A search for Cosmic High Energy Neutron
A search for Cosmic High Energy Neutron
批准号:
04402003
负责人:
TESHIMA Masahiro
金额:
$24.19万
依托单位:
依托单位国家:
日本
项目类别:
Grant-in-Aid for General Scientific Research (A)
财政年份:
1992
资助国家:
日本
项目状态:
已结题
起止时间:
1992 至 1994
中文摘要
利用光学技术研制了用于寻找高能宇宙中子的高分辨率宇宙射线探测器。制作了由8个512像素多阳极光电倍增管组成的高分辨率相机及数据采集电子器件。它被安装在犹他大学提供的固定定向反射镜系统的靶面上。为了获得对高能宇宙射线的最佳灵敏度,望远镜的俯仰角为19‰。观察时间为-100小时。Nd: YAG激光监测系统由美国犹他大学的合作者操作。利用该系统,我们可以校准探测器并监测大气状况。通过100小时的观测,我们探测到了100张宇宙射线雨的图像。其中,10幅星雨图像被识别为能量大于3*10^<18>eV,撞击参数距离探测器10Km-30Km的星雨图像。通过数据分析,我们证明了淋浴探测器平面的几何形状可以确定,精度为-0.03‰。这个角度分辨率比目前所达到的分辨率要好得多。我们建立了高精度探测宇宙射线的实验方法。
英文摘要
The high resolution cosmic ray detector using optical tequniques were developped to search for high energy cosmic neutrons.The high resolution camera consisiting of eight multi anode photomultipliers of 512 pixels, and the data aquisition electronics were made. It was mounted on the fucul plane of the fixed directional mirror systems provided by University of Utah. The telesope was directed at elevation angle of 19゚ to get the best sensitivity for the high energy cosmic rays. The observation were carried out for -100hrs.The monitoring system with Nd : YAG laser were operated by the collaborators of University of Utah. Using this system, we could calibrate our detector and monitor the atmospheric condition.With 100hr observation, we have detected 100 cosmic ray shower images. Among them, 10 shower images were identified as showers with energy of greater than 3*10^<18>eV,and with the impact parameter of 10Km-30Km from detector. Through the data anlaysis, we have demonstrated that the geometry of the shower detector plane can be determined with an acuracy of -0.03゚. This angular resolution is much better than the resolution achieved so far. We have established the experimental method to detect cosmic rays with the high accuracy.
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N.Chiba et.al.: "Akeno Giant Air Shower Array(AGASA)covering 100kmX^2 area," Nucl.Inst.and Meth.A311. 338-349 (1992)
N.Chiba 等人:“覆盖 100kmX^2 区域的 Akeno 巨型空气簇射阵列 (AGASA)”,Nucl.Inst.and Meth.A311。
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M.Nagano et al.: "Energy Spectrum of Primary Cosmic RayS above 10X^<17>eV Determined from The Extensive Air Shower Experiment at Akeno," J.Phys.G:Nucl.Phys.18. 423-442 (1992)
M.Nagano等人:“根据Akeno的广泛空气簇射实验确定的10X^ 17 eV以上的初级宇宙射线能量谱”,J.Phys.G:Nucl.Phys.18。
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Yoshida et al.: "The Cosmic Ray Energy Spectrum above3×10^<18>eV by the Akeno Giant Air Shower Array" to be published in Astroparitcle Physics. (1995)
Yoshida 等人:“The Cosmic Ray Energy Spectrum above3×10^<18>eV by the Akeno Giant Air Shower Array”将发表在 Astroparitcle Chemistry (1995) 上。
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N.Chiba et al.: "Possible Evidence for ≧ 10GeV Neutrons Associated with The Solar Flare of 4 June 1991," Astroparticle Phys.1. 27-32 (1992)
N.Chiba 等人:“与 1991 年 6 月 4 日太阳耀斑相关的 ≧ 10GeV 中子的可能证据”,Astroarticle Phys.1 (1992)。
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Honda et al.: "Inelastic Cross Section for P-Air Collisions from Air Shower Ex-periment and Total Cross Section for P-P Collisions up to √s=24Te" Phys.Rev.Lett.50. 2058-2061 (1993)
Honda 等人:“来自空气喷淋实验的 P-Air 碰撞的非弹性横截面和高达 √s=24Te 的 P-P 碰撞的总横截面”Phys.Rev.Lett.50 (1993)。
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共 22 条
Study of the Extreme Universe with High Energy Gamma Rays
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批准号:24000004
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项目类别:Grant-in-Aid for Specially Promoted Research
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资助金额:$336.96万
-
财政年份:2012
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负责人:TESHIMA Masahiro
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依托单位:
Study of the highest energy cosmic rays with air fluorescence technique
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批准号:11691117
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项目类别:Grant-in-Aid for Scientific Research (A)
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资助金额:$10.23万
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财政年份:1999
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负责人:TESHIMA Masahiro
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依托单位:
The Study of the Highest Energy Cosmic Ray
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批准号:07247102
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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:$165.31万
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财政年份:1995
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负责人:TESHIMA Masahiro
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依托单位:
Development of Imaging Camera for Ultra High Energy Cosmic Rays
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批准号:04554005
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项目类别:Grant-in-Aid for Developmental Scientific Research (B)
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资助金额:$12.03万
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财政年份:1992
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负责人:TESHIMA Masahiro
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依托单位:
A Study of Neutral Particles from Cygnus X-3 above 10^<18>eV
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批准号:02452021
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项目类别:Grant-in-Aid for General Scientific Research (B)
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资助金额:$3.33万
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财政年份:1990
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负责人:TESHIMA Masahiro
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依托单位:
国内基金
海外基金
基于新型co-Neutron-Encoding技术对蛋白质精氨酸二甲基化修饰进行质谱精准鉴定研究
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批准号:21675006
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项目类别:面上项目
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资助金额:65.0万元
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批准年份:2016
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负责人:贾辰熙
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依托单位: