共查询到19条相似文献，搜索用时 296 毫秒
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提出了一种精确测定数码相机投影中心位置的方法,详细介绍了其工作原理和实施方法。利用Metro In经纬仪三坐标测量系统和Metro In-DPM数字工业摄影测量系统的高精度测量特点,提高了控制点坐标测量精度、控制点标志中心像点坐标量测精度并实现了相机的高精度标校。在一个试验里完成了高精度相机标校和投影中心位置精确测定,实现的投影中心位置测定精度优于5 mm。 相似文献
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对经纬仪工业测量系统应用于亚毫米级的大型工件的测量 ,提出了一种快速坐标转换的方法。利用定向参数作为坐标转换参数 ,导出了在统一坐标系下点位坐标的计算公式 ,并对转换后的坐标进行了精度分析。 相似文献
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针对利用数字照相天顶望远镜(DZT)测量地球自转参数中确定测站的瞬时天文坐标和国际地球参考架(ITRF)下的精确坐标问题，该文利用国家授时中心2017—2021年在丽江等多个台站的观测样机的长期测量数据，通过对分布在不同位置的多个测站的数据解算，分析了不同测站的坐标测量精度及对UT1测量的精度影响。基于2017—2021年的观测数据，进行DZT测量的精度分析。结果表明：几个测站的长期测量精度相近，天文经度长期测量标准差约为0.05 as,纬度方向为0.03 as,对UT1测量影响小于3.5 ms,该结果可为DZT测量ERP提供精确的初始坐标值。 相似文献
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简要介绍了以航线为单元,通过相位平滑递推算法在航求解双差载波相位观测量整周相位模糊度,进而确定各摄站空间位置的无初始化ＧＰＳ动态定位原理,对某测区一组实际航摄资料进行ＧＰＳ数据处理和ＧＰＳ辅助光束法区域网平差,证实所介绍的算法是正确的、有效的、所获取的ＧＰＳ摄站坐标可满足空中三角测量的精度要求,并且用该数据与经初始化ＧＰＳ动态定位获取的ＧＰＳ摄站坐标数据进行ＧＰＳ辅助光束法区域网平差的总体精度是完全一致的。 相似文献
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地球参考框架是一切测绘活动、地球科学研究的物理基础。目前,地球参考框架常采用长期解的形式,即利用一组全球分布的基准站在某一参考历元的坐标和速度来表示。由于观测有误差,且各基准站又具有非线性变化,故需要对不同历元的瞬时地球参考框架进行累积,形成稳定的长期参考框架。以不同历元观测数据得到的瞬时参考框架成果为输入,构建了一种基于多历元观测数据建立参考框架长期累积解的融合模型。从坐标转换模型和测站坐标的时变模型出发,详细推导了建立长期解的函数模型,依据该函数模型的秩亏数设计了转换参数的内约束基准。采用2010-08—2014-12的国际全球导航卫星系统服务第2次处理结果进行试算,并与国际地球参考框架2014成果进行了对比。结果表明,X、Y、Z方向标准偏差分别为3.45 ?mm、4.04 mm、2.84 mm,速度精度分别为1.53 mm/a、1.46 mm/a、1.21 mm/a,X、Y、Z方向的加权均方根误差优于3 ?mm。 相似文献
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施工期平整度测量对地坪施工质量的控制与评估具有重要意义。采用靠尺或水准仪的传统地坪平整度测量方法存在测点稀疏、效率低等不足,难以适应超大地坪施工期平整度快速、精细的测量需求。提出了一种全站仪与惯性导航系统（inertial navigation system,INS）融合的平整度快速测量方法,通过卡尔曼滤波融合全站仪和INS数据,解算小车运动轨迹,根据轨迹点的高程计算平整度指标,发明研制相应的测量设备,应用于2022年北京冬奥会国家速滑馆冰面混凝土基底施工期平整度检测。实验结果表明,所提方法精度与水准仪相当,而测量效率显著提高,不仅能对地坪施工期整体平整度质量进行评估,而且可以对平整度异常进行检测和定位,为地坪的磨平工作提供指导,具有良好的工程价值。 相似文献
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多边交会系统利于提高激光跟踪仪坐标测量精度,但测量精度易受测站布局和系统参数标定精度的影响。引入球心拟合的无定向点系统参数标定法,避免传统系统参数标定精度受定向点分布的影响,根据无定向点系统参数标定模型推导出多边交会的最佳测站布局——直角正三棱锥,从而保证多边交会测量精度。仿真结果表明,在5 m范围内,球心拟合的无定向点系统参数标定中误差为0.006 4 mm,最佳测站布局下多边交会的点位中误差为0.005 mm。经标准尺长度测量验证和四面体标准器坐标测量验证,优化后多边交会的长度测量中误差为0.003 6 mm,坐标测量中误差为0.005 3 mm。在无定向点系统参数标定和直角三棱锥布局下,激光跟踪仪多边交会能够实现微米级三维坐标测量。 相似文献
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A new and comprehensive method is presented that can be used for estimating eccentricity vectors between global positioning system (GPS) antennas, doppler orbitography and radiopositioning integrated by satellites (DORIS) antennas, azimuth-elevation (AZ-EL) very long baseline interferometry (VLBI) telescopes, and satellite laser ranging (SLR) and lunar laser ranging (LLR) telescopes. The problem of reference point (RP) definition for these space-geodetic instruments is addressed and computed using terrestrial triangulation and electronic distance measurement (EDM) trilateration. The practical ground operations, the surveying approach and the terrestrial data processing are briefly illustrated, and the post-processing procedure is discussed. It is a geometrically based analytical approach that allows computation of RPs along with a rigorous statistical treatment of measurements. The tight connection between the geometrical model and the surveying procedure is emphasized. The computation of the eccentricity vector and the associated variance–covariance matrix between an AZ-EL VLBI telescope (with or without intersecting axes) and a GPS choke ring antenna is concentrated upon, since these are fundamental for computing the International Terrestrial Reference Frame (ITRF). An extension to RP computation and eccentricity vectors involving DORIS, SLR and LLR techniques is also presented. Numerical examples of the quality that can be reached using the authors approach are given. Working data sets were acquired in the years 2001 and 2002 at the radioastronomical observatory of Medicina (Italy), and have been used to estimate two VLBI-GPS eccentricity vectors and the corresponding SINEX files. 相似文献
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全球导航卫星系统(global navigation satellite system,GNSS)技术在大坝、桥梁、滑坡等形变监测领域应用广泛。针对传统监测方法需要架设基准站、导致监测成本增加的问题,提出一种基于虚拟参考站的GNSS变形监测方法,利用连续运行参考站(continuously operating reference stations,CORS)观测数据,生成虚拟参考站(virtual reference station,VRS)代替实体参考站,实现高精度变形监测。利用中国云南省屏边苗族自治县约30处滑坡监测点进行实验分析,结果表明,当CORS基准站间距小于40 km时,双差对流层和电离层延迟模型内插精度优于10 mm,利用观测时长大于8 h的数据,可以实现平面精度优于5 mm、高程精度优于10 mm的形变监测。 相似文献
