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電子書籍・電子雑誌EPS : Earth, Planets and Space
Volume number68
Relationsh...

Relationship between solar wind dynamic pressure and amplitude of geomagnetic sudden commencement (SC)

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Relationship between solar wind dynamic pressure and amplitude of geomagnetic sudden commencement (SC)

Persistent ID (NDL)
info:ndljp/pid/10193165
Material type
記事
Author
Tohru Arakiほか
Publisher
Springer science+business media
Publication date
2016-05-28
Material Format
Digital
Journal name
EPS : Earth, Planets and Space 68(90)
Publication Page
-
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The local time variation of geomagnetic sudden commencements (SCs) has not been taken into account in the Siscoe's linear relationship which connects ...

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Digital

Material Type
記事
Author/Editor
Tohru Araki
Atsuki 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
Persistent ID (NDL)
info:ndljp/pid/10193165
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
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

Digital

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.
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.
References
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Sudden impulses at low latitude stations: Steady state response for southward interplanetary magnetic field
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Simulation of the prompt energization and transport of radiation belt particles during the March 24, 1991 SSC
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Special features of the September 24–27, 1998 storm during high solar wind dynamic pressure and northward interplanetary magnetic field
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Local time variation of the amplitude of geomagnetic sudden commencements (SC) and SC-associated polar cap potential
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A new theory of magnetic storms
A new theory of magnetic storms
Shocks and Storm Sudden Commencements
Characteristics of geomagnetic sudden commencement observed in middle and low latitudes
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Characteristics of Pi 2 magnetic pulsations observed at the CPMN stations: A review of the STEP results
Historically largest geomagnetic sudden commencement (SC) since 1868
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