Determination of thermodynamic conditions in the chromosphere above a sunspot by solving an inverse problem. II - Numerical modeling of pressure and density distributions

Details Determination of thermodynamic conditions in the chromosphere above a sunspot by solving an inverse problem. II - Numerical modeling of pressure and density distributions Determination of thermodynamic conditions in the chromosphere above a sunspot by solving an inverse problem. II - Numerical modeling of pressure and density distributions

Jun 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992kfnt....8...27t&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 8, no. 3, May-June 1992, p. 27-37. In Russian.

Computer Science

3

Chromosphere, Solar Electrons, Sunspots, Thermodynamic Properties, Computerized Simulation, Density Distribution, Gas Pressure, Umbras

Scientific paper

The temperature and electron density distributions are used to reconstruct the total pressure, mass density, and geometric height of the chromosphere above a sunspot. The hypothesis of hydrostatic equilibrium is not applied. The calculations are performed using a test model that simulates conditions in the chromosphere above the sunspot umbra. A criterion is formulated which makes it possible to use these calculations to determine whether equilibrium exists in the umbra chromosphere. It is suggested that the algorithm proposed will also make it possible to estimate the inclination of the sunspot flux tube axis within the framework of magnetohydrostatic equilibrium.

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