:ar-repo/semantics/artículo info:eu-repo/semantics/publishedVersion application/pdf eng info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_01039733_v32_n2B_p632_Dasso
institution Universidad de Buenos Aires
institution_str I-28
repository_str R-134
collection Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA)
language Inglés
orig_language_str_mv eng
description The enhancement of the resonant instability of right-hand polarized electromagnetic ion cyclotron waves by alpha particles for physical parameters corresponding to coronal mass ejections is studied. We focus on the effects of alpha thermal anisotropy and relative He++/H+ abundance on growth and absorption rates. The first parameter governs directly wave emission, while the second modifies also the wave speed and indirectly enhances the wave excitation.
format Artículo
Artículo
publishedVersion
author Dasso, S.
Gratton, F.T.
Farrugia, C.J.
spellingShingle Dasso, S.
Gratton, F.T.
Farrugia, C.J.
The role of alpha particles in the emission of plasma waves inside solar ejecta
author_facet Dasso, S.
Gratton, F.T.
Farrugia, C.J.
author_sort Dasso, S.
title The role of alpha particles in the emission of plasma waves inside solar ejecta
title_short The role of alpha particles in the emission of plasma waves inside solar ejecta
title_full The role of alpha particles in the emission of plasma waves inside solar ejecta
title_fullStr The role of alpha particles in the emission of plasma waves inside solar ejecta
title_full_unstemmed The role of alpha particles in the emission of plasma waves inside solar ejecta
title_sort role of alpha particles in the emission of plasma waves inside solar ejecta
publishDate 2002
url http://hdl.handle.net/20.500.12110/paper_01039733_v32_n2B_p632_Dasso
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