深空探测巡视器视觉导航定位方法研究与地面试验场验证

地外天体表面巡视器就位探测是深空探测研究的重要手段,其自主导航定位能力是任务开展的重要前提。本文主要对视觉导航方法中的视觉同时定位与地图构建(SLAM)方案开展应用研究。介绍了当下经典的视觉SLAM框架,并以具有代表性的ORB-SLAM3算法为例开展研究;分别利用公开数据集、深空探测地面模拟场数据进行试验验证,探索视觉导航定位算法在深空探测场景下的有效性。本文研究为我国后续开展长距离连续巡视任务提供参考。     

从地球测绘到地外天体测绘

随着人类空间探测技术的不断发展,月球与深空探测已成为测绘遥感科学与技术的前沿和新战场。在多类型深空探测任务的驱动下,测绘遥感技术也得到了新的发展。本文结合国内外深空探测的各类任务,对地外天体环绕遥感测图、着陆导航遥感避障、巡视环境感知与视觉导航定位方面的研究现状和成果进行了系统总结;结合未来月球与深空探测任务需求,对深空遥感测绘技术的发展,包括地外天体海量全球遥感数据智能处理、全球控制网精化、月球南极精细三维形貌测绘、多传感器融合的着陆导航避障和巡视环境感知与定位等进行了探讨。     

低应变反射波法在岩溶地区灌注桩检测的初步探讨

根据基桩低应变反射波法的基本原理,结合低应变反射波法在岩溶地区灌注桩检测工程实例,对岩溶地区灌注桩检测的经验进行总结。     

基于科学知识图谱的水文化变迁研究方法探析简

Cultural transformation (including knowledge innovation, ideological emancipation and slogan publicity, etc.) is one of the most important drivers of changes in water management policies. Earlier studies into water culture were mainly based on qualitative methods. However, using only qualitative methods, it is difficult to reveal the stage characteristics of water culture evolution objectively and accurately. Mapping knowledge domains, a rising knowledge discovery method, can holistically reveal the sources of knowledge and the laws of its development. This paper is devoted to exploiting its potential as a quantitative method for researches targeting at water culture evolution. By extracting the key words related to water from People’s Daily, knowledge domains on water culture evolution in China during 1946 2012 are mapped and interpreted, based on which the water culture evolution is unveiled. By comparing the water culture evolution with changes in water policies, stages of water resource development and extreme hydrological events, it is found that there exist clear relationships. This convinces us that mapping knowledge domains could play an effective role in quantitative research on water culture evolution. Further steps towards better quantitative researches on water culture evolution using this method include the enhancement of the universality of newspapers, improvement on the accuracy of key words extraction, and increase in the precision of visualization analysis.     

湘中印支期关帝庙岩体地球化学特征及成因

关帝庙岩体位于湘中盆地,据年龄资料可分为中三叠世末和晚三叠世中期两个形成时期。中三叠世花岗岩中发育闪长质暗色微粒包体,自早至晚依次为细中粒角闪石黑云母花岗闪长岩、细中粒斑状角闪石黑云母二长花岗岩、细-细中粒(斑状)黑云母二长花岗岩。晚三叠世花岗岩自早至晚依次为细中粒-粗中粒斑状二云母二长花岗岩、细粒二云母二长花岗岩。岩石高硅、富铝、高钾,(Na2O+K2O)含量为6.80%~8.87%,平均7.74%;K2O/Na2O比值在1.35~2.66之间,平均为1.58;ASI值为0.99~1.40。总体属镁质、高钾钙碱性系列过铝质花岗岩类。中三叠世花岗岩Ba、Nb、Sr、P、Ti表现为明显亏损,Rb、(Th+U+K)、(La+Ce)、Nd、(Zr+Hf+Sm)、(Y+Yb+Lu)等则相对富集。中、晚三叠世花岗岩ΣREE含量为121.60~197.56μg/g,平均为158.70μg/g;δEu值0.28~0.68,平均为0.53;(La/Yb)N值为5.94~17.53,平均13.80。中三叠世花岗岩ISr值为0.71302~0.71758,εSr(t)值为121~186,εNd(t)值为-9.95~-8.74,t2DM为1.72~1.82Ga。C/MF-A/MF图解显示源岩主要为碎屑岩、少量基性岩和泥质岩。地质地球化学特征表明,印支期关帝庙花岗岩属S型花岗岩,形成于碰撞-后碰撞构造环境。     

新疆山区低层云水资源时空分布特征

采用云与地球辐射能量系统(CERES)2003～2007年的CERESSSF Aqua MODIS云资料,选取新疆阿尔泰山、天山和昆仑山三大山区,通过考察云量和云液态水柱含量分析了低层云水资源的多年空间分布和季节变化特征。结果表明,三大山区多年平均的云量年平均区域值在24.4%～27.5%之间,云液态水柱含量在51～56.3g/m2之间。三大山区低层云量和云液态水柱含量有明显的季节变化特征。综合云量和云水柱含量来看,春季是三大山区低层云量资源最丰富的季节,冬季是三大山区低层云中的含水量最丰富的季节。     

半参数平差模型参数的两步估计

考虑半参数平差模型L=Bx+S+Δ,xεRd,S为未知回归参数,为未知Borel函数。本文首先利用自然样条函数法,找到符合条件的非参数自然样条插值函数。其次利用偏残差法并综合最小二乘法,导出了参数和非参数的解算公式,讨论了窗宽参数的选取方法。在本文的最后,将这种估计方法应用到重力场的计算中,说明了利用半参数平差模型估计参数的有效性。     

BLLac天体ON231的光变周期研究

从大量文献中收集了BLLac天体ON231光学B波段约100年的观测数据,在此基础上分析了光变周期。用两种不同的方法（Jurkevich方法和小波分析法）分析周期光变,发现其光变曲线中存在13．6±1．5及26．1年的周期。     

The connections between bulk Lorentz factor,black hole mass and accretion in Fermi FSRQs

We have analyzed a large sample of FSRQs detected by Fermi LAT. Our main intents are to investigate the relations between bulk Lorentz factor and black hole mass, between bulk Lorentz factor and Eddington ratio. Using archive and calculation, we obtained the distributions of bulk Lorentz factor, black hole mass and Eddington ratio. After excluding redshift effect, there is still significant correlation between bulk Lorentz factor and black hole mass, but not correlation between bulk Lorentz factor and Eddington ratio, which suggest that faster jets have a close relation with more massive black holes, and the Blandford–Znajek (BZ) mechanism may dominate over the Blandford–Payne (BP) mechanism for Fermi FSRQs.     

The evolutionary sequence of Fermi blazars

Using γ-ray data (α _γ , F _γ ) detected by Fermi Large Area Telescope (LAT) and black hole mass which has been compiled from literatures for 116 Fermi blazars, we calculated intrinsic γ-ray luminosity, intrinsic bolometric luminosity, intrinsic Eddington ratio and studied the relationships between all above parameters and redshift, between α _γ and L _γ . Furthermore, we obtained the histograms of key parameters. Our results are the following: (1) The main reason for the evolutionary sequence of three subclasses (HBLs, LBLs, FSRQs) may be Eddington ratio rather than black hole mass; (2) FSRQs occupy in the earlier, high-luminosity, high Eddington ratio, violent phase of the galactic evolution sequence, while BL Lac objects occur in the low luminosity, low Eddington ratio, late phase of the galactic evolution sequence; (3) These results imply that the evolutionary track of Fermi blazars is FSRQs ? LBLs ? HBLs.