Multi-Criteria Decision Analysis integrated with GIS and remote sensing for astronomical observatory site selection in Antalya province,Turkey

Astronomical observatory site selection is a complex problem that involves evaluation of multiple factors from different sources. The aim of this study is to select the best possible candidates for astronomical observations sites using Multi-Criteria Decision Analysis integrated with Geographical Information Systems and remote sensing technologies. The study was implemented in the Antalya province of Turkey, which is convenient for astronomical site observatory facilities with its appropriate climate properties and weather conditions. Eleven factors (cloud cover, precipitable water, earthquake zones, geology, landslide inventory, active fault lines, Digital Elevation Model, city lights, mining activities, settlement areas, roads) were determined, splitting into three categories; meteorological, geographical and anthropogenic criteria. These factors were evaluated using Analytical Hierarchy Process method and the weights of criteria layers were determined. As a result, the most suitable areas were located extensively in western and eastern part of Antalya. This study offers a robust, accurate, cost and time effective procedure for preliminary site selection for astronomical observatory. However, for a final decision of the best location of astronomical observatory, site testing measurements and atmospheric seeing observations will be further required in these preliminary areas.     

Mercury’s Surface Composition and Character as Measured by Ground-Based Observations

Mercury’s surface is thought to be covered with highly space-weathered silicate material. The regolith is composed of material accumulated during the time of planetary formation, and subsequently from comets, meteorites, and the Sun. Ground-based observations indicate a heterogeneous surface composition with SiO₂ content ranging from 39 to 57 wt%. Visible and near-infrared spectra, multi-spectral imaging, and modeling indicate expanses of feldspathic, well-comminuted surface with some smooth regions that are likely to be magmatic in origin with many widely distributed crystalline impact ejecta rays and blocky deposits. Pyroxene spectral signatures have been recorded at four locations. Although highly space weathered, there is little evidence for the conversion of FeO to nanophase metallic iron particles (npFe⁰), or “iron blebs,” as at the Moon. Near- and mid-infrared spectroscopy indicate clino- and ortho-pyroxene are present at different locations. There is some evidence for no- or low-iron alkali basalts and feldspathoids. All evidence, including microwave studies, point to a low iron and low titanium surface. There may be a link between the surface and the exosphere that may be diagnostic of the true crustal composition of Mercury. A structural global dichotomy exists with a huge basin on the side not imaged by Mariner 10. This paper briefly describes the implications for this dichotomy on the magnetic field and the 3 : 2 spin : orbit coupling. All other points made above are detailed here with an account of the observations, the analysis of the observations, and theoretical modeling, where appropriate, that supports the stated conclusions.     

地球观测科学的发展以及空间站对地观测

综述了地球观测科学的发展以及空间站对地观测。对载人空间站在对地观测中的优势、类型和应用进行了重点论述。介绍了我国空间站对地观测应用的重要意义。最后，论述了以空间站为核心的天基信息网和遥感技术的快速发展是空间对地观测的主要发展趋势。     

Sol-gel法制备CuSO4，Cu〈AC）2掺杂SnO2的气敏性能研究

以溶胶-凝胶法（Sol-gel）制备纳米SnO2及其不同比例的铜源掺杂物。采用热分析（TG-DTA），XRD等手段对其产物进行表征，利用静态配气法测试了掺杂产物的气敏性能。实验结果表明：采用Sol-gel法制备掺杂SnO2的气敏性能，同时受铜源和掺杂量的影响，且掺杂产物对乙醇不很敏感，但在150℃工作温度下对0．005％的H2S具有36367倍的高灵敏度。     

基于小波变换的遥感图像边缘检测方法研究

遥感图像处理对于航空、航天、军事侦察、灾害预报等许多军事和民用领域至关重要,本文针对遥感图像的特点,提出了一种基于小波变换的图像边缘检测方法,同时还对小波变换在图像处理中的适用性进行了详细分析。由实验结果表明,本文方法可以获得非常细致有效的边缘信息,在有效抑制噪声的同时,提高了边缘定位精度。     

嵌入式大气数据传感系统压力传感器设计研究

嵌入式大气数据传感(FADS)系统较之传统的大气数据系统有很大的优势,它依靠飞行器前端的压力传感器间接得到飞行大气数据.在本文中,首先简要介绍了FADS系统的压力模型;然后通过分析压力传感器几何外形设计对系统性能的影响,建立了压力传感器的动力学模型,并提出了FADS系统中的压力传感器的设计准则;最后给出了仿真结果.     

星载光学遥感器消杂光技术现状与发展

通过对国内外杂散辐射理论发展状况的研究和消杂光技术的探讨，归纳出杂光技术领域目前的国际水平以及该项技术的发展趋势；分别从散射理论、分析软件、测试途径以及杂光抑制措施等７个方面，力图全面系统地阐述该项技术的诸方面内容。文章从国情出发，根据当前中国消杂光技术现状和未来高水平空间遥感器的要求，提出下一步中国消杂光技术发展的建议。     

Technology Progress Report for Microwave Remote Sensing

In this presentation, technological progress for China's microwave remote sensing is introduced. New developments of the microwave remote sensing instruments for China's lunar exploration satellite (Chang'E-1), meteorological satellite FY-3 and ocean dynamic measurement satellite (HY-2) are reported.     

CCD星敏感器光学系统设计

介绍ＣＣＤ星敏感器用光学系统设计的参数选择,光学系统的设计光谱范围０．４８、０．８５μｍ;焦距为７５ｍｍ,Ｆ／１．４４,视场８．５°。该系统为复杂化的Ｐｅｔｚｖａｌ结构形式;以点列图能量集中度和能量重心偏评价光学系统的成像质量。所选用的ＣＣＤ芯片像元尺寸为２３μｍ×２３μｍ,像元数３８４×２８８,全视场内混色光点列图能量重心偏最大值１．６μｍ,对应于４．３９角秒。     

信道状态信息无线感知数据获取及应用综述

近年来,基于信道状态信息（CSI）的无线感知技术在室内定位、活动识别、健康检测等方向有众多探索性研究应用。然而,现有研究获取CSI数据主要依靠自主采集,对CSI开源数据集和数据采集设备/工具的研究现状不够清晰。首先阐述了基于无线保真（WiFi）CSI的无线感知技术,详细介绍了9种CSI数据采集设备/工具,概括了CSI的应用方向及研究现状,并汇总了近5年的CSI开源数据集,分析了现有CSI无线感知研究的局限性与面临的挑战,最后总结全文并对CSI无线感知未来的发展进行展望。