Show simple item record Ramadurai, S 2005-02-10T13:59:15Z 2005-02-10T13:59:15Z 1986
dc.identifier.citation Kodaikanal Observatory Bulletins Series A, Vol. 6, pp. 49-56 en
dc.identifier.issn 0374-3632
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

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