• 제어로봇시스템학회:학술대회논문집
• /
• 제어로봇시스템학회 1991년도 한국자동제어학술회의논문집(국제학술편); KOEX, Seoul; 22-24 Oct. 1991
• /
• pp.1649-1654
• /
• 1991

In 1995 the VSOP satellite, which is called MUSES-B in Japan, will be launched under the VLBI Space Observatory Programme(VSOP) promoted by ISAS(Institute of Space and Astronautical Science) of Japan. We are now developing the GPS Receiver(GPSR) and On-board Orbit Determination System. This paper describes the GPS(Global Positioning System), VSOP, GPSR(GPS Receiver system) configuration and the results of the GPS system analysis. The GPSR consists of three GPS antennas and 5 channel receiver package. In the receiver package, there are two 16 bits microprocessing units. The power consumption is 25 Watts in average and the weight is 8.5 kg. Three GPS antennas on board enable GPSR to receive GPS signals from any NAVSTARs(GPS satellites) which are visible. NAVSATR's visibility is described as follows. The VSOP satellite flies from 1, 000 km to 20, 000 km in height on the elliptical orbit around the earth. On the other hand, the orbit of NAVSTARs are nearly circular and about 20, 000 km in height. GPSR can't receive the GPS signals near the apogee, because NAVSTARs transmit the GPS signals through the NAVSTAR's narrow beam antennas directed toward the earth. However near the perigee, GPSR can receive from 12 to 15 GPS signals. More than 4 GPS signals can be received for 40 minutes, which are related to GDOP(Geometric Dillusion Of Precision of selected NAVSTARs). Because there are a lot of visible NAVSTARs, GDOP is small near the perigee. This is a favorqble condition for GPSR. Orbit determination system onboard VSOP satellite consists of a Kalman filter and a precise orbit propagator. Near the perigee, the Kalman filter can eliminate the orbit propagation error using the observed data by GPSR. Except a perigee, precise onboard orbit propagator propagates the orbit, taking into account accelerations such as gravities of the earth, the sun, the moon, and other acceleration caused by the solar pressure. But there remain some amount of calculation and integration errors. When VSOP satellite returns to the perigee, the Kalman filter eliminates the error of the orbit determined by the propagator. After the error is eliminated, VSOP satellite flies out towards an apogee again. The analysis of the orbit determination is performed by the covariance analysis method. Number of the states of the onboard filter is 8. As for a true model, we assume that it is based on the actual error dynamics that include the Selective Availability of GPS called 'SA', having 17 states. Analytical results for position and velocity are tabulated and illustrated, in the sequel. These show that the position and the velocity error are about 40 m and 0.008 m/sec at the perigee, and are about 110 m and 0.012 m/sec at the apogee, respectively.

• 대한원격탐사학회:학술대회논문집
• /
• 대한원격탐사학회 1999년도 Proceedings of International Symposium on Remote Sensing
• /
• pp.485-490
• /
• 1999

Wind vector information over the ocean is currently obtained using multiple beam scatterometer data. The scatterometers on ERS-1/2 generate wind vector information with a spatial resolution of 50km and accuracies of $\pm$2m/s in wind speed and $\pm$20$^{\circ}$ in wind direction. Synthetic aperture radar (SAR) data over the ocean have the potential of providing wind vector information independent of weather conditions with finer resolution. Finer resolution wind vector information can often be useful particularly in coastal regions where the scatterometer wind information is often corrupted because of the lower resolution system characteristics which is often contaminated by the signal returns from the coastal areas or ice in the case of arctic environments. In this paper we tested CMOD_4 and CMOD_IFR2 algorithms for extracting the wind vector from SAR data. These algorithms require precise estimation of normalized radar cross-section and wind direction from the SAR data and the local incidence angle. The CMOD series algorithms were developed for the C-band, VV-Polarized SAR data, typically for the ERS SAR data. Since RADARSAT operates at the same C-band but with HH-Polarization, the CMOD series algorithms should not be used directly. As a preliminary approach of resolving with this problem, we applied the polarization ratio between the HH and VV polarizations in the wind vectors estimation. Two test areas, one in front of Inchon and several sites around Jeju island were selected and investigated for wind vector estimation. The new results were compared with the wind vectors obtained from CMOD algorithms. The wind vector results agree well with the observed wind speed data. However the estimation of wind direction agree with the observed wind direction only when the wind speed is greater than approximately 3.0m/s.

