• Korean Journal of Remote Sensing
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• v.37 no.5_2
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• pp.1235-1243
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• 2021

Geostationary Ocean Color Imager 2 (GOCI-II) on Geo-KOMPSAT-2 (GK2B)satellite was developed as a mission successor of GOCI on COMS which had been operated for around 10 years since launch in 2010 to observe and monitor ocean color around Korean peninsula. GOCI-II on GK2B was successfully launched in February of 2020 to continue for detection, monitoring, quantification, and prediction of short/long term changes of coastal ocean environment for marine science research and application purpose. GOCI-II had already finished IAC and IOT including early in-orbit calibration and had been handed over to NOSC (National Ocean Satellite Center) in KHOA (Korea Hydrographic and Oceanographic Agency). Radiometric calibration was periodically conducted using on-board solar calibration system in GOCI-II. The final calibrated gain and offset were applied and validated during IOT. And three video parameter sets for one day and 12 video parameter sets for a year was selected and transferred to NOSC for normal operation. Star measurement-based INR (Image Navigation and Registration) navigation filtering and landmark measurement-based image geometric correction were applied to meet the all INR requirements. The GOCI2 INR software was validated through INR IOT. In this paper, status and results of IOT, radiometric calibration and INR of GOCI-II are analysed and described.

• Journal of Astronomy and Space Sciences
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• v.26 no.1
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• pp.111-126
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• 2009

We used an optical observation system with a 0.6m wide-field telescope and 5 computers system in KASI (Korean Astronomy and Space Science Institute) for satellite optical observation. Optical data have errors that are caused by targeting, expose start time and end-point determination. Gauss method for initial orbit determination was tested using angle-only data simulated by KODAS. And suitable time span is confirmed for result which has minimum errors. Initial orbit determination results are proved that optical observation system in KASI is possible satellite tracking for a short period. And also through differential correction, initial orbit determination results are improved.

• Journal of Advanced Navigation Technology
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• v.20 no.5
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• pp.425-432
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• 2016

When user estimates user's position, GPS positions can be obtained from the navigation message transmitted from the GPS. However, the broadcast ephemeris cannot be used in the applications required high-level accuracies because it can cause errors of several meters. To correct satellite positions and clocks, user can use RTS corrections provided by IGS. In this paper, the accuracy of broadcast and RTS corrections are analyzed by comparing with the IGS final for 3-months. The RTS errors are analyzed for each user's locations and satellite blocks. The correlations between errors and shadow condition, and solar and geomagnetic activities are analyzed. The latency is applied to the RTS corrections, and these are extrapolated by polynomial. Then, the extrapolated RTS are compared with true RTS. The single-day performances of the PPP by broadcast ephemeris and RTS corrected ephemeris are analyzed. As a result, RTS 3D orbit and clock errors are 1/20 and 1/3 less than broadcast ephemeris errors. 3D positioning error of the RTS is 1/5 less than that of broadcast ephemeris.

• Journal of the Korea Institute of Information and Communication Engineering
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• v.24 no.1
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• pp.15-21
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• 2020

In this paper, the observation performance of the electro-optical telescope system which surveils the unknown space objects, is analyzed by the Modeling & Simulation(M&S). The operation concept for the observation of the unknown space objects using two telescope systems is considered and the M&S models are constructed. Based on the operation concept for observing the unknown space objects, the estimated orbit is generated by Initial Orbit Determination(IOD) and the observation performance is analyzed according to the offset compensation cycle for the estimated orbit. The result of the M&S based analysis in this paper shows that the observation performance increases with the shorter offset compensation cycle, and decreases with the longer offset compensation cycle. Therefore, to improve the performance of the telescope system which surveils the unknown space objects, the observation system with accurate initial orbit determination or shorter offset compensation cycle should be designed and constructed.

• Journal of Astronomy and Space Sciences
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• v.5 no.1
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• pp.31-43
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• 1988

The differential correction process determining osculating orbital elements as correct as possible at a given instant of time from tracking data of artificial satellite was accomplished. Preliminary orbital elements were used as an initial value of the differential correction procedure and iterated until the residual of real observation (O) and computed observation(C) was minimized. Tracking satellite was NOAA-9 or TIROS-N series. Two types of tracking data were prediction data precomputed from mean orbital elements of TBUS and real data obtained from tracking 1.70 GHz HRPT signal of NOAA-9 using 5 meter auto-track antenna in Radio Research Laboratory. Accrding to thacking data either Gause method or Herrick-Gibbs method was applied to preliminary orbit determination. In the differential correction stage we used both of the Escobal(1975)'s analytical method and numerical method using f, g series for the comparision. The results between analytical and numerical ones are nearly consistent. And the differentially corrected orbit converged to the same value in spite of the differences between preliminary orbits of each time span.

