Depth of the dynamo region and zonal circulation of the molecular layer in Saturn inferred from its equatorially symmetric gravitational field (2019)
Attributed to:
Magnetism and Fluid Flows in our Solar-Planetary Environment
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1093/mnras/stz2019
Publication URI: http://dx.doi.org/10.1093/mnras/stz2019
Type: Journal Article/Review
Parent Publication: Monthly Notices of the Royal Astronomical Society
Issue: 4