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Solar wind electrons reflected by lunar electric and magnetic fields
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  • 作者:YongYong Feng (1) (2)
    YiTeng Zhang (1)
    Hua Zhao (1)
    ZhenXing Liu (1)
  • 关键词:surface potential ; solar wind electron ; remote sensing
  • 刊名:Science China Earth Sciences
  • 出版年:2011
  • 出版时间:November 2011
  • 年:2011
  • 卷:54
  • 期:11
  • 页码:1796-1800
  • 全文大小:1221KB
  • 参考文献:1. Feng Y Y, Xu R L, Zhao H. Solar wind electrons reflected by the lunar crustal magnetic field (in Chinese). Chin J Space Sci, 2009, 29: 1鈥?
    2. Halekas J S, Mitchell D L, Lin R P, et al. Evidence for negative charging of the lunar surface in shadow. Geophys Res Lett, 2002, 29, doi: 10.1029/2001GL014428
    3. Halekas J S, Lin R P, Mitchell D L. Inferring the scale height of the lunar night-side double layer. Geophys Res Lett, 2003, 30, doi:10.1029/2003GL08421
    4. Halekas J S, Lin R P, Mitchell D L. Large negative lunar surface potentials in sunlight and shadow. Geophys Res Lett, 2005, 32: GL022627 CrossRef
    5. Halekas J S, Delory G T, Brain D A, et al. Extreme lunar surface charging during solar energetic particle events, Geophys Res Lett, 2007, 34: L02111, doi: 10.1029/2006GL028517 CrossRef
    6. Freeman J W, Ibrahim M. Lunar electric fields, surface potential and associated plasma sheaths. Moon, 1975, 14: 103鈥?14 CrossRef
    7. Stubbs T J, Halekas J S, Farrell W M, et al. A dynamic fountain model for lunar dust. Adv Space Res, 2006, 37: 59鈥?6 CrossRef
    8. Shina K, Tomoko N. Electromagnetic full particle simulation of the electric field structure around the moon and the lunar wake. Earth Planet Spance, 2008, 60: 591鈥?99
    9. Zong Q G, Wilken, B, Reeves G D, et al. Geotail observation of energetic ion specics and magnetic field in plasmoid-like structures in the course of an isolated substorm event. J Geophys Res, 1997, 102: 11409鈥?1428 CrossRef
    10. Zong, Q G, Wilken B, Woch J, et al. Energetic oxygen ion bursts in distant magneto-tail as a product of intense substorms: Three case studies. J Geophys Res, 1998, 103: 20339鈥?0363 CrossRef
    11. Zong Q G, Fritz T A, Pu Z Y, et al. Cluster observations of earthward flowing plasmoid in the tail. Geophys Res Lett, 2004, 31: L18803, doi: 10.1029/2004GL020692 CrossRef
    12. Xu R L, Li L. Magnetospheric Particle Dynamic. Beijing: Science Press, 2005
    13. Shi Q Q, Pu Z Y, Soucek J. Spatial structures of magnetic depression in the Earth鈥檚 high-altitude cusp: Cluster multipoint observations. J Geophys Res, 2009, 114: A10202, doi: 10.1029/2009JA014283 CrossRef
    14. Shi Q Q, Zong Q G, Zong H, et al. Cluster observations of the entry layer equator-ward of the cusp under northward interplanetary magnetic field. J Geophys Res, 2009, 114: A12219, doi: 10.1029/2009JA 014475 CrossRef
    15. Feng Y Y, Zhao H, Liu Z X. Simulation of electrons鈥?trajectories in the lunar electric and magnetic field (in Chinese). Chin J Space Sci, 2011, 31: 165鈥?69
    16. Shi Q Q, Shen C, Pu Z Y, et al. Dimensional analysis of observed structures using multipoint magnetic field measurements: Application to Cluster. Geophys Res Lett, 2005, 32, L12105, doi: 10.1029/2005 GL022454 CrossRef
  • 作者单位:YongYong Feng (1) (2)
    YiTeng Zhang (1)
    Hua Zhao (1)
    ZhenXing Liu (1)

    1. State Key Laboratory of Space Weather, Center for Space Science and Applied Research, Chinese Academy of Sciences, Beijing, 100190, China
    2. Graduate University of Chinese Academy of Sciences, Beijing, 100049, China
  • ISSN:1869-1897
文摘
In this paper, we report on our study of the trajectories of solar wind electrons reflected by lunar electric and magnetic fields through analysis of reflectivity and distribution under different conditions. Our calculations and simulations showed that the variations of both the magnetic field and surface potential play important roles in changing the directions of the traces of electrons. Furthermore, we were able to distinguish the changes resulting from these two variations through further analysis of the results. Thus, both the magnitude of the crustal field and the surface potential can be acquired from the data of satellites such as the Lunar Prospector. These findings could also contribute to the design and development of new devices in future lunar programs.

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