动态压力校准技术现状分析

动态压力校准技术是确保航天型号压力测试数据准确可靠、量值统一的关键。介绍了动态压力校准的 必要性和特殊性,分别从阶跃压力校准法、周期压力校准法以及脉冲压力校准法三个方面,系统总结了国内外动态 压力校准技术的研究现状,提出目前仍存在的问题并对未来动态压力校准技术的发展提出改进措施。     

水下爆轰燃气泡形态与激波传播过程研究

针对脉冲爆轰发动机在水下工作过程中形成的燃气射流问题,搭建了水下爆轰燃气实验系统,研究了第一个爆轰循环中燃气泡发展变化过程。建立了基于气液两相双流体模型的脉冲爆轰发动机水下喷射模型,采用时-空守恒元和求解元方法,模拟了爆轰波与水相互作用形成的激波的传播及衰减过程。研究结果表明：燃气射流冲击水面时,燃气泡形态在膨胀阶段受到水介质的阻滞作用呈现“豌豆”状,其轴向与径向尺寸有不同的发展规律;同时燃气泡内由于气水冲击作用和燃气扩散受限一直保持较高压力;前导激波传播速度远大于燃气泡发展速度,脱离燃气泡后激波压力值迅速衰减至常压量级,且在中心轴线上的衰减最为剧烈,导致其强度指向性发生改变;前导激波在气液交界面处产生反射,回传的反射激波与后续气流形成的拦截激波碰撞在燃气泡内出现回击现象,使管口附近形成较高的压力峰值。     

障碍物对脉冲爆震火箭发动机性能影响的实验研究（爆震专刊）

为了探究障碍物对脉冲爆震火箭发动机在无阀自适应工作方式下性能的影响,采用汽油为燃料,富氧空气为氧化剂,开展了工作频率为20 Hz的无阀式多循环实验研究。实验中使用Shchelkin螺旋、螺旋凹槽、环形凹槽和孔板等作为障碍物,并分析了其对起爆和推进性能的影响。研究结果表明,Shchelkin螺旋、螺旋凹槽和环形凹槽在阻塞比0.36 ~ 0.56都可实现PDRE的稳定工作,孔板在阻塞比0.56时无法实现爆震的起始;Shchelkin螺旋的DDT距离和DDT时间最短;实验测得的平均推力较理论值有13.3% ~ 39.3%的亏损,阻塞比0.36的Shchelkin螺旋推力损失最小;虽然螺旋凹槽与环形凹槽的流阻损失小,但没有明显的增推效果。     

原子自旋陀螺气室加热电磁噪声抑制实验研究

原子自旋陀螺仪作为目前最新一类陀螺仪,具有超高的理论精度。碱金属气室是原子自旋陀螺仪承载原子自旋的敏感表头。通过电加热使碱金属达到饱和蒸气压,但是电加热过程中会引入电磁干扰等噪声,进而影响原子自旋陀螺仪的精度和灵敏度。为减小碱金属气室加热的电磁噪声对原子自旋陀螺仪的影响,从加热器结构与加热驱动信号2个方面进行了电磁噪声抑制实验研究。设计了具有磁场噪声抑制作用的异形加热膜,使高频正弦波作为加热驱动信号,构建了碱金属气室集成化无磁电加热单元。通过实验验证,系统的等效磁场噪声优于17 fT/Hz1/2,气室内部的温度稳定度优于±0.006 ℃,为原子自旋陀螺仪的性能提升提供了可靠保障。      

用于EMI测量接收机脉冲响应校准的标准脉冲信号产生方法

EMI测量接收机作为电磁兼容测试中的关键仪器应用越来越广泛，但目前该类仪器的脉冲响应校准所用的标准源完全依赖于进口，国内尚无可替代的标准脉冲信号产生器。介绍一种用于EMI测量接收机脉冲响应校准的标准脉冲信号产生方法，首先建立标准脉冲信号的参数模型并对其进行数值分析和仿真，验证其符合CISPR 16-1-1标准的要求，之后搭建实验系统，利用标准脉冲信号生成软件控制任意脉冲信号发生器输出标准脉冲信号并对其进行补偿修正，获得符合CISPR 16-1-1标准要求的标准脉冲信号，该信号可用于EMI测量接收机脉冲响应的校准。     

基于DOA聚类算法的ARM抗有源诱偏技术研究

有源诱偏技术是雷达对抗反辐射导弹的一种重要手段,可以大大降低反辐射导弹的作战效能.为提高对敌目标的精确打击能力,在分析闪烁诱饵诱偏原理的基础上,针对有源诱偏干扰下被动雷达测角精度与稳定度不高的问题,通过对有源诱偏信号的时域特征进行分析,提出一种基于脉冲前沿检测的 DOA 聚类分选算法,找出前沿超前的辐射源信号,实现了高...     

