Solar system plasmas are highly structured and dynamic and are characterized by great variability in both space and time. The variations in their spatial distribution and temporal evolution occur on a variety of scales, ranging from kilometers (ion gyroradius) to hundreds of thousands of kilometers
โฆ LIBER โฆ
Plasma and magnetic fields in the solar system
โ Scribed by Gold, Thomas
- Book ID
- 119722949
- Publisher
- American Geophysical Union
- Year
- 1959
- Tongue
- English
- Weight
- 582 KB
- Volume
- 64
- Category
- Article
- ISSN
- 0148-0227
No coin nor oath required. For personal study only.
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The connection between the magnetic field geometry and the thermal properties of solar coronal structures is investigated. Gravitational effects, that can modify the spatial dependence of the thermodynamical quantities, but have no influence on the plasma-field interaction, are omitted to simplify t