Optimization of Saturn paraboloid magnetospheric field model parameters using Cassini equatorial magnetic field data
The paraboloid model of Saturn's magnetosphere describes the magnetic field as being due to the sum of contributions from the internal field of the planet, the ring current, and the tail current, all contained by surface currents inside a magnetopause boundary which is taken to be a paraboloid o...
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| Principais autores: | , , , , , , , |
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| Formato: | Artigo |
| Idioma: | Inglês |
| Publicado em: |
Copernicus Publications
2016-07-01
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| coleção: | Annales Geophysicae |
| Acesso em linha: | https://www.ann-geophys.net/34/641/2016/angeo-34-641-2016.pdf |
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