R141b在圆形微通道内的沸腾换热实验研究

为提高换热强度、解决设备内部高热流密度散热问题,采用实验方法研究R141b在不同直径(D=0.5mm和1.0mm)水平圆形微通道内的沸腾换热特性,分析了热流密度(q=2.0kW/m~2～47.6kW/m~2)、质量干度(x=0～0.6)、质量流速(G=111.11kg/(m~2·s)～333.33kg/(m~2·s))的变化对平均传热系数h的影响,探究不同情况下影响沸腾换热的主导因素。实验研究表明:平均传热系数h随热流密度q的增加而减小,在不同范围内减小速率有明显差异;热流密度q=2kW/m~2～5kW/m~2时质量流速G对平均传热系数h影响较明显,热流密度较高时质量流速G对换热影响很小;在质量流速G=111.11kg/(m~2·s)～333.33kg/(m~2·s),质量干度x0.3时,平均传热系数h随质量干度x增加而明显下降,在设计微通道换热器时应尽量使R141b处于初始沸腾阶段以获得更好换热效果,并采取一定措施预防干度过高引起的换热恶化。     

R141b在矩形微尺度通道中的两相流传热特性

设计搭建水力直径分别为1mm和0.5mm的矩形微尺度通道实验台,研究了以R141b型制冷剂作为工质的两相流沸腾传热特性。实验取热流密度为1～16kW/m2、质量流速为111.1～333.3kg/(m2·s)和质量干度为0～1,分析了三者对平均传热系数的影响,探究影响换热的主导因素。结果表明:热流密度较高时,平均传热系数随热流密度增加而减小,流动换热主要受到沸腾传热的影响;当质量流速较大且热流密度较低时,平均传热系数随热流密度增加而有所增长;热流密度较低时,平均传热系数随质量流速变化明显,热流密度升高到一定值后,质量流速对平均传热系数的影响很小;当质量流速处于111.1～333.3kg/(m2·s)时,平均传热系数随质量干度的增加而减小。      

反舰导弹单发命中概率检验方法

结合武器装备试验鉴定工作实际,给出了反舰导弹单发命中概率几种常用检验方法,并给出了不同检验方法的适用条件,使检验方案确定的试验弹数不仅完成单发命中概率的检验,还能完成其他的战技指标的检验,实现导弹武器系统的全面综合评定。     

论WLAN的安全标准及安全机制

无线局域网WLAN是现有的有线局域网的扩展,它使用无线电波来承载数据。利用WLAN进行通讯必须具有较高的通讯保密能力。本文分析了WLAN目前存在的主要安全问题,并根据WLAN的发展动态分别介绍了WLAN网络产品现行采用的IEEE802.11b标准、思科的LEAP协议和PEAP协议的安全技术原理及存在的主要问题,论述了我国提出WAPI新安全机制的工作原理及特点,指出随着技术及应用的发展和进步,WLAN的通讯安全能力会越来越强,而WAPI完全遵循国际标准化,体现了我国标准制定工作的公信力。     

Time-dependent thermal X-ray afterglows from GRBS

Time-dependent thermal X-ray spectra are calculated from physically plausible conditions around GRB. It is shown that account for time-dependent ionization processes strongly affects the observed spectra of hot rarefied plasma. These calculations may provide an alternative explanation to the observed X-ray lines of early GRBs afterglows (such as GRB 011211). Our technique will allow one to obtain independent constraints on the GRB collimation angle and on the clumpiness of circumstellar matter.     

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.     

Two years of INTEGRAL observation of the BHC IGR J17464-3213

On March 2003, IBIS, the γ-ray imager on board the INTEGRAL satellite, detected an outburst from a new source, IGR J17464-3213, that turned out to be an HEAO-1 transient, namely H1743-322. The spectral and temporal evolutions of the source were observed by INTEGRAL in different periods. Also RXTE observed the source for the first time on 2003 March 29 during a PCA Galactic bulge scan. The source flux decayed below the RXTE PCA sensitivity limit in November 2003, then in April 2004 it was again detected by INTEGRAL. On July 3, 2004 the source was again detected by RXTE/PCA at a 2–10 keV intensity of 16 mCrab and on July 7, reached 69 mCrab. Recently, a new outburst was observed on August 2005. We briefly summarise here the behaviour of the source observed by INTEGRAL from March 2003 to August 2005. The new outbursts of the source and the analysis of all the data collected (now public) give a global view of the spectral and time behaviour of this X-ray transient.     

LXI-新一代测试总线技术

LXI是继GPIB、VXI和PXI总线技术之后,基于以太网络的新一代自动测试系统模块化构架平台标准.LXI技术构建在久经证明的工业标准上,融合了GPIB 仪器的高性能、VXI/PXI 卡式仪器的小体积以及LAN 的高速吞吐率, 能够快速、高效率、高性价比的构建测试系统.介绍了LXI技术规范,分析了网络消息触发、IEEE-1588时钟同步触发和触发总线等三种定时与同步技术的原理,重点分析了LXI技术特点及其诸多优点,最后简要阐述了LXI的应用前景.     

机载蒸发循环系统动态仿真

从部件的数学模型出发,根据闭环系统各部件的耦合关系,建立了机载蒸发循环系统的动态数学模型。对充注R142b的机载蒸发循环系统进行了动态仿真,仿真数据与试验数据基本吻合,仿真方法可靠,可以作为机载蒸发循环系统优化及系统控制的依据。