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arXiv 1405.1990gr-qc
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卡西尼引力实验中非引力加速度的模拟

Modelling the nongravitational acceleration during Cassini's gravitation experiments

O. Bertolami, F. Francisco, P. J. S. Gil, J. Páramos

摘要:

在本文中,我们提出了一个计算的卡西尼号探测器在其太阳合实验,从航天器模型获得的热产生的加速度。我们建立了一个热模型的车辆和执行蒙特卡罗模拟找到一个热加速度的主要组成部分的$(3.01 \pm 0.33) \times 10^{-9} {\rm m/s^2}$。该结果与通过多普勒数据分析进行的该效应的估计非常一致。

英文摘要:

In this paper we present a computation of the thermally generated acceleration of the Cassini probe during its solar conjunction experiment, obtained from a model of the spacecraft. We build a thermal model of the vehicle and perform a Monte Carlo simulation to find a thermal acceleration with a main component of $(3.01 \pm 0.33) \times 10^{-9} {\rm m/s^2}$. This result is in close agreement with the estimates of this effect performed through Doppler data analysis.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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