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基于低轨卫星的分布式超宽带电磁脉冲对地面接收机干扰技术

李永龙 袁雪林 刘九龙 陈正坤 戴志强

李永龙, 袁雪林, 刘九龙, 等. 基于低轨卫星的分布式超宽带电磁脉冲对地面接收机干扰技术[J]. 强激光与粒子束, 2023, 35: 033006. doi: 10.11884/HPLPB202335.220225
引用本文: 李永龙, 袁雪林, 刘九龙, 等. 基于低轨卫星的分布式超宽带电磁脉冲对地面接收机干扰技术[J]. 强激光与粒子束, 2023, 35: 033006. doi: 10.11884/HPLPB202335.220225
Li Yonglong, Yuan Xuelin, Liu Jiulong, et al. Jamming technology of distributed ultra-wideband electromagnetic pulse to ground receivers based on low-orbit satellites[J]. High Power Laser and Particle Beams, 2023, 35: 033006. doi: 10.11884/HPLPB202335.220225
Citation: Li Yonglong, Yuan Xuelin, Liu Jiulong, et al. Jamming technology of distributed ultra-wideband electromagnetic pulse to ground receivers based on low-orbit satellites[J]. High Power Laser and Particle Beams, 2023, 35: 033006. doi: 10.11884/HPLPB202335.220225

基于低轨卫星的分布式超宽带电磁脉冲对地面接收机干扰技术

doi: 10.11884/HPLPB202335.220225
基金项目: 广东省重点领域研发计划项目(2019B111101001); 国防科技创新特区项目(20-163-OO-KX-003-001-02)
详细信息
    作者简介:

    李永龙,liylong27@mail2.sysu.edu.cn

    通讯作者:

    袁雪林,yuanxlin3@mail.sysu.edu.cn

  • 中图分类号: TN972

Jamming technology of distributed ultra-wideband electromagnetic pulse to ground receivers based on low-orbit satellites

  • 摘要: 随着抗干扰技术的不断发展和进步,以阻塞式和欺骗式干扰为代表的传统干扰技术面临挑战。为此,提出了一种基于低轨卫星的分布式超宽带电磁脉冲干扰技术,相比于传统干扰机,超宽带电磁脉冲干扰是一种新型电磁攻击体制。首先,理论推导了重频超宽带电磁脉冲的功率谱;其次,对分布式干扰技术可行性进行分析,并计算了基于低轨卫星平台的分布式干扰所需的发射功率;最后,开展了针对导航接收机低噪放的超宽带电磁脉冲效应实验,并利用STK(Satellite Tool Kit)设计了中低纬度下用于搭载超宽带电磁脉冲干扰机的低轨卫星星座布局。实验结果表明,UWB电磁脉冲可以使低噪声放大器出现暂时增益压缩现象,脉宽为0.7 ns的单脉冲可以使导航信号经过低噪声放大器后被压制近400 ns,重频形式下可以实现信号的完全压制。因此,基于低轨卫星的分布式超宽带电磁脉冲干扰体系可以有效增强干扰效果,有望实现目标区域的全覆盖。
  • 图  1  T=1 ns, fprf=1 MHz时的UWB电磁脉冲序列时频特性

    Figure  1.  Time-frequency characteristics of UWB pulse sequence at T=1 ns and fprf=1 MHz

    图  2  导航接收机射频前端框图

    Figure  2.  Block diagram of the RF front-end of the navigation receiver

    图  3  放大器的非线性压缩示意图

    Figure  3.  Schematic diagram of nonlinear compression of amplifier

    图  4  分布式UWB电磁脉冲干扰体系示意图

    Figure  4.  Schematic diagram of distributed UWB pulse jamming system

    图  5  Marx电路原理图

    Figure  5.  Schematic of Marx circuit

    图  6  UWB电磁脉冲源核心电路

    Figure  6.  Core circuit of UWB electromagnetic pulse source

    图  7  60 dB衰减后UWB输出波形

    Figure  7.  UWB output waveform after 60 dB attenuation

    图  8  LNA效应实验

    Figure  8.  LNA jamming effect experiment

    图  9  星座设计

    Figure  9.  Constellation design

    图  10  卫星覆盖重数

    Figure  10.  Multi-coverage of satellites

    表  1  h=500 km, α=28°时,各干信比下的所需最小合成功率

    Table  1.   Minimum synthetic power required under different JSR at h=500 km and α=28°

    (J/S)/dBminimum synthetic power/dBW
    306.97
    9066.97
    125101.97
    下载: 导出CSV

    表  2  中低纬度卫星覆盖重数

    Table  2.   Multi-coverage of mid-low latitudes satellite

    latitude/(°)minimum visible satellitesmaximum visible satellitesaverage visible satellites
    031.03936.2
    103441.137.2
    2031.039.136.2
    3045.053.049.2
    4068.075.071.5
    5064.071.067.6
    6043.050.046.2
    下载: 导出CSV
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出版历程
  • 收稿日期:  2022-12-26
  • 修回日期:  2023-01-04
  • 录用日期:  2023-01-05
  • 网络出版日期:  2023-01-10
  • 刊出日期:  2023-03-01

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