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MARS SCIENCE LABORATORY ENTRY, DESCENT, AND LANDING TRAJECTORY AND ATMOSPHERE RECONSTRUCTION

机译:火星科学实验室的录入,下降和着陆轨迹及大气重建

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On August 5th 2012, The Mars Science Laboratory entry vehicle successfully entered Mars'atmosphere and landed the Curiosity rover on its surface. A Kalman filter approach hasbeen implemented to reconstruct the entry, descent, and landing trajectory based on all availabledata. The data sources considered in the Kalman filtering approach include the inertialmeasurement unit accelerations and angular rates, the terrain descent sensor, the measuredlanding site, orbit determination solutions for the initial conditions, and a new set of instrumentationfor planetary entry reconstruction consisting of forebody pressure sensors, knownas the Mars Entry Atmospheric Data System. These pressure measurements are unique forplanetary entry, descent, and landing reconstruction as they enable a reconstruction of thefreestream atmospheric conditions without any prior assumptions being made on the vehicleaerodynamics. Moreover, the processing of these pressure measurements in the Kalman filterapproach enables the identification of atmospheric winds, which has not been accomplishedin past planetary entry reconstructions. This separation of atmosphere and aerodynamicsallows for aerodynamic model reconciliation and uncertainty quantification, which directlyimpacts future missions. This paper describes the mathematical formulation of the Kalmanfiltering approach, a summary of data sources and preprocessing activities, and results of thereconstruction.
机译:2012年8月5日,火星科学实验室的入门车成功进入火星 大气层并将好奇号流浪者降落在其表面上。卡尔曼滤波方法具有 已实施以根据所有可用的路径重建进入,下降和着陆的轨迹 数据。卡尔曼滤波方法中考虑的数据源包括惯性 测量单位的加速度和角速度,地形下降传感器, 着陆点,用于初始条件的轨道确定解决方案以及一套新的仪器 用于由前体压力传感器组成的行星进入重建 作为火星进入大气数据系统。这些压力测量对于 行星进入,下降和着陆重建,因为它们可以重建 自由气流大气条件,无需事先对车辆进行任何假设 空气动力学。此外,这些压力测量值在卡尔曼滤波器中的处理 这种方法可以识别尚未完成的大气风 在过去的行星入口重建中。空气和空气动力学的这种分离 可以进行空气动力学模型对账和不确定性量化,直接 影响未来的任务。本文介绍了卡尔曼的数学公式 过滤方法,数据源和预处理活动的摘要以及结果 重建。

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