Event calendar file
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The GLE of December 13, 2006 according to the ground level and balloon observations
Speakers
- Mr. Eduard VASHENYUK
Primary authors
- Mr. Eduard VASHENYUK (Polar Geophysical Institute of RAS)
Co-authors
- Ms. Galina BAZILEVSKAYA (Lebedev Physical Institute of RAS)
- Mr. Vladimir MAKHMUTOV (Lebedev Physical Institute of RAS)
- Mr. Yury STOZHKOV (Lebedev Physical Institute of RAS)
- Mr. Nicolay SVIRZHEVSKY (Lebedev Physical Institute of RAS)
- Ms. Albina SVIRZHEVSKAYA (Lebedev Physical Institute of RAS)
- Mr. Yury BALABIN (Polar Geophysical Institute of RAS)
- Mr. Boris GVOZDEVSKY (Polar Geophysical Institute of RAS)
- Leonid SCHUR (Polar Geophysical Institute of RAS)
Files
Abstract content
The analysis of the GLE 13.12.2006 using the data of neutron monitors, balloons, and modeling computations has been carried out. The event was connected to the flare and appeared rather unexpected, as it occurred during the ongoing phase of solar minimum. The characteristics of relativistic solar protons were derived by modeling technique from the neutron monitors data. The direct solar proton data obtained by balloons in Apatity and Mirny (Antarctica) allowed to extend the energetic spectra derived from ground based measurements from relativistic to moderate energies (hundreds MeV). The dynamics of solar proton spectra and pitch-angular distributions during the event is investigated.
Reference
Proceedings of the 30th International Cosmic Ray Conference; Rogelio Caballero, Juan Carlos D'Olivo, Gustavo Medina-Tanco, Lukas Nellen, Federico A. Sánchez, José F. Valdés-Galicia (eds.); Universidad Nacional Autónoma de México, Mexico City, Mexico, 2008; Vol. 1 (SH), pages 221-224
