THE GENERAL EFFECTS AND MODEL ANALYSIS OF MAJOR MAGNETIC STORM IN MARCH,1989

Kong Nan; Xiang Jingtian; Gao Meiqing; Wen Xiaolei

Publications of the Yunnan Observatory > 1990 > 0(4): 122-127.

Kong Nan, Xiang Jingtian, Gao Meiqing, Wen Xiaolei. THE GENERAL EFFECTS AND MODEL ANALYSIS OF MAJOR MAGNETIC STORM IN MARCH,1989[J]. Publications of the Yunnan Observatory, 1990, (4): 122-127.

Citation:

Kong Nan, Xiang Jingtian, Gao Meiqing, Wen Xiaolei. THE GENERAL EFFECTS AND MODEL ANALYSIS OF MAJOR MAGNETIC STORM IN MARCH,1989[J]. Publications of the Yunnan Observatory, 1990, (4): 122-127.

Citation:

Kong Nan, Xiang Jingtian, Gao Meiqing, Wen Xiaolei. THE GENERAL EFFECTS AND MODEL ANALYSIS OF MAJOR MAGNETIC STORM IN MARCH,1989[J]. Publications of the Yunnan Observatory, 1990, (4): 122-127.

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THE GENERAL EFFECTS AND MODEL ANALYSIS OF MAJOR MAGNETIC STORM IN MARCH,1989

1.
Institute of Building and Construction of MMI Beijing 100088, China
2.
Institute of Applied Mathematics, Chinese Academy of Sciences, Beijing 100080, China
3.
Institute of Geophysics, Chinese Academy of Sciences, Beijing 100101, China

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Published Date: October 14, 1990

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Abstract

Abstract

This paper has analysed the general solar-Terrestrial effect of major event in March, 1989 from 7 parameters using same time scale.The largest magnetic storm from AA index is compared on 8 stations of Changchun(43°49' 38" N), Beijing(40°02' 22" N), Wuhan(30°31' 39" N) and Guangzhou(23°05' 34" N) in China and Newport of Washington(48. 263°N), Boulder of Colorado(40. 138°N), Fredericksburg of VA(38. 205°N) and Norda of Mississippi in U. S. A.The ARMA(p, q) Autoregressive slide average model is used to simulate the geomagnetic storm data in 4 stations of China. The periodicity analysis, characteristic root and equation are used. The different models and characters are shown and explained.

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