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

Please use this identifier to cite or link to this item: http://dspace.mediu.edu.my:8181/xmlui/handle/123456789/7829

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DC Field	Value	Language
dc.creator	Dasso S.	-
dc.creator	Gratton F.T.	-
dc.creator	Farrugia C.J.	-
dc.date	2002	-
dc.date.accessioned	2013-06-01T09:28:22Z	-
dc.date.available	2013-06-01T09:28:22Z	-
dc.date.issued	2013-06-01	-
dc.identifier	http://www.scielo.br/scielo.php?script=sci_arttext&pid=S0103-97332002000300026	-
dc.identifier	http://www.doaj.org/doaj?func=openurl&genre=article&issn=01039733&date=2002&volume=32&issue=2b&spage=632	-
dc.identifier.uri	http://koha.mediu.edu.my:8181/jspui/handle/123456789/7829	-
dc.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.	-
dc.publisher	Sociedade Brasileira de Física	-
dc.source	Brazilian Journal of Physics	-
dc.title	The role of alpha particles in the emission of plasma waves inside solar ejecta	-
Appears in Collections:	Physics and Astronomy

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