导航卫星用时钟监视和控制装置

D. Felbach, F. Soualle, L. Stopfkuchen, A. Zenzinger
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引用次数: 5

摘要

导航卫星有效载荷中的所有信号产生和传输频率通常来自单个10.23 MHz主时钟。在伽利略或其他导航系统当前有效载荷架构的情况下,该主定时参考(MTR)是在基于单个原子参考的时钟监控单元(CMCU)中合成的。为了实现这一目标,在当前的伽利略设计中,CMCU从两个铷原子频率标准(RAFS)和两个被动h -脉射(PHM)池中选择有源时钟,并从该源合成MTR。第二个原子钟保持在热冗余状态,并在CMCU内部监控其相对于活动时钟的相位漂移。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Clock monitoring and control units for navigation satellites
All signal generation and transmission frequencies in the payload of a navigation satellite are typically derived from a single 10.23 MHz master clock. In case of the current payload architecture of the Galileo or other Navigation System this Master Timing Reference (MTR) is synthesized in a Clock Monitoring and Control Unit (CMCU) based on one single atomic reference. To achieve this, in the current Galileo design the CMCU selects the active clock from a pool of two Rubidium Atomic Frequency Standards (RAFS) and two Passive H-Masers (PHM) and synthesizes the MTR from this source. A second atomic clock is kept in hot redundancy and monitored inside the CMCU for its phase drift against the active clock.
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