• 한국광학회지
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• 제13권6호
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• pp.537-542
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• 2002

서로 다른 null optics를 사용하는 null test의 측정결과를 상호 비교함으로써 null CGH test 신뢰성을 알아보았다. 회전대칭 포물면경(90mm, F/0.76) 형상측정 및 측정장치 정렬용 null CGH를 설계, encoding, 제작 후 null CGH test를 실시하였다. 결과를 평면경을 null optics로 사용하는 autocollimation test측정치와 비교하여 null CGH test의 정확성을 평가하였다.

• Current Optics and Photonics
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• 제3권5호
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• pp.374-381
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• 2019

This study examined a method for designing the optical cavity of a non-dispersive infrared gas detector. The infrared gas detector requires an optical cavity design to lengthen the ray path. However, the optical cavity with multiple reflecting surfaces has off-axis aberration due to the characteristics of the reflecting optical system. The rays were parallelized by using the off-axis parabolic mirror to easily increase the ray path and eliminate off-axis aberration so that the rays are admitted to the effective area of the infrared detector uniformly. A prototype of an infrared gas detector was produced with the designed optical cavity to confirm the performance.

• 한국광학회지
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• 제17권3호
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• pp.256-261
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• 2006

본 논문에서는 비축 포물 거울을 통과한 레이저 빔의 파면을 측정하는 방식으로 국내 및 국외에서 제작된 비축 포물 거울을 평가하였으며, 이로부터 비축 포물 거울의 집속 성능 및 정렬 민감도를 측정하였다. 국외에서 제작된 비축 포물 거울은 직경 약 34 mm의 레이저 빔에 대해 고차 파면 수차(higher-order aberration)의 rms 값이 $0.03{\mu}m$ 정도로 작아 광학적으로 좋은 품질을 갖는 것으로 판명되었다. 국내에서 제작된 비축 포물 거울은 같은 34 mm의 레이저 빔에 대해 고차 파면 수차의 rms 값이 $2.01{\mu}m$나 관측되어 아직 개선이 필요한 것으로 보인다. 또한, 비축 포물 거울의 회전 정렬 오차에 대한 비점수차(astigmatism)의 민감도를 측정한 결과 회전 정렬 오차에 대한 비점수차의 민감도는 $0.371{\mu}m/mrad$인 것으로 관측되었다. 이는 광선 추적 소프트웨어를 사용하여 계산한 값과 거의 같은 양으로 이러한 비점수차의 정렬 민감도 측정은 비축 포물 거울을 정렬하는데 도움을 줄 것으로 생각된다.

• 한국광학회지
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• 제11권2호
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• pp.80-84
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• 2000

Diamond turning machine으로 알루미늄을 가공하여 f/1.5, 구경 50mm인 포물명경을 제작하였다. 이진위상(binary phase) 홀로그램으로 포물면경 현상측정을 위한 computer generated hologram(CGH)을 encoding하였으며 staircase encodling 방법으로 간섭무늬 곡선의 직선근사를 하였다. 간섭무늬 데이터를 포스트스크립트(PostScript) 파일로 변환한 후 CGH 원도를 레이저 프린터로 확대 출력하고 축소 촬영하여 CGH를 제작하였다. 측정부(viewing arm)에 CGH가 위치하는 Twyman-Green 간섭계를 구성하여 포물면경의 표면형상을 측정하였다. 측정결과를 직접표면형상측정법 및 간섭계를 이용한 자동시준법의 측정 결과와 비교하고 오치를 분석하였다.

• 한국태양에너지학회 논문집
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• 제27권1호
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• pp.29-38
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• 2007

In order to analyze the performance comparison of dish solar collector with mirror arrays and receiver shapes, the radiative heat flux distribution inside the cavity receiver is numerically investigated. The solar irradiation reflected by dish solar collector is traced using the Monte-Carlo method. Five different dish solar collectors and three different cavity receivers are considered. A parabolic-shaped perfect mirror of which diameter is 1.5 m is considered as a reference dish solar collector and four different arrays of twelve identical parabolic-shaped mirror facets of which diameter are 0.4 m are used. Their reflecting areas, which are $1.5\;m^2$, are the same. Three different cavity receiver shapes are dome, conical, and cylindrical. In addition, the radiative properties of the concentrating surfaces can vary the thermal performance of the cavity receiver so that variation of the surface reflectivity of each mirror is considered. Based on the calculation, the design information of dish solar collector for producing the electric power can be obtained. The results show that the dome type has the best performance in receiver shapes and the 2AND4 INLINE has the best performance in mirror arrays except perfect mirror.

