直升机旋翼与机体耦合的空中与地面共振稳定性分析

直升机旋翼气动机械稳定性的一个重要方面是空中与地面稳定性问题。本文从旋翼桨叶的结构型式、气动模型和分析方法几个方面对直升机空中与地面稳定性研究进行了回顾与展望。在简单分析方法的基础上 ,也对更精确的分析方法进行探讨     

两端固定输流管道在脉动内流作用下参数共振的最优控制

采用压电片作为控制执行元件,对两端固定输流管道在脉动流作用下的参数共振进行了最优控制.基于二次型性能指标最优控制原理,针对离散后的运动方程在零平衡点附近Jacobian矩阵的非时变部分设计了最优控制器.最后,通过数值仿真的方法对控制方案的有效性进行了验证.结果表明,该方案对输流管道在第一、第二振型次谐波共振区域及组合共振区域的参数共振的控制均有很好的效果.     

矩形微波谐振腔单模谐振条件

本文首次推导出矩形微波谐振腔的单膜谐振于TE101模的条件。所给出的结论以于单模矩形谐振腔的工程设计具有非常重要的指导意义。     

直升机尾桨/尾梁耦合稳定性分析研究

单桨带尾桨直升机的尾旋翼设计成摆振柔软型后,带来了新的动力学问题:尾桨与尾梁耦合动不稳定性问题。本文简述了它与主旋翼/机体耦合动不稳定问题的差别,主要介绍了尾桨与尾梁耦合动不稳定性问题的分析方法,通过算例分析,为消除这种不稳定性,对一些关键设计参数提出了设计要求。     

Study of ionospheric D region changes during solar flares using MF radar measurements

During solar flares, the X-ray radiation suddenly increases, resulting in an increase in the electron density of the atmospheric D region and a strong absorption of short-wave radio waves. Based on Langfang medium frequency (MF) radar, this paper analyzed the variation characteristics of D region in the lower ionosphere from 62 km to 82 km. The analysis focused on multiple C-level and M-level solar flare events before and after the large-scale flare event at 11:53 (UT) on September 6, 2017. The results show that it is difficult to detect the electron density over 70 km in Langfang during solar flares, but the electron density value can be obtained as low as 62 km, and the stronger the flare intensity, the lower the detectable electron density height. Besides, the equal electron density height, the received power of X and O waves will also be significantly reduced during the flares, and the reduction of equal electron density height has a weak linear relationship with flare intensity.     

相位检测误差对核磁共振陀螺输出频率的影响

针对核磁共振陀螺中采用相位检测方案时可能引起额外频率误差的问题,提出了通过控制电子顺磁共振失谐量及静磁场扰动来抑制额外频率误差的方案。基于Bloch方程,推导了惰性气体原子系综输出频率的表达式,并将相位检测的过程包含在内。建立了考虑相位检测误差的核磁共振陀螺频率误差方程,给出了相位检测引入的额外频率误差表达式并进行了数值仿真。仿真结果表明,通过设定合适的共振失谐量,其额外频率误差至少可以抑制1个数量级,而通过精确地抑制静磁场的一阶及二阶扰动,可以进一步抑制1～3个数量级,将额外频率误差降低到nHz量级。     

Evaluation of the IRI-2016 and NeQuick electron content specification by COSMIC GPS radio occultation,ground-based GPS and Jason-2 joint altimeter/GPS observations

We examined performance of two empirical profile-based ionospheric models, namely IRI-2016 and NeQuick-2, in electron content (EC) and total electron content (TEC) representation for different seasons and levels of solar activity. We derived and analyzed EC estimates in several representative altitudinal intervals for the ionosphere and the plasmasphere from the COSMIC GPS radio occultation, ground-based GPS and Jason-2 joint altimeter/GPS observations. It allows us to estimate a quantitative impact of the ionospheric electron density profiles formulation in several altitudinal intervals and to examine the source of the model-data discrepancies of the EC specification from the bottom-side ionosphere towards the GPS orbit altitudes. The most pronounced model-data differences were found at the low latitude region as related to the equatorial ionization anomaly appearance. Both the IRI-2016 and NeQuick-2 models tend to overestimate the daytime ionospheric EC and TEC at low latitudes during all seasons of low solar activity. On the contrary, during high solar activity the model results underestimated the EC/TEC observations at low latitudes. We found that both models underestimated the EC for the topside ionosphere and plasmasphere regions for all levels of solar activity. For low solar activity, the underestimated EC from the topside ionosphere and plasmasphere can compensate the overestimation of the ionospheric EC and, consequently, can slightly decrease the resulted model overestimation of the ground-based TEC. For high solar activity, the underestimated EC from the topside ionosphere and plasmasphere leads to a strengthening of the model underestimation of the ground-based TEC values. We demonstrated that the major source of the model-data discrepancies in the EC/TEC domain comes from the topside ionosphere/plasmasphere system.     

Electron density inversed by plasma lines induced by suprathermal electron in the ionospheric modification experiment

Incoherent scatter radar (ISR) is the most powerful ground-based measurement facility to study the ionosphere. The plasma lines are not routinely detected by the incoherent scatter radar due to the low intensity, which falls below the measured spectral noise level of the incoherent scatter radar. The plasma lines are occasionally enhanced by suprathermal electrons through the Landau damping process and detectable to the incoherent scatter radar. In this study, by using the European Incoherent Scatter Association (EISCAT) UHF incoherent scatter radar, the experiment observation presents that the enhanced plasma lines were observed. These plasma lines were considered as manifest of the suprathermal electrons generated by the high-frequency heating wave during the ionospheric modification. The electron density profile is also obtained from the enhanced plasma lines. This study can be a promising technique for obtaining the accurate electron density during ionospheric modification experiment.     

基于GaN HEMT和平面变压器的高效率谐振DC/DC变换器

为了提高航天领域高压直流母线DC/DC变换器的效率性能和功率密度,基于氮化镓器件和谐振变换器拓扑,研究矩阵变压器和平面磁元件的优化方法,提出了一种包含等效半匝绕组的变压器绕组结构,实现了多个并联副边绕组间以及多个并联整流器件间的均流,降低了损耗,提高了低压大电流输出时的效率。此外,还研究了模块的并联均流方法,搭建了270 V转28 V、1.2 kW输出的模块单体样机和2.4 kW的多模块并联样机,验证了所提出方法的可行性。     

叶盘耦合振动转/静子叶片数与节径数关系

针对航空发动机中叶盘结构的共振分析问题，通过研究气体激励力和叶盘节径型振动在转子坐标系下的数学表达形式，利用叶盘结构共振时，气体激励力需要对叶盘系统做正功的条件，推导了叶盘发生共振时，节径数与转/静子叶片数应满足的关系式dm=kNv-nNb。通过3个数值算例对上述关系式进行了阐述:从气动功和谐响应分析的角度验证了当上述关系存在时，且激励频率等于结构固有频率时，叶盘系统会发生危害共振；同时指出，当上述变量不满足上述关系时，若激励频率等于叶盘结构的固有频率，也会引起部分叶片发生较大振动的可能。