Solar wind dynamic pressure and electric field as the main factors controlling Saturn's aurorae-Reference-Cited by-同舟云学术

Solar wind dynamic pressure and electric field as the main factors controlling Saturn's aurorae

Published:2005-02 Issue:7027 Volume:433 Page:720-722
ISSN:0028-0836
Container-title:Nature
language:en
Short-container-title:Nature

Author:

Crary F. J.,Clarke J. T.,Dougherty M. K.,Hanlon P. G.,Hansen K. C.,Steinberg J. T.,Barraclough B. L.,Coates A. J.,Gérard J.-C.,Grodent D.,Kurth W. S.,Mitchell D. G.,Rymer A. M.,Young D. T.

Publisher

Springer Science and Business Media LLC

Subject

Multidisciplinary

Link

http://www.nature.com/articles/nature03333.pdf

Reference18 articles.

1. Dungey, J. W. Interplanetary magnetic field and the auroral zone. Phys. Rev. Lett. 6, 47–48 (1961)

2. Hill, T. W., Dessler, A. J. & Goertz, C. K. in Physics of the Jovian Magnetosphere (ed. Dessler, A. J.) 353–394 (Cambridge Univ. Press, Cambridge, 1983)

3. Clarke, J. T. et al. Morphological differences of Saturn's ultraviolet aurorae and those of Earth and Jupiter. Nature doi:10.1038/nature03331 (this issue)

4. Meurant, M., Gerard, J.-C., Blockx, C., Hubert, B. & Coumans, V. Propagation of electron and proton shock-induced aurora and the role of the interplanetary magnetic field and solar wind. J. Geophys. Res. 109, A10210, doi:10.1029/2004JA010453 (2004)

5. Cowley, S. W. H. & Bunce, E. J. Origin of the main auroral oval in Jupiter's coupled magnetosphere-ionosphere system. Planet. Space Sci. 49, 1067–1088 (2001)

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