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The dependence of MHD turbulence spectra on the inner solar wind stream structure near solar minimum

โœ Scribed by Tu, C.-Y.; Marsch, E.; Rosenbauer, H.

Book ID
119708925
Publisher
American Geophysical Union
Year
1990
Tongue
English
Weight
433 KB
Volume
17
Category
Article
ISSN
1944-8007

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๐Ÿ“œ SIMILAR VOLUMES

On the effect of latitude dependent base
On the effect of latitude dependent base conditions on the structure of the solar wind
โœ I. W. Roxburgh; C. Singer ๐Ÿ“‚ Article ๐Ÿ“… 1975 ๐Ÿ› Springer ๐ŸŒ English โš– 224 KB

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