The relationship of magnetic flux ropes to substorms
β Scribed by K.K Khurana; M.G Kivelson; L.A Frank
- Publisher
- Elsevier Science
- Year
- 1996
- Tongue
- English
- Weight
- 485 KB
- Volume
- 18
- Category
- Article
- ISSN
- 0273-1177
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π SIMILAR VOLUMES
Energy storage in chromospheric flux ropes is discussed, in the context of solar flares. The structure is represented by a cylindrically symmetric magnetic field of finite length. The field is assumed to be approximately force-free. The stability of the field to a kink perturbation is investigated.
Magnetic flux ropes are created in the ionosphere of Venus and Mars during the interaction of the solar wind with their ionospheres and also at Titan during the interaction of the Saturnian magnetospheric plasma flow with Titan's ionosphere. The flux ropes at Venus and Mars were extensively studied