Volume 36 Issue 3
May  2016
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WANG Yabing, ZHENG Yuqing, GU Bin, DING Liuguan, LE Guiming, LÜ Jianyong. Calculation of the SEP Flux at 1 AU Orbit and Its Comparison with Multi-satellites Observations[J]. Chinese Journal of Space Science, 2016, 36(3): 331-335. doi: 10.11728/cjss2016.03.331
Citation: WANG Yabing, ZHENG Yuqing, GU Bin, DING Liuguan, LE Guiming, LÜ Jianyong. Calculation of the SEP Flux at 1 AU Orbit and Its Comparison with Multi-satellites Observations[J]. Chinese Journal of Space Science, 2016, 36(3): 331-335. doi: 10.11728/cjss2016.03.331

Calculation of the SEP Flux at 1 AU Orbit and Its Comparison with Multi-satellites Observations

doi: 10.11728/cjss2016.03.331 cstr: 32142.14.cjss2016.03.331
  • Received Date: 2015-06-16
  • Rev Recd Date: 2015-12-18
  • Publish Date: 2016-05-15
  • The SEP (Solar Energetic Particles) flux at 1 AU orbit is an important index of space weather condition.Based on the parameterized Green Function solution of the SEP transport equation in the ecliptic plane,the flux profile of the SEP event on 28 Sept.2012 at GOES,STEREO-A and STEREO-B positions on the 1 AU orbit is calculated,and results are compared with available observations.The results show that the flux peak Imax and its occurrence time tmax of the SEP profile are well consistent with the observation of GOES and STEREO-B.However,for STEREO-A, there is an evident difference between our calculation and the observation,which may be induced by the large angle distance between the site and the SEP source and the unknown solar activities on the backside of the Sun.The parameterized SEP flux formula may be applicable for single source impulsive SEP events.

     

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  • [1]
    FANG C, DING M D, CHEN P F. Physics of Solar Active Regions[M]. Nanjing:Nanjing University Press, 2008:337-341(方成, 丁明德, 陈鹏飞. 太阳活动区物理[M]. 南京:南京大学出版社, 2008:337-341)
    [2]
    WANG S, WEI F S. Progress of space weather research in China[J]. Prog. Geophys., 2007, 22(4):1025-1029(王水, 魏奉思. 中国空间天气研究进展[J]. 地球物理学进展, 2007, 22(4):1025-1029)
    [3]
    SCHWENN R. Space weather:the solar perspective[J]. Living Rev. Solar Phys., 2006, 3:1-72
    [4]
    PARKER E N. The passage of energetic charged particles through interplanetary space[J]. Planet. Space Sci., 1965, 13:9-49
    [5]
    BURLAGA W I. Anisotropic diffusion of solar cosmic rays[J]. J. Geophs. Res., 1967, 72(17):4449-4466
    [6]
    QIN G, HE H Q, ZHANG M. An effect of perpendicular diffusion on the anisotropy of solar energetic particles from unconnected sources[J]. Astrophys. J., 2011, 738(1):28
    [7]
    KALLENRODE M B, WIBBERENZ G. Propagation of particles injected from interplanetary shocks:a black box model and its consequences for acceleration theory and data interpretation[J]. J. Geophys. Res., 1997, 102:22311-22334
    [8]
    BIEBER J W, CLEM J, EVENSON P, et al. Relativistic solar neutrons and protons on 28 October 2003[J]. Geophys. Res. Lett., 2005, 32:L03S02
    [9]
    WANG Y, QIN G, ZHANG M, et al. A numerical simulation of solar energetic particle dropouts during impulsive events[J]. Astrophys. J., 2014, 789(2):157
    [10]
    QIN G, WANG Y. Simulations of a gradual solar energe-tic particle event observed by Helios 1, Helios 2, and hboxIMP 8 simultaneously[J]. Astrophys. J., 2015, 809:177
    [11]
    HE H Q, QIN G, ZHANG M. Propagation of solar energe-tic particles in three-dimensional interplanetary magnetic fields:in view of characteristics of sources[J]. Astrophys. J., 2011, 734(2):74
    [12]
    HUANG Y N, WANG Z D, WANG X Y. The interplanetary disturbance of solar cosmic rays[J]. Chin. J. Geophys., 1998, 41(20):149-155(黄永年, 王志丹, 汪学毅. 太阳宇宙线的行星际扰动[J]. 地球物理学报, 1998, 41(20):149-155)
    [13]
    HUANG Y N, WANG Z D, WANG Y L. Propagation models of energetic solar cosmic ray in interplanetary and Green function[J]. Chin. Sci. A, 1998, 41(11):1198-1205
    [14]
    HUANGY N, WANG X Y. Two-step coronal transport of solar flare particles from magnetic multipolarity sources in a flare region[J]. Chin. Phys. Lett., 2001, 18(2):304-307
    [15]
    GU B, NI S L, XIN J, et al. LE G M,DING L G. The calculation of particle flux of impulsive SEP events based on the two-phase model and Green functional theory[J]. Submitted tolinebreak Space Weather
    [16]
    REID G C. A diffusive model for the initial phase of a solar proton event[J]. J. Geophys. Res., 1964, 69:2659-2667
    [17]
    MUELLER-MELLIN R, BOETTCHER S, FALENSKI J, et al. The solar electron and proton telescope for the STEREO mission[J]. Space Sci. Rev., 2008, 136(1/2/3/4):363-389
    [18]
    BAYIN S S. Mathematical Methods in Science and Engineering[M]. New Jersey:Wiley, 2006
    [19]
    DING L G, JIANG Y, ZHAO L, et al. The "twin-CME" scenario and large solar energetic particle events in solar cycle 23[J]. Astrophys. J., 2013, 763(1):30
    [20]
    WANG Y, QIN G. Estimation of the release time of solar energetic particles near the Sun[J]. Astrophys. J., 2015, 799(1):111
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