A parametric study of the influence of ion and electron properties on the excitation of electromagnetic ion cyclotron waves in coronal mass ejections

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Interplanetary coronal mass ejections (ICMEs) often possess a negative proton thermal anisotropy, Ap = T⊥,p/T ∥.p - 1 < 0 (T∥, T⊥: parallel and perpendicular temperatures, respectively) so that right-hand polarized electromagnetic ion cyclotron waves (EICWs) may be amplified by a kinetic inst...

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Detalles Bibliográficos
Autores principales:	Dasso, S., Gratton, F.T., Farrugia, C.J.
Formato:	Artículo publishedVersion
Lenguaje:	Inglés
Publicado:	2003
Materias:	Interplanetary coronal mass ejections Ion-cyclotron instability Kinetic instabilities Magnetic clouds Plasma waves Thermal anisotropy
Acceso en línea:	http://hdl.handle.net/20.500.12110/paper_01480227_v108_nA4_p_Dasso
Aporte de:	Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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