利用参数独立分解的星载SAR干涉测量检校方法

在星载干涉合成孔径雷达中,干涉参数的准确性对高程精度起着至关重要的作用。传统干涉测量检校方法往往将影响量级不同的干涉参数组合在一起解算,无法精确获得每项干涉参数的修正量。针对此问题,本文提出一种利用参数独立分解的干涉测量检校方法。首先,根据三维重建模型,确定与干涉SAR测高有关的参数;随后,在确保几何参数精度的前提下,对干涉参数的敏感度进行定量分析;最后,采用独立检校算法解算每一项干涉参数误差,完成干涉测量检校模型的建立。本文选择陕西渭南区域4对TerraSAR-X/TanDEM-X数据进行了试验分析。结果表明,对于该试验数据,采用本文提出的参数独立分解方法,干涉测量检校后干涉结果的高程精度优于2.54 m,平原地区获取DEM的绝对高程精度优于1.21 m,山地地区获取DEM的绝对高程精度优于3.11 m,验证了本文方法的有效性和正确性,为我国平原及山区1∶25 000比例尺的干涉SAR地形图测绘提供了技术基础。     

Monitoring surface changes in discontinuous permafrost terrain using small baseline SAR interferometry,object-based classification,and geological features: a case study from Mayo,Yukon Territory,Canada

Permafrost-induced deformation of ground features is threating infrastructure in northern communities. An understanding of permafrost distribution is therefore critical for sustainable adaptation planning and infrastructure maintenance. Considering the large area underlain by permafrost in the Yukon Territory, there is a need for baseline information to characterize the permafrost in this region. In this study, the Differential Interferometric Synthetic Aperture Radar (DInSAR) technique was used to identify areas of ground movement likely caused by changes in permafrost. The DInSAR technique was applied to a series of repeat-pass C-band RADARSAT-2 observations collected in 2015 over the Village of Mayo, in central Yukon Territory, Canada. The conventional DInSAR technique demonstrated that ground deformation could be detected in this area, but the resulting deformation maps contained errors due to a loss of coherence from changes in vegetation and atmospheric phase delay. To address these limitations, the Small BAseline Subset (SBAS) InSAR technique was applied to reduce phase error, thus improving the deformation maps. To understand the relationship between the deformation maps and land cover types, an object-based Random Forest classification was developed to classify the study area into different land cover types. Integration of the InSAR results and the classification map revealed that the built-up class (e.g., airport) was affected by subsidence on the order of ?2 to ?4 cm. The spatial extent of the surface displacement map obtained using the SBAS InSAR technique was then correlated with the surficial geology map. This revealed that much of the main infrastructure in the Village of Mayo is underlain by interbedded glaciofluvial and glaciolacustrine sediments, the latter of which caused the most damage to human made structures. This study provides a method for permafrost monitoring that builds upon the synergistic use of the SBAS InSAR technique, object-based image analysis, and surficial geology data.     

Speckle observations with PISCO in Merate (Italy): XIV. Astrometric measurements of visual binaries in 2013 and new orbits for ADS 1097, 5871, 7203, 7775, 9378, 9578, and 11186

We present relative astrometric measurements of visual binaries made in 2013 with the speckle camera PISCO at the 102‐cm Zeiss telescope of Brera Astronomical Observatory, in Merate. Our observing list contains orbital couples as well as binaries whose motion is still uncertain. We obtained 134 new measurements of 129 visual binary stars, with angular separations in the range 0.≈23–5 and an average accuracy of 0.≈01. The mean error on the position angles is 0.°5. Most of the position angles were determined without the usual 180° ambiguity with the application of triple‐correlation techniques and/or by inspection of the long integration files. We also present new revised orbits for ADS 1097, 5871, 7203, 7775, 9378, 9578, and 11186, partly derived from PISCO observations. The corresponding estimated values for the masses of those systems are compatible with the spectral types. (© 2015 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)     

