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

Lu Hong; Liu Shaomin; Dang Linkal; Mu Jun; Wang Hui; Feng Zhenyong; Ren Jingru; Xu Xianwu; Yu Guangce; Zhou Wendel

Chinese Physics C> 1999, Vol. 23> Issue(4) : 313-319

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

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

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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.

References

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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.

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Received: 1998-03-30
Revised: 1900-01-01

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通讯作者: 陈斌, bchen63@163.com

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沈阳化工大学材料科学与工程学院沈阳 110142

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

Received Date: 1998-03-30

Accepted Date: 1900-01-01

Available Online: 1999-04-05

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

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通讯作者: 陈斌, bchen63@163.com

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