Abstract
A comparison of the sizes of terms in the equation of motion
shows that the inertial terms on the left-hand side may be neglected when the flow speed is much smaller than both the sound speed (γp 0/ρ 0)1/2, the Alfvén speed B 0/(μρ 0)1/2 and the gravitational free-fall speed (2gl 0)l/2 for a vertical scale-length l 0. The result is a magnetohydrostatic balance
between the pressure gradient, the Lorentz force and the gravitational force. The object of the present chapter is to solve Equation (3.1) together with the subsidiary equations
And (in general) an energy equation for the temperature.
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© 2000 D. Reidel Publishing Company, Dordrecht, Holland
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Priest, E.R. (2000). Magnetohydrostatics. In: Solar Magnetohydrodynamics. Geophysics and Astrophysics Monographs, vol 21. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-7958-1_3
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DOI: https://doi.org/10.1007/978-94-009-7958-1_3
Publisher Name: Springer, Dordrecht
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