Comparison between GOES flares, SOHO/LASCO CMEs and RSTN 1.4 GHz solar radio bursts
- 1 (UAH)
Editor: e-cienciaDatos
Year of publication: 2020
Type: Dataset
DOI:
10.21950/PPD8ZW
lock_openOpen access editor
Abstract
Study 1.4 GHz solar radio bursts as counterparts to coronal mass ejections. For a list of GOES X-ray flares of class M5 or higher, this dataset provides the time integral of their associated 1.4 GHz solar radio burst and compares them with the speed, angular width and kinetic energy of the associated CME, if any.