Heating in the solar mantle

Details Heating in the solar mantle Heating in the solar mantle

Jan 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985nascp2358..101c&link_type=abstract

In NASA. Goddard Space Flight Center The Origin of Nonradiative Heating/Momentum in Hot Stars p 101-105 (SEE N85-17755 08-88)

Physics

Chromosphere, Plasma Heating, Solar Atmosphere, Solar Corona, Solar Physics, Stellar Temperature, Energy Transfer, Magnetohydrodynamic Waves, Solar Magnetic Field, Stellar Models

Scientific paper

In the case of the solar chromosphere and corona (the solar mantle) the primary energy source is the mechanical energy from photospheric motions. Plenty of energy is available; the problem is to transfer the needed amount of energy to the proper place to account for the observations. The global problem is reviewed from the point of view of the generation and transmission of energy, the intermediate storage of energy, and the release of energy in such a way that the observed features are generated.

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