基于TOPMODEL的饮马河流域暴雨洪水模拟研究

将TOPMODEL应用于饮马河流域,选取2013-2019年共6次暴雨洪水过程进行模拟和评估,将饮马河模拟流量与实测流量对比分析,探讨该模型在该流域洪水模拟的可用性.结果表明:TOPMODEL实现了空间产流面积分布的可视化;TOPMODEL在饮马河流域模拟效果较好,可用于该流域流量预报;不同等级降雨量、不同的降雨落区以及前期降雨多寡对饮马河的流量影响较大,即累计雨量越大、雨强越强、强降雨越靠近上游、前期降雨越多,洪峰流量也越大.因此,TOPMODEL可为饮马河流域的防洪调度和防灾减灾提供技术支持.     

A pilot survey on antimicrobial activity and diversity of soil-derived actinobacteria from different depths in Gudzhirganskoe saline lake in Eastern Siberia

To explore pharmaceutical actinobacteria from salty environments in Siberia, 8 soil samples were collected from different depths of Gudzhirganskoe saline lake, the Republic of Buryatia, Russia.Totally, 635 actinobacterial strains affiliated with 21 genera in 12 families of 7 orders were obtained by culture-dependent approaches. The predominant genus was Streptomyces(74.5%), followed by Microbacterium(4.9%), Agromyces(3.5%), Nocardiopsis(3.0%), and Kitasatospora(2.5%). Seven strains showed relati...     

The Variability and Radial Velocity of Planetary Nebula Central Stars

The extremely accurate estimates of stellar variability and radial velocity in the Gaia Data Release 3(Gaia DR3)have enabled us to examine the close binarity and radial velocity(RV) of central stars(CSs) of planetary nebulae(PNe). This study is twofold:(1) searching for new close binary CS candidates to better understand how binarity affects the formation and evolution of PNe; and(2) extending the sample size of known RVs of PNe in order to understand their kinematics and the dynamics of the Mil...     

基于ORB-SLAM3的惯性RGB-D稠密地图构建方法

针对ORB-SLAM3构建的稀疏地图不能直观展现室内环境问题,同时验证ORB-SLAM3中惯性RGB-D相对于RGB-D稠密地图构建的优势以及回环检测环节对于惯性RGB-D稠密地图构建的影响,本文探讨了一种基于ORB-SLAM3的惯性RGB-D稠密地图构建方法。该方法在分析ORB-SLAM3惯性RGB-D模式工作的基础上,增加了稠密建图模块,通过稠密点云构建、体素滤波、稠密点云回环更新等步骤,最终得到能够直观反映周围环境的稠密地图。通过实验验证,本文探讨的ORB-SLAM3的惯性RGB-D稠密地图构建方法是有效可行的,惯性RGB-D模式能够有效解决相机运动中特征跟踪容易丢失问题;稠密点云回环更新能够消除IMU初始不稳定运行导致点云模型杂乱问题。在实地采集的数据集下的实验结果表明,基于ORB-SLAM3的惯性RGB-D稠密地图相比于RGB-D稠密地图,在特征线段测量方面精度提升68%,在角度测量方面精度提升91%,表现出更高的精度和地图构建能力。     

我国南方西南和中东部区域两次持续性低温雨雪过程与关键环流系统的关系研究

利用NCEP再分析资料和国家气象信息中心提供的753站逐日气温和降水资料,对比分析了我国南方西南和中东部区域两次持续10 d以上的低温雨雪过程,结果表明:(1)两次过程中欧亚大陆中高纬东亚大槽均加深,但环流形势有差异。西南过程呈现"北高南低"形势,关键脊区在贝加尔湖,而中东部区域过程"北高南低"和"西高东低"形势共存,关键脊区从乌拉尔山延伸至贝加尔湖。两次过程异常的环流与北大西洋向东传播的波列有关。(2)西南过程关键脊区提前过程3 d发展并东移至贝加尔湖,形成稳定形势;而中东部区域过程关键脊区提前过程一周发展,在开始日达最强。两次过程均伴随蒙古高压东移南压使地面降温,500 hPa关键脊区超前蒙古高压2 d变化。西南过程降温主要受到冷平流和绝热冷却影响,而中东部区域过程主要受到冷平流的影响。(3)西南过程水汽来自孟加拉湾,只受南支槽支配。中东部区域过程水汽来自孟加拉湾、南海和西太平洋,由南支槽和西太平副热带高压的共同影响。两次过程水汽正收支主要来自南边界。     

Analysis of petroleum hydrocarbons in mangrove sediments of Red Sea of Yemen

A field work has been carried out to identify the occurrence of oil and oil products pollution in mangrove sediment from Red Sea of Yemen. The concentration of total petroleum hydrocarbons is from 700ng/g at Kamaran Island station to 400 ng/g at Al-Hodiedah station, and the total organic carbon （TOC） in samples ranges from 0. 07% at Dhubab station to 0. 03% at Kamaran Island station. This pollution is as a result of localized oil pollution and/or heavy ship traffic in the Red Sea and Gulf of Aden.     

广西某矿田磁黄铁矿的研究及其区别特征

Naturally occurring hexagonal and monoclinie pyrrhotites have been recognized by X-ray diffraction analysis and DTA from an ore deposit in Guangxi. They are distinguishable from each other in magnetism, reflectivity, hardness and some other properties. A correct distinction between hexagonal and monoclinie pyrrhotites is of practical importance in prospecting and theoretical study.     

Could CoRoT-7b and Kepler-10b be remnants of evaporated gas or ice giants?

We present thermal mass loss calculations over evolutionary time scales for the investigation if the smallest transiting rocky exoplanets CoRoT-7b (∼1.68R_Earth) and Kepler-10b (∼1.416R_Earth) could be remnants of an initially more massive hydrogen-rich gas giant or a hot Neptune-class exoplanet. We apply a thermal mass loss formula which yields results that are comparable to hydrodynamic loss models. Our approach considers the effect of the Roche lobe, realistic heating efficiencies and a radius scaling law derived from observations of hot Jupiters. We study the influence of the mean planetary density on the thermal mass loss by placing hypothetical exoplanets with the characteristics of Jupiter, Saturn, Neptune, and Uranus to the orbital location of CoRoT-7b at 0.017 AU and Kepler-10b at 0.01684 AU and assuming that these planets orbit a K- or G-type host star. Our findings indicate that hydrogen-rich gas giants within the mass domain of Saturn or Jupiter cannot thermally lose such an amount of mass that CoRoT-7b and Kepler-10b would result in a rocky residue. Moreover, our calculations show that the present time mass of both rocky exoplanets can be neither a result of evaporation of a hydrogen envelope of a “Hot Neptune” nor a “Hot Uranus”-class object. Depending on the initial density and mass, these planets most likely were always rocky planets which could lose a thin hydrogen envelope, but not cores of thermally evaporated initially much more massive and larger objects.