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Modes of Uncontrolled Rotational Motion of the Progress M-29M Spacecraft

机译:M-29M航天器的不受控制的旋转运动模式

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摘要

We have reconstructed the uncontrolled rotational motion of the Progress M-29M transport cargo spacecraft in the single-axis solar orientation mode (the so-called sunward spin) and in the mode of the gravitational orientation of a rotating satellite. The modes were implemented on April 3-7, 2016 as a part of preparation for experiments with the DAKON convection sensor onboard the Progress spacecraft. The reconstruction was performed by integral statistical techniques using the measurements of the spacecraft's angular velocity and electric current from its solar arrays. The measurement data obtained in a certain time interval have been jointly processed using the least-squares method by integrating the equations of the spacecraft's motion relative to the center of mass. As a result of processing, the initial conditions of motion and parameters of the mathematical model have been estimated. The motion in the sunward spin mode is the rotation of the spacecraft with an angular velocity of 2.2 deg/s about the normal to the plane of solar arrays; the normal is oriented toward the Sun or forms a small angle with this direction. The duration of the mode is several orbit passes. The reconstruction has been performed over time intervals of up to 1 h. As a result, the actual rotational motion of the spacecraft relative to the Earth-Sun direction was obtained. In the gravitational orientation mode, the spacecraft was rotated about its longitudinal axis with an angular velocity of 0.1-0.2 deg/s; the longitudinal axis executed small oscillated relative to the local vertical. The reconstruction of motion relative to the orbital coordinate system was performed in time intervals of up to 7 h using only the angular-velocity measurements. The measurements of the electric current from solar arrays were used for verification.
机译:我们以单轴太阳方向模式(所谓的向阳自旋)和旋转卫星的重力方向模式重构了Progress M-29M运输货物航天器的不受控制的旋转运动。该模式已于2016年4月3日至7日实施,这是在Progress航天器上使用DAKON对流传感器进行实验的准备工作的一部分。重建是通过积分统计技术使用航天器的角速度和来自其太阳电池阵列的电流的测量值进行的。通过积分航天器相对于质心的运动方程,使用最小二乘法对在一定时间间隔内获得的测量数据进行了联合处理。作为处理的结果,已经估计了运动的初始条件和数学模型的参数。向阳自旋模式下的运动是航天器围绕太阳电池阵列平面的法线以2.2度/秒的角速度旋转的过程;法线朝向太阳或与该方向成小角度。该模式的持续时间为几次轨道通过。重建已进行了长达1小时的时间间隔。结果,获得了航天器相对于地球-太阳方向的实际旋转运动。在重力定向模式下,航天器绕其纵轴以0.1-0.2 deg / s的角速度旋转;纵轴相对于局部垂线执行小振荡。仅使用角速度测量,就可以在长达7小时的时间间隔内完成相对于轨道坐标系的运动重建。来自太阳能电池阵列的电流测量结果用于验证。

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  • 来源
    《Cosmic research》 |2018年第1期|54-67|共14页
  • 作者单位

    Korolev Rocket & Space Corp Energia, Korolev 141070, Russia;

    Korolev Rocket & Space Corp Energia, Korolev 141070, Russia;

    Korolev Rocket & Space Corp Energia, Korolev 141070, Russia;

    Korolev Rocket & Space Corp Energia, Korolev 141070, Russia;

    Russian Acad Sci, Keldysh Inst Appl Math, Moscow 125047, Russia;

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