Non-axisymmetric magnetostatic equilibrium in cylindrical coordinates and its application to sunspots

Details Non-axisymmetric magnetostatic equilibrium in cylindrical coordinates and its application to sunspots Non-axisymmetric magnetostatic equilibrium in cylindrical coordinates and its application to sunspots

Sep 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985cha%26a...9..254h&link_type=abstract

Chinese Astronomy and Astrophysics, Volume 9, Issue 3, p. 254-258.

Astronomy and Astrophysics

Astrophysics

Scientific paper

This paper describes a general solution to the 3-dimensional, 2-component magnetostatic equation assuming the total pressure (gas plus magnetic) to be a function of the height only. By adjusting the two arbitrary functions appearing in the general solution one may obtain various particular solutions which are not subject to the assumption of perturbations being small when applied to solar phenomena. One such particular solution qualitatively accounts for the observed asymmetry in the shape of the sunspots and the filamentary structure in them.

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