大功率UVLED分布式驱动技术研究

以工业印刷过程中UVLED固化为应用背景,研究并设计了一种UVLED驱动控制系统。分析了采用分布式驱动的优势,确定了驱动电源采用两级驱动结构,包括前端AC/DC恒压模块和后端DC/DC恒流模块。对该系统的驱动电源模块进行了试验测试和结果分析,试验结果验证了该UVLED驱动控制系统的可行性。     

Assessment on critical technologies for conceptual design of blended-wing-body civil aircraft

Civil aviation faces great challenges because of its robust projected future growth and potential adverse environmental effects. The classical Tube-And-Wing(TAW) configuration following the Cayley's design principles has been optimized to the architecture's limit, which can hardly satisfy the further requirements on green aviation. By past decades' investigations the BlendedWing-Body(BWB) concept has emerged as a potential solution, which can simultaneously fulfill metrics of noise, emission and fuel burn. The purpose of the present work is to analyze the developments of critical technologies for BWB conceptual design from a historical perspective of technology progress. It was found that the high aerodynamic efficiency of BWB aircraft can be well scaled by the mean aerodynamic chord and wetted aspect ratio, and should be realized with the trade-offs among stability and control and low-speed performance. The structure concepts of non-cylinder pressurized cabin are of high risks on weight prediction and weight penalty. A static stability criterion is recommended and further clear and adequate criteria are required by the evaluations of flying and handling qualities. The difficulties of propulsion and airframe integration are analyzed. The energy to revenue work ratios of well-developed BWB configurations are compared,which are 31.5% and 40% better than that of TAW, using state-of-art engine technology and future engine technology, respectively. Finally, further study aspects are advocated.     

屋面现浇板裂缝的防治

从设计、施工、材料、气候等多方面分析现浇板裂缝产生的原因,并总结一些防治措施。     

面内强磁场下铁磁板壳的自由振动

本文研究了面内强磁场环境下铁磁板壳的自由振动问题。基于Eringen-Maugin的关于磁弹性作用的理性力学模型,从理论上推导了一般壳体在磁场中的运动方程,进而求解了面内强磁场作用下的小磁化率悬臂铁磁薄板自由振动频率。数值计算结果表明,本文模型和已有的实验结果吻合很好。     

梁纵向与横向耦合非线性振动分析

纵向振动和横向振动耦合是捆绑火箭等结构中的典型振动现象.以Rayleigh梁为研究对象,通过Hamilton变分原理推导了考虑应变二次项的纵向振动与横向振动耦合控制方程,并用有限元方法对该非线性系统的行为进行了模拟.针对线性系统固有振动频率和非线性纵横耦合动态响应情况,把所得结果与NASTRAN结果进行了比较,二者结果吻合,证明了本方法的正确性.在此基础上,借助振动控制方程和模拟结果,讨论了非线性系统频率与模态的时变特性,非线性动态响应频率成分特性,横向振动和纵向振动相互影响以及共振现象等.研究结果为本方法的实际应用提供了理论基础.      

航空电子设备NSEE试验评价方法

本文定义了航空电子设备大气中子单粒子效应(NSEE)硬失效、硬错误与软错误等大气中子辐射可靠性表征参数,提出了一套航空电子设备抗大气中子单粒子效应危害能力的试验评价方法,包括试验应力终止条件与起始条件的确定方法、M_NSEE预估方法、试验程序、试验评价方法等,并通过某航空用卫星导航接收机试验案例证明了该方法在工程应用中的可操作性与有效性,通过掌握数字信号处理(DSP)、静态随机存储器(SRAM)、现场可编程门阵列(FPGA)的NSEE敏感特性,可为航空用卫星导航接收机NSEE危害防控提供针对性的技术支持.本文为我国航空电子产品大气中子单粒子效应试验评价奠定了理论与应用基础,同时也为其他电子信息产品在大气中子单粒子效应试验评价方面提供了重要依据和参考.      

北斗/GNSS高精度时频终端测试方法探讨

基于虚拟仪器技术、网络技术和批量化测量技术,探讨北斗/GNSS高精度时频应用终端的测试手段;提出应用测试模块化和VXI/PXI/LXI总线技术的测试设计方案,该方案具有多路标准时间频率参考信号一致性设计和网络远程测试校准设计;同时,提出北斗/GNSS高精度时频终端测试校准系统的结构设计及其应用模式。这将能有效提高北斗/GNSS时频终端测试的集成化和智能化水平。     

Universal scaling laws for fully-developed magnetic field turbulence near and far upstream of the Earth’s bow shock

We analyze the multifractal scaling of the modulus of the interplanetary magnetic field near and far upstream of the Earth’s bow shock, measured by Cluster and ACE, respectively, from 1 to 3 February 2002. The maximum order of the structure function is carefully estimated for each time series using two different techniques, to ensure the validity of our high-order statistics. The first technique consists of plotting the integrand of the pth order structure function, and the second technique is a quantitative method which relies on the power-law scaling of the extreme events. We compare the scaling exponents computed from the structure functions of magnetic field differences with the predictions obtained by the She–Lévêque model of intermittency in anisotropic magnetohydrodynamic turbulence. Our results show a good agreement between the model and the observations near and far upstream of the Earth’s bow shock, rendering support for the modelling of universal scaling laws based on the Kolmogorov phenomenology in the presence of sheet-like dissipative structures.     

Numerical modeling of inhomogeneous orographic wave influence on planetary waves in the middle atmosphere

Parameterization of dynamical and thermal effects of stationary orographic gravity waves (OGWs) generated by the Earth’s surface topography is incorporated into a numerical model of general circulation of the middle and upper atmosphere. Responses of atmospheric general circulation and characteristics of planetary waves at altitudes from the troposphere up to the thermosphere to the effects of OGWs propagating from the earth surface are studied. Changes in atmospheric circulation and amplitudes of planetary waves due to variations of OGW generation and propagation in different seasons are considered. It is shown that during solstices the main OGW dynamical and heat effects occur in the middle atmosphere of winter hemispheres, where changes in planetary wave amplitudes due to OGWs may reach up to 50%. During equinoxes OGW effects are distributed more homogeneously between northern and southern hemispheres.     

A survey of radio jets with Chandra and HST

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.