复杂电磁环境下无线接收机电磁兼容快速测试技术应用CSCD

复杂射频电磁环境下,无线接收机作为主要的敏感设备,其电磁兼容性直接影响着整个武器装备的电磁兼容特性. 本文针对GJB 151B中对于接收机非线性测试方法的局限性,引入了一种利用自动双频测试系统对接收机干扰响应的快速测试方法;并搭建了实验室半实物仿真测试平台,检测了某接收机在（ 4-6 ） GHz组合频率干扰下的所有非线性的干扰响应通道. 测试结果对于评估接收机及其所在系统的外部电磁环境适应性具有重要参考价值.     

自制一种高效便利的静压接头

大气数据系统泄漏测试中静压连接困难,目前在用的两种静压接头都各有缺陷,因此自制了一种适用于各种机型的静压接头,其结构简单、高效易用、可靠性高,提高了工作效率。     

飞机变形自动化测量方法研究

为解决以往飞机变形测量模式中人工干预较多,受测量环境影响较大,测量时间长等问题,基于Geo COM技术和RS232,在计算机与全站仪之间进行数据交换,设计了一套自动化测量系统。在测量过程中由标志点的机体理论坐标反算其在当前测站中的极坐标,从而在测量过程中驱动全站仪指向待测点,减少人工瞄准时间,并由计算机实时解算结果数据。经实际飞行试验验证表明,测量时间缩短为原来时间一半,大大提高了工作效率。     

飞翼模型高速风洞PIV试验研究

对小展弦比飞翼标模在2.4米跨声速风洞中创新开展了PIV试验。对空风洞进行了测速校核,并对小展弦比飞翼标模开展了二维、三维涡迹PIV测试,试验马赫数为0.4~0.9。测试结果表明,2.4m风洞PIV试验数据具有较高的准确度,M≤0.8时空风洞测速结果与理论值相差不超过1%,M=0.9时相差不超过2%。小展弦比飞翼标模测试结果显示,M数增大使机翼尾涡涡量和切向速度增大,涡核向内展向方向移动。前缘涡与上翼面分离具有密切关系:当M=0.8、α≤12°时,翼梢测试截面的前缘涡尚未破裂,上翼面未发生显著的流动分离;当α≥13°时,前缘涡破碎时机提前,当地后1/2弦长区域产生了比较明显的流动分离。     

耐高液（气）压部附件测试系统的开发

飞机上耐高液（气）压部附件易发生泄漏破损等问题，对飞机的安全运行至关重要。本文开发了一种测试系统，以气体和液体为介质，以飞机蓄压器为例，通过压力检查、泄露测试、摩擦阻力测试，检测待测部件是否合格。检测结果证明，该测试系统可作为飞机机械系统耐高液（气）压部附件检测的一种参考方法。     

带先进桨尖的模型旋翼悬停噪声计算与试验

为进行旋翼噪声水平对比，在全消声室开展了3副不同下反角桨尖模型旋翼噪声试验研究，完成了悬停状态下不同总距和不同观测点上的噪声测量试验，获得了多组噪声数据。数值计算方面，以RANS方程为主控方程求解旋翼流场气动信息，在获取精确声源信息的基础上，基于FW-H方程进行噪声计算和分析。在相同的状态下，计算结果与试验结果显示出较好的一致性，表明了本文数值方法的准确性。最后，根据试验结果，对比分析了不同下反角桨尖对旋翼气动 噪声特性的影响规律。     

整体加筋壁板剪切试验件的分析与设计

采用有限元方法,对整体加筋壁板5种典型缺口区细节试验件进行了应力分析及屈曲载荷计算,给出了加筋壁板试验件较优结构形式.并对连接区厚度和宽度进行参数化影响分析,得到了剪应力及临界屈曲载荷变化曲线.依据计算结果设计出连接区变宽度变厚度试验件.设计思路和分析方法可为整体加筋壁板剪切试验件的设计提供参考.     

G-16EP通用航空电瓶充放电及寿命研究

为了对G-16EP型电瓶进行维护和保养，根据电瓶厂家规定和适航规范，总结了该型电瓶的充电和容量测试（放电）方法，指出了影响电瓶寿命的主要因素，为该型号电瓶的维护提供了参考。     

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.     

Effects on winter circulation of short and long term solar wind changes

Indices of the North Atlantic Oscillation and the Arctic Oscillation show correlations on the day-to-day timescale with the solar wind speed (SWS). Minima in the indices were found on days of SWS minima during years of high stratospheric aerosol loading. The spatial distribution of surface pressure changes during 1963–2011 with day-to-day changes in SWS shows a pattern resembling the NAO. Such a pattern was noted for year-to-year variations by Boberg and Lundstedt (2002), who compared NAO variations with the geo-effective solar wind electric field (the monthly average SWS multiplied by the average southward component, i.e., negative Bz component, of the interplanetary magnetic field). The spatial distribution of the correlations of geopotential height changes in the troposphere and stratosphere with the SWS; the geo-effective electric field (SWS∗Bz); and the solar 10.7 cm flux suggests that solar wind inputs connected to the troposphere via the global electric circuit, together with solar ultraviolet irradiance acting on the stratosphere, affect regional atmospheric dynamics.