Peculiar abundances in Solar particle emissions

dc.contributor.author	Vahia, M. N
dc.date.accessioned	2005-01-08T08:11:36Z
dc.date.available	2005-01-08T08:11:36Z
dc.date.issued	1988
dc.identifier.citation	Kodaikanal Observatory Bulletins Series A, Vol. 9, pp. 195-200	en
dc.identifier.issn	0374-3632
dc.identifier.uri	http://hdl.handle.net/2248/200
dc.description.abstract	In this paper we attempt to show that currently available data on solar flare particle abundances allows studies of abundance and enchancement patterns. In particular we show that solar particles originate from regions of temperature around 6 x 10/sup5/K. We also take a look at the direct charge state measurements in small and large flares and show that it is possible to distinguish between the coronal and photospheric components of solar flares. We then deduce the thermal conditions that must be existing during various stages of solar particle flare build up and release.	en
dc.format.extent	180679 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en
dc.publisher	Indian Institute of Astrophysics, Bangalore	en
dc.subject	Solar flare particle	en
dc.title	Peculiar abundances in Solar particle emissions	en
dc.type	Article	en