Magnetohydrostatic structures in the solar atmosphere

Details Magnetohydrostatic structures in the solar atmosphere Magnetohydrostatic structures in the solar atmosphere

May 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984soph...92...15m&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 92, May 1984, p. 15-31.

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11

Atmospheric Physics, Magnetohydrostatics, Solar Atmosphere, Solar Physics, Isothermal Processes, Lines Of Force, Photosphere, Topology

Scientific paper

Separable two-dimensional solutions to the isothermal magnetohydrostatic equations are presented which include the effect of gravity. Examples of three types of linear solution are given in which photospheric magnetic fields are prescribed and the field topologies are discussed. In addition, a new nonlinear solution is discussed. The functional form of the pressure distribution is restricted by the separable assumption. An analysis suggests that these are the only separable analytical solutions.

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