旋转调制式激光惯性测量单元的误差标定研究

本文针对旋转调制式激光惯性测量单元的结构特点,分析了其误差特性,提出了单元体自旋转的误差标定方法,实现了惯性测量单元的误差分离与快速精确标定.实验证明该方法测试方法简单,操作过程容易,标定结果满足系统精度的需要.     

一种脉宽调制式舵系统舵机模拟器设计方法

针对脉宽调制式舵系统放大器电性能高效测试的问题,提出了一种基于移相脉冲计数的舵机模拟器设计方法。该模拟器硬件由电平转换单元、PWM占空比采集单元、数字PID控制单元和DAC单元四部分组成,软件主要采用移相脉冲计数法和数字PID控制算法,实现了对真实舵机电性能的替代。同时,由单通道扩展的多通道模拟器的应用,能够大幅节约舵机放置空间,缩短研制周期,在短时间内实现PWM放大器电性能大批量测试的目的。试验结果表明,该舵机模拟器能够模拟真实电动舵机的电性能特性,具有实时性好、测试效率高、操作性好的优点,且具有较高的应用价值。     

基于速度积分匹配的旋转调制惯导系统动基座对准方法

卫星导航信息辅助动基座对准过程中,速度噪声会影响对准精度和快速性,制约了旋转调制惯导角秒级高精度快速对准的实现.针对这一问题,提出了一种基于旋转调制惯导速度积分匹配的快速动基座对准方法,通过建立旋转调制惯导动基座对准误差方程和卡尔曼滤波观测模型,以消除动基座对准对载机特殊运动的要求.最后,在实验室静态环境和车载环境下,分别开展了速度积分匹配和速度十位置组合导航动基座对准仿真实验.仿真结果表明,提出的速度积分匹配方法具有误差估计量收敛速度快的特点,在对准精度不降低的情况下相对组合导航匹配方式能有效缩短动基座对准时间,并能基于旋转调制惯导取消动基座对准对载机的机动需求.     

基于Turbo方法的乘积码脉冲位置迭代调制解调译码

脉冲位置调制（PPM）无线光通信系统易受到大气湍流影响，针对于此，将Turbo技术引入到PPM的解调和乘积码译码中。基于极大似然准则导出了PPM软检测解调方法，结合分组码的SISO译码，构建了检测解调和译码联合迭代的Turbo结构，推导了其迭代原理算法。仿真分析结果表明，误码性能可随迭代次数增加改善，其中，在大气闪烁指数0.1和误码率10-6条件下，迭代3~5次相比非迭代系统获得了0.8 dB以上的增益。     

First measurements of periodicities and anisotropies of cosmic ray flux observed with a water-Cherenkov detector at the Marambio Antarctic base

A new water-Cherenkov radiation detector, located at the Argentine Marambio Antarctic Base (64.24S-56.62 W), has been monitoring the variability of galactic cosmic ray (GCR) flux since 2019. One of the main aims is to provide experimental data necessary to study interplanetary transport of GCRs during transient events at different space/time scales. In this paper we present the detector and analyze observations made during one full year. After the analysis and correction of the GCR flux variability due to the atmospheric conditions (pressure and temperature), a study of the periodicities is performed in order to analyze modulations due to heliospheric phenomena. We can observe two periods: (a) 1 day, associated with the Earth’s rotation combined with the spatial anisotropy of the GCR flux; and (b) $～$ 30 days due to solar impact of stable solar structures combined with the rotation of the Sun. From a superposed epoch analysis, and considering the geomagnetic effects, the mean diurnal amplitude is $～$ 0.08% and the maximum flux is observed in $～$ 15 h local time (LT) direction in the interplanetary space. In such a way, we determine the capability of Neurus to observe anisotropies and other interplanetary modulations on the GCR flux arriving at the Earth.