TY - JOUR
T1 - Results of a measurement of solar neutrons emitted on March 5, 2012 using a fiber-type neutron monitor onboard the SEDA-AP attached to the ISS
AU - Koga, K.
AU - Matsumoto, H.
AU - Okudaira, O.
AU - Goka, T.
AU - Obara, T.
AU - Masuda, S.
AU - Muraki, Y.
AU - Shibata, S.
AU - Yamamoto, T.
PY - 2015/1/1
Y1 - 2015/1/1
N2 - The solar neutron detector SEDA-FIB onboard the International Space Station (ISS) has detected several events from the solar direction associated with three large solar flares observed on March 5th (X1.1), 7th (X5.4), and 9th (M6.3) of 2012. In this study, we present the time profiles of those neutrons and discuss the physics that may be related to a possible acceleration scenario for ions over the solar surface. We compare our data with the dynamical pictures of the flares obtained by the ultra-violet telescope of the space-based Solar Dynamics Observatory.
AB - The solar neutron detector SEDA-FIB onboard the International Space Station (ISS) has detected several events from the solar direction associated with three large solar flares observed on March 5th (X1.1), 7th (X5.4), and 9th (M6.3) of 2012. In this study, we present the time profiles of those neutrons and discuss the physics that may be related to a possible acceleration scenario for ions over the solar surface. We compare our data with the dynamical pictures of the flares obtained by the ultra-violet telescope of the space-based Solar Dynamics Observatory.
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M3 - Conference article
AN - SCOPUS:84988692257
VL - 30-July-2015
JO - Proceedings of Science
JF - Proceedings of Science
SN - 1824-8039
M1 - 068
T2 - 34th International Cosmic Ray Conference, ICRC 2015
Y2 - 30 July 2015 through 6 August 2015
ER -