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성세현,김석환,류동옥,홍진석,Seong, Sehyun,Kim, Sug-Whan,Ryu, Dongok,Hong, Jinsuk,Lockwood, Mike 한국천문학회 2012 天文學會報 Vol.37 No.2
The on-orbit test simulation for predicting the instrument directional responsivity was conducted by the Monte Carlo based integrated ray tracing (IRT) computation technique and analytic flux-to-signal conversion algorithms. For the on-orbit test simulation, the Sun model consists of the Lambertian scattering sphere and emitting spheroid rays, the Amon-Ra instrument is a two-channel including a broadband scanning radiometer (energy channel) and an imager with ${\pm}2^{\circ}$ FOV (visible channel). The solar radiation produced by the Sun model is directed to the instrument viewing port and traced through the dual channel optical train. The instrument model is rotated on its rotation axis and this gives a slow scan of the Sun model over the full field of view. The direction of the incident lights are fed with scanned images obtained from the visible channel instrument. The instrument responsivity was computed by the ratio of the incident radiation input to the instrument output. In the radiometric simulation, especially, measured BRDF of the 3D CPC was used for scattering effects on radiometry. With diamond turned 3D CPC inner surface, the anisotropic surface scattering model from the measured data was applied to ray tracing computation. The technical details of the on-orbit test simulation are presented together with field-of-view calibration plan.
류동옥,김성환,성세현,Ryu, Dongok,Kim, Sug-Whan,Seong, Sehyun 한국천문학회 2012 天文學會報 Vol.37 No.2
Previously we introduced ray-tracing based 3D optical earth system model for specular and scattering properties of all components of the system (i.e. clear-sky atmosphere, land surfaces and an ocean surface). In this study, we enhanced 3-dimensional atmospheric structure with vertical atmospheric profiles for multiple layer and cloud layers using Lambertian and Mie theory. Then the phase dependent disk averaged spectra are calculated. The main results, simulated phase dependent disk averaged spectra and light curves, are compared with the 7 bands(300~1000nm) light curves data of the Earth obtained from High Resolution Instrument(HRI) in Deep Impact spacecraft during Earth flyby in 2008. We note that the results are comparable with the observation.
장거리 화염 탐지용 적외선 카메라 성능 광선추적 수치모사
윤지연,류동옥,김상민,성세현,윤웅섭,김지은,김석환,Yoon, Jeeyeon,Ryu, Dongok,Kim, Sangmin,Seong, Sehyun,Yoon, Woongsup,Kim, Jieun,Kim, Sug-Whan 한국광학회 2014 한국광학회지 Vol.25 No.5
본 논문에서는 사거리가 수백 km에 이르는 장거리 미사일의 화염을 발사 초기에 탐지할 수 있는 적외선 카메라에 대한 현실적 영상성능 수치모사 결과를 제시한다. 적외선 카메라는 중적외선 대역용 다수의 렌즈로 구성된 굴절식 광학계이다. 관측대상과 배경의 모델링 전체를 포함하는 규모의통합적 광선추적을 수행함으로 카메라를 통해 보는 영상과 검출기에 도달하는 빛의 세기에 대한 정보를 획득하였다. 관측대상이 되는 미사일 화염의 방사휘도(radiance)는 CFD 타입의 복사전달 기법으로 계산하였으며 이를 광원으로 삽입하여 광선추적을 수행하였다. 관측배경이 되는 대기 모델은 MODTRAN을 사용하여 열복사의 경로, 단일/다중 산란 복사와 투과율을 계산하였다. 광선추적 수치모사의 결과로써 관측대상의 이미지와 도달한 복사전달 성능(radiometric performance)의 검증을 통해 적외선 카메라가 요구사항을 만족함을 입증하였다. We report a realistic field-performance simulation for a new MWIR camera. It is designed for early detection of missile plumes over a distance range of a few hundred kilometers. Both imaging and radiometric performance of the camera are studied by using real-scale integrated ray tracing, including targets, atmosphere, and background scene models. The simulation results demonstrate that the camera would satisfy the imaging and radiometric performance requirements for field operation.