Two-dimensional non-symmetric models of quiescent prominences in potential magnetic fields

Details Two-dimensional non-symmetric models of quiescent prominences in potential magnetic fields Two-dimensional non-symmetric models of quiescent prominences in potential magnetic fields

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988a%26a...207..154a&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 207, no. 1, Dec. 1988, p. 154-161.

Astronomy and Astrophysics

Astrophysics

10

Solar Magnetic Field, Solar Prominences, Two Dimensional Models, Current Sheets, Magnetic Field Configurations, Solar Gravitation, Stellar Models

Scientific paper

The authors present a general method which allows to construct in the half-space {z > 0} non-y-symmetric x invariant models describing the equilibrium of a massive current sheet submitted to the action of a vertical gravitational field and of a potential magnetic field. They also derive general relations which determine the current and the mass of the sheet and the total energy of the configuration from the only value of the magnetic field on the plane {z = 0}.

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