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MAP Attitude Control System Design and Flight Performance

机译:MAP姿态控制系统设计和飞行性能

摘要

The Microwave Anisotropy Probe (MAP) is a follow-on to the Differential Microwave Radiometer (DMR) instrument on the Cosmic Background Explorer (COBE) spacecraft. To make a full-sky map of cosmic microwave background fluctuations, a combination fast spin and slow precession motion will be used that will cover the entire celestial sphere in six months. The spin rate should be an order of magnitude higher than the precession rate, and each rate should be tightly controlled. The sunline angle should be 22.5 +/- 0.25 deg. Sufficient attitude knowledge must be provided to yield instrument pointing to a standard deviation of 1.3 arc-minutes RSS three axes. In addition, the spacecraft must be able to acquire and hold the sunline at initial acquisition, and in the event of a failure. Finally. the spacecraft must be able to slew to the proper burn orientations and to the proper off-sunline attitude to start the compound spin. The design and flight performance of the Attitude Control System on MAP that meets these requirements will be discussed.
机译:微波各向异性探测器(MAP)是宇宙背景探测器(COBE)航天器上的差分微波辐射计(DMR)仪器的后续产品。为了绘制宇宙微波背景波动的全天候图,将使用快速自旋和缓慢进动的组合,这些运动将在六个月内覆盖整个天球。自旋速率应比进动速率高一个数量级,并且每个速率都应严格控制。阳光角度应为22.5 +/- 0.25度。必须提供足够的姿态知识,以使仪器指向的标准偏差为1.3弧分RSS 3轴。此外,航天器必须能够在初次捕获时以及发生故障时捕获并保持阳光。最后。航天器必须能够旋转到正确的燃烧方向并以正确的偏离阳光的姿势开始复合旋转。将讨论满足这些要求的MAP姿态控制系统的设计和飞行性能。

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