新型冠状病毒肺炎疫情可视化进展与分析

新冠肺炎疫情期间,疫情数据成为民众关注的重点,涌现出了大量可视化图件,及时地向公众传达着疫情的数量信息和时空分布及变化,帮助大众快速了解疫情当前状况、推断发展趋势.本文从疫情数据可视化表达内容的维度出发,分析不同可视化的表达形式以及其对疫情数据的加工程度,结合示例把可视化分为"1阶"、"2阶"和"多阶",并分析各自表达...     

基于加权Voronoi图评价安徽省城市空间吸引力影响范围

为了评价安徽省城市空间吸引力的影响范围,本文利用Voronoi图的空间剖分特性,结合主客观综合赋权法,提出了运用组合权计算中心性强度,将其作为权重引入模型,建立安徽省城市加权Voronoi图,与周长-面积分形理论和新一线城市研究所2019年发布的新一线城市排名作对比分析,分析了安徽省城市的空间吸引力影响范围。经分析验证,建立的组合权Voronoi图能够有效地对安徽省城市的吸引力影响范围进行评价。此外对城市等级的划分,也提供了借鉴和参考。     

非平衡非耗散热力学及非平衡相图计算

非平衡非耗散热力学是现代热力学中的一个全新领域。该领域的基本情况可参见王季陶的最新英文专著《Nonequilibrium Nondissipative Themodynamics》一书[Springer的网页：http://www.springer.de/egi-bin/search book.pl？isbn=3-540-42802-x]。文中对现代热力学完整的基本分类系统和非平衡相图的计算展开一定的讨论。     

Schmidt plate survey in the galactic centre direction. 1. Investigation of open clusters in the Sagittarius-Carina spiral arm

A study of four open clusters on Tautenburg Schmidt plates in the direction to the Galactic Centre (l = 17.0°, b = +0.8°) is presented. In a field of 8.95 square degrees proper motions and B, V magnitudes were determined for about 36 500 stars up to the limiting magnitudes B = 17^m.9, V = 16^m.8. For stars brighter than B = 16^m an accuracy of about 3 mas/year has been estimated for proper motions. The rms errors of stellar magnitudes and (B—V) colours is about 0.1 mag. There are two open clusters already known in this sky area: Trumpler 32 (C 1814-133) and NGC 6611 (C 1816-138). By the inspection of the plates two additional anonymous clusters were identified near the double star ADS 11285 or BD −14°5014 (C 1819-146) and near the star BD −14°5016 (C 1820-146). The cluster membership determination was carried out using information on spatial and proper motion distributions of stars in the field. The colour-magnitude diagrams up to the limiting stellar magnitude were constructed. For each cluster interstellar extinction A_V, diameters of the core and corona, ages and spatial velocity components (V, W) relative to the LSR in the Y, Z-galactic directions were derived. The distances to the clusters were obtained to 1720 pc, 2260 pc, 2130 pc and 2130 pc for Trumpler 32, NGC 6611, C 1819-146 and C 1820-146, respectively. All clusters are situated in the Sagittarius-Carina spiral arm. Their spatial location confirms the assumption that galactic spiral arms are close to logarithmic spirals with a characteristic angle of about 20 degrees.     

盐田兑卤法提高光卤石矿质量的方法探讨

通过相图分析及计算,介绍了一种"由盐湖卤水兑卤除氯化钠后,首先获得成矿卤水,然后对其蒸发制取质量较好光卤石矿"的生产方法。