Magnetic cloud

Results: 86



#Item
31STEP Team at USTC http://space.ustc.edu.cn/dreams/ August 12, 2013, 2:20am  Full halo coronal mass ejections: Do we need to correct the

STEP Team at USTC http://space.ustc.edu.cn/dreams/ August 12, 2013, 2:20am Full halo coronal mass ejections: Do we need to correct the

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Source URL: space.ustc.edu.cn

Language: English - Date: 2013-08-12 11:21:54
32Astrophysical Journal, 548:L91–L94, 2001 February 10 q[removed]The American Astronomical Society. All rights reserved. Printed in U.S.A. RADIO SIGNATURES OF CORONAL MASS EJECTION INTERACTION: CORONAL MASS EJECTION CANNIB

Astrophysical Journal, 548:L91–L94, 2001 February 10 q[removed]The American Astronomical Society. All rights reserved. Printed in U.S.A. RADIO SIGNATURES OF CORONAL MASS EJECTION INTERACTION: CORONAL MASS EJECTION CANNIB

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Source URL: cdaw.gsfc.nasa.gov

Language: English - Date: 2001-04-27 18:19:32
33In-Situ Signatures of Interplanetary Coronal Mass Ejections Ian G. Richardson,  NASA/Goddard Space Flight Center

In-Situ Signatures of Interplanetary Coronal Mass Ejections Ian G. Richardson, NASA/Goddard Space Flight Center

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Source URL: www-ssg.sr.unh.edu

Language: English - Date: 2010-06-26 12:08:45
34Connecting Magnetic Clouds to Solar Surface Features Vasyl Yurchyshyn Big Bear Solar Observatory  • Coronal mass ejecta (CMEs) are known to cause strongest 

Connecting Magnetic Clouds to Solar Surface Features Vasyl Yurchyshyn Big Bear Solar Observatory • Coronal mass ejecta (CMEs) are known to cause strongest 

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Source URL: hmi.stanford.edu

Language: English - Date: 2009-09-17 15:45:25
352-1-3 Structure of Interplanetary Magnetic Cloud Estimated by Fitting Magnetic Flux Rope Models ISHIBASHI Hiromitsu We examined the relationship between interplanetary magnetic cloud observed by the ACE satellite on Apri

2-1-3 Structure of Interplanetary Magnetic Cloud Estimated by Fitting Magnetic Flux Rope Models ISHIBASHI Hiromitsu We examined the relationship between interplanetary magnetic cloud observed by the ACE satellite on Apri

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Source URL: www.nict.go.jp

Language: English - Date: 2013-11-21 20:27:25
36J. Space Weather Space Clim[removed]A10 DOI: [removed]swsc[removed]  Owned by the authors, Published by EDP Sciences 2012 Presence of solar filament plasma detected in interplanetary coronal mass ejections by in situ sp

J. Space Weather Space Clim[removed]A10 DOI: [removed]swsc[removed]  Owned by the authors, Published by EDP Sciences 2012 Presence of solar filament plasma detected in interplanetary coronal mass ejections by in situ sp

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Source URL: www.swsc-journal.org

Language: English
37The Relative Abundance of Chromium and Iron in the Solar Wind J.A. Paquette∗ , F.M. Ipavich∗ , S.E. Lasley∗ , P. Bochsler† and P. Wurz† ∗  Department of Physics, University of Maryland, College Park, MD, USA

The Relative Abundance of Chromium and Iron in the Solar Wind J.A. Paquette∗ , F.M. Ipavich∗ , S.E. Lasley∗ , P. Bochsler† and P. Wurz† ∗ Department of Physics, University of Maryland, College Park, MD, USA

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Source URL: umtof.umd.edu

Language: English - Date: 2006-05-03 13:32:10
38Comments on  Leif Svalgaard Journal Club Discussion Stanford University Wed. 19 Feb. 2014

Comments on Leif Svalgaard Journal Club Discussion Stanford University Wed. 19 Feb. 2014

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Source URL: www.leif.org.

Language: English
39Connecting Magnetic Clouds to Solar Surface Features Vasyl Yurchyshyn Big Bear Solar Observatory  • Coronal mass ejecta (CMEs) are known to cause strongest 

Connecting Magnetic Clouds to Solar Surface Features Vasyl Yurchyshyn Big Bear Solar Observatory • Coronal mass ejecta (CMEs) are known to cause strongest 

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Source URL: hmi.stanford.edu

Language: English - Date: 2009-09-17 15:45:25
40The Magnetic Universe BY BRYAN GAENSLER Magnets are everywhere, but we don’t know how they got here.  M

The Magnetic Universe BY BRYAN GAENSLER Magnets are everywhere, but we don’t know how they got here. M

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Source URL: www.physics.usyd.edu.au

Language: English - Date: 2009-01-10 16:48:30