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首页> 外文期刊>Journal of Spacecraft and Rockets >Neutral Density and Crosswind Determination from Arbitrarily Oriented Multiaxis Accelerometers on Satellites
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Neutral Density and Crosswind Determination from Arbitrarily Oriented Multiaxis Accelerometers on Satellites

机译:卫星上任意定向的多轴加速度计的中性密度和侧风确定

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摘要

An iterative algorithm for determining density and crosswind from multiaxis accelerometer measurements onnsatellites is presented, which works independently of the orientation of the instrument in space. The performance ofnthe algorithm is compared with previously published algorithms using simulated data for the challengingnminisatellite payload.Without external error sources, the algorithm reduces rms density errors from 0.7 to 0.03%nand rmswind errors from38 to 1 m=s in this test.However, the effects of the errors in the instrument calibration andnthe external models that are used in the density and wind retrieval are dominant for the challenging minisatellitenpayload. These lead to mostly systematic density errors of the order of u000110–15%. The accuracy of the wind resultsnwhen using the newalgorithmis almost fully determined by the sensitivity of the cross-track acceleration componentnto the calibration and radiation pressure modeling errors. The applicability of the iterative algorithm and thenaccuracy of its results are demonstrated by presenting challengingminisatellite payload data froma period in whichnthe satellite was commanded to fly sideways and by comparing the density and wind results with those fromadjacentndays for which the satellite was in its nominal attitudemode. These investigations result in recommendations for thendesign of future satellite accelerometer missions for thermosphere research.
机译:提出了一种通过多轴加速度计测量云母确定密度和侧风的迭代算法,该算法与仪器在空间中的方向无关。将该算法的性能与先前发布的算法进行了比较,该算法使用具有挑战性的最小卫星有效载荷的模拟数据进行了测试。在没有外部误差源的情况下,该测试将算法的均方根密度误差从0.7降低到0.03%n,将均方根误差从38降低到1 m = s。仪器校准误差的影响以及用于密度和风量获取的外部模型是极具挑战性的最小有效载荷的主要因素。这些导致大多数系统密度误差约为u000110–15%。当使用新算法时,风的精确度几乎完全取决于交叉轨道加速度分量对校准和辐射压力建模误差的敏感性。通过呈现被命令向侧面倾斜的卫星发出的极具挑战性的最小卫星有效载荷数据,并将密度和风的结果与卫星处于标称姿态模式的相邻时刻的密度和风的结果进行比较,证明了迭代算法的适用性以及其结果的准确性。这些调查为今后设计热球研究卫星加速度计任务提供了建议。

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