面向多基线干涉SAR高程反演的全局最优相干方法

本文针对多基线极化干涉SAR数据,提出了面向多基线干涉SAR高程反演的全局最优相干方法。该方法将多景全极化干涉影像联合在一起,构建多基线极化相干矩阵,由多基线最优相干准则指导,求解全局条件下的最优干涉图。该方法可以有效降低多基线干涉中散射中心不一致对干涉相位影响,从而提高干涉相位的精度和可靠性,并提高最终获取DEM的精度。利用国产X-SAR系统和德国E-SAR系统获取的多基线全极化数据进行全局最优相干方法试验,利用多基线极化最优相干方法生成全局条件下的最优干涉图,依据多基线高程反演方法计算目标高程,验证了本文提出的方法的有效性。     

自适应精致极化Lee滤波的复相干性估计方法

干涉相干性包含了极化SAR干涉测量(PolInSAR)中的极化和干涉信息,滑动窗口大小和滤波方法是准确估计干涉相干性的前提。本文以精致极化Lee滤波为基础,根据边缘检测和邻域相干性高低区分同质区域和异质区域,建立了自适应精致极化Lee滤波方法并估计相干性矩阵和干涉相干性。自适应精致极化Lee滤波能够根据边缘检测信息和邻域相干性高低程度调整滑动窗口大小并选择合适的估计方法,不仅提高了抑制斑点噪声的能力,而且保持了图像的边缘信息,有利于提高干涉相干性的估计精度。试验结果表明,该方法有效抑制了斑点噪声,较好地保持了SAR图像的边缘信息,有利于提高植被参数反演的精度。     

IBIS-L系统及其在大坝变形监测中的应用

主要介绍了地基合成孔径雷达,阐述了干涉测量成像系统IBIS-L的结构和基本原理,将IBIS-L系统应用于国内外几个大坝的变形计算与分析,获得了较为准确的大坝位移量,认为IBIS-L系统可以应用于大坝的变形监测,同时认为大坝变形监测时受大气的影响较大,如何有效地进行大气影响改正和提高IBIS-L技术的变形监测精度是值得深入研究的课题。     

GNSS-R反演海浪有效波高实验分析

阐述了基于GNSS-R技术利用干涉复数场（ICF）测量有效波高的技术原理以及方法。并对这种方法进行了实验,对实验结果进行了分析。实验结果得出：此方法所测得的结果随有效波高变化,与测波仪测得的波高比较一致,说明GNSS-R遥感测试有效波高方法可以作为一种低成本有效的测量有效波高的手段。     

Vertical coherency function model of spatial ground motion

Many studies have focused on horizontal ground motion, resulting in many coherency functions for horizontal ground motion while neglecting related problems arising from vertical ground motion. However, seismic events have demonstrated that the vertical components of ground motion sometimes govern the ultimate failure of structures. In this paper, a vertical coherency function model of spatial ground motion is proposed based on the Hao model and SMART 1 array records, and the validity of the model is demonstrated. The vertical coherency function model of spatial ground motion is also compared with the horizontal coherency function model, indicating that neither model exhibits isotropic characteristics. The value of the vertical coherency function has little correlation with that of the horizontal coherency function. However, the coherence of the vertical ground motion between a pair of stations decreases with their projection distance and the frequency of the ground motion. When the projection distance in the wave direction is greater than 800 meters, the coherency between the two points can be neglected.     

利用小波相干技术检测致密储层裂缝发育带

目前国内、外油气勘探已经进入岩性油气藏勘探阶段,其中致密碳酸盐岩或页岩油气勘探具有远大前景。这类致密储层中裂缝是油气储集的主要空间。用模拟地震子波的小波函数对原始三维地震数据体作小波变换,可以得到不同频带（分辨率）的地震数据体。分别对具有不同分辨率的三维地震数据体进行C3相干处理,其中低频相干体突出了断裂的信息,而高频相干体则突出反映了受断裂控制下的小断裂或裂缝的发育信息,通过合理的融合系数有选择地对C3相干数据进行融合,获得了能够高精度分辨裂缝发育特征的相干数据体,由此提高了裂缝检测和储层预测的精度。     

Micro-arcsecond Celestial Reference Frames: definition and realization - Impact of the recent IAU Resolutions

The adoption of the International Celestial Reference System (ICRS),based on Very Long Baseline Interferometry (VLBI) observations of extragalactic radiosources by the International Astronomical Union ...