Speaker
Dr
Yutaka Matsubara
(STE-Laboratory, Nagoya University)
Description
At 16:06UT on July 8, 2014, an M6.5-class flare was observed at N12E56 of the solar surface.
In association with this flare, solar neutron detectors located on two high mountains, Mt. Sierra Negra and Chacaltaya and at the space station observed enhancements in the neutral channel.
The authors analyzed these data and a possible scenario of enhancements produced by high-energy protons and neutrons is proposed; based on data from continuous observation of a solar surface using the ultraviolet telescope onboard the Solar Dynamical Observatory (SDO).
| Registration number following "ICRC2015-I/" | 1090 |
|---|---|
| Collaboration | -- not specified -- |
Author
Prof.
Yasushi Muraki
(Professor emiritus)
Co-authors
Mr
Diego Lopez
(STEL, Nagoya University)
Prof.
Fumio Kakimoto
(Tokyo Institute of Technology)
Dr
Haruhisa Matsumoto
(space environment monitor group, JAXA)
Mr
J Salinas
(Instituto de Investigaciones Físicas, UMSA, La Paz, Bolivia)
Prof.
J.F. Valdes-Galicia
(Institute de Geofisica, UNMA, Mexico)
Dr
Kiyokazu Koga
(Space environment monitor group, Tsukuba space center, JAXA)
Dr
Kyoko Watanabe
(Hinode group, ISAS. JAXA)
Dr
Luis Xavier Gonzalez
(Instituto de Geofísica, Unidad Michoacán, Universidad Nacional Autónoma de México, 58089, Morelia, Michoacán. Mexico)
Dr
Osamu Okudaira
(Space environment monitor group, JAXA)
Mr
P Miranda
(Instituto de Investigaciones Físicas, UMSA, La Paz, Bolivia)
Dr
Satoshi Masuda
(STE-lab. Nagoya University)
Prof.
Syoichi Shibata
(Engineering Science Laboratory, Chubu University)
Prof.
Takahiro Obara
(Planet atomospheric plasma center, Tohoku University)
Dr
Takashi Sako
(STE-Laboratory, Nagoya University)
Dr
Tateo Goka
(tskuba, JAXA)
Dr
Tokonatsu Yamamoto
(Department of Physics, Konan University)
Dr
Yoshiki Tsunesada
(Department of Physics, Tokyo Institute of Technology)
Dr
Yutaka Matsubara
(STE-Laboratory, Nagoya University)
Dr
Yuya Nagai
(STEL, Nagoya University)
