Validation of coronal mass ejection arrival-time forecasts by magnetohydrodynamic simulations based on interplanetary scintillation observations

• Material Type: 記事
• Title: Validation of coronal mass ejection arrival-time forecasts by magnetohydrodynamic simulations based on interplanetary scintillation observations
• Author/Editor: Kazumasa Iwai; Daikou Shiota; Munetoshi Tokumaru
• Publication, Distribution, etc.: 日本 : Springer Nature
• Publication Date: 2021-01-06
• Publication Date (W3CDTF): 2021-01-06
• Periodical title: EPS : Earth, Planets and Space
• No. or year of volume/issue: 73(9)
• Volume: 73(9)
• ISSN (Periodical Title): 1880-5981
• ISSN-L (Periodical Title): 1343-8832
• Text Language Code: eng
• DOI: 10.1186/s40623-020-01345-5; https://doi.org/10.1186/s40623-020-01345-5
• Persistent ID (NDL): info:ndljp/pid/11667906; https://dl.ndl.go.jp/pid/11667906
• Collection: 障害者向け資料
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• Collection (particular): 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
• Acquisition Basis: オンライン資料収集制度
• Date Accepted (W3CDTF): 2021-04-28T11:35:34+09:00
• Date Captured (W3CDTF): 2021-04-28
• Format (IMT): application/pdf
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• Periodical Title (URI): https://earth-planets-space.springeropen.com/articles
• Periodical Title (Persistent ID (NDL)): info:ndljp/pid/11667897; https://dl.ndl.go.jp/pid/11667897
• Data Provider (Database): 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

• Summary, etc.: 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/s40623-020-01345-5; https://doi.org/10.1186/s40623-020-01345-5; 10.21203/rs.3.rs-32257/v1; https://doi.org/10.21203/rs.3.rs-32257/v1; 10.21203/rs.3.rs-32257/v3; https://doi.org/10.21203/rs.3.rs-32257/v3; 10.21203/rs.3.rs-32257/v2; https://doi.org/10.21203/rs.3.rs-32257/v2; 10.21203/rs.3.rs-32257/v4; https://doi.org/10.21203/rs.3.rs-32257/v4; 10.48550/arxiv.2012.12635; https://doi.org/10.48550/arxiv.2012.12635
• Access Restrictions: インターネット公開
• Related Material (URI): http://id.ndl.go.jp/digimeta/11667906; https://dl.ndl.go.jp/pid/11667906; https://www.researchsquare.com/article/rs-32257/v1; https://www.researchsquare.com/article/rs-32257/v1.html; https://www.researchsquare.com/article/rs-32257/v3; https://www.researchsquare.com/article/rs-32257/v3.html; https://www.researchsquare.com/article/rs-32257/v2; https://www.researchsquare.com/article/rs-32257/v2.html; http://link.springer.com/content/pdf/10.1186/s40623-020-01345-5.pdf; http://link.springer.com/article/10.1186/s40623-020-01345-5/fulltext.html; https://www.researchsquare.com/article/rs-32257/v4; https://www.researchsquare.com/article/rs-32257/v4.html
• Is Referenced By: The Solar and Geomagnetic Storms in 2024 May: A Flash Data Report; https://cir.nii.ac.jp/crid/1360306904396420864; Testing the Alfvén-wave Model of the Solar Wind with Interplanetary Scintillation; https://cir.nii.ac.jp/crid/1360579812086735360; Magnetohydrodynamic simulation of coronal mass ejections using interplanetary scintillation data observed from radio sites ISEE and LOFAR; https://cir.nii.ac.jp/crid/1360584341820448640; Application of novel interplanetary scintillation visualisations using LOFAR: A case study of merged CMEs from September 2017; https://cir.nii.ac.jp/crid/1360865815495438592; Forecasting Heliospheric CME Solar-Wind Parameters Using the UCSD Time-Dependent Tomography and ISEE Interplanetary Scintillation Data: The 10 March 2022 CME; https://cir.nii.ac.jp/crid/1360865816797729408; 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
• References: Magnetohydrodynamic simulation of interplanetary propagation of multiple coronal mass ejections with internal magnetic flux rope (SUSANOO‐CME); https://cir.nii.ac.jp/crid/1360002214350204544; A newly developed UHF radiotelescope for interplanetary scintillation observations: Solar Wind Imaging Facility; https://cir.nii.ac.jp/crid/1360004233289579648; Modeling 3-D solar wind structure; https://cir.nii.ac.jp/crid/1360011144218620800; Observing interplanetary disturbances from the ground; https://cir.nii.ac.jp/crid/1360011146195387264; The Large Angle Spectroscopic Coronagraph (LASCO); https://cir.nii.ac.jp/crid/1360011146255991424; Inner heliosphere MHD modeling system applicable to space weather forecasting for the other planets; https://cir.nii.ac.jp/crid/1360285704778136064; CONNECTING SPEEDS, DIRECTIONS AND ARRIVAL TIMES OF 22 CORONAL MASS EJECTIONS FROM THE SUN TO 1 AU; https://cir.nii.ac.jp/crid/1360292619883394304; Verification of real-time WSA−ENLIL+Cone simulations of CME