Solar flare 1982 April 14

dc.contributor.author	Bagare, S. P
dc.date.accessioned	2005-12-08T05:52:40Z
dc.date.available	2005-12-08T05:52:40Z
dc.date.issued	1985-12
dc.identifier.citation	BASI, Vol. 13, No. 4, pp. 394-398	en
dc.identifier.uri	http://hdl.handle.net/2248/670
dc.description.abstract	We have obtained a good time sequence of spectroheliograms and spatial sequence spectra in the K-line of Ca II using the Kodaikanal tower telescope. We have derived the two dimensional pattern of the mass motions of the plasma associated with the flare at this level in the solar atmosphere. We find that significant mass motions are practically confined to the two ribbons that developed soon after the flaring event.	en
dc.format.extent	605970 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en
dc.publisher	Astronomical Society of India	en
dc.subject	Solar flare	en
dc.subject	Ca K spectra	en
dc.title	Solar flare 1982 April 14	en
dc.type	Article	en