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《Chinese Journal of Geophysics》 2002-06
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PREDICTION OF THE IMF B_z USING 3-D KINEMATIC CODE

WANG CHUAN-BING 1) ZHAO JI-KUN 2)CHENG HE-HONG 2)LI YI 1)WANG SHUI 1) SUN WEI 3)AKASOFU S.I. 3)1) Department of Earth and Space Sciences,University of Science and Technology of China,Hefei 230026,China2) Institute of space sciences,National Center University,Chunli Taiwan,China3) Geophysical Institute,University of Alaska,Fairbanks,AK99701,U.S.A  
A scenario is introduced for predicting the perturbations of the north-south component B_z of interplanetary magnetic field (IMF) ahead of fast Coronal Mass Ejection (CME). The three-dimensional (3-D) kinematic code of Hakamada-Akasofu-Fry (1986) is improved according to the scenario,and is used to investigate the perturbation of IMF and plasma caused by the Halo CME at 06:30UT,May 12,1997 observed by SOHO in detail. Seventeen events of CME between 1978 and 1981 are examined,for 14 events of which (82%) the kinematic code correctly predicts the direction of perturbation of the north-south component of IMF. This shows that the direction predicted by the improved code agrees with observations very well.
【Fund】: 国家自然科学基金项目 (4 0 0 0 40 0 6 4983 40 3 0 499740 3 6);; 国家科学技术部支持的国家重点基础研究项目(G2 0 0 0 0 7840 5 ) ;; 中国科学技术大学青年基金项目 (ka0 71 5 ) .
【CateGory Index】: P353
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【References】
Chinese Journal Full-text Database 1 Hits
1 XIONG Ming, ZHENG Hui-Nan, WANG Yu-Ming, FU Xiang-Rong, WANG Shui, DOU Xian-KangSchool of Earth and Space Science, University of Science and Technology of China, Heifei 230026, China;A numerical simulation on the solar-terrestrial transit time of successive CMEs during November 4-5, 1998[J];Chinese Journal of Geophysics;2005-04
【Citations】
Chinese Journal Full-text Database 1 Hits
1 LIU SI-QING; WEI FENG-SI(Laboratory of Numerical Study Of Heliospheric Physics, Space Sience and Appolied Research Institute,Chinese Academy of Sciences, Beijing, 100080 China)CHAO JI-KWIN;CHEN HE-HONG ;SUN WEI; AKASOFU S. I.(Space Science Institute, Nati;RELATIONSHIP BETWEEN FILAMENT DISAPPEARANCE EVENTS AND INTERPLANETARY DISTURBANCES STUDIED BY A 3-D KINEMATIC METHOD[J];Chinese Journal of Geophysics;1998-06
【Co-references】
Chinese Journal Full-text Database 10 Hits
1 WANG Shui1,WEI Feng-si2(1.School of Earth and Space Sciences,University of Science and Technology of China,Hefei 230026,China;2.Center for Space Science and Applied Research,Chinese Academy of Sciences,Beijing 100080,China);Progress of space weather research in China[J];Progress in Geophysics;2007-04
2 WEI FENG-SI(Institute of Space Physics, Academia Sinica);PRELIMINARY RESULTS OF PREDICTING GEOMAGNETIC SSC BY USING IPS OBSERVATIONS[J];Chinese Journal of Geophysics;1984-05
3 WET FENG-SI(Center for Space Science and Applied Research, Acadcmta Sinica of China, Group of Interplanetary Dynamics, Beijing)ZHANG JIAN-HONG(Dept. of Earth and Space Science, University of Science and Technology of China, Hefei)HUANG SUI-PING(Dept. of Geophysics, Peking University, Beijing);STUDY OF THE PROPAGATION CHARACTERISTICS OF FLARE-ASSOCIATED INTERPLANETARY SHOCK WAVES IN THE FLARE-HELIOSPHERIC CURRENT SHEET COORDINATE SYSTEM[J];Chinese Journal of Geophysics;1990-02
4 WEI FENG-SI LIU SI-QING ZHANG JIAN-HONG(Center for Space Science and Applied Research. Academia Sinica, Group of Interplanetary Dynamics, Beijing 100080);STUDY OF DISTRIBUTION CHARACTERISTICS OF THE GEOMAGNETIC DISTURBANCES CORRESPONDING TO THE FLARE-ASSOCIATED INTERPLANETARY SHOCK WAVES IN THE FIARE-HELIOSPHERIC CURRENT SHEET COORDINATE SYSTEM[J];Chinese Journal of Geophysics;1991-02
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6 WANG Yu Ming YE Pin Zhong WANG Shui School of Earth and Space Sciences, University of Science and Technology of China, Hefei 230026, China;AN INTERPLANETARY ORIGIN OF GREAT GEOMAGNETIC STORMS:MULTIPLE MAGNETIC CLOUDS[J];Chinese Journal of Geophysics;2004-03
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【Secondary References】
Chinese Journal Full-text Database 2 Hits
1 ZHANG Ying FENG Xueshang YANG Liping (State Key Laboratory of Space Weather,Center for Space Science and Applied Research, Chinese Academy of Sciences,Beijing 100190);Predicting the Shock Arrival Time Using 1D-MHD CE/SE Solar Wind Model[J];Chinese Journal of Space Science;2010-02
2 ZHANG Ying1,2, CHEN JingYi2 & FENG XueShang2 1 Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing 100029, China; 2 State Key Laboratory of Space Weather, Center for Space Sciences and Applied Research, Chinese Academy of Sciences, Beijing 100190, China;Predicting the shock arrival time using 1D-HD solar wind model[J];科学通报(英文版);2010-11
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