Relationship between three-dimensional velocity of filament eruptions and CME association
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DOI[10.1186/s40623-021-01378-4]to the data of the same series
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- Material Type
- 記事
- Author/Editor
- Daikichi SekiKenichi OtsujiTakako T. Ishii
- Publication, Distribution, etc.
- Publication Date
- 2021-02-26
- Publication Date (W3CDTF)
- 2021-02-26
- Periodical title
- EPS : Earth, Planets and Space
- No. or year of volume/issue
- 73(58)
- Volume
- 73(58)
- ISSN (Periodical Title)
- 1880-5981
- ISSN-L (Periodical Title)
- 1343-8832
- Text Language Code
- eng
- DOI
- 10.1186/s40623-021-01378-4
- Persistent ID (NDL)
- info:ndljp/pid/11667955
- Collection
- Collection (Materials For Handicapped People:1)
- 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
- 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
- Access Restrictions
- 国立国会図書館内限定公開
- Service for the Digitized Contents Transmission Service
- 図書館・個人送信対象外
- Availability of remote photoduplication service
- 可
- Periodical Title (URI)
- Periodical Title (Persistent ID (NDL))
- info:ndljp/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
- 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/s40623-021-01378-410.48550/arxiv.2102.0457810.17863/cam.65288
- Related Material (URI)
- Is Referenced By
- Probable detection of an eruptive filament from a superflare on a solar-type starMultiwavelength Campaign Observations of a Young Solar-type Star, EK Draconis. II. Understanding Prominence Eruption through Data-driven Modeling and Observed Magnetic EnvironmentApache 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 DataSimple Model for Temporal Variations of Hα Spectrum by an Eruptive Filament from a Superflare on a Solar-type StarMultiwavelength Campaign Observations of a Young Solar-type Star, EK Draconis. I. Discovery of Prominence Eruptions Associated with SuperflaresHigh-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 EruptionsSpecial issue "Solar-terrestrial environment prediction : toward the synergy of science and forecasting operation of space weather and space climate"PSTEP : project for solar–terrestrial environment prediction
- References
- A filament eruption and accompanying coronal field changes on November 5, 1992The Nobeyama radioheliographAssessment of Geomagnetic Hazard to Power Systems in Canada<i>Hinode</i>,<i>TRACE</i>,<i>SOHO</i>, and Ground‐based Observations of a Quiescent ProminenceSmall-scale motions in solar filaments as the precursors of eruptionsOn the Relation between Filament Eruptions, Flares, and Coronal Mass EjectionsActive and Eruptive Prominences and Their Relationship to Coronal Mass EjectionsA New Solar Imaging System for Observing High-Speed Eruptions: Solar Dynamics Doppler Imager (SDDI)Machine Leaning-Based Investigation of the Associations between CMEs and FilamentsIncrease in the Amplitude of Line-of-sight Velocities of the Small-scale Motions in a Solar Filament before EruptionThe Large Angle Spectroscopic Coronagraph (LASCO)Eruptive Prominences and Their Association with Coronal Mass EjectionsThe Atmospheric Imaging Assembly (AIA) on the Solar Dynamics Observatory (SDO)MODELING THE METALLICITY DISTRIBUTION OF GLOBULAR CLUSTERSObservation of a coronal transient from 1.2 to 6 solar radiiA large polar crown coronal mass ejection and a “problem” goemagnetic storm: April 14–23, 1994A catalog of white light coronal mass ejections observed by the SOHO spacecraftSolar Prominences: ObservationsProminence Eruptions and Coronal Mass Ejection: A Statistical Study Using Microwave ObservationsGlobular cluster population of the HST Frontier Fields galaxy J07173724+3744224On the sudden disappearances of solar filamentsand their relationship with coronal mass ejectionsApplication of a New Technique for Deriving Prominence Mass from<i>SOHO</i>EIT Fe<scp>xii</scp>(19.5 nm) Absorption FeaturesEruptive and Quasi-Eruptive Disappearing Solar Filaments and Their Relationship with Coronal ActivitiesDetecting bimodality in astronomical datasetsTrajectories of microwave prominence eruptionsProminence and Filament Eruptions Observed by the Solar Dynamics Observatory: Statistical Properties, Kinematics, and Online Catalog
- Data Provider (Database)
- 国立情報学研究所 : CiNii Research
- Original Data Provider (Database)
- 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科学研究費助成事業データベースCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossref
- Bibliographic ID (NDL)
- 11667955