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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
Affiliation:
Space Research Center, University of Costa Rica (CINESPA) email: [email protected]
K.-L. Klein
Affiliation:
LESIA - UMR 8109, Observatoire de Paris, CNRS, Univ. Paris 6 & 7 email: [email protected]
L. Taliashvili
Affiliation:
Space Research Center, University of Costa Rica (CINESPA) email: [email protected]
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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.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2013 

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