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On the Magnetic Field Orientation and Plasma Flows in Solar Filament Barbs

✍ Scribed by Yuri E. Litvinenko


Book ID
110221933
Publisher
Springer
Year
2000
Tongue
English
Weight
43 KB
Volume
196
Category
Article
ISSN
0038-0938

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πŸ“œ SIMILAR VOLUMES


Restrictions on radial magnetic field an
✍ M. S. Gussenhoven; R. L. Carovillano πŸ“‚ Article πŸ“… 1973 πŸ› Springer 🌐 English βš– 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