The nature of velocity fields in quiescent prominences

dc.contributor.author	Bondal, K. R.
dc.contributor.author	Pande, M. C.
dc.date.accessioned	2010-01-19T09:01:11Z
dc.date.available	2010-01-19T09:01:11Z
dc.date.issued	1991
dc.identifier.citation	This article downloded from ADS Free Online Journal	en_US
dc.identifier.uri	http://hdl.handle.net/123456789/461
dc.description.abstract	It is shown that for certain definite conditions of symmetry imposed on the permitting magnetic field geometry for an isothermal case in Kippenhahn and Schluter's (1957) model of a quiescent prominence, any irrotational velocity field would quickly get converted to rotational.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	ass181-161
dc.subject	Quiescent prominence, Kippenhahn and Schluter's	en_US
dc.title	The nature of velocity fields in quiescent prominences	en_US
dc.type	Article	en_US