• 제목/요약/키워드: Three-Mirror-Anastigmat (TMA)

검색결과 5건 처리시간 0.021초

Design and Manufacture of an Off-axis Aluminum Mirror for Visible-light Imaging

  • Zhang, Jizhen;Zhang, Xin;Tan, Shuanglong;Xie, Xiaolin
    • Current Optics and Photonics
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    • 제1권4호
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    • pp.364-371
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    • 2017
  • Compared to one made of glass, an aluminum mirror features light weight, compact design, low cost, and quick manufacturing. Reflective mirrors and supporting structures can be made from the same material, to improve the athermal performance of the system. With the rapid development of ultraprecise machining technologies, the field of applications for aluminum mirrors has been developed rapidly. However, most of them are rotationally symmetric in shape, and are used for infrared applications. In this paper, the design and manufacture of an off-axis aluminum mirror used for a three-mirror-anastigmat (TMA) optical system at visible wavelengths is presented. An optimized, lightweight design provides a weight reduction of more than 40%, while the surface deformation caused by earth's gravity can meet the required tolerance. The two pieces of an off-axis mirror can be diamond-turned simultaneously in one setup. The centrifugal deformation of the off-axis mirror during single-point diamond turning (SPDT) is simulated through the finite-element method (FEM). The techniques used to overcome centrifugal deformation are thoroughly described in this paper, and the surface error is reduced to about 1% of the original value. After post-polishing, the form error is $1/30{\lambda}$ RMS and the surface roughness is better than 5 nm Ra, which can meet the requirements for visible-light imaging.

타원면경 측정 Null 렌즈 설계 (Null lens design for testing of elliptical surface)

  • 김연수
    • 한국광학회지
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    • 제11권4호
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    • pp.246-249
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    • 2000
  • 고해상도 원격관측용 카메라오 설계된 비축 3반사 광학계의 제3거울인 타원면(원추계수>0) 형상측정 Null 렌즈를 설계하였다. Null 렌즈 설계방식으로는 측정감도는 2배로 높으면서 작은 기준 평면경을 사용하는 혼합방식을 제안하였다. 혼합방식과 autostigmatic 방식으로 설계한 Null 렌즈의 광파면 왜곡 민감도를 비교하여 혼합방식이 보다 유리한 Null 측정 광학게임을 제시하였다.

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쌍곡면 측정 null 렌즈 설계 (Design of null lenses for testing of hyperbolic surfaces)

  • 김연수;김병윤;이윤우
    • 한국광학회지
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    • 제12권5호
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    • pp.352-355
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    • 2001
  • 고해상도 원격관측용 카메라로 설계된 비축 3반사 광학계의 제1거울인 쌍곡면 형상 측정을 위한 null 렌즈를 설계하였다. Null 렌즈는 autostigmatic 방식과 mixed 방식으로 설계하였으며, 렌즈의 곡률반경, 두께등의 변수에 대한 상대적 민감도를 비교 분석하여 보다 측정이 용이한 null 렌즈를 제시하였다.

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Structural Design Development of GOCI

  • Yeon Jeoung-Heum;Kang Song-Doug;Kim Jongah;Kang Gurrl.sil;Myung Hwan-Chun;Youn Heong-Sik
    • 대한원격탐사학회:학술대회논문집
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    • 대한원격탐사학회 2005년도 Proceedings of ISRS 2005
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    • pp.104-107
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    • 2005
  • COMS(Communication, Ocean, and Meteorological Satellite) is the geostationary satellite for the mission of satellite communication, ocean monitoring, and meteorological service. It is scheduled to be launched at the end of 2008. Ocean payload of COMS named as GOCI(Geostationary Ocean Color Imager) observes ocean color and derives the chlorophyll concentrlition, the concentration of dissolved organic material and so on. In operational oceanography, satellite derived data products are used to provide forecasting and now casting of the ocean and coastal water state. In this work, conceptual design of structural part of GOCI is carried out and two baseline concepts are proposed. The one is dioptric module that uses lens system and the other is TMA(Three Mirror Anastigmat) module that uses mirror system. Trade-off studies between two concepts are investigated by considering optical and mechanical performances. Finally, on-going tasks and future development plan are briefly discussed.

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Straylight analysis for preliminary filter and baffle design for New Generation GOCI

  • Oh, Eun-Song;Ahn, Ki-Beom;Jung, Kil-Jae;Ryu, Dong-Ok;Kim, Sug-Whan
    • 한국우주과학회:학술대회논문집(한국우주과학회보)
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    • 한국우주과학회 2010년도 한국우주과학회보 제19권1호
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    • pp.25.4-26
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    • 2010
  • We present a three-mirror anastigmat(TMA) optical system for New Generation GOCI. In order to reduce the ghost optimized filter and baffle. By using carefully chosen antireflective coating and tilted filter angle, we fulfilled the design SNR requirement of 1500. We then designed a new entrance baffle and an internal baffle capable of producing the ghost ratio better than 0.01% of the nominal signal. The entrance baffle limits FOV to $0.75^{\circ}$ (E/W) $\times$ $0.60^{\circ}$ (S/N), and prevents the system from strong sun illumination, and the internal baffle prevents stray and scattered ray from entering into the telescope cavity. From these filter and baffle design, we confirmed that the instrument signal to noise ratio can be met with the current conceptual opto-mechanical design.

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