Ultraviolet emissions from the magnetic footprints of Io, Ganymede and Europa on Jupiter-Reference-Cited by-同舟云学术

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Ultraviolet emissions from the magnetic footprints of Io, Ganymede and Europa on Jupiter

Published:2002-02 Issue:6875 Volume:415 Page:997-1000
ISSN:0028-0836
Container-title:Nature
language:en
Short-container-title:Nature

Author:

Clarke J. T.,Ajello J.,Ballester G.,Ben Jaffel L.,Connerney J.,Gérard J.-C.,Gladstone G. R.,Grodent D.,Pryor W.,Trauger J.,Waite J. H.

Publisher

Springer Science and Business Media LLC

Subject

Multidisciplinary

Link

http://www.nature.com/articles/415997a.pdf

Reference25 articles.

1. Connerney, J. E. P. et al. Images of excited H+3 at the foot of the Io flux tube in Jupiter's atmosphere. Science 262, 1035–1038 (1993).

2. Clarke, J. T. et al. Far-ultraviolet imaging of Jupiter's aurora and the Io “footprint”. Science 274, 404–409 (1996).

3. Prangé, R. et al. Rapid energy dissipation and variability of the Io–Jupiter electrodynamic circuit. Nature 379, 323–325 (1996).

4. Goldreich, P. & Lynden-Bell, D. Io, a Jovian unipolar inductor. Astrophys. J. 156, 59–78 (1969).

5. Belcher, J. W. The Jupiter–Io connection, an Alfven engine in space. Science 238, 170–176 (1987).

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