Relationship between three-dimensional velocity of filament eruptions and CME association

• 資料種別: 記事
• タイトル: Relationship between three-dimensional velocity of filament eruptions and CME association
• 著者・編者: Daikichi Seki; Kenichi Otsuji; Takako T. Ishii
• 出版事項: 日本 : Springer Nature
• 出版年月日等: 2021-02-26
• 出版年（W3CDTF）: 2021-02-26
• タイトル（掲載誌）: EPS : Earth, Planets and Space
• 巻号年月日等（掲載誌）: 73(58)
• 掲載巻: 73(58)
• 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/s40623-021-01378-4; https://doi.org/10.1186/s40623-021-01378-4
• 国立国会図書館永続的識別子: info:ndljp/pid/11667955; https://dl.ndl.go.jp/pid/11667955
• 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）: 2021-04-28T11:35:34+09:00
• 保存日（W3CDTF）: 2021-04-28
• 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/11667897; https://dl.ndl.go.jp/pid/11667897
• 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/s40623-021-01378-4; https://doi.org/10.1186/s40623-021-01378-4; 10.48550/arxiv.2102.04578; https://doi.org/10.48550/arxiv.2102.04578; 10.17863/cam.65288; https://doi.org/10.17863/cam.65288
• 関連情報（URI）: http://id.ndl.go.jp/digimeta/11667955; https://dl.ndl.go.jp/pid/11667955; http://link.springer.com/content/pdf/10.1186/s40623-021-01378-4.pdf; http://link.springer.com/article/10.1186/s40623-021-01378-4/fulltext.html
• 参照: Probable detection of an eruptive filament from a superflare on a solar-type star; https://cir.nii.ac.jp/crid/1050572633033232896; Multiwavelength Campaign Observations of a Young Solar-type Star, EK Draconis. II. Understanding Prominence Eruption through Data-driven Modeling and Observed Magnetic Environment; https://cir.nii.ac.jp/crid/1050583933990844800; Apache Point Observatory (APO)/SMARTS Flare Star Campaign Observations. I. Blue Wing Asymmetries in Chromospheric Lines during Mid-M-Dwarf Flares from Simultaneous Spectroscopic and Photometric Observation Data; https://cir.nii.ac.jp/crid/1360021389808607360; Simple Model for Temporal Variations of Hα Spectrum by an Eruptive Filament from a Superflare on a Solar-type Star; https://cir.nii.ac.jp/crid/1360306906079577600; Multiwavelength Campaign Observations of a Young Solar-type Star, EK Draconis. I. Discovery of Prominence Eruptions Associated with Superflares; https://cir.nii.ac.jp/crid/1360865815514802688; High-time-cadence Spectroscopy and Photometry of Stellar Flares on M dwarf YZ Canis Minoris with the Seimei Telescope and TESS. I. Discovery of Rapid and Short-duration Prominence Eruptions; https://cir.nii.ac.jp/crid/1360869855143598848; Special issue "Solar-terrestrial environment prediction : toward the synergy of science and forecasting operation of space weather and space climate"; https://cir.nii.ac.jp/crid/2050307417129948032; PSTEP : project for solar–terrestrial environment prediction; https://cir.nii.ac.jp/crid/2050588892104455680
• 参照: A filament eruption and accompanying coronal field changes on November 5, 1992; https://cir.nii.ac.jp/crid/1360011143714501120; The Nobeyama radioheliograph; https://cir.nii.ac.jp/crid/1360292617907055616; Assessment of Geomagnetic Hazard to Power Systems in Canada; https://cir.nii.ac.jp/crid/1360292619708983808; <i>Hinode</i>,<i>TRACE</i>,<i>SOHO</i>, and Ground‐based Observations of a Quiescent Prominence; https://cir.nii.ac.jp/crid/1360292621044329472; Small-scale motions in solar filaments as the precursors of eruptions; https://cir.nii.ac.jp/crid/1360567184690185216; On the Relation between Filament Eruptions, Flares, and Coronal Mass Ejections; https://cir.nii.ac.jp/crid/1360574095291895680; Active and Eruptive Prominences and Their Relationship to Coronal Mass Ejections; https://cir.nii.ac.jp/crid/1360574095697062272; A New Solar Imaging System for Observing High-Speed Eruptions: Solar Dynamics Doppler Imager (SDDI); https://cir.nii.ac.jp/crid/1360846640362071424; Machine Leaning-Based Investigation of the Associations between CMEs and Filaments; https://cir.nii.ac.jp/crid/1360855569059967744; Increase in the Amplitude of Line-of-sight Velocities of the Small-scale Motions in a Solar Filament before Eruption; https://cir.nii.ac.jp/crid/1360855570878717184; The Large Angle Spectroscopic Coronagraph (LASCO); https://cir.nii.ac.jp/crid/1361137045416810880; Eruptive Prominences and Their Association with Coronal Mass Ejections; https://cir.nii.ac.jp/crid/1361699993681562240; The Atmospheric Imaging Assembly (AIA) on the Solar Dynamics Observatory (SDO); https://cir.nii.ac.jp/crid/1362262945745626752; MODELING THE METALLICITY DISTRIBUTION OF GLOBULAR CLUSTERS; https://cir.nii.ac.jp/crid/1362262946104363648; Observation of a coronal transient from 1.2 to 6 solar radii; https://cir.nii.ac.jp/crid/1362262946161752960; A large polar crown coronal mass ejection and a “problem” goemagnetic storm: April 14–23, 1994; https://cir.nii.ac.jp/crid/1362544421035419776; A catalog of white light coronal mass ejections observed by the SOHO spacecraft; https://cir.nii.ac.jp/crid/1362825893624387712; Solar Prominences: Observations; https://cir.nii.ac.jp/crid/1362825894310759936; Prominence Eruptions and Coronal Mass Ejection: A Statistical Study Using Microwave Observations; https://cir.nii.ac.jp/crid/1363107368933594368; Globular cluster population of the HST Frontier Fields galaxy J07173724+3744224; https://cir.nii.ac.jp/crid/1363388846003963136; On the sudden disappearances of solar filamentsand their relationship with coronal mass ejections; https://cir.nii.ac.jp/crid/1363670320990389504; Application of a New Technique for Deriving Prominence Mass from<i>SOHO</i>EIT Fe<scp>xii</scp>(19.5 nm) Absorption Features; https://cir.nii.ac.jp/crid/1364233268307862912; Eruptive and Quasi-Eruptive Disappearing Solar Filaments and Their Relationship with Coronal Activities; https://cir.nii.ac.jp/crid/1364233268375282816; Detecting bimodality in astronomical datasets; https://cir.nii.ac.jp/crid/1364233270278553344; Trajectories of microwave prominence eruptions; https://cir.nii.ac.jp/crid/1364233271000541056; Prominence and Filament Eruptions Observed by the Solar Dynamics Observatory: Statistical Properties, Kinematics, and Online Catalog; https://cir.nii.ac.jp/crid/1364233271125831552
• 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
• 書誌ID（NDLBibID）: 11667955; http://id.ndl.go.jp/bib/11667955