Energy Determination of Solar Neutrons by the SEDA-AP on-board JEM of ISS

Details Energy Determination of Solar Neutrons by the SEDA-AP on-board JEM of ISS Energy Determination of Solar Neutrons by the SEDA-AP on-board JEM of ISS

2009-09-07

arxiv.org/abs/0909.1181v1

Astronomy and Astrophysics

Astrophysics

Solar and Stellar Astrophysics

4 pages, 4 figures, submitted to the Proceeding of the 31st International Cosmic Ray Conference at Lodz, Poland

Scientific paper

A solar neutron detector has been launched on the Japan Exposure Module (JEM) of the International Space Station (ISS) in August 4, 2009. The detector works satsifactory. The detector comprises scintillation fiber and is designated as the Space Environment Data Acquisition (SEDA)-FIB. It tracks the recoil protons induced by neutrons and measurement of the proton energy using the range method. The energy resolution of the detector was measured using the proton beam at Riken. Herein, we report the energy resolution of the FIB detector by two different methods.

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