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NTIS 바로가기한국광학회지 = Korean journal of optics and photonics, v.32 no.6, 2021년, pp.314 - 322
김고은 (한국표준과학연구원 첨단측정장비연구소 우주광학팀) , 이윤우 (한국표준과학연구원 첨단측정장비연구소 우주광학팀) , 양호순 (한국표준과학연구원 첨단측정장비연구소 우주광학팀)
A reflecting telescope consists of a concave primary mirror and a convex secondary mirror. The primary mirror is easy to measure, because it converges the beam from an interferometer, while the secondary mirror diverges the beam and so is not easy to measure, even though it is smaller than the prima...
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