• 제목/요약/키워드: Satellite Imager

검색결과 265건 처리시간 0.032초

순간 고도 변화에 대한 위성 영상 기기의 Time Delay and Integration 일치 연구 (Study on the Synchronization of Time Delay and Integration against Osculating Altitude Variation in Satellite Imager)

  • 조영민;김해동
    • 대한원격탐사학회지
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    • 제20권4호
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    • pp.227-234
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    • 2004
  • Tome Delay and Integration (TDI) 기법을 사용하는 고해상도 위성 영상 기기에 있어서 실제 위성 운영시 발생하는 위성 고도의 순간적 변화에 대한 TDI 일치를 연구하였다. 시간에 따라 변하는 순간 고도의 특성을 분석하였고 순간 고도 변화가 TDI 불일치를 초래하여 위성 영상 기기의 성능에 미치는 영향을 분석하였다. TDI 시간 지연을 조절하여 실제 위성 운영에서 순간적으로 발생하는 TDI 불일치를 보정하는 방법을 제안하였고 제안한 방법을 이용할 경우 성능 향상이 가능함을 보였다. 본 연구 결과는 실제 위성 운영에 원활히 적용할 수 있으며 위성 영상 품질 향상에 활용될 수 있다.

The Ground Checkout Test of OSMI(Ocean Scanning Multispectral Imager) on KOMPSAT-1

  • Yong, Sang-Soon;Shim, Hyung-Sik;Heo, Haeng-Pal;Cho, Young-Min;Oh, Kyoung-Hwan;Woo, Sun-Hee;Paik, Hong-Yul
    • 대한원격탐사학회:학술대회논문집
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    • 대한원격탐사학회 1999년도 Proceedings of International Symposium on Remote Sensing
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    • pp.375-380
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    • 1999
  • Ocean Scanning Multispectral Imager (OSMI) is a payload on the KOMPSAT satellite to perform worldwide ocean color monitoring for the study of biological oceanography. The instrument images the ocean surface using a wisk-broom motion with a swath width of 800 km and a ground sample distance (GSD) of<1km over the entire field of view (FOV). The instrument is designed to have an on-orbit operation duty cycle of 20% over the mission lifetime of 3 years with the functions of programmable gain/offset and on-board image data compression/storage. The instrument also performs sun and dark calibration for on-board instrument calibration. The OSMI instrument is a multi-spectral imager covering the spectral range from 400nm to 900nm using CCD Focal Plane Array (FPA). The ocean colors are monitored using 6 spectral channels that can be selected via ground commands. KOMPSAT satellite with OSMI was integrated and the satellite level environment tests and instrument aliveness/functional test as well, such as launch environment, on-orbit environment (Thermal/vacuum) and EMl/EMC test were performed at KARI. Test results met the requirements and the OSMI data were collected and analyzed during each test phase. The instrument is launched on the KOMPSAT satellite in the late 1999 and the image is scheduled to start collecting ocean color data in the early 2000 upon completion of on-orbit instrument checkout.

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The Ground Checkout Test of OSMI on KOMPSAT-1

  • Yong, Sang-Soon;Shim, Hyung-Sik;Heo, Haeng-Pal;Cho, Young-Min;Oh, Kyoung-Hwan;Woo, Sun-Hee;Paik, Hong-Yul
    • 대한원격탐사학회지
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    • 제15권4호
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    • pp.297-305
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    • 1999
  • Ocean Scanning Multispectral Imager (OSMI) is a payload on the KOMPSAT satellite to perform global ocean color monitoring for the study of biological oceanography. The instrument images the ocean surface using a wisk-broom motion with a swath width of 800km and a ground sample distance (GSD) of < 1km over the entire field of view (FOV). The instrument is designed to have an on-orbit operation duty cycle of 20% over the mission lifetime of 3 years with the functions of programmable gain/offset and on-board image data compression/storage. The instrument also performs sun and dark calibration for on-board instrument calibration. The OSMI instrument is a multi-spectral imager covering the spectral range from 400nm to 900nm using CCD Focal Plane Array (FPA). The ocean colors are monitored using 6 spectral channels that can be selected via ground commands. KOMPSAT satellite with OSMI was integrated and the satellite level environment tests including instrument aliveness/functional test, such as launch environment, on-orbit environment (Thermal/Vacuum) and EMI/EMC test were performed at KARl. Test results met the requirements and the OSMI data were collected and analyzed during each test phase. The instrument is launched on the KOMPSAT satellite on December 21,1999 and is scheduled to start collecting ocean color data in the early 2000 upon completion of on-orbit instrument checkout.

