Please use this identifier to cite or link to this item: http://hdl.handle.net/2381/38309
Title: Dependence of the open-closed field line boundary in Saturn's ionosphere on both the IMF and solar wind dynamic pressure: comparison with the UV auroral oval observed by the HST
Authors: Belenkaya, E. S.
Cowley, S. W. H.
Badman, S. V.
Blokhina, M. S.
Kalegaev, V. V.
First Published: 4-Feb-2008
Publisher: European Geosciences Union (EGU), Copernicus Publications, Springer Verlag
Citation: Annales Geophysicae, 2008, 26 (1), pp. 159-166 (8)
Abstract: We model the open magnetic field region in Saturn's southern polar ionosphere during two compression regions observed by the Cassini spacecraft upstream of Saturn in January 2004, and compare these with the auroral ovals observed simultaneously in ultraviolet images obtained by the Hubble Space Telescope. The modelling employs the paraboloid model of Saturn's magnetospheric magnetic field, whose parameters are varied according to the observed values of both the solar wind dynamic pressure and the interplanetary magnetic field (IMF) vector. It is shown that the open field area responds strongly to the IMF vector for both expanded and compressed magnetic models, corresponding to low and high dynamic pressure, respectively. It is also shown that the computed open field region agrees with the poleward boundary of the auroras as well as or better than those derived previously from a model in which only the variation of the IMF vector was taken into account. The results again support the hypothesis that the auroral oval at Saturn is associated with the open-closed field line boundary and hence with the solar wind interaction.
DOI Link: 10.5194/angeo-26-159-2008
ISSN: 0992-7689
eISSN: 1432-0576
Links: http://www.ann-geophys.net/26/159/2008/
http://hdl.handle.net/2381/38309
Version: Publisher Version
Status: Peer-reviewed
Type: Journal Article
Rights: © Author(s) 2008. This work is distributed under the Creative Commons Attribution 3.0 License.
Appears in Collections:Published Articles, Dept. of Physics and Astronomy

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