基于GPS双频原始观测值的精密单点定位算法及应用

本文提出一种基于GPS双频原始观测值的PPP算法,与基于消电离层组合观测值的传统PPP算法不同,新算法通过参数化站星视线方向的电离层延迟以消除其对PPP估值的不利影响;该新算法可以有效避免观测值组合过程所引起的观测数据噪声以及多路径效应被放大的不利影响;同时在利用扩展卡尔曼滤波模型进行未知参数的递归估计过程中,通过对大气延迟参数引入符合实际的约束,可以加快滤波收敛,提高参数估值的可靠性;视线方向电离层延迟可与其他未知参数同时估计得到,进而便于利用PPP技术进行精密电离层研究;此外,对于可能的模型误差（如码观测值粗差、相位观测值周跳等）,基于DIA的质量控制策略以消除或削弱其对参数估值的不利影响。利用实测数据对新算法在静态、低动态以及高动态定位应用方面的精度进行检验,结果表明,静、动态定位结果的外符合精度可分别达到1~2 cm和7~8 cm,验证了新算法的可行性和有效性。     

一种改进的混合差分实时GPS卫星钟差估计算法及其实现

提出一种改进的混合差分算法,实现实时GPS卫星钟差估计。算法实现过程主要采用4个解算步骤,最终生成播发至用户的实时钟差产品。利用全球分布的68个测站实时数据流进行GPS卫星实时钟差解算,并对2018-01-14～01-19的实时GPS卫星钟差产品采用2种方法进行检核:1)与IGS快速钟差产品比较;2)运用实时动态PPP结果检核。结果显示,基于改进的混合差分算法,利用实时数据流实现的GPS实时卫星钟差产品具备STD为0.15 ns、RMS为0.63 ns的精度,可提供实时cm级定位服务。     

Light rare earth element enrichments in ureilites: A detailed ion microprobe study

Abstract— This paper explores the possible origin of the light rare earth element (LREE) enrichments observed in some ureilites, a question that has both petrogenetic and chronologic implications for this group of achondritic meteorites. Rare earth element and other selected elemental abundances were measured in situ in 14 thin sections representing 11 different ureilites. The spatial microdistributions of REEs in C‐rich matrix areas of the three ureilites with the most striking V‐shaped whole‐rock REE patterns (Kenna, Goalpara, and Novo Urei) were investigated using the ion imaging capability of the ion microprobe. All olivines and clinopyroxenes measured have LREE‐depleted patterns with little variation in REE abundances, despite large differences in their major element compositions from ureilite to ureilite. Furthermore, we searched for but did not find any minor mineral phases that carry LREEs. The only exception is one Ti‐rich area (～20μm) in Lewis Cliff (LEW) 85400 with a major element composition similar to that of titanite; REE abundances in this area are high, ranging from La ? 400 × CI to Lu ? 40 × CI. In contrast, all ion microprobe analyses of C‐rich matrix in Kenna, Goalpara, and Novo Urei revealed large LREE enrichments. In addition, C‐rich matrix areas in the three polymict ureilites, Elephant Moraine (EET) 83309, EET 87720, and North Haig, which have less pronounced V‐shaped whole‐rock REE patterns, show smaller but distinct LREE‐enrichments. The C‐rich matrix in Antarctic ureilites tends to have much lower LREE concentrations than the matrix in non‐Antarctic ureilites. There is no obvious association of the LREEs with other major or minor elements in the C‐rich areas. Ion images further show that the LREE enrichments are homogeneously distributed on a microscale in most C‐rich matrix areas of Kenna, Goalpara, and Novo Urei. These observations suggest that the LREEs in ureilites most probably are absorbed on the surface of fine‐grained amorphous graphite in the C‐rich matrix. It is unlikely that the LREE enrichments are due to shock melts or are the products of metasomatism on the ureilite parent body. We favor LREE introduction by terrestrial contamination.     

非差非组合PPP-RTK:模型算法、终端样机与实测结果

智能驾驶、精密农业和无人机等新兴行业要求全球导航卫星系统(GNSS)提供更加快速、准确的导航定位服务。非差非组合PPP-RTK融合了精密单点定位(PPP)和实时动态定位(RTK)两者的优势,能灵活处理多频多模数据并实现区域广覆盖的快速高精度定位。然而,PPP-RTK仍处于技术研发阶段,产业化应用尚未完全成型。本文从理论到实践,构建了码分多址和频分多址非差非组合PPP-RTK模型,开发了相应的实时解算软件,并研制了一款终端样机。基于平均站间距为154 km的京津冀参考网估计的精密改正产品,将终端样机分别搭载在无人机、农机和跑车上,开展了实时动态定位试验。试验结果表明,PPP-RTK终端样机在3个场景下的模糊度首次固定时间分别为5、2和7 s,模糊度固定成功率分别为99.79%、99.14%和98.96%,水平和高程定位精度分别在1 cm和4 cm左右。试验结果证明了自研PPP-RTK终端样机能提供连续、可靠、高精度的定位服务。     

