A time-frequency analysis of the thermal radiation background anomalies caused by large earthquakes: A case study of the Wenchuan 8.0 earthquake

Strong earthquakes have an impact on the regional thermal radiation background, which has been both observed and confirmed. This effect produces anomalies in the thermal radiation background (TRBA) and increases the difficulty of extracting a thermal radiation anomaly (TRA) that is associated with an earthquake occurring during the same time period. The extraction and identification of such anomalies has been ignored by previous studies. In this study, we investigate the time-frequency analysis (TFA) method, together with the wavelet filtering of the Daubechies method and the relative power spectrum analysis of the Fourier Welch method to extract and analyse the TRBA caused by the 2008 Wenchuan Ms 8.0 earthquake and the TRA of the 2013 Minxian-Zhangxian Ms 6.6 earthquake using data concerning the brightness temperature of a black body (TBB) from the Fengyun-2 series of geostationary meteorological satellites developed by China. The result showed that this method can effectively extract and analyse the TRBA caused by the Wenchuan earthquake and the TRA of the Minxian-Zhangxian earthquake form a complex background environment. Furthermore, we discussed the impact of the earthquake on the TRBA and segmented the process. The impact is mainly reflected by three aspects; the characteristic period of the TRBA changes, the TRBA occurs at the same time every year, which is identical to the time at which the earthquake anomaly occurred, and the impact process is in stages. We also summarized the correlation between the characteristic parameters of a TRA and the regional thermal radiation background, geography, and climatic factors.     

WSO-UV project

During last three decades, astronomers have enjoyed continuous access to the 100–300 nm ultraviolet (UV) spectral range where the resonance transitions of the most abundant atoms and ions (at temperatures between 3000 and 300 000 K) reside. This UV range is not accessible from ground-based facilities. The successful International Ultraviolet Explorer (IUE) observatory, the Russian ASTRON mission and successor instruments such as the Galaxy Evolution Explorer (GALEX) mission or the COS and STIS spectrographs on-board the Hubble Space Telescope (HST) prove the major impact of observations in the UV wavelength range in modern astronomy. Future access to space-based observatories is expected to be very limited. For the next decade, the post-HST era, the World Space Observatory – Ultraviolet (WSO–UV) will be the only 2-m class UV telescope with capabilities similar to the HST. WSO–UV will be equipped with instruments for imaging and spectroscopy and it will be a facility dedicated, full-time, to UV astronomy. In this article, we briefly outline the current status of the WSO–UV mission and the science management plan.     

陆基无线电授时系统信号分析与解算

时间应用的广泛性以及授时战的提出,使国家更加重视授时服务体系的完备性以及灵活性。为顺应授时战要求,从我国整体授时体系出发,简单介绍授时系统的工作原理,从多方面对比各类授时系统;主要分析了我国陆基无线电授时系统的发播程序以及信号格式等,对BPM短波呼号以及时码结构进行补充与修正,并讲解对陆基无线电授时信号的解算过程,利用实际试验验证解算方法的可行性;最后根据我国目前授时体系的现状以及授时战的要求,给出应对授时战的技术路线,对未来我国授时体系发展方向提出建议。     

飞行器表面红外辐射的模型以及红外特征分析(英文)

隐身最重要的技术之一是评估飞行器被红外探测器接收到的红外辐射强度。本文针对飞行器表面红外辐射特征计算的问题提出一个方法。首先通过分析飞行器表面气动加热、发动机热部件等主要热源,建立了CFD计算模型并获得了飞行表面的温度场。并结合反向蒙特卡洛方法建立求解飞行器表面复杂几何外形的红外辐射模型。通过数值模拟,比较了飞行器主要部件在水平和侧向上红外辐射强度所占的比重;并针对飞行器主要部件冷却对红外辐射强度的影响效果进行了研究。计算结果表明:在水平方向降低飞行器头部、垂尾、机翼部件表面温度10K能降低红外辐射强度大于8%;而在侧方向降低飞行器头部、垂尾、机翼部件表面温度10K能降低红外辐射强度小于8%。计算结果可为隐身设计提供参考。     

再入体实验模型热化学非平衡绕流流场的数值分析

利用数值求解一个和多个振动温度热化学非平衡Navier-Stokes方程的CFD计算程序,对爆轰风洞球锥试验模型的热化学非平衡绕流流场进行了数值模拟,分析了分子组分振动温度在全流场(头身部流场和底部流场)中的分布规律.研究结果表明:(1)计算的压力、电子数密度以及流场的光辐射数据与试验数据符合较好;(2)在再入体身部,大多数分子的振动温度峰值大大高于平动温度的峰值;在再入体近尾出现振动温度冻结并大大高于平动温度的现象;CO2的两个振动态的振动温度分布非常接近平动温度分布.     

