A Computationally Efficient, Time-Dependent Model of the Solar Wind for Use as a Surrogate to Three-Dimensional Numerical Magnetohydrodynamic Simulations (2020)
Attributed to:
Reading Solar System Science
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1007/s11207-020-01605-3
Publication URI: http://dx.doi.org/10.1007/s11207-020-01605-3
Type: Journal Article/Review
Parent Publication: Solar Physics
Issue: 3