Magnetohydrodynamics modeling of coronal magnetic field and solar eruptions based on the photospheric magnetic field
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- 資料種別
- 記事
- 著者・編者
- Satoshi Inoue
- 出版年月日等
- 2016-07-04
- 出版年（W3CDTF）
- 2016-07-04
- タイトル（掲載誌）
- Progress in earth and planetary science
- 巻号年月日等（掲載誌）
- 3(19)
- 掲載巻
- 3(19)
- ISSN（掲載誌）
- 2197-4284
- ISSN-L（掲載誌）
- 2197-4284
- 本文の言語コード
- eng
- DOI
- 10.1186/s40645-016-0084-7
- 国立国会図書館永続的識別子
- info:ndljp/pid/10265302
- 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）
- 2017-01-19T19:10:18+09:00
- 保存日（W3CDTF）
- 2017-01-18
- 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/10016350
- 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/s40645-016-0084-7
- 関連情報（URI）
- 参照
- Data-driven MHD Simulation of Successive Solar Plasma EruptionsDistribution characteristics of coronal electric current density as an indicator for the occurrence of a solar flareNon-potential Field Formation in the X-shaped Quadrupole Magnetic Field ConfigurationThe Triggering of the 2014 March 29 Filament EruptionMagnetohydrodynamic Modeling of a Solar Eruption Associated with an X9.3 Flare Observed in the Active Region 12673A Comparative Study of Solar Active Region 12371 with Data-constrained and Data-driven Magnetohydrodynamic SimulationsData-driven MHD Simulation of the Formation of a Magnetic Flux Rope and an Inclined Solar EruptionFlare-productive active regionsExtrapolation of Three-dimensional Magnetic Field Structure in Flare-productive Active Regions with Different Initial ConditionsAn Evolution and Eruption of the Coronal Magnetic Field through a Data-driven MHD SimulationA Data-constrained Magnetohydrodynamic Simulation of the X1.0 Solar Flare of 2021 October 28Serial Flaring in an Active Region: Exploring Why Only One Flare Is EruptiveIntrusion of Magnetic Peninsula toward the Neighboring Opposite-polarity Region That Triggers the Largest Solar Flare in Solar Cycle 24Achievements of Hinode in the first eleven yearsComparative Study of Data-driven Solar Coronal Field Models Using a Flux Emergence Simulation as a Ground-truth Data SetOnset Mechanism of M6.5 Solar Flare Observed in Active Region 12371
- 参照
- MAGNETIC FIELD STRUCTURES TRIGGERING SOLAR FLARES AND CORONAL MASS EJECTIONSOBSERVATIONS AND MAGNETIC FIELD MODELING OF THE FLARE/CORONAL MASS EJECTION EVENT ON 2010 APRIL 8Magnetofrictional Extrapolations of Low and Lou’s Force-Free EquilibriaMAGNETIC STRUCTURE PRODUCING X- AND M-CLASS SOLAR FLARES IN SOLAR ACTIVE REGION 11158The Solar Optical Telescope for the Hinode Mission: An OverviewGeneration mechanisms for magnetosphere‐ionosphere current systems deduced from a three‐dimensional MHD simulation of the solar wind‐magnetosphere‐ionosphere coupling processesMean Field Model for the Formation of Filament Channels on the SunExtrapolation of a nonlinear force-free field containing a highly twisted magnetic loopThe Helioseismic and Magnetic Imager (HMI) Investigation for the Solar Dynamics Observatory (SDO)Three‐dimensional Simulation Study of Flux Rope Dynamics in the Solar CoronaTorus InstabilityA Twisted Flux Rope Model for Coronal Mass Ejections and Two-Ribbon Flares3D Coronal magnetic field from vector magnetograms: non-constant-<i>α</i>force-free configuration of the active region NOAA 8151Coronal Mass Ejection: Initiation, Magnetic Helicity, and Flux Ropes. I. Boundary Motion–driven EvolutionNew Boundary Integral Equation Representation for Finite Energy Force-Free Magnetic Fields in Open Space above the SunMagnetohydrodynamic Simulation of a Solar Flare with Chromospheric Evaporation Effect Based on the Magnetic Reconnection ModelINITIATION AND ERUPTION PROCESS OF MAGNETIC FLUX ROPE FROM