毫米波雷达的挑战及电子战的应用

当今雷达技术已进入了利用毫米波电磁频谱特性阶段。EW的ESM和ECM也随之发展起来,如同当年EW那样,很快地赶上了VHF,UHF和微波领域雷达技术的发展。很久以来,雷达一直在使用毫米波的低段,最近才扩展到中段。在雷达上应用,毫米波频段要优于微波和光电频段。当然与后两个频段相比,毫米波也存在不足之处。在性能,技术和应用上,毫米波雷达与微波雷达相比较,具有以下特征。     

FY-2D Successfully Launched

China launched its fourth geostationary orbit meteorological satellite FY-2D on December 8, 2006 by a LM-3A launch vehicle from Xichang Satellite Launch Center. The satellite was sent into the preset geostationary transfer orbit 24 minutes after ignition and successfully positioned at 86.5" E above the equator on December 13.     

CASC Products On The Airshow China 2006

CASC brought 110 products to the Airshow China 2006, which was the showcase of the achievements of CASC in the past two years covering civil space, manned spaceflight, lunar exploration and deep space exploration. Over 70 products were open to the public for the first time. New products on display at the airshow included MS-1 micro-satellite, small launch vehicle and Kuafu Program and space solar telescope.     

现代表面分析——俄歇电子谱(AES)和X-射线光电子谱(XPS)在冶金学中的应用 第一讲 AES和XPS技术的基础

现代表面分析技术已广泛应用于当代科学的各个领域中。应用俄歇电子谱学(AES)与X-射线光电子谱学(XPS或ESCA)研究自由表面或内界面的化学成分分布及化合物的化学结合状态,对于分析金属材料、复合材料以及粘接、镀层、腐蚀等领域有关结合强度、断裂机理、缺陷成因等问题有重要意义。对于电子元器件失效分析,这些技术尤为重要。 从本期开始,我们将组织稿件介绍有关这些先进分析技术的基础理论和在材料工艺研究中的应用情况。     

利用卫星实现与飞行中巡航导弹的通信

本文讨论了与飞行中远程巡航导弹通信的需求以及卫星作为中继平台的潜力。国防卫星通信系统Ⅲ(DSCSⅢ)和舰队卫星通信(FLTSATCOM)星至少能够同时为70枚巡航导弹向水面舰只和陆基指挥中心传送200bit的状态信息。DSCSⅢ还可以同时为至少70枚巡航导弹提供准实时有人末制导支持(只要巡航导弹装有共形天线阵)。FLTSATCOM可以为2枚装有全向天线阵的巡航导弹提供相同的能力。这种能力包括传输末段敏感器图象数据,该图象数据的速率为每枚每秒40kbits,取决于可实现的图象数据压缩比。本文还论述了指挥员利用这些系统重新瞄准新目标,允许一枚巡航导弹向地面传送一路末段敏感器图象。     

Combustion modeling in a model combustor

The flow-field of a propane-air diffusion flame combustor with interior and exterior conjugate heat transfers was numerically studied.Results obtained from four combustion models,combined with the re-normalization group(RNG) k-ε turbulence model,discrete ordinates radiation model and enhanced wall treatment are presented and discussed.The results are compared with a comprehensive database obtained from a series of experimental measurements.The flow patterns and the recirculation zone length in the combustion chamber are accurately predicted,and the mean axial velocities are in fairly good agreement with the experimental data,particularly at downstream sections for all four combustion models.The mean temperature profiles are captured fairly well by the eddy dissipation(EDS),probability density function(PDF),and laminar flamelet combustion models.However,the EDS-finite-rate combustion model fails to provide an acceptable temperature field.In general,the flamelet model illustrates little superiority over the PDF model,and to some extent the PDF model shows better performance than the EDS model.      

Recent SETI observations at Arecibo

During 1980 and 1981, the 305-m radio telescope at the Arecibo Observatory in Puerto Rico was used to conduct a high resolution search for narrowband signals from the direction of 210 nearby solar type stars and 5 OH masers. For each star at least 4 MHz of bandwidth surrounding the 21-cm HI line and/or the 18-cm OH lines was studied with a spectral resolution of 5.5 Hz in both right and left circular polarization. The formal limit of sensitivity achieved during the course of this search varied depending upon the particular receivers available. In all cases the search could have detected a narrowband transmitter of power comparable to the Arecibo planetary radar, had any such been transmitting on the frequencies searched during the time of observation out to the distance of the farthest target star. As in previous searches, the number of "false alarms" encountered was far greater than predicted on the basis of Gaussian noise statistics. A small number of stars have exhibited signals which cannot immediately be explained in terms of astrophysical or man-made sources and deserve reobservation. This is typical of the results of previous non-real-time searches and does not yet constitute the detection of an ETI.