Statistical relationship between CME speed and soft X-ray peak flux of the associated flare during solar cycle 23

 

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Detaylı Bibliyografya
Yazarlar: Salas Matamoros, Carolina, Klein, Karl Ludwig, Taliashvili Enacolopas, Lela
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