An optimization principle for computing stationary MHD equilibria with solar wind flow (2020)
Attributed to:
Solar and Magnetospheric Magnetohydrodynamics and Plasmas: Theory and Application
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.5194/egusphere-egu2020-3029
Publication URI: http://dx.doi.org/10.5194/egusphere-egu2020-3029
Type: Other