New developments in space geodetic research: VLBI observations to space probes and GNSS remote sensi

来源 :2014年大地测量研究进展学术研讨会 | 被引量 : 0次 | 上传用户:fantasy1998
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
  Space geodetic techniques such as the GNSS, VLBI, SLR/LLR, and DORIS have reached a high quality level with respect to the classical applications in geodesy such as precise determination of station positions and of the Earth orientation parameters.Two research activities at GFZ are presented which go beyond these standard applications.The goal of the first project briefly described here (called D-VLBI) is the realization of frame ties between the dynamic reference frames of space probes like satellites, spacecrafts, the Moon or other planetary bodies, the kinematically defined International Celestial Reference Frame (ICRF) consisting of precise coordinates of extragalactic radio sources (radio galaxies or quasars), and the International Terrestrial Reference Frame (ITRF) realized on Earth.This can be done best by using the differential Very Long Baseline Interferometry (method, connecting a space probe to a close-by quasar by alternately observing signals of those two sources.In the research project D-VLBI a general concept for future applications of VLBI measurements to space probes will be developed.The benefit of observing GNSS satellites by VLBI radio telescopes is investigated by simulations.It is well known that the troposphere is the main error source of VLBI.It was found that changing the observation interval and entering additional observations to quasars in order to increase the sky coverage for each station are proper means to reach the expected accuracies of a few millimeters 3D station root mean square (rms).In addition we briefly review the innovative GNSS remote sensing activities at GFZ.Ground and space based (radio occultation) atmosphere sounding was pioneered by GFZ scientists since several years and reached an operational application level.Best example for this development is the routine use of atmospheric GNSS data products to improve regional and global weather forecasts of the leading weather centres, which was started in 2006.The GNSS atmospheric data are also widely used by a large, international user community of geodesists, atmospheric scientists and climate researchers.The importance of the related GNSS data products will increase during the next years with the upcoming new GNSS systems, the larger GNSS ground networks and the continuously increasing number of GNSS occultation receivers at Low Earth Orbiting satellites.In the recent years the international research focus in GNSS remote sensing was more and more focused on the GNSS reflectometry, which complements the atmosphere sounding techniques.Geophysical parameters of water, ice and land surfaces can be derived using the GNSS reflectometry.Several successful ground and airborne experiments demonstrated already the large potential of this innovative space geodetic technique for Earth Observation.Recently also first dedicated satellite based experiments are in preparation.However more international research work and cooperation is necessary to develop the GNSS reflectometry onto a similar application level as the GNSS atmosphere sounding.
其他文献
针对GNSS反演大气可降水量的Askne-Nordius(AN)模型和李延兴提出的水汽转换模型,使用中国地区探空资料和NCEP全球2010年再分析资料进行实验.结果表明使用天顶静力学延迟反演水汽的AN模型和使用天顶干延迟反演水汽的李延兴模型的平均偏差分别为-0.4mm和-0.1mm,并且李延兴模型的相对偏差明显小于AN模型.最后通过误差分析发现可降水量绝对偏差主要受其大小的影响,而可降水量相对偏差
对于天气预报来说水气扮演着相当重要的角色,藉由观测水气的分布,有助于评估天气系统的变化,因此利用GPS讯号穿过大气层的天顶向湿延迟量(zenithal wet delay,ZWD),进而计算大气可降水量(preeipitable water vapor,PWV),对于掌握特定天气现象具有相当大的帮助.本研究利用分为5区的台湾100个GPS连续观测站,计算2006-2011年间每小时一笔之ZWD数据
GNSS-R(GNSS-Reflectometry)遥感是利用导航卫星的反射信号对地物进行遥感.已经应用于海洋遥感,近期应用于土壤湿度和植被遥感,但主要从实验角度出发进行研究.本文以后向PO(Physical-Optics model)和MIMICS(Michigan Microwave Canopy Scattering Model)模型为基本工具,在其双站散射模型的基础上,根据极化合成的方法,
采用精密定轨同时获得北斗星载原子钟差数据进行稳定性分析时,由于星载原子钟钟差数据中粗差、更换参考钟等因素的影响,使得稳定度计算结果与真实结果偏离较大,不能正确反映原子钟的稳定水平.基于此,本文设计了一种上下限约束的方法剔除粗差、对更换参考钟造成的频率跳变进行平移,减小了这些异常数据对频率稳定度的影响,通过对实际数据的处理表明,北斗星载原子钟的天稳处在10-13-10-14水平.
为规避GPS等国外卫星导航系统动态偏航姿态控制模式中的地影机动以及正午和午夜机动,北斗IGSO/MEO卫星采用了动态偏航和零偏航两种姿态控制模式.本文通过对卫星姿态及受照的分析,查找由于姿态变化所造成的卫星光压摄动力变化的转换点,比较两种姿态控制模式下光压摄动力的差异,梳理其产生机制,为北斗卫星轨道确定提供技术支持.
军用潜艇水下导航主要采用无源自主的惯性导航系统,但惯导系统的导航定位误差随航行时间累积,使得单一的惯导系统在远程/长时下很难提供精确的导航位置信息.惯导/重力组合导航技术是当前实现潜艇高精度无源自主定位的重要手段,本文在借鉴和吸收国内外最新研究成果的基础上,通过理论分析、仿真试验、海上验证以及系统研制等方面,对重力匹配辅助惯性导航定位所涉及的多项关键技术进行了深入的探讨,提出应进一步提高海洋重力场
捷联式航空重力测量系统与平台式系统相比具有体积小、重量轻、功耗低等许多优点,近些年来取得了显著的研究进展.本文给出了捷联式航空重力测量的两种算法模型:捷联式惯性标量重力测量(SISG)和旋转不变式标量重力测量(RISG)模型.利用中国首套捷联式航空重力仪SGA-WZ01在某海域的部分试验数据,对两种算法模型进行了比较分析,表明其一致性对于200s的滤波长度好于0.5mGal.同时,利用两组重复测线
We adopt the linearized Lagrangian equations of motion in the vector form.They govern time varying small elasto-gravitation disturbances away from the equilibrium of a spherical non-rotating and unifo
重力固体潮观测值的潮汐因子与理论预期通常相差很小,重力潮汐因子均在1.15-1.17附近小幅波动。钻孔体应变仪和分量钻孔应变仪记录的应变固体潮数据的潮汐因子同伸缩仪一样,由观测数据计算的M2波潮汐因子,大者2.70,小者仅0.07,数值同样十分离散。通过"中国数字地震观测网络"工程中40个分量钻孔应变观测站提供的观测数据,发现应变固体潮观测值各向强异性响应现象的发现过程.
引潮力位调和展开是固体潮研究的理论基础.根据完全规格化Doodson展开公式和面球谐函数展开公式,采用ELP2000-85月亮历书和Newcomb太阳历书,构建了适用于引潮力位解析展开的数据结构,基于MATLAB语言计算得到了包含21895项的完全规格化Doodson展开表和21372项的面球谐函数展开表,计算结果表明这两个表之间的符合程度随着截断值的减小而增加.