Statistical relationship between CME speed and soft X-ray peak flux of the associated flare during solar cycle 23
Guardado en:
| Autores: | , , |
|---|---|
| 格式: | comunicación de congreso |
| Fecha de Publicación: | 2014 |
| 实物特征: | The relationship between the speed of coronal mass ejections and the peak soft X-ray flux of the associated flares is studied for events occurring near the solar limbs between 1996 and 2008. An improved, though still moderate, correlation between the two parameters is found. |
| País: | Kérwá |
| 机构: | Universidad de Costa Rica |
| Repositorio: | Kérwá |
| 语言: | Inglés |
| OAI Identifier: | oai:kerwa.ucr.ac.cr:10669/100163 |
| 在线阅读: | https://hdl.handle.net/10669/100163 https://doi.org/10.1017/S1743921313011678 |
| Palabra clave: | Coronal mass ejections flares X-ray emission |