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	2010-03-04T09:27:24Z
dc.date.available	2010-03-04T09:27:24Z
dc.date.issued	1985
dc.identifier.citation	This article is downloaded for ADS	en_US
dc.identifier.uri	http://hdl.handle.net/123456789/613
dc.description.abstract	We present an analysis which indicates that in several cases coronal holes exist in the vicinity of the active region producing type II bursts. It is inferred that shock waves which produce type II bursts essentially along the coronal magnetic field.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	basi13-62
dc.subject	Type II Burst, Coronal holes - Sun	en_US
dc.title	Propagation of type II burst shock waves along the radial magnetic field in the solar corona	en_US
dc.type	Article	en_US