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星地无线电双向时间比对模型及试验分析 总被引：3，自引：0，他引：3
星地时间同步是卫星导航系统的一个关键技术,是实现卫星导航定位的基础.针对星地时间同步问题,讨论了一种星地无线电双向时间比对方法,详细推导了该方法中星地上下行伪距的归算模型,给出了星地钟差的实用计算模型.该方法通过上下行伪距求差.消除了对流层延迟,卫星星历误差和地面站站址坐标误差等共有误差影响,与信号频率有关的电离层延迟也被很大程度地削弱,从而大大提高了时间比对精度.最后,利用实测数据进行了试验分析,结果表明:星地无线电双向时间比对精度能够达到约0.34ns,验证了理论方法和模型的正确性. 相似文献
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多站联合星地时间同步及预报性能分析 总被引：1，自引：0，他引：1
无线电双向法通过上行与下行观测量比对实现星载钟与地面站时间同步,比对过程中消除或削弱了绝大多数的公共误差项,因此时间比对精度高。卫星不可视时该方法不能实施,此时卫星钟预报精度只能依赖卫星钟自身的物理性能,不可视弧长越长卫星钟预报精度衰减越快。为了削弱因卫星不可视带来的精度损失,多站联合星地时间同步是一种有效的解决方案。给出了多站联合星地时间同步的基本原理、推导了时间比对模型,并利用COMPASS实测数据分析了多站联合时间同步及预报性能,实验结果表明,多站联合观测有效延长了卫星的可视弧长,为提升卫星钟预报精度提供了数据基础。由于观测设备之间的系统性偏差,各站得到的星地钟差结果可能存在跳变,影响卫星钟预报精度。因此系统性偏差成为制约多站联合星地时间同步性能的关键性因素,系统性偏差的精确标定能确保多站联合星地时间同步及预报精度的大幅提升。 相似文献
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从1995年起,GPS 共视法时间比对技术成为用于国际原子时 TAI 归算中使用的一种主要时间连接手段。由于许多因素诸如 SA 对 GPS 共视比对精度的影响.BIPM 一直在建议使用其它具有ns 准确度潜力的时间传递手段,比如“GLONASS 共视法时间比对”和“卫星双向法时间比对”等手段。当前国际上装备 GLONASS 系统并进行常规共视比对的实验室主要有8个:DLRL(德国)、LDS(英国)、SU(俄罗斯)、VSL(荷兰)、NIST 和 USNO(美国)、CRL(日本),当然还有 BIPM。 相似文献
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分析了在卫星双向时间频率传递中,由地面站间钟差和卫星运动引起的双向几何路径不对等导致的双向几何路径时延差对双向时间比对计算结果的影响。选取了3颗卫星（中卫1号、北斗3G、IGSO70）和3组地面站（北京-成都、北京-喀什、北京-三亚）组成的9条卫星双向时间频率传递链路作仿真计算。对于这9条链路,仿真结果显示：1）当两地面站间钟差在1μs～10 ms范围内时,通过GEO卫星比通过IGSO卫星的双向不对等几何路径时延之差对双向时间比对计算结果的影响（τ值）较小;2）假设地面站间钟差在1 ms内时,通过 GEO卫星的卫星双向时间比对链路所对应的τ值均在皮秒量级,一般可忽略;通过 IGSO 卫星的卫星双向时间比对链路所对应的τ值均在纳秒量级,一般不可忽略。 相似文献
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中国科学院国家授时中心在全国范围内部署建设了卫星地面观测系统,利用该系统可以进行C波段卫星双向时间频率传递(TWSTFT);TWSTFT是目前国际上远程时间频率标准之间比对精度最高的比对手段之一,但是如何验证TWSTFT的性能,仍是目前研究的难点;为验证该系统TWSTFT的性能,设计了三站闭合方法,在3个站点间两两进行TWSTFT,根据两组比对结果推算第3组比对结果,与第3组实测结果的偏差反映了卫星双向时间传递的精度,最后用实际试验结果对卫星双向时间传递的性能进行了分析;该实验结果表明两两进行TWSTFT得到的三站闭合差数据均优于1 ns。 相似文献
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基于北斗卫星导航载波相位共视(BDS CP(CV))时间传递模型,使用IGS多GNSS试验先导项目(MGEX)提供的精密轨道和钟差产品,研究分析GEO,IGSO和MEO 3种北斗在轨卫星进行时间传递的不确定度。实验结果表明:相对于双向卫星比对结果和光纤比对结果,基于IGSO载波相位时间传递结果的标准差较好,相对于双向卫星比对结果,西安—长春观测数据比对结果的标准差中IGSO较好,可以达到0.39 ns;相对于光纤比对结果,西安—临潼观测数据比对结果的标准差中IGSO较好,可以达到0.18 ns;基于GEO和IGSO的载波相位时间传递结果的稳定度比基于MEO的较好。 相似文献
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We have carried out multi-station TV observations since 1994 in order to determine the orbit of the Arietid daytime meteor
stream. In 1999, one possible Arietid meteor was recorded by our simultaneous observations and its orbit was determined. In
2003, two Arietid meteors were observed from two stations of our observing site, those orbits were determined precisely, the
orbital elements were in good agreement with each other. This is the first time that determination of the precise orbit of
the Arietids has been made from optical observations. The orbit of these Arietid meteors, and comparison with the orbit obtained
from radar observations are discussed. 相似文献