• 한국신재생에너지학회:학술대회논문집
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• 한국신재생에너지학회 2007년도 춘계학술대회
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• pp.662-667
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• 2007

The thermal performance comparisons of the dish solar collector system are numerically investigated with mirror arrays and receiver shapes. In order to compare the performances of the dish solar collector systems, six different mirror arrays and four different receiver shapes are considered and the radiative heat flux distribution on the inside of the receiver is analyzed. A parabolic-shaped perfect mirror of which diameter is 1.5 m is considered as a reference of the mirror arrays. Five different mirror arrays of twelve identical parabolic -shaped mirror facets of which diameter are 0.4 m are proposed in this study. Their reflecting areas, which are 1.5 $m^2$, are the same. Four different receiver shapes are a dome, a conical, a cylindrical and a unicorn type. The solar irradiation reflected by mirrors is traced using the Monte-Carlo method. In addition, the radiative properties of the mirror surface can vary the thermal performance of the dish solar collector system so that the effects of the surface reflectivity and the surface absorptivity are considered. Based on the calculation, the design information of dish solar collector system for producing the electric power can be obtained. The results show that the dome type has the best performance in receiver shapes and the 2AND4INLINE has the best performance in mirror arrays except the perfect mirror.

• 설비공학논문집
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• 제20권1호
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• pp.35-41
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• 2008

The radiative heat loss from a receiver of a dish solar collector is numerically investigated. The dish solar collector considered in this paper consists of a receiver and multi-faceted mirrors. In order to investigate the performance comparison of dish solar collectors, six different mirror arrays and four different receivers are considered. A parabolic- shaped perfect mirror of which diameter is 1.40 m is considered as the reference for the mirror arrays. The other mirror arrays which consist of twelve identical parabolic-shaped mirror facets of which diameter are 0.405 m are suggested for comparison. Their reflecting areas, which are 1.545 $m^{2}$, are the same. Four different receiver shapes are a conical, a dome, a cylindrical, and a unicorn type. The radiative properties of the mirror surfaces and the receiver surfaces may vary the thermal performance of the dish solar collector so that various surface properties are considered. In order to calculate the radiative heat loss in the receiver, two kinds of methods are used. The Net Radiation Method that is based on the radiation heat balance on the surface is used to calculate the radiation heat transfer rate from the inside surface of the receiver to the environment. The Monte-Carlo Method that is the statistical approach is adopted to predict the radiation heat transfer rate from the reflector to the receiver. The collector efficiency is defined as the results of the optical efficiency and the receiver efficiency. Based on the calculation, the unicorn type has the best performance in receiver shapes and the STAR has the best performance in mirror arrays except the perfect mirror.

• 한국광학회지
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• 제17권2호
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• pp.165-174
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• 2006

직경 450 mm(f/2.7) 포물면경 제작을 위해 자동무수차점방식의 널 광학계를 설계 및 제작하였으며, 설계프로그램(CODE V)의 공차분석기법을 이용하여 널 광학계의 제작과 정렬 오차에 따른 측정 신뢰도를 이론적으로 검증하였다. 그리고 광학계를 실제로 구축하여 포물면경의 제작에 적용하였다. 또한, 널 렌즈를 사용하지 않고 평면거울만 사용하는 자동시준방식의 측정방법으로 포물경을 재평가하여, 역으로 자동무수차점방식의 널 렌즈 정렬오차에 의한 측정 신뢰도를 확인하였다.

• Advances in Energy Research
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• 제8권3호
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• pp.155-163
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• 2022

The current study presents experimental research on a parabolic trough collector with tube and cavity receivers. The primary concentrating parabolic reflector is designed for an aperture area of 2×2 m² with mirror-polished stainless steel sheet reflectors. The cavity receiver consists of a compound parabolic secondary reflector and a copper tube. Both the conventional tube receiver and the cavity receiver tube are coated with black powder. The experiments are carried out to compare the efficiency of the cavity receiver with the tube receiver for fluid temperature rise, thermal efficiency, and overall losses. The experiments showed significantly higher fluid temperature rise and overall efficiency and lower thermal losses for the cavity receiver compared to the tube receiver within the parameters explored in this study.

• Current Optics and Photonics
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• 제4권1호
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• pp.50-56
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• 2020

The design of a concentration system for a solar side-pumped slab laser was investigated. The side size of the slab laser medium is 2 mm × 20 mm. Based on the principle of the edge ray, a secondary concentrating system consisting of a rectangular parabolic mirror (RPM) and a rectangular dielectric-filled compound parabolic concentrator (RDCPC) was demonstrated. The focal length of RPM is 1200 mm and the size is 734 mm × 2000 mm. The outlet size of the RDCPC is 2 mm × 20 mm. The concentration effect was analyzed by using Tracepro optical software. The results showed that the concentration efficiency reached 81.3% and the uniformity of the spot was 91.4% after optimization. This design of concentration system is of great reference value for a solar side-pumped slab laser.