31![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 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](https://www.pdfsearch.io/img/09ac2142be1a0983cda65d8dd39324da.jpg) | Add to Reading ListSource URL: space.ustc.edu.cnLanguage: English - Date: 2013-08-12 11:21:54
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32![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 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](https://www.pdfsearch.io/img/5fb82a53f4424bcf87ca1b10c5d85440.jpg) | Add to Reading ListSource URL: cdaw.gsfc.nasa.govLanguage: English - Date: 2001-04-27 18:19:32
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33![In-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](https://www.pdfsearch.io/img/54a34200daea82c91644847a96c97d30.jpg) | Add to Reading ListSource URL: www-ssg.sr.unh.eduLanguage: English - Date: 2010-06-26 12:08:45
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34![Connecting 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](https://www.pdfsearch.io/img/3bcbd4a940fbcd7b806b31f27bdba4cd.jpg) | Add to Reading ListSource URL: hmi.stanford.eduLanguage: English - Date: 2009-09-17 15:45:25
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35![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 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](https://www.pdfsearch.io/img/1e7088d9aa86cb2febe3c9271396ebad.jpg) | Add to Reading ListSource URL: www.nict.go.jpLanguage: English - Date: 2013-11-21 20:27:25
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36![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 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](https://www.pdfsearch.io/img/6005be36bb30fa89bb0d516cfc1d2ae7.jpg) | Add to Reading ListSource URL: www.swsc-journal.orgLanguage: English |
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37![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 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](https://www.pdfsearch.io/img/2662ad7c7925df2e8b711964475cff49.jpg) | Add to Reading ListSource URL: umtof.umd.eduLanguage: English - Date: 2006-05-03 13:32:10
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38![Comments 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](https://www.pdfsearch.io/img/4b6e397785af0137332eed0d746abe52.jpg) | Add to Reading ListSource URL: www.leif.org.Language: English |
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39![Connecting 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](https://www.pdfsearch.io/img/cc2f5a353d63965f224df1f071825f87.jpg) | Add to Reading ListSource URL: hmi.stanford.eduLanguage: English - Date: 2009-09-17 15:45:25
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40![The 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](https://www.pdfsearch.io/img/a1948af2769956fcf040f5ebe66988f5.jpg) | Add to Reading ListSource URL: www.physics.usyd.edu.auLanguage: English - Date: 2009-01-10 16:48:30
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