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The goal of all time laboratories’ pursue is to produce and keep a stable, precise and reliable time scale. The long-term stability of the time scale is mainly taken into account in the traditional ALGOS algorithm, while the local atomic time scale should give consideration to both the long-term and shortterm stabilities. From the analysis and research on the atomic clock noise model and under the condition that the long-term stability of the local atomic time scale does not drop, a complete algorithm is proposed which is suitable for the calculation of the local time scale TA (NTSC) carried out at the time laboratory with the time-keeping clocks of a unitary type and being close in performance at the National Time Service Center, called the NTSC for short, of Chinese Academy of Sciences. The data of all the clocks in the NTSC which participated in the calculation of the International Atomic Time (TAI) all the year round in 2008 are applied to the test and verification of the new algorithm, with the result showing that both the short- and long-term stability indexes of the obtained TA (NTSC) are improved. The research result is suitable for the calculation of the atomic time scale of the time laboratory whose time keeping system is similar to that of the NTSC. 相似文献
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We present fast algorithms used in IKI and IFSI for the analysis of the Martian spectra measured in the Planetary Fourier Spectrometer (PFS) experiment onboard Mars Express orbiter. The first algorithm is based on a new very general and precise approach applicable to planetary atmospheres with quite arbitrary absorption and scattering properties. The method is aimed at the simulation of high-resolution planetary spectrum in a broad spectral region with computational expenses typical to two-stream algorithms and a precision close to that of time consuming exact methods. The basic idea is to compute first a required quantity with an approximate method and then to evaluate a correction to the first approximation with just a few runs of a precise code in representative spectral channels. The correction is built as a function of the first-approximation quantity itself. The necessary input to the radiative transfer—monochromatic gaseous opacity—was evaluated by means of simple interpolation from pre-computed tables. As far as the algorithm deals with monochromatic quantities, its applications are limited to direct and even inverse problems that require the exact treatment of scattering and the absence of small-scale distortions of the spectrum. The second of the presented algorithms, based on the interpolations of the convolved transmission functions, is designed to be used in inverse problems that need a very fast evaluation of the synthetic spectrum over a broad spectral region. Performances of both methods are considered. 相似文献
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讨论利用全球定位系统 (GPS)共视观测数据 (GGTTS格式 )测定接收机天线坐标的原理和方法 ,采用此方法 ,发现日本国家计量研究院 (NRLM )、墨西哥国家计量院 (CNM )、土耳其国家计量院 (UME)在进行TAIGPS共视观测时采用的GPS接收机天线坐标存在明显偏差。经坐标偏差改正后 ,日本国家计量研究院与日本通信综合研究所 (NRLM CRL)、墨西哥国家计量院与美国国家标准、技术研究院 (CNM NIST)、土耳其国家计量院与法国巴黎天文台 (UME OP)的比对精度分别由 1 8.6ns、7.0ns、2 83.0ns提高到 3.0ns、4 .5ns、4 .7ns。 相似文献
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G. S. Kurbasova G. N. Shlikar 《Bulletin of the Crimean Astrophysical Observatory》2009,105(1):135-139
