A gas dynamic model of the rotating solar atmosphere

Details A gas dynamic model of the rotating solar atmosphere A gas dynamic model of the rotating solar atmosphere

Dec 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991soph..136..263n&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 136, Dec. 1991, p. 263-268.

Physics

1

Atmospheric Models, Gas Dynamics, Solar Atmosphere, Solar Rotation, Atmospheric Temperature, Mach Number, Shock Heating

Scientific paper

A model is presented of a solar atmosphere which is heated by the periodic passage of shock waves. The outer atmosphere rotates and is assumed not to affect the strength of the shock waves. This constant shock strength hypothesis is used as the basis of the model of the outer solar atmosphere. From the model it is concluded that the chromospheric temperature rise and flow Mach number are slightly affected by the rotation of the atmosphere.

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