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Magnetohydrostatics

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Book cover Solar Magnetohydrodynamics

Part of the book series: Geophysics and Astrophysics Monographs ((GAAM,volume 21))

Abstract

A comparison of the sizes of terms in the equation of motion

$$ \rho \frac{{Dv}}{{Dt}} = - \nabla p + k \times B + \rho g $$
(2.21)

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

$$ O = - \nabla p + j \times B + \rho g $$
(3.1)

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

$$ j = curl\,B/\mu $$
(3.2)
$$ div\,B = 0 $$
(3.3)
$$ \rho = \frac{{mp}} {{{k_B}T}} $$
(3.4)

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

  • Print ISBN: 978-90-277-1833-4

  • Online ISBN: 978-94-009-7958-1

  • eBook Packages: Springer Book Archive

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