Statistical relationship between CME speed and soft X-ray peak flux of the associated flare during solar cycle 23
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| Авторы: | , , |
|---|---|
| Формат: | comunicación de congreso |
| Дата публикации: | 2014 |
| Описание: | 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. |
| Страна: | Kérwá |
| Институт: | Universidad de Costa Rica |
| Repositorio: | Kérwá |
| Язык: | Inglés |
| OAI Identifier: | oai:kerwa.ucr.ac.cr:10669/100163 |
| Online-ссылка: | https://hdl.handle.net/10669/100163 https://doi.org/10.1017/S1743921313011678 |
| Ключевое слово: | Coronal mass ejections flares X-ray emission |