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Influence of the Interplanetary Magnetic Field on the Solar Wind Flow about Planetary Obstacles

✍ Scribed by Nikolai Erkaev; Alexander Mezentsev; Helfried Biernat

Publisher
Springer Netherlands
Year
2006
Tongue
English
Weight
673 KB
Volume
122
Category
Article
ISSN
0038-6308

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πŸ“œ SIMILAR VOLUMES

Restrictions on radial magnetic field an
Restrictions on radial magnetic field and flow solutions for the solar wind
✍ 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

On the three-dimensional structure of th
On the three-dimensional structure of the solar magnetic field in interplanetary space
✍ Osamu Kaburaki; Yuzuru Yoshii πŸ“‚ Article πŸ“… 1979 πŸ› Springer 🌐 English βš– 487 KB

The three-dimensional structure of the solar magnetic field in the interplanetary space is inferred from a theoretical point of view. We use the magnetic field produced by a magnetic dipole rotating obliquely in vacuum. The correction for the presence of a plasma surrounding the Sun is taken into ac