Convection in stars and heating of coronae

Details Convection in stars and heating of coronae Convection in stars and heating of coronae

Mar 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991iraj...20....1m&link_type=abstract

Irish Astronomical Journal (ISSN 0021-1052), vol. 20, March 1991, p. 1-25.

Computer Science

Sound

Atmospheric Heating, Convective Heat Transfer, Cool Stars, Solar Corona, Stellar Cores, Stellar Coronas, Computer Programs, Gas Flow, Mixing Length Flow Theory, Sound Waves, Stellar Magnetic Fields, Stellar Oscillations

Scientific paper

The properties of convection in the sun and other cool stars are summarized. Recent studies of convection which have involved the use of supercomputers to model the flow of compressible gas in three dimensions are discussed. It is shown how the results of these computations may eventualy provide an understanding of how nonthermal processes heat coronal gas to temperatures of millions of degrees.

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