非正侧视阵列机载雷达多空间角补偿算法

 非正侧阵列机载雷达的杂波分布随距离变化而变化,各距离单元的杂波分布不再满足独立同分布条件,造成统计型空时自适应处理(STAP)处理器性能下降。本文提出了一种多空间角补偿(MSAC)的非正侧视机载雷达杂波抑制方法,该方法先通过角度-多普勒补偿(ADC)预处理以消除在谱中心处的杂波非均匀,然后采用MSAC法在多个多普勒方向使参考单元和待检测单元的杂波谱保持一致,从而进一步消除在其余方位的杂波非均匀。仿真结果表明了该方法的性能明显优于ADC法,且运算量增加不多。     

基于滑动滤波技术的激光陀螺评价方法

激光陀螺是一种以量化脉冲的形式输出角增量的数字传感器，量化误差如同白噪声一样影响着激光陀螺的测试精度。为了准确评价激光陀螺的性能，减少量化误差对激光陀螺测试数据的影响，本文应用滑动滤波技术对激光陀螺采样数据进行滤波处理，理论分析及实验结果表明，该方法有效地降低了量化噪声从而实现了对激光陀螺的准确评价。     

基于不同前角的航空铝合金切削过程分析

为合理选用刀具前角,研究前角变化对航空铝合金7050-T7451切削过程的影响.对前角影响进行理论分析,并借助有限元软件ABAQUS/Explict建立热力耦合的平面应变正交切削模型,采用Johnson-Cook材料本构关系及失效准则模拟不同刀具前角时切屑的形成过程,对比分析了前角变化对切屑形态、切削力和切削温度的影响.仿真结果表明,大前角的刀具有利于改善切削过程,但为避免产生带状切屑,合理的前角范围应为8°～l6°.通过对两种方法的分析结果对比,验证了有限元模型的准确性,对实际加工具有一定的指导意义.     

Digital fixed-frequency hysteresis current control of a BLDC motor applied for aerospace electrically powered actuators

In the conventional cascade control structure of aerospace electrically powered actuators, the current (or electromagnetic torque) loop plays a critical role in realizing a rapid response for a digitally controlled BrushLess Direct Current (BLDC) motor. Hysteresis Current Control (HCC) is an effective method in improving the performance of current control for a BLDC motor. Nevertheless, the varying modulating frequency in the traditional HCC causes severe problems on the safety of power devices and the electromagnetic compatibility design. A triangular carrier-based fixed-frequency HCC strategy is expanded by relaxing the constraints on the rising and descending rates of the winding current to advance the capability of HCC to realize fixed-frequency modulation in the steady state. Based on that, a new flexible-bound-size quasi-fixed-frequency HCC is proposed, and the range feasible to realize fixed-frequency modulation control can cover the entire running process in the steady state. Meanwhile, a corresponding digital control strategy is designed, and four digitalization rules are proposed to extend the capacity to achieve fixed-frequency modulation control to the unsteady working state, that is, a novel fixed-frequency modulation is realized. Simulation and experimental results prove the effectiveness of this improved fixed-frequency HCC strategy.     

Sunspot activity and cosmic ray modulation at 1 a.u. for 1900–2013

The descent of sunspot cycle 23 to an unprecedented minimum of long duration in 2006–2009 led to a prolonged galactic cosmic ray (GCR) recovery to the highest level observed in the instrumental era for a variety of energetic charged particle species on Earth, over a wide range of rigidities. The remarkable GCR increase measured by several ground-based, balloon-borne, and detectors on a satellite is described and discussed. It is accompanied by a decrease in solar wind velocity and interplanetary magnetic field at 1 a.u., reaching the lowest values since measurements of the solar wind began in October 1963; the solar polar field strength (μT) measured at the Wilcox Solar Observatory (WSO) is also significantly reduced compared to prior cycles since the start of the program in 1976, the polar field in the northern hemisphere reversed in June 2012 and again in February 2014, that in the southern hemisphere reversed in July 2013. If updates of WSO data confirm the second reversal in northern solar hemisphere, it would pose a serious challenge to the Dynamo Theory. The long-term change in solar behavior may have begun in 1992, perhaps earlier. The physical underpinnings of these solar changes need to be understood and their effect on GCR modulation processes clarified. The study discusses the recent phenomena in the context of GCR modulation since 1900. These happenings affected our empirical predictions for the key parameters for the next two sunspot cycles (they may be progressively less active than sunspot cycle 24) but it enhanced support for our prediction that solar activity is descending into a Dalton-like grand minimum in the middle of the twentyfirst century, reducing the frequency of the coronal mass ejections; they determine the space weather affecting the quality of life on Earth, radiation dose for hardware and human activities in space as well as the frequency of large Forbush decreases at 1 a.u.     

