Evolution of the current system during solar wind pressure pulses based on aurora and magnetometer observations
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- Material Type
- 記事
- Author/Editor
- Yukitoshi NishimuraTakashi KikuchiYusuke Ebihara
- Publication, Distribution, etc.
- Publication Date
- 2016-08-11
- Publication Date (W3CDTF)
- 2016-08-11
- Periodical title
- EPS : Earth, Planets and Space
- No. or year of volume/issue
- 68(144)
- Volume
- 68(144)
- ISSN (Periodical Title)
- 1880-5981
- ISSN-L (Periodical Title)
- 1343-8832
- Text Language Code
- eng
- DOI
- 10.1186/s40623-016-0517-y
- Persistent ID (NDL)
- info:ndljp/pid/10193221
- 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)
- 2016-09-08T09:53:02+09:00
- Date Captured (W3CDTF)
- 2016-08-26
- 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/9963599
- 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/s40623-016-0517-y
- Access Restrictions
- インターネット公開
- Rights (production)
- © 2016 The Author(s). 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.
- Related Material (URI)
- Is Referenced By
- Enhanced response of thermospheric cooling emission to negative pressure pulse
- References
- Structures of dayside whistler‐mode waves deduced from conjugate diffuse auroraEffect of interplanetary shock strengths and orientations on storm sudden commencement rise timesA numerical simulation of the geomagnetic sudden commencement: 1. Generation of the field‐aligned current associated with the preliminary impulseTransient changes in magnetospheric‐ionospheric currents caused by the passage of an interplanetary shock: Northward interplanetary magnetic field caseTHEMIS Ground-Based MagnetometersResponse of the ionosphere to a density pulse in the solar wind: Simulation of traveling convection vorticesGeomagnetic response to solar wind dynamic pressure impulse events at high‐latitude conjugate pointsTransmission line model for the near‐instantaneous transmission of the ionospheric electric field and currents to the equatorField‐aligned current effects on midlatitude geomagnetic sudden commencements“Compression aurora”: Particle precipitation driven by long‐duration high solar wind ram pressureCircumpolar ground‐based optical measurements of proton and electron shock auroraPreliminary impulse of the geomagnetic storm sudden commencement of November 18, 1993Quasi‐stationary auroral patches observed at the South Pole StationA regional climate model study of how biomass burning aerosol impacts land‐atmosphere interactions over the AmazonGlobal MHD simulation of the geomagnetic sudden commencement on 21 October 1999Propagation of the preliminary reverse impulse of sudden commencements to low latitudesShock aurora: FAST and DMSP observationsGlobal structure of geomagnetic sudden commencementsHigh‐latitude reconnection effect observed at the dayside dip equator as a precursor of a sudden impulseThe chain response of the magnetospheric and ground magnetic field to interplanetary shocksPropagation of electron and proton shock‐induced aurora and the role of the interplanetary magnetic field and solar windRapid intensification and propagation of the dayside aurora: Large scale interplanetary pressure pulses (fast shocks)Understanding the response of the ionosphere-magnetosphere system to sudden solar wind density increasesStatistical study of the effect of solar wind dynamic pressure fronts on the dayside and nightside ionospheric convectionThe SuperMAG data processing techniqueEffect of the orientation of interplanetary shock on the geomagnetic sudden commencementA Physical Model of the Geomagnetic Sudden CommencementSimultaneous ground‐satellite optical observations of postnoon shock aurora in the Southern HemisphereEvidence of transmission of polar electric fields to the low latitude at times of geomagnetic sudden commencementsThe Effect of the January 10, 1997, pressure pulse on the magnetosphere-ionosphere current systemDecrease of auroral intensity associated with reversal of plasma convection in response to an interplanetary shock as observed over Zhongshan station in AntarcticaMapping electrodynamic features of the high‐latitude ionosphere from localized observations: TechniquePolar cap convection and PC index during sudden changes in solar wind dynamic pressureIonospheric screening effect and storm sudden commencementAn improvement of the Kamide‐Richmond‐Matsushita Scheme for the estimation of the three‐dimensional current systemGround and satellite observations of postdawn aurorae near the time of a sudden storm commencementMagnetic latitude and local time dependence of the amplitude of geomagnetic sudden commencementsDeformation and evolution of solar wind discontinuities through their interactions with the Earth's bow shockSummer‐winter hemisphere asymmetry of the preliminary reverse impulse of geomagnetic storm sudden commencements at midlatitudesA detailed description of the solar wind triggers of two dayside transients: Events of 25 July 1997Simulations of observed auroral brightening caused by solar wind dynamic pressure enhancements under different interplanetary magnetic field conditionsA multipoint determination of the propagation velocity of a sudden commencement across the polar ionosphereExtension of a polar ionospheric current to the nightside equatorEffect of solar wind pressure pulses on the size and strength of the auroral ovalOccurrence Characteristics of the Preliminary Impulse of Geomagnetic Sudden Commencement Detected at Middle and Low Latitudes.Rise time of geomagnetic sudden commencements —Statistical analysis of ground geomagnetic data—
- Data Provider (Database)
- 国立情報学研究所 : CiNii Research
- Original Data Provider (Database)
- 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Crossref
- Bibliographic ID (NDL)
- 10193221
- NAID
- 120005973253