GOES-9 Raw Data Acquisition & Image Extraction

  • Kang C. H.;Park D. J.;Koo I. H.;Ahn S. I.;Kim E. K.
    • 대한원격탐사학회:학술대회논문집
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    • 대한원격탐사학회 2005년도 Proceedings of ISRS 2005
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    • pp.582-585
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    • 2005
  • The Geostationary Operational Environmental Satellite (GOES) 9, which is currently located at 155°E geostationary orbits, has transmitted earth observation data acquired by imager to CDA at NOAA. After the acquisition on ground, observation data are corrected on ground and re-transmitted to GOES-9 for the dissemination to users. In this paper, the procedure and result from raw data acquisition and pre-processing for earth observation imagery retrieval from GOES-9 Raw data acquired in Korea at May 2005 are introduced.

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Initial On-Orbit Modulation Transfer Function Performance Analysis for Geostationary Ocean Color Imager

  • Oh, Eun-Song;Kim, Sug-Whan;Cho, Seong-Ick;Ryu, Joo-Hyung;Ahn, Yu-Hwan
    • Journal of Astronomy and Space Sciences
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    • 제29권2호
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    • pp.199-208
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    • 2012
  • The world's first geostationary ocean color imager (GOCI) is a three-mirror anastigmat optical system 140 mm in diameter. Designed for 500 m ground sampling distance, this paper deals with on-orbit modulation transfer function (MTF)measurement and analysis for GOCI. First, the knife-edge and point source methods were applied to the 8th band (865 nm) image measured April 5th, 2011. The target details used are the coastlines of the Korean peninsula and of Japan, and an island 400 meters in diameter. The resulting MTFs are 0.35 and 0.34 for the Korean East Coastline and Japanese West Coastline edge targets, respectively, and 0.38 for the island target. The daily and seasonal MTF variations at the Nyquist frequency were also checked, and the result is $0.32{\pm}0.04$ on average. From these results, we confirm that the GOCI on-orbit MTF performance satisfies the design requirements of 0.32 for 865 nm wavelength.

COMS CADU DATA GENERATION FOR COMS IMPS TEST

  • Seo, Seok-Bae;Ahn, Sang-II
    • 대한원격탐사학회:학술대회논문집
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    • 대한원격탐사학회 2008년도 International Symposium on Remote Sensing
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    • pp.88-91
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    • 2008
  • The COMS IMPS (Communication Ocean and Meteorological Satellite IMage Pre-processing Subsystem) is developed for image pre-processing of COMS. For a test of the COMS IMPS, 7 support software are developed in KARI GS using simulated MI/GOCI WB (Wide-Band) data; COMS Fill Adder, MI (Meteorological Imager) CADU generator, GOCI (Geostationary Ocean Colour Imager) CADU generator, COMS CADU combiner, MI SD (Sensor Data) analyzer, GOCI SD analyzer, and COMS DM (Decomposition Module) test harness. This paper explains functions of developed support software and the COMS IMPS test using those software.

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OVERVIEW OF COMS GROUND SYSTEM AT METEOROLOGICAL SATELLITE CENTER OF KMA

  • Lee, Hyun-Kyoung;Lee, Bong-Ju;Lee, Yong-Sang;Shim, Jae-Myun;Suh, Ae-Sook;Kim, Hong-Sic;Je, Chang-Eon
    • 대한원격탐사학회:학술대회논문집
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    • 대한원격탐사학회 2006년도 Proceedings of ISRS 2006 PORSEC Volume I
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    • pp.159-162
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    • 2006
  • This paper describes the ground system for COMS (Communication, Ocean, and Meteorological Satellite), the first Korean multi-purposed geostationary satellite, at MSC (Meteorological Satellite Center) in Korea. The overview of COMS MI (Meteorological Imager) will be introduced as well. KMA would implement mission planning for COMS MI operation and receive, process, interpret, disseminate, and archive MI data operationally for domestic and foreign user groups. Major missions of COMS MI are mitigation of natural hazard such as typhoon, dust storm, and heavy rain, and short-term warning of severe weather to protect human health and commerce. Moreover, research of climate variability and long-term changes will be supported. In accordance with those missions, the concept and design of COMPASS (COMS operation and meteorological products application service system), the ground system for COMS MI in MSC, have been setting up since 2004. Currently, COMPASS design is being progressed and will have finished the end of 2006. The development of COMPASS has three phases: first phase is development of fundamental COMPASS components in 2007, second phase is to integrate and test all of the COMPASS components in 2008, and the last phase is to operate COMPASS after COMS In-Orbit Tests in 2009.

