Astronomy and Astrophysics – Astrophysics
Scientific paper
Sep 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985chjss...5r..75h&link_type=abstract
(Chinese Journal of Space Science, vol. 5, no. 1, 1985, p. 75-83) Chinese Astronomy and Astrophysics (ISSN 0275-1062), vol. 9, S
Astronomy and Astrophysics
Astrophysics
Cylindrical Coordinates, Magnetostatics, Sunspots, Density Distribution, Magnetic Field Configurations, Pressure Distribution, Solar Prominences, Solar Temperature
Scientific paper
This paper describes a general solution to the three-dimensional, two-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.
Hu Yong-Qing
Xu D.-W.
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