Statistical relationship between CME speed and soft X-ray peak flux of the associated flare during solar cycle 23
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| Autorzy: | , , |
|---|---|
| Format: | comunicación de congreso |
| Data wydania: | 2014 |
| Opis: | 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. |
| Kraj: | Kérwá |
| Instytucja: | Universidad de Costa Rica |
| Repositorio: | Kérwá |
| Język: | Inglés |
| OAI Identifier: | oai:kerwa.ucr.ac.cr:10669/100163 |
| Dostęp online: | https://hdl.handle.net/10669/100163 https://doi.org/10.1017/S1743921313011678 |
| Słowo kluczowe: | Coronal mass ejections flares X-ray emission |