Sorba, AM;
Achilleos, NA;
Guio, P;
Arridge, CS;
Pilkington, NM;
Masters, A;
Sergis, N;
... Dougherty, MK; + view all
(2017)
Modeling the compressibility of Saturn's magnetosphere in response to internal and external influences.
Journal of Geophysical Research: Space Physics
, 122
(2)
pp. 1572-1589.
10.1002/2016JA023544.
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Abstract
The location of a planetary magnetopause is principally determined by the balance between solar wind dynamic pressure DP and magnetic and plasma pressures inside the magnetopause boundary. Previous empirical studies assumed that Saturn's magnetopause stand-off distance varies as math formula, and measured a constant compressibility parameter α corresponding to behavior intermediate between a vacuum dipole appropriate for Earth (α≈6), and a more easily compressible case appropriate for Jupiter (α≈4). In this study we employ a 2D force-balance model of Saturn's magnetosphere to investigate magnetospheric compressibility in response to changes in DP and global hot plasma content. For hot plasma levels compatible with Saturn observations, we model the magnetosphere at a range of stand-off distances and estimate the corresponding DP values by assuming pressure balance across the magnetopause boundary. We find that for ‘average’ hot plasma levels, our estimates of α are not constant with DP, but vary from ∼4.8 for high DP conditions, when the magnetosphere is compressed (≤25RS), to ∼3.5 for low DP conditions. This corresponds to the magnetosphere becoming more easily compressible as it expands. We find that the global hot plasma content influences magnetospheric compressibility even at fixed DP, with α estimates ranging from ∼5.4 to ∼3.3 across the range of our parameterized hot plasma content. We suggest that this behavior is predominantly driven by reconfiguration of the magnetospheric magnetic field into a more disk-like structure under such conditions. In a broader context, the compressibility of the magnetopause reveals information about global stress balance in the magnetosphere.
| Type: | Article |
|---|---|
| Title: | Modeling the compressibility of Saturn's magnetosphere in response to internal and external influences |
| Open access status: | An open access version is available from UCL Discovery |
| DOI: | 10.1002/2016JA023544 |
| Publisher version: | http://dx.doi.org/10.1002/2016JA023544 |
| Language: | English |
| Additional information: | ©2017. 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 Physics and Astronomy UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Space and Climate Physics |
| URI: | https://discovery.ucl.ac.uk/id/eprint/1538777 |
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