• 대한공간정보학회지
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• 제21권3호
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• pp.63-71
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• 2013

본 연구에서는 산림 바이오매스와 식생지수의 상관성을 분석하기 위해 현장조사 자료, 위성영상과 LiDAR 자료를 이용하여 산정된 산림 바이오매스 분포도를 기준으로 고해상도 KOMPSAT-2 영상과 LANDSAT 영상을 이용하여 식생지수인 SR, NDVI, SAVI, LAI를 계산한 값과 비교하였다. 분석결과, 고해상도 KOMPSAT-2 영상의 식생지수가 LANDSAT 영상의 식생지수보다 침엽수의 상관성이 더 높게 나타났으며 활엽수의 경우는 LANDSAT 영상의 식생지수가 높은 상관성을 보였다. 식생지수 중에는 NDVI 값이 다른 지수에 비해 상관성이 높게 나타났다. 또한 STSAT-3 위성의 소형영상분광기(Compact Imaging Spectrometer, COMIS)와 유사 센서인 EO-1 위성의 Hyperion 영상을 이용하여 하이퍼스펙트럴 영상을 분석하고 바이오매스와 상관성이 상대적으로 높은 식생지수를 동일한 GSD 조건의 LANDSAT 위성의 식생지수와 비교하고 하이퍼스펙트럴 영상의 임상 추출에 대한 활용가능성을 분석하였다.

• 한국우주과학회:학술대회논문집(한국우주과학회보)
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• 한국우주과학회 2009년도 한국우주과학회보 제18권2호
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• pp.44.3-44.3
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• 2009

The MIRIS (Multi-purpose IR Imaging System), as the main payload of Science and Technology Satellite-3 (STSAT-3), is being developed by KASI in collaboration with several institutes for wide-field space observation in near IR wavelength. The Engineering Qualification Model (EQM) of MIRIS has been designed and fabricated in the laboratory. The system performance tests have been made including opto-mechanics, vibration test, thermal-vacuum environmental test and passive cooling test down to 200K. Most of the performance test results were satisfied with system requirements. The results of MIRIS performance tests have been presented at Critical Design Review (CDR) on September 2009. Several revisions were also recommended for Flight Model (FM) design, and detailed plan to develop FM of MIRIS is discussed in this paper.

• 천문학회보
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• 제39권1호
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• pp.49.2-49.2
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• 2014

The MIRIS (Multi-purpose InfraRed Imaging System) is a compact IR space Telescope, which has been developed by KASI since 2008 as the main payload of Korean STSAT-3. It was launched successfully by a Dnepr Rocket at Yasny Launch site, Russia in November 2013. After the launch, the STSAT-3 successfully settled down at Sun synchronous orbit with altitude of ~ 600km. Communications were regularly made between the ground station and the MIRIS with other secondary payload. We made a series of tests of the MIRIS during the verification period and found that all functions including the passive cooling are working as expected. The MIRIS has a wide-field of view $3.67{\times}3.67$ degrees and wavelength coverage from 0.9 to 2.0 micro-meter with the angular resolution of 51.6 arcsec. The main science missions of the MIRIS are (1) mapping of the Galactic plane with Paschen-alpha line (1.88 micro-meter) for the study of warm interstellar medium and (2) the measurement of large angular fluctuations of cosmic near infrared background radiation with I (1.05 micro meter) and H (1.6 micro meter) bands to identify their origin. We present the results of MIRIS initial operation in this paper.

• 천문학논총
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• 제22권4호
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• pp.201-209
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• 2007

We have preliminarily designed two infrared optical systems of the multi-purpose infrared camera system (MIRIS) which is the main payload of STSAT-3. Each optical system consists of a Cassegrain telescope, a field lens and a 1:1 re-imaging lens system that is essential for providing a cold stop. The Cassegrain telescope is identical for both of two infrared cameras, but the field correction lens and re-imaging lens system are different from each other because of different bands of wavelength. The effective aperture size is 100mm in diameter and the focal ratio is f/5. The total length of the optical system is 300mm and the position of the cold stop is 25mm from the detector focal plane. The RMS spot size is smaller than $40{\mu}m$ over the whole detector plane.

• 천문학회보
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• 제39권1호
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• pp.50.1-50.1
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• 2014

The Multi-purpose InfraRed Imaging System (MIRIS) is the main payload of Science and Technology Satellite 3 (STSAT-3), which was launched onboard Dnepr rocket from Russian Yasny Launch Base in November 2013. The MIRIS is an infrared (IR) camera, and the telescope has to be cooled down to below 200K in order to reduce thermal background noise. For the effective cooling and low-power consumption, we applied passive cooling method to the thermal design of the MIRIS. We also conducted thermal analysis and tested for the passive cooling before the launch of STSAT-3. After the launch, we have received State-of-Health (SOH) data from the satellite on orbit, including temperature monitoring results. It is important that the temperature of the telescope was shown to be cooled down to below 200K. In this paper, we present both the temperature data of the MIRIS on orbit and the thermal analysis results in the laboratory. We also compare these results and discuss the verification of the passive cooling.

