1993The Astrophysical JournalRequires access

On the magnetic and velocity field geometry of simple sunspots

A. M. Title, Z. Frank, Richard A. Shine, T. D. Tarbell, Kenneth P. Topka, G. B. Scharmer, Wolfgang Schmidt

Open publisher page 182 citations

Abstract

It is presently shown that a simple sunspot model with azimuthal variations in inclination, but lacking azimuthal field-strength variations, is free from azimuthal Lorentz forces. The meridional currents arising from the inclination variations are parallel to the field lines, suggesting that a cylindrically symmetric magnetostatic sunspot model can be perturbed into one with azimuthal variations in inclination with adjustment of the meridional force balance.

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What this paper is about

It is presently shown that a simple sunspot model with azimuthal variations in inclination, but lacking azimuthal field-strength variations, is free from azimuthal Lorentz forces. The meridional currents arising from the inclination variations are parallel to the field lines, suggesting that a cylindrically symmetric magnetostatic sunspot model can be perturbed into one with azimuthal variations in inclination with adjustment of the meridional force balance.

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Available abstract

It is presently shown that a simple sunspot model with azimuthal variations in inclination, but lacking azimuthal field-strength variations, is free from azimuthal Lorentz forces. The meridional currents arising from the inclination variations are parallel to the field lines, suggesting that a cylindrically symmetric magnetostatic sunspot model can be perturbed into one with azimuthal variations in inclination with adjustment of the meridional force balance.

Key concepts: Physics, Sunspot, Lorentz force, Magnetic field, Azimuth, Astrophysics, Zonal and meridional, Field (mathematics)

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