Characterization & consequences of GPS Rb clock lamplight variations

J. Camparo, V. Formichella, I. Sesia, G. Signorile, L. Galleani, P. Tavella
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引用次数: 2

Abstract

In the rubidium atomic frequency standard (RAFS), an rf-discharge lamp produces the device's atomic signal. As a consequence of the light-shift effect, variations in the lamplight's intensity result in variations in the RAFS' output frequency. While the basic physics of the light-shift is reasonably well understood, its operational implications for GNSS performance are only beginning to be fully appreciated. Here, we summarize results examining decade-long histories of on-orbit GPS RAFS lamplight variations. In addition to a deterministic variation that is well modeled by the sum of an exponential and linear trend, the stochastic variations appear to be of three types: lamplight jumps, repeating lamplight ramps, and non-stationary lamplight noise. Employing an estimated GPS RAFS light-shift coefficient, these variations can be used to infer lamplight-induced RAFS frequency variations.
GPS Rb时钟灯光变化的特征和后果
在铷原子频率标准(rfs)中,射频放电灯产生器件的原子信号。由于光移效应,灯光强度的变化导致RAFS输出频率的变化。虽然人们对光移的基本物理特性已经相当了解,但其对GNSS性能的操作影响才刚刚开始得到充分认识。在这里,我们总结了长达十年的在轨GPS RAFS灯光变化历史的结果。除了由指数和线性趋势的总和很好地模拟的确定性变化之外,随机变化似乎有三种类型:灯光跳跃、重复灯光斜坡和非平稳灯光噪声。利用估计的GPS RAFS光移系数,这些变化可以用来推断灯光引起的RAFS频率变化。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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