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Solar Activity Monitoring of Flares and CMEs Precursors through Lyman-Alpha Imaging and Tracking of Filaments and Prominences

Published online by Cambridge University Press:  06 January 2014

Luc Damé  and
Safinaz A. Khaled
Luc Damé
Affiliation:
LATMOS/IPSL/CNRS/UVSQ, 11 Boulevard d'Alembert, 78280 Guyancourt, France email: luc.dame@latmos.ipsl.fr
Safinaz A. Khaled
Affiliation:
LATMOS/IPSL/CNRS/UVSQ, 11 Boulevard d'Alembert, 78280 Guyancourt, France email: luc.dame@latmos.ipsl.fr Space Weather Monitoring Center, Helwan University, Helwan, Egypt email: safinaz_1986@yahoo.com
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Abstract

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We investigate the advantages of imaging solar filaments and prominences in Lyman-Alpha, coupled to H-Alpha on ground, to develop more reliable precursors indicators for large flares, several hours before their occurrence.

Keywords

Solar flaresfilamentsultraviolet
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. 523 - 524
Copyright
Copyright © International Astronomical Union 2013 

References

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