SOLAR ACTIVE REGION NOAA 11719 TO EARTH-DIRECTED CMESIMULATIONS OF EMERGING MAGNETIC FLUX. II. THE FORMATION OF UNSTABLE CORONAL FLUX ROPES AND THE INITIATION OF CORONAL MASS EJECTIONSSTABILITY AND DYNAMICS OF A FLUX ROPE FORMED VIA FLUX EMERGENCE INTO THE SOLAR ATMOSPHEREON THE ERUPTION OF CORONAL FLUX ROPESRadiation dose forecast of WASAVIES during ground‐level enhancementTHE ROLE OF A FLUX ROPE EJECTION IN A THREE-DIMENSIONAL MAGNETOHYDRODYNAMIC SIMULATION OF A SOLAR FLAREThe writhe of helical structures in the solar coronaThe X-Ray Telescope (XRT) for the Hinode MissionDynamical evolution of a solar coronal magnetic field arcadeTHREE-DIMENSIONAL SOLAR<i>WIND</i>MODELING FROM THE SUN TO EARTH BY A SIP-CESE MHD MODEL WITH A SIX-COMPONENT GRIDStructure and evolution of magnetic fields associated with solar eruptionsModeling solar force-free magnetic fieldsFIELD TOPOLOGY ANALYSIS OF A LONG-LASTING CORONAL SIGMOIDEvolution of the Sheared Magnetic Fields of Two X-Class Flares Observed by Hinode/XRTNonlinear Force-Free Modeling of Coronal Magnetic Fields. II. Modeling a Filament Arcade and Simulated Chromospheric and Photospheric Vector FieldsThe Atmospheric Imaging Assembly (AIA) on the Solar Dynamics Observatory (SDO)CATASTROPHE VERSUS INSTABILITY FOR THE ERUPTION OF A TOROIDAL SOLAR MAGNETIC FLUX ROPEThe Effect of Nonzero ∇ · B on the numerical solution of the magnetohydrodynamic equationsA CRITICAL ASSESSMENT OF NONLINEAR FORCE-FREE FIELD MODELING OF THE SOLAR CORONA FOR ACTIVE REGION 10953Clear Evidence of Reconnection Inflow of a Solar FlareSTUDY ON THE TRIGGERING PROCESS OF SOLAR FLARES BASED ON<i>HINODE</i>/SOT OBSERVATIONSNONLINEAR FORCE-FREE EXTRAPOLATION OF THE CORONAL MAGNETIC FIELD BASED ON THE MAGNETOHYDRODYNAMIC RELAXATION METHODAn Emerging Flux Trigger Mechanism for Coronal Mass EjectionsNONLINEAR FORCE-FREE MODELING OF A THREE-DIMENSIONAL SIGMOID OBSERVED ON THE SUNNonlinear Force-Free Modeling of Coronal Magnetic Fields Part I: A Quantitative Comparison of MethodsIdeal kink instability of a magnetic loop equilibriumThe writhe of open and closed curvesAn Optimization Approach to Reconstructing Force‐free FieldsThe “Stress‐and‐Relax” Method for Reconstructing the Coronal Magnetic Field from Vector Magnetograph DataThe magnetic nature of solar flaresOBSERVATIONS AND NONLINEAR FORCE-FREE FIELD MODELING OF ACTIVE REGION 10953Coronal Mass Ejections as Loss of Confinement of Kinked Magnetic Flux RopesThe topological properties of magnetic helicityOptimization code with weighting function for the reconstruction of coronal magnetic fieldsA NEW IMPLEMENTATION OF THE MAGNETOHYDRODYNAMICS-RELAXATION METHOD FOR NONLINEAR FORCE-FREE FIELD EXTRAPOLATION IN THE SOLAR CORONATHE IMPORTANCE OF GEOMETRIC EFFECTS IN CORONAL LOOP MODELSMAGNETOHYDRODYNAMIC MODELING OF THE SOLAR ERUPTION ON 2010 APRIL 8CORONAL MASS EJECTION INITIATION: ON THE NATURE OF THE FLUX CANCELLATION MODELThe standard flare model in three dimensionsA Model for Solar Coronal Mass EjectionsRESPONSE OF THE PHOTOSPHERIC MAGNETIC FIELD TO THE X2.2 FLARE ON 2011 FEBRUARY 15A MODEL FOR MAGNETICALLY COUPLED SYMPATHETIC ERUPTIONSTWIST AND CONNECTIVITY OF MAGNETIC FIELD LINES IN THE SOLAR ACTIVE REGION NOAA 10930THE MAGNETIC SYSTEMS TRIGGERING THE M6.6 CLASS SOLAR FLARE IN NOAA ACTIVE REGION 11158Thickness variations along coronal loops inferred from vector magnetograph dataHyperbolic Divergence Cleaning for the MHD EquationsBUILDUP AND RELEASE OF MAGNETIC TWIST DURING THE X3.4 SOLAR FLARE OF 2006 DECEMBER 13Confined and Ejective Eruptions of Kink-unstable Flux RopesObservations and Modeling of a Filament on the SunWell posed reconstruction of the solar coronal magnetic fieldModeling Nonpotential Magnetic