Statistical relationship between CME speed and soft X-ray peak flux of the associated flare during solar cycle 23
Kaydedildi:
| Yazarlar: | , , |
|---|---|
| Materyal Türü: | comunicación de congreso |
| Yayın Tarihi: | 2014 |
| Diğer Bilgiler: | 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. |
| Ülke: | Kérwá |
| Kurum: | Universidad de Costa Rica |
| Repositorio: | Kérwá |
| Dil: | Inglés |
| OAI Identifier: | oai:kerwa.ucr.ac.cr:10669/100163 |
| Online Erişim: | https://hdl.handle.net/10669/100163 https://doi.org/10.1017/S1743921313011678 |
| Anahtar Kelime: | Coronal mass ejections flares X-ray emission |