Correction Method of Antenna Pointing Error Caused by the Main Reflector Deformation

The pointing accuracy of a radio telescope is usually less than one-tenth of its antenna beam width. For large-aperture antennas at the short-centimeter band or millimeter-wave band, the pointing accuracy must be as high as several arc seconds. Therefore, for large-diameter and high-frequency reflector antennas, the pointing problem has become an important focal point to realize the antenna performance. Among many structural subsystem factors that affect the antenna pointing accuracy, there has been only less study on the factor of main reflector deformation. Based on the structural characteristics of the antenna, a reflector space coordinate system is established in this paper. And based on the space coordinates of the main reflector surface points after deformation, a non-linear least squares fitting method with 3 degrees of freedom is proposed to accurately predict the antenna pointing. Finally, the space geometric relationship is used to strictly derive the precise adjustments on the elevation and azimuth in order for correcting the antenna pointing error, and the indirect relationship between the main reflector deformation and the pointing error is constructed. This has certain guiding significance for improving the pointing accuracy of large radio antennas.     

银川地震台CTS-1数字地震仪震级校正初探

主要分析讨论了2002年1月~2005年2月银川台数字地震仪测定的震级与中国数字地震台网观测报告震级的误差,给出银川台CTS-1数字地震仪震级的校正值,以提高银川台地震速报的精度。同时初步探讨分析了银川台数字地震仪震级误差的原因。     

多波束测深波束脚印位置归算模型研究

推导了多波束测深脚印位置归算模型,通过与CARIS软件进行实例比对,验证了该模型的有效性。在数据处理过程中,采用时标序列检索的方式处理导航时间延迟,取得了良好的效果;采用条带姿态进行姿态改正避免了"杠杆"旋转对边缘波束深度的影响。实例比对表明,该模型结果与CARIS软件输出结果一致。     

敦煌壁画计算机存贮与管理信息系统研究

该研究以０４５号窟为例，应用近景摄影测量、数字图象处理、色度学和信息系统理论和技术方法，以现有的仪器设备为基础，对洞窟内壁画、塑象等进行近景摄影测量、图象几何纠正和彩色失真矫正，建立了可操作的“敦煌壁柬计算机存贮与管理信息系统”。为敦煌英高窟壁画、逆象等文物图象数据永久保存、修复、还原和进一步开发研究等提供服务。     

A geotechnical correction for post-depositional sediment compression: examples from the Forth valley,Scotland

Fine-grained sediments usually suffer post-depositional compression (compaction), which reduces bed thickness and lowers the elevations of sample positions and marker horizons. This reduction has been calculated for two general cases using geotechnical theory, and a correction (decompaction factor) is presented that can be applied to many field situations. Its use is illustrated by two examples from the clay sediments of the Claret Formation of the Forth valley. In the first, the correction is calculated for ¹⁴C samples from the Bothkennar research site near Grangemouth, and the effect on the reconstruction of water depths is discussed. In the second example, corrections are obtained for published sea-level index points from former shorelines in the Forth valley, using a method for a postiori estimation of geotechnical data. General conclusions are drawn between the size of the correction and the sample position relative to the local depocentre. Some applications to palaeotidal modelling are also suggested. © 1998 John Wiley & Sons, Ltd.     

西河水文站水准点稳定性分析

西河水文站设置有4个水准点,均埋设在冲击层地区。在该地区设置的水准点,即便严格执行《国家一、二等水准测量规范》(GB/T12898-2006)规定的埋石深度和尺寸标准,也很难认为它们是稳定不变的。利用西河水文站1999~2016年8次水准点高程校测成果,采用结点法,对4个水准点的稳定性指标进行分析计算,以期解决西河水文站水准测量工作中引据点选择的随意性,保证用稳定的水准点作为水准测量的引据点,达到既节约测量时间,又提高测量精度的目的。     

