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质子辐射带辐射中心区域模型

陶宏任 林瑞淋 师立勤 刘四清 张效信 龚建村

陶宏任, 林瑞淋, 师立勤, 刘四清, 张效信, 龚建村. 质子辐射带辐射中心区域模型[J]. 空间科学学报, 2015, 35(3): 293-305. doi: 10.11728/cjss2015.03.293
引用本文: 陶宏任, 林瑞淋, 师立勤, 刘四清, 张效信, 龚建村. 质子辐射带辐射中心区域模型[J]. 空间科学学报, 2015, 35(3): 293-305. doi: 10.11728/cjss2015.03.293
Tao Hongren, Lin Ruilin, Shi Liqin, Liu Siqing, Zhang Xiaoxin, Gong Jiancun. Central Radiation Model of Proton Radiation Belt[J]. Journal of Space Science, 2015, 35(3): 293-305. doi: 10.11728/cjss2015.03.293
Citation: Tao Hongren, Lin Ruilin, Shi Liqin, Liu Siqing, Zhang Xiaoxin, Gong Jiancun. Central Radiation Model of Proton Radiation Belt[J]. Journal of Space Science, 2015, 35(3): 293-305. doi: 10.11728/cjss2015.03.293

质子辐射带辐射中心区域模型

doi: 10.11728/cjss2015.03.293
基金项目: 国家重点基础研究计划项目资助(2012CB825606,2011CB811406)
详细信息
  • 中图分类号: P353

Central Radiation Model of Proton Radiation Belt

  • 摘要: 利用AP-8和CRRESPRO质子辐射带模式数据库, 比较了二者在磁赤道面上计算结果 的差异并给出其差异原因. 利用AP-8模式数据库数据, 建立起质子辐射带函数形式的辐射中心区域模式, 包括各能道全向微分通量峰值所对应的L值(Lc) 随能量E的变化模式以及各能道全向微分通量峰值Jmax随能量E的变化模式. 利用RBSP A卫星REPT望远镜在磁赤道面上的高能质子观测数据, 分别与 AP-8模式、CRRESPRO模式及本文所得辐射中心区域模式计算结果进行比较, 发现在78.9, 102.6和208MeV三个能道上, RBSP A卫星观测所得各能道全向微分 通量明显偏大, 而Lc与AP-8或本文辐射中心模式所得结果基本一致; RBSP A卫星也观测到CRRESPRO Quiet模式所得的隐性第二质子辐射带结构.

     