• 천문학회보
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• 제36권1호
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• pp.64.1-64.1
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• 2011

MIRIS (Multipurpose Infra-Red Imaging System), is a small infrared space telescope which is being developed by KASI, as the main payload of Science and Technology Satellite 3 (STSAT-3). Two wideband filters (I and H) of the MIRIS enables us to study the cosmic infrared background by detecting the absolute background brightness. The narrow band filter for Paschen ${\alpha}$ emission line observation will be employed to survey the Galactic plane for the study of warm ionized medium and interstellar turbulence. The opto-mechanical design of the MIRIS is optimized to operate around 200K for the telescope, and the cryogenic temperature around 90K for the sensor in the orbit, by using passive and active cooling technique, respectively. The engineering and qualification model of the MIRIS has been fabricated and successfully passed various environmental tests, including thermal, vacuum, vibration and shock tests. The flight model was also assembled and is in the process of system optimization to be launched in 2012 by a Russian rocket. The mission operation scenario and the data reduction software is now being developed. After the successful mission of FIMS (the main payload of STSAT-1), MIRIS is the second Korean space telescope, and will be an important step towards the future of Korean space astronomy.

• 한국항공우주학회지
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• 제37권6호
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• pp.586-594
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• 2009

본 논문은 국내 최초의 소형 복합재 위성인 과학기술위성3호의 proto 모델에 대하여 랜덤, 정현파, 충격 진동응답에 대한 연구이다. 과학기술위성3호의 구조체는 여러 장의 패널을 서로 연결하여 만든 박스형의 구조이며 패널은 탄소섬유강화 복합재를 적층한 스킨에 알루미늄 허니컴 구조를 접착한 하이브리드샌드위치구조로 되어있다. 상용 FEA 코드인 MSC/NASTRAN을 사용하여 주파수 및 시간영역에서 위성의 설계요구조건으로 주어진 진동시험수준에 대한 모드, 응력, 변위, 가속도의 응답을 계산하였다. 이러한 해석결과를 바탕으로 발사 시 야기되는 진동으로 인한 파괴, 안전율 및 설계 타당성을 검토하였다. 이 연구결과들은 실제 위성구조설계 신뢰성 실험에 있어서 검증 및 비교의 자료로 사용될 수 있고, 위성개발의 중요한 자료로 활용된다.

• 한국우주과학회:학술대회논문집(한국우주과학회보)
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• 한국우주과학회 2010년도 한국우주과학회보 제19권1호
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• pp.37.4-37.4
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• 2010

KASI is developing the MIRIS (Multi-purpose IR Imaging System), as the main payload of Science and Technology Satellite-3 (STSAT-3). The Engineering Qualification Model (EQM) of the MIRIS has been recently fabricated, and Flight Model (FM) is now in final development stage. The system performance tests have been made mainly with EQM, and partly with FM in the laboratory, including opto-mechanics test, vibration test, thermal-vacuum test and passive cooling test down to 200K, using a thermal controlled vacuum chamber. Most of the system performance test results of the MIRIS are satisfied with the required specifications and its results were reflected in development of the FM with several revisions of the system design. In this paper, we present detailed system performance test procedures of the MIRIS and its results.

• 한국광학회:학술대회논문집
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• 한국광학회 2009년도 동계학술발표회 논문집
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• pp.363-364
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• 2009

초소형 영상 분광기 COMIS는 과학기술위성3호에 탑재되어 지표면 및 대기의 분광 촬영을 할 예정으로 개발되고 있다. COMIS는 궤도 700km 상공에서 약 30m의 해상도 및 30km의 관측 폭을 갖고 있으며, 가시광 및 근적외선 영역에서 $16{\sim}62$대역($2{\sim}15nm$ 파장 분해능)의 초분광 관측을 수행할 수 있다. COMIS는 CCD 등의 일부 전자 부품 단위에서의 수입을 제외하곤 설계, 제작 및 평가를 포함한 모든 개발이 국내의 연구진 및 업체에 의하여 진행되고 있다. COMIS는 2010년 말 발사를 목표를 개발되고 있으며, 현재 시험 모델 개발이 진행 중에 있다. 본 논문에서는 현재 진행 중인 시험 모델의 개발 현황을 보고한다.

• 대한원격탐사학회:학술대회논문집
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• 대한원격탐사학회 2005년도 Proceedings of ISRS 2005
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• pp.733-736
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• 2005

This paper presents the design of two antennas for the Dual-channel Radiometers for Earth and Atmosphere Monitoring (DREAM) the main payload, will be launched at NARO space center in Korea in 2007. The antennas are designed to meet stringent requirements of a very high beam efficiency, good pattern symmetry, and low VSWR, at 23.8 GHz and 37 GHz bands. Corrugated horn antennas are used. The simulation results of the electrical performance are presented.