The Observation of Diffuse Cosmic and Atmospheric Gamma Rays with an Electron-Tracking Compton Camera Loaded on a Balloon
Author(s) -
Atsushi Takada,
H. Kubo,
H. Nishimura,
K. Ueno,
T. Tanimori,
K. Miuchi,
Kenn'ichi Tsuchiya,
S. Kabuki,
K. Hattori,
Shunsuke Kurosawa,
Chihiro Ida,
Satoru Iwaki,
N. aka,
Eiichi Mizuta
Publication year - 2009
Publication title -
journal of the physical society of japan
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 0.76
H-Index - 139
eISSN - 1347-4073
pISSN - 0031-9015
DOI - 10.1143/jpsjs.78sa.161
Subject(s) - physics , gamma ray , telescope , cosmic ray , compton scattering , photon , gamma ray astronomy , tracking (education) , recoil , electron , optics , astrophysics , nuclear physics , pedagogy , psychology
As next-generation MeV gamma-ray telescope, we have developed an electron-tracking Compton camera (ETCC) that consists of a gaseous tracker and an absorber. The ETCC obtains the energy and direction of both a scattered gamma ray and a recoil electron, and determines both the energy and direction of an incident gamma ray, photon by photon. Furthermore, this camera features powerful background rejection based on Compton-scattering kinematics. To prepare for future spacecraft loading, we planned the balloon experiment, “Sub-MeV gamma-ray Imaging Loaded-on-balloon Experiment” (SMILE). As the first step in SMILE, we demonstrated gamma-ray detection using our camera by observing diffuse cosmic gamma rays and secondary gamma rays generated by collisions between high-energy cosmic rays and nuclei in the air. On September 1, 2006, our detector was loaded on a balloon and launched from Sanriku Balloon Center, ISAS/JAXA. The balloon realized level flight at an altitude of about 35 km during a live time of 3.0 h. We ...
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