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Boosting a tethered satellite's orbit around an oblate planet through resonant pumping.

机译:通过共振泵浦推动扁圆行星上的系留卫星的轨道。

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摘要

The center of mass of a satellite, which consists of two masses connected by a rigid, massless tether, moves in a circular non-equatorial orbit about an oblate planet. The satellite is made to tumble forward essentially in the orbital plane such that its average pitch rate relative to the local vertical equals the orbital rate. This tumbling motion is phased such that the tether axis is aligned with the local vertical 1/8th of an orbit prior to each crossing of the equatorial bulge and with the local horizontal 1/8th of an orbit alter each crossing. The angular momentum of the orbit is increased by this phasing of the force from the equatorial bulge with the variations in satellite orientation. Periodic modulation or "pumping" of the tether length in resonance with the equatorial crossings is required to maintain this phasing, and the resulting transfer of energy from the pumping mechanism to the orbit increases the altitude of the mass center.;The dynamics of this orbit-boosting effect are examined in detail through a second-order perturbation analysis. Elastic deflections of the tether and the effects of atmospheric drag are neglected. Equations of motion governing the orbital and attitude behavior of the satellite are presented, and a formula for the rate of orbit-boosting is obtained and shown to be maximized for a polar orbit. The correct schedule for varying the tether length is derived through consideration of the rate of work required by the tether-pumping mechanism. The analytical results for the polar orbit case are checked through a numerical simulation which includes a feedback control scheme for maintaining the optimum orbit/attitude phasing. Out-plane deviations from the nominally in-plane tumbling motion are analyzed for the non-polar orbit case and are shown to remain small. The effects of higher-order perturbations and some practical application issues are also discussed.
机译:卫星的质心由两个质量组成,这些质量由刚性的,无质量的系链连接,并围绕扁圆行星在圆形的非赤道轨道中移动。使卫星基本上在轨道平面中前倾,使得其相对于本地垂直线的平均俯仰速率等于轨道速率。该翻滚运动的相位是这样的,以使系绳轴在每次越过赤道隆起之前与轨道的局部垂直1/8对齐,并且与轨道的局部水平1/8改变每次相交。随着卫星方向的变化,来自赤道隆起的力的相位增加了轨道的角动量。为了保持该相位,需要与赤道交叉点进行周期性调制或对“系绳”进行“泵送”,以保持该相位,并且能量从泵送机构向轨道的传递增加了质心的高度。通过二阶扰动分析详细检查了增强效果。可以忽略系绳的弹性变形和大气阻力的影响。提出了控制卫星轨道和姿态行为的运动方程,并获得了提升轨道速率的公式,并证明该公式对于极地轨道而言是最大化的。更改系绳长度的正确时间表是通过考虑系绳泵送机构所需的工作速率得出的。通过数值模拟检查极地轨道情况的分析结果,该数值模拟包括用于维持最佳轨道/姿态定相的反馈控制方案。对于非极性轨道情况,分析了与名义上的平面翻滚运动的平面外偏差,并且该偏差仍然很小。还讨论了高阶扰动的影响和一些实际应用问题。

著录项

  • 作者

    Gearhart, James Walter.;

  • 作者单位

    Stanford University.;

  • 授予单位 Stanford University.;
  • 学科 Aerospace engineering.
  • 学位 Ph.D.
  • 年度 1990
  • 页码 119 p.
  • 总页数 119
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

  • 入库时间 2022-08-17 11:50:30

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