面向应急条件的多星动态调度方法

 针对应急条件下多星动态调度问题,建立了多目标数学规划模型,提出了应急条件多星成像任务合成策略:建立多星多轨任务合成图(MSMOTMG)模型,提出任务合成算法CP-TM。为克服合成导致任务成像机会减少的缺陷,提出了基于合成任务分解的修复技术。此外,为进一步提高调度效率,考虑了任务在等待队列中的向后移位策略,提出了综合考虑任务合成、修复和向后移位的多星动态应急调度(TMRBS-DES)算法。通过大量模拟实验,将TMRBS-DES算法同RBHA算法,以及3个baseline算法(BS-DES、TMR-DES和TMBS-DES)进行了比较。实验结果表明TMRBS-DES算法提高了调度质量,适用于应急条件下多星动态调度问题。     

MSK信号解调算法研究及其性能仿真比较

最小频移键控(MSK)信号具有相位连续、包络恒定并且带宽占用小的优点,被广泛应用于现代无线通信领域。对MSK解调算法进行了分析总结,将MSK解调算法分为逐符号检测算法和多符号检测算法。根据这两大类检测算法的核心思想,对算法的误码率性能、运算复杂度及应用环境进行了详细分析,总结归纳了各检测算法的优点及存在的问题。实际工程中考虑到接收机的可靠性和成本因素,可以在误码率性能和复杂度之间选取一个折衷,采用合适的解调算法。     

Cosmic ray modulation with a Fisk-type heliospheric magnetic field and a latitude-dependent solar wind speed

The effect of a latitude-dependent solar wind speed on a Fisk heliospheric magnetic field [Fisk, L. A. Motion of the footpoints of heliospheric magnetic field lines at the Sun: implications for recurrent energetic particle events at high heliographic latitudes. J. Geophys. Res. 101, 15547–15553, 1996] was first discussed by Schwadron and Schwadron and McComas [Schwadron, N.A. An explanation for strongly underwound magnetic field in co-rotating rarefaction regions and its relationship to footpoint motion on the the sun. Geophys. Res. Lett. 29, 1–8, 2002. and Schwadron, N.A., McComas, D.J. Heliospheric “FALTS”: favored acceleration locations at the termination shock. Geophys. Res. Lett. 30, 41–1, 2003]. Burger and Sello [Burger, R.A., Sello, P.C. The effect on cosmic ray modulation of a Parker field modified by a latitudinal-dependent solar wind speed. Adv. Space Res. 35, 643–646, 2005] found a significant effect for a simplified 2D version of a latitude-dependent Fisk-type field while Miyake and Yanagita [Miyake, S., Yanagita, S. The effect of a modified Parker field on the modulation of the galactic cosmic rays. In: Proceedings of 30th International Cosmic Ray Conference. Merida, Mexico, vol. 1, 445–448, 2007] found a smaller effect. The current report improves on a previous attempt Hitge and Burger [Hitge, M., Burger, R.A. The effect of a latitude-dependent solar wind speed on cosmic-ray modulation in a Fisk-type heliospheric magnetic field. In: Proceedings of 30th International Cosmic Ray Conference. Merida, Mexico, vol. 1, pp. 449–450, 2007] where the global change in the solar wind speed and not the local speed gradient was emphasized. The sheared Fisk field of Schwadron and McComas [Schwadron, N.A., McComas, D.J. Heliospheric “FALTS”: Favored acceleration locations at the termination shock. Geophys. Res. Lett. 30, 41–1, 2003.) is similar to the current Schwadron–Parker hybrid field. Little difference is found between the effects of a Parker field and a Schwadron–Parker hybrid field on cosmic-ray modulation, in contrast to the results of Burger and Sello and Miyake and Yanagita [Burger, R.A., Sello, P.C. The effect on cosmic ray modulation of a Parker field modified by a latitudinal-dependent solar wind speed. Adv. Space Res. 35, 643–646, 2005 and Miyake, S., Yanagita, S. The effect of a modified Parker field on the modulation of the galactic cosmic rays. In: Proceedings of 30th International Cosmic Ray Conference. Merida, Mexico, vol. 1, pp. 445–448, 2007]. The two-dimensional approximation used by these authors is therefore inadequate to model the complexities of the actual three-dimensional field. We also show that a Fisk-type field with a latitude-dependent solar wind speed (Schwadron–Parker hybrid field) decreases both the relative amplitude of recurrent cosmic ray intensity variations and latitude gradients and yields similar constants of proportionality for these quantities as for the constant solar wind speed case.     

