Q/V频段电磁波在等离子体鞘套下的传输特性

高超声速飞行器再入地面时,由于飞行器表面等离子体电子密度分布不均匀,因此从背风面向天基中继卫星传输,可避开迎风面的高电子密度,并以Q/V频段为测控频段,经中继卫星转发至地面测控站。本文以波阻抗方法为基础,分析了Q/V频段在不同等离子体参数下的传输特性,并仿真了等离子体对Q/V频段天线波束指向的影响。结果表明：Q/V频段在等离子体中穿透性更好,可在更高的等离子体电子密度和碰撞频率下保持较低的衰减值。但Q/V频段下的天线波束指向偏差较大,随着频段的提高和入射角度的减小,偏差值逐渐减小。因此,应用Q/V频段,通过中继卫星转发实现实时通信,有利于缓解再入飞行器“黑障”现象。     

基于室内无线模型的穿墙损耗校正

K-M（Keenan-Motley）模型将单墙固定损耗值相加来计算室内无线信号穿透多墙的总损耗值,存在较大误差。针对该问题选取多种室内场景分别进行连续波（Continuous Wave,CW）测试,对无线信号穿墙损耗的影响因素和变化规律进行分析,提出了一种基于人工神经网络的室内无线模型穿墙损耗校正方法,对预处理后的测试数据进行训练并建立预测模型。经验证该预测模型符合校正判别准则,在实际场景下具有良好的预测准确度。     

CO2焊模糊波控逆变电源与平特性逆变电源焊接性能对比研究

本文介绍了CO2 焊模糊波控逆变电源的原理 ,对其焊接性能与带电子电抗器的平特性逆变电源作了对比研究。结果表明 :模糊波控逆变电源无论在焊接飞溅量 ,焊缝成型及可控性 ,还是在焊接过程的稳定性上都较带电子电抗器的平特性逆变电源有很大的提高。并对其原因进行了探讨     

Hemispheric Distribution of Lower-band Chorus Waves Observed by Van Allen Probes

Whistler mode chorus waves are important electromagnetic emissions due to their dual roles in acceleration and loss processes of Earth’s radiation belt electrons. A detailed global survey of lower-band chorus is performed using EMFISIS data from Van Allen Probes in near-equatorial orbits. In addition to the confirmation of the positive correlation of chorus wave intensities to geomagnetic activity and dayside-nightside distribution asymmetry of wave amplitude and occurrence probability, the analysis results find that in statistics lower-band chorus emissions exhibit higher wave occurrence rates and larger normalized peak wave frequencies in the magnetically northern hemisphere but somehow stronger peak wave intensities in the magnetically southern hemisphere. While overall the differences between the two magnetically hemispheric distributions tend to be not significant, it is important to establish the magnetically hemispheric distribution profiles of lowerband chorus with respect to L-shell, magnetic local time, and geomagnetic latitude for improved understanding of chorus-induced dynamics of radiation belt electrons.     

Spatio-temporal structure of the wave packets generated by the solar terminator

Using long-term (1998--2009) total electron content (TEC) measurements from the GPS global network including dense network of GPS sites in USA and Japan, we have obtained the first data regarding the spatio-temporal structure and the statistics of medium-scale traveling wave packets (MS TWPs) excited by the solar terminator (ST). Total amount of the detected TWPs exceeds 565,000. There is no correlation between TWPs occurrence and geomagnetic and solar activity. We found that the diurnal, seasonal and spectral MS TWPs characteristics are specified by the solar terminator (ST) dynamics. MS TWPs are the chains of narrow-band TEC oscillations with single packet’s duration of about 1–2 h and oscillation periods of 10–20 min. The total duration of chain is about 4–6 h. The MS TWPs spatial structure is characterized by a high degree of anisotropy and coherence at the distance of more than 10 wavelengths. Occurrence rate of daytime MS TWPs is high in winter and during equinoxes. Occurrence rate of nighttime MS TWPs has its peak in summer. These features are consistent with previous MS travelling ionosphere disturbance (TID) statistics obtained from 630-nm airglow imaging observations in Japan. In winter, MS TWPs in the northern hemisphere are observed 3–4 h after the morning ST passage. In summer, MS TWPs are detected 1.5–2 h before the evening ST appearance at the point of observations, but at the moment of the evening ST passage in the magneto-conjugate point. The obtained results are the first experimental evidence for the hypothesis of the ST-generated ion sound waves.     