Hydrogen Isotopes of Glassy and Phyllosilicate Spherules in AI Rais （CR） and Orgueil （CI） Chondrites

The hydroxyl in phyllosilicate minerals is the most common occurrence of water in primitive meteorites.Direct hydrogen isotopic analysis of this water component using an ion microprobe has been made in some glassy or phyllosilicate spherules from the A1 Rais (CR) and Orgueil (CI) chondrites. The spherules from A1 Rais show largedeuterium excesses (δD= 200- 800‰) relative to terrestrial standards, whereas deuterium-enrichments in the spherules from Orgueil are much smaller (δD= 40- 130‰). The phyllosilicate spherules are products of aqueous alteration of glassy precursors. In A1 Rais the phyllosilicate spherules have relatively higher δD values than the glassy ones, indicating that water introduced during aqueous alteration was deuterium-enriched. The deuterium-enrichments in the phyllosilicate spherules from Orgueil could result from isotopic exchange under thermodynamic conditions within the solar nebula. The much larger δD excesses of the A1 Rais spherules, however, cannot be attributed to the similar process;instead, an interstellar origin needs to be invoked.     

Accurate Trace Element Reporting in Corundum: Development of Secondary Ion Mass Spectrometry Relative Sensitivity Factors

The attractive physical and chemical properties of corundum lend to this material’s importance in both its natural and synthetic forms. However, much of the quantitative work performed on this material is plagued by unknown inaccuracy as non‐matrix‐matched reference materials are used. To conduct accurate quantitative analysis using SIMS, matrix‐specific relative sensitivity factors (RSFs) were determined for eighteen trace elements in corundum using dose‐verified ion implants. The RSF values ranged from 2.56 × 10²² to 3.29 × 10²⁴ cm^‐1 with total combined uncertainty values ranging from 7 to 10%. The RSF values, which are related to ionisation potentials, showed trends consistent with expectations for an insulating oxide. The developed values were applied to calibrate reference materials for LA‐ICP‐MS and to study other natural and synthetic corundum samples. A measurement reference material calibrated for Mg, Si, Ti, V, Fe and Ga produced consistent results over ten sessions in 4 years with relative standard deviations per trace element of 5% or less, confirming the repeatability of our process. A key finding was that calibrating LA‐ICP‐MS with NIST SRM 610 and 612 glasses to analyse corundum resulted in under‐reporting trace elements Be, Ti, V, Fe, Co, Ni and Ga compared with using matrix‐matched reference materials.     

一种用于GPS整周模糊度OTF求解的整数白化滤波改进算法

提出一种用于整周模糊度OTF求解的整数白化滤波改进算法。该算法首先对整周模糊度的协方差矩阵进行整数白化滤波处理,以降低整周模糊度间的相关性,然后构造搜索空间来判定是否需要进行搜索。如果需要,则通过搜索来确定变换后的整周模糊度;如果不需要,则通过直接取整来确定整周模糊度,进而得到原始的整周模糊度和基线分量的固定解。初步试验结果显示,采用改进方法解算整周模糊度可以提高成功率和解算效率。     

火星探测器转移轨道的自主导航方法

针对火星探测巡航段轨道导航需求,结合不同的星载敏感器提出了一种基于太阳、地球、火星及恒星信息的火星巡航段自主导航方法。该方法根据导航天体的特点,在分析不同导航天体观测模型基础上,根据地球视线矢量和火星视线矢量的可观性,结合信息融合技术,建立了基于太阳、地球、恒星观测以及太阳、火星、恒星观测两种模式下的多源天体数据融合处理方案,实现了探测器位置与速度信息的实时估计。仿真结果表明,本文方法能够有效地利用多源导航天体观测信息,为巡航轨道提供高精度的导航结果,可满足火星探测巡航段任务要求。     

利用信息融合进行月球卫星自主导航

研究了绕月卫星自主导航方法,提出了由星敏感器、紫外月球敏感器和测高仪组成的多源信息组合导航方案。将Unscented Kalman滤波(UKF)应用于非线性导航系统,采用信息融合技术设计了相关的联邦滤波算法,实现了系统的信息互补,完成了卫星轨道的最优估计。利用数学仿真对这种导航系统的有效性进行了验证,并与基于扩展Kal man滤波(EKF)的信息融合算法进行了比较。仿真结果表明,所提出的UKF融合算法具有良好的稳定性,可进一步提高导航系统的精度。     

月球软着陆自主组合导航研究

针对惯性测量单元(IMU)存在误差积累的特点,提出了利用探测器上的光学敏感器,通过对预先选定的特征点的测量得出探测器的相对位置,根据这些光学导航信息再结合惯性导航输出轨迹,通过多模自适应滤波完成对IMU导航的修正。对整个导航系统的可观性进行了分析,并通过数值仿真验证了所提出的自主导航方法的可行性。