Projects of optical space-based stellar interferometers

被引：0

作者：

Ryabova, NV ^{[1
]}

Es'kov, DN ^{[1
]}

机构：

[1] SI Vavilov State Opt Inst, St Petersburg, Russia

来源：

JOURNAL OF OPTICAL TECHNOLOGY | 1999年 / 66卷 / 02期

关键词：

D O I：

10.1364/JOT.66.000083

中图分类号：

O43 [光学];

学科分类号：

070207 ; 0803 ;

摘要：

We describe projects of space-based stellar interferometers developed in different countries as astronomical multipurpose tools of the next generation after the Hubble space telescope (HST). The short-baseline systems (baseline length of about 2 m) are designed for astrometry with an accuracy of 10 mu as rms. The long-baseline systems (baseline length >5 m) are studied for image formation in the aperture synthesis mode of operation with a resolution of about 1 mas. Fundamental technologies of this type are based on the use of active optics and smart-design. (C) 1999 The Optical Society of America. [S1070-9762(99)00102-5].

引用

页码：83 / 96

页数：14

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