Galactic-disk enhancement of cosmic rays at E > 1012eV
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Ogio, S
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Tokyo Inst Technol, Dept Phys, Meguro Ku, Tokyo 1528551, JapanTokyo Inst Technol, Dept Phys, Meguro Ku, Tokyo 1528551, Japan
Ogio, S
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Tsunesada, Y
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Kakimoto, F
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Tokyo Inst Technol, Dept Phys, Meguro Ku, Tokyo 1528551, JapanTokyo Inst Technol, Dept Phys, Meguro Ku, Tokyo 1528551, Japan
Kakimoto, F
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Burgoa, O
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Tokyo Inst Technol, Dept Phys, Meguro Ku, Tokyo 1528551, JapanTokyo Inst Technol, Dept Phys, Meguro Ku, Tokyo 1528551, Japan
Burgoa, O
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Gotoh, E
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Tokyo Inst Technol, Dept Phys, Meguro Ku, Tokyo 1528551, JapanTokyo Inst Technol, Dept Phys, Meguro Ku, Tokyo 1528551, Japan
Gotoh, E
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Harada, D
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Tokyo Inst Technol, Dept Phys, Meguro Ku, Tokyo 1528551, JapanTokyo Inst Technol, Dept Phys, Meguro Ku, Tokyo 1528551, Japan
Harada, D
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Kaneko, T
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Matsubara, Y
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Tokyo Inst Technol, Dept Phys, Meguro Ku, Tokyo 1528551, JapanTokyo Inst Technol, Dept Phys, Meguro Ku, Tokyo 1528551, Japan
Matsubara, Y
[1
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Miranda, P
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Tokyo Inst Technol, Dept Phys, Meguro Ku, Tokyo 1528551, JapanTokyo Inst Technol, Dept Phys, Meguro Ku, Tokyo 1528551, Japan
Miranda, P
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Mizumoto, Y
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Tokyo Inst Technol, Dept Phys, Meguro Ku, Tokyo 1528551, JapanTokyo Inst Technol, Dept Phys, Meguro Ku, Tokyo 1528551, Japan
Mizumoto, Y
[1
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Morizawa, A
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Tokyo Inst Technol, Dept Phys, Meguro Ku, Tokyo 1528551, JapanTokyo Inst Technol, Dept Phys, Meguro Ku, Tokyo 1528551, Japan
Morizawa, A
[1
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Murakami, K
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Tokyo Inst Technol, Dept Phys, Meguro Ku, Tokyo 1528551, JapanTokyo Inst Technol, Dept Phys, Meguro Ku, Tokyo 1528551, Japan
Murakami, K
[1
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Nakatani, H
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Tokyo Inst Technol, Dept Phys, Meguro Ku, Tokyo 1528551, JapanTokyo Inst Technol, Dept Phys, Meguro Ku, Tokyo 1528551, Japan
Nakatani, H
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Nishi, K
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Tokyo Inst Technol, Dept Phys, Meguro Ku, Tokyo 1528551, JapanTokyo Inst Technol, Dept Phys, Meguro Ku, Tokyo 1528551, Japan
Nishi, K
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Shimoda, S
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Tokyo Inst Technol, Dept Phys, Meguro Ku, Tokyo 1528551, JapanTokyo Inst Technol, Dept Phys, Meguro Ku, Tokyo 1528551, Japan
Shimoda, S
[1
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Shirasaki, Y
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Tokyo Inst Technol, Dept Phys, Meguro Ku, Tokyo 1528551, JapanTokyo Inst Technol, Dept Phys, Meguro Ku, Tokyo 1528551, Japan
Shirasaki, Y
[1
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Tajima, N
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Tokyo Inst Technol, Dept Phys, Meguro Ku, Tokyo 1528551, JapanTokyo Inst Technol, Dept Phys, Meguro Ku, Tokyo 1528551, Japan
Tajima, N
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Tokunou, H
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Tokyo Inst Technol, Dept Phys, Meguro Ku, Tokyo 1528551, JapanTokyo Inst Technol, Dept Phys, Meguro Ku, Tokyo 1528551, Japan
Tokunou, H
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Toyoda, Y
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Velarde, A
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Tokyo Inst Technol, Dept Phys, Meguro Ku, Tokyo 1528551, JapanTokyo Inst Technol, Dept Phys, Meguro Ku, Tokyo 1528551, Japan
Velarde, A
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Yamada, Y
[1
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Yoshii, H
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Tokyo Inst Technol, Dept Phys, Meguro Ku, Tokyo 1528551, JapanTokyo Inst Technol, Dept Phys, Meguro Ku, Tokyo 1528551, Japan
Yoshii, H
[1
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机构:
[1] Tokyo Inst Technol, Dept Phys, Meguro Ku, Tokyo 1528551, Japan
来源:
NUOVO CIMENTO DELLA SOCIETA ITALIANA DI FISICA C-GEOPHYSICS AND SPACE PHYSICS
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2001年
/
24卷
/
4-5期
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摘要:
We observed an enhancement of cosmic rays from the Vela region with SAS array at Mt. Chacaltaya in Bolivia. It is not possible to conclude that this enhancement is caused by primary gamma-rays, since the observed events not limited with the less muons in the air showers show the same enhancement. In order to confirm this result with improved statistics and to investigate the energy dependence of this enhancement, we have installed a new array, called NIAS array. All the data with much higher statistics show the enhancement along the whole galactic disk.