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Influence of atmospheric turbulence on planetary transceiver laser ranging

机译:大气湍流对行星收发器激光测距的影响

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In this paper we investigate the influence of atmospheric turbulence on the performance of the uplink of a planetary transceiver laser ranging system using a single photon detector. We numerically combine the influence of turbulence in the mean intensity profile variations, scintillation, beam-wander induced pointing errors and stochastic time-of-flight variations, using the Hufnagel-Valley turbulence profile to model the ground turbulence behavior. We map the intensity variations due to turbulence to variations in the probability distribution of the arrival time of the 1st photon in a laser pulse, which influences the range measurement error probability distribution. The turbulence models are applied to assess the influence on single-pass range accuracy and precision statistics, as well as the parameter estimation quality of a Phobos Laser Ranging (PLR) mission. The difference in range measurement error between weak and strong turbulence is 3-4 mm in a PLR concept. This indicates that turbulence is a potentially important contributor to the error budget of interplanetary laser ranging missions, which aim at mm-level accuracy and precision. The single-shot precision is weakly influenced by turbulence, but strong turbulence is found to cause a strong decrease in detected pulse fraction, reducing normal point precision. We show that a trade-off between range accuracy and precision must be made when selecting laser system parameters, considerations for which are influenced by atmospheric turbulence effects. By consistently operating at the single-photon signal strength level, accuracy variations can be largely removed, at the expense of normal point precision, due to the reduced detection probability. We perform parameter estimation of Phobos initial state and observation biases using simulated measurements with and without turbulence, using a daily periodic turbulence strength model. We show that the parameter estimation quality is degraded significantly below that of the turbulence-free case only in the presence of strong turbulence. This shows the existence of a limit of ground turbulence strength below which its influence on parameter estimation becomes negligible.
机译:在本文中,我们研究了大气湍流对使用单光子探测器的行星收发器激光测距系统的上行链路性能的影响。我们使用Hufnagel-Valley湍流剖面对地面湍流行为进行建模,将湍流对平均强度剖面变化,闪烁,波束漂移引起的指向误差和随机飞行时间变化的影响数值结合起来。我们将湍流引起的强度变化映射到激光脉冲中第一光子到达时间的概率分布中的变化,这会影响距离测量误差的概率分布。湍流模型用于评估对单程范围精度和精度统计数据的影响,以及对Phobos激光测距(PLR)任务的参数估计质量的影响。在PLR概念中,弱湍流和强湍流之间的距离测量误差之差为3-4 mm。这表明湍流可能是导致行星际激光测距任务误差预算的潜在重要因素,该任务的目标是毫米级的精度和精度。单次脉冲精度受湍流的影响较小,但发现强烈的湍流会导致检测到的脉冲分数的强烈下降,从而降低法线点精度。我们表明,在选择激光系统参数时,必须在范围精度和精度之间进行权衡,这些参数受大气湍流效应的影响。通过以单光子信号强度水平一致地进行操作,由于降低了检测概率,因此可以以法线点精度为代价,大大消除精度变化。我们使用每日周期性湍流强度模型,使用有无湍流情况下的模拟测量结果,对Phobos初始状态和观测偏差进行参数估计。我们表明,仅在存在强湍流的情况下,参数估计质量才大大低于无湍流情况下的质量。这表明存在地面湍流强度极限,在该极限之下,其对参数估计的影响可以忽略。

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