Plasma Upflows Induced by Magnetic Reconnection Above an Eruptive Flux Rope (2021)
Attributed to:
How do weak shocks accelerate high energy particles?
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1007/s11207-021-01849-7
Publication URI: http://dx.doi.org/10.1007/s11207-021-01849-7
Type: Journal Article/Review
Parent Publication: Solar Physics
Issue: 6