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.     

关于CCSDS体制数据安全保护实施位置的探讨

主要阐述CCSDS（空间数据系统咨询委员会）标准的信息安全问题，重点是航天器安全，从分析空间数据面临的安全威胁出发，讨论了CCSDS不同安全实施位置的特点；并在此基础上，通过对CCSDS业务及数据结构的影响对比，总结出不同安全实施方法的优缺点，该结合对于采用CCSDS标准的空间数据系统如何解决信息安全问题，具有一定的参考价值。     

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.     

基于CPLD的高速可重构PCM帧同步器的实现

给出一种基于 CPL D的高速可重构帧同步器的设计思路和实现方法 ,探讨如何提高系统速度及其可靠性。既采用数字化相关检测技术和可容错的校验保护技术 ,又采用系统内在线可编程 ISP(In- System Programm ing)技术和提高系统速度的流水线技术 ,综合高速 PCI总线接口设计 ,完成了在线可重新配置的高速帧同步器的实现     

固体火箭发动机燃烧室和喷管热防护安全限设计系统

随着固体推进技术的发展，越来越多的战术导弹采用了单室双推力固体火箭发动机，燃烧室和喷管的受热情况严重，必须对其进行深入研究，以保证发动机可靠工作。文中对此建立了集药柱几何计算、内流场、传热与烧蚀于一体的计算系统，并形成了成熟的软件，对一具体算例进行了绝热结构和烧蚀结构防护层的安全厚度设计，与工程实际应用厚度的比较表明，此系统用于工程中方便可靠。     

论航天遥感器研制过程中的防静电

文章从应用新技术、新器件可能对航天遥感器产品带来的静电损伤的现象入手 ,介绍了静电放电原理、带来的危害及生成的因素。分析了航天遥感器在研制过程中出现的静电放电现象和产生的原因 ,提出了研制过程中应采取的防静电措施     

“长征三号”一,二级火箭的防潮,防水

叙述了“长征三号”火箭，首次在雨季发射时，采用的防潮防水技术的实施方案及使用后的效果。它给运载火箭的电气系统正常工作创造了良好的环境条件，保证了火箭安全、可靠、及时发射。     

TC4钛合金的微动磨损及防护

对Ｔｉ－６Ａｌ－４Ｖ合金在１８℃，１００℃２５０℃下的微动磨损特性及防护工艺进行了研究。表明：该合金微动磨损的主要磨损形式是疲劳脱层，其磨损量随温度升高而下降，高渐微动磨损量与磨损区表面所形成的氧化层的性质及厚度有关。     

基于神经网络的电机智能保护器研究

介绍了一种电机智能保护装置系统，分析了对电动机进行各类保护的原理，并且针对过载保护．提出一种基于人工神经网络的电动机长期过载运行温升预测的算法，将这种算法应用于实际的保护中．有效地弥补了不能用数学模型精确描述电机运行中发热和散热过程的缺陷。实验证明，在样本足够多的情况下，这种方法是切实可行的。