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정지궤도 해색탑재체(GOCI) 데이터의 수신.처리 시스템과 배포 서비스 (Introduction of Acquisition System, Processing System and Distributing Service for Geostationary Ocean Color Imager (GOCI) Data)

  • 양찬수;배상수;한희정;안유환;유주형;한태현;유홍룡
    • 대한원격탐사학회지
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    • 제26권2호
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    • pp.263-275
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    • 2010
  • 정지궤도 해색탑재체(GOCI, Geostationary Ocean Color Imager)의 주관 운영기관인 해양위성센터 (KOSC, Korea Ocean Satellite Center)는 한국해양연구원에 기반시설을 구축하였다. 또한, 해양위성센터는 수신시스템(GDAS), 전처리시스템(IMPS), 처리시스템(GDPS), 배포시스템(GDDS), 자료교환시스템(DMS), 기관간 자료교환시스템(EDES), 통합감시제어시스템(TMC) 등 GOCI 데이터의 서비스를 위한 준비를 완료하였다. 해양위성센 터에서는 매일 8번 관측되는 GOCI 데이터를 수신하고, 처리하여 배포정책에 따라 Level 1B 이후의 데이터를 사용자에게 배포하게 된다. 여기서는 해양위성센터의 시스템과 배포정책에 대한 개요를 설명하고, 사용자가 해양위성센터의 홈페이지에서 GOCI 데이터를 검색 요청하고 다운로드할 수 있는 방법을 소개한다.

구면 지표에서 경사촬영을 이용한 위성 영상기의 고도 저하 성능 보정 (Performance Compensation of the Satellite Imager below Normal Altitude Using Line-Of-Sight Tilt over Spherical Earth Surface)

  • 조영민
    • 대한원격탐사학회지
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    • 제20권2호
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    • pp.117-124
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    • 2004
  • 구면 지표 위를 비행하는 위성 영상기의 경사 촬영에 대한 공간 해상도 특성을 분석하고, Time Delay and Integration(TDI) 기법을 사용하는 위성 영상기의 고도가 정상 운영 범위 이하로 저하되었을 때 TDI 불일치로 발생하는 기하 성능 저하를 구면 지표에 대한 경사 촬영으로 보정하였다. 영상기의 시선 방향을 서로 독립적인 두 방향의 각들로 정의하여 구면 지표상의 임의의 관측 점에 대한 경사 촬영 특성을 분석하였고, 임의의 2차원 방향 경사 촬영으로 TDI 영상기의 고도 저하에 대해 성능 보정이 가능함을 해석적으로 보였다. 성능 보정은 TDI 재일치를 통해 Modulation Transfer Function(MTF) 감소 없이 약간의 지상화소거리 증가로 이루어졌다. 연구 결과로 고도 저하 성능 보정을 위한 2차원 경사 촬영의 효과적 방법을 제시하였다. 본 연구에서 제시한 고도 저하에 대한 해결책은 TDI 위성 영상기의 실제 운영에 있어서 임무 수행 보장 및 유연성에 도움이 될 수 있으리라 기대한다.

COMS METEOROLOGICAL IMAGER SPACE LOOK SIDE SELECTION ALGORITHM

  • Park, Bong-Kyu;Lee, Sang-Cherl;Yang, Koon-Ho
    • 대한원격탐사학회:학술대회논문집
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    • 대한원격탐사학회 2008년도 International Symposium on Remote Sensing
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    • pp.100-103
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    • 2008
  • COMS(Communication, Ocean and Meteorological Satellite) has multiple payloads; Meteorological Image(MI), Ocean Color Imager(GOCI) and Ka-band communication payloads. MI has 4 IR and 1 visible channel. In order to improve the quality of IR image, two calibration sources are used; black body image and cold space look data. In case of COMS, the space look is performed at 10.4 degree away from the nadir in east/west direction. During space look, SUN or moon intrusions are strictly forbidden, because it would degrade the quality of collected IR channel calibration data. Therefore we shall pay attention to select space look side depending on SUN and moon location. This paper proposes and discusses a simple and complete space look side selection logic based on SUN and moon intrusion event file. Computer simulation has been performed to analyze the performance of the proposed algorithm in term of east/west angular distance between space look position and hazardous intrusion sources; SUN and moon.

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