Substorm

Results: 223



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111J. Space Weather Space Clim[removed]A28 DOI: [removed]swsc[removed] Ó M.G. Johnsen, Published by EDP Sciences 2013 OPEN

J. Space Weather Space Clim[removed]A28 DOI: [removed]swsc[removed] Ó M.G. Johnsen, Published by EDP Sciences 2013 OPEN

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Source URL: www.swsc-journal.org

Language: English
112Microsoft Word - 12-CAO Jinbin_new_.doc

Microsoft Word - 12-CAO Jinbin_new_.doc

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Source URL: english.nssc.cas.cn

Language: English - Date: 2014-10-24 03:54:39
113Journal of Geophysical Research: Space Physics RESEARCH ARTICLE[removed]2014JA020105 Key Points: • Fast flows in CPS (X > −15 Re) can be classified into two classes

Journal of Geophysical Research: Space Physics RESEARCH ARTICLE[removed]2014JA020105 Key Points: • Fast flows in CPS (X > −15 Re) can be classified into two classes

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Source URL: english.cssar.cas.cn

Language: English - Date: 2014-11-04 03:19:19
114IMAGE Newsletter Number 6 IMAGE Team

IMAGE Newsletter Number 6 IMAGE Team

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Source URL: space.fmi.fi

Language: English - Date: 2004-11-16 03:53:27
115IMAGE Newsletter Number 6 IMAGE Team

IMAGE Newsletter Number 6 IMAGE Team

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Source URL: www.geo.fmi.fi

Language: English - Date: 2004-11-16 03:53:27
116Radio & Space Plasma Physics Group Publications Group authors are shown boldface Calendar Year 2007 Refereed research papers 07-01

Radio & Space Plasma Physics Group Publications Group authors are shown boldface Calendar Year 2007 Refereed research papers 07-01

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Source URL: www.ion.le.ac.uk

Language: English - Date: 2009-03-09 10:32:00
117Major magnetic storm events also lead to spectacular auroral displays even at low geographic latitudes. Substorms were first documented in 1964 by Syun-Ichi Akasofu of the University of Alaska using a network of all-sky

Major magnetic storm events also lead to spectacular auroral displays even at low geographic latitudes. Substorms were first documented in 1964 by Syun-Ichi Akasofu of the University of Alaska using a network of all-sky

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Source URL: cse.ssl.berkeley.edu

Language: English - Date: 2010-01-11 17:34:45
118Exercise 3. Find the magnetic latitudes for field lines that cross the equatorial plane at L = 3.0, L=10.0, L=20.0 and L = 30.0. If magnetic storms are produced by magnetic reconnection events between L=15 and L = 35, at

Exercise 3. Find the magnetic latitudes for field lines that cross the equatorial plane at L = 3.0, L=10.0, L=20.0 and L = 30.0. If magnetic storms are produced by magnetic reconnection events between L=15 and L = 35, at

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Source URL: cse.ssl.berkeley.edu

Language: English - Date: 2010-01-11 17:34:22
1192-2-5 Application of the Magnetospheric Model for Numerical Forecast - Validation Using the AE IndexKITAMURA Kentarou, SHIMAZU Hironori, FUJITA Shigeru, WATARI Shinichi, KUNITAKE Manabu, SHINAGAWA Hiroyuki, and TANAKA Ta

2-2-5 Application of the Magnetospheric Model for Numerical Forecast - Validation Using the AE IndexKITAMURA Kentarou, SHIMAZU Hironori, FUJITA Shigeru, WATARI Shinichi, KUNITAKE Manabu, SHINAGAWA Hiroyuki, and TANAKA Ta

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Source URL: www.nict.go.jp

Language: English - Date: 2013-11-21 20:29:36
120each other. The subjects then climbed into the shielded room, where the strength of the magnetization of their chest area was measured. During the year of observations the amount of dust declined steadily to about 10% of

each other. The subjects then climbed into the shielded room, where the strength of the magnetization of their chest area was measured. During the year of observations the amount of dust declined steadily to about 10% of

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Source URL: cse.ssl.berkeley.edu

Language: English - Date: 2010-01-11 17:35:53