arrival-time at the CCMC from 2010 to 2016; https://cir.nii.ac.jp/crid/1360292619950032256; Coronal flux ropes and their interplanetary counterparts; https://cir.nii.ac.jp/crid/1360292619989118080; Modeling of Flux Rope Coronal Mass Ejections; https://cir.nii.ac.jp/crid/1360292620111995264; On observing mass ejections in the interplanetary medium; https://cir.nii.ac.jp/crid/1360292620172618496; Heliospheric tomography using interplanetary scintillation observations: 2. Latitude and heliocentric distance dependence of solar wind structure at 0.1–1 AU; https://cir.nii.ac.jp/crid/1360574095701920128; Interplanetary Scintillation of Small Diameter Radio Sources; https://cir.nii.ac.jp/crid/1360855568934122624; Tracking heliospheric disturbances by interplanetary scintillation; https://cir.nii.ac.jp/crid/1360855570676284800; Automated recognition of coronal mass ejections (CMEs) in near-real-time data; https://cir.nii.ac.jp/crid/1360855571334414464; Ensemble Modeling of CME Propagation; https://cir.nii.ac.jp/crid/1361137046112870912; MEASURING AN ERUPTIVE PROMINENCE AT LARGE DISTANCES FROM THE SUN. II. APPROACHING 1 AU; https://cir.nii.ac.jp/crid/1361418520156429824; CME Projection Effects Studied with STEREO/COR and SOHO/LASCO; https://cir.nii.ac.jp/crid/1361418520223693312; 3D Reconstruction of Interplanetary Scintillation (IPS) Remote-Sensing Data: Global Solar Wind Boundaries for Driving 3D-MHD Models; https://cir.nii.ac.jp/crid/1361699995617916800; EUHFORIA: European heliospheric forecasting information asset; https://cir.nii.ac.jp/crid/1361699996003300864; “Yin‐Yang grid”: An overset grid in spherical geometry; https://cir.nii.ac.jp/crid/1362544420968626560; A catalog of white light coronal mass ejections observed by the SOHO spacecraft; https://cir.nii.ac.jp/crid/1362825893624387712; Improvement in the prediction of solar wind conditions using near‐real time solar magnetic field updates; https://cir.nii.ac.jp/crid/1362825894509562240; Solar and interplanetary sources of major geomagnetic storms (<i>Dst</i> ≤ −100 nT) during 1996–2005; https://cir.nii.ac.jp/crid/1362825895117149312; An Intense Flare–CME Event in 2015: Propagation and Interaction Effects Between the Sun and Earth’s Orbit; https://cir.nii.ac.jp/crid/1362825895294019840; Interplanetary-scintillation observations of coronal mass ejections near the maximum of the 24th solar-activity cycle; https://cir.nii.ac.jp/crid/1363107368408780544; Influence of the aerodynamic drag on the motion of interplanetary ejecta; https://cir.nii.ac.jp/crid/1363107368751424896; Evolution of Coronal Mass Ejections in the Inner Heliosphere: A Study Using White-Light and Scintillation Images; https://cir.nii.ac.jp/crid/1363107371324578816; An operational software tool for the analysis of coronagraph images: Determining CME parameters for input into the WSA‐Enlil heliospheric model; https://cir.nii.ac.jp/crid/1363388844167333888; Interpretation of Interplanetary Scintillations; https://cir.nii.ac.jp/crid/1363388844227842432; Stream structure and coronal sources of the solar wind during the May 12th, 1997 CME; https://cir.nii.ac.jp/crid/1363388845556800384; Heliospheric tomography using interplanetary scintillation observations: 1. Combined Nagoya and Cambridge data; https://cir.nii.ac.jp/crid/1363388846138682240; Theory of prominence eruption and propagation: Interplanetary consequences; https://cir.nii.ac.jp/crid/1363670319557919488; Toroidal‐shaped interplanetary disturbance associated with the halo coronal mass ejection event on 14 July 2000; https://cir.nii.ac.jp/crid/1363951795045943680; MHD tomography using interplanetary scintillation measurement; https://cir.nii.ac.jp/crid/1363951796068716288; Predicting the 1‐AU arrival times of coronal mass ejections; https://cir.nii.ac.jp/crid/1364233268911071744; Solar wind speed and coronal flux-tube expansion; https://cir.nii.ac.jp/crid/1364233268928176128; Forecasting the Arrival Time of Coronal Mass Ejections: Analysis of the CCMC CME Scoreboard; https://cir.nii.ac.jp/crid/1364233269274582272; The UCSD kinematic IPS solar wind boundary and its use in the ENLIL 3‐D MHD prediction model; https://cir.nii.ac.jp/crid/1364233270041059200; Development of a coronal mass ejection arrival time forecasting system using interplanetary scintillation observations; https://cir.nii.ac.jp/crid/2050870367067472128
• Data Provider (Database): 国立情報学研究所 : CiNii Research; https://cir.nii.ac.jp/
• Original Data Provider (Database): 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
• Bibliographic ID (NDL): 11667906; http://id.ndl.go.jp/bib/11667906