Transitional wave configurations between Type III and Type IV oblique-shock/bow-shock interactions

The interactions of oblique/bow shock waves are the key flow phenomena restricting the design and aerothermodynamic performance of high-speed vehicles. Type III and Type IV Shock/Shock Interactions(SSIs) have been extensively investigated, as such interactions can induce abnormal aerodynamic heating problems in hypersonic flows of vehicles. The transition process between these two distinct types of shock/shock interactions remains unclear. In the present study, a subclass of shock/shock interaction configuration is revealed and defined as Type IIIa. Type IIIa interaction can induce much more severe aerodynamic heating than a Type IV interaction which was ever reported to be the most serious in literature. The intense aerodynamic heating observed in this configuration highlights a new design point for the thermal protection system of hypersonic vehicles. A secondary Mach interaction between shock waves in the supersonic flow path of a Type III configuration is demonstrated to be the primary mechanism for such a subclass of shock/shock interaction configuration.     

固液捆绑火箭热振防护涂层及其防热性能评价

固液捆绑火箭的高温喷焰、固体粒子冲蚀和随机振动相互耦合，对火箭尾部结构造成恶劣的“热振”环境。本文自主研发一种短切碳纤维增强甲基硅橡胶复合烧蚀涂层用于抵抗热振环境。首先，通过廉价的甲基硅橡胶取代昂贵的苯基硅橡胶作为成膜剂从而较大程度降低成本;其次，采用60%孔隙率和80 MPa抗压强度的氧化锆陶瓷微球补强隔热层，引入高比表面积的螺旋状陶瓷纤维强化增韧烧蚀层，利用近红外波段发射率为0.85的MoSi2弥合辐射层的裂纹。经地面热振试验对比分析显示，提出的热振涂层试片背温较主流烧蚀涂层降低约45 ℃，质量烧蚀率降低约38.5%，经过长征六号甲运载火箭的首飞试验验证，该热振涂层具有良好的热振防护性能。     

用于铯光泵磁强计的无磁恒温控制系统设计

针对铯光泵磁强计对原子气室温度高稳定性及无磁干扰的要求，设计了一种用于铯光泵磁强计的无磁恒温控制系统。该系统主要包括无磁加热器件与无磁恒温控制电路。无磁加热器件采用微机电系统工艺的双层对称四线结构，可有效抑制电流产生的磁场；无磁恒温控制电路通过交流加热进一步减小恒定磁场干扰，以现场可编程门阵列为核心，使用直接数字式频率合成技术产生高频加热信号，再经功率放大进行无磁恒温控制，减少硬件电路资源。测试结果表明，气室恒温控制的温度噪声峰峰值可达到0.02 ℃，满足光泵磁强计的性能要求。     

Aspects related to variability of radiative cooling by NO in lower thermosphere,TEC and O/N2 correlation,and diffusion of NO into mesosphere during the Halloween storms

Nitric Oxide is a very important trace species which plays a significant role acting as a natural thermostat in Earth’s thermosphere during strong geomagnetic activity. In this paper, we present various aspects related to the variation in the NO Infrared radiative flux (IRF) exiting the thermosphere by utilizing the TIMED/SABER (Thermosphere Ionosphere Mesosphere Energetics and Dynamics/ Sounding of the Atmosphere using Broadband Emission Radiometry) observational data during the Halloween storm which occurred in late October 2003. The Halloween storm comprised of three intense-geomagnetic storms. The variability of NO infrared flux during these storm events and its connection to the strength of the geomagnetic storms were found to be different in contrast to similar super storms. The connection between the quantum of energy outflux from the upper atmosphere into space in terms of NO IRF and the duration of storms is established. The NO radiative cooling, and the closely correlated depletion in O/N₂ ratio are controlled by the Joule heating intensity (proxied by AE-index). The collisional excitation rate of NO, calculated using the modelled datasets of WACCM-X (Whole Atmosphere Community Climate Model with thermosphere and ionosphere extension), correlates well with the observed pattern of radiative emission by NO. Observational datasets from TIMED/GUVI (Global Ultra-Violet Imager) and MIT Haystack observatory madrigal GNSS (Global navigation satellite system) total electron content (TEC) database shows that the TEC and O/N₂ enhancement in low-mid northern hemispheric latitudes are mainly controlled by the z-component of Interplanetary magnetic field (IMF-B_z). The penetration of eastward electric field during the storm events is found to be responsible for the overall enhancement of TEC. The contribution of enhanced day-side TEC in observed variation of O/N₂ ratio by GUVI is also reported. It is also seen that during substorms related events the night-time polar region experiences more cooling due to NO than the daytime polar region. The connections between the mid- and low-latitude enhancement in NO IRF with the propagation of LSTIDs (Large-scale traveling ionospheric disturbances) in combination with the O/N₂ variability, and the altitudinal variation in NO flux with the progression of the storm is also investigated. This study presents the evidence on the role of diffusion processes in the large scale enhancement of NO in the mesospheric altitudes.