Redistribution of energy by vertical oscillations in the solar atmosphere

Details Redistribution of energy by vertical oscillations in the solar atmosphere Redistribution of energy by vertical oscillations in the solar atmosphere

Jun 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981soph...71..203t&link_type=abstract

Solar Physics, vol. 71, June 1981, p. 203-213.

Physics

2

Energy Distribution, Solar Atmosphere, Solar Corona, Solar Oscillations, Atmospheric Density, Atmospheric Heating, Atmospheric Models, Atmospheric Temperature, Boundary Value Problems, Energy Dissipation, Energy Sources, Mathematical Models

Scientific paper

The effect of vertical oscillations with periods between 90s and 300s on a solar atmosphere governed by heat conduction and radiation loss is examined. The effect is found to be primarily a redistribution, rather than a net addition or subtraction, of energy within the low corona, mainly by long period (180 to 300s) oscillations. The redistribution of energy is found to affect time-averaged temperature and density profiles of such an atmosphere, particularly in the low corona. The amount of energy redistributed is found to increase with increasing period.

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