基于改进近似模型的水下鱼雷打靶快速预报方法

鱼雷打靶试验对评价武器系统对目标的打击性能具有重要意义。水动力参数是模拟鱼雷水下运动轨迹、预报鱼雷打靶落点的关键参数。随着现代CFD技术的发展,采用数值方法获取水动力参数,提高了轨迹预报精度,但计算效率不高,不利于多工况下鱼雷打靶预报。首先,基于刚体动量和动量矩定理建立了鱼雷的水下运动方程组,运用4阶龙格–库塔（Runge-Kuta）法对运动方程组进行数值求解,对鱼雷水下轨迹进行模拟,从而获取鱼雷打靶性能。其次,提出了基于遗传算法的近似模型（GA-BP）和自适应遗传算法优化的近似模型（AGA-BP）模拟鱼雷水下打靶落点,对鱼雷打靶性能进行快速预报。通过仿真和数据对比,结果表明：AGA-BP预测模型相对于BP预测模型更稳定、GA-BP预测模型收敛速度更快,实现对鱼雷水下打靶快速预报。     

两次北上相似路径台风导致的暴雨湿位涡诊断分析

利用2012年8月28—29日和2019年9月7—8日水平分辨率为0.25°×0.25°的ERA5再分析资料、地面观测资料和中国气象局热带气旋最佳移动路径数据,对两次北上相似移动路径的台风“布拉万”和“玲玲”导致东北地区暴雨天气过程的湿位涡进行诊断分析。结果表明：台风导致的强降水与假相当位温的密集带对应较好,降水主要位于假相当位温密集带偏暖一侧,锋区越强,降水量越大。两个台风过程均在降水前期存在对流不稳定层结,为台风降水提供初始能量积累。初始时刻出现湿对称不稳定,是台风中心西北侧暴雨出现的主要因素。降水增强时刻,大气对流不稳定再次参与,说明低层对流不稳定提供了降水快速增强的主要能量。低层湿正压项(MPV1)和湿斜压项(MPV2)的绝对值均出现先增大后减小再增大的趋势,强降水主要分布在两个极值中间过渡时段。两次北上台风引起的吉林省中部暴雨带均与低层850 hPa的MPV2负值区和MPV1的正值区有较好的对应关系。     

基于GIS地理空间关系的消防审查知识图谱构建

BIM具有精细三维建模的优点,能够通过计算机平台展示消防设备的具体细节,GIS具有强大的空间分析功能,可以反映出BIM模型内构件的空间关系^[1]。随着消防审查技术要求的日益提高,审查人员在消防设备的运营和管控中,大都缺少对消防设备地理空间信息属性的审查环节,这无疑会对审查结果的准确性造成一定影响。本研究针对上述问题,提出将建筑信息建模(BIM)技术与地理信息系统(GIS)技术相结合,实现这两种技术的相辅相成,并引入了知识图谱来改良建模。该方法以《建规》为基础语料库,通过改良的Methontology法,实现半自动化的图谱本体构建;接着采用Stanford大学开发的DeepDive新型数据管理系统,实现消防规范的特征关系抽取;最后在KGB(Knowledge Graph Builder)智能开发平台完成知识图谱的构建。该研究的意义在于一方面能够促进建筑行业与GIS技术的结合,另一方面也能够推动知识图数据库与文本规则条例的融合配对,实现综合楼宇消防构件的实景三维自动化审查。     

基于AHP-TOPSIS的武夷山国家森林步道功能评价及其优化策略

森林步道作为满足民众户外游憩需求的重要空间载体,为游客提供多样化的功能体验。本研究构建了森林步道的功能评价体系,并运用AHP-TOPSIS法对武夷山国家森林步道(邵武段)进行功能评价研究。结果显示：1)生态功能是进行森林步道功能评价的首要因素,森林步道功能影响排序为：生态功能>游憩功能>社会功能>景观功能;2)武夷山国家森林步道(邵武段)各路段功能体验差异较大,不同路段间的生态功能、社会功能、游憩功能、景观功能尚未实现协同发展。最后依据结果提出邵武段国家森林步道功能建设的优化对策。     

激光雷达点云树木建模研究进展与展望

三维树木几何模型是数字城市与数字林业工程的重要组成部分.针对点云树木建模,深入分析了基于广义(泛在)激光雷达点云的树木模型重建方法,提出了聚类思想建模、图论方法建模、先验假设建模、拉普拉斯算子建模与轻量化表达建模5类建模体系,归纳总结了不同建模体系在树冠枝干的细节表达、建模算法性能、树木模型的多层次细节表达、建模体系综...     

撤县(市)设区对城市空间扩展的影响机理——以杭州市为例

城镇化的持续推进对城市空间扩展产生了新的需求,撤县（市）设区是中国城市市辖区实现扩容提质的主要手段之一。以杭州为例,定量测度撤县（市）设区后杭州城区空间扩展的时空特征及其各方面的影响,并探讨了这一区划调整对城市空间扩展影响的作用机理。研究发现：通过撤县（市）设区,杭州城区的建设用地东扩趋势明显,萧山和余杭两区的建设用地新增面积和扩展速度均高于平均水平,且两地建设用地空间存在多中心集聚特征,成为新一轮的杭州建设用地扩展高密度区,城市功能不断凸显。总体来看,撤县（市）设区对城市空间的影响是间接的,具有一定的滞后性,通过引导城市空间扩展的主要方向,实现中心城市人口和产业向新设市辖区的转移和集聚,提供城市空间扩展的载体。撤县（市）设区后需要通过后续的城市规划修编、土地性质和权限调整、生产要素集聚与空间重组等路径,对城市空间扩张与空间演变产生直接影响。     

