Simulation study of near-Earth space disturbances : 1. magnetic storms
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DOI[10.1186/s40645-019-0264-3]のデータに遷移します
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- 資料種別
- 記事
- 著者・編者
- Yusuke Ebihara
- 出版年月日等
- 2019-02-13
- 出版年（W3CDTF）
- 2019-02-13
- タイトル（掲載誌）
- Progress in earth and planetary science
- 巻号年月日等（掲載誌）
- 6(16)
- 掲載巻
- 6(16)
- 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/s40645-019-0264-3
- 国立国会図書館永続的識別子
- info:ndljp/pid/11249504
- 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）
- 2019-03-05T23:10:26+09:00
- 保存日（W3CDTF）
- 2019-03-05
- 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/11249488
- 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
- A magnetic storm is the world-wide geomagnetic disturbance taking place in near-Earth space environment, lasting for a few days. Geomagnetic fields can be depressed by ~ 1% on the ground for large magnetic storms. The prime cause of the long-lasting, world-wide geomagnetic disturbance is the development of the ring current that surrounds the Earth. The ring current is an electric current carried by charged particles. Thus, the growth and decay of the ring current correspond to accumulation and loss of the ring current particles, respectively. The ring current is strong enough to modulate near-Earth space environment, and leads to many observable effects. In this sense, the ring current can be regarded as an important mediator in the near-Earth space environment. Here, the dynamics and structure of the ring current and its active role are briefly reviewed on the basis of numerical simulation results.
- DOI
- 10.1186/s40645-019-0264-3
- オンライン閲覧公開範囲
- インターネット公開
- 著作権情報
- © The Author(s). 2019. This article is distributed under the terms of the Creative Commons Attribution 4.0 International License (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted use, distribution, and reproduction in any medium, provided you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons license, and indicate if changes were made.
- 関連情報（URI）
- 参照
- Rapid decay of storm time ring current due to pitch angle scattering in curved field lineEnergy-dependent evolution of ring current protons during magnetic stormsCounter electrojet and overshielding after substorm onset: Global MHD simulation studyNumerical Simulation of the Ring Current: ReviewRevision of empirical electric field modeling in the inner magnetosphere using Cluster dataPitch-angle distributions of 100- to 300-kev protons measured by the Esro IB satelliteRing current protons in the upper atmosphere within the plasmasphereModeling of inner plasma sheet and ring current during substormsThe ring current, geomagnetic disturbance, and the Van Allen radiation beltsDynamical property of storm time subauroral rapid flows as a manifestation of complex structures of the plasma pressure in the inner magnetosphereLimit on stably trapped particle fluxesModeling ring current proton precipitation by electromagnetic ion cyclotron waves during the May 14–16, 1997, stormLosses of ring current ions by strong pitch angle scatteringStatistical distribution of the storm‐time proton ring current: POLAR measurementsStable auroral red arcs, sinks for energy of<i>D</i><sub><i>st</i></sub>main phasePhase space variations of near equatorially mirroring ring current ionsHydromagnetic theory of geomagnetic stormsKinetic model of the ring current‐atmosphere interactionsComment on “Modeling Extreme “Carrington‐Type” Space Weather Events Using Three‐Dimensional Global MHD Simulations” by C. M. Ngwira, A. Pulkkinen, M. M. Kuznetsova, and A. Glocer”Two‐dimensional observations of overshielding during a magnetic storm by the Super Dual Auroral Radar Network (SuperDARN) Hokkaido radarModeling the electromagnetic ion cyclotron wave‐induced formation of detached subauroral proton arcsSubauroral proton spots visualize the Pc1 sourceOn the extraterrestrial ring current during geomagnetic stormsRelationship of interplanetary magnetic field structure with development of substorm and storm main phaseLifetime of ring current particles due to coulomb collisions in the plasmasphereA simulation of the storm-time ring currentThree‐Dimensional Ring Current Decay ModelThe motion of a proton in the equatorial magnetosphereSimulations of ring current proton pitch angle distributionsThe ring current: a short biographyA general relation between the energy of trapped particles and the disturbance field near the EarthThe amplitude distribution of field-aligned currents at northern high latitudes observed by TriadGeomagnetic storms: historical perspective to modern viewA proposed production model of rapid subauroral ion drifts and their relationship to substorm evolutionComprehensive computational model of Earth's ring currentMathematical Models of Magnetospheric Convection and its Coupling to the IonospherePitch-angle scattering of energetic