Driving of the solar p-modes by radiative pumping in the upper photosphere

Details Driving of the solar p-modes by radiative pumping in the upper photosphere Driving of the solar p-modes by radiative pumping in the upper photosphere

Jan 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990aipc..198..218f&link_type=abstract

IN: Astrophysics in Antarctica (A92-22401 07-89). New York, American Institute of Physics, 1989, p. 218-221. Research supported

Physics

2

Photosphere, Radiant Heating, Radiative Heat Transfer, Solar Atmosphere, Solar Oscillations, Solar Physics, Relaxation Time, Solar Flux

Scientific paper

It is shown that one viable driver of the solar p-modes is radiative pumping in the upper photosphere where the opacity is dominated by the negative hydrogen ion. This new option is suggested by the similar magnitudes of two energy flows that have been evaluated by independent empirical methods. The similarity indicates that the p-modes are radiatively pumped in the upper photosphere and therefore provide the required nonradiative cooling.

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