Evolution of magnetic fields in the solar atmosphere

dc.contributor.author	Ravindra, B
dc.date.accessioned	2006-03-15T08:44:19Z
dc.date.available	2006-03-15T08:44:19Z
dc.date.issued	2005-09
dc.identifier.citation	BASI, Vol. 33, No. 3, pp. 333-336	en
dc.identifier.uri	http://hdl.handle.net/2248/790
dc.description.abstract	The Sun affects the terrestrial climate and weather as well as near Earth space by its high energy radiation and particle emissions. It is now becoming clear that the solar magnetic field, which controls all the physical processes in the solar atmosphere, is the driver for these two processes. In this thesis we have studied the role of the evolution of magnetic fields in the production of enhanced high energy radiation and particle emission from the Sun.	en
dc.format.extent	111297 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.subject	Sun	en
dc.subject	activity- Sun	en
dc.subject	coronal mass ejections (CMEs) -Sun	en
dc.subject	oscil- lations Sun	en
dc.subject	magenetic fields	en
dc.title	Evolution of magnetic fields in the solar atmosphere	en
dc.type	Article	en