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Note on the solar wind heating (two fluid models)

โœ Scribed by S. Cuperman

Publisher
Springer Netherlands
Year
1973
Tongue
English
Weight
98 KB
Volume
20
Category
Article
ISSN
0004-640X

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๐Ÿ“œ SIMILAR VOLUMES

A two-fluid solar wind model with anisot
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A two-fluid model of the solar wind with anisotropic proton temperature and allowing for extended coronal proton-heating is considered for the case of a purely radial and of a spiral magnetic field. Proton-proton Coulomb-collisions together with a spiral interplanetary magnetic field are found to be

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The two-fluid equations for the solar wind are written down in a simplified form, similar to that suggested by Roberts (1971) for the one-fluid model. The equations are shown to depend only on one parameter, where G is the gravitational constant, M the mass of the star, xe the thermal electron cond

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A simple model of the lower corona which allows for a possible difference in the electron and proton temperatures is analyzed. With the introduction of a phenomenological heating term, temperature and density profiles are calculated for several different cases. It is found that, under certain circum