Deriving Large Coronal Magnetic Loop Parameters Using LOFAR J burst Observations (2022)
Attributed to:
Solar System Consolidated Grant 2022-25
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.48550/arxiv.2212.02161
Publication URI: https://arxiv.org/abs/2212.02161
Type: Other