提高InSAR测量精度的研究

来源 :中国科学院大学 | 被引量 : 0次 | 上传用户:aboutt
下载到本地 , 更方便阅读
声明 : 本文档内容版权归属内容提供方 , 如果您对本文有版权争议 , 可与客服联系进行内容授权或下架
论文部分内容阅读
Synthetic Aperture Radar (SAR) Interferometry, usually referred to as InSAR or IFSAR, is the synthesis of conventional SAR.techniques and interferometry techniques in radio astronomy.It has enabled fine spatial resolution, wide coverage, and competitive accuracy measurements of ground deformations related to, e.g.,earthquake, volcano, and underground work.Such measurements are however affected by the atmosphere and the decorrelation noise.With an aim to improve the accuracy of InSAR measurements, this report investigates the ways to mitigate the effects from the atmosphere and the de correlation noise.  Firstly, using Shanghai as an example, this report analyze the characteristics of atmospheric effects in SAR interferogram.The results show that atmospheric effects in SAR interferograms are anisotropic, non-Gaussian and following approximately a power law distribution.The scaling exponents estimated show that the atmospheric signatures in all the interferograms are non-stationary but with stationary increments.It is estimated based on the estimated scaling exponents that external data with spatial resolutions as high as about 0.3 km, are required to determine and correct for over 90% of the atmospheric effects in the SAR interferograms.Based on the results, an elevation-dependent InSAR atmospheric correction model is developed.Test results over Mount Etna with data from 16 continuous GPS stations show that an improvement of about 27% can be achieved when applying the model.  Secondly, this report investigate the ways to mitigate the decorrelation noise with post-filtering.Two filters have been developed in this part.The first one is an improved version of the commonly used Goldstein filter, where a new noise-dependent filtering parameter is defined to replace the original constant filtering parameters.Very consistent results can be achieved when the improved Goldstein filter is applied to interferograms with different noise level.The second one is an extension of the one dimensional Vondrak filter, i.e., a two dimensional (2D) Vondrak filter.Test results show that the 2D Vondrak filter outperform some existing filters.
其他文献
我做了末任南京市社会局长南京市社会局,是中华民国首都的社会行政机构。社会部成立后,国民政府行政院议决,在省设社会处。故苏、浙、赣、鄂、川、闽、粤、滇、黔、陇、陕、
二十世纪书法美学理论中,“形式”无疑成为一个带有强烈“修辞的优势”的词语,以至于在当下泛化为“视觉效果”之类的外在感性表述。以“形式分析”为手段的书法教学,往往仅
学位
中子星是天文学的重要研究对象之一。中子星集四大基本相互作用于一身,为人们提供了非常极端的天文实验室。在中子星物理中,中子星的自转减慢机制、高的自行速度的来源、超强磁
中南地区党史宣传教育协作会议于2000年5月24日至27日在湖南省衡阳市举行。河南、广东、广 西、湖北、湖南五省(区)党史期刊代表出席了会议。会议还特邀《中共党史研究》杂志社参加。中
本文对太阳高能粒子进行了研究。工作主要包括:筛选太阳23周以来120个较大质子事件,构建由相关X射线耀斑、射电暴、CME和质子流强组成的数据样本。对这些事件按强度进行分类,研
<正>谈及类型学摄影,必谈贝歇夫妇(贝恩德&#183;贝歇,1931-2007;希拉&#183;贝歇,1934-;均为德国人)。1960年代中期,当代艺术开始崛起,左翼思潮在欧洲风行一时,和其他艺术形式
随着客观世界的变化 ,马列主义也在不断发展。高校的思想政治工作必然地要加强和改进。据此 ,文章提出高校基层党组织思想政治工作的功能、思想政治工作的主体和载体及其当前
博士三年期间,我的工作重点是研究星系的形成与演化,分别研究了不同类型超新星的宿主星系性质和近邻宇宙中低面亮度星系的形成和演化,对这两类星系的形成和演化有了进一步的理解
赛弗特星系NGC4151是一个离我们最近(当哈勃常数取75 km s-1Mpc-1时,红移为0.00332,距离为13.2 Mpc)和最亮的赛弗特1型星系之一。NGC4151的寄主星系是一个典型的旋涡星系SABab(