自来水中的TOC、UV254和浊度的相关性研究

通过应用回归分析方法,对西安市某水厂的出水、管网中间水和管网末梢水的TOC、UV254和浊度的监测数据进行了相关性分析。结果表明：随着供水管网的延长,浊度和UV254的线性相关系数明显增加;随着供水管网的延长,浊度和TOC的线性相关系数明显降低。     

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.     

薄膜生长工艺对TiO_2基紫外探测器光电性能的影响

分别采用磁控溅射和溶胶-凝胶工艺制备了相同厚度的TiO2薄膜,并用以制备了金属-半导体-金属(MSM)结构TiO2基紫外探测器。通过紫外光电性能测试、扫描电子显微镜(SEM)观察及X射线衍射(XRD)分析,研究了TiO2薄膜生长工艺对探测器光电性能的影响规律。结果表明:磁控溅射工艺下,探测器的光电流虽然较低,但响应时间和暗电流远小于溶胶-凝胶工艺制备的探测器,其具备了高辐射灵敏度和快速响应特性。磁控溅射工艺制备的TiO2薄膜结构较为致密,晶界和缺陷较少,方阻较高,这是其取得优良的光电特性的原因。     

Manifestation of magnetic reconnection in coronal streamer current sheets

We investigate the possibility of observing the effects of magnetic reconnection inside a current sheet forming in a coronal streamer in the extended corona. In particular we study the possibility to observe with the UVCS of SOHO the excitation of the tearing instability in the current sheet.     

掺Ce^3＋的碱土氟化物的紫外发光特性研究

研究了掺杂稀土离子Ce^3＋的碱土氟化物发光体LiXAlF6：Ce^3＋（X=Ca^2＋,Sr^2＋或Ba^2＋）,XBaAlF6：Ce^3＋（X=Li6＋,Na^＋或K^＋）及LiBaXF6：Ce^3＋（X=Al^3＋,Ga^3＋或In^3＋）的紫外发光特性。实验发现,在LiXAlF6=Ce^3＋中,随着X元素原子序数的增大,Ce^3＋的发光峰就向短波方向移动。首次研究了在XBaAlF6：Ce^3＋与LiBaXF6：Ce^3＋中的X元素的一价与三价离子对Ce^3＋发光的影响,发现这些一价与三价离子的原子序数的变化并不影响Ce^3＋的发射光谱的峰值,它们只在晶格中起着填隙和电荷补偿作用,这有利于Ce^3＋的发光,使发光强度有所增强。这些紫外发光可用来增强X射线影像板中所包含的储存辐射的发光体BaFBr：Eu“的发光,使X射线影像板的显像增强。     

TiO2光催化薄膜在空间污染防护 应用中的探索

文章采用溶胶凝胶法在JGS1石英玻璃上制备了TiO₂薄膜,并对其晶体结构与光催化性能之间的关系进行了研究,探讨了紫外光辐照下TiO₂薄膜对大分子链硅油光催化效果。结果表明:经500 ℃热处理后的TiO₂薄膜为锐钛矿结构,具有较高的光催化活性;在253 nm紫外光辐照下,TiO₂薄膜对大分子链硅油表现出较好的光催化降解效果。该研究将为空间环境下飞行器光学表面污染净化材料的开发提供有益参考。     

Plant mineral nutrition,gas exchange and photosynthesis in space: A review

Successful growth and development of higher plants in space rely on adequate availability and uptake of water and nutrients, and efficient energy distribution through photosynthesis and gas exchange. In the present review, literature has been reviewed to assemble the relevant knowledge within space plant research for future planetary missions. Focus has been on fractional gravity, space radiation, magnetic fields and ultimately a combined effect of these factors on gas exchange, photosynthesis and transport of water and solutes.     

天基导弹紫外预警及紫外预警探测仪

文章简单介绍了国外导弹紫外预警的研究现状,分析了紫外预警的关键要素。     

Hierarchy of spatial scales in UV prominences

Ultraviolet spectra of a quiescent prominence observed with theHigh Resolution Telescope and Spectrograph (HRTS) are analyzed. Different techniques lead to greatly different spatial scales for the prominence structures. The UV spectra show strong variations in intensity and Doppler shift on scales larger than 1700 km. Spectroscopic diagnostics employing line intensity ratios indicate the existence of scales between 400 m to some hundred kilometers. We attempt to interpret various aspects of the prominence intensities and velocities with a multiple thread model.