• Journal of Astronomy and Space Sciences
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• 제30권4호
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• pp.255-267
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• 2013

In this research, the ground contact opportunity for the fictitious low lunar orbiter is analyzed to prepare for a future Korean lunar orbiter mission. The ground contact opportunity is basically derived from geometrical relations between the typical ground stations at the Earth, the relative positions of the Earth and Moon, and finally, the lunar orbiter itself. Both the cut-off angle and the orbiter's Line of Sight (LOS) conditions (weather orbiter is located at near or far side of the Moon seen from the Earth) are considered to determine the ground contact opportunities. Four KOMPSAT Ground Stations (KGSs) are assumed to be Korea's future Near Earth Networks (NENs) to support lunar missions, and world-wide separated Deep Space Networks (DSNs) are also included during the contact availability analysis. As a result, it is concluded that about 138 times of contact will be made between the orbiter and the Daejeon station during 27.3 days of prediction time span. If these contact times are converted into contact duration, the duration is found to be about 8.55 days, about 31.31% of 27.3 days. It is discovered that selected four KGSs cannot provide continuous tracking of the lunar orbiter, meaning that international collaboration is necessary to track Korea's future lunar orbiter effectively. Possible combinations of world-wide separated DSNs are also suggested to compensate for the lack of contact availability with only four KGSs, as with primary and backup station concepts. The provided algorithm can be easily modified to support any type of orbit around the Moon, and therefore, the presented results could aid further progress in the design field of Korea's lunar orbiter missions.

• 대한원격탐사학회:학술대회논문집
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• 대한원격탐사학회 2006년도 Proceedings of ISRS 2006 PORSEC Volume I
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• pp.398-401
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• 2006

Dual channel Radiometer for Earth and Atmospheric Monitoring (DREAM) is the main payload on Science and Technology SATellite-2 (STSAT-2) of Korea. DREAM is two-channel microwave radiometer with linear polarization, and operating at center frequencies of 23.8 GHz and 37 GHz. An equation for DREAM calibration is derived which accounts for losses and re-radiation in the microwave components of the radiometer due to physical temperature. This paper describes the radiometric calibration equation to get antenna temperature ($T_A$) from the measured output data. At lower altitude, the measured deep space temperature is contaminated by middle atmosphere and earth radiation. In this paper, we presented the detail mathematical formulation to find the altitude up to which cold source brightness temperature is not affected by earth and middle atmosphere radiation. The DREAMPFM data is used to calculate the performance parameters (linearity, sensitivity, dynamic range, and etc.) of the system.

• 한국우주과학회:학술대회논문집(한국우주과학회보)
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• 한국우주과학회 2005년도 한국우주과학회보 제14권2호
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• pp.50-50
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• 2005

• 한국지구과학회지
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• 제23권5호
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• pp.442-453
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• 2002

남극 드레이크해협 남부에서 채취한 코아퇴적물(GC 98-06)로부터 32개의 시료를 얻어 고생물학적으로 연구한 결과 총 23속 64종의 규조 미화석이 감정되었다. 산출된 규조 미화석의 군집 조성 중 Actinocyclus actinochilus, Coscinodiscus asteromphalus, Eucampia antarctica, Fragilariopsis kerguelensis, Thalassiosira lentiginosa, T. ritscheri와 T. anguste-lineata 등이 우점종으로 전체 군집의 73%를 차지한다. 공해환경을 지시해 주는 종들이 Bransfield Strait Water에 의해 유입된 해빙종들에 비해서 다량 산출되며, 제 4기 지시종과 제 3기의 마이오세와 플라이오세를 지시해주는 종들이 혼합되어 산출되는 것은, 퇴적물의 퇴적 당시 고환경이 주로 남극 순환수에 의해 운반된 남극저층수(Circumpolar deep water)에 의해 영향을 받아서 주변의 고기 퇴적물로부터 규조 화석들이 재이동 되었음을 의미한다.

• Geomechanics and Engineering
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• 제15권5호
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• pp.1061-1070
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• 2018

The main purpose of retaining wall methods for deep excavation is to keep the construction site safe from the earth pressure acting on the backfill during the construction period. Currently used retaining wall methods include the common strut method, anchor method, slurry wall method, and raker method. However, these methods have drawbacks such as reduced workspace and intrusion into private property, and thus, efforts are being made to improve them. The most advanced retaining wall method is the prestressed wale system, so far, in which a load corresponding to the earth pressure is applied to the wale by using the tension of a prestressed (PS) strand wire. This system affords advantages such as providing sufficient workspace by lengthening the strut interval and minimizing intrusion into private properties adjacent to the site. However, this system cannot control the tension of the PS strand wire, and thus, it cannot actively cope with changes in the earth pressure due to excavation. This study conducts a preliminary numerical analysis of the field applicability of the controllable prestressed wale system (CPWS) which can adjust the tension of the PS strand wire. For the analysis, back analysis was conducted through two-dimensional (2D) and three-dimensional (3D) numerical analyses based on the field measurement data of the typical strut method, and then, the field applicability of CPWS was examined by comparing the lateral deflection of the wall and adjacent ground surface settlements under the same conditions. In addition, the displacement and settlement of the wall were predicted through numerical analysis while the prestress force of CPWS was varied, and the structural stability was analysed through load tests on model specimens.

