金属基高功率CO2激光沉积超硬Si3N4膜层性能研究

本文采用高功率ＣＯ２激光在金属基材汽相沉积出厚度－３０μｍ标准化学计量配比、平均硬度达２２００ＨＫ的ａ－Ｓｉ３Ｎ４膜层，与基材有良好的结合界面，实验分析表明所沉积膜具有超硬和良好的耐磨抗蚀等性能。     

卫星舱内两类剂量计测量结果的比较

本文利用1994年和1996年两次返回式卫星的搭载条件对舱内辐射剂量进行了对比测量．通过对比测量,研究不同掺杂、不同厚度LiF剂量计测量空间辐射剂量的特点;研究GM计数管计数和LiF剂量间的转换系数以及转换系数随屏蔽状况的变化;由剂量和GM计数研究粒子平均碰撞阻止本领的估计方法．结果表明,不同掺杂、不同厚度的LiF剂量计测量结果间无显著差异,而转换系数几乎不受舱内位置和屏蔽状态的影响．不同厚度LiF剂量计,不同屏蔽状态的GM计数管计数和剂量—计数转换系数的比较研究以及对粒子平均碰撞阻止本领的估计表明,舱内辐射剂量起决定作用的是高能粒子成分,其平均碰撞阻止本领估计约为5MeV／cm．     

Is "the right stuff" the right stuff?

In 1979 the author Tom Wolfe likened US astronauts to sacrificial gladiators characterized by competitiveness, independence, self-sufficiency, extroversion and a sense of moral righteousness and superiority--in short, 'the right stuff'. But are these the qualities needed for long-duration international missions? The author's hunch is that they are on the whole still necessary but not sufficient, but he emphasizes that systematic study of past behavioural reactions and analogous environments is needed if vital questions of interpersonal dynamics are to be answered correctly.     

A high-resolution Ge spectrometer for Gamma-Ray burst astronomy

The Transient Gamma-Ray Spectrometer (TGRS) to be flown aboard the WIND spacecraft is primarily designed to perform high resolution spectroscopy of transient -ray events, such as cosmic -ray bursts and solar flares over the energy range 25 keV to 8.2 MeV with an expected spectroscopic resolution of 3 keV at 1 MeV. The detector itself consists of a 215 cm³ high purityn-type Ge crystal kept at cryogenic temperatures by a passive radiative cooler. The geometric field of view defined by the cooler is 1.8 steradian. To avoid continuous triggers by soft solar events, a thin BeCu Sun-shield around the sides of the cooler has been provided. A passive Mo/Pb occulter, which modulates signals from within ±5° of the ecliptic plane at the spacecraft spin frequency, is used to identify and study solar flares, as well as emission from the galactic plane and center. Thus, in addition to transient event measurements, the instrument will allow the search for possible diffuse background lines and monitor the 511 keV positron annihilation radiation from the galactic center. In order to handle the typically large burst count rates, which can be in excess of 100 kHz, burst data are stored directly in an onboard 2.75 Mbit burst memory with an absolute timing accuracy of ±1.5 ms after ground processing. The memory is capable of storing the entire spectral data set of all but the largest bursts. WIND is scheduled to be launched on a Delta II launch vehicle from Cape Canaveral on November 1, 1994. After injection into a phasing orbit, the spacecraft will execute a double lunar swing-by before being moved into a controlled halo orbit about theL1 Lagrangian point (250R _e towards the Sun). This will provide a 5 light-second light travel time with which to triangulate gamma-ray burst sources with Earth-orbiting systems, such as those on-board the Gamma-Ray Observatory (GRO). The response of instrument to transient -ray events such as GRB's and solar flares will be presented as well as the expected response to steady state point sources and galactic center line emission.     

Lessons learned from the York University Rover Team (YURT) at the University Rover Challenge 2008–2009

In this paper, we explore the lessons learned from the work of the York University Rover Team (YURT), which designed, built, and operated two prototype rovers for the University Rover Challenge (URC) in 2008 and 2009, placing third in the first year, and winning first place in the second year. We outline the competition, the team, and briefly describe the York University space engineering program. Both of the rovers are described with evaluations of each major component and the resulting design changes. A general trend toward design modularity, purpose-driven customizations, and better critical thinking in the design process is evident as the team gains experience. Also, the value of this project as an educational medium is evaluated with respect to traditional classroom learning. Participating students from a wide range of disciplines gained real-world experience in both “hard” engineering skills such as mechanical and electronic design, fabrication, and testing, and “soft” skills such as project management, system-level thinking, creative problem solving, and interpersonal skills. Lessons learned from this include the necessity of good financial management, the importance of marketing and outreach, the use of short and simple development steps, and the need for comprehensive contingency planning. We conclude that the URC provided an inter-disciplinary, cooperative educational environment, and that student engineering projects such as this can provide “soft” skills through experiential education that are normally difficult to teach in the classroom.