The Correlation Between the Deviation of Sun’s Shadows and the Mean Solar Magnectic Field

  • Using the data of the Sun's shadows for the 10 TeV cosmic ray flux, which are obtained in the period of June 1990-August 1996 by the Tibet air shower array, the correlation betWeen the deviahons of Sun's shadows and the strength of the mean solar magnectic field at the same period has been studied. One simple model used to calculate and explain this relations is also presented.
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  • [1] Clark G W Phys.Rev,1957,108:4502 Amenomori M et al.Phys.Rev.,1993,D47:26753 Amenomori M et al. ApJ, 1994, 415:L147 4 Amenomori M et al.ApJ,1996,464:9545 Liu Shaomin et al.High Energy Physics and Nuclear Physics(in Chinese),1997,21(10):865 (刘绍敏等.高能物理与核物理,1997,21(10):865)6 Amenomori M et al.High Enerpy Physics and Nuclear Physics(in Chinesc),1993,17:385 (Amenomori M et al.高能物理与核物理, 1993, 17: 385.)7 Li Tipei.Mathematical treatment of Experiment Beijing:Academic Press,1980 (李惕培.实验的数学处理.北京:科学出版社,1980)8 Cuperman s,Li J,Semel M.Astron.Astrophys.,1993,268:7469 Swinson D B et al.Possible Displacement of the Neutral Sheet due to Asymmetry of Activity on the Sun. In:Proc. 21th ICRC. Autralia: Adelaide Press,1991,SH 6.2—2 br10 NOAA/USAF Space Environmental Information Center, Solar Geophysical Deta, 1990–1996
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Lu Hong, Liu Shaomin, Dang Linkal, Mu Jun, Wang Hui, Feng Zhenyong, Ren Jingru, Xu Xianwu, Yu Guangce, Zhou Wendel, The Correlation Between the Deviation of Sun’s Shadows and the Mean Solar Magnectic Field[J]. Chinese Physics C, 1999, 23(4): 313-319.
Lu Hong, Liu Shaomin, Dang Linkal, Mu Jun, Wang Hui, Feng Zhenyong, Ren Jingru, Xu Xianwu, Yu Guangce, Zhou Wendel, The Correlation Between the Deviation of Sun’s Shadows and the Mean Solar Magnectic Field[J]. Chinese Physics C, 1999, 23(4): 313-319. shu
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Received: 1998-03-30
Revised: 1900-01-01
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The Correlation Between the Deviation of Sun’s Shadows and the Mean Solar Magnectic Field

    Corresponding author: Lu Hong,
  • Laboratory of Cosmic Ray and High Energy Astrophysics, Institute of High Energy Physics, The Chinese Academy of sciences, Beijing 1000392 Institute for Cosmic Ray Research, Tibet University, Lhasa 8500003 Department of Physics, South West Jiaotong University, Chengdu 6100314 Department of Physics, Yunnan University, Kunming 650091

Abstract: Using the data of the Sun's shadows for the 10 TeV cosmic ray flux, which are obtained in the period of June 1990-August 1996 by the Tibet air shower array, the correlation betWeen the deviahons of Sun's shadows and the strength of the mean solar magnectic field at the same period has been studied. One simple model used to calculate and explain this relations is also presented.

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