3He Rich Solar Flares

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