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Energy spectrum for the solar neutron event of September 7 2005, derived from the SNT at Sierra Negra.
Speakers
- Dr. Luis Xavier GONZÁLEZ
Primary authors
- Dr. Luis Xavier GONZÁLEZ (Instituto de Geofísica, UNAM. México.)
Co-authors
- Dr. José Francisco VALDÉS-GALICIA (Instituto de Geofísica, UNAM. México.)
- Dr. Y. MURAKI (Solar-Terrestrial Environment Laboratory, Nagoya University, Japan.)
- Dr. T. SAKO (Solar-Terrestrial Environment Laboratory, Nagoya University, Japan.)
- Dr. K. WATANABE (Space Sciences Laboratory University of California, Berkeley, US.)
- Dr. Y. MATSUBARA (Solar-Terrestrial Environment Laboratory, Nagoya University, Japan.)
- Dr. S SHIBATA (College of Engineering, Chubu University, Japan.)
- Dr. T. SAKAI (College of Industrial Technologies, Nihon University, Japan.)
- Dr. H. TSUJIHARA (Solar-Terrestrial Environment Laboratory, Nagoya University, Japan.)
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Abstract content
The Solar Neutron Telescope (SNT) at Mt. Sierra Negra in Mexico (19.0°N, 97.3°W) is taking data since June of 2004. A solar neutron event was registered by this SNT, associated with the flare of September 7 of 2005, at the minimum phase of solar cycle 23. In this work we calculate the energy spectrum for this solar neutron event, using the attenuation model by Dorman & Valdés-Galicia (J. Geophys. Res. 495. 1999), and the detector efficiency calculation of Valdés-Galicia (Nucl. Inst. Meth., A535, 656, 2004).
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 57-60
