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作为地球极点定位器的太阳光子推进器。

The solar photon thruster as a terrestrial pole sitter.

作者信息

Matloff Gregory L

机构信息

Department of Physical and Biological Sciences, NYC College of Technology, CUNY, 300 Jay Street, Brooklyn, NY 11201, USA.

出版信息

Ann N Y Acad Sci. 2004 May;1017:468-74. doi: 10.1196/annals.1311.028.

DOI:10.1196/annals.1311.028
PMID:15220163
Abstract

Geosynchronous satellites are invisible at high latitudes. A pole-sitting spacecraft would have communication, climate-studies, and near-polar Earth observation applications. We present a pole-sitter based on the solar photon thruster (SPT), a two-sail variant of the solar sail using a large curved collector sail (always normal to the Sun) to direct sunlight against a much smaller thruster. Thrust decreases slower for an SPT than for a conventional sail arrangement as the angle between sunlight and the collector normal increases. An SPT pole-sitter is offset from the terrestrial pole so that a component of Earth gravity balances the solar radiation-pressure component pushing the SPT off station. The component of gravitational attraction of the Earth pulling the spacecraft towards Earth is also balanced by a solar radiation-pressure component. Results are presented for 80-100% collector/thruster reflectivities. For a spacecraft areal mass thickness of 0.002 kg/m(2), collector and thruster reflectivities of 0.9, the SPT can be situated above latitude 45 degrees at a distance of approximately 60 Earth radii. An SPT pole sitter would be affected by lunar perturbation, which can be compensated for by an on-board rocket thruster producing 2 x 10(-6) g acceleration, a second SPT thruster sail thrusting against the influence of the Moon, or by directing a microwave beam against the spacecraft. Since an SPT pole sitter is in a position rather than an orbit, the effect of terrestrial gravitation limits the size and design of the payload package, which limits terrestrial target resolution.

摘要

地球同步卫星在高纬度地区是不可见的。一个驻极航天器将具有通信、气候研究和近极地地球观测应用。我们提出了一种基于太阳光子推进器(SPT)的驻极器,它是太阳帆的一种双帆变体,使用一个大的弯曲收集帆(始终垂直于太阳)将阳光导向一个小得多的推进器。随着阳光与收集器法线之间的角度增加,SPT的推力下降速度比传统帆装置慢。一个SPT驻极器偏离地极,以便地球引力的一个分量平衡将SPT推离位置的太阳辐射压力分量。将航天器拉向地球的地球引力分量也由一个太阳辐射压力分量平衡。给出了收集器/推进器反射率为80 - 100%时的结果。对于航天器面质量厚度为0.002 kg/m²、收集器和推进器反射率为0.9的情况,SPT可以位于纬度45度以上约60个地球半径的距离处。一个SPT驻极器会受到月球摄动的影响,这可以通过产生2×10⁻⁶g加速度的机载火箭推进器、第二个抵抗月球影响的SPT推进帆或通过向航天器发射微波束来补偿。由于一个SPT驻极器处于一个位置而非轨道,地球引力的影响限制了有效载荷包的尺寸和设计,从而限制了地面目标分辨率。

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