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	An Improved Aerosol Retrieval Algorithm for FY-4A/AGRI Data Based on the GRASP Framework 期刊论文 OAI收割 IEEE TRANSACTIONS ON GEOSCIENCE AND REMOTE SENSING, 2025, 卷号: 63, 页码: 4103517 作者: Wang, Huaxuan; Fan, Meng; Jiao, Sunxin; Yan, Huanhuan; Xu, Benben \| 收藏 \| 浏览/下载：5/0 \| 提交时间：2025/04/21 Aerosols Sea surface Spatial resolution Monitoring MODIS Atmospheric modeling Reflectivity Instruments Accuracy Land surface Advanced Geostationary Radiation Imager (AGRI) aerosol optical depth (AOD) Fengyun-4A (FY-4A) generalized retrieval of atmosphere and surface properties (GRASP) optimal estimation method
	The YAG Lidar System Applied in LHAASO 会议论文 OAI收割 Virtual, Berlin, Germany, 2021-07-12 作者: Sun, Q. N.; Geng, L. S.; Li, X.; Chen, L.; Liu, H. \| 收藏 \| 浏览/下载：55/0 \| 提交时间：2022/12/30 YAG-Lidar system atmosphere monitoring LHAASO
	二噁英分析方法与大气中的分布特征研究学位论文 OAI收割博士, 北京: 中国科学院研究生院, 2014 作者: 周志广收藏 \| 浏览/下载：35/0 \| 提交时间：2016/08/15 二噁英，高分辨气相色谱-高分辨质谱，快速筛查法，大气，多级监测体系，Dioxins, HRGC-HRMS, rapid screening method, atmosphere, multilevel monitoring solution
	TSP和PM10监测指标对新疆城市空气质量级别的影响/Influence of monitoring index TSP and PM10 on ambient air quality grade at cities of Xinjiang, China[J] 期刊论文 OAI收割干旱区地理, 2014, 卷号: 37, 期号: 4, 页码: 731-743 作者: 郭宇宏; 王自发; 康宏; 张小啸; 纪元 \| 收藏 \| 浏览/下载：20/0 \| 提交时间：2017/12/29 总悬浮颗粒物可吸入颗粒物空气质量级别影响监测指标 Tsp Pm10 Air Quality Influence Atmosphere Environment Monitoring Indexes
	Research on the support structure of the primary mirror of large-aperture telescope (EI CONFERENCE) 会议论文 OAI收割 3rd International Symposium on Advanced Optical Manufacturing and Testing Technologies, AOMATT 2007: Large Mirrors and Telescopes, July 8, 2007 - July 12, 2007, Chengdu, China Yang W.; Jingxu Z. 收藏 \| 浏览/下载：26/0 \| 提交时间：2013/03/25 Large-aperture telescope can be used in surveying battlefield researching landform searching object real-time monitoring imaging detecting and identifying spatial targets and so on. A large-aperture telescope for achieving high resolution power is designed to monitor spatial target and image in real time. Real-time monitoring plays an important role in military conflicts. The orbit parameter of object quantity geometrical shape parameter and so on can be obtained by detect spatial target. With the development of optical technology people require larger aperture in optics-electronic (OE) system. By increasing optical aperture the ability of collecting light and resolution power in the system can be enhanced. But the support structure of the primary mirror of large-aperture telescope will be a very difficult problem. With the increase of primary mirror aperture the weight of the primary mirror will become larger than before. The root mean square (rms) of the primary mirror is affected by many factors such as deadweight deformation of heat environment and so on. Due to the primary mirror of telescope is an important component of telescope system. By reducing the weight of primary mirror precision of the system is ensured. During the designing phase one can consider the supporting project of the primary mirror synthetically and analyze it roundly according to technical requirement of optical system and the effect factors. The final structural design can be reasonable. In an astronomical telescope the surface of reflector is an important part for collecting dark radiation of celestial bodies. Its surface shape will have an effect on collecting efficiency of telescope radiant energy directly. So the rms must be very high. Optical system of large aperture small wavelength and small focus can receive maximal light intensity. For ground-based optical astronomical telescope the design proposed in the paper can satisfy the requirement of the possible minimum atmosphere seeing at astronomical observatory site and exert the use efficiency of the telescope adequately. So the accuracy of the traditional surface of reflector can assure that 90% of all the light energy can be focused on within the angle diameter range of the minimum atmosphere seeing then 100% of light energy should be focused on the angle diameter range of minimum atmosphere seeing. Because the rms of mirror is very high precise surface machining and accurate the support of mirror are very important tasks during designing and manufacturing the telescope. In the paper various support techniques of a large-aperture telescope primary mirror are discussed and a 3.5 meter telescope system at the Starfire Optical Range (SOR) overviewed simply which was operated by the Directed Energy Directorate of the Air Force Research Laboratory Kirtland AFB NM USA from the ground-based O-E system for the observations of spatial target. We also analyze Theoretical elastic deformation of the Steward Observatory 2.3 meter mirror is analyzed.