Fields in Solar Active RegionsThe ∇·B=0 Constraint in Shock-Capturing Magnetohydrodynamics CodesOnset of the Magnetic Explosion in Solar Flares and Coronal Mass EjectionsThe Hinode (Solar-B) Mission: An OverviewLimitations of force-free magnetic field extrapolations: Revisiting basic assumptionsModel of the High-Energy Phase of Solar FlaresThree-Dimensional Nonlinear Force-Free Field Reconstruction of Solar Active Region 11158 by Direct Boundary Integral EquationModeling a space weather event from the Sun to the Earth: CME generation and interplanetary propagationEffects of reconnection on the coronal mass ejection processEffects of toroidal forces in current loops embedded in a background plasmaWhat is the condition for fast magnetic reconnection?Formation and eruption of solar prominencesMAGNETOHYDRODYNAMIC MODELING FOR A FORMATION PROCESS OF CORONAL MASS EJECTIONS: INTERACTION BETWEEN AN EJECTING FLUX ROPE AND AN AMBIENT FIELDHOW COMMON ARE HOT MAGNETIC FLUX ROPES IN THE LOW SOLAR CORONA? A STATISTICAL STUDY OF EUV OBSERVATIONSTopological Evolution of a Fast Magnetic Breakout CME in Three DimensionsMagnetohydrodynamics of the SunExact Green's function method of solar force-free magnetic-field computations with constant alpha. I - Theory and basic test casesELECTRIC CURRENTS IN FLARE RIBBONS: OBSERVATIONS AND THREE-DIMENSIONAL STANDARD MODELA review on the genesis of coronal mass ejectionsEquilibrium of a Magnetically Confined Plasma in a ToroidNumerical simulation of a catastrophe model for coronal mass ejectionsEvidence of Magnetic Reconnection in Solar Flares and a Unified Model of FlaresA TWISTED FLUX ROPE AS THE MAGNETIC STRUCTURE OF A FILAMENT IN ACTIVE REGION 10953 OBSERVED BY<i>HINODE</i>EXTRAPOLATION OF THE SOLAR CORONAL MAGNETIC FIELD FROM<i>SDO</i>/HMI MAGNETOGRAM BY A CESE-MHD-NLFFF CODETriggering an Eruptive Flare by Emerging Flux in a Solar Active-Region Complex[ITAL]Yohkoh[/ITAL] SXT Observations of X-Ray “Dimming” Associated with a Halo Coronal Mass EjectionFAN–SPINE TOPOLOGY FORMATION THROUGH TWO-STEP RECONNECTION DRIVEN BY TWISTED FLUX EMERGENCEObservational constraints on well-posed reconstruction methods and the optimization-Grad-Rubin methodRECURRENT EXPLOSIVE ERUPTIONS AND THE “SIGMOID-TO-ARCADE” TRANSFORMATION IN THE SUN DRIVEN BY DYNAMICAL MAGNETIC FLUX EMERGENCEComparing Values of the Relative Magnetic Helicity in Finite VolumesNonlinear Force‐free Field Modeling of a Solar Active Region around the Time of a Major Flare and Coronal Mass EjectionNONLINEAR FORCE-FREE FIELD EXTRAPOLATION OF A CORONAL MAGNETIC FLUX ROPE SUPPORTING A LARGE-SCALE SOLAR FILAMENT FROM A PHOTOSPHERIC VECTOR MAGNETOGRAMMagnetic fields and the structure of the solar coronaEVOLUTION OF MAGNETIC FIELD AND ENERGY IN A MAJOR ERUPTIVE ACTIVE REGION BASED ON<i>SDO</i>/HMI OBSERVATIONThe Solar Dynamics Observatory (SDO)The standard flare model in three dimensionsA SELF-CONSISTENT NONLINEAR FORCE-FREE SOLUTION FOR A SOLAR ACTIVE REGION MAGNETIC FIELDMagnetic Field Overlying Solar Eruption Regions and Kink and Torus InstabilitiesPhotospheric Magnetic Field Evolution and Eruptive FlaresCoronal Mass Ejection: Initiation, Magnetic Helicity, and Flux Ropes. II. Turbulent Diffusion–driven EvolutionThe initiation of coronal mass ejections by newly emerging magnetic fluxNUMERICAL MODELING OF THE INITIATION OF CORONAL MASS EJECTIONS IN ACTIVE REGION NOAA 9415FORMATION AND ERUPTION OF AN ACTIVE REGION SIGMOID. I. A STUDY BY NONLINEAR FORCE-FREE FIELD MODELINGFORMATION OF TORUS-UNSTABLE FLUX ROPES AND ELECTRIC CURRENTS IN ERUPTING SIGMOIDSMagnetic Helicity, Tilt, and TwistMAGNETOHYDRODYNAMIC SIMULATION OF THE X2.2 SOLAR FLARE ON 2011 FEBRUARY 15. II. DYNAMICS CONNECTING THE