The correlation between the deviation of Sun's shadows and the mean solar magnetic field

被引：0
|
作者：
Lu, H [1 ]
Liu, SM
Ding, LK
Zhaxiciren
Zhaxisangzhu
Mu, J
Wang, H
Feng, ZY
Ren, JR
Xu, XW
Yu, GC
Zhou, WD
Labaciren
Meng, XR
Meng, L
Zhang, JL
Zhang, CS
Zhang, HM
Shi, ZZ
Jia, HY
Huang, Q
Tan, YH
Huo, AX
Dai, BZ
机构：
[1] Chinese Acad Sci, Inst High Energy Phys, Inst Cosm Ray & High Energy Astrophys, Beijing 100039, Peoples R China
[2] Tibet Univ, Inst Cosm Ray Res, Lhasa 850000, Peoples R China
[3] South West Jiaotong Univ, Dept Phys, Chengdu 610031, Peoples R China
[4] Yunnan Univ, Dept Phys, Kunming 650091, Peoples R China
来源：
HIGH ENERGY PHYSICS AND NUCLEAR PHYSICS-CHINESE EDITION | 1999年 / 23卷 / 04期
关键词：
cosmic ray; deviation of Sun's shadow; mean solar magnetic field;
D O I：
暂无
中图分类号：
O57 [原子核物理学、高能物理学];
学科分类号：
070202 ;
摘要：
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 deviations 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.
引用
收藏
页码：313 / 319
页数：7
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