Particle Acceleration Due to Coronal Non-null Magnetic Reconnection. (2017)
Attributed to:
Solar and Magnetospheric Plasma Theory
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1007/s11207-017-1060-0
PubMed Identifier: 32226172
Publication URI: http://europepmc.org/abstract/MED/32226172
Type: Journal Article/Review
Volume: 292
Parent Publication: Solar physics
Issue: 3
ISSN: 0038-0938