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

  • Luc Damé (a1) and Safinaz A. Khaled (a1) (a2)

Abstract

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.

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References

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Damé, L., The SWUSV Team 2013, Journal of Adv. Research, 4, 235
Kretzschmar, M., Dominique, M., & Dammasch, I. E. 2013, Solar Phys., 286, 221
Labrosse, N., Heinzel, P., Vial, J.-C., Kucera, T., Parenti, S., Gunár, S., Schmieder, B., & Kilper, G. 2010, Space Sci. Rev., 151, 243
Mierla, M., Heinzel, P., Seaton, D. B., Berghmans, D., Chifu, I., De Groof, A., Inhester, B., Rodriguez, L., Stenborg, G., & Zhukov, A. N. 2013, Solar Phys., 286, 241
Milligan, R. O., Chamberlin, P., Hudson, H., Woods, T., Mathioudakis, M., Fletcher, L., Kowalski, A., & Keenan, F. 2011, ApJ., 748, L14
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