基于模态反转的半球谐振陀螺零位自校准方法

针对半球谐振陀螺的零位漂移问题，本文研究了基于模态反转电路控制技术的零位自校准方法。首先，从动力学模型引入阻尼不对称、频率裂解等非理想因素，讨论半球谐振陀螺的工作机理及驻波漂移特性。其次，通过理论分析模态反转的零位校准以及虚拟进动控制的模态反转技术。最后，基于FPGA数字控制平台，设计并实现了半球谐振陀螺零位自校准半实物仿真实验。实验结果表明，基于模态反转的半球谐振陀螺零位校准，实现了半球谐振陀螺的零位从15 降低至2 ，短期零偏稳定性和长期稳定性也分别提高了11.8％和45.86％，有效地抑制了零位漂移，提高了半球谐振陀螺测量精度。     

同轴离心式喷嘴热声不稳定性递归分析

为获得同轴离心式喷嘴燃烧动力学特性，开展了喷注单元稳定性试验研究。试验中燃料流量不变，随氧化剂流量增加，热声系统依次经历了燃烧噪声状态、阵发状态和准周期振荡状态。采用递归方法对实验结果进行分析。首先，利用交互信息法和虚假最邻近法分别求解最优延迟时间和嵌入维数，获得了典型工况下的相空间轨迹图。其次，递归图分析表明系统出现了第II类阵发现象，意味着系统发生了亚临界Hopf分叉，与实验结果一致。最后，递归量化分析表明，确定率可以将阵发状态和准周期振荡状态与燃烧噪声状态区分出来，并可以对热声振荡进行预报。     

Injection of 40-kHz-modulated electron beam from the satellite: II. Excitation of electrostatic and whistler waves

Beam-plasma interaction effects are studied during the active space experiment with electron and Xe-ion beam injections in an ionospheric plasma. Permanent 40-kHz-modulated electron beam injection occurs simultaneously with a xenon-ion beam injected by the Hall-type plasma thruster operating in a square-pulse mode (100/50 s for a job/pause duration). The unusual behavior of the background charged particle fluxes and wave activity stimulated during the beam-plasma interaction have been registered by the scientific instruments onboard Intercosmos-25 station (IK-25) and Magion-3 subsatellite. The longitudinal and electromagnetic wave instabilities and their mutual relationship are considered in order to explain the observed effects. The excitation of electrostatic waves by the electron injection has been considered for different resonance conditions near the linear stability boundary. Beam-driven electromagnetic instability is responsible for the backward-propagating whistler waves excited via cyclotron resonance. Competition of these two beam instabilities is one of the subjects of the present study.     

Two-stream instability generation in the lunar ionosphere

The Two-stream Instability (TSI) generation is studied analytically in the lunar ionosphere. The TSI is a tiny perturbation in the electron plasma density, due to which an electric field grows with time and this growth is facilitated by the electron plasma in the background. In lunar ionosphere, the TSI comes into existence when the solar wind interacts unhindered with the tenuous lunar electron plasma in the surface bound exosphere. In this study, the conditions which allow the TSI to form and the subsequent instability growth with time i.e. the growth factor, is estimated. Initially, the threshold condition for the TSI to take place is determined. Thereafter, the solar wind and lunar plasma parameter contribution to trigger TSI is investigated along with the effect of these parameters in the evolution of TSI. The plasma TSI evolution with the passage of time is also depicted in phase space diagram with Particle-In-Cell simulations.     

Daytime VHF amplitude scintillations recorded at an Indian low-latitude station,Waltair (17.7°N, 83.3°E) during 1997–2003

In this research, it is presented the daytime amplitude scintillations recorded at VHF frequency (244 MHz) at an Indian low-latitude station, Waltair (17.7°N, 83.3°E) during seven continuous years (1997–2003). Contrary to the nighttime scintillation seasonal trends, the occurrence of daytime scintillations maximizes during summer followed by winter and the equinox seasons. The fade depths, scintillation indices and the patch durations of daytime scintillations are meager when compared with their nighttime counterparts. A co-located digital high frequency (HF) ionosonde radar confirms the presence of sporadic (Es) layers when daytime scintillations are observed. The presence of daytime scintillations is evident when the critical frequency of the Es-layer (foEs) is ≥4 MHz and Es-layers are characterized by a highly diffuse range spread Es echoes as can be seen on ionograms. It is surmised that the gradient drift instability (GDI) seems to be the possible mechanism for the generation of these daytime scintillations. It is quite likely that the spread Es-F-layer coupling is done through polarization electric fields (Ep) that develop inside the destabilized patches of sporadic E layers, which are mapped up to the F region along the field lines as to initiate the daytime scintillations through the GDI mechanism. Further, the presence of additional stratification of ionosphere F-layer, popularly known as the F3-layer, is observed on ionograms once the Es-layers and daytime scintillations are ceased.     

