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Flux transfer event observation at Saturn's dayside magnetopause by the Cassini spacecraft

Jasinski, JM; Slavin, JA; Arridge, CS; Poh, G; Jia, X; Sergis, N; Coates, AJ; ... Waite, JH; + view all (2016) Flux transfer event observation at Saturn's dayside magnetopause by the Cassini spacecraft. Geophysical Research Letters , 43 (13) pp. 6713-6723. 10.1002/2016GL069260. Green open access

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Abstract

We present the first observation of a flux rope at Saturn's dayside magnetopause. This is an important result because it shows that the Saturnian magnetopause is conducive to multiple X-line reconnection and flux rope generation. Minimum variance analysis shows that the magnetic signature is consistent with a flux rope. The magnetic observations were well fitted to a constant-α force-free flux rope model. The radius and magnetic flux content of the rope are estimated to be 4600-8300 km and 0.2-0.8 MWb, respectively. Cassini also observed five traveling compression regions (remote signatures of flux ropes), in the adjacent magnetosphere. The magnetic flux content is compared to other estimates of flux opening via reconnection at Saturn.

Type: Article
Title: Flux transfer event observation at Saturn's dayside magnetopause by the Cassini spacecraft
Open access status: An open access version is available from UCL Discovery
DOI: 10.1002/2016GL069260
Publisher version: http://dx.doi.org/10.1002/2016GL069260
Additional information: © 2016 The Authors. This is an open access article under the terms of the Creative Commons Attribution License, which permits use, distribution and reproduction in any medium, provided the original work is properly cited.
UCL classification: UCL
UCL > Provost and Vice Provost Offices > UCL BEAMS
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Space and Climate Physics
URI: https://discovery-pp.ucl.ac.uk/id/eprint/1498350
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