The effect of magnetic shear on the MHD stability of a prominence model

Details The effect of magnetic shear on the MHD stability of a prominence model The effect of magnetic shear on the MHD stability of a prominence model

Dec 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994soph..155..267l&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 155, no. 2, p. 267-284

Physics

3

Magnetic Effects, Magnetohydrodynamic Stability, Shear Flow, Solar Prominences, Stellar Models, Ballooning Modes, Euler-Lagrange Equation, Plasma Equilibrium, Polarity, Pressure Effects

Scientific paper

The Hood-Anzer prominence model (Hood and Anzer, 1990) is modified to include magnetic shear. The stability properties of the model are then assessed to see if significant magnetic shear can stabilize ideal magnetohydrodynamic (MHD) disturbances. It is shown that a strong shear gradient in the magnetic field near the base of the prominence provides a stabilizing effect and realistic prominence heights are indeed possible.

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