Statistical relationship between CME speed and soft X-ray peak flux of the associated flare during solar cycle 23
में बचाया:
| लेखकों: | , , |
|---|---|
| स्वरूप: | comunicación de congreso |
| प्रकाशन तिथि: | 2014 |
| विवरण: | 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. |
| देश: | Kérwá |
| संस्थान: | Universidad de Costa Rica |
| Repositorio: | Kérwá |
| भाषा: | Inglés |
| OAI Identifier: | oai:kerwa.ucr.ac.cr:10669/100163 |
| ऑनलाइन पहुंच: | https://hdl.handle.net/10669/100163 https://doi.org/10.1017/S1743921313011678 |
| संकेत शब्द: | Coronal mass ejections flares X-ray emission |