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Analysis of an extended Pioneer 10 and 11 data set

机译:分析扩展先锋10和11数据集

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A previous JPL study of Doppler tracking data from Pioneer 10 and 11 detected an anomalous and apparently constant acceleration, ap, acting against the spacecraft's general direction of motion (ap~8·10?10 ms?2) [1]. The existence of this anomaly has been independently confirmed, but as yet there is no satisfactory explanation of the observed Pioneer 10 and 11 trajectories, that is, the systematic origin of the phenomena is still unknown.A new effort to study the origin of ap is underway by an international collaboration led by JPL since extended Pioneer 10 and 11 data sets are now available. These contain housekeeping telemetry data for the missions' entirety as well as additional Doppler tracking data that cover the missions' early phases (4.6 to 80.2 AU for Pioneer 10 and 1.0 to 41.7 AU for Pioneer 11). Housekeeping telemetry data can be used to investigate maneuvers and fly–by events in detail, as well as provide verification of a FE(finite element) thermal model of the spacecraft.Here in this paper aspects of the data analysis as being performed at ZARM are discussed.
机译:来自先驱10和11的多普勒跟踪数据的先前JPL研究检测到异常且明显恒定的加速度AP,作用于宇宙飞船的一般运动方向(AP〜8·10?10ms?2)[1]。这种异常的存在已经独立证实了,但对于观察到的先驱10和11个轨迹没有令人满意的解释,即,现象的系统来源仍然是未知的。研究AP的起源的新努力通过JPL领导的国际合作以来,由于扩展先锋10和11数据集现在可用。这些包含特派团全部的内务遥测数据以及覆盖任务早期阶段的额外多普勒跟踪数据(Pioneer 10和1.0至41.7 AU的4.6到80.2 AU)。家务遥测数据可用于详细研究机动和飞行事件,并提供验证航天器的FE(有限元)热模型。在数据分析的本文中,在ZARM执行的数据分析方面讨论。

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