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Solar wind properties at the Earth as predicted by the one-fluid model with helioclassical thermal electron conductivity

✍ Scribed by Durney, B. R.

Book ID: 119711428
Publisher: American Geophysical Union
Year: 1973
Tongue: English
Weight: 537 KB
Volume: 78
Category: Article
ISSN: 0148-0227
DOI: 10.1029/ja078i031p07229

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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