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Wu, Chin-Chun, Dryer, Murray (1996) predicting the initial IMF Bzpolarity's change at 1 AU caused by shocks that precede coronal mass ejections. Geophysical Research Letters, 23 (14) 1709-1712 doi:10.1029/96gl01721

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Reference TypeJournal (article/letter/editorial)
Titlepredicting the initial IMF Bzpolarity's change at 1 AU caused by shocks that precede coronal mass ejections
JournalGeophysical Research Letters
AuthorsWu, Chin-ChunAuthor
Dryer, MurrayAuthor
Year1996 (July 1)Volume23
Issue14
PublisherAmerican Geophysical Union (AGU)
DOIdoi:10.1029/96gl01721Search in ResearchGate
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Mindat Ref. ID783221Long-form Identifiermindat:1:5:783221:9
GUID0
Full ReferenceWu, Chin-Chun, Dryer, Murray (1996) predicting the initial IMF Bzpolarity's change at 1 AU caused by shocks that precede coronal mass ejections. Geophysical Research Letters, 23 (14) 1709-1712 doi:10.1029/96gl01721
Plain TextWu, Chin-Chun, Dryer, Murray (1996) predicting the initial IMF Bzpolarity's change at 1 AU caused by shocks that precede coronal mass ejections. Geophysical Research Letters, 23 (14) 1709-1712 doi:10.1029/96gl01721
In(1996, July) Geophysical Research Letters Vol. 23 (14) American Geophysical Union (AGU)

See Also

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Hundhausen, A. J., Holzer, T. E., Low, B. C. (1987) Do slow shocks precede some coronal mass ejections?. Journal of Geophysical Research, 92. 11173 doi:10.1029/ja092ia10p11173
Howard, T. A., Tappin, S. J. (2005) Interplanetary shocks unconnected with earthbound coronal mass ejections. Geophysical Research Letters, 32 (14) doi:10.1029/2005gl023056
Dryer, Murray (1996) Comments on the origins of coronal mass ejections. Solar Physics, 169 (2). doi:10.1007/bf00190618
Wu, Chin-Chun, Dryer, Murray, Smith, Z., Wu, S.T., Lyn, L.H. (1996) Recipe for predicting the IMF Bz polarity's change of direction following solar disturbances and at the onset of geomagnetic storms. Journal of Atmospheric and Terrestrial Physics, 58 (15). 1805-1814 doi:10.1016/0021-9169(96)00010-4
Howard, Tim A. (2006) Reply to comment by N. Gopalswamy et al. on “Interplanetary shocks unconnected with earthbound coronal mass ejections”. Geophysical Research Letters, 33 (11) doi:10.1029/2005gl025233
Wang, C. (2004) Interplanetary coronal mass ejections observed by Voyager 2 between 1 and 30 AU. Journal of Geophysical Research, 109. doi:10.1029/2004ja010379
Odstrčil, D., Smith, Z., Dryer, M. (1996) Distortion of the heliospheric plasma sheet by interplanetary shocks. Geophysical Research Letters, 23 (18) 2521-2524 doi:10.1029/96gl00159
Shen, Fang, Wu, S. T., Feng, Xueshang, Wu, Chin-Chun (2012) Acceleration and deceleration of coronal mass ejections during propagation and interaction. Journal of Geophysical Research: Space Physics, 117. doi:10.1029/2012ja017776
Gosling, J. T., Riley, Pete (1996) The acceleration of slow coronal mass ejections in the high-speed solar wind. Geophysical Research Letters, 23 (21) 2867-2870 doi:10.1029/96gl02843
Wu, Chin-Chun, Dryer, Murray, Wu, S. T., Wood, Brian E., Fry, Craig D., Liou, Kan, Plunkett, Simon (2011) Global three-dimensional simulation of the interplanetary evolution of the observed geoeffective coronal mass ejection during the epoch 1-4 August 2010. Journal of Geophysical Research: Space Physics, 116. doi:10.1029/2011ja016947
Bravo, Silvia (1998) Coronal mass ejections associated with interplanetary ejecta. Geophysical Research Letters, 25 (23) 4285-4288 doi:10.1029/1998gl900168
 
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