๐”– Bobbio Scriptorium
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On the effect of latitude dependent base conditions on the structure of the solar wind

โœ Scribed by I. W. Roxburgh; C. Singer

Publisher
Springer
Year
1975
Tongue
English
Weight
224 KB
Volume
41
Category
Article
ISSN
0038-0938

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โœฆ Synopsis

The isothermal solar wind equations are solved for the case where the coronal conditions vary with latitude. It is found that the solutions are not uniquely determined by the base density but require knowledge of the injection angle of the fluid. Even for the case of spherically symmetric density at the corona, the solutions are not unique and form a one parameter set, but the latitude variation decreases rapidly with increasing heliocentric distance. * This is also true of homentropic (uniform entropy) solution since in this case the relation T~ NZl 8 leads to an equation similar to (10) with again three well behaved asymptotic solutions.

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