Far-UVC light as a new tool to reduce microbial burden during spacecraft assembly

This work aims to investigate far-UVC light at 222 nm as a new microbial reduction tool for planetary protection purposes which could potentially be integrated into the spacecraft assembly process. The major advantage of far-UVC (222 nm) compared to traditional germicidal UVC (254 nm) is the potential for application throughout the spacecraft assembly process in the presence of humans without adverse health effects due to the limited penetration of far-UVC light into biological materials. Testing the efficacy of 222-nm light at inactivating hardy bacterial cells and spores isolated from spacecraft and associated surfaces is a necessary step to evaluate this technology. We assessed survival of Bacillus pumilus SAFR-032 and Acinetobacter radioresistens 50v1 exposed to 222-nm light on proxy spacecraft surfaces simulated by drying the bacteria on aluminum coupons. The survival fraction of both bacteria followed a single stage decay function up to 60 mJ/cm², revealing similar susceptibility of both species to 222-nm light, which was independent of the exposure rate. Irradiation with far-UVC light at 222 nm is an effective method to decontaminate the proxy spacecraft materials tested in this study.     

滑油量对恒速传动装置的影响

本文介绍了中外航空公司飞机发动机恒速传动装置几个故障典例及造成的危害,分析了填加滑油量不当对发动机恒速传动装置的影响,提出了预防措施。     

Late Stages of Stellar Evolution

A large fraction of ISO observing time was used to study the late stages of stellar evolution. Many molecular and solid state features, including crystalline silicates and the rotational lines of water vapour, were detected for the first time in the spectra of (post-)Asymptotic Giant Branch (AGB) stars. Their analysis has greatly improved our knowledge of stellar atmospheres and circumstellar environments. A surprising number of objects, particularly young planetary nebulae with Wolf-Rayet (WR) central stars, were found to exhibit emission features in their ISO spectra that are characteristic of both oxygen-rich and carbon-rich dust species, while far-IR observations of the PDR around NGC 7027 led to the first detections of the rotational line spectra of CH and CH⁺. Based on observations with ISO, an ESA project with instruments funded by ESA Member States (especially the PI countries: France, Germany, The Netherlands, and the United Kingdom), and with the participation of ISAS and NASA.     

Emergence of a Habitable Planet

We address the first several hundred million years of Earth’s history. The Moon-forming impact left Earth enveloped in a hot silicate atmosphere that cooled and condensed over ∼1,000 yrs. As it cooled the Earth degassed its volatiles into the atmosphere. It took another ∼2 Myrs for the magma ocean to freeze at the surface. The cooling rate was determined by atmospheric thermal blanketing. Tidal heating by the new Moon was a major energy source to the magma ocean. After the mantle solidified geothermal heat became climatologically insignificant, which allowed the steam atmosphere to condense, and left behind a ∼100 bar, ∼500 K CO₂ atmosphere. Thereafter cooling was governed by how quickly CO₂ was removed from the atmosphere. If subduction were efficient this could have taken as little as 10 million years. In this case the faint young Sun suggests that a lifeless Earth should have been cold and its oceans white with ice. But if carbonate subduction were inefficient the CO₂ would have mostly stayed in the atmosphere, which would have kept the surface near ∼500 K for many tens of millions of years. Hydrous minerals are harder to subduct than carbonates and there is a good chance that the Hadean mantle was dry. Hadean heat flow was locally high enough to ensure that any ice cover would have been thin (<5 m) in places. Moreover hundreds or thousands of asteroid impacts would have been big enough to melt the ice triggering brief impact summers. We suggest that plate tectonics as it works now was inadequate to handle typical Hadean heat flows of 0.2–0.5 W/m². In its place we hypothesize a convecting mantle capped by a ∼100 km deep basaltic mush that was relatively permeable to heat flow. Recycling and distillation of hydrous basalts produced granitic rocks very early, which is consistent with preserved >4 Ga detrital zircons. If carbonates in oceanic crust subducted as quickly as they formed, Earth could have been habitable as early as 10–20 Myrs after the Moon-forming impact.     

一种大容量100MHz数据采集记录系统的设计实现

本文提出一种实用的高速数据采集记录系统的设计方案,介绍该系统中各主要模块的功能与设计思路,讨论高速数据存储模块的设计,控制调度流程与高速数字电路设计相关处理方法。针对高速与大容量的数据采集特点,提出用存储速率受限的FLASH芯片来实现高速、大容量数据采集记录的设计方法。     

智能控制大功率氨压机制冷系统

本文将模糊控制、神经元控制等智能控制技术成功地应用于大型活塞式氨压机制冷系统，实现了恒转矩负载的变频调速节能。实际运行结果证明，该智能控制的大功率氨压机制冷系统工作稳定、控制精度高、节能效果显著，具有很好的经济效益及推广应用价值。     

一种高速低噪声信号处理电路的方案研究

文章针对中国遥感高分辨率传输型相机的发展趋势，提出了一种高速低噪声的遥感CCD相机信号处理电路的设计方案。从信号完整性理论出发，利用Cadence软件进行了仿真与验证，取得了良好的效果。     

不同风速下海洋粗糙面散射系数的计算

在考虑风速的条件下,计算了海洋粗糙面的散射特性。用矩量法(MOM)计算了一维介质海洋粗糙面在Durden-Vesecky功率谱下的散射系数,由此获得了一定风速时的双站散射系数。仿真结果表明,计算值与文献数据非常吻合。由计算的不同风速下双站散射系数可知,风速对海洋粗糙面散射特性的影响较大。在一定的海拔高度上,散射角相同(除后向散射方向外)时,风速越大,散射就越强。     

Estimation of sea surface temperature, wind speed and water vapor with microwave radiometer data based on simulated annealing

A method for estimation of sea surface temperature, ocean wind speed and water vapor with microwave radiometer data based on simulated annealing is proposed. The proposed method shows about 60% improvement of sea surface temperature estimation accuracy in comparison to the existing method using Newton’s iterative algorithm.     

壁压法在非矩形风洞中的应用

 解决大攻角洞壁干扰修正的壁压法,是利用一定数量固定位置和形状的线源和线涡来模拟风洞内模型的堵塞效应和升力效应。矩形风洞实验段边界对绕模型流动的影响,可用两个方向有限层的镜像线源和线涡来代替,并利用在风洞上下壁和侧壁上测压点处测量所得