An empirical model of Saturn's bow shock: Cassini observations of shock location and shape

Author:

Masters A.1,Achilleos N.2,Dougherty M. K.1,Slavin J. A.3,Hospodarsky G. B.4,Arridge C. S.56,Coates A. J.56

Affiliation:

1. Space and Atmospheric Physics Group, The Blackett Laboratory; Imperial College London; London UK

2. Atmospheric Physics Laboratory, Department of Physics and Astronomy; University College London; London UK

3. Heliophysics Science Division; NASA GSFC; Greenbelt Maryland USA

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

5. Mullard Space Science Laboratory, Department of Space and Climate Physics; University College London; Dorking UK

6. Centre for Planetary Sciences; University College London; London UK

Publisher

American Geophysical Union (AGU)

Subject

Paleontology,Space and Planetary Science,Earth and Planetary Sciences (miscellaneous),Atmospheric Science,Earth-Surface Processes,Geochemistry and Petrology,Soil Science,Water Science and Technology,Ecology,Aquatic Science,Forestry,Oceanography,Geophysics

Reference60 articles.

1. Orientation, location and velocity of Saturn's bow shock: Initial results from the Cassini spacecraft;Achilleos;J. Geophys. Res.,2006

2. Large-scale dynamics of Saturn's magnetopause: Observations by Cassini;Achilleos;J. Geophys. Res.,2008

3. The magnetic field of Saturn: Pioneer 11 observations;Acuña;Science,1980

4. Arridge , C. S. 2007 On the configuration and dynamics of Saturn's magnetosphere Univ. of London London, U.K.

5. Modeling the size and shape of Saturn's magnetopause with variable dynamic pressure;Arridge;J. Geophys. Res.,2006

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