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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 (2008)

First Author: Belenkaya E

Attributed to: Rolling Grant Support for a Programme of Research in Solar-Planetary and Atmospheric Physics at the University of Leicester funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.5194/angeo-26-159-2008

Publication URI: http://dx.doi.org/10.5194/angeo-26-159-2008

Type: Journal Article/Review

Parent Publication: Annales Geophysicae

Issue: 1