• 한국농림기상학회지
• /
• 제7권1호
• /
• pp.98-106
• /
• 2005

지하수는 복잡 경관에 위치한 광릉 산림 소유역의 물과 탄소 순환에 중요한 역할을 담당한다. 지하수가 지하 매질의 전기비저항(ER)에 크게 영향을 미치기 때문에, ER을 사용하여 지하수의 깊이와 지하 수분 함량을 조사할 수 있다. 따라서 최근 전기비저항 탐사를 통해 토양수분과 지하수 함양률, 수위변동을 측정하는 연구가 진행되고 있다. 정량적으로 적용할 수 있는 연구 결과가 나온다면 전기비저항 탐사가 다양한 시간과 공간규모의 물 수지의 닫힘을 확인하는 데에 중요한 기여를 할 수 있을 것으로 기대된다. 본 논문에서는 광릉 산림 소유역에서 지하수의 역할을 규명하기 위해 설치될 지하수 관정의 정확한 깊이와 위치를 파악하고자 실시한 ER 현지 조사의 예비 결과를 제시하였다 앞으로의 연구는 유용성이 입증된 전기비저항 탐사와 더불어 GPR 탐사, 전자탐사, 탄성파 탐사 등의 복합 물리탐사와 GIS를 이용한 분석을 통해 더 정확한 지하구조의 정보와 지하수공 최적의 위치를 추정할 수 있을 것으로 보인다.

• 한국지구과학회지
• /
• 제27권1호
• /
• pp.20-31
• /
• 2006

본 연구에서는 초등학교 과학교과서 지구과학 부문에 대한 예비교사들의 질문을 분석하였다. 주요 질문의 대상이 된 교과 내용은 교과서 단원별로 쪽 당 평균 질문수의 3배 이상이 나온 교과서 쪽의 내용(주요 질문 교과 내용1)과 2배 이상 3배 미만의 질문수가 나온 내용(주요 질문 교과 내용2)으로 구별하고, 각 교과 내용별로 질문 속에 나타나는 주요 용어들 간 상호관련성을 분석한 결과는 다음과 같다. 첫째, 주요 질문 교과 내용1은 ‘구름관찰’, 지층의 생성 과정‘ 등이 발견되었고, 주요 질문 교과 내용2는 ’강수량 측정‘, ’하룻밤 동안 달의 이동‘ 등으로 4-2학기를 제외한 모든 학기에서 발견되었다. 둘째, 각 교과 내용 당 질문용어의 상호관련성을 보이는 경우는 질문수가 많은 주요 질문 교과내용에서 증가하고 있지만, 4개 용어 유형은 오히려 교과 내용2에서 다수 발견되었다. 셋째, 상호관련성이 큰 질문 용어 묶음은 교과내용1에서 ’석탄과 석유-생성‘, ’변성-열과 압력‘, ’변성-열과 압력-변성암‘, ’행성-태양-혜성-공전‘ 등이며, 교과내용2에서는 ’별자리판-사용‘, ’건습구습도계-원리‘, ’건습구습도계-원리-습도‘, ’지진계-원리-습도‘, ’지진계-원리-지진‘, ’지구자전축-기울어짐-발생‘, ’별자리판-별자리-관찰-사용‘ 등이다. 본 연구에서 분석 자료로 사용된 질문의 원천은 대체로 교과서의 구체적인 구성체제로부터 비롯된 것이거나 지구과학내용에 대한 예비교사들의 일반적인 의문점에서 비롯된 것으로 판단된다. 전자의 경우라면 교과서의 집필과정에서 문장의 서술방법이나 관련 삽화 등의 문제점에서 유발된 것일 가능성이 크기 때문에 교과서 집필상의 문제점을 개선함으로서 해결 가능하지만, 후자는 소양교육 내용과 기초 지구과학개념으로서의 초등학교 교육과정에 대한 재고가 필요하다.

