3-11 July 2007
Merida, Mexico
Mexico/General timezone
- icrc2007@icrc2007.unam.mx
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Contribution Poster
Merida, Mexico
-
Regency (Hyatt)
HE.3.1
The halo and the high energy jet in stratospheric STRANA superfamily with E0>10^16 eV
Speakers
- Dr. Vladislav OSEDLO
Primary authors
- Dr. Vladislav OSEDLO (Skobeltsyn Institute of Nuclear Physics, Moscow State University)
Co-authors
- Dr. Tatiana ROGANOVA (Skobeltsyn Institute of Nuclear Physics, Moscow State University)
- Dr. Lyubov SVESHNIKOVA (Skobeltsyn Institute of Nuclear Physics, Moscow State University)
- Dr. Vladimir GALKIN (Skobeltsyn Institute of Physical Department of Moscow State University)
- Prof. Irina RAKOBOLSKAYA (Physical Department of Moscow State University)
- Ms. Ludmila GONCHAROVA (P.N.Lebedev Physical Institute, Academy of Sciences of Russia)
- Dr. Konstantin KOTELNIKOV (P.N.Lebedev Physical Institute, Academy of Sciences of Russia)
- Natalia POLUKHINA (P.N.Lebedev Physical Institute, Academy of Sciences of Russia)
- Dr. Alexander MANAGADZE (Skobeltsyn Institute of Nuclear Physics, Moscow State University)
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Abstract content
Gamma-hadron superfamily STRANA with E0 > 10^16 eV and unusual features was detected by emulsion chamber at the board of stratospheric balloon. In the center of the family there was found a halo. The halo and the high energy jet producing it in the chamber are analysed here.
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. 4 (HE part 1), pages 663-666