Aero-optical effects simulation technique for starlight transmission in boundary layer under high-speed conditions

Aero-optical effects for starlight transmission in the high-speed flow field will reduce the accuracy of the star sensor on an aircraft. Numerical simulations for aero-optical effects usually require plenty of calculations, which cause difficulties when designing a celestial navigation system for a high-speed aircraft. In this study, an Aero-Optical Simulator For Starlight Transmission (AOSST) in the boundary layer is developed. It effectively reduces the computational burden compared to that of the widely used CFD simulation, and it achieves satisfactory accuracy. In this simulator, gas ellipsoids satisfying certain design rules are used to simulate coherent density structures in boundary layers. Design rules for the gas ellipsoids are found from published experimental and high-fidelity CFD simulation results. The generated wavefront distortion by AOSST is anchored with the scale law for aero-optical distortion in the boundary layer by determining some control parameters, which enables the simulator to output reliable results over a wide range of flight states. Four numerical examples are provided to verify the performance of AOSST. The results demonstrate that AOSST is able to simulate the directional dependence of aero-optical distortions in boundary layers, the variation trend of distorted wavefront shapes with Reynolds number, and the grayscale distribution on the disturbed star map.     

Calibration errors in determining slant Total Electron Content (TEC) from multi-GNSS data

The global navigation satellite system (GNSS) is presently a powerful tool for sensing the Earth's ionosphere. For this purpose, the ionospheric measurements (IMs), which are by definition slant total electron content biased by satellite and receiver differential code biases (DCBs), need to be first extracted from GNSS data and then used as inputs for further ionospheric representations such as tomography. By using the customary phase-to-code leveling procedure, this research comparatively evaluates the calibration errors on experimental IMs obtained from three GNSS, namely the US Global Positioning System (GPS), the Chinese BeiDou Navigation Satellite System (BDS), and the European Galileo. On the basis of ten days of dual-frequency, triple-GNSS observations collected from eight co-located ground receivers that independently form short-baselines and zero-baselines, the IMs are determined for each receiver for all tracked satellites and then for each satellite differenced for each baseline to evaluate their calibration errors. As first derived from the short-baseline analysis, the effects of calibration errors on IMs range, in total electron content units, from 1.58 to 2.16, 0.70 to 1.87, and 1.13 to 1.56 for GPS, Galileo, and BDS, respectively. Additionally, for short-baseline experiment, it is shown that the code multipath effect accounts for their main budget. Sidereal periodicity is found in single-differenced (SD) IMs for GPS and BDS geostationary satellites, and the correlation of SD IMs over two consecutive days achieves the maximum value when the time tag is around 4?min. Moreover, as byproducts of zero-baseline analysis, daily between-receiver DCBs for GPS are subject to more significant intra-day variations than those for BDS and Galileo.     

基于石墨烯的量子化霍尔电阻研究综述

电阻作为重要的元器件在电气电子及其他非电领域得到了广泛应用,对其阻值进行准确溯源和量值传递至关重要。相较于实物电阻计量标准,量子化霍尔电阻标准稳定性和准确性更高。目前我国国家/国防量子化霍尔电阻计量基准是基于砷化镓-铝砷化镓异质材料制成的,其对环境温度和外磁场要求高,普通计量实验室难以复现。石墨烯材料的出现为新型量子化霍尔电阻基准/标准的研制提供了可能。本文简述了石墨烯材料的制备方法及其量子化霍尔效应,介绍了石墨烯量子化霍尔效应的国外研究现状,分析了基于石墨烯材料的量子化霍尔电阻标准在研制过程中存在的问题,旨在为我国新型量子化霍尔电阻标准的研制提供参考。     

On the anthropogenic and natural injection of matter into Earth’s atmosphere

Every year, more and more objects are sent to space. The increasing number of countries with space programs, advancing commercialization, and ambitious satellite constellation projects raise concerns about space debris and the increase of mass flux into the atmosphere due to deorbiting of satellites and rocket bodies. A comparison of this anthropogenic influx to the natural influx due to meteoroids is presented giving detailed information about the mass, composition and ablation of the entering matter. Currently, anthropogenic material does make up about 2.8% compared to the annual injected mass of natural origin. For two different future scenarios considering planned and already partially installed large satellite constellations this fraction increases to nearly 13%, respectively 40%. For these cases, the anthropogenic injection of several metals prevails the injection by natural sources by far. Considering different ablation products, we find that the anthropogenic injection of aerosols into the atmosphere increases disproportionately. Today, they make up about 1% compared to the injected aerosol mass of natural origin, increasing to 30% and 94% for the two future scenarios, respectively. Considering the injection of atoms, the natural injection is dominant by far. For the two future scenarios, the anthropogenic injection is only at 5%, respectively 15% compared to the annual natural atom injection. The predicted strong increase in anthropogenic injection will make it significant in comparison to the natural injection which can have yet unknown effects on Earth’s atmosphere and the terrestrial habitat.     

