Relationship between the low-latitude coronal hole area, solar wind velocity, and geomagnetic activity during solar cycles 23 and 24

• 資料種別: 記事
• タイトル: Relationship between the low-latitude coronal hole area, solar wind velocity, and geomagnetic activity during solar cycles 23 and 24
• 著者・編者: Yumi Nakagawa; Satoshi Nozawa; Atsuki Shinbori
• 出版事項: 日本 : Springer Nature
• 出版年月日等: 2019-02-28
• 出版年（W3CDTF）: 2019-02-28
• タイトル（掲載誌）: EPS : Earth, Planets and Space
• 巻号年月日等（掲載誌）: 71(24)
• 掲載巻: 71(24)
• ISSN（掲載誌）: 1880-5981
• ISSN-L（掲載誌）: 1343-8832
• 本文の言語コード: eng
• DOI: 10.1186/s40623-019-1005-y; https://doi.org/10.1186/s40623-019-1005-y
• 国立国会図書館永続的識別子: info:ndljp/pid/11286858; https://dl.ndl.go.jp/pid/11286858
• コレクション（共通）: 障害者向け資料
• コレクション（障害者向け資料：レベル1）: テキストデータ
• コレクション（個別）: 国立国会図書館デジタルコレクション > 電子書籍・電子雑誌 > その他; https://dl.ndl.go.jp/collections/B00035
• 収集根拠: オンライン資料収集制度
• 受理日（W3CDTF）: 2019-05-27T20:17:25+09:00
• 保存日（W3CDTF）: 2019-05-27
• 記録形式（IMT）: application/pdf
• オンライン閲覧公開範囲: 国立国会図書館内限定公開
• デジタル化資料送信: 図書館・個人送信対象外
• 遠隔複写可否（NDL）: 可
• 掲載誌（URI）: https://earth-planets-space.springeropen.com/articles
• 掲載誌（国立国会図書館永続的識別子）: info:ndljp/pid/11245705; https://dl.ndl.go.jp/pid/11245705
• 連携機関・データベース: 国立国会図書館 : 国立国会図書館デジタルコレクション; https://dl.ndl.go.jp

• 要約等: コレクション : 国立国会図書館デジタルコレクション > 電子書籍・電子雑誌 > その他
• DOI: 10.1186/s40623-019-1005-y; https://doi.org/10.1186/s40623-019-1005-y
• オンライン閲覧公開範囲: インターネット公開
• 関連情報（URI）: http://id.ndl.go.jp/digimeta/11286858; https://dl.ndl.go.jp/pid/11286858; http://link.springer.com/content/pdf/10.1186/s40623-019-1005-y.pdf; http://link.springer.com/article/10.1186/s40623-019-1005-y/fulltext.html
• 参照: Earth’s geomagnetic response to solar wind changes associated with solar events at low latitude regions at the TRE MAGDAS Station; https://cir.nii.ac.jp/crid/1360017280651847936
• 参照: Relation Between Coronal Hole Areas and Solar Wind Speeds Derived from Interplanetary Scintillation Measurements; https://cir.nii.ac.jp/crid/1050845763735833344; Is Something Wrong With the Present Solar Maximum?; https://cir.nii.ac.jp/crid/1360004230308973184; Statistical properties of coronal hole rotation rates: Are they linked to the solar interior?; https://cir.nii.ac.jp/crid/1360011145298928000; The Atmospheric Imaging Assembly (AIA) on the Solar Dynamics Observatory (SDO); https://cir.nii.ac.jp/crid/1360292617917560448; EIT: Extreme-ultraviolet Imaging Telescope for the SOHO mission; https://cir.nii.ac.jp/crid/1360292619139608832; Solar Wind and Interplanetary Magnetic Field: A Tutorial; https://cir.nii.ac.jp/crid/1360292619677556608; Coronal Holes and Solar Wind High-Speed Streams: I. Forecasting the Solar Wind Parameters; https://cir.nii.ac.jp/crid/1360574095006327296; A Study of Coronal Holes Observed by SOHO/EIT and the Nobeyama Radioheliograph; https://cir.nii.ac.jp/crid/1360574095862574592; Geoeffectiveness of corotating interaction regions as measured by <i>Dst</i> index; https://cir.nii.ac.jp/crid/1360574095902606080; Analysis software for upper atmospheric data developed by the IUGONET project and its application to polar science; https://cir.nii.ac.jp/crid/1360848664542472960; Real-Time Solar Wind Prediction Based on SDO/AIA Coronal Hole Data; https://cir.nii.ac.jp/crid/1360855569335184512; Forecasting the Maxima of Solar Cycle 24 with Coronal Fe xiv Emission; https://cir.nii.ac.jp/crid/1360855569653631616; Space Weather: The Solar Perspective; https://cir.nii.ac.jp/crid/1360855570190773504; THE BEHAVIOR OF THE 17 GHz SOLAR RADIUS AND LIMB BRIGHTENING IN THE SPOTLESS MINIMUM XXIII/XXIV; https://cir.nii.ac.jp/crid/1361137044054126592; The