基于化学物质释放的电离层闪烁抑制方法研究
详细信息    查看全文 | 推荐本文 |
  • 英文篇名:Ionospheric scintillation suppression based on chemical release
  • 作者:赵海生 ; 许正文 ; 徐朝辉 ; 薛昆 ; 郑延帅 ; 谢守志 ; 冯杰 ; 吴健
  • 英文作者:Zhao Hai-Sheng;Xu Zheng-Wen;Xu Zhao-Hui;Xue Kun;Zheng Yan-Shuai;Xie Shou-Zhi;Feng Jie;Wu Jian;National Key Laboratory of Electromagnetic Environment,China Research Institute of Radiowave Propagation;
  • 关键词:电离层闪烁 ; 化学物质释放 ; 闪烁抑制
  • 英文关键词:ionospheric scintillation;;chemical release;;scintillation suppression
  • 中文刊名:WLXB
  • 英文刊名:Acta Physica Sinica
  • 机构:中国电波传播研究所电波环境特性及模化技术重点实验室;
  • 出版日期:2019-05-23
  • 出版单位:物理学报
  • 年:2019
  • 期:v.68
  • 基金:国家自然科学基金(批准号:61871352,11672068,61601419)资助的课题~~
  • 语种:中文;
  • 页:WLXB201910035
  • 页数:9
  • CN:10
  • ISSN:11-1958/O4
  • 分类号:305-313
摘要
中低纬地区经常发生的电离层闪烁,严重影响卫星链路的无线电信号传播过程,导致卫星通信导航信号质量下降,甚至中断.在电离层闪烁发生前的酝酿生成期,通过向电离层闪烁"种子因素"的等离子体泡内释放电子密度增强类化学物质,填充等离子体泡,改变等离子体环境特性,调控电离层动力学过程,能够降低电离层等离子体不稳定性增长率,进而抑制闪烁的发生.本文开展了基于化学物质释放的电离层闪烁抑制理论及方法研究,根据化学物质释放对电离层等离子体环境的影响,定量计算控制因素改变对不稳定性增长率的贡献,建立了基于电子密度增强类化学物质释放的电离层闪烁抑制物理模型,仿真了等离子体泡的填充过程及等离子体不稳定性增长率的演化过程.仿真结果表明该方法具有较好的闪烁抑制效果,为我国中低纬地区卫星信号电离层闪烁抑制研究奠定了理论基础.
        There occur frequently the ionospheric scintillation events at low and middle latitudes, which seriously affect the radio transmission process of satellite link, resulting in the decline of satellite communication and navigation signal quality and even interrupt. During the gestation period before the ionospheric scintillation, the growth rate of plasma instability can be reduced and thus suppress the scintillation events by releasing the electron density-enhancing chemicals in the ionosphere plasma bubble, filling with plasma bubble, changing the plasma environmental characteristics, and regulating the ionospheric dynamics process. The theory and method of suppressing the ionospheric scintillation based on chemical release are tnvestigated. According to the change of the plasma environment caused by the chemical release, and the quantitatively calculating of the contribution of control factors to the growth rate of instability, an ionospheric scintillation suppression model is built, which is based on chemical release into ionosphere. The process of plasma bubble filling out is simulated and the results of the simulation show that the plasma cloud is completely filled with plasma bubbles after 1200 seconds, which reduces the plasma density gradient and suppresses the growth of plasma instability. The growth of plasma instability decreases from 0.2 before releasing to about 0.0004 after releasing, and no new instability is excited within 20 minutes after the plasma bubble has been filled up. Guangdong, South China Sea and other regions in China are at the peak of equatorial anomalies, and the occurrence rate and severity of scintillation are more significant than those in the equatorial and Polar Regions, thus these regions become the regions where there occur most frequently the scintillation and the most serious influence globally. The research work of this paper will lay a solid theoretical foundation for the technology of suppressing the satellite signal ionospheric scintillation in middle and low latitude area of China.
