Propagation of type II burst shock waves along the radial magnetic field in the solar corona

dc.contributor.author	Shelke, R. N
dc.contributor.author	Pande, M. C
dc.date.accessioned	2005-12-07T07:22:56Z
dc.date.available	2005-12-07T07:22:56Z
dc.date.issued	1985-03
dc.identifier.citation	BASI, Vol. 13, No. 1, pp 62-67	en
dc.identifier.uri	http://hdl.handle.net/2248/647
dc.description.abstract	We present an analysis which indicates that in several cases coronal holes exist in the vicinity of the active regions producing type II bursts. It is inferred that shock waves which produce type II bursts essentially travel along the coronal magnetic field.	en
dc.format.extent	497967 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en
dc.publisher	Astronomical Society of India	en
dc.subject	Type II bursts	en
dc.subject	Coronal holes	en
dc.subject	The Sun	en
dc.title	Propagation of type II burst shock waves along the radial magnetic field in the solar corona	en
dc.type	Article	en