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How does the Sun influence the magnetospheres of Jupiter and Saturn?

How does the Sun influence the magnetospheres of Jupiter and Saturn?
How does the Sun influence the magnetospheres of Jupiter and Saturn?
Spacecraft have visited Jupiter and Saturn at all phases of the solar cycle and thus we have a wealth of data with which to explore both upstream parameters and magnetospheric response. In this paper we review upstream parameters including interplanetary magnetic field strength and direction, solar wind dynamic pressure, plasma beta and Mach number. We consider the impact of changing solar wind on dayside coupling via reconnection. We also comment on how solar UV flux variability over a solar cycle influences the plasma and neutral tori in the inner magnetospheres of Jupiter and Saturn, and thus estimate the solar cycle effects on internally driven magnetospheric dynamics. Finally we place our results in the context of the now complete set of data from the Cassini mission at Saturn and the current data streaming in from Juno at Jupiter, outlining future avenues for research.
1743-9213
109-113
Jackman, Caitriona
9bc3456c-b254-48f1-ade0-912c5b8b4529
Arridge, Christopher S.
cddea13c-2c2a-44c8-9607-309820a0fb0f
Jackman, Caitriona
9bc3456c-b254-48f1-ade0-912c5b8b4529
Arridge, Christopher S.
cddea13c-2c2a-44c8-9607-309820a0fb0f

Jackman, Caitriona and Arridge, Christopher S. (2017) How does the Sun influence the magnetospheres of Jupiter and Saturn? Proceedings of the International Astronomical Union, 13 (Symposium S335), 109-113. (doi:10.1017/S1743921317011620).

Record type: Article

Abstract

Spacecraft have visited Jupiter and Saturn at all phases of the solar cycle and thus we have a wealth of data with which to explore both upstream parameters and magnetospheric response. In this paper we review upstream parameters including interplanetary magnetic field strength and direction, solar wind dynamic pressure, plasma beta and Mach number. We consider the impact of changing solar wind on dayside coupling via reconnection. We also comment on how solar UV flux variability over a solar cycle influences the plasma and neutral tori in the inner magnetospheres of Jupiter and Saturn, and thus estimate the solar cycle effects on internally driven magnetospheric dynamics. Finally we place our results in the context of the now complete set of data from the Cassini mission at Saturn and the current data streaming in from Juno at Jupiter, outlining future avenues for research.

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Published date: July 2017

Identifiers

Local EPrints ID: 430258
URI: https://eprints.soton.ac.uk/id/eprint/430258
ISSN: 1743-9213
PURE UUID: 9c7f4f65-4f80-4b23-ab0c-164951f1e6da

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Date deposited: 23 Apr 2019 16:30
Last modified: 23 Apr 2019 16:30

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