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101.
中国空气动力研究与发展中心研制了可更换喷嘴的中压气体引射器 ,利用现有中压气源驱动 ,建成一座增压回流引射式跨声速风洞。试验段截面尺寸 2 .4m×2 .4m ,M =0 .3~ 1 .2。稳定段最高工作压力为 0 .45MPa ,最高模型试验雷诺数Rec=1 5× 1 0 6(M =0 .90 ,C =0 .2 4m) ,稳定吹风时间≥ 1 5s。风洞气动回路上分别配置有多喷管引射器、栅指扩散段、跨声速试验段驻室抽气系统及特殊的主排气系统等装置。采用智能自适应解耦控制技术 ,实现总压和M数独立、快速、精确地控制。该气动布局与部段配置及其功能设计 ,在国内跨声速风洞中均是首次采用。 相似文献
102.
本文研究了阻尼介质对刚塑性圆板在高载(冲击荷载)作用下塑性动力响应的影响,得到了解析解并对此解进行了讨论。当阻尼介质参数趋于零时,本文结果与无阻尼解一致。文中还画出了荷载与阻尼介质对圆板运动时间和板中心点残余挠度的影响曲线。 相似文献
103.
针对利用GPS进行定时校频技术开展了一系列的应用基础研究,包括GPS定时校频的方法及其不确定度、定时校频数据的处理等。在给出实验结果的同时,对影响GPS定时精度的各种因素(包括SA影响)进行了讨论;同时对提高GPS定时精度的途径作了初步探讨。 相似文献
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Rita M. Sambruna 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2004,34(12):2571-2578
Relativistic jets are a common property of radio-loud Active Galactic Nuclei (AGN). Understanding jet physical properties is an essential precursor to understanding the mechanisms of energy transport, and ultimately, how energy is extracted from the central black hole. In this paper, I highlight recent developments from Chandra and HST observations of kpc-scale jets in AGN, with particular emphasis on our survey of 17 radio jets in a sample of FRII radio galaxies. These observations show that (1) X-ray and optical emission is common from kpc-scale jets, (2) a large fraction of the bolometric luminosity is emitted at X-rays, and (3) in most sources, a candidate emission process for the X-rays is inverse Compton scattering of the Cosmic Microwave Background off the relativistic electrons in the jet. If the latter scenario holds, the implication is that jets are still relativistic on kpc scales. 相似文献
106.
The rising demand for Unmanned Aerial Systems(UASs) to perform tasks in hostile environments has emphasized the need for their simulation models for the preliminary evaluations of their missions. The efficiency of the UAS model is directly related to its capacity to estimate its flight dynamics with minimum computational resources. The literature describes several techniques to estimate accurate aircraft flight dynamics. Most of them are based on system identification. This paper presents an alternative methodology to obtain complete model of the S4 and S45 unmanned aerial systems. The UAS-S4 and the UAS-S45 models were divided into four sub-models, each corresponding to a specific discipline: aerodynamics, propulsion, mass and inertia, and actuator. The‘‘aerodynamic" sub-model was built using the Fderivatives in-house code, which is an improvement of the classical DATCOM procedure. The ‘‘propulsion" sub-model was obtained by coupling a two-stroke engine model based on the ideal Otto cycle and a Blade Element Theory(BET) analysis of the propeller. The ‘‘mass and the inertia" sub-model was designed utilizing the Raymer and DATCOM methodologies. A sub-model of an actuator using servomotor characteristics was employed to complete the model. The total model was then checked by validation of each submodel with numerical and experimental data. The results indicate that the obtained model was accurate and could be used to design a flight simulator. 相似文献
107.
航空测距器DME的开发、调试和性能验证都要用到高斯双脉冲调制格式的DME信号。由于专用的DME信号模拟器技术复杂、价格昂贵,人们常用具有快沿双脉冲调制功能的模拟信号源替代。本文以航空测距器DME信号要求为依据,初步分析了这种替代可能存在的问题,并通过实验对不同边沿条件下高斯双脉冲、矩形双脉冲调制信号的功率频谱占用情况进行了验证。 相似文献
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109.
Paul O’Brien 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2011
The ASTROSAT satellite is an Indian National Space Observatory under development in India. Due for launch in 2010, ASTROSAT will carry a complement of five scientific instruments enabling simultaneous observations from the optical through to the hard X-ray energy band. This capability will enable broad-band spectroscopy and high time-resolution monitoring of both galactic and extra-galactic targets, such as X-ray binaries and AGN. One of the instruments is being built in collaboration with the Canadian Space Agency and another in collaboration with the University of Leicester. ASTROSAT also carries a scanning sky monitor to observe the variable X-ray sky. After an initial period of science verification and guaranteed time, a certain fraction of ASTROSAT observing time will also be made available to the community via a call for proposals. Here I summarise the instrument complement and principle scientific objectives of the mission. 相似文献
110.