Comparison between GOES flares, SOHO/LASCO CMEs and RSTN 1.4 GHz solar radio bursts

  1. Flores-Soriano, Manuel 1
  2. Cid Tortuero, Consuelo 1
  1. 1 (UAH)

Éditeur: e-cienciaDatos

Année de publication: 2020

Type: Dataset

DOI: 10.21950/PPD8ZW lock_openAccès ouvert editor

Résumé

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.