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

No abstract provided

Type: Journal Article/Review

Parent Publication: Annales Geophysicae

Issue: 1