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An Analytical Study of the Structure of Two-Dimensional Magnetostatic Equilibria in the Presence of Gravity
Published online by Cambridge University Press: 27 September 2017
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In order to understand how prominences are supported in the solar corona, we have recently developed several 2D models describing x-invariant equilibrium configurations of a plasma occupying a half-space {z > 0} and submitted to a magnetic field then of the form
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- Type
- Session III: Theory
- Information
- International Astronomical Union Colloquium , Volume 104 , Issue 2: Solar and Stellar Flares , 1989 , pp. 271 - 273
- Copyright
- Copyright © Kluwer 1989