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

Published online by Cambridge University Press:  06 January 2014

C. Salas-Matamoros ,
K.-L. Klein  and
L. Taliashvili
C. Salas-Matamoros
Affiliation:
Space Research Center, University of Costa Rica (CINESPA) email: carolina.salas@planetario.ucr.ac.cr
K.-L. Klein
Affiliation:
LESIA - UMR 8109, Observatoire de Paris, CNRS, Univ. Paris 6 & 7 email: ludwig.klein@obspm.fr
L. Taliashvili
Affiliation:
Space Research Center, University of Costa Rica (CINESPA) email: carolina.salas@planetario.ucr.ac.cr
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Abstract

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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.

Keywords

Coronal mass ejectionsflaresX-ray emission
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S300: Nature of Prominences and their role in Space Weather , June 2013 , pp. 487 - 488
Copyright
Copyright © International Astronomical Union 2013 

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