• Title/Summary/Keyword: 궤도보정

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EXB 하전입자빔 에너지 필터의 광학 특성 II

  • Jo, Bok-Rae
    • Proceedings of the Korean Vacuum Society Conference
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    • 2013.08a
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    • pp.270.2-270.2
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    • 2013
  • 직선운동하는 하전입자의 진행방향에 수직한 평면상에 서로 직교하는 전기장과 자기장을 걸어주면, 하전입자에는 전기장에 의한 힘 FE와 자기장과 속도 v에 의한 로렌츠력 $F_B=q(v{\times}B)$가 동시에 작용하게 된다. 이때 Wien 조건 FB=-FE를 만족하는 질량 mA과, 에너지 EA를 가지는 하전입자 A는 휘지 않고 직선운동을 계속하나, 하전입자 A와 다른 에너지 $E_B\;(=E_A+{\delta}E)$나 질량 $m_B\;(=m_A+{\delta}m)$을 가지는 하전입자는 휘게 되며, 그 휘는 정도는 ${\delta}E$${\delta}m$에 비례하게 된다. 이 현상을 이용하여 다양한 종류의 에너지 또는 질량 분석기가 독일, 미국, 일본 등의 분석기기 선진국에서 개발되어 왔고, 전자현미경의 이미지 필터로도 활용되고 있으며, 통상 EXB 필터 또는 발명자의 이름을 딴 Wien 필터로 불리어지고 있다. $E{\times}B$ 필터는 일반적인 하전입자빔 렌즈와 다른 광학특성을 가지며, 지난 발표에서는 $E{\times}B$ 필터의 기본 궤도 방정식 및 다양한 2차 기하 수차 방정식의 유도과정 및 결과를 보여주었다. 본 발표에서는 EXB 필터의 전후에 배치시켜, 초점거리 등의 조정을 수행할 4극자와, $E{\times}B$ 필터에서 발생하는 2차 수차의 보정을 수행할 6극자의 광학특성의 계산 결과를 보여준다. 4극자-6극자-EXB필터-6극자-4극자 조합의 기본 광학궤도 계산 결과는 빔 다이어그램으로 보여준다. 6극자에 의해 수차를 줄여서 향상되는 에너지 분해능 값은 수치적으로 추정한다. 실제 제작이 된 각 부품의 외형 및 사진을 보여주어 에너지 필터의 제작 진행 상황을 보고한다.

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A Study on the DGPS Service Utilization for the Low-cost GPS Receiver Module Based on the Correction Projection Algorithm (위성배치정보와 보정정보 맵핑 알고리즘을 이용한 저가형 GPS 수신기의 DGPS 서비스 적용 방안 연구)

  • Park, Byung-Woon;Yoon, Dong-Hwan
    • Journal of Navigation and Port Research
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    • v.38 no.2
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    • pp.121-126
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    • 2014
  • This paper suggests a new algorithm to provide low-cost GPS modules with DGPS service, which corrects the error vector in the already-calculated position by projecting range corrections to position domain using the observation matrix calculated from the satellite elevation and azimuth angle in the NMEA GPGSV data. The algorithm reduced the horizontal and vertical RMS error of U-blox LEA-5H module from 1.8m/5.8m to 1.0m/1.4m during the daytime. The algorithm has advantage in improving the performance of low-cost module to that of DGPS receiver by a software update without any correction in hardware, therefore it is expected to contribute to the vitalization of the future high-precision position service infrastructure by reducing the costumer cost and vender risk.

Estimating Photosynthetically Available Radiation from Geostationary Ocean Color Imager (GOCI) Data (정지궤도 해양관측위성 (GOCI) 자료를 이용한 광합성 유효광량 추정)

  • Kim, Jihye;Yang, Hyun;Choi, Jong-Kuk;Moon, Jeong-Eon;Frouin, Robert
    • Korean Journal of Remote Sensing
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    • v.32 no.3
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    • pp.253-262
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    • 2016
  • Here, we estimated daily Photosynthetically Available Radiation (PAR) from Geostationary Ocean Colour Imager (GOCI) and compared it with daily PAR derived from polar-orbiting MODIS images. GOCI-based PAR was also validated with in-situ measurements from ocean research station, Socheongcho. GOCI PAR showed similar patterns with in-situ measurements for both the clear-sky and cloudy day, whereas MODIS PAR showed irregular patterns at cloudy conditions in some areas where PAR could not be derived due to the clouds of sunglint. GOCI PAR had shown a constant difference with the in-situ measurements, which was corrected using the in-situ measurements obtained on the days of clear-sky conditions at Socheongcho station. After the corrections, GOCI PAR showed a good agreement excepting on the days with so thick cloud that the sensor was optically saturated. This study revealed that GOCI can estimate effectively the daily PAR with its advantages of acquiring data more frequently, eight times a day at an hourly interval in daytime, than other polar orbit ocean colour satellites, which can reduce the uncertainties induced by the existence and movement of the cloud and insufficient images to map the daily PAR at the seas around Korean peninsula.

