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Depth of the dynamo region and zonal circulation of the molecular layer in Saturn inferred from its equatorially symmetric gravitational field (2019)

First Author: Kong D

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