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七十厘米流光室系统

A 70cm STREAMER CHAMBER SYSTEM

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【作者】 于小红王孝良王殿荣王继华王德武卢新华李云山李成泽李志刚邰永生韩缨陈元柏杜远才尧宗元林建锋周伟姜孆嫄赵海泉张家铨高文绣徐雨林徐蓉芬崔化传童国樑谢一冈

【Author】 THE SECOND EXPERIMEHTAL GROUP Institute of High Energy Physics, Academia Sinica Yu Xiao-hong;Wang Xiao-liang;Wang Dian-rong;Wang Ji-hua;Wang De-wu;Lu Xin-hua;Li Yun-shan;Li Cheng-ze;Li Zhi-gang;Tai Yong-sheng;Han Ying;Chen Yuan-bo;Du Yuan-cai;Yao Zong-yuan;Lin Jian-feng;Zhou Wei;Jiang Ying-yuan;Zhao Hai-quan;Zhang Jia-quan;Gao Wen-xiu;Xu Yu-lin;Xu Yong-fen;Cui Hua-chuan;Tong Guo-liang;Xie Yi-gang

【机构】 中国科学院高能物理研究所物理二室中国科学院高能物理研究所物理二室

【摘要】 本文描述70×50×(15×2)cm~3双间隙流光室系统的设计、建造和性能。用一个25级Marx产生器(600kV)与四间隙圆柱形Blumlein线相连已成功地得到上升时间2ns、宽度10ns的快脉冲。该系统由三重大面积闪烁计数器望远镜选择宇宙线粒子触发,通过控制线路接一定的逻辑程序自动控制各组成部分协同动作。在杂质含量小于0.2%的情况下,先后在Ne及Ne-He混合气体中观察到流光径迹,并用国产示波器像机和28DIN底片得到了流光径迹照片。

【Abstract】 In this paper, the design, construction and characteristics of a 70cm streamerchamber system are deseribed. A very fast pulse with rise time 2 ns and duration 10ns has been successfullyobtained by using a four-spark-gap cylindrical Blumlein line with a 25 stage Marxgenerator (up to 600kV) connected to it. The output pulse of the Blumlein line isthen fed to the chamber, via heteromorphic transmission line with pulse shapeminimum distortion. The system are triggered by three-fold large area scintillation counter telescopeto pick up particle of the cosmic ray traversing the sensitive volume of the chamber.The coincidence-counting rate is ~5 particles/min., the resolving time is 10ns, andthe ratio of the true-accidental coincidence is more than 700. The chamber has two 15 cm gaps and is 70 cm long, 50 cm wide, with 30Ω ofcharacteristic impedence. In order to photograph through the electrodes, the central and the ground electrodes towards the cameras are made of 0.2mm diameter beryl-lium-copper wire stands spaced 2 mm apart, with transparency~90%. Pure neon and mixtures of neon-helium gas were used to fill the chamber, oneatmosphere, and a cycling and purifier system were designed to maintain its purity.The gas is passed through type 5A and 13x molecular sieve operated at room andliquid -nitrogen temperature to remove CO2, H2O and O2, N2, respectively. The im-purities of the chamber gas can be reduced to 0.2% within 2hr., at the gas flow rate500 1/hr. All photographs are taken with one or two oscilloscope cameras on 35mm film of28 DIN. A demagnification 30x and a resolution 30 line pairs/mm at the maximumaperture (f/2) are used. The sizes of the visual streamers were estimated about3 to 4 mm in diameter (view along the E field), and 10 to 15 mm long (view perpen-dicular to the E field). The delay time between the penetration of charged particle and the supply of thehigh voltage pulse on the chamber was ~3.5μs. The system was suggested in June1975. The whole facility began to mount and adjust in January 1979, and the strea-mer tracks were seen on July 26, 1979. We plan to make the performance tests, to reduce the delay time of the system,and to improve the chamber suitable for use in high energy accelerator and cosmic-ray experiments in the near future.

  • 【文献出处】 高能物理与核物理 ,High Energy Physics and Unclear Physics , 编辑部邮箱 ,1982年01期
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