Statistical relationship between CME speed and soft X-ray peak flux of the associated flare during solar cycle 23
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| Autores: | , , |
|---|---|
| פורמט: | comunicación de congreso |
| Fecha de Publicación: | 2014 |
| תיאור: | 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 |
| מוסד: | Universidad de Costa Rica |
| Repositorio: | Kérwá |
| שפה: | Inglés |
| OAI Identifier: | oai:kerwa.ucr.ac.cr:10669/100163 |
| גישה מקוונת: | https://hdl.handle.net/10669/100163 https://doi.org/10.1017/S1743921313011678 |
| מילת מפתח: | Coronal mass ejections flares X-ray emission |