A study of the Earth’s rotation in space reveals a complex pattern of variations in its orientation, the excitation mechanisms of these variations, and their manifestations in various natural processes. The Earth’s rotation rate is not constant but exhibits complex fluctuations that account for some fraction of 108 (corresponding to variations of several milliseconds (ms) in the length of the day). These variations span a wide spectrum of time scales, from hours to centuries or longer, reflecting the fact that they are produced by a wide variety of geophysical and astronomical processes. We discuss the results of our statistical comparison of long series of observations to reveal the most coherent variations. The spectral composition of the experimental time series has been determined using modified periodogram and single-channel autoregression methods. A comparative analysis has been performed by a two-channel autoregression spectral estimation method. The results of our comparison of the time series suggest that the fluctuations with periods of about 73 years are highly coherent. 相似文献
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The ground based full disk velocity Doppler measurements used in helioseismology suffer from an atmospheric noise component when the sky transparency is not perfect. It is due to the non uniform integration of the line of sight component of the solar rotation produced by the differential atmospheric extinction across the direction of the solar equator. A simple two-channel differential photometer is proposed for measuring this differential extinction. The first laboratory tests of this instrument show that it has the capability of performing the required correction without adding a significant level of new instrumental noise contribution.
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Cryogenic detectors have a long history of success in the field of rare event searches. In particular scintillating calorimeters are very suitable detectors for this task since two signals are induced by a particle interaction in a scintillating crystal. The thermal signal provides a precise measurement of the deposited energy while the simultaneously measured scintillation light signal yields particle discrimination as the amount of produced scintillation light depends on the nature of the interacting particle. We investigate the calorimetric properties and background rejection capabilities of two large CsI (undoped) crystals (∼122 g each) operated as scintillating calorimeters at milli-Kelvin temperatures. Furthermore, we discuss the feasibility of this detection approach towards a future background-free dark matter experiment based on alkali halide crystals, with active particle discrimination via the two-channel detection. 相似文献
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由单颗脉冲星定义的脉冲星时受多种噪声源的影响,其短期和长期稳定度都不够好.为了削弱这些噪声源对单脉冲星时的影响,可以采取合适的算法对多个单脉冲星时进行综合得到综合脉冲星时,从而提高综合脉冲星时的长期稳定度.文中介绍4种综合脉冲星时算法:经典加权算法、小波分析算法、维纳滤波算法和小波域中的维纳滤波算法,将这4种算法分别应用于Arecibo天文台对两颗毫秒脉冲星PSR B1855+09和PSRB1937+21观测得到的计时残差并作出比较. 相似文献
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LAGEOS卫星精密定轨及残差分析 总被引：6，自引：2，他引：6
介绍LAGEOS卫星用卫星激光测距(SLR)资料精密定轨和在精密定轨基础上的残差分析处理．SLR资料的分析处理方法、采用的力学模型和解参数的多少根据目标的不同而不同．对不同的方案进行了详细分析、比较．其关键是对LAGEOS卫星进行精密定轨．得出了目前上海天文台在SLR资料的分析处理中已采用的解算模式．作为例证，该解算模式分析处理了1998年12月31日至1999年6月29日LAGEOS卫星的SLR资料，得到每3天一个弧段的精密轨道．结果显示每3天一个弧段的定轨残差rms都小于2厘米．上海天文台从1999年10月1日开始了全球LAGEOS—l和LAGEOS—2资料的快速分析服务，结果可从APSG的网址：http：／／center．shao．ac．cn／APSG／result获得． 相似文献
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由单脉冲星定义的脉冲星时受几种噪声源的影响,为削弱这些影响得到一种更稳定的时间尺度,采取将多颗脉冲星定义的单脉冲星时进行综合的分析方法得到综合脉冲星时．用两种方法:经典加权算法和小波分解算法,对PSRB1855 09和PSR B1937 21两颗脉冲星进行综合计算并做出比较,经典加权算法无法兼顾脉冲星不同频率上的稳定度,而用小波分析的方法对PSR B1855 09和PSR B1937 21两颗脉冲星进行综合,能够有效抑制不同频率上噪声的影响,达到更好的效果． 相似文献