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gdj3.140.pdf | 12.27 MB | Adobe PDF | 見る/開く |
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DCフィールド | 値 | 言語 |
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dc.contributor.author | Hayakawa, Hisashi | en |
dc.contributor.author | Ebihara, Yusuke | en |
dc.contributor.author | Hata, Hidetoshi | en |
dc.contributor.alternative | 早川, 尚志 | ja |
dc.contributor.alternative | 海老原, 祐輔 | ja |
dc.contributor.alternative | 畑, 英利 | ja |
dc.date.accessioned | 2023-01-17T06:46:15Z | - |
dc.date.available | 2023-01-17T06:46:15Z | - |
dc.date.issued | 2023-01 | - |
dc.identifier.uri | http://hdl.handle.net/2433/278451 | - |
dc.description | 歴史的観測から蘇る1957~1958年のオーロラ観測の全貌:過去4世紀最大の太陽活動極大期に起きた太陽嵐の痕跡. 京都大学プレスリリース. 2022-03-28. | ja |
dc.description.abstract | Solar Cycle 19 was probably the greatest solar cycle over the last four centuries and significantly disrupted the solar-terrestrial environments with a number of solar eruptions and resultant geomagnetic storms. At its peak, the International Geophysical Year (IGY: 1957–1958) was organised under international collaborations and benefitted scientific developments, capturing multiple unique extreme space weather events including the third and fourth greatest geomagnetic storms in the space age. In this article, we review and analyse original records of Japanese auroral observations around the IGY. These observations were organised by Masaaki Huruhata in collaboration with professional observatories and citizen contributors. We have digitised and documented these source documents, which comprise significant auroral displays in March 1957 (minimum Dst = −255 nT), September 1957 (minimum Dst = −427 nT), and February 1958 (minimum Dst = −426 nT). These records allow us to visualise temporal and spatial evolutions of these auroral displays, reconstruct their equatorward auroral boundaries down to 41.5°, 38.3°, and 33.3° in invariant latitudes, and contextualise their occurrences following contemporary geomagnetic disturbances. Our results have been compared with significant auroral displays during other extreme space weather events. These aurorae generally showed reddish colourations occasionally with yellowish rays. Their colourations are attributed to reddish oxygen emission and its mixture with greenish oxygen emission. Overall, these archival records provide the references for future discussions on the auroral activities during the uniquely intense and extreme space weather events. | en |
dc.language.iso | eng | - |
dc.publisher | Royal Meteorological Society | en |
dc.publisher | Wiley | en |
dc.rights | © 2021 The Authors. Geoscience Data Journal published by Royal Meteorological Society and John Wiley & Sons Ltd. | en |
dc.rights | This is an open access article under the terms of the Creative Commons Attribution License, which permits use, distribution and reproduction in any medium, provided the original work is properly cited. | en |
dc.rights.uri | http://creativecommons.org/licenses/by/4.0/ | - |
dc.subject | aurorae | en |
dc.subject | geomagnetic storms | en |
dc.subject | International Geophysical Year | en |
dc.subject | Solar Cycle 19 | en |
dc.subject | space weather | en |
dc.title | A review for Japanese auroral records on the three extreme space weather events around the International Geophysical Year (1957–1958) | en |
dc.type | journal article | - |
dc.type.niitype | Journal Article | - |
dc.identifier.jtitle | Geoscience Data Journal | en |
dc.identifier.volume | 10 | - |
dc.identifier.issue | 1 | - |
dc.identifier.spage | 142 | - |
dc.identifier.epage | 157 | - |
dc.relation.doi | 10.1002/gdj3.140 | - |
dc.textversion | publisher | - |
dc.address | Institute for Space-Earth Environmental Research, Nagoya Universit; Institute for Advanced Research, Nagoya University; Rutherford Appleton Laboratory, RAL Space, Science and Technology Facilities Council; Nishina Centre, Riken | en |
dc.address | Research Institute for Sustainable Humanosphere, Kyoto University; Unit of Synergetic Studies for Space, Kyoto University | en |
dc.address | Kisomachi Junior High School; Kiso Observatory, Institute of Astronomy, School of Science, The University of Tokyo | en |
dc.relation.url | https://www.kyoto-u.ac.jp/ja/research-news/2022-03-28-2 | - |
dcterms.accessRights | open access | - |
datacite.awardNumber | 20K22367 | - |
datacite.awardNumber | 20K20918 | - |
datacite.awardNumber | 20H05643 | - |
datacite.awardNumber | 21K13957 | - |
datacite.awardNumber.uri | https://kaken.nii.ac.jp/grant/KAKENHI-PROJECT-20K22367/ | - |
datacite.awardNumber.uri | https://kaken.nii.ac.jp/grant/KAKENHI-PROJECT-20K20918/ | - |
datacite.awardNumber.uri | https://kaken.nii.ac.jp/grant/KAKENHI-PROJECT-20H05643/ | - |
datacite.awardNumber.uri | https://kaken.nii.ac.jp/grant/KAKENHI-PROJECT-21K13957/ | - |
dc.identifier.eissn | 2049-6060 | - |
jpcoar.funderName | 日本学術振興会 | ja |
jpcoar.funderName | 日本学術振興会 | ja |
jpcoar.funderName | 日本学術振興会 | ja |
jpcoar.funderName | 日本学術振興会 | ja |
jpcoar.awardTitle | 近代アナログ観測を用いた激甚宇宙天気現象の規模推定・定量比較の試験的研究 | ja |
jpcoar.awardTitle | 宇宙線生成核種を用いたシュワーベサイクル検出手法の確立 | ja |
jpcoar.awardTitle | 過去1万年間の太陽活動 | ja |
jpcoar.awardTitle | 同時代黒点観測の歴史的文書に基づくダルトン極小期復元の試験的検討 | ja |
出現コレクション: | 学術雑誌掲載論文等 |

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