基于DVB-S2系统APSK信号的分析与干扰仿真

针对DVB-S2系统采用的幅度相位键控(APSK)等高阶调制方式,分析了APSK信号的调制与解调原理,推导了16APSK信号的误比特率(BER)。仿真讨论了基于DVB-S2系统APSK信号在受不同噪声调制干扰和数字调制信号干扰时的误比特率及干扰效果。结果表明:在低干信比(J/s)时数字调制干扰信号干扰效果更好。研究结果可为APSK信号的抗干扰性能研究提供参考。     

集成低频脉冲功率解耦端口的机载电源系统

为了消除高峰均功率比低频脉冲负载对有限容量机载交流供电系统的周期性冲击等不利影响,对开关器件进行集成和复用,提出了能够同时提供功率解耦端口和直流输出端口的三端口功率解耦整流器。通过将三端口整流器与DC/DC变换器组合,构造出集成低频脉冲功率解耦端口的机载电源系统,实现了直流侧周期性脉动功率和交流源侧功率的解耦,并保证低频脉冲负载正常供电需求。详细分析了三端口整流器的工作原理,提出了与之相适应的功率控制方法和调制策略,基于开关器件分时复用原理,实现了交流端口到两个直流端口的功率传输和分配,并实现了两个直流端口功率切换过程的平滑过渡。实验结果验证了所提三端口脉冲功率解耦整流器的有效性和可行性。     

钝锥有攻角分离流动的数值模拟及其分析

本文定性分析了开式分离的性状,并对钝锥有攻角超声速绕流的开式分离作了数值模拟。分析指出,开式分离可能存在两种形态,第一种分离线的起点为正常点,第二种分离线的起始为鞍、结点(包括螺旋点)的组合。对于第一种形态,分离线的起点是横向分离的起始点,除分离线外,分离面上的流线不是从分离线的起点发出的。对文中计算的情况,流动属第一种开式分离。计算证实了定性分析的结论。计算和分析均指出,对第一种开式分离,在分离的起始区域,分离流面尚未卷曲,但在下游,则变成卷曲面。文中还研究了围绕物体的流管在分离诱导下的变形情况。     

星载电场探测仪的传感器空间布局研究

电场探测仪是卫星进行高精度电场探测的关键载荷,其传感器的空间布局对探测精度影响很大。文章对传感器空间布局的影响因素和分析方法进行了研究,并以轨道高度500km的太阳同步轨道卫星为例,结合卫星的实际任务运行,对虚假光电场控制、电场探测仪传感器的几何布局构型、传感器与卫星的相互遮挡和干涉关系进行了分析,并最终优化确定了传感器的空间布局。研究结果表明,优化的传感器空间布局可以在设计阶段就针对多种误差,有效地提高其探测精度。     

双波束天线阵时空调制OFDM通信测向方法

为解决利用通信信号的测向和通信定位综合设计问题,提出了一种载有方向信息的OFDM时空调制技术。该技术采用两副同中心但方向图有偏差的特殊天线阵列发射,使单天线接收机接收的信号是OFDM特性,每个OFDM子载波调制信号载有空间方位信息和数字通信信息,接收机通过解调信号即可通信测向。文中详细介绍了非正交四相和非均匀八相子载波时空调制信号设计思想,阐述了子载波间伪随机码空间调制编码方法,给出了数据信息调解和方位角估计算法。计算机仿真结果表明:在高斯信道下系统的误码性能与普通PSK-OFDM一样,实现了在调制信号设计层面上的数字通信与测向的深度综合。