Interplanetary coronal mass ejection and the sun's Shadow Observed by the Tibet Air Shower Array

Tibet ASγ Collaboration

研究成果: Conference article

抜粋

We continuously observed the Sun's shadow in 3 TeV cosmic-ray intensity with the Tibet-III air shower array since 2000. We find a clear solar-cycle variation of the deficit intensity in the Sun's shadow during the periods between 2000 and 2009. The MC simulation of the Sun's shadow based on the coronal magnetic field model does not well reproduce the observed deficit intensity around the solar maximum. However, when we exclude the transit periods during ICMEs towards to the Earth, the MC simulation shows better reproducibility. In the present paper, we report on the MC simulation and the analysis method of the Sun's shadow observed by the Tibet-III array.

元の言語English
ジャーナルProceedings of Science
出版物ステータスPublished - 2017 1 1
外部発表Yes
イベント35th International Cosmic Ray Conference, ICRC 2017 - Bexco, Busan, Korea, Republic of
継続期間: 2017 7 102017 7 20

ASJC Scopus subject areas

  • General

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