一种数字调制方式自动识别算法

介绍了利用6个特征参数对7种数字调制方式进行调制方式的自动识别模型算法及仿真结果,表明所提出的自动识别算法能够很好的识别出各种数字调制信号,同时具备算法简单、速度快和准确率高的优点。     

一种小功率逆变电源的设计及实现

介绍了一种小功率逆变电源电路的实现方法。对逆变主电路、电压控制电路、驱动电路、SCOTT电路进行了研究。该逆变电源具有工作可靠、波形失真小的特点。     

高升阻比翼型的设计

使用解析形状函数法和参数化翼型表示方法,将求解绕翼型流场的N-S方程解与优化方法相结合,可设计出新的高升阻比翼型.计算结果表明,设计的新翼型满足设计要求,且获得比原始翼型高得多的升阻比,翼型设计方法是实用的.参数化翼型表示法比解析形状函数法对给定的初始翼型离散数据的准确度影响更小,更适合用于新翼型的设计.     

Fe—10Ni—14Co钢标准状态的组织研究

用透射电子显微镜重点研究了Ｆｅ－１０Ｎｉ－１４Ｃｏ钢的标准处理状态（８３０℃风冷＋—７３℃＋５１０℃Ｓｈ）的微观组织结构。５１０℃回火不同时间，由于Ｍ２Ｃ的析出状态发生变化，钢也由峰时效（５１０℃／１０ｍｉｎ）→过时效（５１０℃／５ｈ）→明显过时效转变。５１０℃５ｈ合会开始发生逆转变。     

合成信号发生器参量的测量不确定度评定

对合成信号发生器测量结果的不确定度进行分析。     

关于阵列式雷达目标模拟器的理论分析

本文权述了阵列式雷达目标模拟器的基本原理。根据模拟目标与实际目标在接收处的反射场及视在中心均应相同的关系导出了三元阵三个阵元的调制信号,并指出这种射频目标仿真既适用于单站情况,也适用于双站情况。     

输出误差函数的交-交矩阵变换器数字PWM调制技术

针对矩阵变换器调制方式的特点，提出了基于输出电压误差函数分析的矩阵变换器离散调制技术，推导了基于时间离散和差分原理的电路方程。根据最小误差函数确定矩阵变换器开关模式，实现了系统闭环控制时开关状态的优化组合。利用α-β平面内的空间矢量描述开关组合状态，使得误差函数的计算工作量小、过程简单，易于实现。数字仿真和实验结果验证了时间离散调制技术的正确性和控制方法的可行性。     

双轴连续旋转调制捷联惯导系统大失准角初始对准技术

由于可以补偿惯性器件在三个轴向上的输出误差，双轴旋转调制技术被广泛应用于捷联惯导系统(SINS)。选择了一种合理且实用的十六次序双轴转位方案，并对其调制原理和误差进行了分析。初始对准技术是捷联惯导系统的一项重要技术，其对准精度直接决定了后续导航的精度。在粗对准完成后，当姿态误差角较大时，后续的精对准误差模型呈非线性特性，故选择了滤波精度高、稳定性强的平方根容积Kalman滤波算法(SCKF)来解决这一问题。考虑到在实际对准过程中，量测噪声的统计特性易发生变化，将SCKF算法与Sage-Husa算法相结合，在传统Sage-Husa SCKF算法的基础上提出了一种改进的自适应滤波算法(ASCKF)。该算法采用QR分解来完成对噪声协方差的平方根矩阵估计，从而避免了传统Sage-Husa SCKF算法中所估噪声协方差矩阵不正定的问题。最后，通过仿真证实了ASCKF算法可被很好地应用于量测噪声统计特性发生变化的初始对准中。     

基于频谱仪的脉冲调制信号功率校准技术研究

脉冲调制信号是雷达和数字通信系统中的一类重要信号。本文主要研究脉冲调制信号的功率测量方法,讨论并分析了脉冲调制信号的频谱特点,提出使用频谱分析仪实现脉冲调制信号的平均功率和峰值功率的测量,并采用正弦调幅法对频谱分析仪的测量结果进行验证。实验表明使用频谱仪测量脉冲调制信号功率简单易行且具有较高的测量精度。     

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.