Mapping of moraine dammed glacial lakes and assessment of their areal changes in the central and eastern Himalayas using satellite data

The relatively rapid recession of glaciers in the Himalayas and formation of moraine dammed glacial lakes(MDGLs) in the recent past have increased the risk of glacier lake outburst floods(GLOF) in the countries of Nepal and Bhutan and in the mountainous territory of Sikkim in India. As a product of climate change and global warming, such a risk has not only raised the level of threats to the habitation and infrastructure of the region, but has also contributed to the worsening of the balance of the unique ecosystem that exists in this domain that sustains several of the highest mountain peaks of the world. This study attempts to present an up to date mapping of the MDGLs in the central and eastern Himalayan regions using remote sensing data, with an objective to analyse their surface area variations with time from 1990 through 2015, disaggregated over six episodes. The study also includes the evaluation for susceptibility of MDGLs to GLOF with the least criteria decision analysis(LCDA). Forty two major MDGLs, each having a lake surface area greater than 0.2 km2, that were identified in the Himalayan ranges of Nepal, Bhutan, and Sikkim, have been categorized according to their surface area expansion rates in space and time. The lakes have been identified as located within the elevation range of 3800 m and6800 m above mean sea level(a msl). With a total surface area of 37.9 km2, these MDGLs as a whole were observed to have expanded by an astonishing 43.6% in area over the 25 year period of this study. A factor is introduced to numerically sort the lakes in terms of their relative yearly expansion rates, based on their interpretation of their surface area extents from satellite imageries. Verification of predicted GLOF events in the past using this factor with the limited field data as reported in literature indicates that the present analysis may be considered a sufficiently reliable and rapid technique for assessing the potential bursting susceptibility of the MDGLs. The analysis also indicates that, as of now, there are eight MDGLs in the region which appear to be in highly vulnerable states and have high chances in causing potential GLOF events anytime in the recent future.     

Dynamic metabolite alterations of Portunus trituberculatus during larval development

A mass mortality often occurs from molting to the megalopa stage during the larval development of the swimming crab Portunus trituberculatus. Larvae with insuffcient nutrient accumulation during the zoeal stages are probably unable to develop into juvenile swimming crabs. However, the nutritional information such as the primary metabolites is scarce for P. trituberculatus larvae. The aim of this work is to obtain an insight into the metabolite traits of P. trituberculatus at early developmental stages. 1 H nuclear magnetic resonance spectroscopy coupled with multivariate data analysis was used to determine how the metabolite pro?les shift during larval development in P. trituberculatus. Our results show that the trend of total metabolites exhibited a rise from zoea 1 to zoea 3, followed by a drop from zoea 4 to megalopa and recovery during the ?rst juvenile stage. A large-scale depletion of total metabolites in the zoea 4 and megalopa stages suggests a deep depression of metabolic activity, which may be linked to the mass mortality from molting to the megalopa stage. These ?ndings provided essential metabolic information about the larval development of P. trituberculatus and important clues for understanding the nutritional requirements of P. trituberculatus in early developmental stages.     

CCD astrometric observations of 2017 VR12, Camillo and Midas

We have observed three near-Earth objects(NEOs), 2017 VR12, Camillo and Midas, during 2018.The observations were made with the 1-m telescope, operated by Yunnan Observatories, over two nights.Their precise astrometric positions are derived from 989 CCD observations. The theoretical positions of asteroids are retrieved from the Jet Propulsion Laboratory(JPL) Horizons System and Institut de M′ecanique C′eleste et de Calcul des ′Eph′em′erides(IMCCE). The positions of three asteroids are measured with respect to stars in the Gaia DR2 star catalog. For 2017 VR12, the means(O-C) of right ascension and declination are -0.090′′and-0.623′′respectively based on the published JPL ephemeris, but the corresponding means(O-C) are 3.122′′and-0.636′′based on the published IMCCE ephemeris. The great difference in declination could be explained by several factors.(1) The degraded CCD images caused by the fast apparent motion of the objects lead to a reduction in positioning accuracy.(2) The poor timing system may introduce systematic errors, especially in the high speed direction.(3) The asteroid may be perturbed by Earth when it approaches the Earth too closely. These astrometric results demonstrate that the centroid centering method can reduce the dispersion of non-Gaussian images as compared with the PSF modeling method.For Camillo and Midas, the astrometric results are consistent based on the two ephemerides. Implementing a high-precision timing system, and analyzing some astronomical effects and geometric distortions in CCD images should be carefully considered in future works.     

Transition-region explosive events produced by plasmoid instability

Magnetic reconnection is thought to be a key process in most solar eruptions. Thanks to highresolution observations and simulations, the studied scale of the reconnection process has become smaller and smaller. Spectroscopic observations show that the reconnection site can be very small, which always exhibits a bright core and two extended wings with fast speeds, i.e., transition-region explosive events.In this paper, using the PLUTO code, we perform a 2-D magnetohydrodynamic simulation to investigate small-scale reconnection in double current sheets. Based on our simulation results, such as the line-of-sight velocity, number density and plasma temperature, we can synthesize the line profile of SiIV 1402.77? which is a well known emission line used to study transition-region explosive events on the Sun. The synthetic line profile of Si IV 1402.77? is complex with a bright core and two broad wings which can extend to nearly 200 km s^-1. Our simulation results suggest that the transition-region explosive events on the Sun are produced by plasmoid instability during small-scale magnetic reconnection.