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burst探测器
相关语句
  burst detector
     Monte Carlo Simulation of Burst Detector
     Burst探测器的Monte-Carlo模拟
短句来源
     The Δx,Δy distributions of burst detector indicate that the hybrid equipment of Yangbajing arranged in 1996 worked well.
     模拟了Burst探测器对入射粒子的响应,给出了Δx,Δy分布.
短句来源
  “burst探测器”译为未确定词的双语例句
     The contribution for detection of primary cosmic ray protons composition of hybrid equipment(EAS and EC) was discussed.
     考虑了广延空气族射(EAS)与乳胶室(EC)及Burst探测器联合实验的可能性及其对原初宇宙线质子成分测量的贡献;
短句来源
  相似匹配句对
     Monte Carlo Simulation of Burst Detector
     Burst探测器的Monte-Carlo模拟
短句来源
     Infra-red Detectors
     红外探测器
短句来源
     Characteristics of detector is discussed.
     讨论了探测器的特性 ;
短句来源
     The Δx,Δy distributions of burst detector indicate that the hybrid equipment of Yangbajing arranged in 1996 worked well.
     模拟了Burst探测器对入射粒子的响应,给出了Δx,Δy分布.
短句来源
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  burst detector
(2) A deep-space burst detector, the first spacecraft instrument built specifically for gamma-ray burst studies, was recently successfully integrated into the Helios-B space probe.
      
(3) Our gamma-ray instrument on the IMP-7 satellite is presently the most sensitive burst detector still operating in orbit.
      
A sea-level cosmic ray burst detector was in operation at the time of occurrence of 16 Vela bursts, between 1970 and 1973.
      
The LASL Pioneer Venus Orbiter Gamma Burst Detector (OGBD) is a vital element in the long base-line array of similar instruments intended to precisely locate sources of gamma-ray bursts.
      
Two flights from Alice Springs, Australia, were achieved in November 1977 and November 1978 with a plastic scintillator γ-burst detector, effective area 6.3 m2, thickness 5 cm, energy response in the range 50 keV to 2 MeV.
      
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The contribution for detection of primary cosmic ray protons composition of hybrid equipment(EAS and EC) was discussed.The lateral development in emulsion chamber of particle which energy greater than 100GeV were given by Monte Carlo simulation.The influence of 1cm iron in EC for the lateral development was analyzed.The Δx,Δy distributions of burst detector indicate that the hybrid equipment of Yangbajing arranged in 1996 worked well.

考虑了广延空气族射(EAS)与乳胶室(EC)及Burst探测器联合实验的可能性及其对原初宇宙线质子成分测量的贡献;MonteCarlo模拟给出了入射能量大于100GeV的粒子在乳胶室中纵向发展的过程,分析了乳胶室中1cm铁对级联发展的影响;模拟了Burst探测器对入射粒子的响应,给出了Δx,Δy分布.

With the development of γ-ray astronomy, a cosmic ray observatory was founded in the Yangbajing valley of Tibet highland (4300 m.a.s.l.) 10 years ago. Its EAS array of China-Japan ASγ Collaboration detected successfully the steady emission of multi-TeV γ rays from the Crab Nebula, the strong outbursts from AGN Mrk 501 in 1997 and from Mrk 421 in 2000, which is the first detections in the EAS experiments. The deviation and movement of Sun shadow by cosmic rays induced by solar and interplanetary magnetic field,...

With the development of γ-ray astronomy, a cosmic ray observatory was founded in the Yangbajing valley of Tibet highland (4300 m.a.s.l.) 10 years ago. Its EAS array of China-Japan ASγ Collaboration detected successfully the steady emission of multi-TeV γ rays from the Crab Nebula, the strong outbursts from AGN Mrk 501 in 1997 and from Mrk 421 in 2000, which is the first detections in the EAS experiments. The deviation and movement of Sun shadow by cosmic rays induced by solar and interplanetary magnetic field, has been only observed and will be adopted to monitor the variations of solar activity. Taking the advantages of high altitude and the combination of experiments of EAS array and emulsion chambers + burst detectors, the primary energy spectrum and composition of ultra-high energy cosmic ray have been studied. For exploring the 100 GeV gap region between the space and ground-based experiments, the project of China-Italy ARGO Collaboration is under constructing. Finally, to challenge the 5 GeV low threshold and the highly variable extragalactic sources, a high altitude huge IACT project 5@YorG in the future is discussed.

随着γ射线天文学的兴起,10年前在西藏高原海拔4300 m的羊八井谷地,出现并成长着一个国际知名的宇宙线实验站。其中日合作的ASγ阵列在国际同类实验中,首先观测到了蟹状星云的Multi-TeV稳定γ射线发射及活动星系核Mrk 501在1997年、Mrk 421在2000年的Multi-TeV γ射线强爆发,独家测出了反映太阳和行星际磁场状态的宇宙线太阳阴影的偏移并将之用于太阳活动变化的监测,利用高海拔优势及乳胶室和Burst探测器与阵列的联合实验进行了超高能宇宙线能谱和成分的研究。以高阻板探测器(RPC)地毯式阵列迈入≈100 GeV空白能区的中意合作ARGO(Astroparticle physics Research at Ground-based Observatory)计划,已进入大规模安装调试阶段。欲牢固占领Multi-GeV-TeV能区和满足对高可变、大峰流、短时标河外γ源的观测所需的高海拔巨型大气契仑可夫光成像望远镜计划5@YorG,也正在酝酿之中。

 
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