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Search for Steady Emission of 10—TeV Gamma Rays from the Crab Nebula,Cygnus X—3,and Hercules X—1 Using the Tibet Air Shower Array
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作者 M.Amenomori Z.Cao.L.K.Ding +49 位作者 Z.Y.Feng K.Hibino N.Hotta Q.Huang A.X.Huo H.Y.Jia G.Z.Jiang S.Q.Jiao F.Kajino K.Kasahara Labaciren D.M.Mei L.Meng X.R.Meng Mimaeiren K.Mizutani J.Mu H.Nanjo M.Nishizawa Nusang A.Oguro M.Ohnishi I.Ohta J.R.Ren To.saito M.Sakata Z.Z.Shi M.Shibata T.shirai H.sugimoto X.X.Sun A.Tai K.Taira Y.H.Tan N.Tateyama S.Torii H.Wang C.Z.Wen Y.Yamamoto X.Y.Yao G.C.Yu P.Yuan T.Yuda J.G.Zeng C.S.Zhang H.M.Zhang L.Zhang Zhasang Zhaxlclren w.d.zhou 《西藏大学学报(社会科学版)》 1993年第4期71-75,共5页
寻找到高能和超高能的Gamma射线点源,在宇宙射线源方面有着极为重要的意义,本文就西藏羊八井观测到的空气簇射阵列及共它资料,对寻找稳定的10-TeV Gamma射线进行了分析论述。
关键词 西藏空气簇射 Gamma射线点源 大气厚度 10TeV
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Cosmic—Ray Deficit from the Directions of the moon and the Sun Detected with the Tibet Air Shower Array 被引量:1
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作者 M.Amenomori Z.Cao +49 位作者 L.K.Ding Z.Y.Feng Hibino N.Hotta Q.Huang A.X.Huo H.Y.Jia G.z.Jiang S.Q.Jiao F.Kajino K.Kasahara Labaciren D.M.Mei L.Meng X.R.Meng Mimaciren K.Mizutani J.Mu H.Nanjo M.Nishizawa Nusang A.Oguro M.Ohnishi I.Ohta To.Saito M.Sakata Z.Z.shi M.Shibata T.Shirai H.Sugimoto X.X.Sun A.Tai K.Taira Y.H.Tan N.Tateyama S.Torii H.Wang C.Z.Wen Y.Yamamoto X.Y.Yao G.C.Yu P.Yuan T.Yuda J.G.Zeng C.S.Zhang H.M.Zhang L.Zhang Zhasang Zhaxiciren w.d.zhou 《西藏大学学报(社会科学版)》 1993年第4期76-85,共10页
Data from the Tibet air shower array were used to examine the cosmic ray shadows of the Moon and the Sun at energies around 10Tev.The shadowing effect was clearly observed at the 5.8level for the Moon,while the shadow... Data from the Tibet air shower array were used to examine the cosmic ray shadows of the Moon and the Sun at energies around 10Tev.The shadowing effect was clearly observed at the 5.8level for the Moon,while the shadow of the Sun was found in the direction away from the sun by 0.86°tothe west and 0.43°to the south.The effect of the geomagnetic field has also been observed in the shadow of cosmic rays by the Moon.The observed deflection of the sun’s shadow is briefly discussed in connection with the effect of the magnetic fields between the sun and the Earth.This is the first observation of the effects of such magnetic fields on the cosmic ray shadow.The maximum-likelihood analysis of the Moon data set shows that the angular resolutions of the array for showers with its mode energies 7TeVand 35TeV are 0.87°-0.13°+0.10°and 0.54°-0.08°+0.11°,respectively. 展开更多
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