Volume 37 Issue 6
Nov.  2017
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BAI Tienan, LE Guiming, ZHAO Haofeng. Statistical Properties of Solar Proton Events during Solar Cycle 23 and 24[J]. Chinese Journal of Space Science, 2017, 37(6): 649-658. doi: 10.11728/cjss2017.06.649
Citation: BAI Tienan, LE Guiming, ZHAO Haofeng. Statistical Properties of Solar Proton Events during Solar Cycle 23 and 24[J]. Chinese Journal of Space Science, 2017, 37(6): 649-658. doi: 10.11728/cjss2017.06.649

Statistical Properties of Solar Proton Events during Solar Cycle 23 and 24

doi: 10.11728/cjss2017.06.649
  • Received Date: 2016-12-07
  • Rev Recd Date: 2017-05-21
  • Publish Date: 2017-11-15
  • There were totally 128 Solar Proton Events (SPEs) from 1997 to 2016. Their peak flux ranges are from 10pfu to 99pfu, 100 to 999pfu, 1000 to 2999pfu and greater than 3000pfu, and the percentage is 55.15%, 27.94%, 9.56% and 7.35% respectively. The results show that SPEs with different peak flux have different asymmetry. The SPEs with peak flux ranged from 1000pfu to 2999pfu have the largest asymmetry, while those with peak flux greater than 3000pfu have smallest asymmetry. In Solar Cycle 23, the SPEs mainly occurred during the period from the first peak to the second peak and after the second peak of the smoothed monthly mean sunspot numbers. In Solar Cycle 24, the SPEs mainly occurred during the period before maximum of smoothed monthly mean sunspot numbers.

     

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  • [1]
    REAMES D V. Particle acceleration at the Sun and in the heliosphere[J]. Rev. Space Sci., 1999, 90(3/4):413-419
    [2]
    TYLKA A J, COHEN C M S, DIETRICH W F, et al. Shock geometry, seed populations, and the origin of variable elemental composition at high energies in large gra-dual solar particle events[J]. Astrophys. J., 2005, 625(1):474-495
    [3]
    GOPALSWAMY N, YASHIRO S, MICHALEK G, et al. Interacting coronal mass ejections and solar energetic particles[J]. Astrophys. J., 2002, 572(1):L103-L107
    [4]
    RICHARDSON I G, LAWRENCE G R, HAGGERTY D K, et al. Are CME interactions really important for accele-rating major solar energetic particle events[J]. Geophys. Res. Lett., 2003, 30(12):8014
    [5]
    KAHLER S W, VOURLIDAS A. Do Interacting coronal mass ejections play a role in solar energetic particle events[J]. Astrophys. J., 2014, 784(1):47
    [6]
    CHEN Minhao, CHEN Yulin, LE Guiming, et al. Dependence of the intensity of solar energetic particle event on the twin-CME:two cases study[J]. Chin. J. Space Sci., 2016, 36(3):267-271(陈#
    [7]
    CANE H V, RICHARDSON I G, VONROSENVINGE T T. A study of solar energetic particle events of 1997-2006:their composition and associations[J]. J. Geophys. Res., 2010, 115(A8):A08101
    [8]
    KUBO Y, AKIOKA M. Existence of thresholds in proton flares and application to solar energetic particle alerts[J]. Space Weather, 2004, 2(1):S01002
    [9]
    LE Guiming. The Carrington longitude distribution of solar proton event source locations during 1997-2003[J]. Chin. J. Space Sci., 2004, 24(2):81-88(乐贵明. 1997-2003年太阳质子事件源区的卡林顿经度分布[J]. 空间科学学报, 2004, 24(2):81-88)
    [10]
    昊, 陈玉林, 乐贵明, 等. 太阳高能粒子事件强度与相关双CME事件关系的两个事例[J]. 空间科学学报, 2016, 36(3):267-271)
    [10]
    LE Guiming, CHEN Yanhong. The statistical analy-sis of solar flares during the interval 1996-2002[J]. Chin. J. Space Sci., 2003, 23(5):321-328(乐贵明, 陈艳红. 1996-2002年太阳耀斑的统计分析[J]. 空间科学学报, 2003, 23(5):321-328)
    [11]
    CHENG Libin, LE Guiming, LU Yangping, et al. The analysis of the properties of super solar proton events and the associated phenomena[J]. Acta Astron. Sin., 2014, 55(3):203-210
    [12]
    MCINTOSH P S. The classification of sunspotgroups[J]. Solar Phys., 1990, 125(2):251-267
    [13]
    GNVEYSHEV M N. On the 11-year cycle of solar activi-ty[J]. Solar Phys., 1967, 1:107-120
    [14]
    GNEVYSHEV M N. Essential features of the 11-year solar cycle[J]. Solar Phys., 1977, 51(1):175-183
    [15]
    BAZILEVSKAYA G A, MAKHMUTOV V S, SLADKOVA A I. Gnevyshev gap effects in solar energetic particle activity[J]. Adv. Space Res., 2006, 38(3):484-488
    [16]
    WANG Jialong, XIAO Zuo, GAO Yufen. Study of high solar activity in February 1986 IV. A preliminary analysis of the relationship between solar and terrestrial events[J]. Chin. J. Space Sci., 1998, 18(4):290-295(王家龙, 肖佐, 高玉芬. 1986年2月的高太阳活动研究——IV日地扰动事件耦合初析[J]. 空间科学学报, 1998, 18(4):290-295)
    [17]
    LE Guiming, YANG Xingxing, DING Liuguan, et al. Solar cycle distribution of strong solar proton events and the related solar-terrestrial phenomena[J]. Astrophys. Space Sci., 2014, 352(2):403-408
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