Irrotational motion in quiescent prominences

Details Irrotational motion in quiescent prominences Irrotational motion in quiescent prominences

Aug 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991ap%26ss.182..201p&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 182, no. 2, Aug. 1991, p. 201-206.

Astronomy and Astrophysics

Astrophysics

2

Conducting Fluids, Magnetohydrostatics, Solar Magnetic Field, Solar Prominences, Magnetic Field Configurations, Solar Rotation, Velocity Distribution

Scientific paper

On the basis of Kippenhahn and Schlueter'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 irrotational velocity field. It is found that, under such a condition, the magnetic field geometry in the model does not change.

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