共查询到18条相似文献，搜索用时 410 毫秒
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高精度的卫星轨道确定是卫星应用的基础和保证,本文以新一代DORIS接收机观测数据DORIS 3.0的相位观测数据为基础,研究了相位观测数据与传统的DORIS距离变化率数据的转换方法,并以JASON-2卫星为例,基于卫星动力学定轨原理,分析了不同数据类型、不同定轨方案得到的卫星轨道精度.结果表明,1)利用3天弧段的DORIS 2.2格式距离变化率数据和数据文件提供的相位中心偏差改正,或者采用模型对天线相位中心偏差进行改正并同时对地面测站进行偏心改正时,两种方案得到的轨道三维位置精度基本一致,均优于8.7cm,说明新一代DORIS接收机相位中心稳定,变化较小,采用模型进行偏差修正完全能够满足定轨精度要求.2)采用3.0格式的DORIS数据以及天线相位中心偏差修正模型和地面测站偏心改正模型时,得到的卫星定轨精度略有降低,大约为9.2cm;SLR校核残差约为6.5cm(均方根误差).3)采用2.2和3.0两种格式的DORIS数据,利用不同的定轨方案对JASON-2卫星进行精密定轨,均可以达到2cm左右的径向定轨精度,不同的定轨方案对径向定轨精度的影响可忽略不计.因此,对于最关心卫星径向定轨精度的海洋测高卫星而言,采用本文的数据格式转换方法和定轨方案,完全可以满足其定轨任务需求. 相似文献
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井间电磁测井技术测量井间地层电磁波传播特性,通过正反演获得井间电阻率分布信息,由此揭示地层油气水的分布信息.井间电磁接收是井间电磁测井技术中一项重要内容,是开展井间电磁成像测井系统研制中必须攻克的难题之一.本文通过对比磁反馈与无磁反馈两种天线接收幅度与相位特性,发现磁反馈接收天线频带平稳无相位跳变点,相比无反馈天线具有明显优势.在磁反馈天线的基础上,本文分析不同天线磁芯、不同天线缠绕方式对天线幅频特性的响应,发现这些参数均对天线幅频特性有不同影响,为天线设计与研制提供参考设计参数.在接收天线研究的基础上,采用噪声匹配放大、1/f滤波、工频压制、数字锁相放大、相敏检波等软硬件处理技术,进一步降低噪声,提高接收精度和灵敏度.为有效开展井间同步发射与接收采集,采用高精度时间同步技术,提高同步与电磁波相位提取的精度.针对接收线路与系统中存在的误差,采用两距离井间电磁刻度方法进行压制.井间电磁接收样机研制完成后,分别在现场进行井下噪声测试、非金属套管井间、金属套管井间等系列井间电磁接收测量实验,研究与实验结果表明:本文所研究的井间电磁接收技术可实现500 m以上大井距和双层金属套管井间测量． 相似文献
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GPS测量的广泛应用 总被引：1，自引：0，他引：1
GPS测量是测量界关心的重要课题之一 ,为此全国测量技术大会也曾以此为题召开过多次研讨会。由于测量仪器的不断开发、改进和完善 ,GPS在防灾、建设和气象等领域的应用正逐步扩展。目前 ,国土地理院正在备置电子基准点 ,实时动态测量便成为中心话题。下面介绍包括将来 GPS的可能性在内的有关多种GPS测量应用的见解。1 下世纪 GPS测量展望基本测量中的 GPS测量始于 1992年的 2次基准点测量 ,1995年引进了临时基准点测量。目前 ,国土地理院以 2 5 km间距的均等密度在整个日本列岛布设了约 10 0 0个 GPS连续观测点 (电子基准点 )。这… 相似文献
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基于星载GPS的HY-2卫星高精度精密定轨模拟研究(英文) 总被引：2，自引：0，他引：2
HY-2卫星是我国第一颗测高卫星,其径向定轨精度要求厘米量级,搭载了星载GPS接收机。目前HY-2还处于测试阶段,没有公布观测数据。为了确定基于星载GPS的HY-2精密定轨流程及其定轨精度,本文模拟了HY-2卫星星载GPS观测数据,结果表明HY-2星载GPS天线每个历元至少观测7颗GPS卫星。给出了基于星载GPS的精密定轨流程,分别采用简化动力学方法和动态几何法进行了精密定轨实验。对于相位1mm和3mm随机误差的相位观测数据,简化动力学法和动态几何法定轨都能够实现厘米量级的径向精密定轨,几何法定轨精度略低于简化动力定轨。地球重力场模型是影响HY-2卫星精密定轨的重要因素,本文对不同阶次的重力场模型EIGEN2、EGM96、TEG4和GEMT3进行了简化动力学定轨实验,高于50阶次的重力场模型都能够实现厘米级径向精密定轨,主要原因在于大量的高精度星载GPS观测数据和重力场模型精度的提高。 相似文献
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LEO GPS观测已成为空间电离层研究重要手段之一,通过GPS双频观测值获取的TEC则是电离层探测的一个重要参量,为获取高精度TEC需估计和消除GPS接收机仪器偏差（DCB）.本文旨在探索一种全新的LEO GPS接收机仪器偏差的估计方法：基于电离层球对称的假设,利用CHAMP和COSMIC原始GPS观测数据,采用几何映射函数,通过最小二乘解算出GPS接收机仪器偏差.结果表明：(1)2008年1月份期间,通过上述方法解算的仪器偏差都较稳定,相比COSMIC网上发布结果,标准偏差都在0.6 ns以内;（2）COSMIC（轨道高度大约800 km）仪器偏差估计结果优于CHAMP（轨道高度大约400 km）的结果,原因为：对于不同轨道高度LEO GPS仪器偏差估计,其较高轨道高度的电离层球对称假设影响较小. 相似文献
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在电离层局部地区球对称假设下,推导了利用双频和单频无线电掩星观测数据,反演电离层电子密度剖面的两种方法. 双频反演的误差来自于载波相位的观测误差,单频反演误差则主要由伪距的观测精度决定. 由于载波相位测量精度比伪距测量精度高两个量级,因此双频反演的精度一般比单频反演的高些. 不过,两载波信号L1和L2之间的传播路径差异会给双频方法带来误差. 利用三维射线追踪的程序模拟的无线电掩星数据来评估这些方法,结果表明,反演出的电离层剖面与给定的模式电离层非常吻合,验证了两种方法的可靠性和准确性. 将这两种反演方法应用于处理实测的GPS/MET掩星观测数据,均能获取合理的电离层剖面信息. 且单频方法得到的反演剖面与双频方法相当一致, 这为利用LEO星载单频GPS接收机进行电离层掩星观测提供了理论基础. 相似文献
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N. DE VOOGD 《Geophysical Prospecting》1978,26(3):509-524
