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南大西洋异常区高能质子通量南北向差异

闫兴亚 陈鸿飞 于向前 邹鸿 施伟红

闫兴亚, 陈鸿飞, 于向前, 邹鸿, 施伟红. 南大西洋异常区高能质子通量南北向差异[J]. 空间科学学报, 2016, 36(6): 888-896. doi: 10.11728/cjss2016.06.888
引用本文: 闫兴亚, 陈鸿飞, 于向前, 邹鸿, 施伟红. 南大西洋异常区高能质子通量南北向差异[J]. 空间科学学报, 2016, 36(6): 888-896. doi: 10.11728/cjss2016.06.888
YAN Xingya, CHEN Hongfei, YU Xiangqian, ZOU Hong, SHI Weihong. The Southward and Northward Difference of Proton Flux in South Atlantic Anomaly[J]. Chinese Journal of Space Science, 2016, 36(6): 888-896. doi: 10.11728/cjss2016.06.888
Citation: YAN Xingya, CHEN Hongfei, YU Xiangqian, ZOU Hong, SHI Weihong. The Southward and Northward Difference of Proton Flux in South Atlantic Anomaly[J]. Chinese Journal of Space Science, 2016, 36(6): 888-896. doi: 10.11728/cjss2016.06.888

南大西洋异常区高能质子通量南北向差异

doi: 10.11728/cjss2016.06.888
基金项目: 

国家自然科学基金项目(41374181)和国家重大科学仪器专项项目(2012YQ03014207)共同资助

详细信息
    通讯作者:

    闫兴亚,E-mail:yanxia0522@163.com

  • 中图分类号: P353.4

The Southward and Northward Difference of Proton Flux in South Atlantic Anomaly

  • 摘要: 利用2012年8月NOAA N15,N16,N17,N18卫星中能质子和电子探测器(MEPED)>6.9MeV质子能档的数据,研究了800km高度处南大西洋异常区(SAA)质子分布的南北方向差异.数据显示,质子计数率沿经线随纬度的变化近似满足高斯分布,且向南运动的质子多于向北运动的质子.MEPED具有0°和90°两个探测方向,可对质子投掷角分布进行估算,从而消除在探测南向和北向质子时探测器方向角偏差所造成的影响.结果表明,在经度40°W、纬度13°S至23°S位置上,仍然存在南向质子比北向质子多20%~30%的现象.其原因可能与地磁异常使南向质子镜像点更低,更多质子散射进入大气层沉降有关.分析还发现,南大西洋异常区质子通量存在地方时变化.日侧比夜侧强约20%,这可能是由于地磁场日变化引起的.

     

  • [1] CHEN Guozhen, LIN Guocheng. The influence of charged particle radiation environment on the spacecraft at LEO[J]. Chin. Space Sci. Tech., 1994(6):43-48(陈国珍, 林国成. 低地球轨道带电粒子辐射环境对航天器的影响[J].中国空间科学技术, 1994(6):43-48)
    [2] TVERSKAYA L. Dynamics of the Earth's radiation belt[J]. Moscow Univ. Phys. Bull., 2010, 65(4):246-251
    [3] BADHWAR G D, KONRADI A. Conversion of omnidirectional proton fluxes into a pitch angel distribution[J]. J. Spacecraft Rockets, 1990, 27(3):350-352
    [4] EVANS H, DALY E. Anisotropies in the low altitude radiation environment[J]. J. Br. Interplanet. Soc., 1995, 48:149-151
    [5] GLAUERT S A, RICHARD B H. Calculation of pitch angle and energy diffusion coefficients with the PADIE code[J]. J. Geophys. Res: Space Phys., 2005, 110(A4). DOI: 10.1029/2004JA010851
    [6] KUZNETSOV N V, NIKOLAYEVA N I. Empirical model of pitch angel distributions of trapped protons on the inner boundary of the earth radiation belt[J]. Cosmic Res., 2012, 50(1):13-20
    [7] QIN M R, ZHANG X G, NI B B, et al. Solar cycle variations of trapped proton flux in the inner radiation belt[J]. J. Geophys. Res. Space Phys., 2014, 119(12):9658-9669
    [8] YANG X C, WANG S J, LIANG J B, et al. Multidirectional design research of the sun-synchronous orbit electron detectors[J]. J. Astron., 2013, 33(2):281-284(杨晓超, 王世金, 梁金宝, 等. 太阳同步轨道电子探测器的多方向设计研究[J]. 宇航学报, 2013, 33(2):281-284)
    [9] SLESNICK R S, BAKER D N, JAYNES A N, et al. Observations of inner radiation belt: CRAND and trapped solar protons[J]. J. Geophys. Res.: Space Phys., 2014, 119(8):6541-6552
    [10] ZHAO H, LI X, BLAKE J B, et al. Characteristic of pitch angel distribution of hundreds of keV eletrons in the slot region and inner radiation belt[J]. J. Geophys. Res.: Space Phys., 2014, 119(12):9543-9557
    [11] ZHAO H, LI X, BLAKE J B, et al. Peculiar pitch angel distribution of relativistic eletrons in inner radiation belt and slot region[J]. Geophys. Res. Lett., 2014, 41(41): 2250-2257
    [12] CAMPANA R, ORLANDINI M, MONTE E D, et al. The radiation environment in a low earth orbit: the case of BeppoSAX[J]. Exp. Astron., 2014, 37:599-613
    [13] HEIRTZLER J R. The future of the South Atlantic anomaly and implications for radiation damage in space[J]. J. Atmos. Solar-Terr. Phys., 2002, 64:1701-1708
    [14] EVANS D S, GREER M S. Polar orbiting Environmental Satellite Space Environment Monitor-2: Instrument Descriptions and Archive Data Documentation: NOAA Technical Memorandum OAR SEC-93[R]. Boulder, Colorado: NOAA, 2000
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出版历程
  • 收稿日期:  2015-11-13
  • 修回日期:  2016-03-31
  • 刊出日期:  2016-11-15

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