Estimated errors in a global gravity wave climatology from GPS radio occultation temperature profiles

In a previous paper by Schmidt et al. (2008), from CHAllenging Minisatellite Payload (CHAMP) Global Positioning System (GPS) radio occultation data, a comparison was made between a Gaussian filter applied to the “complete” temperature profile and to its “separate” tropospheric and stratospheric height intervals, for gravity wave analyses. It was found that the separate filtering method considerably reduces a wave activity artificial enhancement near the tropopause, presumably due to the isolation process of the wave component. We now propose a simple approach to estimate the uncertainty in the calculation of the mean specific wave potential energy content, due exclusively to the filtering process of vertical temperature profiles, independently of the experimental origin of the data. The approach is developed through a statistical simulation, built up from the superposition of synthetic wave perturbations. These are adjusted by a recent gravity wave (GW) climatology and temperature profiles from reanalyses. A systematic overestimation of the mean specific wave potential energy content is detected and its variability with latitude, altitude, season and averaging height interval is highlighted.     

波段探测率D_(△λ)~*替代峰值探测率D_(λp)~*的讨论

文中描述了波段探测率D_(Δλ)~*的定义和计算方法,通过对空间应用的长波红外探测器的波段探测率D_(Δλ)~*与目标辐射源温度T的关系讨论,来说明波段探测率D_(Δλ)~*(和波段响应率)替代峰值探测率D_(Δλ)~*(和峰值响应率)的优越性,文中还给出了波段探测率D_(Δλ)~*的测试方法和实验计算。     

Shock/shock interactions between bodies and wings

This paper examines the Shock/Shock Interactions (SSI) between the body and wing of aircraft in supersonic flows. The body is simplified to a flat wedge and the wing is assumed to be a sharp wing. The theoretical spatial dimension reduction method, which transforms the 3D problem into a 2D one, is used to analyze the SSI between the body and wing. The temperature and pressure behind the Mach stem induced by the wing and body are obtained, and the wave configurations in the corner are determined. Numerical validations are conducted by solving the inviscid Euler equations in 3D with a Non-oscillatory and Non-free-parameters Dissipative (NND) finite difference scheme. Good agreements between the theoretical and numerical results are obtained. Additionally, the effects of the wedge angle and sweep angle on wave configurations and flow field are considered numerically and theoretically. The influences of wedge angle are significant, whereas the effects of sweep angle on wave configurations are negligible. This paper provides useful information for the design and thermal protection of aircraft in supersonic and hypersonic flows.     

卫星姿态控制系统在轨实时健康评估

面向航天器在轨智能自主管控的技术需求,提出一种基于多级模糊综合评价架构的卫星姿态控制系统的在轨实时健康评估方法.根据卫星姿态控制系统的性能特点,按实际功能将其划分为姿态测量、控制器和执行机构3个部分.在确定各部分单元部件健康信息的基础上,基于模糊综合评价算法对各部分的健康度分别进行评估.基于评估所得到的姿态测量、控制器和执行机构3部分健康信息,根据各部分对系统健康的影响情况结合变权综合原理确定健康影响权重,采用模糊综合评价算法实现对姿态控制系统整体健康性能的综合评估.仿真实验结果表明,所提出的方法能够有效实现卫星姿态控制系统的在轨实时健康评估.     

行波管放大器非线性特性对调幅信号边带压缩影响

为了更精确地测试星上功率放大器的饱和点,研究分析了TWTA(Travelling-Wave Tube Amplifier,行波管放大器)的非线性特性对AM(Amplitude Modulation,调幅)信号的边带压缩影响。文中基于Saleh模型描述TWTA,分析其在AM信号放大过程中的非线性特性,研究表明:随着输入AM信号的功率不断增大,放大后的输出信号畸变越来越严重;该变化主要体现在AM信号的边带上,与线性工作区相比,在TWTA的饱和点处,经放大后的AM信号的边带压缩程度达到最大。实验结果与理论分析结果完全一致。该研究为通信卫星星上功放饱和点测试提供了一种可行方法。