Experimental study of curvature effects on jet impingement heat transfer on concave surfaces

Experimental study of the local and average heat transfer characteristics of a single round jet impinging on the concave surfaces was conducted in this work to gain in-depth knowledge of the curvature effects. The experiments were conducted by employing a piccolo tube with one sin-gle jet hole over a wide range of parameters: jet Reynolds number from 27000 to 130000, relative nozzle to surface distance from 3.3 to 30, and relative surface curvature from 0.005 to 0.030. Exper-imental results indicate that the surface curvature has opposite effects on heat transfer characteris-tics. On one hand, an increase of relative nozzle to surface distance (increasing jet diameter in fact) enhances the average heat transfer around the surface for the same curved surface. On the other hand, the average Nusselt number decreases as relative nozzle to surface distance increases for a fixed jet diameter. Finally, experimental data-based correlations of the average Nusselt number over the curved surface were obtained with consideration of surface curvature effect. This work con-tributes to a better understanding of the curvature effects on heat transfer of a round jet impinge-ment on concave surfaces, which is of high importance to the design of the aircraft anti-icing system.     

临近空间高超声速飞行器天文导航系统综述

临近空间是航天与航空业务领域的结合部，具有重要的战略价值。高超声速飞行器是临近空间力量部署的重要载体，已逐渐进入应用部署阶段。临近空间高超声速飞行器的飞行环境和任务条件对导航系统提出了新的更高要求。在总结临近空间高超声速飞行器的导航技术研究进展的基础上，对天文导航技术的应用环境和条件进行了系统的分析和探讨，提出了5个重点研究方向，包括：星图采集效能、光学误差模型、视场观测机理、姿态更新速率、小型化模块化工程化等。研究结果可为临近空间高超声速飞行器天文导航系统的设计提供参考。     

极端瞬态力作用下金属壳谐振陀螺结构强度分析

金属壳谐振陀螺是利用驻波的进动特性来敏感输入角速率的一种新型壳体振动陀螺，其具有结构简单、功耗低、抗冲击性强、稳定性高等优点，可被广泛应用于中低精度角速度测量领域。针对极端瞬态力作用下金属壳谐振陀螺的结构强度进行了研究，在分析其工作原理和基本数学模型的基础上，利用有限元仿真方法，在通用炮射环境条件下进行了分析。通过仿真计算，给出了金属壳谐振陀螺的结构强度分析结果，验证了其抗过载能力。     

舰载机着舰舰面效应及其补偿方法研究

根据舰面效应的作用机理,分析了舰面效应对舰载机着舰的影响,总结了舰载机在不同着舰模式下的舰面效应补偿方法.针对舰载机自动着舰模式,通过分析舰面效应所产生的附加升力造成的着舰偏差,提出了引导信号指令修正的舰面效应补偿方法,并给出了舰面效应自动补偿方法的具体流程,分析了自动补偿方法的特性及其应用面临的关键问题.     

蜂窝状薄壁管拉伸时的收缩分析

为研究蜂窝材料拓扑结构与其整体力学性能的关系，从非平面Vertex模型的势能形式出发，结合蜂窝薄壁管拉伸时的轴对称特征，通过变分法得到了管拉伸时母线满足的控制方程，证实了边界效应是蜂窝状薄壁管受拉时产生收缩的原因，并结合控制方程的若干特解，考察了非平面Vertex模型中材料参数对管弯曲程度的影响。结果表明，非平面Vertex模型中表征夹角势强度的参数决定了材料的整体抗弯性，而距离管端最近的3层元胞是管拉伸时的主要收缩区。最后进一步探讨了蜂窝薄壁管曲率与收缩幅度之间的非线性关系，揭示了构型曲率是蜂窝材料泊松比的影响因素之一。     

Effects of tooth bending damage on the leakage performance and rotordynamic coefficients of labyrinth seals

Tooth bending damage resulting from an intense impact by the rotor sometimes occurs in the transient operation. To investigate the influence of after-damage clearance and tooth bending length on the leakage performance and rotordynamic coefficients of labyrinth seals, three tooth bending damages were taken into consideration, including the unbent tooth damage (abbreviated as Unbent), the partial tooth bending damage (abbreviated as Pbent) and the complete tooth bending damage (abbreviated as Cbent). The transient CFD solution was utilized to calculate the leakage flow rates and rotordynamic coefficients of labyrinth seals with clearances of 0.3, 0.4, 0.5, 0.6 mm for three tooth bending damages. The obtained result shows that the Unbent tooth damage leaks least while the Pbent tooth bending damage leaks most, and an increase of 6.1% for Cbent tooth bending damage and an increase of 19.4% for Pbent tooth bending damage are discovered at the tooth clearance of 0.6 mm in comparison with the Unbent tooth damage. Compared to the Unbent tooth damage, the effective damping for Pbent tooth bending damage and Cbent tooth bending damage is lower and drops by 9.7%–33.6% and 8.5%–22.6% respectively at the tooth clearance of 0.6 mm, suggesting that Pbent tooth bending damage or Cbent tooth bending damage tends to weaken the seal stability when compared to the Unbent tooth damage.