中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Sun's shadow by 10 TeV cosmic rays under the influence of solar activity

文献类型:期刊论文

作者Tibet ASγ Collaboration
刊名TRANSPORT OF GALACTIC AND ANOMALOUS COSMIC RAYS IN THE HELIOSPHERE: OBSERVATIONS, SIMULATIONS AND THEORY
出版日期1999
卷号23期号:3页码:#REF!
通讯作者Amenomori, M (reprint author), Hirosaki Univ, Dept Phys, Hirosaki, Aomori 036, Japan.
英文摘要We examined the Sun's shadow by 10 TeV cosmic rays observed with the Tibet air shower array during the period from 1991 through 1997. The results suggest that there is a causal relation between the shadow's movement and the changing inclination of the heliospheric current sheet of the large-scale solar magnetic field. Thus, further observations with higher statistics may provide direct information on the relation between a time variation of the large-scale structure of the solar and interplanetary magnetic fields and the phase of solar activity cycle. (c)1999 COSPAR. Published by Elsevier Science Ltd.
学科主题Engineering; Astronomy & Astrophysics; Geology; Meteorology & Atmospheric Sciences
类目[WOS]Engineering, Aerospace ; Astronomy & Astrophysics ; Geosciences, Multidisciplinary ; Meteorology & Atmospheric Sciences
收录类别SCI
WOS记录号WOS:000081205800032
公开日期2016-05-03
源URL[http://ir.ihep.ac.cn/handle/311005/227742]  
专题高能物理研究所_粒子天体物理中心
推荐引用方式
GB/T 7714
Tibet ASγ Collaboration. Sun's shadow by 10 TeV cosmic rays under the influence of solar activity[J]. TRANSPORT OF GALACTIC AND ANOMALOUS COSMIC RAYS IN THE HELIOSPHERE: OBSERVATIONS, SIMULATIONS AND THEORY,1999,23(3):#REF!.
APA Tibet ASγ Collaboration.(1999).Sun's shadow by 10 TeV cosmic rays under the influence of solar activity.TRANSPORT OF GALACTIC AND ANOMALOUS COSMIC RAYS IN THE HELIOSPHERE: OBSERVATIONS, SIMULATIONS AND THEORY,23(3),#REF!.
MLA Tibet ASγ Collaboration."Sun's shadow by 10 TeV cosmic rays under the influence of solar activity".TRANSPORT OF GALACTIC AND ANOMALOUS COSMIC RAYS IN THE HELIOSPHERE: OBSERVATIONS, SIMULATIONS AND THEORY 23.3(1999):#REF!.

入库方式: OAI收割

来源:高能物理研究所

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