天基干涉仪的计量方法研究

E. F. Tubbs
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引用次数: 0

摘要

设计了一种用于控制结构变形对天基天文干涉仪性能影响的计量方法。假设了一种多臂反射光学像面干涉仪。假设视场很小,科学对象很弱或延伸,因此需要盲指向。进一步假设收集孔在波前平面上的位置是由航天器结构充分确定的,不需要监测。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
An Approach to the Metrology for a Space-Based Interferometer
A metrology approach to be used in the control of the effects of structural deformations on the performance of a space-based astronomical interferometer has been devised. A multi-armed, image-plane interferometer with reflection optics has been assumed. It is assumed that the field of view will be small and that the science objects will be weak or extended so that blind pointing will be required. It is further assumed that the locations of the collecting apertures in the plane of the wavefront are sufficiently well determined by the spacecraft structure and do not require monitoring.
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