Properties of local plasma injections in Saturn's magnetosphere-Reference-Cited by-同舟云学术

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Properties of local plasma injections in Saturn's magnetosphere

Published:2005-06-01 Issue:14 Volume:32 Page:n/a-n/a
ISSN:0094-8276
Container-title:Geophysical Research Letters
language:en
Short-container-title:Geophys. Res. Lett.

Author:

Burch J. L.¹,Goldstein J.¹,Hill T. W.²,Young D. T.¹,Crary F. J.¹,Coates A. J.³,André N.⁴,Kurth W. S.⁵,Sittler E. C.⁶

Affiliation:

1. Southwest Research Institute; San Antonio; Texas; USA

2. Rice University; Department of Physics and Astronomy; Houston; Texas; USA

3. Mullard Space Science Lab; University College London; Dorking, Surrey; U. K.

4. Centre d'Etude Spatiale des Rayonnements; Toulouse; France

5. University of Iowa; Department of Physics and Astronomy; Iowa City; Iowa; USA

6. NASA, Goddard Space Flight Center; Greenbelt; Maryland; USA

Publisher

American Geophysical Union (AGU)

Subject

General Earth and Planetary Sciences,Geophysics

Reference12 articles.

1. The centrifugal flute instability and the generation of Saturn kilometric radiation;Curtis;J. Geophys. Res.,1986

2. The Cassini radio and plasma wave science investigation;Gurnett;Space Sci. Rev.,2004

3. Interchange stability of a rapidly rotating magnetosphere;Hill;Planet. Space Sci.,1976

4. Corotating magnetospheric convection;Hill;J. Geophys. Res.,1981

5. Evidence for rotationally driven plasma transport in Saturn's magnetosphere;Hill;Geophys. Res. Lett.,2005

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