Deriving Large Coronal Magnetic Loop Parameters Using LOFAR J Burst Observations (2023)
Attributed to:
Solar System Consolidated Grant 2022-25
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1007/s11207-022-02096-0
Publication URI: http://dx.doi.org/10.1007/s11207-022-02096-0
Type: Journal Article/Review
Parent Publication: Solar Physics
Issue: 1