嵌入式大气数据测量系统技术研究进展

针对高超声速飞行器大气数据测量问题,对嵌入式大气数据测量系统(FADS)技术研究背景、发展历程、国内外研究现状等进行了概括。重点围绕FADS关键技术、FADS解算算法及面向FADS/INS组合测量系统信息融合算法方面,对FADS技术进行了深入的剖析。最后,展望了FADS技术未来的发展方向及应用前景。     

垂直喷流与外流干扰的计算方法

将实验数据库方法应用于侧喷与主流干扰的绕流单独体的复杂流动，得到了相似参数Q，即一比与干扰因子Kn、Km和Q之积的线性关系。应用该线性关系，成功地相关了关于Kn、Km和Q的实验数据，并使用这一关系式，很容易计算出干扰气动力和压力中心，计算结果表明，该 具有纠正实验偏差的能力，并提出了获得可靠实验结果的建议。     

未来智能化网络化多功能卫星系统技术发展思考

我国卫星领域经过几十年的发展,现在正面临技术创新突破的关键时期。以美国“星链”为代表的大规模星座系统的出现,展现了互联网+航天时代的前景雏形。同时,人工智能技术迅猛发展,神经网络、机器学习和大数据挖掘等成果转化应用,可大幅提升卫星自主运行、星上数据处理以及多任务适应能力。本文通过对近年来国外典型卫星系统发展进行深入解剖,从未来卫星网络化、智能化和多功能特点分析技术发展布局、应用模式创新和研产模式转型等影响,提出适应上述改变的举措建议,为我国卫星技术创新发展提供有益参考。     

Determination of the solar rotation parameters via orthogonal polynomials

Accurate measurements of the solar differential rotation parameters are necessary for understanding the solar dynamo mechanism. We use the orthogonalization process to estimate these parameters. The advantage of the orthogonalization of the data in the tracer motion statistical analysis is outlined. The differential rotation is represented in terms of various types of polynomials. We compare the quality of a set of models of the solar differential rotation using the Akaike information criterion and choose the best one. Applying the proposed method, we studied the solar differential rotation and its North-South asymmetry using observations of coronal holes. A statistical analysis of observations from the Atmospheric Imaging Assembly (AIA) on Solar Dynamics Observatory (SDO) reveals the differential rotation pattern of coronal holes and its North-South asymmetry.     

The impact of different background errors in the assimilation of satellite radiances and in-situ observational data using WRFDA for three rainfall events over Iran

Satellite radiances and in-situ observations are assimilated through Weather Research and Forecasting Data Assimilation (WRFDA) system into Advanced Research WRF (ARW) model over Iran and its neighboring area. Domain specific background error based on x and y components of wind speed (UV) control variables is calculated for WRFDA system and some sensitivity experiments are carried out to compare the impact of global background error and the domain specific background errors, both on the precipitation and 2-m temperature forecasts over Iran. Three precipitation events that occurred over the country during January, September and October 2014 are simulated in three different experiments and the results for precipitation and 2-m temperature are verified against the verifying surface observations. Results show that using domain specific background error improves 2-m temperature and 24-h accumulated precipitation forecasts consistently, while global background error may even degrade the forecasts compared to the experiments without data assimilation. The improvement in 2-m temperature is more evident during the first forecast hours and decreases significantly as the forecast length increases.     

Background-sensitive event selection in the search for gamma-ray sources

Poor angular resolution of present day gamma ray telescopes (1° at 100 MEV) together with the complicated gamma ray sky structures at compareable angular extents and poor statistics available necessitate the selection of those gammas which will increase the observable signal from a suspected source. A method for such a selection using the pre-known time signature of the source as its signal, has been developed (Özel and Mayer-Haβelwander, 1983). In an iterative procedure based on the improvement of source signal, generalized zones around the source are defined, from which gamma rays should be accepted to construct the optimum light curve of the source. These zones depend on the energy of the probed gamma rays, on the spatial structure and intensity of the background around the source, on the (estimated and/or tentative) intetnsity of the source and finally on the observing instrument's angular and energy response functions. The method, when applied to simulated and observed COS-B data demonstrated its feasibility and merits over the previonsly used circular event-acceptance cones method which was the basis of searches for gamma ray emission from radio pulsars (see for example Kniffen et al., 1974; Ögelman, et al. 1976; Kanbach, et al., 1977; and references therein). Present method does not introduce “trials” which usually reduce the significance of the results obtained, fully accounts the available knowledge on the topography of gamma ray sky, makes use of all the information about the sky, source and the instrument and therefore is the proper way of handling gamma ray data in pulsar-type searches.Presently, method is applied in the analyses of COS-B data in the context of searches for gamma ray emitting X-ray and radio pulsars. Results will be published elsewhere.     

CBERS-1卫星IRMSS数据及融合技术在鸭绿江口示范应用评价

文章通过丹东鸭绿江口与大连地区典型研究中采用的 CBERS-1卫星IRMSS数据,对数据图像的质量、图像信息的处理方法和专业应用潜力进行评价。通过评价IRMSS不同波段数据的应用效果,加速IRMSS数据的推广应用。     

φ50毫米微波测速系统

本文叙述了在50毫米二级轻气炮发射管内采用的微波反射技术:当模型运动的时候,将射入炮管内的微波和从模型上反射的微波间的相位变化记录下来,便可以获得炮管中模型运动速度的连续测量。     

冲裁模CAD系统的标准件建库技术及其界面设计

在开发模具ＣＡＤ系统时使用三维实体建立标准件图形库，采用Ｃ－ＡＰＩ编写编图程序，将国标尺寸数据集成于其中，编制ＤＣＬ对话框控制程序，产生方便，友好，美观的人机界面，一次性实现数据输入，检索和自动绘图，进一步提高设计效率。     

二维物体相交检验的线性四叉树方法

在物体的平面布局问题中，判别两个物体是否相交是一个难点，以往的方法数据结构不统一，计算量大，算法复杂，本文首先讨论了二值图象的线性四叉树的表示及其有关术语和性质，然后在此基础上首次提出了二维物体相交检验的线性四叉树方法及其实现的算法，最后进行了算法的时空分析，与以往的方法相经，本文所提方法具有数据结构统一，算法简单，时空效率高等优点。