软件无线电的可重构流处理器体系结构

 针对软件无线电中存在通用数字信号处理器（DSP）计算能力不足以及专用基带处理器缺乏扩展性的问题,提出了一种新的处理器：面向软件无线电的可重构流处理器及相应的专用指令集。仿真证明,该处理器的可重构设计具备指令集扩展能力,可以对多种无线通信标准甚至是新的通信标准提供支持;面向软件无线电的流体系结构和专用指令集保证了对多种高速无线基带信号的实时处理,运算能力是通用DSP的5~13倍。该处理器为软件无线电中的硬件设计难题提供了一种新的解决途径。     

机载雷达罩热载荷仿真分析关键技术研究

研究了机载雷达罩热载荷仿真分析的3个关键技术,一是雷达罩及天线的CAD建模技术,并应用Fluent计算罩体外表面温度;二是建立雷达罩的多腔体热辐射模型,以得到雷达罩内表面的温度分布;三是温度插值技术,用以将流场计算得到的温度值插值到对应的热应力分析模型上。     

航空发动机燃烧室出口高温热电偶校准技术

在高温校准风洞上,对测量航空发动机燃烧室出口温度气冷式和非气冷式这两种形式的高温热电偶进行校准,确定了高温热电偶的辐射修正系数.校准实验结果表明:高温热电偶的辐射误差随气流速度和压力的增加而降低,而且气流温度与航空发动机机匣壁面温度的温差越大,辐射误差也越大.比较两种结构形式的高温热电偶,非冷却式高温热电偶的测量误差比气冷式高温热电偶的相对较小.      

涡扇发动机轴对称引射收敛喷管红外辐射特性

数值研究了涡扇发动机轴对称引射收敛喷管的红外辐射特性.排气系统的流场计算采用商用数值模拟软件,红外辐射特性计算采用自主开发的软件NUAA-IR,计算分析了轴对称收敛喷管和引射收敛喷管在3~5μm波段红外辐射特性以及喷管内不同固体壁面在探测方向上的红外辐射贡献.结果表明:引射收敛喷管的红外抑制作用主要在于引射加强了尾喷流与环境大气的掺混,减小了尾喷流的长度,降低了燃气流的红外辐射;引射收敛喷管对喷管内固体壁面的遮挡以及降温作用很小,只在方位角为20°方向上对内涵壁面、外涵内壁等中低温壁面有效;引射收敛喷管的总积分辐射强度在方位角为0°~15°范围内与收敛喷管几乎相等,在其他方位角范围内均小于收敛喷管,且在方位角为40°方向上降低幅度达到最大,约为34%.      

球面收敛二元矢量喷管气动及红外特性研究:模拟地面状态

采用数值模拟方法对涡扇发动机排气系统球面收敛二元矢量喷管的气动和红外辐射特性进行了研究,研究仅针对地面状态和俯仰偏转.结果表明:俯仰偏转角在小于20°范围内,俯仰偏转对排气系统推力系数和总压恢复系数的影响微弱,气动推力矢量角与俯仰偏转角几乎相等;由于气体的容积性热辐射特征,喷管俯仰偏转角的变化引起高温喷流红外辐射的方向性变化明显,喷管俯仰偏转时的热喷流在3~5μm波段红外辐射呈现一定幅度的增加;排气系统在3~5μm波段的红外辐射峰值随俯仰偏转角的增加而趋于减小,其出现位置小于俯仰偏转角;在大的俯仰偏转角下,排气系统在垂直探测平面上方的红外辐射较无矢量偏转情形有所降低,但在探测面下方却有明显的增强,导致另一个峰值的出现.