Does H/-/ truly cool the solar chromosphere

Details Does H/-/ truly cool the solar chromosphere Does H/-/ truly cool the solar chromosphere

Nov 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980soph...68..125a&link_type=abstract

Solar Physics, vol. 68, Nov. 1980, p. 125-133. NSF-sponsored research;

Physics

11

Atmospheric Heating, Chromosphere, Hydrogen Ions, Radiant Cooling, Solar Atmosphere, Atmospheric Models, Radiant Heating, Solar Physics, Thermodynamic Equilibrium

Scientific paper

The controversial problem of H(-) radiative cooling in the solar chromosphere is examined. It is found, in agreement with Praderie and Thomas (1972, 1976), that H(-) is a substantial source of radiative heating in the outer atmosphere, especially when departures from LTE are important. The role of H(-) as a chromospheric heating agent must be considered carefully before net radiative cooling rates can be assessed from empirical chromospheric models, or calculations of nonradiative heating, for example by acoustic waves, can be pursued meaningfully.

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