A finite realization of a discrete random noise process may be considered as a one-sided energy signal. Its phase property can then be described by means of the center position. The samples of such a realization are the components of a random signal vector and the center position is therefore a random variable. A statistical analysis shows that the expected value of the center position equals half the time duration of the realization. This implies that the Z-transform of the realization may be expected to have an equal number of poles and zeros inside and outside the unit circle. The standard deviation from the expected value of the center position is shown to depend on the time duration of the realization and on the autocorrelation of the process. It follows that, for processes that can be described by the convolution of a white series and a disturbance wavelet, the center position is independent of the phase property of the wavelet. A conclusion based on these results is that the homomorphic technique of wavelet estimation through cepstrum stacking must give questionable outcomes. Another conclusion is that the super-position of a realization of random noise on a minimum phase wavelet will in general give a mixed phase resulting signal. It is pointed out that schemes for the derivation of deconvolution filters do not take account of this phenomenon. 相似文献
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Karol Dawidowicz 《Studia Geophysica et Geodaetica》2018,62(1):38-56
It is well-known that the phase center of a Global Navigation Satellite System (GNSS) antenna is not a stable point coinciding with a mechanical reference. The phase center position depends on the direction of the received signal, and is antenna-and signaldependent. Phase center corrections (PCC) models of GNSS antennas have been available for several years. The first method to create antenna PCC models was the relative field calibration procedure. Currently only absolute calibration models are generally recommended for use. In this study we investigate the differences between position estimates obtained using individual and type-mean absolute antenna calibrations in order to better understand how receiver antenna calibration models contribute to the Global Positioning System (GPS) positioning error budget. The station positions were estimated with two absolute calibration models: the igs08.atx model, which contains typemean calibration results, and individual antenna calibration models. Continuous GPS observations from selected Polish European Permanent Network (EPN) stations were used for these studies. The position time series were derived from the precise point positioning (PPP) technique using the NAPEOS scientific GNSS software package. The results show that the differences in the calibrations models propagate directly into the position domain, affecting daily as well sub-daily results. In daily solutions, the position offsets, resulting from the use of individual calibrations instead of type-mean igs08.atx calibrations, can reach up to 5 mm in the Up component, while in the horizontal one they generally stay below 1 mm. It was found that increasing the frequency of sub-daily coordinate solutions amplifies the effects of type-mean vs individual PCC-dependent differences, and also gives visible periodic variations in time series of GPS position differences. 相似文献