引文
[1]Kelley M C 2009 The Earth’s Ionosphere:Plasma Physics&Electrodynamics 2nd Ed(Burlington:Academic Press)pp96-112
    [2]Kuo S P,Cheo B R,Lee M C 1983 J.Geophys.Res.88 417
    [3]Baker D N 2000 IEEE Trans.Plasma Sci.28 2007
    [4]Frederickson A R,Dennison J R 2003 IEEE Trans.Nucl.Sci.50 2284
    [5]Gubby R,Evans J 2002 Atmos.Terr.Phys.64 1723
    [6]Yokoyama T,Shinagawa H,Jin H 2014 J.Geophys.Res.:Space Phys.119 474
    [7]Yokoyama T,Jin H,Shinagawa H 2015 J.Geophys.Res.Space Phys.120
    [8]Klobuchar J A,Abdu M A 1989 J.Geophys.Res.:Space Phys.94 2721
    [9]Dwight P S,Manfred A B,Hake R D 1981 Planet.Space Sci.29 1267
    [10]Sharpee B D,Slanger T G 2006 J.Phys.Chem.110 6707
    [11]Reasoner D L 1992 J.Spacecraft Rockets 29 580
    [12]Caton R G,Pedersen T R,Groves K M,et al.2017 Radio Sci.52 539
    [13]Rettere J,Groves K M,Pedersen T R,Caton R G 2017Radio Sci.52 604
    [14]Bernhardt P A,Siefring C L,Briczinski S J,Viggiano A,Caton R G,Pedersen T R,Holmes J M,Ard S,Shuman N,Groves K M 2017 Radio Sci.52 559
    [15]Holmes J M,Dressler R A,Pedersen T R,Caton R G,Miller D 2017 Radio Sci.52 521
    [16]Pedersen T R,Caton R G,Miller D,Holmes J M,Groves KM,Sutton E 2017 Radio Sci.52 578
    [17]Joshi D,Groves K M,McNeil W,et al.2017 Radio Sci.52710
    [18]Huang W G,Gu S F 2005 J.Space Sci.25 254(in Chinese)[黄文耿,古士芬2005空间科学学报25 254]
    [19]Huang W G,Gu S F 2005 J.Space Sci.28 81(in Chinese)[黄文耿,古士芬2005空间科学学报28 81]
    [20]Hu Y G,Zhang Y N,Zhao Z Y 2010 Acta Phys.Sin.59 8293(in Chinese)[胡耀垓,张援农,赵正予2010物理学报59 8293]
    [21]Hu Y G,Zhao Z Y,Zhang Y N 2011 J.Geophys.Res.116A07307
    [22]Hu Y G,Zhao Z Y,Xiang W 2010 Acta Phys.Sin.60 099402(in Chinese)[胡耀垓,赵正予,项薇2010物理学报60 099402]
    [23]Hu Y G,Zhang Y N,Zhao Z Y 2012 Acta Phys.Sin.61089401(in Chinese)[胡耀垓,张援农,赵正予2012物理学报61 089401]
    [24]Wang S C,Fang H X,Yang S G,et al.2012 Prog.Geophys.27 2464(in Chinese)[汪四成,方涵先,杨升高,等2012地球物理学进展27 2464]
    [25]Wang S C,Fang H X 2013 J.Geophy.56 2906(in Chinese)[汪四成,方涵先2013地球物理学报56 2906]
    [26]Wang S C,Fang H X,Yang S G,et al.2012 J.Atmos.Sci.36 499(in Chinese)[汪四成,方涵先,杨升高,等2012大气科学学报36 499]
    [27]Zhao H S,Feng J,Xu Z W,Wu J,Wu Z S,Xu B,Xue K,Hu Y L 2016 J.Geophys.Res.:Space Phys.121
    [28]Xu Z W,Zhao H S,Wu J,Feng J,Xu B,Zhang Y B,Xue K,Ma Z Z 2017 Adv.Space Res.59 1810
    [29]Zhao H S,Xu Z W,Wu Z S,et al.2016 Acta Phys.Sin.65209401(in Chinese)[赵海生,许正文,吴振森,等2016物理学报65 209401]
    [30]Zhao H S,Xu Z H,Xu Z W,Wu Z S,et al.2018 Acta Phys.Sin.67 019401(in Chinese)[赵海生,许正文,吴振森,等2018物理学报67 019401]
    [31]Liu Y,Cao J,Xu L,et al.2014 Geophys.Res.Lett.45 1413
    [32]Liu Y,Cao J,Xu L,et al.2014 J.Geophys.Res.:Space Phys.119 4134
    [33]Luo W H,Xu J S,Xu L 2009 J.Geophy.Res.52 849(in Chinese)[罗伟华,徐继生,徐良2009地球物理学报52 849]
    [34]Gao J,Guo L,Xu Z,et al.2018 Adv.Space Res.61 2234

© 2004-2018 中国地质图书馆版权所有 京ICP备05064691号 京公网安备11010802017129号

地址:北京市海淀区学院路29号 邮编:100083

电话:办公室:(+86 10)66554848;文献借阅、咨询服务、科技查新:66554700