武汉基准台超导重力仪重力潮汐观测结果

本文采用重力残差信号对武汉基准台超导重力仪的原始观测数据（２０秒采样）作预处理，将原始观测信号分解成重力潮汐和残差两部分，在残差信号中消除一些已知的干扰因素的影响。利用ＥＴＥＲＮＡ软件作调和分析，两主波（Ｏ１和Ｍ２）的重力潮汐参数（振幅因子和相位滞后）为：Ｏ１：１．１７８８±０．０００６，－０．５９７５°±０．０２８°；Ｍ２：１．１７１３±０．０００２，－０．５８７３°±０．００８°经海潮改正以后，Ｏ１和Ｍ２波的潮汐参数与Ｗａｈｒ－Ｄｅｈａｎｔ潮汐模型值相比，振幅因子的偏差优于０．１％。     

JX—3解析测图仪上航测高倍放大成图的试验

介绍试用１：３３０００比例尺航测资料，在ＪＸ－３解析测图仪上高倍放大航测１：１０００比例尺地形图的成图方案和应采取的技术措施，运用 解析法模型绝对定向的原理，在全野布点时采用两种方案对照比较，进行理论和试验精度的分析，并给出试验结果。     

从Lacoste－Romberg重力仪零位移特性的分析论提高观测精度的途径

零位校正误差是重力仪除标定以外最主要的误差来源.本文根据作者数年来从事高精度重力勘探工作中所积累的资料,对此问题进行了较为全面客观的分析研究.(l)对Lacoste-Romberg重力仪的正常零位变化和零位突变特性提出了分析结论;(2)对实测资料采用动、静分高处理方法,分析了重力仪连续工作时(数日至数十日)由于零位非线性变化可能引起的零位校正误差;(3)通过对实测资料的分析计算,得到了零位突变对重力仪观测精度影响的参考值;(4)针对重力仪使用中的实际问题提出了改善零位移线性度的实施对策.     

疏散星团NGC2244天区恒星的绝对自行研究

利用上海天文台相隔35年的两期照相底片资料,测定了疏散星团NGC2244所在天区55’×55’范围内495颗恒星基于Tycho-2星表的位置和绝对自行,并对自行精度作了初步分析。     

西边界流在边界“豁口”的形变及其机制

大洋西边界流在边界豁口处由于失去边界的支持而发生形变。本文将西边界流视为一种惯性射流，遵循绝对涡度守恒原理，推导了流轴及其两侧流体在西边界豁口处不同形式的弯曲，发现在一定的豁口尺度条件下，西边界流自身的相对涡度分布特点和地球旋转的β效应决定了在失去西侧陆坡支持时，其主体会沿反气旋路径发生一段经向的位移而圈回入射点所在的经度位置。主轴变形的经向尺度与初始速度及西边界流的入射角度有关；主轴西侧可能会出现一小部分分支进入邻近的内海并形成气旋或反气旋式环流；主轴东侧的流体则在豁口以东沿反气旋路径弯曲，从而论证了西边界豁口处形成西边界流弯曲的可能性和原因     

GPS单点测速技术在海浪测量中的应用研究

分析比对了GPS单点测速技术与其他已有测波手段的不同,讨论了基于多普勒频移的GPS测速方法,并分析了各类误差对测速精度的影响。分别利用原始多普勒值和导出多普勒值进行了静态测速试验和动态测速试验,将导出多普勒测速结果与RTK（RealTimeKinematic,实时动态测量系统）位置差分测速进行了比测。结果表明,使用静态数据采用高频导出多普勒值测速的精度可以达到亚厘米级每秒,而采用原始多普勒观测值进行测速因接收机型号的不同,结果差异较大;动态测速试验中,采用导出多普勒测速的方法与RTK位置差分测速的符合精度可达cm／s。     

Loading effect of a self-consistent equilibrium ocean pole tide on the gravimetric parameters of the gravity pole tides at superconducting gravimeter stations

