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