The nature of velocity fields in quiescent prominences

Details The nature of velocity fields in quiescent prominences The nature of velocity fields in quiescent prominences

Jul 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991ap%26ss.181..161b&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 181, no. 1, July 1991, p. 161-163.

Astronomy and Astrophysics

Astrophysics

Magnetic Field Configurations, Solar Magnetic Field, Solar Prominences, Magnetohydrodynamic Flow, Potential Flow, Rotating Fluids, Velocity Distribution

Scientific paper

Attention is given to the twin problem of irrotational and rotational velocity fields in quiescent prominences. It is shown that for certain definite conditions of symmetry imposed on the permitting magnetic field geometry for an isothermal case in the model of a quiescent prominence of Kippenhahn and Schlueter, any irrotational velocity field is quickly converted to rotational.

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