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Solar System: A Model of the Magnetized Solar Wind

Published online by Cambridge University Press:  25 April 2016

I. H. Urch
I. H. Urch*
Affiliation:
Department of Physics, University of Adelaide
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Extract

Parker realized that the solar corona would expand into a supersonic wind, whose flow could be described by hydrodynamics. Subsequently a number of such steady state models have been developed which include the energy transport equation. These models assume that the heating of the gas is confined to a thin shell at the base of the corona, but neglect the effects of solar rotation and the general magnetic field, which is carried into space by the solar wind.

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 1 , Issue 5 , March 1969 , pp. 198 - 199
Copyright
Copyright © Astronomical Society of Australia 1969

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References

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