传统宽带自适应波束形成算法在信号带宽较宽时硬件实现困难且形成零陷较窄.针对此问题,利用传感器延迟线阵列结构替代传统的时域抽头延迟线结构,在此基础上提出基于空间响应偏差约束的宽带零陷展宽波束形成方案.对参考频率干扰信号方向...传统宽带自适应波束形成算法在信号带宽较宽时硬件实现困难且形成零陷较窄.针对此问题,利用传感器延迟线阵列结构替代传统的时域抽头延迟线结构,在此基础上提出基于空间响应偏差约束的宽带零陷展宽波束形成方案.对参考频率干扰信号方向邻域的波束响应进行最大值约束,然后利用SRV约束将零陷展宽,通过凸优化工具求得最优加权向量.仿真结果表明,该算法可在保证波束宽度的同时实现宽带零陷展宽.在零陷宽度设定为10?、零陷深度为-30 d B的条件下,零陷宽度实测值可以达到14.7?,且具有较高的输出信干噪比.展开更多
Magnetic reconnection is a main process converting the magnetic energy into thermal and kinetic energy in plasmas. It is one of the fundamental problems of crucial importance not only to space plasmas physics and spac...Magnetic reconnection is a main process converting the magnetic energy into thermal and kinetic energy in plasmas. It is one of the fundamental problems of crucial importance not only to space plasmas physics and space weather studies,such as the solar flare,coronal mass ejections and magnetospheric substorms,but also to the stability analysis in magnetically confined fusion. In general,except for cases with periodical boundary conditions,three-dimensional(3D) magnetic re-connection occurs on magnetic separatrices generated by magnetic nulls. Here we briefly introduce/review the theories and some recent satellite observations of 3D magnetic reconnection. Topics to be further studied are also discussed.展开更多
文摘传统宽带自适应波束形成算法在信号带宽较宽时硬件实现困难且形成零陷较窄.针对此问题,利用传感器延迟线阵列结构替代传统的时域抽头延迟线结构,在此基础上提出基于空间响应偏差约束的宽带零陷展宽波束形成方案.对参考频率干扰信号方向邻域的波束响应进行最大值约束,然后利用SRV约束将零陷展宽,通过凸优化工具求得最优加权向量.仿真结果表明,该算法可在保证波束宽度的同时实现宽带零陷展宽.在零陷宽度设定为10?、零陷深度为-30 d B的条件下,零陷宽度实测值可以达到14.7?,且具有较高的输出信干噪比.
基金Supported by the National Natural Science Foundation of China (Grant Nos. 40390150, 40504021, 10575018, 40536030, 10603008 and 10778613)the National Basic Research Program of China (Grant No. 2006CB806300)+1 种基金as well as the Chinese Academy of Sciences Project (Grant No. KJCX2-YW-T04)the China Double Star-Cluster Science Team
文摘Magnetic reconnection is a main process converting the magnetic energy into thermal and kinetic energy in plasmas. It is one of the fundamental problems of crucial importance not only to space plasmas physics and space weather studies,such as the solar flare,coronal mass ejections and magnetospheric substorms,but also to the stability analysis in magnetically confined fusion. In general,except for cases with periodical boundary conditions,three-dimensional(3D) magnetic re-connection occurs on magnetic separatrices generated by magnetic nulls. Here we briefly introduce/review the theories and some recent satellite observations of 3D magnetic reconnection. Topics to be further studied are also discussed.
