A note on the rotational motion in quiescent prominences

dc.contributor.author	Pande, M. C
dc.contributor.author	Bondal, K. R
dc.date.accessioned	2007-09-13T11:08:59Z
dc.date.available	2007-09-13T11:08:59Z
dc.date.issued	1995
dc.identifier.citation	BASI, Vol. 23, No. 1, pp. 97-100	en
dc.identifier.uri	http://hdl.handle.net/2248/1781
dc.description.abstract	Following an earlier paper (Pande & Bondal 1991) we have, on the basis of Kippenhahn and Schluter's magnetohydrostatic model of a quiescent prominence, attempted to study the effect of a rotational velocity field in the vertical plane. However, it was not possible to establish whether the rotational velocity field in the vertical plane could be accomodated in the model. We now find that the rotational motion is possible both in the vertical and horizontal planes, without violating the basic assumptions in that model; this is a modification over earlier conclusion.	en
dc.format.extent	194111 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1995BASI...23...97P	en
dc.subject	quiescent prominences	en
dc.subject	rotational motion	en
dc.title	A note on the rotational motion in quiescent prominences	en
dc.type	Article	en