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Large-Scale Structure in the Magnetospheres of Jupiter and Saturn

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Part of the book series: IAGA Special Sopron Book Series ((IAGA,volume 3))

Abstract

The magnetospheres surrounding Jupiter and Saturn are unique in the solar system because of their important internal plasma sources, rapid planetary rotation and strong magnetosphere-ionosphere coupling, the prevailing solar wind conditions, and the complex multi-phase and multi-species nature of their magnetospheric plasma and neutral environments. In this chapter the large-scale structure of the jovian and saturnian magnetospheres will be reviewed. The physical origins of this structure will be examined and we discuss dynamical and periodic modulations within each system and their responses to internal and external perturbations.

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Acknowledgements

CSA was funded by an STFC postdoctoral fellowship under grant ST/G007462/1 and the STFC rolling grant to MSSL/UCL. CSA thanks Nick Achilleos, Fran Bagenal, Stan Cowley, Michele Dougherty, Caitríona Jackman, Margy Kivelson, Krishan Khurana, Chris Russell, Beth Semikin, David Southwood, and the Cassini CAPS, MAG, MIMI and RPWS teams for insightful discussions and comments on the manuscript, and both reviewers for useful comments.

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Correspondence to Christopher S. Arridge .

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Arridge, C.S. (2011). Large-Scale Structure in the Magnetospheres of Jupiter and Saturn. In: Liu, W., Fujimoto, M. (eds) The Dynamic Magnetosphere. IAGA Special Sopron Book Series, vol 3. Springer, Dordrecht. https://doi.org/10.1007/978-94-007-0501-2_19

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