The gravimetric parameters of the gravity pole tide are the amplitude factor δ, which is the ratio of gravity variations induced by polar motion for a real Earth to variations computed for a rigid one, and the phase difference κ between the observed and the rigid gravity pole tide. They can be estimated from the records of superconducting gravimeters (SGs). However, they are affected by the loading effect of the ocean pole tide. Recent results from TOPEX/Poseidon (TP) altimeter confirm that the ocean pole tide has a self-consistent equilibrium response. Accordingly, we calculate the gravity loading effects as well as their influence on the gravimetric parameters of gravity pole tide at all the 26 SG stations in the world on the assumption of a self-consistent equilibrium ocean pole tide model. The gravity loading effect is evaluated between 1 January 1997 and 31 December 2006. Numerical results show that the amplitude of the gravity loading effect reaches 10⁻⁹ m s⁻², which is larger than the accuracy (10⁻¹⁰ m s⁻²) of a SG. The gravimetric factor δ is 1% larger at all SG stations. Then, the contribution of a self-consistent ocean pole tide to the pole tide gravimetric parameters cannot be ignored as it exceeds the current accuracy of the estimation of the pole tide gravity factors. For the nine stations studied in Ducarme et al. [Ducarme, B., Venedikov, A.P., Arnoso, J., et al., 2006. Global analysis of the GGP superconducting gravimeters network for the estimation of the pole tide gravimetric amplitude factor. J. Geodyn. 41, 334–344.], the mean of the modeled tidal factors δ_m = 1.1813 agrees very well with the result of a global analysis δ_CH = 1.1816 ± 0.0047 in that paper. On the other hand, the modeled phase difference κ_m varies from −0.273° to 0.351°. Comparing to the two main periods of the gravity pole tide, annual period and Chandler period, κ_m is too small to be considered. Therefore, The computed time difference κ_L induced by a self-consistent ocean pole tide produces a negligible effect on κ_m. It confirms the results of Ducarme et al., 2006, where no convincing time difference was found in the SG records.     

具有VRL8350静电反馈装置的拉科斯特重力仪性能的研究

1983年,美日科学家Harrison和Sato发展的一种静电反馈技术成功地用于拉科斯特流动重力仪,使这一技术迅速推广到世界各国。本文将讨论具有VRL 8350静电反馈装置的拉科斯特重力仪的线性问题,研究拉科斯特重力仪在非反馈和反馈条件下,仪器纵水泡对重力仪的灵敏度、固有周期和阻尼的影响。     

Time stability of spring and superconducting gravimeters through the analysis of very long gravity records

Long gravity records are of great interest when performing tidal analyses. Indeed, long series enable to separate contributions of near-frequency waves and also to detect low frequency signals (e.g. long period tides and polar motion). In addition to the length of the series, the quality of the data and the temporal stability of the noise are also very important. We study in detail some of the longest gravity records available in Europe: 3 data sets recorded with spring gravimeters in Black Forest Observatory (Germany, 1980–2012), Walferdange (Luxemburg, 1980–1995) and Potsdam (Germany, 1974–1998) and several superconducting gravimeters (SGs) data sets, with at least 9 years of continuous records, at different European GGP (Global Geodynamics Project) sites (Bad Homburg, Brussels, Medicina, Membach, Moxa, Vienna, Wettzell and Strasbourg). The stability of each instrument is investigated using the temporal variations of tidal parameters (amplitude factor and phase difference) for the main tidal waves (O1, K1, M2 and S2) as well as the M2/O1 factor ratio, the later being insensitive to the instrumental calibration. The long term stability of the tidal observations is also dependent on the stability of the scale factor of the relative gravimeters. Therefore we also check the time stability of the scale factor for the superconducting gravimeter C026 installed at the J9 Gravimetric Observatory of Strasbourg (France), using numerous calibration experiments carried out by co-located absolute gravimeter (AG) measurements during the last 15 years. The reproducibility of the scale factor and the achievable precision are investigated by comparing the results of different calibration campaigns. Finally we present a spectrum of the 25 years of SG records at J9 Observatory, with special attention to small amplitude tides in the semi-diurnal and diurnal bands, as well as to the low frequency part.     

大气重力信号的理论计算及其检测

基于标准大气定律和大气圆柱体分布模型,本文引进了大气重力格林函数,用离散格积方法求得了大气对重力场观测的影响,对台站高程、周围地形和地表温度变化等因素的影响问题进行了讨论．结果说明台站近区气压变化是大气重力信号的主要贡献者,考虑大气质量负荷引起的弹性地球形变效应后,对距台站0．5°的区域积分获得的大气重力导纳值为-0．3603μGal／hPa,占全球大气变化引起的总信号的90％以上,这一理论模型结果与超导重力仪实测结果相吻合,并能较有效地用于消除重力观测中的气压干扰成分．