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雷暴电场对宇宙线次级粒子中电子的影响

周勋秀 王新建 黄代绘 贾焕玉

周勋秀, 王新建, 黄代绘, 贾焕玉. 雷暴电场对宇宙线次级粒子中电子的影响[J]. 空间科学学报, 2016, 36(1): 49-55. doi: 10.11728/cjss2016.01.049
引用本文: 周勋秀, 王新建, 黄代绘, 贾焕玉. 雷暴电场对宇宙线次级粒子中电子的影响[J]. 空间科学学报, 2016, 36(1): 49-55. doi: 10.11728/cjss2016.01.049
ZHOU Xunxiu, WANG Xinjian, HUANG Daihui, JIA Huanyu. Effects of Thunderstorms Electric Field on Intensity of Cosmic Ray Electronsormalsize[J]. Journal of Space Science, 2016, 36(1): 49-55. doi: 10.11728/cjss2016.01.049
Citation: ZHOU Xunxiu, WANG Xinjian, HUANG Daihui, JIA Huanyu. Effects of Thunderstorms Electric Field on Intensity of Cosmic Ray Electronsormalsize[J]. Journal of Space Science, 2016, 36(1): 49-55. doi: 10.11728/cjss2016.01.049

雷暴电场对宇宙线次级粒子中电子的影响

doi: 10.11728/cjss2016.01.049
基金项目: 国家自然科学基金项目(11175147, 11475141) 和 中央高校基本科研业务经费专项资金项目(2682014CX091)共同资助
详细信息
    通讯作者:

    周勋秀,E-mail:zhouxx@ihep.ac.cn

  • 中图分类号: P353

Effects of Thunderstorms Electric Field on Intensity of Cosmic Ray Electronsormalsize

  • 摘要: 雷暴期间宇宙线次级粒子强度变化与大气电场的关联研究, 对分析大气电场 加速宇宙线次级带电粒子的机制具有重要意义. 采用Monte Carlo方法, 模拟 研究了雷暴电场对宇宙线次级粒子中电子强度的影响. 结果显示, 在强度为 1000V·cm-1的雷暴电场中, 高海拔处电子数目呈指数增长, 在大气深度约300g·cm-2处达到极大值, 与以往研究提出的相 对论电子逃逸雪崩机制相符. 模拟结果表明, 在地面宇宙线观测实验中, 要想 得到明显的观测效应, 雷暴电场距离探测面的高度应<600m, 电场厚度应 达到约2000m. 模拟结果为分析雷暴电场与地面宇宙线次级粒子中电子强度 的关联性提供了重要参考, 为进一步模拟研究雷暴期间高山地面宇宙线强度的变 化提供了重要信息.

     

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出版历程
  • 收稿日期:  2015-02-04
  • 修回日期:  2015-09-01
  • 刊出日期:  2016-01-15

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