Development of a coronal mass ejection arrival time forecasting system using interplanetary scintillation observations
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DOI[10.1186/s40623-019-1019-5]のデータに遷移します
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- 資料種別
- 記事
- 著者・編者
- Kazumasa IwaiDaikou ShiotaMunetoshi Tokumaru
- 出版年月日等
- 2019-04-04
- 出版年(W3CDTF)
- 2019-04-04
- タイトル(掲載誌)
- EPS : Earth, Planets and Space
- 巻号年月日等(掲載誌)
- 71(39)
- 掲載巻
- 71(39)
- 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/s40623-019-1019-5
- 国立国会図書館永続的識別子
- info:ndljp/pid/11286873
- コレクション(共通)
- コレクション(障害者向け資料:レベル1)
- 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
- 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(国立国会図書館永続的識別子)
- info:ndljp/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
- 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/s40623-019-1019-510.48550/arxiv.1903.11769
- 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)
- 参照
- Spectral Structures of Type II Solar Radio Bursts and Solar Energetic ParticlesBepiColombo Science Investigations During Cruise and Flybys at the Earth, Venus and MercuryThe Solar and Geomagnetic Storms in 2024 May: A Flash Data ReportVenus's induced magnetosphere during active solar wind conditions at BepiColombo's Venus 1 flybyTesting the Alfvén-wave Model of the Solar Wind with Interplanetary ScintillationMagnetohydrodynamic simulation of coronal mass ejections using interplanetary scintillation data observed from radio sites ISEE and LOFARApplication of novel interplanetary scintillation visualisations using LOFAR: A case study of merged CMEs from September 2017Structure of Solar Atmosphere and Magnetic PhenomenaForecasting Heliospheric CME Solar-Wind Parameters Using the UCSD Time-Dependent Tomography and ISEE Interplanetary Scintillation Data: The 10 March 2022 CMEValidation of coronal mass ejection arrival-time forecasts by magnetohydrodynamic simulations based on interplanetary scintillation observationsPSTEP : project for solar–terrestrial environment prediction
- 参照
- Radial speed evolution of coronal mass ejections during solar cycle 23Kinematic Properties of Slow ICMEs and an Interpretation of a Modified Drag Equation for Fast and Moderate ICMEsMagnetohydrodynamic simulation of interplanetary propagation of multiple coronal mass ejections with internal magnetic flux rope (SUSANOO‐CME)A newly developed UHF radiotelescope for interplanetary scintillation observations: Solar Wind Imaging FacilityModeling 3-D solar wind structureThree‐dimensional propagation of interplanetary disturbances detected with radio scintillation measurements at 327 MHzObserving interplanetary disturbances from the groundThe Large Angle Spectroscopic Coronagraph (LASCO)Inner heliosphere MHD modeling system applicable to space weather forecasting for the other planetsSpacecraft radio scattering observations of the power spectrum of electron density fluctuations in the solar windHeliospheric tomography using interplanetary scintillation observations: 2. Latitude and heliocentric distance dependence of solar wind structure at 0.1–1 AUElEvoHI: A NOVEL CME PREDICTION TOOL FOR HELIOSPHERIC IMAGING COMBINING AN ELLIPTICAL FRONT WITH DRAG-BASED MODEL FITTINGTracking heliospheric disturbances by interplanetary scintillationTime-dependent tomography of hemispheric features using interplanetary scintillation (IPS) remote-sensing observationsWhy the Shock-ICME Complex Structure Is Important: Learning from the Early 2017 September CMEs3D Reconstruction of Interplanetary Scintillation (IPS) Remote-Sensing Data: Global Solar Wind Boundaries for Driving 3D-MHD ModelsAUTOMATED LASCO CME CATALOG FOR SOLAR CYCLE 23: ARE CMEs SCALE INVARIANT?“Yin‐Yang grid”: An overset grid in spherical geometryA catalog of white light coronal mass ejections observed by the SOHO spacecraftImprovement in the prediction of solar wind conditions using near‐real time solar magnetic field updatesAn Intense Flare–CME Event in 2015: Propagation and Interaction Effects Between the Sun and Earth’s OrbitModeling observations of solar coronal mass ejections with heliospheric imagers verified with the Heliophysics System ObservatoryInterplanetary-scintillation observations of coronal mass ejections near the maximum of the 24th solar-activity cycleInfluence of the aerodynamic drag on the motion of interplanetary ejectaEvolution of Coronal Mass Ejections in the Inner Heliosphere: A Study Using White-Light and Scintillation ImagesInterpretation of Interplanetary ScintillationsThree-dimensional reconstruction of heliospheric structure using iterative tomography: A reviewHeliospheric tomography using interplanetary scintillation observations: 1. Combined Nagoya and Cambridge dataTheory of prominence eruption and propagation: Interplanetary consequencesToroidal‐shaped interplanetary disturbance associated with the halo coronal mass ejection event on 14 July 2000MHD tomography using interplanetary scintillation measurementPredicting the 1‐AU arrival times of coronal mass ejectionsThe UCSD kinematic IPS solar wind boundary and its use in the ENLIL 3‐D MHD prediction model
- 連携機関・データベース
- 国立情報学研究所 : CiNii Research
- 提供元機関・データベース
- 雑誌記事索引データベースCrossref科学研究費助成事業データベース科学研究費助成事業データベースCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossref
- 書誌ID(NDLBibID)
- 11286873