Measurement of high energy cosmic rays originated from Vela SNR
Measurement of high energy cosmic rays originated from Vela SNR
批准号:
12573003
负责人:
KAKIMOTO Fumio
金额:
$9.98万
依托单位国家:
日本
项目类别:
Grant-in-Aid for Scientific Research (B)
财政年份:
2000
资助国家:
日本
项目状态:
已结题
起止时间:
2000 至 2002
中文摘要
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英文摘要
The establishment of the origin of primary cosmic rays is most important theme in cosmic ray physics. To get the final answer it is most important to measure the anisotropy of primary cosmic rays. However, the order of the magnitude of the anisotropy is expected to be 0.1%. Then the observation must be done with sufficient accuracy. This is achieved so to make an observation around the atmospheric depths of air shower maximum developments, that is, with a high altitude air shower array.In this research, we observed air showers at Mt. Chacaltaya (5,200m a. s. l.) to measure the anisotropy due to the cosmic rays emitted from Vela SNR, which is one of the most active astronomical objects in X-and gamma-ray regions.We stated the observation from 2001 after the installment of the equipments. The observation and analyzes were made continuously and preliminary results were presented in the international conference of cosmic rays in Hamburg, Germany 2001 and the meetings of the Physical Societ … More y of Japan.The observed result is summarized as the follows :(1)The enhancement of primary cosmic rays from the galactic disk is observed.(2)The degree of the enhancement around the galactic longitudinal region from 220 to 260 degree is about 0.3%.(3)Our Monte-Carlo simulation on the cosmic rays propagation in the galaxy shows that if Vela SNR is made at 100,000 years ago if the distance of the SNR from the solar system is about 250 pc, the observed result is well explained due to the cosmic rays emitted from the SNR. Since the present accepted values are 10,000 years and 500 pc, respectively, the resent ROSAT results show that the distance is about 250pc and there is another explosion at 100,000 years ago.(3)Our Monte-Carlo simulation on the cosmic rays propagation in the galaxy shows that if Vela SNR is made at 100,000 years ago if the distance of the SNR from the solar system is about 250 pc, the observed result is well explained due to the cosmic rays emitted from the SNR. Since the present accepted values are 10,000 years and 500 pc, respectively, the resent ROSAT results show that the distance is about 250pc and there is another explosion at 100,000 years ago. Less
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S.Ogio et al.: "Measurement of cosmic ray chemical composition at Mt.Chacaltaya"III Nuovo Cimento. 24C. 591-597 (2001)
S.Ogio 等人:“Chacaltaya 山宇宙射线化学成分的测量”III Nuovo Cimento。
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S. Ogio et al.: "Galactic disk enhancement of cosmic rays at E 〉10^12 eV"I11 Nuovo Cimento. 24C. 625-630 (2001)
S. Ogio 等人:“E ≥10^12 eV 处宇宙射线的银河盘增强”I11 Nuovo Cimento 24C (2001)。
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F. Kakimoto: "The laboratory for cosmic ray research at 5, 200m above the sea level"Mathematical Science. 40[11]. 78-83 (2002)
F. Kakimoto:“海拔5、200m处的宇宙射线研究实验室”数学科学。
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垣本史雄: "標高5,200mの宇宙線観測所"数理科学. 40[11]. 78-83 (2002)
Fumio Kakimoto:“5,200m 高度的宇宙射线观测站”,《数学科学》40[11]。
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作者:
[]
通讯作者:
S. Ogio et al.: "Measurement of cosmic ray chemical composition at Mt. Chacaltaya"I11 Nuovo Cimento. 24C. 591-597 (2001)
S. Ogio 等人:“Chacaltaya 山宇宙射线化学成分的测量”I11 Nuovo Cimento。
DOI:
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发表时间:
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共 11 条
Study on galactic origns of high energy cosmic rays
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批准号:23403002
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项目类别:Grant-in-Aid for Scientific Research (B)
-
资助金额:$12.4万
-
财政年份:2011
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负责人:KAKIMOTO Fumio
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依托单位:
Study on origins of cosmic rays with energies above 10^<16>eV
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批准号:16340068
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项目类别:Grant-in-Aid for Scientific Research (B)
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资助金额:$10.31万
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财政年份:2004
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负责人:KAKIMOTO Fumio
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依托单位:
Study both on the super-GZK problem and on the chemical composition of high energy cosmic rays
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批准号:15077203
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项目类别:Grant-in-Aid for Scientific Research on Priority Areas
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资助金额:$134.46万
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财政年份:2003
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负责人:KAKIMOTO Fumio
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依托单位:
Study on chemical composition of primary cosmic rays with energies above 10^<16> eV
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批准号:11640260
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项目类别:Grant-in-Aid for Scientific Research (C)
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资助金额:$2.37万
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财政年份:1999
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负责人:KAKIMOTO Fumio
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依托单位:
Measurement of Nuclear Composition of Primary Cosmic Rays
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批准号:08041101
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项目类别:Grant-in-Aid for international Scientific Research
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资助金额:$6.85万
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财政年份:1996
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负责人:KAKIMOTO Fumio
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依托单位:
Measurement of Nuclear Composition of Primary Cosmic rays
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批准号:06041039
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项目类别:Grant-in-Aid for international Scientific Research
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资助金额:$7.3万
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财政年份:1994
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负责人:KAKIMOTO Fumio
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依托单位:
Low Frequency Radio Signals from Giant Air Showers
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批准号:02452023
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项目类别:Grant-in-Aid for General Scientific Research (B)
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资助金额:$4.48万
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财政年份:1990
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负责人:KAKIMOTO Fumio
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依托单位:
海外基金