• Aerospace Engineering and Technology
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• v.11 no.2
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• pp.80-86
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• 2012

A fast maneuvering LEO satellite producing high resolution images was developed by Korea Aerospace Research Institute and launched successfully. To achieve accurate pointing and stringent pointing stability, the attitude orbit control subsystem implements high performance star trackers and gyroscopes. In addition, series of on-orbit calibration need to be performed to compensate mainly misalignment errors due to launch shock and on-orbit thermal environment. In this paper, the on-orbit calibration approach is described with the performance enhancement result through flight data analysis.

• Proceedings of the KSRS Conference
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• 2000.04a
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• pp.131-136
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• 2000

Ocean Scanning Multi-spectral Imager (OSMI)는 다목적 실용위성 (KOMPSAT) 1호기 아리라위성에 탑재되어 1999년 12월 21일 발사된 해양 관측 기기이다. OSMI는 발사후 3년 이상 생물학적 해양지리학 연구를 위해 전세계 바다색을 관측하는 임무를 수행할 것이다. OSMI는 센서 성능의 궤도상 보정을 위해 태양광 보정과 암흑 보정을 수행한당. 태양광 보정은 궤도상에서 장기간에 걸친 해양 결상계의 노화에 따른 성능 변화 감지 및 보정에 있다. 발사 직후의 초기 태양과 보정 측정 자료는 추후 성능 변화 감지에 대한 기준이 될 뿐만아니라 발사 직후 OSMI 센서 성능 파악 및 점검에도 사용될 수 있으므로 매우 중요하다. 태양광 보정의 구조 및 광학적 특성을 분석하고 OSMI 주요 관측파 장대역별로 태양광 보정계의 출력신호량을 예측하였다. 초기 운영 기간동안 얻은 OSMI 태양광 보정계의 발사후 최초 측정 자료를 분석하고 발사전 예측 성능과 비교하였다. 이 연구는 OSMI 센서 보정 및 영상 품질 이해에 유용할 것이다.

• Information and Communications Magazine
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• v.17 no.6
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• pp.100-114
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• 2000

본 논문은 정지궤도위성을 이용한 표준시각/주파수 전송시스템의 동기 오차 요인을 분석하고, 한국과 같이 영토가 작은 국가의 경우, 정지궤도 위성을 이용하는 방식의 이점을 단파 또는 광 전용망을 이용하는 지상망 방식, 그리고 저궤도 위성을 이용하는 GPS방식과 비교 분석한다. 또한, 본 논문은 현재 서비스를 제공 중이거나 연구가 진행중인 단방향 위성 시각 전송 서비스를 고찰하고 특히, 무궁화 위성을 이용한 고정밀도의 표준시각/주파수 전 송서비스를 제공하기 위해 요구되는 동기오차 보정기술에 관하여 연구한다. 국가적 통신망 동기를 위한 표준 시각/주파수의 동기 정확도를 만족시킬 수 있는 효과적인 동기 오차 보정 방식으로 차동(differential mode)보정방식을 제안하고 그 성능을 분석하였으며 시각 정확도 와 주파수 정확도의 관계를 분석하였다. 모의실험 결과, 정상적인 시스템 운영하에서 시각 정확도와 주파수 정확도는 각각 100ns(95%)와 10-11(7일이상) 보다 우수한 것으로 분석되었 으며 본 논문에서 제시한 성능 개선 방안을 적용함으로써 보다 높은 정확도의 시각/주파수 동기가 가능함을 확인하였다.

• Proceedings of the Korean Society of Propulsion Engineers Conference
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• 2006.05a
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• pp.66-69
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• 2006

A two-dimensional Particle-In-Cell (PIC) simulation of a Hall thruster is presented. The thruster is being developed for orbit transfer and correction of a small satellite. Preliminary investigation of the simulation result finds well separated acceleration and ionization layers. The simulation further shows that collisional ionization of the xenon neutrals allows sufficient acceleration of the ionized plasmas that is adequate for the intended correction and transfer of small satellite orbits. Anticipated performance of the thruster based upon the present results will be calculated.

• Journal of the Korean Society for Aeronautical & Space Sciences
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• v.38 no.9
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• pp.875-881
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• 2010

During the lunar mission, spacecraft are subject to various unexpected disturbance sources such as third body attraction, solar pressure and operating impulsive maneuver error. Therefore, efficient trajectory correction maneuver (TCM) strategy must be required to follow the designed mission trajectory. In the early days of space exploration, the mission trajectory has been designed by using patched conic approach based on two-body dynamics for the lunar mission. Thus the TCM based on two-body dynamics has been usually adopted. However, with the advanced in computing power, the mission trajectory based on three-body dynamics is attempted recently. Thus, these approaches based on two-body dynamics are essentially different from real environment and large amount of energy for the TCM is required. In this work, we study the trajectory correction maneuver based on three-body dynamics.