中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Evaluation of the Interplanetary Magnetic Field Strength Using the Cosmic-Ray Shadow of the Sun

文献类型:期刊论文

作者Tibet ASy Collaboration
刊名PHYSICAL REVIEW LETTERS
出版日期2018
卷号120期号:3页码:31101
ISSN号0031-9007
DOI10.1103/PhysRevLett.120.031101
文献子类Article
英文摘要We analyze the Sun's shadow observed with the Tibet-III air shower array and find that the shadow's center deviates northward (southward) from the optical solar disk center in the "away" ("toward") interplanetary magnetic field (IMF) sector. By comparing with numerical simulations based on the solar magnetic field model, we find that the average IMF strength in the away (toward) sector is 1.54 +/- 0.21(stat) +/- 0.20(syst) (1.62 +/- 0.15(stat) +/- 0.22(syst)) times larger than the model prediction. These demonstrate that the observed Sun's shadow is a useful tool for the quantitative evaluation of the average solar magnetic field.
电子版国际标准刊号1079-7114
WOS关键词AIR-SHOWER ARRAY
WOS研究方向Physics
语种英语
WOS记录号WOS:000423131700002
源URL[http://ir.ihep.ac.cn/handle/311005/285550]  
专题高能物理研究所_粒子天体物理中心
作者单位中国科学院高能物理研究所
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Tibet ASy Collaboration. Evaluation of the Interplanetary Magnetic Field Strength Using the Cosmic-Ray Shadow of the Sun[J]. PHYSICAL REVIEW LETTERS,2018,120(3):31101.
APA Tibet ASy Collaboration.(2018).Evaluation of the Interplanetary Magnetic Field Strength Using the Cosmic-Ray Shadow of the Sun.PHYSICAL REVIEW LETTERS,120(3),31101.
MLA Tibet ASy Collaboration."Evaluation of the Interplanetary Magnetic Field Strength Using the Cosmic-Ray Shadow of the Sun".PHYSICAL REVIEW LETTERS 120.3(2018):31101.

入库方式: OAI收割

来源:高能物理研究所

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