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Determination of critical parameters for solar probe plus shielding .

机译:太阳探针加屏蔽的关键参数的确定。

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摘要

A methodology to determine critical design parameters such as critical "design" particle size, and critical "design" impact speed for the shielding of the Solar Probe Plus spacecraft was developed in this thesis. Several critical components and surfaces of the spacecraft such as the Solar Array North, the Thermal Protection System, and the ISIS Instruments were analyzed in this study. The methodology determines the critical "design" particle size based on the required reliability or probability of no impact. Current NASA methods do not provide means to calculate critical "design" impact speeds for missions such as Solar Probe Plus, where the distributions of impact speeds can vary significantly from particle size to particle size and with position of the spacecraft as a function of time due to the non-circular orbital trajectory that the spacecraft will follow. Previous methodologies attempted to determine the critical "design" impact speed based on the distribution of speeds from the smallest particle size, and yielded conservative results. This thesis uses the entire distributions of impact speeds for all dust particle sizes in an attempt to reduce conservatism and thus launching and material costs for the mission. This is crucial because it accounts for the dependency of the impact speed distribution on particle size, and is achieved by normalizing the total cumulative number of impacts as a function of the normal component of impact speed for every particle size. Results from this thesis show that the critical impact speed is significantly reduced when compared to previous methodologies. As the required probability of no impact increases, the critical particle size also increases, and the critical impact decreases.
机译:本文提出了一种确定关键设计参数的方法,如确定关键的“设计”粒径和关键的“设计”撞击速度以屏蔽Solar Probe Plus航天器。在这项研究中,分析了航天器的几个关键组件和表面,例如北太阳阵列,热保护系统和ISIS仪器。该方法根据所需的可靠性或无影响的概率来确定关键的“设计”粒度。当前的NASA方法没有提供用于计算任务(例如Solar Probe Plus)的关键“设计”撞击速度的手段,其中撞击速度的分布因粒子大小而异,并且航天器的位置随时间的变化而显着不同。到航天器将遵循的非圆形轨道轨迹。先前的方法试图根据最小粒度的速度分布来确定关键的“设计”冲击速度,并得出保守的结果。为了减少保守性,从而减少任务的发射和材料成本,本论文使用了所有尘埃粒径的冲击速度的整个分布。这是至关重要的,因为它考虑了冲击速度分布对粒度的依赖性,并且是通过对每个粒度的冲击总累积数作为冲击速度的正常分量的函数进行归一化来实现的。论文的结果表明,与以前的方法相比,临界冲击速度显着降低。随着所需的无冲击概率增加,临界粒度也增加,并且临界冲击减小。

著录项

  • 作者

    Mendez, Sergio Rafael.;

  • 作者单位

    The University of Texas at El Paso.;

  • 授予单位 The University of Texas at El Paso.;
  • 学科 Engineering Aerospace.;Engineering Civil.
  • 学位 M.S.
  • 年度 2011
  • 页码 73 p.
  • 总页数 73
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类 语言学;
  • 关键词

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