Excitation of Solar p-mode Oscillations by Flares

dc.contributor.author	Ambastha, A
dc.contributor.author	Basu, S
dc.contributor.author	Antia, H. M
dc.date.accessioned	2008-06-05T07:39:23Z
dc.date.available	2008-06-05T07:39:23Z
dc.date.issued	2003
dc.identifier.citation	BASI, Vol. 31, No. 3&4, pp. 319 - 320	en
dc.identifier.uri	http://hdl.handle.net/2248/2405
dc.description.abstract	Solar flares release large amounts of energy at different layers of the solar atmosphere. It is, therefore, expected that major flares would be able to excite waves, thereby affecting the p-mode oscillation characteristics. From the analysis of MDI data, we find that power in p-modes appears to increase for some flares, beyond the normal values expected from the influence of magnetic field.	en
dc.format.extent	67975 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.relation.uri	http://adsabs.harvard.edu/abs/2003BASI...31..319A	en
dc.subject	Solar flares	en
dc.subject	p-mode oscillations	en
dc.title	Excitation of Solar p-mode Oscillations by Flares	en
dc.type	Article	en