The rotational motion in quiescent prominences

Details The rotational motion in quiescent prominences The rotational motion in quiescent prominences

Aug 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991em%26p...54..119p&link_type=abstract

Earth, Moon, and Planets (ISSN 0167-9295), vol. 54, Aug. 1991, p. 119-124.

Physics

2

Rotating Fluids, Solar Prominences, Velocity Distribution, Magnetohydrostatics, Solar Physics

Scientific paper

The analysis takes into consideration the results of a previous study of velocity fields in quiescent prominences, assuming an irrotational velocity field. Retaining the same model demonstrating that such a field does not change the magnetic-field geometry of that model, the possibility of accommodating a rotational velocity field is considered. It is demonstrated that elliptically closed isovelocity contours for the model in the x-y plane cannot be obtained, however, if isovelocity contours are traced for the x-y plane, the magnetic-field geometry of the model is not affected, and the solutions for this case are possible.

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