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PROGRESS REPORT OF CNES ACTIVITIES REGARDING THE ABSOLUTE CALIBRATION METHOD

机译:关于绝对校准方法的CNES活动的进度报告

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Global Navigation Satellite System (GNSS) time and frequency transfer is among the most useful tools for comparisons of remote clocks. It represents the basis of the time laboratories contributions for the realization of Temps Atomique International (TAI). The GNSS reception chains (antenna, antenna cable, geodetic receiver), used currently to perform the time comparisons, must be calibrated periodically to ensure their accuracy and their long-term stability. The most widely approach used to determine the electrical delay and the time stability of these chains is the differential method developed by the BIPM. Since 2005, CNES (French Space Agency) has developed the absolute calibration, using artificial signals, which opens the possibility to calibrate independently each element of the reception chain with a low uncertainty. The time-delay uncertainties of receiver and cable are respectively about of 0.40 ns and 0.050 ns for k=1. Recently, our efforts have mainly focused on the behavior of several receivers (Ashtech Z12-T, Septentrio PolaRx2, and Dicom GTR50) and a GNSS signal simulator (Spirent 4760) according to the temperature and the hygrometry variations. The first results of this study have been presented during the last EFTF meeting. At the present time, we have a good comprehension of the behavior of investigated receivers and the simulator according to the environment where they are located. Since 2009, the absolute calibration investigations have mainly concerned the last element of the reception chain, the GNSS antenna. Through this paper, we give a progress report of the CNES activities relating to the absolute calibration. First of all, it displays the variations of the internal electrical delay of some devices (several receivers and a simulator) according to the temperature, the hygrometry, and the aging. The antenna calibration procedure is then described.
机译:全球导航卫星系统(GNSS)时间和频率传输是远程时钟比较的最有用的工具之一。它代表了实现Temps Atomique International(TAI)的时间实验室贡献的基础。目前用于执行时间比较的GNSS接收链(天线,天线电缆,大地测量接收器)必须定期校准,以确保其准确性和长期稳定性。用于确定这些链的电延迟和时间稳定性的最广泛的方法是由BIPM开发的差分方法。自2005年以来,CNES(法国空间局)使用人工信号开发了绝对校准,这使得能够独立地校准接收链的每个元件,具有低不确定性。接收器和电缆的时间延迟不确定性分别约为0.40ns和0.050ns的k = 1。最近,我们的努力主要集中在若干接收器(Ashtech Z12-T,Septentrio PolarX2和DICOM GTR50)和GNSS信号模拟器(螺旋4760)的行为上的特征在于温度和湿法变化。在最后一次EFTF会议期间,这项研究的第一个结果已经呈现。目前,我们对调查接收器和模拟器的行为进行了良好的理解,根据它们所在的环境。自2009年以来,绝对校准调查主要涉及接收链的最后一个元素,GNSS天线。通过本文,我们提供了与绝对校准有关的CNES活动的进度报告。首先,它根据温度,湿度测定和老化显示一些设备(多个接收器和模拟器)的内部电延迟的变化。然后描述天线校准程序。

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