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ACES microwave link requirements

机译:ACES微波链路要求

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摘要

Atomic Clock Ensemble in Space (ACES) is a project of the EuropeannSpace Agency on-board the future International Space Station (ISS). Thenpayload consists mainly of two atomic frequency standards, one spacenhydrogen maser (SHM) prepared by the Observatoire de Neuchateln(Switzerland), and one cold atom caesium clock called PHARAO prepared bynthe CNES (France), with the participation of the BNM-LPTF, the ENS-LKB,nand the CNRS-LHA. Because of the anticipated performances of thesenclocks on-board the ISS, the requirements of the links between thenpayload and the clocks on the Earth are at the limits of the knownnpotential of the optical or microwave techniques. The microwave linkn(MWL) requirements are described in this paper. Taking into account thencharacteristics of the ISS orbit, and fixing an arbitrary limit to thenadditional noise brought to the clock readings by the MWL, thencomputation of the required stability leads to two kinds ofnrequirements: the first one at the subpicosecond level over each singlencontinuous pass of the ISS above any Earth station, and the second onenat the level of one part in 1016 and below over a one day ornmore averaging period. Moreover, the ISS orbit parameters should lead tona knowledge of the ACES clock position at the m level, and of the ACESnclock speed at the mm/s level
机译:太空中的原子钟组(ACES)是欧洲航天局在未来的国际空间站(ISS)上的一个项目。然后,有效载荷主要由两个原子频率标准组成,一个是由纳沙泰恩天文台(瑞士)准备的空间氢质激波(SHM),另一个是由法国国家科学与技术委员会(法国)准备的,名为PHARAO的冷原子铯钟,由BNM-LPTF参与, ENS-LKB和CNRS-LHA。由于ISS上时钟的预期性能,因此有效载荷与地球上时钟之间的链接的要求处于光学或微波技术的已知潜力的极限。本文介绍了微波链路(MWL)的要求。考虑到ISS轨道的特性,并固定一个任意限制,然后由MWL带到时钟读数的额外噪声,然后计算所需的稳定性会导致两种要求:第一个要求在皮秒级上的每次单次连续通过国际空间站上方的国际空间站,然后在一天或更长时间的平均时间内第二次到达1016年及以下部分的水平面。此外,国际空间站的轨道参数应使人们了解m级的ACES时钟位置,以及mm / s级的ACESnclock速度。

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