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Very short baseline interferometry: assessment of the relative stability of the GPS stations at the Yebes Observatory (Spain) 总被引：1，自引：0，他引：1
Alvaro Santamaría-Gómez 《Studia Geophysica et Geodaetica》2013,57(2):233-252
Using a very short baseline interferometer, the relative stability of the YEBE and YEB1 GPS stations at the Yebes Observatory (Spain) is assessed. A baseline length bias of 1 mm was found between estimates from different observed frequencies due most likely to phase center errors resulting from antenna calibration uncertainties and/or phase center migrations caused by the electromagnetic coupling of antenna and monument. Also a bias of 0.5 mm in the vertical component of the baseline length was found between estimates from different cut-off elevation angles due to elevation-dependent errors as phase center and multipath. In addition to these biases, significant variations in the horizontal component of the baseline length were found, mostly in the form of a trend of ?0.45 ± 0.10 mm/yr and an annual oscillation of amplitude 1 ± 0.1 mm and phase 155 ± 5 (beginning of June). The annual oscillation showed a high correlation with ambient temperature variations. Bedrock thermal expansion seems not to be a significant contributor to the annual variation due to the excellent agreement between the phases of the baseline and temperature annual signals. Thermoelastic expansion of the station monuments, which are comprised of concrete pillars and buildings, driven by the sunshine heating, is likely the origin of this oscillation. Near-field multipath and phase center errors are also rejected as being the main contributor to the annual signal. Conversely, near-field multipath and phase center errors may significantly contribute together to the time-correlated noise content of the baseline time series at long periods (flicker noise amplitude of 1.2 ± 0.1 mm). This research provides thus an assessment of the GPS station stability at the Yebes Observatory, which may be extended to the level of station-dependent contamination of geophysical and geodetic studies (e.g., plate tectonics, surface loadings, local ties) when similar station installations on top of buildings are used. 相似文献
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在海上实施三维地震探测过程中,人工震源枪阵中心与船上GPS的距离及地震探测作业中的船行方向造成炮点实际位置与预设位置有一定偏差;自由落体投放的OBS由于海流的影响会偏离原定设计位置(投放点),因此,炮点与海底地震仪(OBS)的位置校正是三维地震结构研究中的基本环节.本文利用艏向信息校正了炮点位置;采用蒙特卡洛和最小二乘法方法对海底地震仪的位置进行了校正,并探讨了直达水波曲线特征.结果表明 OBS位置一般偏离设计点1 km左右,其误差范围在20 m以内,校正后的OBS记录剖面展示了真实的记录情况.该研究结果为下一步西南印度洋的三维层析成像研究提供了坚实数据基础,同时为今后南海的三维深部地壳结构探测提供经验与借鉴. 相似文献
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本文通过实例阐述前兆手段观测数据基本特性(平稳性、周期性和正态性)在地震前的差异,说明连续观测数据中包含平稳随机过程和非平稳随机过程;亦包含常态下的年变周期和非年变周期,非平稳随机过程和非年周期变化可能产生在地震前兆发育期,其特征与地震孕育进程有关,可用非参数轮次法和方差分析法加以检验。随机过程的特征量正态分布的标准离差用以衡量过程的分散程度,异常时段与正常时段的标准差,相差可达数量级,用统计参量值X~2能在一定信度下检验其是否超出了限界。可见它们是前兆识别的基础依据,在其基础上可进一步选择科学计算方法剖析资料。同时在莱以特准则(3σ)判别异常的基础上,讨论了格罗布斯准则和狄克松准则在常熟地震(M_s5.1)和南黄海地震(M_s6.2)短期和中短期异常判别上的应用。 相似文献