SOLAR FLARE AND THE CORONAL MASS EJECTIONACHIEVING SELF-CONSISTENT NONLINEAR FORCE-FREE MODELING OF SOLAR ACTIVE REGIONSTHE 2011 FEBRUARY 15 X2 FLARE, RIBBONS, CORONAL FRONT, AND MASS EJECTION: INTERPRETING THE THREE-DIMENSIONAL VIEWS FROM THE<i>SOLAR DYNAMICS OBSERVATORY</i>AND<i>STEREO</i>GUIDED BY MAGNETOHYDRODYNAMIC FLUX-ROPE MODELINGGreen's function methods for potential magnetic fieldsPhotospheric flux cancellation and associated flux rope formation and eruptionObservations of the Failed Eruption of a FilamentSimulation of magnetohydrodynamic flows - A constrained transport methodEstimating the Relative Helicity of Coronal Magnetic FieldsUSING CORONAL LOOPS TO RECONSTRUCT THE MAGNETIC FIELD OF AN ACTIVE REGION BEFORE AND AFTER A MAJOR FLAREA Comprehensive View of the 2006 December 13 CME: From the Sun to Interplanetary SpaceDynamics of the Solar Magnetic Field. I. Method of Examination of Force-Free Magnetic FieldsTheoretical model of flares and prominencesCORONAL MASS EJECTION INITIATION BY CONVERGING PHOTOSPHERIC FLOWS: TOWARD A REALISTIC MODELSpace Weather Modeling Framework: A new tool for the space science communityCharacterizing and predicting the magnetic environment leading to solar eruptionsDRIVING MECHANISM AND ONSET CONDITION OF A CONFINED ERUPTIONA loop-top hard X-ray source in a compact solar flare as evidence for magnetic reconnectionMAGNETOHYDRODYNAMIC SIMULATION OF THE X2.2 SOLAR FLARE ON 2011 FEBRUARY 15. I. COMPARISON WITH THE OBSERVATIONSCORONAL MAGNETIC RECONNECTION DRIVEN BY CME EXPANSION—THE 2011 JUNE 7 EVENTTHE DRIVER OF CORONAL MASS EJECTIONS IN THE LOW CORONA: A FLUX ROPEPlasma Beta above a Solar Active Region: Rethinking the ParadigmBifurcation and Stability of Coronal Magnetic Arcades in a Linear Force-free FieldCalculation of force-free magnetic field with non-constant ?A METHOD FOR DATA-DRIVEN SIMULATIONS OF EVOLVING SOLAR ACTIVE REGIONSTWIST ACCUMULATION AND TOPOLOGY STRUCTURE OF A SOLAR MAGNETIC FLUX ROPESelf‐Consistent Magnetohydrodynamic Modeling of a Coronal Mass Ejection, Coronal Dimming, and a Giant Cusp‐shaped Arcade FormationCRITERIA FOR FLUX ROPE ERUPTION: NON-EQUILIBRIUM VERSUS TORUS INSTABILITYEvolution of Conjugate Footpoints inside Flare Ribbons during a Great Two‐Ribbon Flare on 2001 April 10Numerical simulations of fast and slow coronal mass ejectionsOn the numerical computation of nonlinear force-free magnetic fieldsTRIGGER MECHANISM OF SOLAR SUBFLARES IN A BRAIDED CORONAL MAGNETIC STRUCTUREInteractive desktop analysis of high resolution simulations: application to turbulent plume dynamics and current sheet formationMagnetic field evolution during prominence eruptions and two-ribbon flaresA Three‐dimensional Line‐tied Magnetic Field Model for Solar EruptionsDescription of a Singular Appearance seen in the Sun on September 1, 1859THE MECHANISMS FOR THE ONSET AND EXPLOSIVE ERUPTION OF CORONAL MASS EJECTIONS AND ERUPTIVE FLARESCHARACTERISTICS OF THE PHOTOSPHERIC MAGNETIC FIELD ASSOCIATED WITH SOLAR FLARE INITIATIONMAGNETOHYDRODYNAMIC SIMULATION OF A SIGMOID ERUPTION OF ACTIVE REGION 11283THE MAGNETIC FIELD OF ACTIVE REGION 11158 DURING THE 2011 FEBRUARY 12-17 FLARES: DIFFERENCES BETWEEN PHOTOSPHERIC EXTRAPOLATION AND CORONAL FORWARD-FITTING METHODSFlare-CME Models: An Observational Perspective (Invited Review)TEMPORAL EVOLUTION OF THE MAGNETIC TOPOLOGY OF THE NOAA ACTIVE REGION 11158The 3-D boundary element formulation of linear force-free magnetic fields with finite energy content in semi-infinite spaceStructure and Dynamics of Magnetic Reconnection in a Solar Flare
- 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CrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossref
- 書誌ID（NDLBibID）
- 10265302