Relationship between solar wind dynamic pressure and amplitude of geomagnetic sudden commencement (SC)
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DOI[10.1186/s40623-016-0444-y]to the data of the same series
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- Material Type
- 記事
- Author/Editor
- Tohru ArakiAtsuki Shinbori
- Publication, Distribution, etc.
- Publication Date
- 2016-05-28
- Publication Date (W3CDTF)
- 2016-05-28
- Periodical title
- EPS : Earth, Planets and Space
- No. or year of volume/issue
- 68(90)
- Volume
- 68(90)
- ISSN (Periodical Title)
- 1880-5981
- ISSN-L (Periodical Title)
- 1343-8832
- Text Language Code
- eng
- DOI
- 10.1186/s40623-016-0444-y
- Persistent ID (NDL)
- info:ndljp/pid/10193165
- 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.
- The local time variation of geomagnetic sudden commencements (SCs) has not been taken into account in the Siscoe's linear relationship which connects the SC amplitude with the corresponding dynamic pressure variation of the solar wind. By considering the physical background of SC, we studied which local time is best to extract the information of the solar wind dynamic pressure and concluded that the SC amplitude at 4-5 h local time of middle- and low-latitude stations most directly reflects the dynamic pressure effect. This result is used to re-check the order of magnitude of the largest 3 SCs observed since 1868.
- DOI
- 10.1186/s40623-016-0444-y
- Access Restrictions
- インターネット公開
- Rights (production)
- © 2016 Araki and Shinbori. 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)
- References
- Night-time sudden commencements observed by CHAMP and ground-based magnetometers and their relationship to solar wind parametersThe solar diurnal variation in the amplitude of sudden commencements of magnetic storms at the geomagnetic equatorA numerical simulation of the geomagnetic sudden commencement: 2. Plasma processes in the main impulseA numerical simulation of the geomagnetic sudden commencement: 1. Generation of the field‐aligned current associated with the preliminary impulseA new theory of magnetic stormsMagnetic local time and latitude dependence of amplitude of the main impulse (MI) of geomagnetic sudden commencements and its seasonal variationInjection of electrons and protons with energies of tens of MeV into L < 3 on 24 March 1991Field‐aligned current effects on midlatitude geomagnetic sudden commencementsAnalysis software for upper atmospheric data developed by the IUGONET project and its application to polar scienceAnomalous sudden commencement on March 24, 1991Penetration of magnetospheric electric fields to the equator during a geomagnetic stormLarge amplitude electric and magnetic field signatures in the inner magnetosphere during injection of 15 MeV electron drift echoesParametric study of shock‐induced transport and energization of relativistic electrons in the magnetosphereSudden impulses at low‐latitude stations: Steady state response for northward interplanetary magnetic fieldGeomagnetic field variations caused by changes in the quiet-time solar wind pressureGlobal structure of geomagnetic sudden commencementsThe effect of solar wind dynamic pressure changes on low and mid‐latitude magnetic recordsSudden impulses at low latitude stations: Steady state response for southward interplanetary magnetic fieldA Physical Model of the Geomagnetic Sudden CommencementSimulation of the prompt energization and transport of radiation belt particles during the March 24, 1991 SSCRelation between geomagnetic sudden impulses and solar wind pressure changes-An experimental investigationDeformation of the geomagnetic field by the solar windDirect detection of solar wind dynamic pressure effect on ground geomagnetic fieldMagnetic latitude and local time dependence of the amplitude of geomagnetic sudden commencementsSpecial features of the September 24–27, 1998 storm during high solar wind dynamic pressure and northward interplanetary magnetic fieldAnomalous occurrence features of the preliminary impulse of geomagnetic sudden commencement in the South Atlantic Anomaly regionLocal time variation of the amplitude of geomagnetic sudden commencements (SC) and SC-associated polar cap potentialMagnetic field depression at the Earth's surface calculated from the relationship between the size of the magnetosphere and the<i>Dst</i>valuesA new theory of magnetic stormsA new theory of magnetic stormsShocks and Storm Sudden CommencementsCharacteristics of geomagnetic sudden commencement observed in middle and low latitudesNighttime enhancement of the amplitude of geomagnetic sudden commencements and its dependence on IMF-BzCharacteristics of Pi 2 magnetic pulsations observed at the CPMN stations: A review of the STEP resultsHistorically largest geomagnetic sudden commencement (SC) since 1868
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