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A method for the identification of a tethered satellite

机译:识别系留卫星的方法

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The dynamics of a tethered satellite are greatly affected by the perturbing force transmitted to the satellite through the tether. The existence of this tether force causes the satellite to behave in a non-Keplerian manner. when a tethered satellite is first detected and tracked, its modified Keplerian motion makes it difficult to identify the satellite as being tethered without prior knowledge that it is so. Classical orbit determination methods are unable to account for this modified Keplerian motion and the subsequent estimation procedure will commonly result in an inaccurate prediction of the satellite's trajectory. The predicted trajectory in such cases could appear to be balistic in nature, thereby causing great concern for individuals and organizations who are responsible for monitoring these types of scenarios. In such scenarios, the speed at which an accurate identification of the satellite can be made may also be very important.
机译:通过系链传输到卫星的干扰力极大地影响了系留卫星的动力学。这种系绳力的存在导致卫星以非吉普利人的方式运行。当首次检测到并跟踪拴系卫星时,如果没有事先知道,经过修正的开普勒运动,很难确定该卫星是否处于拴系状态。经典的轨道确定方法无法解决这种修正的开普勒运动,因此后续的估算程序通常会导致对卫星轨迹的预测不准确。在这种情况下,预测的轨迹在本质上似乎是平衡的,因此引起负责监视此类情况的个人和组织的极大关注。在这种情况下,准确识别卫星的速度也可能非常重要。

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