WSO-UV project

During last three decades, astronomers have enjoyed continuous access to the 100–300 nm ultraviolet (UV) spectral range where the resonance transitions of the most abundant atoms and ions (at temperatures between 3000 and 300 000 K) reside. This UV range is not accessible from ground-based facilities. The successful International Ultraviolet Explorer (IUE) observatory, the Russian ASTRON mission and successor instruments such as the Galaxy Evolution Explorer (GALEX) mission or the COS and STIS spectrographs on-board the Hubble Space Telescope (HST) prove the major impact of observations in the UV wavelength range in modern astronomy. Future access to space-based observatories is expected to be very limited. For the next decade, the post-HST era, the World Space Observatory – Ultraviolet (WSO–UV) will be the only 2-m class UV telescope with capabilities similar to the HST. WSO–UV will be equipped with instruments for imaging and spectroscopy and it will be a facility dedicated, full-time, to UV astronomy. In this article, we briefly outline the current status of the WSO–UV mission and the science management plan.     

进离港分离下的进近管制员工作负荷统计模型

主要研究了在进离港航线分离同时不考虑跑道影响条件下,提出了进离港分开考虑统计进近管制员工作负荷,在此基础上建立了进近管制员工作负荷统计模型。最后结合上海进近扇区2对模型进行了检验,验证了模型的准确性和可靠性。     

密集编队中飞机发动机的疲劳损伤差异

选取典型密集编队飞行任务,利用实测飞行数据,研究了在飞行动作几乎完全相同的条件下飞机发动机疲劳损伤的差异.经过二次雨流法统计循环次数和线性累积损伤理论折合到标准循环,得出了密集编队中长、僚机因位置不同而造成的发动机疲劳损伤的差异及其统计规律,发现疲劳损伤差异分布为威布尔分布,单机差异一般为2～4倍,最大可以达到9～10倍.进一步揭示了发动机疲劳载荷/损伤的分散性和单机疲劳寿命监控的必要性.      

2A12-T4铝合金长期大气腐蚀损伤规律

在海南省万宁地区开展了2A12-T4铝合金暴露7年、12年和20年的大气腐蚀试验,根据腐蚀特征将腐蚀区域划分为单侧腐蚀区和双侧腐蚀区,以结构最小剩余厚度值作为腐蚀特征量,进行了不同年限试验件中不同腐蚀区域最小剩余厚度的测量和统计分析,确定了满足99.9%可靠度与95%置信度的最小剩余厚度值以及95%置信度下的最小剩余厚度置信区间,并开展了腐蚀损伤形貌的金相分析。研究结果表明:2A12-T4铝合金大气腐蚀特征量服从正态分布;在大气腐蚀7~20年间2A12-T4铝合金板件的最小剩余厚度值是线性减小的;2A12-T4铝合金大气腐蚀7年后处于点蚀、晶间腐蚀、剥蚀的过渡期,12年后发生全面剥蚀,20年后剥蚀已相当严重且伴随着点蚀;双侧腐蚀区与单侧腐蚀区相比腐蚀深度更大且剥蚀层剥落严重。     

某航机燃烧室煤油改柴油燃烧特性研究

为了给某型航空发动机改为地面用柴油型燃气轮机的设计提供重要的技术支持,本文借助数值计算的方法,采用FLUENT稳态压力求解器、P1辐射模型和涡耗散破碎(EDU)燃烧模型对某航空发动机燃烧室在巡航工况和最大工况下煤油与柴油两种燃料的燃烧特性进行了计算及对比研究。得到了该燃烧室使用航空煤油(RP-3)和0号柴油的热态流场、空气流量分配、温度场、出口温度分布、污染物排放及头部燃油蒸发量。研究结果表明：当该燃烧室的燃料由航空煤油改为0号柴油后,燃烧室的热态温度场分布基本一致,流量分配最大差异在0.45%之内;燃烧效率降低约4.3%和NO、Soot排放量相当;出口温度分布和总压损失差异分别在1%和4.1%之内。     

Orbital phase spectroscopy of four high mass X-ray binary pulsars to study the stellar wind of the companion

Our work focuses on a comprehensive orbital phase-dependent spectroscopy of the four High Mass X-ray Binary Pulsars (HMXBPs) 4U 1538-52, GX 301-2, OAO 1657-415 and Vela X-1. We hereby report the measurements of the variation of the absorption column density and iron-line flux along with other spectral parameters over the binary orbit for the above-mentioned HMXBPs in elliptical orbits, as observed with the Rossi X-ray Timing Explorer (RXTE) and the BeppoSAX satellites. A spherically symmetric wind profile was used as a model to compare the observed column density variations. Out of the four pulsars, only in 4U 1538-52, we find the model having a reasonable corroboration with the observations, whereas in the remaining three the stellar wind seems to be clumpy and a smooth symmetric stellar wind model appears to be quite inadequate in explaining the data. Moreover, in GX 301-2, neither the presence of a disk nor a gas stream from the companion was validated. Furthermore, the spectral results obtained in the case of OAO 1657-415 and Vela X-1 were more or less similar to that of GX 301-2.     

焊后热处理对高温运行10CrMo910钢管接头持久寿命的影响

本文通过１０ＣｒＭｏ９１０钢大口径厚壁管道高温模拟试验证实，焊后热处理是一个短时超高温运行过程，它使１０ＣｒＭｏ９１０钢管接头组织提前老化，显著降低了接头的持久寿命。试验结果表明，传统的焊后热处理工序应当取消。     

基于运动形态学的掠地飞行器视频检测方法

 结合数学形态学、视频图像运动分析以及数学统计分析方法,提出了一种用于空中预警控制系统(AWACS)的小型掠地飞行器运动形态学视频检测方法。该方法首先应用形态学tophat滤波提取出视频图像中的可疑目标(SO),并求取SO的运动参数,利用真实目标和类目标干扰的不同运动特性,应用数学统计的方法对各运动参数进行分析以剔除部分类目标干扰,从而获得潜在目标(PT)的灰度分布和运动参数。在应用形态学tophat滤波器进行可疑目标提取中,一种新的金字塔型结构元的引入有效减少了虚警数量。外场试验表明,该检测方法能够有效抑制航拍掠地飞行器视频图像中的地物干扰,降低虚警目标的数量。     

The Crab pulsar seen with AquEYE at Asiago Cima Ekar observatory

We are developing fast photon-counter instruments to study the rapid variability of astrophysical sources by time tagging photon arrival times with unprecedented accuracy, making use of a Rubidium clock and GPS receiver. The first realization of such optical photon-counters, dubbed AquEYE (the Asiago Quantum Eye), was mounted in 2008 at the 182 cm Copernicus Observatory in Asiago. AquEYE observed the Crab pulsar several times and collected data of extraordinary quality that allowed us to perform accurate optical timing of the Crab pulsar and to study the pulse shape stability on a timescale from days to years with an excellent definition. Our results reinforce the evidence for decadal stability of the inclination angle between the spin and magnetic axis of the Crab pulsar. Future realizations of our instrument will make use of the Galileo Global Navigation Satellite System (GNSS) time signal.