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)
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