3He Rich Solar Flares

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/360

Full metadata record

DC Field	Value	Language
dc.contributor.author	Ramadurai, S	-
dc.date.accessioned	2005-02-10T13:59:15Z	-
dc.date.available	2005-02-10T13:59:15Z	-
dc.date.issued	1986	-
dc.identifier.citation	Kodaikanal Observatory Bulletins Series A, Vol. 6, pp. 49-56	en
dc.identifier.issn	0374-3632	-
dc.identifier.uri	http://hdl.handle.net/2248/360	-
dc.description.abstract	The various observational features of the 3He rich solar flares like their characteristics and association with other phenomena are discussed. It is shown that 3He rich flares split into two distinct groups, if one plots the 3He/H ratio as a function of maximum proton flux at an energy of about 10 MeV. ISEE 3 observations have shown that 3He rich events are associated with impulsive non-relativistic electron events. Observatons with Type II bursts and coronal mass ejections, unlike the other energetic particle events. Implications of these observations, on any possible model for the origin of 3He rich events, are highlighted.	en
dc.format.extent	295893 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	-
dc.publisher	Indian Institute of Astrophysics, Bangalore	en
dc.subject	solar flares	en
dc.subject	Type II bursts	en
dc.title	3He Rich Solar Flares	en
dc.type	Article	en
Appears in Collections:	IIAP Publications Kodaikanal Observatory Bulletins (1905 - 1997 )

Files in This Item:

File	Description	Size	Format
He Rich Solar Flares.pdf		288.96 kB	Adobe PDF	View/Open

DSpace JSPUI