Autonomous Stationkeeping System for Geostationary Satellite (정지위성 자동위치유지 시스템에 관한 연구)

  • Park, Bong-Kyu;Tahk, Min-Jea;Bang, Hyo-Choong
    • Journal of the Korean Society for Aeronautical & Space Sciences
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    • v.32 no.10
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    • pp.67-76
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    • 2004
  • This paper improves existing 'fly-the-wire' based autonomous station-keeping system, suitable for geostationary satellite and introduces results of computer simulations conducted to verify the algorithm. The on-board stationkeeping system receives pseudo-range signals from two ground equipments located with long baseline, determines the orbit error in realtime and generates orbit control commands. To reduce fuel consumption, this paper proposes an on-board orbit control logic using modified fly-the-wire method. The modified fly-the-wire method de-couples error components into two dynamic modes, harmonic and linear motion. The harmonic error components are removed by applying output commands produced by feedback controller, and the linear motions are controlled by the correction ${\Delta}V\;s$ added to reference maneuvers. The reference maneuvers are generated through the ground based computer simulation and embedded or uploaded into the on-board computer with time tags. Finally, the performance of the proposed algorithm is verified through a series of computer simulations.

Moon Imaging for the Calibration of the COMS Meteorological Imager (천리안 위성의 기상탑재체 보정을 위한 달 영상 획득 방안)

  • Park, Bong-Kyu;Yang, Koon-Ho
    • Aerospace Engineering and Technology
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    • v.9 no.2
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    • pp.44-50
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    • 2010
  • COMS accommodates multiple payloads; Meteorological Image(MI), Ocean Color Imager(GOCI) and Ka-band communication payloads. In order to improve the quality of MI visible channel, the moon image has been taken into account as backup reference in addition to Albedo monitoring. However, obtaining the moon image by adding special mission schedule is not recommended after IOT, because we may miss chances to obtain meteorological images during the time slots for special imaging. As an alternative solution, an approach extracting moon image from MI FD(Full Disk) image has been proposed when the moon is positioned near to the earth. However, prediction of acquisition time of moon image is somewhat difficult as the moon moves while the MI is scanning type sensor. And the moon can not be seen when it is behind the earth or outside of FD field of view. This paper discusses how effectively the moon can be detected by the MI FD imaging. For that purpose, this paper describes an approach taken to predict the time when the moon image is achievable and then introduces the results obtained from computer simulation.

Analysis and application of ocean currents information extracted from SAR satellite image (SAR 위성영상 해수유동 정보추출 및 활용)

  • Lee, Moon-Jin;Kim, Hey-Jin;Lee, Seung-Hyun;Hang, Key-Yong
    • Journal of the Korean Society of Marine Environment & Safety
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    • v.13 no.4
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    • pp.21-26
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    • 2007
  • A study on analysis and application of ocean currents information extracted from SAR (Synthetic Aperture Radar) satellite image. The current information extracted from SAR satellite image is not real vector information but scalar information in normal direction of orbital path. To correct current information extracted from satellite image, observation of currents in the field is carried out at the same time and area as those of satellite image. In the analysis, current information extracted from satellite image is corrected by using observed ones. By this correction, the speed and the direction of current can be estimated. The extract current information seem to agree well with the observed ones.

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A Study on the Diffusion of Gaseous Radioactive Effluents Based on the Statistical Method (통계적 방법을 이용한 방사성 물질의 대기 확산 평가)

  • Na, Man-Gyun;Lee, Goung-Jin
    • Journal of Radiation Protection and Research
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    • v.23 no.4
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    • pp.251-257
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    • 1998
  • A diffusion model of radioactive gaseous effluents is improved to apply for domestic nuclear power plants. Up to now, XOQDOQ computer code package developed by U. S NRC has been used for the assessment of radioactive plume dispersion by normal operation of domestic nuclear power plants. XOQDOQ adopts the straight-line Gaussian plume model which was basically derived for the plane terrain. However, since there are so many mountains in Korea, the several shortcomings of XOQDOQ are improved to consider the complex terrain effects. In this work, wind direction change is considered by modifying the wind rose frequency using meteorological data of the local weather stations. In addition, an effective height correction model, a plume reduction model due to plume penetration into mountain, and a wet deposition model are adopted for more realistic assessments. The proposed methodology is implemented in Yongkwang nuclear power plants, and can be used for other domestic nuclear power plants.

