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Mitigation of Thruster Plume Erosion of International Space Station Solar Array Coatings

机译:减轻国际空间站太阳电池阵列涂层的推进器羽状侵蚀

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Optically sensitive surfaces on the International Space Station (ISS) can be damaged (or eroded/pitted) when impacted by high-velocity particles from unburned liquid propellant present in bipropellant thruster plumes. Surfaces with thin optical coatings, such as solar arrays and radiators, are of primary concern. Thruster plume-induced erosion/pitting of sensitive surfaces has been observed on space shuttle flight experiments. The Boeing ISS Environments Team in Houston has developed an approach to modeling thruster plume-induced erosion/pitting of ISS surface materials. The Boeing team has conducted analyses simulating bipropellant thruster particles impacting sensitive ISS surfaces for various assembly stages. Thruster firings for ISS reboost/attitude control, as well as visiting vehicle thruster firings during approach or separation to ISS docking ports, were simulated. The results of these analyses show that particle impingement angle greatly affects surface damage, with normal impacts being the most severe. Particles with highly oblique impact angles (~75 deg off normal), however, will essentially skid off surfaces without causing any erosion/pitting. A mitigation technique has been developed to prevent plume erosion/pitting of solar array coatings. Before a thruster-firing event, solar arrays may be rotated to a preestablished position that will eliminate plume particle impact damage to the surface. The preestablished positions are defined based on the geometry of the ISS thrusters relative to the solar array panels to ensure that plume particles will impinge at highly oblique angles (greater than 75 deg off normal). Upcoming ISS milestones will introduce new sensitive surfaces and thrusters, making 2005 a critical year for establishing operational constraints to mitigate thruster plume erosion. Some of these milestones include the space shuttle return to flight, the deployment of new ISS solar arrays, and the maiden voyage of ESA's automated transfer vehicle. Operational constraints for plume erosion mitigation are being coordinated with other solar array operational constraints such as power, thermal, and plume-induced structural loads. An integrated operational solution is being implemented to support the ISS assembly flight sequence. This paper will discuss plume erosion analyses and the implementation of operational mitigation as well as ongoing testing to better characterize plume erosion effects.
机译:当受到双推进剂推进器羽流中未燃烧液体推进剂的高速粒子撞击时,国际空间站(ISS)上的光学敏感表面可能会损坏(或腐蚀/凹陷)。具有薄光学涂层的表面(例如太阳能电池板和散热器)是主要关注的问题。在航天飞机的飞行实验中已经观察到推力器羽流引起的敏感表面腐蚀/点蚀。休斯顿的波音ISS环境团队开发了一种方法,用于对推进器羽流引起的ISS表面材料的腐蚀/点蚀建模。波音团队已经进行了分析,以模拟在不同组装阶段撞击敏感ISS表面的双推进剂推进器颗粒。模拟了用于ISS升压/姿态控制的推进器点火装置,以及在进近或分离到ISS对接端口期间访问车辆推进器点火装置的过程。这些分析的结果表明,粒子撞击角极大地影响了表面损伤,其中正常撞击最为严重。但是,具有高倾斜冲击角(偏离法线约75度)的颗粒将基本上从表面滑落而不会引起任何腐蚀/点蚀。已经开发了缓解技术来防止羽状腐蚀/太阳能电池阵列涂层的点蚀。在推进器点火事件之前,可将太阳能电池阵列旋转到预设位置,该位置将消除羽状颗粒对表面的冲击破坏。预先确定的位置是根据ISS推进器相对于太阳能电池板的几何形状定义的,以确保羽状颗粒以高倾斜角度(偏离法线大于75度)撞击。即将到来的ISS里程碑将引入新的敏感表面和推进器,使2005年成为建立操作约束以减轻推进器羽流侵蚀的关键一年。其中一些里程碑式事件包括航天飞机重返太空,部署新的ISS太阳能电池阵列以及ESA自动转运车的首次航行。减轻羽流侵蚀的运行限制正在与其他太阳能电池阵列的运行限制(例如功率,热和羽流引起的结构载荷)进行协调。正在实施一个集成的运营解决方案来支持ISS组装飞行程序。本文将讨论羽流侵蚀分析和缓解措施的实施以及正在进行的测试,以更好地表征羽流侵蚀效应。

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