Different distribution functions of solar x-ray flares

dc.contributor.author	Das, T. K
dc.contributor.author	De, B. K
dc.contributor.author	Bhattacharyya, J
dc.date.accessioned	2006-03-13T05:24:16Z
dc.date.available	2006-03-13T05:24:16Z
dc.date.issued	2004-03
dc.identifier.citation	BASI, Vol. 32, No. 1, pp. 15-23	en
dc.identifier.uri	http://hdl.handle.net/2248 /718
dc.description.abstract	A statistical study has been done on soft x-ray (SXR) flares, the data of which were collected by Geostationary Operational Environmental Satellites (GOES) during the period July 1993?June 1994. From the analysis different distribution functions were obtained empirically which give the number of SXR flares per unit interval of intensity and asymmetry in duration and angular interval of longitude. These distribution functions have been used for evaluating the center to limb variation of optical thickness for SXR flares	en
dc.format.extent	53881 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.subject	X-ray flares	en
dc.title	Different distribution functions of solar x-ray flares	en
dc.type	Article	en