Solar X-ray bursts

dc.contributor.author	Rausaria, R. R
dc.date.accessioned	2005-01-08T06:50:59Z
dc.date.available	2005-01-08T06:50:59Z
dc.date.issued	1988
dc.identifier.citation	Kodaikanal Observatory Bulletins Series A, Vol. 9, pp. 177-194	en
dc.identifier.issn	0374-3632
dc.identifier.uri	http://hdl.handle.net/2248/199
dc.description.abstract	The experimental results of X-ray bursts about spectral characteristics, spatial distribution and directivity measurements carried out with PVO/ISEE-3 spacecraft imaging instruments of HXIS and Hard X-ray burst spectrometers during solar Maximun Mission are briefly reviewed. The observed results about the above characteristics are discussed in detail in terms of a non-thermal and a thermal model. It is shown that the results can be interpreted in terms of beamed thick target model in which electrons stream down to the loop foot points and produce the hard X-rays through electron-ion bremsstrahlung	en
dc.format.extent	665323 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en
dc.publisher	Indian Institute of Astrophysics, Bangalore	en
dc.subject	X-ray bursts	en
dc.subject	PVO/ISEE-3	en
dc.subject	Spacecraft	en
dc.title	Solar X-ray bursts	en
dc.type	Article	en