  • [1] Van Allen J A, McIlwain C E, Ludwig G H. Radiation observations with satellite 1958[J]. J. Geophys. Res., 1959, 64:271-286
    [2] Sawyer D M, Vette J I. AP-8 Trapped Proton Environment for Solar Maximum and Solar Minimum[R]. Greenbelt, MD: NASA Goddard Space Flight Center, 1976
    [3] Mazur J, Friesen L, Lin A, et al. m The Relativistic Proton Spectrometer (RPS) for the radiation belt storm probes mission[J]. Space Sci. Rev., 2013, 179(1-4):221
    [4] Kirby K, Bushman S, Butler M, et al. Radiation belt storm probe spacecraft and impact of environment on spacecraft design[C]//Proceedings of the 2012 IEEE Aerospace Conference. Big Sky Montana: IEEE, 2012
    [5] Lucero A B, Lavine, J P, Vette J I, et al. m Models of the trapped radiation environment, Vol.I[R], NASA SP-3024. Washington DC: NASA, 1966
    [6] King J H. Models of the trapped radiation environment, Vol.IV: low energy protons[R], NASA SP-3024. Washington DC: NASA, 1967
    [7] Lavine J, Vette J I. Models of the trapped radiation environment, Vol.V: Inner belt protons[R], NASA SP-3024. Washington DC: NASA, 1969
    [8] Meffert J D, Gussenhoven M S. CRESSPRO documentation[R]. PL-TR-94-2218. Albuquerque, NM: Phillips Laboratory, the United States Air Force Materiel Command, 1994
    [9] Huston S L, Pfitzer K A. Space environment effects: low-altitude trapped radiation model[R]. Huntsville, AL: Marshall Space Flight Center, 1998
    [10] Heynderickx D, Kruglanski M, Pierrard V, et al. m A low altitude trapped proton model for solar minimum conditions based on SAMPEX/PET data[J]. IEEE Trans. Nucl. Sci., 1999, 46:1475-1480
    [11] Huston S L. Space Environments and Effects: Trapped Proton Model[R]. Huntington Beach, CA: The Boeing Company, 2002
    [12] Xapsos M A, Huston S L, Barth J L, et al. m Probabilistic model for low-altitude trapped-proton fluxes[J]. IEEE Trans. Nucl. Sci., 2002, 49(6):2776-2781
    [13] Lauenstein J M, Barth J L. Radiation belt modeling for spacecraft design: Model comparisons for common orbits[C]//Radiation Effects Data Workshop. Seattle: IEEE, 2005, doi: 10.1109/REDW.2005.1532674
    [14] Ginet G, O'Brien T, Huston S, et al. AE-9, AP-9 and SPM: New models for specifying the trapped energetic particle and space plasma environment[J]. Space Sci. Rev., 2013,179(1-4):579-615
    [15] Cheng Yonghong. The comparison of AP-8 and CRRESPRO[J]. Manned Spacef., 2004(6):56-60. In Chinese (程永宏. 辐射带质子AP-8模式与CRRESPRO模式比较[J]. 载人航天, 2004(6):56-60)
    [16] Miyoshi Y, Morioka A, Misawa H. Long term modulation of low altitude proton radiation belt by the earth's atmosphere[J]. Geophys. Res. Lett., 2000, 27(14):2169-2172
    [17] Shi Liqin, Lin Ruilin, Liu Siqing, et al. m Impact of solar periodic activity on energetic proton in low-altitude radiation belt[J]. Chin. J. Space Sci., 2012, 32(6):804-811. In Chinese (师立勤, 林瑞淋, 刘四清, 等. 太阳周期活动对低高度内辐射带高能质子的影响[J]. 空间科学学报, 2012, 32(6):804-811)
    [18] Zang Zhenqun. The secular variation of geomagnetic field affects the flux computation of radiation belt proton[J]. Chin. J. Space Sci., 1997, 17(1):59-63. In Chinese (臧振群. 地磁场的长期变化对辐射带质子通量计算的影响[J]. 空间科学学报, 1997, 17(1):59-63)
    [19] Fang Xiaohua, Pu Zuyin. Drift shell tracing method and secular variation of inner radiation belt[J]. Chin. J. Space Sci., 2000, 20(2):150-158. In Chinese (方晓华, 濮祖荫. 漂移壳追踪方法与内辐射带的长期变化[J]. 空间科学学报, 2000, 20(2):150-158)
    [20] Yue Guiming, Ye Zonghai, Zhou Guocheng. Low altitude radiation particle environmental variation of satellite orbit caused by geomagnetic secular variation[J]. Chin. J. Space Sci., 2001, 21(3):238-245. In Chinese (乐贵明, 叶宗海, 周国成. 地磁长期变化引起的低高度卫星轨道辐射带粒 子环境的变化[J]. 空间科学学报, 2001, 21(3):238-245)
    [21] Lodhi M, Diaz A B, Wilson T L. Simplified solar modulation model of inner trapped belt proton flux as a function of atmospheric density[J]. Radiat. Meas., 2005, 39(4):391-399
    [22] Stratton J, Harvey R, Heyler G. Mission overview for the radiation belt storm probes mission[J]. Space Sci. Rev. 2014:29-57
    [23] Spence H E, Reeves G D, Baker D N, et al. Science goals and overview of the Radiation Belt Storm Probes (RBSP) Energetic particle, Composition, and Thermal plasma (ECT) suite on NASA's Van Allen Probes Mission[J]. Space Sci. Rev., 2013, 179:311-336
    [24] Baker D N, Kanekal S G, Hoxie V C, et al. The Relativistic Electron-Proton Telescope (REPT) instrument on board the Radiation Belt Storm Probes (RBSP) spacecraft: characterization of Earth's radiation belt high-energy particle populations[J]. Space Sci. Rev., 2013, 179:337-381
    [25] Olson W P, Pfitzer K A. Magnetospheric Magnetic Field Modeling[R]. Huntington Beach, California: McDonnell Douglas Astronaut. Co., 1977
    [26] Finlay C C, Maus S, Beggan C D, et al. International geomagnetic reference field: The eleventh generation[J]. Geophys. J. Intern., 2010, 183:1216-1230, doi:10.1111/j. 1365-246X.2010.04804.x
    [27] Lazutin L. Creation of solar proton belts during magnetic storms: Comparison of two models[C]//Proceedings of the 7th International Conference Problems of Geocosmos. St. Petersburg, Petrodvorets: Saint-Petersburg State University, 2008:152-157
    [28] Mullen E, Gussenhoven M, Ray K, Violet M. A double-peaked inner radiation belt: cause and effect as seen on CRRES[J]. IEEE Trans. Nuc. Sci., 1991, 38(6):1713-1718
    [29] Gussenhoven M S, Mullen E G, Violet M D. Solar particle events as seen on CRRES[J]. Adv. Space Res., 1994:619-629
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出版历程
  • 收稿日期:  2014-04-11
  • 修回日期:  2015-01-14
  • 刊出日期:  2015-05-15

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