电感耦合等离子体质谱法测定高锡地质样品中的痕量镉

应用电感耦合等离子体质谱法(ICP-MS)测定地质样品中的痕量镉,存在多种质谱干扰,通常采用在线或离线方程进行校正,当样品中含锡较高时,采用传统固定系数校正方程,易导致测定结果有明显偏离,甚至结果出现负数。本文针对含高锡的地质样品,应用ICP-MS测定其中的镉,采用氢氟酸-高氯酸-硝酸敞开酸溶消解、硝酸浸提体系处理样品,通过测定~(111)Cd、~(113)Cd、~(114)Cd同位素,研究了干扰元素Sn、In、Zr、Mo对镉测定的影响。结果表明镉与干扰源浓度变化呈非简单的正相关性。①同质异位素Sn或In产生的干扰增值Δ(~(114)Cd/~(114)Sn或~(113)Cd/~(113)In)随干扰源浓度增大逐渐变大,~(114)Sn对~(114)Cd的干扰系数在0.0272～0.0222,~(113)In对~(113)Cd的干扰系数在0.0670～0.0412;②Zr和Mo在测定条件下形成氧化物和多原子复合离子物质对Cd均产生不同程度的质谱干扰。通过测定与样品中干扰源浓度相近的单一标准溶液产生的Cd干扰值,经在线修正干扰系数(γ),建立了精确的校正方程。该方法经标准物质验证,准确度高,相对标准偏差在6.57%～9.94%(n=7),方法检出限为0.03mg/kg,达到了地质分析检测要求,为高锡地质样品中的痕量镉分析提供了依据。     

High‐Precision Cd Isotope Measurements of Soil and Rock Reference Materials by MC‐ICP‐MS with Double Spike Correction

This study presents a high‐precision Cd isotope measurement method for soil and rock reference materials using MC‐ICP‐MS with double spike correction. The effects of molecular interferences (e.g., ¹⁰⁹Ag¹H⁺, ⁹⁴Zr¹⁶O⁺, ⁹⁴Mo¹⁶O⁺ and ⁷⁰Zn⁴⁰Ar⁺) and isobaric interferences (e.g., Pd, In and Sn) to Cd isotope measurements were quantitatively evaluated. When the measured solution has Ag/Cd ≤ 5, Zn/Cd ≤ 0.02, Mo/Cd ≤ 0.4, Zr/Cd ≤ 0.001, Pd/Cd ≤ 5 × 10^?5 and In/Cd ≤ 10^?3, the measured Cd isotope data were not significantly affected. The intermediate measurement precision of pure Cd solutions (BAM I012 Cd, Münster Cd and AAS Cd) was better than ± 0.05‰ (2s) for δ^114/110Cd. The δ^114/110Cd values of soil reference materials (NIST SRM 2709, 2709a, 2710, 2710a, 2711, 2711a and GSS‐1) relative to NIST SRM 3108 were in the range of ?0.251 to 0.632‰, the δ^114/110Cd values of rock reference materials (BCR‐2, BIR‐1, BHVO‐2, W‐2, AGV‐2, GSP‐2 and COQ‐1) varied from ?0.196‰ to 0.098‰, and that of the manganese nodule (NOD‐P‐1) was 0.163 ± 0.040‰ (2s, n = 8). The large variation in Cd isotopes in soils and igneous rocks indicates that they can be more widely used to study magmatic and supergene processes.     

天宫二号三维成像微波高度计大气斜距时延校正

2016-09-15随天宫二号空间实验室发射升空的三维成像微波高度计（简称天宫二号成像高度计）是国际上第一个采用小入射角、短干涉基线实现宽刈幅海面高度测量的高度计。由于天宫二号没有为成像高度计配备用于大气校正的微波辐射计,因此需要采用模型方法对大气时延进行精确估计。传统高度计采用星下点观测,通常只考虑大气折射率的改变引起传播速度变化的时延。天宫二号成像高度计采用偏离星下点1°—8°的小角度观测,因此在进行大气传输时延校正时不仅要考虑雷达信号传播速度的改变,还应考虑由于传播方向改变带来的路径弯曲效应。本文针对天宫二号成像高度计的观测几何特性,提出基于数值天气模型校正大气斜距时延的算法：采用欧洲中期天气预报中心的天气数据和大气分层模型,通过气象参数计算大气折射率;根据高度计参数和各层大气折射率,依赖折射定律和信号传播的几何关系在路径上逐层积分,计算大气斜距时延的估值。通过对天宫二号成像高度计的陆地角反射器定标实测数据进行处理,经大气斜距时延校正后,角反射器的剩余距离误差的标准差约为6.2 cm,达到厘米量级的斜距测量精度,验证了在不同入射角情况下,所提出的大气斜距时延校正算法的有效性和可靠性。