Physical processes determining the chromospheric temperature distribution

Details Physical processes determining the chromospheric temperature distribution Physical processes determining the chromospheric temperature distribution

Feb 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977soph...51...51j&link_type=abstract

Solar Physics, vol. 51, Jan.-Feb. 1977, p. 51-59.

Computer Science

Sound

12

Chromosphere, Solar Physics, Solar Temperature, Acoustic Propagation, Shock Heating, Sound Waves, Stellar Models

Scientific paper

It is demonstrated that short period acoustic waves appear adequate to heat the low chromosphere in the region just above the temperature minimum, these waves are unlikely to provide sufficient energy to heat the chromosphere above tau-5000 A(normal) less than 10 to the -6th. Calculations also show that the electron density to H density ratio from chromospheric models is too low for the H2 molecule to affect the population of H(-).

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