Case study of inclined sporadic E layers in the Earth’s ionosphere observed by CHAMP/GPS radio occultations: Coupling between the tilted plasma layers and internal waves

We have used the radio occultation (RO) satellite data CHAMP/GPS (Challenging Minisatellite Payload/Global Positioning System) for studying the ionosphere of the Earth. A method for deriving the parameters of ionospheric structures is based upon an analysis of the RO signal variations in the phase path and intensity. This method allows one to estimate the spatial displacement of a plasma layer with respect to the ray perigee, and to determine the layer inclination and height correction values. In this paper, we focus on the case study of inclined sporadic E (E_s) layers in the high-latitude ionosphere based on available CHAMP RO data. Assuming that the internal gravity waves (IGWs) with the phase-fronts parallel to the ionization layer surfaces are responsible for the tilt angles of sporadic plasma layers, we have developed a new technique for determining the parameters of IGWs linked with the inclined E_s structures. A small-scale internal wave may be modulating initially horizontal E_s layer in height and causing a direction of the plasma density gradient to be rotated and aligned with that of the wave propagation vector k. The results of determination of the intrinsic wave frequency and period, vertical and horizontal wavelengths, intrinsic vertical and horizontal phase speeds, and other characteristics of IGWs under study are presented and discussed.     

应用后缘装置的跨声速层流翼型多岛优化设计

高雷诺数状态下,自然层流技术(Natural laminar flow,NLF)是减小机翼表面湍流摩擦阻力的有效方法。然而由于层流翼面上大范围顺压梯度的存在使得后缘处的恢复压差更大,产生更强的激波。因此在减小摩擦阻力的同时又增加了激波阻力。本文采用后缘装置(Trailing edge device,TED)来控制翼型后缘处的激波强度,基于线性稳定性理论(Linear stability theory,LST)的eN方法对流动进行转捩判断,进而应用多岛并行多目标进化算法(multi-objective evolutionary algorithm,MOEA)以获得大范围层流区域和弱化激波强度为目标对翼型进行优化设计。优化结果表明合作均衡策略耦合进化算法可以快速地捕捉到该多目标问题的Pareto阵面解,阵面上翼型的波阻力和摩擦阻力性能较初始翼型大大改善。同时,采用后缘装置控制激波强度时,无论在设计点还是偏离设计点时,优化后翼型均具有良好的升阻力特性和鲁棒性。     

多种工质下螺旋波等离子体源波场结构数值模拟

针对螺旋波等离子体放电机理，开展了多种工质条件下的螺旋波放电等离子体内波场结构数值模拟研究。计算发现:氦气等离子体的Er分量在径向边界处的峰值更为突出，有利于等离子体在径向的输运，波电场径向分量决定了电流密度径向分量在内部的表现。在0.266 Pa和1.064 Pa两种气体压强条件下，通过波场结构验证了气压对于波阻尼影响的结论。波场结构是螺旋波在等离子体内传播以及能量沉积的微观体现，研究螺旋波波场结构是揭示其高电离效率的重要途径。初步探索了功率耦合机制，为实验系统优化及实验方案设定奠定理论基础。     

Flow mechanism between purge flow and mainstream in different turbine rim seal configurations

The rim seal is used to prevent mainstream ingestion to the gap between the vane of a turbine and its blade. In this article, the dolphin lip with a hook configuration and a large seal cavity with hook structures are designed based on the high-pressure turbine datum single shark lip rim seal configuration. The sealing effect and parameters of the flow field are measured by an experiment method and a numerical simulation is used to explain the mechanism. For three configurations, the effect of the leakage slot vortex on the efficiency of the seal and the influence of leakage vortex, generated by the interaction between purge flow and mainstream flow, are discussed in depth. The result shows that the reverse vortex formed by the dolphin lip rim seal with hook structure will increase the sealing efficiency. The seal configuration with a large cavity improves sealing efficiency to a greater extent than the datum structure. At different purge flow rates and with unequal seal structures, the purge flow produces three types of leakage vortices in the passage. Besides, the seal configuration with dolphin lip produces a Kelvin-Helmholtz instability at the interface of the purge and the mainstream flows at a low purge flow rate to induce new leakage vortex branches in the passage of the blade.     

调频连续波合成孔径雷达滑动聚束成像算法

调频连续波(FMCW)体制下,传统脉冲合成孔径雷达(SAR)的"走—停"回波模型已经不再适用,快时间走动项引入的距离-方位耦合项不可以忽略,否则会使图像质量的降低。该文首先构建FMCW回波模型,其次,提出了一种基于两步式的滑动聚束SAR成像算法。所提算法针对滑动聚束模式中,多普勒历程大于脉冲重复频率(PRF)所造成的频谱混叠问题,采用方位频域去斜的预处理加以解决。由于距离徙动校正(RCMC)后方位时域依旧混叠,该算法通过方位去斜在频域完成聚焦避免再一次的解混叠操作。通过仿真验证,该算法能够实现高精度的FMCW SAR滑动聚束成像。