TY - JOUR
T1 - Simultaneous observation of solar neutrons from the ISS and high mountain observatories in association with a flare on July 8, 2014
AU - Muraki, Y.
AU - Lopez, D.
AU - Koga, K.
AU - Kakimoto, F.
AU - Goka, T.
AU - González, L. X.
AU - Masuda, S.
AU - Matsubara, Y.
AU - Matsumoto, H.
AU - Miranda, P.
AU - Okudaira, O.
AU - Obara, T.
AU - Salinas, J.
AU - Sako, T.
AU - Shibata, S.
AU - Ticona, R.
AU - Tsunesada, Y.
AU - Valdés-Galicia, J. F.
AU - Watanabe, K.
AU - Yamamoto, T.
PY - 2015
Y1 - 2015
N2 - An M6.5-class flare was observed at N12E56 of the solar surface at 16:06 UT on July 8, 2014. 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 analysed these data and a possible scenario of enhancements produced by high-energy protons and neutrons is proposed, using the data from continuous observation of a solar surface by the ultraviolet telescope onboard the Solar Dynamical Observatory (SDO).
AB - An M6.5-class flare was observed at N12E56 of the solar surface at 16:06 UT on July 8, 2014. 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 analysed these data and a possible scenario of enhancements produced by high-energy protons and neutrons is proposed, using the data from continuous observation of a solar surface by the ultraviolet telescope onboard the Solar Dynamical Observatory (SDO).
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M3 - Conference article
AN - SCOPUS:84988692851
SN - 1824-8039
VL - 30-July-2015
JO - Proceedings of Science
JF - Proceedings of Science
M1 - 050
T2 - 34th International Cosmic Ray Conference, ICRC 2015
Y2 - 30 July 2015 through 6 August 2015
ER -