• 한국환경보건학회지
• /
• 제30권5호
• /
• pp.410-416
• /
• 2004

The objective of this investigation was to evaluate applicability of precoat filtration that can be substituted for rapid sand filter of conventional water treatment system(CWTS). Precoat filter used in this experiment are candle filter. Element disk of candle are pore size $10{\mu}m(R),\;20{\mu}m(B)$ And diatomaceous earth are cake pore size $3.5{\mu}m$(Standard Super- Cel; A), $7{\mu}m$(Hyflo Super-Cel; B) and $17{\mu}m$(Celite 545RV; C). $2kg/m^2$ diatomaceous earth is used for precoating, it coated candle in $5{\sim}6mm$ thickness. 1. Al adsorption dosages by diatomaceous earth used in experimental we Hyflo Super-Cel 0.843mg/g, Standard Super-Cel 0.782 mg/g and Celite 545RV 0.766 mg/g. 2. Filtrate of precoat filter during 60min are R-C combination 20.7($m^3/m^2$)>B-C 18.3($m^3/m^2$)>B-B 15.0($m^3/m^2$)> R-B 12.9($m^3/m^2$)> R-A 11,093($l/m^2$). 3. Water quality of precoat filter effluent are thus. $KMnO_4$ consumption are $1.10{\sim}2.20mg/l$, removal rate are $30.9{\sim}65.6\%$. They are R-A 1.10(mg/l)(removal rate $65.6\%$). R-C(2.20 mg/l)(removal rate $30.9\%$). 4. $Al^{3+}$ are not detected with all combination, removal rate $100\%$. 5. Considering water quality and flux, continued running time of R-A combination is 7 hr. Accumulated filtrate are $74.4 m^3/m^2$, average flux is $177.2 l/m^2{\cdot}min$. And filtrate per diatomaceous earth 1g are 37.2 l. 6. R-A effluent's water quality are $KMnO_4$ Consumption 1.10(mg/l), DOC 1.161 mg/1, Al 0.0 mg/1, $UV_{254}$ 0.016/cm, Turbidity 0.1(NTU). R-A combination is suitable to precoat filtration for the settling basin effluent treatment.

• 한국대기환경학회지
• /
• 제23권3호
• /
• pp.353-363
• /
• 2007

To differentiate temperature effect from the light intensity effect on the formation of secondary products during the photooxidation of toluene-$NO_x$-air mixtures, steady-state air temperature was changed from $20^{\circ}C\;to\;33^{\circ}C$ at the same light intensity of $0.39min^{-1}$ in an indoor smog chamber. Smog chamber consisted of 64 blacklights and a $5.8m^3$ reaction bag made of Teflon film. Air temperature was controlled by an air-conditioning system. The starting time for rapid conversion of NO to $NO_2$ was slightly delayed with decreasing air temperature. In contrast to light intensity effect, the ozone formation time and the ozone production rate were insensitive to air temperature. Although the formation time for secondary organic aerosols was not changed, the particle number concentration increased with temperature. However, the newly formed secondary organic aerosol mass at lower temperature was higher than that at higher temperature. Since light intensity significantly affected the starting time and quantity of ozone and aerosol formation, it is considered that the temperature could contribute partly the quantity of aerosol formation during the photooxidation of toluene-$NO_x$-air mixtures.

• 한국전자파학회논문지
• /
• 제29권9호
• /
• pp.722-730
• /
• 2018

본 논문에서는 FMCW(frequency modulated continuous wave) 신호기반 SAR 시스템의 스퀸트 각도(squint angle) 설정에 따른 복원영상 내 목표물 분산전력패턴 변화를 예측하기 위한 분석기법에 대해 설명한다. SAR 복원영상 내 목표물 분산 전력패턴은 지면에 투영된 전파진행방향과 합성개구면과 스퀸트 각도가 이루는 방위방향에 따라 일정한 방향으로 변형된 특성을 갖게 되며, 이와 같은 특성변화를 3차원 SAR 기하구조 내에서 분석한다. 스퀸트 설정각도에 따라 변형된 목표물 분산전력패턴은 FMCW 신호모델과 back-projection 알고리즘을 기반으로 한 모의실험을 통해 그 분석결과를 검증한다. 또한, 변형된 분산전력패턴의 예측결과는 SAR 기하구조와 스퀸트 설정각도를 변수로 정리된다.

