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基于GM(1,1)与灰区间估计的SPE通量水平长期预测

DOI: 10.13700/j.bh.1001-5965.2013.0540, PP. 1134-1142

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Abstract:

太阳质子事件(SPE,SolarProtonEvents)是干扰日地空间最主要的源,大规模质子事件会影响在轨空间站实验设备的可靠性,有时甚至会威胁空间站的安全运行.提出一种基于灰色GM(1,1)和区间估计太阳质子事件预测方法;首先对1976—2010年SPE通量水平数据进行预处理,分别建立以发生时间为序列的一般SPE通量序列与极端SPE通量序列;之后将灰色GM(1,1)与区间估计相结合建立预测方法,融合反映一般SPE通量水平随周期性波动的活跃性调节系数,建立SPE通量水平长期预测模型;然后叠加不同SPE类型所得结果合成预测年份的SPE通量水平,给出未来一年或几年间SPE通量水平的变化范围;最后选取1976—2010年太阳质子事件年均值数据,分多批次预测1996—1998年和1999—2001年等SPE通量均值区间,结果表明各年实际发生SPE的通量均值均位于预测区间内,并且多年预测区间偏差最大值小于26%,实验结果还表明单次预测时长以2~3年为宜.

References

[1]  Jackman C H, Marsh D R,Vitt F M.Northern Hemisphere atmospheric influence of the solar proton events and ground level enhancement in January 2005[J].Atmospheric Chemistry and Physics,2011,11(13):6153-6166
[2]  Veselovskii I S, Yakovchuk O S.On forecasting solar proton events using a ground-based neutron monitor[J].Solar System Research,2011,45(4):354-364
[3]  Verma V K. Relationship of great soft X-ray flares with other solar activity phenomena[J].Astrophysics and Space Science,2011,334(1):83-102
[4]  薛炳森,叶宗海. 太阳质子事件长期预测方法研究[J].载人 航天,2007(4):47-53 Xue Bingsen,Ye Zonghai.Solar proton events forecast method research for a long time[J].Manned Space Flight,2007(4):47-53(in Chinese)
[5]  Hironori S. Solar proton event and proton propagation in the earth's magnetosphere[J].Journal of the National Institute of Information and Communications Technology,2009,56(4): 191- 198
[6]  Belov A. Properties of solar X-ray flares and proton event forecasting[J].Advances in Space Research,2009,43(4):467-473
[7]  King J H. Solar proton fluences for 1977-1983 space missions[J].Journal of Spacecraft and Rockets,1974,11(6):401-409
[8]  Feynman J, Armstrong T P,Dao-Gibner L,et al.New interplanetary proton fluence model[J].Journal of Spacecraft and Rockets,1990,27(4):403-410
[9]  Feynman J, Spitale G,Wang J,et al.Interplanetary proton fluence model:JPL 1991[J].Journal of Geophysical Research:Space Physics (1978—2012),1993,98(A8):13281-13294
[10]  Xapsos M A, Summers G P,Shapiro P,et al.New techniques for predicting solar proto fluences for radiation effects applications[J].IEEE Trans on Nucl Science,1996,43(6):2772-2777
[11]  Xapsos M A, Summers G P,Burke E A.Extreme value analysis of solar energetic proton peak fluxes[J].Solar Physics,1998,183(1):157-164
[12]  Xapsos M A, Summers G P,Barth J L,et al.Probability model for cumulative solar proton event fluences[J].Nuclear Science,IEEE Transactions on,2000,47(3):486-490
[13]  刘思峰,党耀国, 方志耕,等.灰色系统理论及其应用[M].北京:科学出版社,2010 Liu Sifeng,Dang Yaoguo,Fang Zhigeng,et al.The grey system theory and its application[M].Beijing:Science Press,2010(in Chinese)
[14]  李婷婷. 太阳质子事件长期预测模型研究[D].北京:中国科学院,2009 Li Tingting.Solar proton events forecast model research for a long time[D].Beijing:Chinese Academy of Sciences,2009(in Chinese)
[15]  Li R,Cui Y M, He H,et al.Application of support vector machine combined with K-nearest neighbors in solar flare and solar proton events forecasting[J].Advances in Space Research,2008,42(9):1469-1474
[16]  Yoichi K, Tateo G.A new modeling method of solar energetic proton events for ISO specification[J].Advances in Space Research,2008,42(7):1293-1299
[17]  Belov A, Garcia H,Kurt V,et al.Proton events and X-ray flares in the last three solar cycles[J].Cosmic Research,2005, 43(3): 165-178

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