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Solar wind: The quasi-radial approximation and its limitations

โœ Scribed by S. T. Suess; S. F. Nerney


Book ID
104649952
Publisher
Springer
Year
1975
Tongue
English
Weight
496 KB
Volume
40
Category
Article
ISSN
0038-0938

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โœฆ Synopsis


The mathematical basis for approximating the solar wind expansion as nearly radial is examined and defined, removing earlier restrictions thought to occur in the presence of a magnetic field and large variations in latitude. The equations and side conditions governing quasi-radial flow are derived and solved for a simple example to illustrate how this technique can be used for global models of the solar wind.


๐Ÿ“œ SIMILAR VOLUMES


Restrictions on radial magnetic field an
โœ M. S. Gussenhoven; R. L. Carovillano ๐Ÿ“‚ Article ๐Ÿ“… 1973 ๐Ÿ› Springer ๐ŸŒ English โš– 383 KB

In Parker's original model, the solar wind is represented as a spherically symmetric hydrodynamic flow. The velocity is radially directed and decoupled from the magnetic field. The simple extension of this model to include a dependence on the polar angle, 0, is shown to be invalid for radial flow an