Determination of the thermodynamic conditions in the chromosphere above a sunspot by solving an inverse problem. I - Numerical simulation of temperature and electron density distributions

Details Determination of the thermodynamic conditions in the chromosphere above a sunspot by solving an inverse problem. I - Numerical simulation of temperature and electron density distributions Determination of the thermodynamic conditions in the chromosphere above a sunspot by solving an inverse problem. I - Numerical simulation of temperature and electron density distributions

Feb 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992kfnt....8....3t&link_type=citations

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 8, Jan.-Feb. 1992, p. 3-11. In Russian.

Mathematics

2

Chromosphere, Electron Density Profiles, Solar Electrons, Sunspots, Temperature Distribution, Iterative Solution, Mathematical Models, Spectral Methods, Thermodynamic Properties

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