書誌事項
- タイトル別名
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- Solar activity research of the Sporer minimum
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It is known that the periods when solar activity was extremely weak (so-called grand minima) existed several times in the last 1000 years. It is reported by Kocharov et al. that the solar activity periodicity during the Maunder minimum was not the 11 year variation but the 22 year variation. What does the cycle of 22 years mean? Does the periodicity of 22 years exist also in the minima other than the Maunder minimum? We have investigated the solar activity of the Sporer minimum, which preceded the Maunder minimum, in order to understand the periodicity of solar activity during the minima. Both the liquid scintillation method and the accelerator mass spectrometry method (AMS method) were used for measuring the ^<14>C concentration in annual tree rings.
収録刊行物
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- 名古屋大学加速器質量分析計業績報告書
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名古屋大学加速器質量分析計業績報告書 13 110-117, 2002-03
名古屋大学年代測定資料研究センター
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詳細情報 詳細情報について
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- CRID
- 1390290699381261696
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- NII論文ID
- 110000475719
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- NII書誌ID
- AN10305282
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- HANDLE
- 2237/13545
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- 本文言語コード
- ja
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- データソース種別
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- JaLC
- IRDB
- CiNii Articles
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- 抄録ライセンスフラグ
- 使用可