OFDM系统定时偏差补偿算法

为了消除正交频分复用(OFDM,Orthogonal Frequency Division Multiplexing)符号定时偏差对信道估计的影响,提出了一种补偿算法.理论分析表明相移可以被看作是信道统计特性的变化,并且在使用线性插值的信道估计方法时估计误差会扩大.该算法利用符号定时偏差会引起子载波相位旋转的特点,对信道估计进行补偿.仿真结果表明,在多径信道下,在信噪比为20 dB定时位置位于循环前缀中点时,使用该算法后信道估计均方误差是通常线性插值算法的25%,因此新算法缩小了信道估计均方误差.实验结果表明,该算法提高了接收机的性能.     

多路导航信号恒包络处理技术

现代化的导航系统需要在一个频段发射多路导航信号以提高频谱利用率。直接组合的复合信号不是恒包络,在通过饱和状态功率放大器时会产生AM/PM失真,从而影响整个导航系统的定位精度。为了解决这个问题,需要增加互调分量,把信号处理成恒包络复合信号。文章在分析GPS和GALILEO系统导航信号恒包络处理方法的基础上,给出了我国导航卫星系统恒包络处理方法的建议。     

基于多组合窗函数的NLFM信号匹配滤波器设计

文章研究了在相位逗留原理的基础上采用由多种窗函数线性组合得到的组合窗设计NLFM信号的波形与脉冲压缩滤波器,重点分析了组合窗函数的组合参数及窗函数数量对NLFM信号脉冲压缩结果的影响。仿真结果表明,在一定条件下对基于三种窗函数线性组合的组合窗设计的NLFM信号进行谱修正滤波后,主副瓣比（RMS）可提高4．6～8．9dB,而主瓣展宽和主瓣损失变化较小。     

三轴磁强计测量误差修正方法

三轴磁强计测量误差修正对卫星姿态确定和控制具有重要意义。文章针对三轴磁强计测量误差的来源进行理论分析,引入磁场输入引起的常值漂移,建立了三轴磁强计测量误差修正模型,并基于该模型在磁环境模拟器中对Honeywell公司的三轴磁强计（HMR2300R）进行标定。实验结果表明改进模型可以将测量误差控制在50 nT以内,满足低成本敏感器在微小卫星姿态确定中的应用要求。     

卫星导航和惯性导航与时间和空间的理论

从卫星导航和惯性导航的测速定位机理分析出发讨论了时间和空间理论的有关基本问题。提供了一种卫星导航的原理完备的观测方程形式,包括惯性和非惯性物理效应。着重讨论了洛伦兹一次项的效应,伽里略变换自然进化到洛伦兹变换,“同地性”的相对性自然导致“同时性”的相对性。从卫星导航的单程光（电磁）信号的特点出发讨论了爱因斯坦“往”和“返”双程光信号定义带来的困惑。指出哈勃红移是超低速度和超大距离的狭义相对论效应验证。用爱因斯坦对惯性质量和引力质量等效原理的论述,论证了惯性导航的理论基础和超过 3×10 8m/s的速度测量机理。     

导弹无线电引信电磁脉冲效应仿真

以LFM导弹无线电引信为研究对象,以Ansoft软件为仿真平台,建立无线电引信天线模型和电路模型,通过计算机仿真对高功率微波(HPM)干扰导弹无线电引信的效应进行了研究。仿真结果表明,在高功率电磁脉冲作用下,混频器和滤波器上分布的电压很高,而进入执行级的电压很低,达不到启动电压的幅度。     

捷联惯导系统中加速度计的时延补偿研究

In view of the phase shift characteristic inconsisteny between gyros and accelerometers in actual SINS (Strapdown Inertial Navigation System), it’s found that non synchronization velocity errors are considerable under SINS angular motion. Through SINS systemic test, a simple and convenient way to identify the accelerometer time delay parameter is proposed. In this way, a rolling test in gravity fields is designed and the relations between accelerometer time delay parameter and the system’s velocity error are obtained. Moreover, two kinds of methods for non synchronization velocity error compensation are given: one is the time delay extrapolation based on the transfer function model of accelerometer and the other is the velocity error direct compensation based on SINS velocity update algorithm. Finally, by using fiber optic gyro SINS, some experiments are carried out and the results verify that the navigation system’s accuracy is improved effectively and the theoretical analysis is correct.