舰面状态直升机机体在起落架上的固有频率分析

针对起落架缓冲支柱和轮胎的非线性特性,应用等效线性模型,提出一种预估刚性机体在弹性起落架上的固有频率计算方法。利用缓冲支柱和轮胎的刚度和阻尼试验数据,采用循环迭代方法计算了机体耦合振动的固有频率;分析了直升机重量、旋翼拉力、舰面运动状态、舰面风力等因素对机体模态固有频率的影响。对最不稳定的机体侧向二阶模态而言,最大设计重量和大升力状态时其固有频率最低,与最小重量、零升力状态相比其稳定转速余度减少约133 r/min;文中假设的舰面运动状态和舰面风力对机体模态的固有频率影响很小,而采用纵、横侧向独立的简化模型来预估机体模态固有频率具有足够的精度。     

GPS授时校频方法研究与试验结果

为了解决多目标综合测量系统各测站之间时间同步和频率校准问题,提出了利用GPS(Global Positioning System)单星或多星共视方法进行站间时间同步与校频,给出了这两种方法的计算公式,分析了星历误差、星钟误差、电离层折射误差、对流层折射误差、多径效应和接收机硬件延迟对时间同步精度的影响.为了验证GPS授时校频精度,进行了相关试验.通过与铯原子钟比对,表明利用GPS可实现纳秒级时间同步,校频精度也优于5.0×10-11,多星共视具有更高的同步校频精度.      

基于直升机平台SAR的方位重影抑制方法

直升机合成孔径雷达(SAR)已成为遥感领域的重要探测工具。针对平台微小高频振动导致方位重影,造成图像质量降低的问题,提出了一种振动相位补偿算法。首先利用回波录取的几何构型,推导基于直升机振动平台的SAR回波表达式,并引入雅可比-安格尔恒等式,对回波完成一阶贝塞尔级数展开,获得高频振动误差与方位向重影的关系式。然后,从直升机SAR实测数据入手,对方位相位进行差分、提取和快速傅里叶变换,得到振动频点信息,并对频点信息进行反演,得到高频误差相位。最后,利用高频误差相位对原始回波进行补偿,抑制成对回波模糊现象,从而消除方位重影。基于实测数据的成像处理结果验证了所提方法的有效性。     

某型干扰机干扰效果提升研究

通过研究某型干扰机对多普勒雷达速度跟踪系统的干扰方式,分析假多普勒频率产生的干扰工作机理,研究对抗科目训练中该模式干扰效果不佳的具体原因,提出了采用数字移向技术替代行波管移相,增大对雷达回波原载频的抑制度,增强干扰效果。通过对样机的测试验证,给出了两种移相电路的假多普勒干扰比较。     

循环频率对CMSX—3单晶合金高温疲劳行为的影响

利用MTS材料试验系统和光学金相、SEM、TEM等分析手段研究了镍单晶高温合金CMSX－3的高温疲劳行为，重点探讨了循环频率对这种行为的影响。结果表明，循环频率的增加会导致合金高渐疲劳寿命的下降及不同的变形机制。     

某型发动机离心通风器齿轮轴组件焊接区域裂纹故障分析

介绍了某型发动机的离心通风器齿轮轴组件在焊接区域裂纹故障的现象。通过结构分析、断口金相检查,并对齿轮轴组件进行了强度、固有频率、共振转速计算和动应力试验研究,结果表明该齿轮轴组件焊接区域裂纹故障属高周疲劳破坏;焊缝与工艺挡边相交处的应力集中较高是导致裂纹故障的主要原因。据此提出排故措施,并完善齿轮结构设计,进行了动态特性分析与试验验证,效果良好。     

超宽带Vivaldi天线的设计及分析

针对机载、弹载等平台的空间有限,设计了一种双指数渐变结构的超宽带Vivaldi天线。天线由微带渐变线馈电,通过矩形共面带线阻抗变换器将小型的超宽带巴伦与天线集成,从而获得2~18GHz的带宽。仿真结果表明:在2~18GHz的工作频段内,天线的回波损耗小于-10dB,天线增益最高可达到10.5dB以上,实测结果与仿真结果基本吻合。将所设计的Vivaldi天线放置于一金属腔体内,对金属腔体对天线性能的影响进行了研究与分析。仿真结果表明:将天线单元放置于金属腔体后,辐射方向相对于原来的辐射方向发生了一定程度的偏转,但随着频率增高,偏转角度逐渐减小。     

Relationship Between Corrosion Level of Steel Bar and Diameter of Corroded Sensing Steel Wire in Wireless Sensor

A kind of wireless sensor was previously developed,which is powered and transmit signals wirelessly instead of using an electrical connection to the embedded reinforcement.Based on this technique,the relationship between diameters of corroded sensing steel wires and corrosion levels of steel bars is established by experiments.Quadratic function is utilized to fit the experiment results,and the correlation coefficients are all larger than 0.95.Estimated corrosion levels of commonly used steel bars are given for different diameters of corroded sensing steel wires fractured due to corrosion.     

熔融石英半球谐振子亚表面缺陷的湿法刻蚀工艺

为了提高半球谐振子的品质因数,提出采用湿法刻蚀的方法去除半球谐振子亚表面的微缺陷。通过研究熔融石英材料的湿法刻蚀机理,在专用半球谐振子湿法刻蚀设备上能够稳定实现半球谐振子亚微米刻蚀精度,半球谐振子经过湿法刻蚀后表面粗糙度优于100nm,半球谐振子Q值能够提高至2000万以上,半球谐振子频差变化小于0.03Hz。     

Monthly mean foF2 model for an African low-latitude station and comparison with IRI

We have employed the hourly values of the ionospheric F-region critical frequency (foF2) obtained from Ouagadougou ionosonde, Burkina Faso (geographic coordinates 12° N, 1.8° W) during the interval of 1985–1995 (solar cycle 22) and solar radio flux of 10 cm wavelength (F10.7) to develop a local model (LM) for the African low-latitude station. The model was developed from regression analysis method, using the two-segmented regression analysis. We validated LM with foF2 data from Korhogo observatory, Cote d’Ivorie (geographical coordinates 9.3° N, 5.4° W). LM as well as the International Reference Ionosphere (IRI) agrees well with observations. LM gave some improvement on the IRI-predicted foF2 values at the sunrise (06 LT) at all solar flux levels and in all seasons except June solstice. The performance of the models at the representing the salient features of the equatorial foF2 was presented. Considering daytime and nighttime performances, LM and IRI are comparable in low solar activity (LSA), LM performed better than IRI in moderate solar activity (MSA), while IRI performed better than LM in high solar activity (HSA). CCIR has a root mean square error (r.m.s.e), which is only 0.10 MHz lower than that of LM while LM has r.m.s.e, which is about 0.05 MHz lower than that of URSI. In general, our result shows that performance of IRI, especially the CCIR option of the IRI, is quite comparable with the LM. The improved performance of IRI is a reflection of the numerous contributions of ionospheric physicists in the African region, larger volume of data for the IRI and the diversity of data sources, as well as the successes of the IRI task force activities.