北斗在南/北极地区的基本定位性能评估

基于BDS、GPS系统的星座结构,对当前的BDS二代导航系统（BD2）、全部建成后的BDS系统在极地科考站（黄河站、昆仑站、中山站、长城站）和北极圈的可见卫星数、DOP值、定位精度等进行评估,并将建成后的BDS、GPS及其组合系统在南/北极的基本定位性能进行对比分析。仿真结果表明,当前的BD2只实现了极地的部分覆盖,对极地提供导航定位的能力有限,大范围内的定位精度大于30.0 m; BDS在极地的定位精度将与GPS相当,可见卫星数可达13颗左右,PDOP值优于1.6,定位精度优于8.0 m;GPS/BDS组合后在极地的PDOP值优于1.4,定位精度优于6.0 m。
     

基于GNSS的LEO卫星TRAIM可用性算法及分析

详细研究了基于GNSS的LEO卫星接收机授时自主完好性（TRAIM）故障检测数学模型以及可用性算法。以GPS和BDS组合为例,分别对500 km、650 km、800 km和1 400 km等几种典型轨道高度的卫星,开展基于GNSS的LEO卫星TRAIM可用性仿真分析。结果表明,在告警阈值100 ns时,基于GPS+BDS组合系统的TRAIM检测可用概率达到99.1%以上,基本满足LEO卫星TRIAM检测可用性需求。     

Spatial distribution of snow depth based on geographically weighted regression kriging in the Bayanbulak Basin of the Tianshan Mountains,China

Snow depth is a general input variable in many models of agriculture,hydrology,climate and ecology.This study makes use of observational data of snow depth and explanatory variables to compare the accuracy and effect of geographically weighted regression kriging(GWRK)and regression kriging(RK)in a spatial interpolation of regional snow depth.The auxiliary variables are analyzed using correlation coefficients and the variance inflation factor(VIF).Three variables,Height,topographic ruggedness index(TRI),and land surface temperature(LST),are used as explanatory variables to establish a regression model for snow depth.The estimated spatial distribution of snow depth in the Bayanbulak Basin of the Tianshan Mountains in China with a spatial resolution of 1 km is obtained.The results indicate that 1)the result of GWRK's accuracy is slightly higher than that of RK(R~2=0.55 vs.R~2=0.50,RMSE(root mean square error)=0.102 m vs.RMSE=0.077 m);2)for the subareas,GWRK and RK exhibit similar estimation results of snow depth.Areas in the Bayanbulak Basin with a snow depth greater than 0.15m are mainly distributed in an elevation range of 2632.00–3269.00 m and the snow in this area comprises 45.00–46.00% of the total amount of snow in this basin.However,the GWRK resulted in more detailed information on snow depth distribution than the RK.The final conclusion is that GWRK is better suited for estimating regional snow depth distribution.     

PS Vir:a short-period solar-like contact binary

We present multi-color photometric observations and a one-dimensional spectrum, acquired from March 2016 to May 2017, for the short-period eclipsing binary PS Vir, by using the 2.16-m,85-cm and 60-cm telescopes at Xinglong station, which is administered by National Astronomical Observatories, Chinese Academy of Sciences. The spectral type was determined as G2V from the onedimensional spectrum. The photometric solution was reduced from BV Rc light curves. The results imply that PS Vir is a W-subtype contact binary with a mass ratio of q = 0.305(±0.008) and a fill-out factor of f = 14.4(±1.8)%. The orbital period may be undergoing a cyclic oscillation with an amplitude of A = 0.0027(±0.0001) d and a modulated period of 11.7(±0.2) yr, which may result from the light-time effect due to a third body. The lower limit on mass for the assumed component is 0.12 M⊙.Moreover, the more massive component of PS Vir may be a bit more evolved star as determined from the mass-luminosity diagram.     

Binary Star Fractions from the LAMOST DR4

Stellar systems composed of single, double, triple or higher-order systems are rightfully regarded as the fundamental building blocks of the Milky Way. Binary stars play an important role in formation and evolution of the Galaxy. Through comparing the radial velocity variations from multiepoch observations, we analyze the binary fraction of dwarf stars observed with LAMOST. Effects of different model assumptions, such as orbital period distributions on the estimate of binary fractions,are investigated. The results based on log-normal distribution of orbital periods reproduce the previous complete analyses better than the power-law distribution. We find that the binary fraction increases with Teff and decreases with [Fe/H]. We first investigate the relation between α-elements and binary fraction in such a large sample as provided by LAMOST. The old stars with high [α/Fe] dominate with a higher binary fraction than young stars with low [α/Fe]. At the same mass, earlier forming stars possess a higher binary fraction than newly forming ones, which may be related with evolution of the Galaxy.     

