珞珈一号01星夜光遥感设计与处理

珞珈一号01星是兼具遥感和导航的一星多用低轨维纳科学试验卫星,本文针对珞珈一号01星夜光遥感设计与处理,详细介绍了卫星平台的有效载荷及平台设计;面向科学的试验目标,制订了科学的夜光成像任务计划,实现了全国夜光一张图任务规划;提出了面向珞珈一号01星的在轨几何辐射定标模型;研制了支持WEB端及移动端访问的数据共享服务系统;针对夜光遥感数据在社会经济应用问题,提出了发展指数和未来发展指数的珞珈一号指数模型,并通过相关实验验证了模型的有效性。珞珈一号01星可为社会经济参数估算、重大事件评估、渔业监测、国家安全等领域提供技术支撑。     

基于天地图的便携式自然资源政务云平台研发

以国家天地图互联网数据为基础,以充分融合的某市地理信息三维倾斜数据、VR数据、专题数据与政务大数据为基础平台数据,在便携式移动设备上研发通用的政务大数据平台。并以云服务的形式提供大数据,为政府现场办公管理提供了科学的数据参考,在河长制管理、生态红线划分保护、工农业经济发展、旅游产业发展等方面进行了应用,在推动数字城市、智慧城市发展方面,具有积极的社会意义。     

Linking shock textures revealed by BSE,CL, and EBSD with U‐Pb data (LA‐ICP‐MS and SIMS) from zircon from the Araguainha impact structure,Brazil

A silicious impact melt rock from polymict impact breccia of the northern part of the alkali granite core of the Araguainha impact structure, central Brazil, has been investigated. The melt rock is thought to represent a large mass of impact‐generated melt in suevite. In particular, a diverse population of zircon grains, with different impact‐induced microstructures, has been analyzed for U‐Pb isotopic systematics. Backscattered electron and cathodoluminescence images reveal heterogeneous intragrain domains with vesicular, granular, vesicular plus granular, and vesicular plus (presumably) baddeleyite textures, among others. The small likely baddeleyite inclusions are not only preferentially located along grain margins but also occur locally within grain interiors. LA‐ICP‐MS U‐Pb data from different domains yield lower intercept ages of 220, 240, and 260 Ma, a result difficult to reconcile with the previous “best age” estimate for the impact event at 254.7 ± 2.7 Ma. SIMS U‐Pb data, too, show a relatively large range of ages from 245 to 262 Ma. A subset of granular grains that yielded concordant SIMS ages were analyzed for crystallographic orientation by EBSD. Orientation mapping shows that this population consists of approximately micrometer‐sized neoblasts that preserve systematic orientation evidence for the former presence of the high‐pressure polymorph reidite. In one partially granular grain (#36), the neoblasts occur in linear arrays that likely represent former reidite lamellae. Such grains are referred to as FRIGN zircon. The best estimate for the age of the Araguainha impact event from our data set from a previously not analyzed type of impact melt rock is based on concordant SIMS data from FRIGN zircon grains. This age is 251.5 ± 2.9 Ma (2σ, MSWD = 0.45, p = 0.50, n = 4 analyses on three grains), indistinguishable from previous estimates based on zircon and monazite from other impact melt lithologies at Araguainha. Our work provides a new example of how FRIGN zircon can be combined with in situ U‐Pb geochronology to extract an accurate age for an impact event.     

苏鲁高压-超高压带的结构、变形特征及形成背景探讨

苏鲁高压-超高压变质带由不同层次、不同级别、不同变质岩石组合的构造岩片堆叠而成,自北向南可分别为9个构造岩片。这种复杂的结构的形成和发展主要受早期的变质变形作用控制,并被晚期构造作用改造。本文重点对高压-超高压变质带的构造变形进行了分析,自元古宙—中生代韧性改造事件可分为4期。最后在以上工作的基础上对其形成的地质背景进行了探讨,指出了两次高压-超高压变质事件存在的可能,而且其新元古代的构造事件可与全球Rodinian超大陆的形成与裂解相对比。     

多粒度时空事件建模与可视化方法初探

基于全空间信息系统的应用背景和多粒度时空对象的思想,探讨了时空事件的内涵和基本特征,并提出了多粒度时空事件的概念;分析了现有时空数据模型特点,基于多粒度时空对象数据模型,提出了多粒度时空事件建模的基本理念;以此为依据,针对现有可视化技术的不足,对全空间信息系统对多粒度时空事件的表达特点进行了初步阐述。     

