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Gyroscope spin axis direction control for the Gravity Probe B satellite.

机译:重力探测器B卫星的陀螺仪旋转轴方向控制。

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The Gravity Probe B Relativity Experiment (GP-B) is a joint NASA/Stanford University orbiting astrophysics experiment, under development, to test two predictions of Einstein's theory of general relativity, the geodetic and frame-dragging effects, using orbiting, ultra-precise, mechanical, electrically-suspended gyroscopes (ESVG) carefully isolated from Newtonian torques. General relativity predicts that the gyroscopes' spin axes will precess with respect to a distant inertial reference frame at a rate of 6.6 arc-sec/year for the geodetic effect, and 42 marc-sec/year due to frame-dragging in the planned orbit. To achieve the needed levels of measurement precision, the gyroscopes' axes must be aligned to within 10 arc-sec of the line-of-sight to a distant guide star.; Presented is a technique by which the initial orientation of each gyroscope can be controlled through the use of residual torques generated by the gyroscope' s electrostatic suspension system. The electrostatic torques acting on the gyroscope depend on the rotor shape, which is nominally spherical but also contains small manufacturing asphericities and a spin-induced bulge. These torques are averaged by rotor spin to take on a simple form: they cause the gyroscope to precess about the suspension electrode axes.; Orientation control torques are applied by introducing additional suspension voltages to the electrodes in combinations which do not exert a force on the gyroscope, but do generate a torque. A control system was developed to use these torques to drive the spin axis to a desired orientation in minimum-time using a bang-bang actuation scheme. A net torque identification scheme was also created to monitor polhode-induced modulations of the spin-averaged torques. This information was used by the orientation control system to keep the spin axis on a minimum-time trajectory.; Laboratory experiments confirmed the validity of the spin-averaged torque models and gave a proof-of-principle of the effectiveness of the bang-bang spin axis orientation control system. Under active orientation control, the polhode modulations of the spin-averaged torques were readily measured using the proposed identification technique. The net result of the tests confirm that the spin axes of the gyroscope may be oriented using these techniques to the accuracy required for the GP-B experiment.
机译:重力探测器B相对论实验(GP-B)是美国宇航局/斯坦福大学联合进行的天体物理学轨道实验,正在开发中,用于测试爱因斯坦的广义相对论的两个预测,即大地测量和框架拖曳效应,使用轨道超精密技术,机械的,电悬挂的陀螺仪(ESVG)与牛顿扭矩仔细隔离。广义相对论预测,陀螺仪的自转轴将相对于遥远的惯性参考系进动,其大地影响的速率为6.6弧秒/年,而由于计划中的轨道被拖曳,速率为42 marc-sec /年。 。为了达到所需的测量精度水平,陀螺仪的轴必须与距离遥远的恒星的视线对准10弧秒以内。提出了一种技术,通过该技术可以通过使用由陀螺仪的静电悬架系统产生的残余扭矩来控制每个陀螺仪的初始方向。作用在陀螺仪上的静电转矩取决于转子的形状,该转子的形状通常为球形,但也包含较小的制造非球形度和自旋引起的凸起。这些扭矩通过转子旋转取平均值,以简单的形式表示:它们使陀螺仪绕悬架电极轴进动。通过将附加的悬浮电压引入电极中来组合施加方向控制扭矩,这些电压不会在陀螺仪上施加力,但会产生扭矩。开发了一种控制系统,可使用这些扭矩在最小时间内使用爆炸驱动方案将旋转轴驱动到所需的方向。还创建了净扭矩识别方案来监视自旋平均扭矩的多极感应调制。定向控制系统使用此信息将旋转轴保持在最小时间轨迹上。实验室实验证实了自旋平均转矩模型的有效性,并给出了自旋自旋轴方向控制系统有效性的原理证明。在主动定向控制下,使用所提出的识别技术可以很容易地测量自旋平均转矩的极化调制。测试的最终结果证实,使用这些技术可以将陀螺仪的旋转轴定向到GP-B实验所需的精度。

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