Irrotational motion in quiescent prominences

dc.contributor.author	Pande, M. C.
dc.contributor.author	Bondal, K. R.
dc.date.accessioned	2010-01-19T04:57:09Z
dc.date.available	2010-01-19T04:57:09Z
dc.date.issued	1991
dc.identifier.uri	http://hdl.handle.net/123456789/453
dc.description.abstract	On the basis of Kippenhahn and Schluter's magnetohydrostatic model of a quiescent prominence, an attempt has been made to study the effect of irrotational motion existing in the prominences on the magnetic field pattern in it, introducing an irrotatinal velocity field. It is found lthat, under such a condition. the magnetic field geometry int the model does not change.	en_US
dc.language.iso	en	en_US
dc.relation.ispartofseries	ass182-201
dc.subject	Astrophysics	en_US
dc.title	Irrotational motion in quiescent prominences	en_US
dc.type	Article	en_US