多粒度时空对象可视分析体系初探

可视分析是用户进行数据认知、知识探索的重要工具和方法。全空间信息系统中以多粒度时空对象来进行现实世界实体的抽象和建模,并将其作为特征分析与计算的核心。本文从全空间信息系统的背景出发,对多粒度时空对象可视分析的概念进行阐述,并分析其流程与特点,在充分考虑全空间信息系统应用场景的基础上,提出了"场景—任务—实施方法"的方法体系,并对各实施方法的技术进行了讨论。最后以大数据交通为例,对多粒度时空对象可视分析在交通领域中的应用作了展望。     

时空对象的聚类方法与应用初探

针对传统GIS数据模型描述信息有限以及对象化聚类分析内容不够全面的问题,提出了基于时空对象的聚类方法的流程和应用特点。首先总结了空间聚类和时空聚类的研究现状和主要方法;根据全空间信息系统中多粒度时空对象的描述框架及时空数据的"三维"特征,认为基于时空对象的聚类方法应包含3个方面:时空对象时间序列的相似性描述、基于时空对象的聚类计算及时空对象聚类的有效性评价;最后总结了该方法的特点并展望了其应用场景。基于时空对象的聚类方法研究有助于更全面地分析时空对象空间位置、属性特征及其变化特点,为多粒度时空对象的时空分析提供一种思路。     

Trophic Interaction in a <Emphasis Type="Italic">Portunus rituberculatus</Emphasis> Polyculture Ecosystem Based on Carbon and Nitrogen Stable Isotope Analysis

Trophic interaction among various biomass groups in a swimming crab Portunus trituberculatus polyculture pond was investigated using carbon and nitrogen stable isotope analysis. The polycultured animal species also included white shrimp Litopenaeus vannamei, short-necked clam Ruditapes philippinarum, and redlip mullet Liza haematochila. The mean δ¹³C value for all the biomass groups in polyculture ecosystem ranged from ?25.61‰ to ?16.60‰, and the mean δ¹⁵N value ranged from 6.80‰ to 13.09‰. Significant difference in the δ¹³C value was found between particulate organic matter (POM) and sediment organic matter (SOM) (P < 0.05), indicating that these two organic matter pools have different material sources. Assuming that a ¹³C-enrichment factor of 1.00‰ and a ¹⁵N-enrichment factor of 2.70‰ existed between consumer and prey, diets of the four cultured animals were estimated using a stable isotope mixing model. The estimated model results indicated that P. trituberculatus mainly feed on Aloidis laevis; L. vannamei mainly feed on shrimp feed; while A. laevis, R. philippinarum and L. haematochelia mainly feed on POM. Shrimp feed was also an important food source of R. philippinarum and L. haematochelia. The diets of P. trituberculatus, L. vannamei, R. philippinarum, and L. haematochila showed complementary effects in this polyculture ecosystem. Our finding indicated that the polyculture of these four organisms with suitable farming density could make an effective use of most of the food sources, which can make a highly efficient polyculture ecosystem.     

The ARIEL Instrument Control Unit design

In this paper we present the electromagnetic modeling and beam pattern measurements of a 16-elements ultra wideband sparse random test array for the low frequency instrument of the Square Kilometer Array telescope. We discuss the importance of a small array test platform for the development of technologies and techniques towards the final telescope, highlighting the most relevant aspects of its design. We also describe the electromagnetic simulations and modeling work as well as the embedded-element and array pattern measurements using an Unmanned Aerial Vehicle system. The latter are helpful both for the validation of the models and the design as well as for the future instrumental calibration of the telescope thanks to the stable, accurate and strong radio frequency signal transmitted by the UAV. At this stage of the design, these measurements have shown a general agreement between experimental results and numerical data and have revealed the localized effect of un-calibrated cable lengths in the inner side-lobes of the array pattern.     

地质工程自动监测硬件系统若干技术问题

地质工程自动监测系统具有监测对象信息变化差异大,监测环境恶劣等显着特点。其硬件系统须具备监测范围广,抗干扰能力强,抗雷击等特殊功能。同时,为了适应现代化工程建设的要求,还应具备先进的智能化和网络化等功能。为此,本文对地质工程自动监测系统的功能和组成、当前的发展趋势及所涉及到一些关键硬件技术问题展开了讨论,着重总结了作者有关地质工程自动监测硬件系统关键技术问题的研究。最后介绍了作者为五强溪水电站边坡工程建立的自动监测系统,以及该系统双端防雷保护和模块化信号调理等难题的解决。