Comparison between GOES flares, SOHO/LASCO CMEs and RSTN 1.4 GHz solar radio bursts
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 associate...
| Autores: | , |
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| Formato: | conjunto de datos |
| Estado: | Versión publicada |
| Fecha de publicación: | 2020 |
| País: | España |
| Recursos: | Consorcio Madroño |
| Repositorio: | e-cienciaDatos, Repositorio de Datos del Consorcio Madroño |
| OAI Identifier: | doi:10.21950/PPD8ZW |
| Acesso em linha: | https://doi.org/10.21950/PPD8ZW |
| Access Level: | acceso abierto |
| Palavra-chave: | Astronomy and Astrophysics Earth and Environmental Sciences Solar radio bursts Solar flares Coronal mass ejections Space weather |
| Resumo: | 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. |
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