• 천문학회보
• /
• 제44권1호
• /
• pp.63.1-63.1
• /
• 2019

Solar system small bodies are unusual objects in astronomical survey data in that they are moving on the celestial sphere. In addition, even in a normal status, their magnitudes are changing over time, firstly because their relative positions with respect to the Sun and Earth are continually changing, secondly because they are rotating bodies with non-spherical shapes. Furthermore, some of them might exhibit unexpected activities, which could be caused by mass ejection or disintegration. Detections and observations of such activities are challenging due to their abrupt nature. Therefore, continuous monitoring observations of large number of Solar system small bodies are required to systematically obtain detailed/transient information about them. Since 2018/2019 winter, we have launched a new project using Korea Microlensing Telescope Network (KMTNet) for detecting such transient phenomena of Solar system objects. Our main goal is to monitor the magnitudes and detect sudden brightness changes. We also plan to discover interesting new objects, and monitor rotational brightness oscillations of asteroids. We intend to monitor the magnitudes of ~ 20,000 known Solar system small bodies per night, and acquire lightcurves of ~ 1,000 asteroids.

• 대한원격탐사학회:학술대회논문집
• /
• 대한원격탐사학회 1999년도 Proceedings of International Symposium on Remote Sensing
• /
• pp.148-153
• /
• 1999

Baikdu-san was a very active volcano during the Cenozoic era and is believed to be formed in late Cenozoic era. Recently it was also reported that there was a major eruption in or around 1002 A.D. and there are evidences which indicate that it is still an active volcano and a potential volcanic hazard. Remote sensing techniques have been widely used to monitor various natural hazards, including volcanic hazards. However, during an active volcanic eruption, volcanic ash can basically cover the sky and often blocks the solar radiation preventing any use of optical sensors. Synthetic aperture radar(SAR) is an ideal tool to monitor the volcanic activities and lava flows, because the wavelength of the microwave signal is considerably longer that the average volcanic ash particle size. In this study we have utilized several sets of SAR data to evaluate the utility of the space-borne SAR system. The data sets include JERS-1(L-band) SAR, and RADARSAT(C-band) data which included both standard mode and the ScanSAR mode data sets. We also utilized several sets of auxiliary data such as local geological maps and JERS-1 OPS data. The routine preprocessing and image processing steps were applied to these data sets before any attempts of classifying and mapping surface geological features. Although we computed sigma nought ($\sigma$$^{0}$) values far the standard mode RADARSAT data, the utility of sigma nought image was minimal in this study. Application of various types of classification algorithms to identify and map several stages of volcanic flows was not very successful. Although this research is still in progress, the following preliminary conclusions could be made: (1) sigma nought (RADARSAT standard mode data) and DN (JERS-1 SAR and RADARSAT ScanSAR data) have limited usefulness for distinguishing early basalt lava flows from late trachyte flows or later trachyte flows from the old basement granitic rocks around Baikdu-san volcano, (2) surface geological structure features such as several faults and volcanic lava flow channels can easily be identified and mapped, and (3) routine application of unsupervised classification methods cannot be used for mapping any types of surface lava flow patterns.

• 한국컴퓨터정보학회논문지
• /
• 제20권3호
• /
• pp.57-67
• /
• 2015

본 논문에서는 적외선 영상에서 탐지된 표적의 픽셀정보를 이용하여 실제 환경에서의 표적의 위치를 추정하는 geolocation 기법에 대하여 제안한다. 제안하는 기법은 지대지 전장 환경에서 공중 정찰을 통한 적대 표적의 위치를 파악하는 시스템에 적용이 가능하다. 적대 표적의 geolocation에 영향을 주는 요소는, 시스템의 광학적 왜곡, 지형적 왜곡, 정찰 모듈의 GPS(Global Positioning System) 및 IMU(Inertial Measurement Unit) 왜곡을 들 수 있다. 본 논문에서는 광학적 왜곡과 지형적 왜곡에 적응적인 geolocation 을 위하여 광학 정보의 다항식 최적화와 지구 곡률을 고려한 시선거리 계산 기법을 적용하였으며, 3차원 모의 환경에서 실험한 결과 시스템 요구사항 내에서 geolocation의 정확도를 만족함을 확인하였다.