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Xavier Collilieux Laurent Métivier Zuheir Altamimi Tonie van Dam Jim Ray 《GPS Solutions》2011,15(3):219-231
The International GNSS Service (IGS) contributes to the construction of the International Terrestrial Reference Frame (ITRF)
by submitting time series of station positions and Earth Rotation Parameters (ERP). For the first time, its submission to
the ITRF2008 construction is based on a combination of entirely reprocessed GPS solutions delivered by 11 Analysis Centers
(ACs). We analyze the IGS submission and four of the individual AC contributions in terms of the GNSS frame origin and scale,
station position repeatability and time series seasonal variations. We show here that the GPS Terrestrial Reference Frame
(TRF) origin is consistent with Satellite laser Ranging (SLR) at the centimeter level with a drift lower than 1 mm/year. Although
the scale drift compared to Very Long baseline Interferometry (VLBI) and SLR mean scale is smaller than 0.4 mm/year, we think
that it would be premature to use that information in the ITRF scale definition due to its strong dependence on the GPS satellite
and ground antenna phase center variations. The new position time series also show a better repeatability compared to past
IGS combined products and their annual variations are shown to be more consistent with loading models. The comparison of GPS
station positions and velocities to those of VLBI via local ties in co-located sites demonstrates that the IGS reprocessed
solution submitted to the ITRF2008 is more reliable and precise than any of the past submissions. However, we show that some
of the remaining inconsistencies between GPS and VLBI positioning may be caused by uncalibrated GNSS radomes. 相似文献
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The paper presents the results of crustal deformation, as evidenced by changed station coordinates, in the Tokyo metropolitan area detected by the satellite laser ranging (SLR) technique. The coordinates of two Key Stone SLR stations, Tateyama and Kashima, were determined from 4 weeks of orbital arcs of the LAGEOS-1 and LAGEOS-2 satellites with respect to 16 SLR stations kept fixed in the ITRF2000 reference frame. The station coordinates were calculated using the NASA GEODYN-II orbital program. The orbital RMS-of-fit for both satellites was 16 mm. The standard deviation of the estimated positions was 3 mm. A jump of about 5 cm in the baseline length between the Kashima and Tateyama stations was detected in June–August 2000 by VLBI and GPS techniques. This work confirms this crustal deformation as determined by SLR and vice versa. Analysis of coordinates of these stations shows that this effect was caused by a 4.5-cm displacement of the Tateyama station in the north-east direction. The change in the vertical component was not significant. 相似文献
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In geodetic and geophysical applications of GPS, it is important to realize the ephemerides of the GPS satellites and the coordinates of station positions in a consistent reference system. At present, more than one reference system is being used by various GPS users depending on their specific applications. The WGS-84 and various reference frames based on satellite laser ranging (SLR), very long baseline interferometry (VLBI), or a combination of SLR and VLBI are the most commonly used in high precision geophysical applications. The WGS-84 is widely used in applications which rely on the GPS broadcast ephemeris. Station coordinates estimated in one system may have to be transformed to another for further use or for evaluation/comparison purposes. This paper presents a seven-parameter transformation between the WGS-84 and SLR/VLBI reference frames. The GPS double-differenced phase measurements for two consecutive weeks from a set of five Defense Mapping Agency (DMA) sites (defined in the WGS-84 frame) and from an augmented set of fifteen CIGNET sites (defined in the SLR/VLBI frame) were processed in a least squares estimation scheme to determine station coordinates, from which the transformation parameters were determined. A scale difference of about 0.2 ppm and an orientation difference in longitude of about 31 milliarcseconds were found to be the only parameters of significance between the adopted SLR/VLBI and the WGS-84 frames. Transformation between WGS-84 and the ITRF90 is also included, in which the scale difference is the same as before but the longitude rotation is about 16 mas. 相似文献