海岸破波带内悬沙空间分布试验研究和解析表达式

关于海岸破波带内悬沙浓度水平和垂向分布的研究对于计算海岸输沙率和地形演变具有重要意义。本研究进行了规则波、波群和不规则波三种波浪情况破波带内悬沙浓度的水平和垂向分布的试验测量。试验在大尺度波浪水槽进行,接近实际海岸波况尺度。给出了破波带内多断面悬沙垂向分布的细致测量结果,并以此为基础给出了预报实际海岸破波带内悬沙浓度水平和垂向分布解析表达式,讨论了形成这些分布的物理原因和不同波况、不同破波带区域对分布的影响。     

椭圆度-凹坑双缺陷海底管道局部屈曲特性研究

海底管道在制造、埋设以及使用过程中极易产生椭圆度-凹坑双缺陷,双缺陷影响管道局部屈曲,对含椭圆度-凹坑双缺陷海底管道的局部屈曲特性研究十分必要。现行规范中采用等效椭圆度对含椭圆度-凹坑海底管道进行评估,该方法无法准确评估不同缺陷形式的屈曲特性。采用形状系数对含椭圆度-凹坑双缺陷的海底管道进行评估,运用有限元软件ABAQUS进行数值模拟,并进行试验验证。在此基础上对含有不同凹坑深度、不同椭圆度的海底管道进行局部屈曲的数值模拟,计算不同形状椭圆度、含有不同凹坑深度海底管道的形状系数,对其进行敏感性分析。计算结果表明:形状系数对海底管道椭圆度、凹坑深度、径厚比敏感性较强;对凹坑宽度敏感性较弱。     

Bearing capacity of offshore umbrella suction anchor foundation in silty soil under varying loading modes

Considering the current disadvantages of present offshore wind turbine foundations, a novel anchor foundation with skirt and branches is proposed, called offshore umbrella suction anchor foundation (USAF). A series of experiments and numerical simulations were performed to explore the bearing capacity of the USAF under various kinds of loading modes. The bearing characteristics and the anchor–soil interactions are described in detail for horizontal static loading, horizontal cyclic loading, and an antidrawing (pullout) test in silty soil. In the static loading test, the load–deflection of the anchor under step loading was analyzed and the normalized curve of the load–deflection was obtained to determine the ultimate horizontal bearing capacity of the anchor under normal working conditions. Under horizontal cyclic loading, the relationship between the plastic cumulative deformation and cyclic number was determined. In addition, the responses of USAF were investigated for a low wave frequency and storm surges. In the drawing test, it was found that a “segmentation phenomenon” occurred during the test. Moreover, a method to identify the maximum antidrawing load of USAF was provided based on dynamic mechanics. The numerical results show that the use of anchor branches and skirt can enhance the bearing performance of USAF to a certain degree. However, the anchor branch has a slight positive influence on the bearing performance improvement. The USAF is not only similar to a stiff short pile, but a rotation occurs. The failure envelope under composite loading (V-M) was obtained and the changes associated with changes in the aspect ratio of the internal compartment were clarified.     

深水海底管道铺设安全辅助系统

此次研发的铺管安全辅助系统是一套自动化、简易化、旨在提高安装经济性和安全性的实时运行安全辅助系统,通过实时数据采集及处理,达到对安装期海管强度进行实时监测目的。系统组成包括设备系统和监测软件两部分。设备为系统提供辅助决策数据源;监测软件采用C++语言编写,用于数据接收、解析,并通过OrcaFlex API调用商业有限元软件OrcaFlex为分析内核进行实时分析计算,以可视化界面输出管道应力、应变、触地点等信息,给予船上作业人员安全指导,及时作出决策。     

纳米 Fe2O3-SnO2 光催化降解海水养殖废水中的氨氮

通过共沉淀法制备纳米Fe_2O_3-SnO_2光催化剂,采用XRD、SEM等测试手段对其进行形貌、物象、粒径一系列的表征,研究结果显示制得的催化剂仍保持纯SnO_2四方金红石型结构.研究了Fe_2O_3-SnO_2光催化剂投加量、Fe_2O_3与SnO_2物质的量比、煅烧温度、煅烧时间、氨氮初始浓度、p H值、H2O2浓度以及光照反应时间等因素对海水养殖废水中氨氮降解效率的影响.在紫外光照射下进行正交实验,确定最优化反应条件:催化剂投加量为0.4 g/dm3,煅烧时间为3 h,物质的量比为1∶2,氨氮初始含量为50 mg/dm3,光照反应时间为2 h.这5个因素对Fe_2O_3-SnO_2光催化氧化速率影响的大小程度依次为:Fe_2O_3与SnO_2物质的量比煅烧时间Fe_2O_3-SnO_2光催化剂投加量氨氮初始浓度光照时间.氨氮去除率可以达到85.1%,相同条件可见光下也可达到82.3%.