Effects of Shell Thickness on Cross-Helicity Generation in Convection-Driven Spherical Dynamos (2020)

First Author: Silva L
Attributed to:  The Virgo consortium for cosmological supercomputer simulations funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.3390/fluids5040245

Publication URI: http://dx.doi.org/10.3390/fluids5040245

Type: Journal Article/Review

Parent Publication: Fluids

Issue: 4