中国城市群热岛效应时空演变及其影响因素分析

基于长期不透水面和MODIS地表温度数据,分析2000—2015年中国城市群扩张及热岛效应时空演变,进而综合采用冗余分析(RDA)、线性回归分析和变异分配分析(VPA)等方法,揭示城市群城市热岛效应的驱动机制。结果表明：城市群内建成区面积快速扩张,不透水面比例从2000年2.08%增长到2015年5.33%,且主要集中于珠江三角洲等沿海城市群;2000—2015年,夏季热岛分布较广,且白天强度高于夜晚。东部以及大部分北部城市群如哈长城市群等,降温强度较大,但其夜晚热岛效应在不同程度增强。冬季夜晚比白天热岛分布广、强度高,北方、西北、东部等地区夜晚热岛效应也在增强;自然环境因素显著影响城市群热岛强度,降水对夏季夜晚热岛强度起显著负贡献(22%),纬度越高,冬季夜晚热岛强度也越高。人为因素显著影响夜晚热岛分布和城市群内热岛强度的平衡,城市植被覆盖显著减少夜晚城市群内热岛分布,灯光强度对夏季夜晚热岛强度起显著负贡献(24%),对热岛比例起显著正贡献(27%),人口密度对夏季夜晚热岛强度起显著负贡献(31%);自然环境因素对热岛强度的贡献占主导,而人为干扰因素对热岛比例的贡献占主导。     

东北地区唐代渤海古城遗址空间格局及影响因素分析

运用ArcGIS软件及空间分析等方法,研究了东北地区234座唐朝渤海国古城遗址分布特征,探讨了古城遗址空间格局与自然条件的关系。通过对234座古城址进行分析,发现唐朝渤海国古城址主要集中在4个集聚区,即图们江?鸭绿江流域集聚区（A）、牡丹江流域集聚区（B）、松花江?辽河流域集聚区（C）、穆棱河流域集聚区（D）。其中图们江?鸭绿江流域集聚区是最主要的遗址分布区,位于研究区的南部,占遗址总量的47.43%。研究区渤海国古代城址呈北疏南密的分布特征,形成明显的“空间组群”格局。在当时的气候环境之下,水热条件等自然因素成为影响城址的主要因素,而政治、经济、军事和交通区位等人文因素则对古城遗址的数量和分布起重要导向作用。     

基于贝叶斯层次时空模型的甘肃省土地利用程度演变分析

以甘肃省为例,在基于Google Earth Engine (GEE)平台实现1995年、2000年、2005年、2010年、2015年和2020年土地变化监测的基础上,利用贝叶斯层次时空模型(BHM)分析土地利用程度的时空变化特征。结果表明：① 研究期间内甘肃省土地利用程度呈增长趋势,其中1995―2000年和2010―2015年增长速度较明显;② 土地利用程度空间格局“东高西低”,热点区域主要分布在陇中、陇东和陇南地区;③ 土地利用程度局部变化呈现明显区域差异,整体表现为“东弱西强”,局部变化热点区域主要分布在河西地区;④ 影响土地利用程度变化的主要因素是经济规模和产业结构,其中经济因素影响程度最高。     

乌兰察布市气象资料应用处理与共享技术分析

乌兰察布市气象资料应用处理与共享系统,以该市已经建成的自动气象站实时监测数据为信息资源,充分利用信息网络通讯技术和数据库存储与查询、分析、统计技术,实现全市气象部门自动气象站资料的整合与管理。通过气象资料应用处理与共享平台的建设,实现了气象资料在全市气象部门内的高效共享,并提高了气象资料在业务领域和服务领域的使用率和共享率。     

基于要素服务的地图在线编辑系统设计与实现

针对空间信息平台用户对空间数据的上传、下载、发布和在线编辑的需求,设计实现了基于ArcGIS Server要素服务和Flex的具有地图数据在线编辑功能的Web GIS系统。本系统应用RIA技术,实现了空间与属性数据的在线编辑,符号在线编辑和用户数据管理等,用户体验上也得到很大提升。通过工程化的设计实现,能够满足＂平台＂跨部门多应用主体的实际需求。     

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The Seasonal Variabilities in the Concentration of Atmospheric Aerosols over Qingdao, China

Mass concentrations of Total Suspended Particles （TSP） and size-segregated particles were obtained from July 2001 to June 2002 in Qingdao to characterize the seasonal variations of atmospheric aerosols and to show the impact of dust events on the air quality in Qingdao. Data on size-segregated aerosols show that 73.74% of the TSP mass concentration is contributed by particles with diameters less than 11 μm. Particles with diameters less than 1.1μm have a higher concentration during the winter. In spring, larger particles tend to have higher mass concentrations. Bimodal particle size distributions have been observed, with maxima around 4.7-7 μand 0.43-0.65 μm in the winter season, and 7-11 μm and 0.65-1.1 μm in the autumn season. Measurements made during the dust events in March 2002 show high concentrations of particles in the size range 2.1-7μm.     

Assessment of code bias variations of BDS triple-frequency signals and their impacts on ambiguity resolution for long baselines

GPS Solutions - Carrier phase ambiguity resolution over long baselines is challenging in BDS data processing. This is partially due to the variations of the hardware biases in BDS code signals and...     

Seawater flux through Taiwan strait

After the winter and summer current structures on two or three latitudinal sections in Taiwan Strait were obtained from the measured current data, the seawater fluxs through the sections were calculated. In summer, the currents in the central and northern part of Taiwan Strait normally flow northward at a net flux of 3.32×10⁶m³/s. In winter, the high temperature and salinity Kuroshio and South China Sea water enter Taiwan Strait from the southem section at 1.69×10⁶m³/s and 0.59×10⁶ m³/s respectively, while the East China Sea water enters Taiwan Strait from the northern section at 1.02×10⁶m³/s. About 0.40×10⁶ m³/s of the seawater enters the South China Sea along the coast of Fujian and Guangdong; the other 0.62×10⁶ m³/s of the seawater is mixed with the Kuroshio water and the South China Sea water in the northern sea areas. The net northward flux is 1.74×10⁶m³/s in winter.     

Semi-empirical models of the white-light flare on October 24, 1991

On October 24, 1991, a white-light flare was observed both from space and from the ground. A multi-waveband spectral analysis shows that the peak time of the continuum emission coincides well with that of a radio burst at 2840 MHz and with the hard X-ray emission. Three semi-empirical models, corresponding to the pre-flare condition and to the peak time of continuum emission both with and without non-thermal excitation and ionization of hydrogen by an electron beam, have been obtained. The results indicate that there is fast heating both in the chromosphere and the photosphere. Some evidence is given that this WLF is very likely a result of bombardment by an electron beam. By taking into account non-thermal effects, the chromospheric temperature of the semi-empirical model is significantly reduced.