Time dependent effects at the foot of the chromosphere

Details Time dependent effects at the foot of the chromosphere Time dependent effects at the foot of the chromosphere

Nov 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984sao..reptq....k&link_type=abstract

Final Report Smithsonian Astrophysical Observatory, Cambridge, MA.

Astronomy and Astrophysics

Astrophysics

Chromosphere, Stellar Models, Sun, Time Dependence, Magnetohydrodynamic Waves, Plane Waves, Solar Atmosphere, Solar Temperature

Scientific paper

A dynamical model was proposed which is in agreement with the observations that suggest the solar chromosphere is heated preferentially in magnetic regions. The dynamical model requires an energy flux that is large enough to lead to amplitudes for which the apparent temperatures match the empirical line temperatures in the UTV lines. Consistency with the observations of chromospheric emission then requires that the emission take place not uniformly over the solar surface but in smaller spatial regions.

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