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
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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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