Thermospheric signature of magnetospheric energy dissipation
✍ Scribed by G.W. Prölss
- Publisher
- Elsevier Science
- Year
- 1981
- Tongue
- English
- Weight
- 282 KB
- Volume
- 1
- Category
- Article
- ISSN
- 0273-1177
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Major geomagnetic storms represent a signiÿcant dissipation of energy by the magnetosphere. The energy is derived from the solar wind ow and the subsequent powerful conversion of that energy takes several di erent forms. Ring current injection and decay, ionospheric Joule heating, particle precipita
In previous experimental investigations of the hypothesis of a lognormal distribution of kinetic-energy dissipation proposed by Kolmogorov and Obukhov in 1962, approximations for the dissipation of kinetic energy were used. By using special measuring equipment, these approximations could be avoided