protons in the magnetotail current sheet as the dominant source of their isotropic precipitation into the nightside ionosphereLifetimes of Trapped Radiation Belt Particles Determined by Coulomb ScatteringModeling of solar wind control of the ring current buildup: A case study of the magnetic storms in April 1997The onset time of magnetospheric substorms determined from ground and synchronous satellite recordsResponse of the magnetospheric convection to sudden interplanetary magnetic field changes as deduced from the evolution of partial ring currentsSimulation study on fundamental properties of the storm‐time ring currentDominant role of the asymmetric ring current in producing the stormtime <i>Dst</i>*Dynamics of Geomagnetically Trapped RadiationNightside thermospheric FUV emissions due to energetic neutral atom precipitation during magnetic superstormsTwo‐step development of geomagnetic stormsDie vollständigste aller bisherigen Beobachtungen über den Einfluss des Nordlichts auf die Magnetnadel angestelltAn empirical relationship between interplanetary conditions and<i>Dst</i>Empirical model for μ scattering caused by field line curvature in a realistic magnetosphereStructure and dynamics of the proton energy density in the inner magnetosphereOn the ring current energy injection rateStorm-associated variations of equatorially mirroring ring current protons, 1-800 keV, at constant first adiabatic invariantOrigin of interplanetary southward magnetic fields responsible for major magnetic storms near solar maximum (1978–1979)Ring current decay time model during geomagnetic storms: a simple analytical approachGeocoronal imaging with Dynamics ExplorerMorphology of the ring current derived from magnetic field observationsAverage characteristics and activity dependence of the subauroral polarization streamDifferences between CME‐driven storms and CIR‐driven stormsThe role of precipitation losses in producing the rapid early recovery phase of the Great Magnetic Storm of February 1986On the asymmetric development of magnetic storm fields in low and middle latitudesInterchange instability in the inner magnetosphere associated with geosynchronous particle flux decreasesA semiempirical model of large-scale magnetospheric electric fieldsGlobal IMAGE/HENA observations of the ring current: Examples of rapid response to IMF and ring current‐plasmasphere interactionRing current and the magnetosphere‐ionosphere coupling during the superstorm of 20 November 2003Regular and chaotic charged particle motion in magnetotaillike field reversals: 1. Basic theory of trapped motionEvolution of the ring current during two geomagnetic stormsEffects of a high‐density plasma sheet on ring current development during the November 2–6, 1993, magnetic stormThe proton ring current and its interaction with the plasmapause: Storm recovery phaseRing current effects on trapped particlesInner magnetospheric modeling with the Rice Convection ModelNonlinear impact of plasma sheet density on the storm‐time ring currentNewtonian Development of the Dynamical Properties of Ionized Gases of Low DensitySolar wind control of density and temperature in the near‐Earth plasma sheet: WIND/GEOTAIL collaborationIonospheric electrical conductances produced by auroral proton precipitationPolar and Magnetospheric SubstormsWhat is a geomagnetic storm?Turbulent loss of ring current protonsPlasma clouds in the magnetosphereThe cause of high-intensity long-duration continuous AE activity (HILDCAAs): Interplanetary Alfvén wave trainsHill model of transpolar potential saturation: Comparisons with MHD simulationsAnalysis of early phase ring current recovery mechanisms during geomagnetic stormsCollisional losses of ring current ionsAdiabatic evolution of trapped particle pitch angle distributions during a storm main phaseSaturation of the ionospheric polar cap potential during the October–November 2003 superstormsTrajectory traces of charged particles in the magnetosphereRing current development during the great geomagnetic storm of February 1986Geomagnetic storms driven by ICME‐ and CIR‐dominated solar windRing current particle distributions during the magnetic storms of December 16-18, 1971The magnetic storm main phase modellingEffects of ionospheric conductivity on convective flow of plasma in the magnetosphereGlobal ena Image SimulationsMagnetic coupling of the ring current and the radiation beltPitch angle diffusion in the Jovian magnetodiscMagnetospheric ConvectionComment on “Modeling extreme “Carrington-type” space weather events using three-dimensional global MHD simulations” by C.M. Ngwira, A. Pulkkinen, M.M. Kuznetsova and A. Glocer”International Geomagnetic Reference Field : the 12th generation
- 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
- 学術機関リポジトリデータベース雑誌記事索引データベースCrossrefCiNii Articles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
- 書誌ID（NDLBibID）
- 11249504
- NII論文ID
- 120006576447