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.     

CFRP反射器型面主动控制和作动器位置优化

研究了运用压电陶瓷作动器对碳纤维增强复合材料（CFRP）格栅反射器的型面主动控制。首先，采用了一种具有独立电压自由度的梁单元，以及考虑高阶剪切变形的板单元，对主控格栅反射器进行有限元建模；运用能量变分哈密尔顿原理推导了主控格栅反射器的有限元控制方程，并给出了反射面型面残余均方根（RMS）误差最小的电压最优控制方法。然后，研究了在典型载荷下，反射面残余RMS误差最小的PZT作动器位置分布的优化配置问题；提出了一种将遗传算法和梯度投影方法相结合的改进优化方法，用来求出在限定作动器数量的条件下，作动器几何位置的优化配置，使控制后反射面的残余RMS误差最小；给出的数值算例验证了方法的正确性和有效性。最后，研制了格栅反射器型面主动控制的实验样机，针对反射器的初始制造误差进行了型面主动控制，验证了控制方法的可行性和有效性。     

Water Partitioning in Planetary Embryos and Protoplanets with Magma Oceans

The water content of magma oceans is widely accepted as a key factor that determines whether a terrestrial planet is habitable. Water ocean mass is determined as a result not only of water delivery and loss, but also of water partitioning among several reservoirs. Here we review our current understanding of water partitioning among the atmosphere, magma ocean, and solid mantle of accreting planetary embryos and protoplanets just after giant collisions. Magma oceans are readily formed in planetary embryos and protoplanets in their accretion phase. Significant amounts of water are partitioned into magma oceans, provided the planetary building blocks are water-rich enough. Particularly important but still quite uncertain issues are how much water the planetary building blocks contain initially and how water goes out of the solidifying mantle and is finally degassed to the atmosphere. Constraints from both solar-system explorations and exoplanet observations and also from laboratory experiments are needed to resolve these issues.     

针对旋翼流场模拟的自适应网格算法

针对基于格心格式求解器的旋翼流场模拟,提出了相应的自适应笛卡尔网格的数据存储结构及自适应算法。给出了相应的单元处理策略,简化了对自适应笛卡尔网格的处理;对于频繁的自适应加密过程中产生的大量重复点,采用了高效的交替数字树算法(Alternating digital tree,ADT)予以删除;对于自适应疏化过程中产生的大量无用点,提出了标记-删除-移动(Mark,delete,move,MDM)算法予以快速地删除,减少了不必要的计算资源消耗。对CaradonnaTung旋翼在不同悬停状态下进行了模拟验证,对比了压力分布系数与桨尖涡位置。之后对HELISHAPE 7A旋翼在前飞情况下进行了模拟验证,计算值与实验值吻合。此外,求解器对桨尖涡的捕捉效果得到了明显的提高,表明本文方法具有良好的有效性与鲁棒性。     

PBT弹性体微相分离及对其力学性能的影响研究

为了获得微相分离对宽温PBT叠氮聚醚弹性体力学性能的影响规律,用红外光谱分析法(FT-IR)和动态热力学分析法(DMA)研究了PBT叠氮聚醚弹性体产生微相分离的机理和影响因素。用调节硬段含量、交联参数的方法调控其微相分离,控制适当的微相分离程度可显著改善推进剂的力学性能。研究结果表明:在二元醇扩链的弹性体体系中,当硬段含量约为15%时,弹性体发生相对最大比例的微相分离,体现出较佳的综合力学性能。通过微相分离的调控可获得宽温范围内综合力学性能较好的叠氮聚醚推进剂用粘合剂基体材料。     

模具CAPP系统

介绍了汽车冷冲压模具行业工艺水平现状和传统CAPP系统特点，以及冷冲压模具厂工艺设计管理模式；分析研究适应于现代汽车模具制造业的模具CAPP系统。     

The Role and Contributions of Energetic Neutral Atom (ENA) Imaging in Magnetospheric Substorm Research

Energetic Neutral Atom (ENA) imaging has contributed substantially to substorm research. This technique has allowed significant advances in areas such as observation and quantification of injected particle drift as a function of energy, observation of dynamics in the tail that are directly related to the effects of imposed (growth phase) and induced (expansion phase) electric fields on the plasma, the prompt extraction of oxygen from the ionosphere during substorms, the relationship between storms and substorms, and the timing of substorm ENA signatures. We present discussion of the advantages and shortcomings of the ENA technique for studying space plasmas. Although the technique is in its infancy, it is yielding results that enrich our understanding of the substorm process and its effects.     

Observations of the Acceleration of Polar Solar Wind Near Solar Maximum

In a previous paper (Tappin et al., 1999) we used cross-correlation analysis of high-cadence observations with the LASCO coronagraphs to trace the acceleration of the solar wind at low latitudes. In this paper we present a similar analysis carried out over the North pole of the Sun. The observations which were made in March 2000 with the C3 coronagraph show low bulk flow speeds (comparable to or lower than those seen at the equator in early 1998). We observe the acceleration continuing to the edge of the C3 field of view at about 30 R _⊙. We also observe, as at low latitude, a high-speed tail but now reaching out well beyond 2000 km s⁻¹. We do not see a clear signature of a fast polar bulk flow. We therefore conclude that at this phase of the solar cycle, any fast bulk flow occupies only a small part of the line of sight and is therefore overwhelmed by the denser slow solar wind in these observations. We also show that the fast component is consistent with observed solar wind speeds at 1 AU. This revised version was published online in August 2006 with corrections to the Cover Date.     

电子工作台在模拟电子技术中的应用

本文简要地介绍了电子工作台的特点和使用方法，结合我们设计具体模拟电子线路的实践，说明了电子工作台在模拟电子技术中的应用。