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달 탐사를 위한 Hyperspectral Camera/Stereo Imager 인증 모델

  • Im, Yeo-Myeong;Min, Gyeong-Uk;Im, Tae-Ho;Choe, Yeon-Ju;Ham, Jong-Uk;Lee, Jin-Geun;Kim, Hui-Jun;Choe, Yeong-Wan;Kim, Seong-Su
    • The Bulletin of The Korean Astronomical Society
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    • v.37 no.2
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    • pp.229.2-229.2
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    • 2012
  • 지금까지 해외의 여러 달 궤도선에서 달의 영상을 다양한 방법으로 관측한 것에서 알 수 있듯이 영상 관측은 달 탐사에서 중요한 부분이다. 특히 그 중에서 입체 영사기(Stereo Imager)는 달의 3차원적 영상을 관측하여 달 표면의 구조를 파악할 수 있고 분광 카메라(Hyperspectral Camera)는 달 표면을 이루고 있는 물질을 분광 정보를 통해서 알아낼 수 있다. 본 연구에서는 우리나라가 2020년경 독자적인 달 궤도선을 계획하고 있는 것에 발맞추어 이 두 관측 장비를 설계해 보았다. 본 연구에서 설계한 탑재체는 하나의 광학계를 이용해 가시광 영역에서 동시에 입체 영상과 분광 영상을 얻을 수 있는 장치이며, 달 표면에서의 궤도선의 속도와 저장 가능한 정보의 양을 고려하여 100 km의 고도에서 속도를 1.6 km/s로 가정할 때 interline CCD가 17.5 m의 공간 분해능을 갖기 위해 92 frame/s 이상의 frame rate로 관측을 수행할 수 있게 하였다. 특히 분광 카메라는 wedge filter를 사용하여 광학계의 부담을 줄였으며 검출기로는 interline CCD를 사용하여 channel 수를 조절할 수 있도록 하였다. 또한 달 표면을 구성하는 입자의 크기에 대한 정보를 얻을 수 있는 편광판도 설치 하였다. 시험 모델의 문제점을 분석하여 새롭게 개선된 탑재체를 설계하여 개발하였다. 렌즈를 수정해 vignetting과 왜곡 현상을 보정하였고 전체 무게를 1.5 kg으로 줄여서 시험 모델보다 30% 이상 줄일 수 있었다. 파장 분해능은 20nm로 시험모델보다 더 개선된 분해능을 얻을 수 있었다. 출력 효율의 증대를 위해 power board의 수정을 수행하였다.

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Method of Differential Corrections Using GPS/Galileo Pseudorange Measurement for DGNSS RSIM (DGNSS RSIM을 위한 GPS/Galileo 의사거리 보정기법)

  • Seo, Ki-Yeol;Kim, Young-Ki;Jang, Won-Seok;Park, Sang-Hyun
    • Journal of Navigation and Port Research
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    • v.38 no.4
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    • pp.373-378
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    • 2014
  • In order to prepare for recapitalization of differential GNSS (DGNSS) reference station and integrity monitor (RSIM) due to GNSS diversification, this paper focuses on differential correction algorithm using GPS/Galileo pesudorange. The technical standards on operation and broadcast of DGNSS RSIM are described as operation of differential GPS (DGPS) RSIM for conversion of DGNSS RSIM. Usually, in order to get the differential corrections of GNSS pesudorange, the system must know the real positions of satellites and user. Therefore, for calculating the position of Galileo satellites correctly, using the equation for calculating the SV position in Galileo ICD (Interface Control Document), it estimates the SV position based on Ephemeris data obtained from user receiver, and calculates the clock offset of satellite and user receiver, system time offset between GPS and Galileo, then determines the pseudorange corrections of GPS/Galileo. Based on a platform for performance verification connected with GPS/Galileo integrated signal simulator, it compared the PRC (pseudorange correction) errors of GPS and Galileo, analyzed the position errors of DGPS, DGalileo, and DGPS/DGalileo respectively. The proposed method was evaluated according to PRC errors and position accuracy at the simulation platform. When using the DGPS/DGalileo corrections, this paper could confirm that the results met the performance requirements of the RTCM.

Sea Fog Detection Algorithm Using Visible and Near Infrared Bands (가시 밴드와 근적외 밴드를 이용한 해무 탐지 알고리즘)

  • Lee, Kyung-Hun;Kwon, Byung-Hyuk;Yoon, Hong-Joo
    • The Journal of the Korea institute of electronic communication sciences
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    • v.13 no.3
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    • pp.669-676
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    • 2018
  • The Geostationary Ocean Color Imager(: GOCI) detects the sea fog at a high horizontal resolution of $500m{\times}500m$ using the Rayleigh corrected reflectance of 8 bands. The visible and the near infrared waves strongly reflect the characteristics of the earth surface, causing errors in cloud and fog detection. A threshold of the Band7 reflectance was set to detect the sea fog entering the land. When the region on which Band4 reflectance is larger than Band8 is determinated as cloud, the error over-estimated as sea fog is corrected by comparing the average reflectance with the surrounding region. The improved algorithm has been verified by comparing the fog images of the Cheollian satellite (COMS: Communication, Ocean, and Meteorological Satellite) as well as the visibility data from the Korea Meteorological Administration.