solar magnetic activity band interaction and instabilities that shape quasi-periodic variability; https://cir.nii.ac.jp/crid/1361137045095601024; Sunspot cycle 24: Smallest cycle in 100 years?; https://cir.nii.ac.jp/crid/1361418519698700288; Statistical analysis of corotating interaction regions and their geoeffectiveness during solar cycle 23; https://cir.nii.ac.jp/crid/1361418519739948288; Comparing Solar Minimum 23/24 with Historical Solar Wind Records at 1 AU; https://cir.nii.ac.jp/crid/1361418520720503936; Polar Coronal Holes During Cycles 22 and 23; https://cir.nii.ac.jp/crid/1361418521209970944; Solar wind high-speed streams and related geomagnetic activity in the declining phase of solar cycle 23; https://cir.nii.ac.jp/crid/1361981469473927424; Coronal holes, solar wind streams, and geomagnetic activity during the new sunspot cycle; https://cir.nii.ac.jp/crid/1362262944730103296; Differences between CME‐driven storms and CIR‐driven storms; https://cir.nii.ac.jp/crid/1362262945041133952; Long-Term Global Solar Activity Observed by the Nobeyama Radioheliograph; https://cir.nii.ac.jp/crid/1362544419320897920; Flux enhancement of radiation belt electrons during geomagnetic storms driven by coronal mass ejections and corotating interaction regions; https://cir.nii.ac.jp/crid/1362544419633490432; Verification of high‐speed solar wind stream forecasts using operational solar wind models; https://cir.nii.ac.jp/crid/1362544419775365120; Introduction to special section on corotating solar wind streams and recurrent geomagnetic activity; https://cir.nii.ac.jp/crid/1362825894237166080; The differences between storms driven by helmet streamer CIRs and storms driven by pseudostreamer CIRs; https://cir.nii.ac.jp/crid/1362825895379341568; Corotating solar wind streams and recurrent geomagnetic activity: A review; https://cir.nii.ac.jp/crid/1363670318234871808; Equatorial coronal holes, solar wind high-speed streams, and their geoeffectiveness; https://cir.nii.ac.jp/crid/1363670320099053440; Solar wind observations at STEREO: 2007 - 2011; https://cir.nii.ac.jp/crid/1363670320232779648; Properties of Stream Interactions at One AU During 1995 – 2004; https://cir.nii.ac.jp/crid/1363670320603387776; Relation Between Coronal Hole Areas on the Sun and the Solar Wind Parameters at 1 AU; https://cir.nii.ac.jp/crid/1363670321146552576; Reversals of the Sun’s Polar Magnetic Fields in Relation to Activity Complexes and Coronal Holes; https://cir.nii.ac.jp/crid/1363951793583924864; Coronal Holes; https://cir.nii.ac.jp/crid/1363951794339899520; Coronal holes, solar wind streams, and geomagnetic disturbances during 1978 and 1979; https://cir.nii.ac.jp/crid/1363951794582917888; Coronal Holes and Open Magnetic Flux over Cycles 23 and 24; https://cir.nii.ac.jp/crid/1363951794719463296; BEHAVIOR OF SOLAR CYCLES 23 AND 24 REVEALED BY MICROWAVE OBSERVATIONS; https://cir.nii.ac.jp/crid/1363951794784006144; IUGONET project team, Inter-university Upper Atmosphere Global Observation NETwork (IUGONET); https://cir.nii.ac.jp/crid/1390001205233255552; Short-term variability of the Sun-Earth system : an overview of progress made during the CAWSES-II period; https://cir.nii.ac.jp/crid/2050307417166181888; Geomagnetic storms of cycle 24 and their solar sources; https://cir.nii.ac.jp/crid/2050588891962946944
• 参照（URI）: https://cir.nii.ac.jp/crid/1370848661783397894
• 連携機関・データベース: 国立情報学研究所 : CiNii Research; https://cir.nii.ac.jp/
• 提供元機関・データベース: 雑誌記事索引データベース; https://ndlsearch.ndl.go.jp; Crossref; https://www.crossref.org; 科学研究費助成事業データベース; https://kaken.nii.ac.jp/ja