基于3DS MAX模型的无人直升机实时监控系统三维建模

分析OpenGL中三维建模的主要方法,结合共轴式无人直升机实时监控飞行系统的设计需要,得出利用3DS MAX的输出模型进行三维建模可以大大提高效率。分析3DS MAX主要输出文件的结构,指出OpenGL建模所需的要素。设计并实现了3DS MAX到OpenGL的模型转换模块,能够分离出3DS MAX场景中的三维模型,为在实时监控系统中再现3DS模型并构造监控飞行系统的三维场景提供灵活性。     

空间互联网应用的三层交换技术探讨及软实现

三层交换技术是运用现有路由技术和交换技术两者的优势,并将其有机地结合,很好地解决了网络路由器的瓶颈问题。文章提出基于Linux操作系统实现纯软件三层交换机,通过Linux网桥实现二层交换,使用开源软件Zebra进行三层路由,并且将二者有机地结合,使其实现＂一次路由,多次交换＂。最后,对软三层交换机的连通性及传输速率进行了实验验证与详细分析。     

Al/Ni含能多层膜在Al2O3陶瓷/不锈钢焊接中的应用

采用磁控溅射设备,生长AuSn合金做焊料层、Al/Ni含能多层膜做热量提供层,实现了不锈钢和Al_2O_3间的异质材料自蔓延高温扩散焊。利用SEM、XRD和DSC等测试手段表征AuSn合金和Al/Ni含能多层膜的微观形貌、相成分和放热量;用万能试验机测试焊接接头的力学性能。结果表明,AuSn合金的质量比基本达到80∶20,而多层膜的层状结构清晰,反应热达到1 239 J/g。焊接实验结果表明,仅使用AuSn焊料时,剪切强度仅为46 MPa,在增加Al/Ni含能多层膜后,其剪切强度可达90 MPa,强度提高了约一倍。焊接接头的界面显微形貌和相结构研究表明,剪切强度的增强主要是Al/Ni多层膜提供了额外能量使得界面处的反应剧烈,陶瓷金属化层与中间层的反应加剧,形成了新的反应生成物。     

三维四向编织复合材料弹性性能的有限元预报

在四步法方型三维编织复合材料细观结构单胞模型的基础上,假设纱线具有六边形横截面,应用ANSYS软件,建立了实体有限元模型,该模型表面与预制件表面平行,更加符合三维编织复合材料的实际结构,且有利于力学性能的分析,同时,该模型中还考虑了织物的编织角与内部编织角的几何关系.基于该模型,计算了材料的弹性常数,分析了编织角和纤维体积含量对弹性常数的影响规律.结果表明,数值计算与实验结果吻合较好.此外,还确定了材料内部的应力场分布,为材料的强度预测奠定了基础.      

A volumetric particle image velocimetry technique based on single color camera with trichromatic mask

A novel single color camera trichromatic mask 3D-PIV technique suitable for measure-ment of complex flow fields in confined spaces is presented in this paper.By using a trichromatic mask to modulate the imaging optical path of a color camera,the RGB(Red,Green,and Blue)channels of the photosensitive chip were used to record full-frame full-resolution images of tracer particles from three viewing angles.The MLOS-SMART particle reconstruction algorithm was used to obtain three-dimensional particle distribution matrix from particle trichromatic mask images.The impact of parameters such as the inter-hole spacing and hole diameter of the trichro-matic mask on the quality of particle reconstruction was analyzed.Through numerical simulation experiments on artificially synthesized three-dimensional flow fields of Gaussian vortex rings,the practicality of this technique in measuring three-dimensional transient velocity fields and the accu-racy of velocity measurements were examined.The accuracy and feasibility of the technique are illustrated based on experimental measurements of a zero-net-mass-flux jet.     

磁响应Fe3O4/HCS复合微球的制备及特性

由壳聚糖与环氧丙烷制备了羟丙基壳聚糖(HCS)。将其配制成水溶液,利用离子凝胶法,与多聚磷酸钠(TPP)反应,制备了粒径在0.6μm羟丙基壳聚糖微球。再用滴定水解法制备了四氧化三铁微粒,激光粒度分析显示滴定水解法制备的Fe3O4粒径分布较窄,粒径小。在此基础上采用交联聚合法制备了Fe3O4/HCS复合微球,微球为实心,四氧化三铁微粒被包裹于微球内部,形状规则,粒径约为0.8μm,经过磁响应分析表明Fe3O4/HCS复合微球具有磁响应性。     

Diurnal and seasonal variations of F2 layer characteristics over Irkutsk during the decrease in solar activity in 2003–2006: Observations and IRI-2001 model predictions

The diurnal and seasonal variations of F2 layer characteristics (critical frequency, peak height and bottomside thickness) over Irkutsk, Russia (52.3 N and 104.3 E) are studied by the method of running medians. The comparison with the IRI-2001 model during the decrease in solar activity in 2003–2006 revealed cases of both close agreement and systematic differences between predictions and observations. The systematic difference is not the only reason for disagreement between IRI and observations; there are also intrayear variations which are not associated with seasonal behavior. The period of observation was too short to make conclusions about solar activity dependence of the noon bottomside thickness and the modification of its diurnal behavior with decreasing solar activity.     

Two years of INTEGRAL result on X-ray binaries

INTEGRAL is the ESA lead International Gamma-Ray Astrophysical Laboratory, successfully launched the 17th October 2002 from Baikonur with a Proton vehicle. In view of the high sensitivity of the two γ-ray instruments IBIS and SPI and their capability to provide at the same time image, spectra and time profiles of all the sources in their wide field of view, a key project was approved as “Core Programme” to obtain deep observations of the Galactic Centre (GCDE) and to exploit regular scan of the whole Galaxy Plane since the beginning of the mission. This paper will briefly review the main astrophysical results obtained in the field of high energy Galactic sources with the INTEGRAL/IBIS γ-ray Imager onboard INTEGRAL, and make a comparison with the previous scenario depicted by the BeppoSAX and RXTE results.