Constraints on Coronal Outflow Velocities Derived from UVCS Doppler Dimming Measurements and in-Situ Charge State Data

We constrain coronal outflow velocity solutions, resolved along the line-of-sight, by using Doppler dimming models of H I Lyman alpha and O VI 1032/1037 Å emissivities obtained with data from the Ultraviolet Coronagraph Spectrometer (UVCS) on SOHO. The local emissivities, from heliocentric heights of 1.5 to 3.0 solar radii, were determined from 3-D reconstructions of line-of-sight intensities obtained during the first Whole Sun Month Campaign (10 August to 8 September 1996). The models use electron densities derived from polarized brightness measurements made with the visible light coronagraphs on UVCS and LASCO, supplemented with data from Mark III at NCAR/MLSO. Electron temperature profiles are derived from 'freezing-in' temperatures obtained from an analysis of charge state data from SWICS/Ulysses. The work concentrates on neutral hydrogen outflow velocities which depend on modeling the absolute coronal H I Lyα emissivities. We use an iterative method to determine the neutral hydrogen outflow velocity with consistent values for the electron temperatures derived from a freezing-in model.     

Observation of Transition Region Fine Structures with Soho/Sumer

We present a preliminary analysis of two quiet Sun transition region areas observed with the SOHO/SUMER spectrometer, using lines from oxygen, nitrogen and silicon. The average quiet Sun physical parameters are studied as a function of line intensity. Systematic variations of line position and width with increasing intensity are found. A large number of small-scale active points have been observed, and preliminary analysis of the physical properties and dynamics of these active features is presented. A jet-like structure, found in an active point, is also investigated and its velocity along the line of sight determined. This revised version was published online in June 2006 with corrections to the Cover Date.     

环氧乙烯基酯树脂耐环境老化性能研究

研究了环氧乙烯基酯树脂基体及其复合材料的耐环境老化性能,包括耐湿热性能、耐自然老化性能及耐紫外光老化性能。研究结果表明,环氧乙烯基酯树脂体系具有良好的力学性能、耐湿热性能,在环境老化及耐紫外光辐射老化试验中表现出一定的稳定性,且工艺操作简便,可以作为户外基础设施用复合材料。     

考虑月球扁率修正的月球卫星自主导航

针对月球扁率对月球紫外敏感器的月心方向矢量确定的不利影响,研究了月球紫外敏感器的测量原理和敏感到月平边缘时满足的几何约束,提出了一种考虑月球扁率的月心矢量确定方法。并进一步的结合地球敏感器和太阳敏感器的测量信息,研究了基于日地月方位信息的月球卫星自主轨道算法,并评估了月球方位确定算法对导航精度的影响。仿真结果表明,在太阳敏感器、地球敏感器和月球敏感器的精度分别为0.02°(3σ)、 0.05°(3σ) 和0.1°(3σ)的假设下,考虑月球扁率修正的月球卫星的自主导航位置精度能达到300m(3σ),导航速度误差能达到0.6m/s(3σ), 从而保证了环月卫星的导航精度。     

Ag/TiO2/ITO紫外探测器的制备及其光电性能

采用胶体晶体模板技术,结合磁控溅射工艺,制备出光电性能较为优异的 Ag反点阵列/TiO2/ITO三明治结构紫外探测器。通过扫描电子显微镜( SEM)、XRD、四探针测试仪及半导体参数测试仪对探测器的微观结构和光电性能进行了测试与表征。结果表明：反点阵列孔径对探测器光电性能影响较为显著;随着孔径增大,探测器的暗电流逐渐增大,光电流先增大后减小,响应时间逐渐延长;孔径为4.2μm时,探测器的光电性能达到最佳;孔径较大的反点阵列电极,具有较高的电导率、较低的紫外光透过率以及较大的光生电子-空穴的复合概率。     

双酚A型环氧树脂的阳离子光固化体系的研究

通过研究光引发剂、光敏剂和链转移剂等对双酚A型环氧树脂阳离子光固化的影响,确定了双酚A型环氧树脂光固化体系的配方组成。利用湿法手工铺叠工艺和紫外光辐照固化技术,制备了玻璃布/双酚A型环氧树脂复合材料,研究了光敏剂和链转移剂等对光固化复合材料力学性能的影响。结果表明:可利用紫外光辐射固化成型技术制备玻璃布/双酚A型环氧树脂复合材料,加入链转移剂的光敏树脂基复合材料具有良好的力学性能。     

空间环境对漫反射板的影响

光学系统在空间环境条件下的衰变对卫星遥感仪器探测精度有重要影响．漫反射板是星载光学遥感仪器辐射定标的重要工具．本文通过对ＡＤＥＯＳ／ＴＯＭＳ和Ｅａｒｔｈ Ｐｒｏｂｅ／ＴＯＭＳ仪器馒反射板漫反射率衰变特性的比较，分析研究了原子氧和太阳紫外辐射对漫反射板的影晌．结果表明，太阳紫外辐照和原子氧剥蚀引起的漫反射板反射率衰变系数分别为０．０００４９／ｈ和１．２ × １０－１７ｃｍ２，但在卫星入轨初期，太阳紫外辐照的影响可增加约４倍．     

紫外探测器光谱响应及噪声测量装置

介绍了紫外探测器相对光谱响应、绝对光谱响应、噪声测量装置,给出了测量结果,并进行了测量不确定度分忻。     

Search for organic molecules at the Mars surface: The “Martian Organic Material Irradiation and Evolution” (MOMIE) project

The life on Mars remains an open question because of the lack of proof of its past emergence and its current presence. The only indices of a potential Martian life were provided by the Viking Landers, and the study of the Martian meteorite ALH84001 discovered in the Antarctic. In the two case, the results of experiments could be explained either by the presence of life forms or by abiotic processes. The recent data of Mars Express orbiter and Mars Exploration Rovers show different proofs of a past environment favourable for life. Among the targets we seek, the organic molecules are primordial because they are necessary to the origin of life. A key question is to know if they are present, in which concentration and under which form. Within the framework of a search for organic, we are developing an experimental setup simulating as close as possible the environmental conditions of Mars surface in order to determine how organic species evolve. We present here the first step of the development of this experiment which focuses on the study of the impact of the solar UV radiations reaching the Mars surface on glycine. First results show that glycine does not resist if directly exposed to UV radiations.