Discrepancies between empirical and theoretical models of the flaring solar chromosphere and their possible resolution

Details Discrepancies between empirical and theoretical models of the flaring solar chromosphere and their possible resolution Discrepancies between empirical and theoretical models of the flaring solar chromosphere and their possible resolution

Aug 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980stin...8119989e&link_type=abstract

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Mathematics

Atmospheric Models, Chromosphere, Magnetohydrodynamics, Mathematical Models, Solar Flares, Sun, Brightness, Electron Beams, Integral Equations, Parameter Identification, Solar Flux Density, Solar X-Rays

Scientific paper

Models of the solar chromosphere during flaring deduced theoretically or empirically are compared. Marked discrepancies are noted and various reasons are offered to explain their existence. A means is presented for testing theoretical heating models (electron heating) by analyzing the net energy loss rates in (observed) empirical atmospheres and inverting the flare energy equation to deduce the parameters of the supposed heating mechanism.

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