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模糊聚类分析在耀斑-地磁扰动研究中的初步应用 被引量:4

PRELIMINARY APPLICATION OF FUZZY CLUSTERING IN THE FLARE-GEOMAGNETIC DISTURBANCE ANALYSES
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摘要 本文运用模糊聚类分析的方法,对1975—1983年可证认出的210个耀斑-IPS激波事件进行了分析研究,给出了它们的聚类指标和模糊等价关系以及大、中、小三类耀斑-磁扰的聚类中心。初步研究结果表明:95%的耀斑-IPS激波会引起地磁扰动(∑Kp≥16);对持续1小时以上的二级耀斑和2小时以上的一级耀斑,以及多个射电源的IPS观测均出现50km/8以上的速度跳跃这类大耀斑-IPS激波事件进行模糊聚类磁扰强弱预报试验,其准确率可达80%;这种大耀斑-IPS激波事件所对应的地磁扰动变化范围很宽,从∑Kp≥12直到∑Kp≤54,这说明耀斑-激波在行星际空间的传播以及向地球的传输过程是十分复杂的。 The method of fuzzy clustering is used to study 210 geomagnetic disturbance events,which were caused by the flare associated interplanetary shock waves during the period of 1975-1983.Clustering centers,fuzzy equivalent relationships and clustering indices for three kinds of clusers (i.e.large,middle and small) are obtained.Main results are: (1) for 95 % of all flare-shock waves could cause the geomagnetic disturbances (∑Kp≥16);(2) success to failure ratio of the fuzzy-clustering prediction test is about 80% for the large geomagnetic disturbance events,which were caused by those flares with importance ≥2,lasting over hour and importance≥1,lasting over 2 hours and for those where a sudden velocity increase in the solar wind,exceeding 50km/s,were observed with at least 3 radio sources;and (3) for these large events,the variation range of the geomagnetic disturbances is very wide,from ∑Kp≥12 to ∑Kp≤54,showing that the geomagnetic effects associated with the flare-interplanetary shock waves are very complicated.
出处 《空间科学学报》 CAS CSCD 北大核心 1992年第1期50-56,共7页 Chinese Journal of Space Science
基金 国家自然科学基金
关键词 模糊聚类 聚类标指 耀斑 地磁 Fuzzy clustering,Clustering indices,Fuzzy equivalent relationship
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参考文献4

  • 1魏奉思,空间科学学报,1990年,10卷,35页
  • 2魏奉思,地球物理学报,1984年,27卷,417页
  • 3冯德益,模糊数学方法与应用,1983年
  • 4魏奉思,空间科学学报,1982年,2卷,63页

同被引文献86

  • 1ZHAO Xinhua1,2 & FENG Xueshang1,3 1. SIGMA Weather Group, Key Laboratory of Space Weather, Center for Space Science and Applied Re-search, Chinese Academy of Sciences, Beijing 100080, China,2. Graduate School of the Chinese Academy of Sciences, Beijing 100039, China,3. School of Geophysics and Geoinformation Systems, China University of Geosciences, Beijing 100083, China.A tentative study for the prediction of the CME related geomagnetic storm intensity and its transit time[J].Science China(Technological Sciences),2005,48(6):648-668. 被引量:4
  • 2章公亮.行星际高密度结构的磁流体动力学特性[J].中国科学(A辑),1989,20(5):502-508. 被引量:1
  • 3魏奉思.关于利用行星际闪烁(IPS)观测进行地球磁暴急始预报的初步探讨[J].地球物理学报,1984,27(5):417-423.
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  • 7Gapper G R, Hewish A, Purvis A, et al. Observing interplanetary disturbances from the ground. Nature, 1982, 296:633-636.
  • 8Kojima M, Kakinuma T J. Solar cycle evolution of solar wind speed structure between 1973 and 1985 observed with the interplanetary scintillation. Journal of Geophysical Research, 1987, 92:7269-7279.
  • 9Wei F S, Yang G, Zhang G. Three-dimensional propagation properties of flare-associated interplanetary shock waves from interplanetary scintillation observations. In: Cornelis de Jager, Chen B, eds. Proceedings of Kunming Workshop on Solar Physics and Interplanetary Travelling Phenomena Ⅱ, Beijing: Science Press, 1985. 1043-1051.
  • 10Wei F S, Dryer M. Propagation of solar flare-associated interplanetary shock waves in the heliospheric merididonal plane.Solar Physics, 1991, 132:373-394.

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