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

dc.creator	Salas Matamoros, Carolina
dc.creator	Klein, Karl Ludwig
dc.creator	Taliashvili Enacolopas, Lela
dc.date.accessioned	2024-11-27T21:12:57Z
dc.date.available	2024-11-27T21:12:57Z
dc.date.issued	2014-01-06
dc.description.abstract	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.
dc.description.procedence	UCR::Vicerrectoría de Docencia::Ciencias Básicas::Facultad de Ciencias::Escuela de Física
dc.identifier.doi	https://doi.org/10.1017/S1743921313011678
dc.identifier.issn	1743-9213
dc.identifier.issn	1743-9221
dc.identifier.uri	https://hdl.handle.net/10669/100163
dc.language.iso	eng
dc.rights	acceso embargado
dc.source	Proceedings of the International Astronomical Union, 8(S300), 487–488
dc.subject	Coronal mass ejections
dc.subject	flares
dc.subject	X-ray emission
dc.title	Statistical relationship between CME speed and soft X-ray peak flux of the associated flare during solar cycle 23
dc.type	comunicación de congreso

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