• 대한원격탐사학회지
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• 제39권5_4호
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• pp.1145-1153
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• 2023

도시 수목은 대기 중 이산화 탄소 흡수, 대기질 개선, 도시열섬 현상 완화 및 생태계서비스 제공과 같은 중요한 역할을 한다. 도시 수목을 효과적으로 관리하고 보전하기 위해서는 위치, 상태, 수종, 개체 수 등에 대한 정확한 공간 정보가 필요하다. 본 연구에서는 딥러닝 기반의 고해상도 도시 수목 면적 지도를 이용해 도시 지표면으로부터 수목을 분리하고, 국지적 최대값 필터링을 통해 수목의 위치를 정확하게 탐지하는 알고리즘을 제안한다. 도시의 다양한 생육 환경을 고려해 일률적인 필터 크기를 사용하는 대신, 수고에 따라 적절한 필터 크기를 선택해 수목 탐지 성능을 향상시켰다. 수원시 전역을 대상으로 구축한 도시 수목 위치 및 수고 정보는 도시 생태계의 지속가능한 관리와 탄소 저감 대책을 위한 기반이 될 것이다.

• 한국우주과학회:학술대회논문집(한국우주과학회보)
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• 한국우주과학회 2011년도 한국우주과학회보 제20권1호
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• pp.31.1-31.1
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• 2011

In this study, we investigated alignment state estimation performances of the three methods i.e. merit function regression (MFR), differential wavefront sampling (DWS) and Multiple Design Configuration Optimization (MDCO). The three target optical systems are 1) a two-mirror Cassegrain system for deep space Earth observation, 2) intermediate size three-mirror anastigmat for Earth ocean monitoring, and 3) extremely large segmented optical system for astronomical observation. We ran alignment state estimation simulation for several alignment perturbation cases including 1mm to 10mm in decenter and from 0.1 to 1 degree in tilt perturbation error for the two-mirror Cassegrain system. In general, we note that MDCO shows more competitive estimation performance than MFR and DWS. The computational concept, case definition and the simulation results are discussed with implications to future works.

• 한국지구과학회지
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• 제44권4호
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• pp.264-274
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• 2023

The Korea Strait comprises a continental shelf in a shallow sea that experienced glacio-eustastic sea-level changes during the Quaternary period. A long core of 76.6 m in length was acquired at the South Sea Drilling Project site (SSDP-101; 34°19.666'E and 128°16.335'N) with a 60 m water deep. The uppermost massive sand beds were interpreted as sandy sediments of the nearshore marine sand ridge in the shallow sea during the transgression of sea level, whereas the lower parts of alternating sandy and muddy beds were interpreted as deposits in marsh, estuary, and tidal flat environments. A three-layered geoacoustic model was reconstructed for the sedimentary succession in the high-resolution seismic profile based on a 140-grain size and sediment type of core SSDP-101. For the actual underwater simulation and experiments, the in-situ P-wave speeds were calculated using the sound speed ratio of the Hamilton method.

• 지구물리와물리탐사
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• 제14권1호
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• pp.18-24
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• 2011

훗카이도 남쪽 태평양 판의 심부 지각 구조를 규명하기 위해 다중채널 탄성파 반사법 탐사가 2009 년에 수행되었다. 탐사 측선은 250km 넓이의 WCR을 가로지르며, 쿠로시오 속류에 의해 생성된 난류가 흐르는 지역에 위치한다. 본 논문에서는 다중채널 탄성파 반사법 자료를 사용하여 WCR의 세부 구조를 규명하고자 하였다. 탐사 측선은 2개의 프로파일로 구성되는데, 그 중 하나는 송신원 간격이 200 미터이고, 다른 하나는 50 미터 간격이다. 밀집된 송신원을 갖는 측선의 기록자료가 성긴 송신원 측선의 기록자료보다 배정 잡음이 훨씬 많은 것을 관찰할 수 있다. 이 잡음의 발생원은 이전 송신원으로부터 발생한 해수면과 해저면, 그리고 지하 불연속면 사이의 음향 다중반향음으로 확인되었다. 음파 속도 정보가 동시에 수행하는 온도 측정으로부터 구해질 수 있다면 중합전 구조보정 기술을 통해 배정잡음에 묻혀 있는 신호를 효과적으로 강조할 수 있음을 알 수 있었다. WCR은 음향학적으로 볼 때 해양쪽으로 급경사(${\sim}2^{\circ}$)이고 해변쪽으로 완경사(${\sim}1^{\circ}$)인 오목한 반사면들의 집합체라고 할 수 있다. WCR 내부에서 30km 넓이의 반사면들로 둘러싸인렌즈 형태의 구조를 확인할 수 있었다.

• 천문학회보
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• 제41권2호
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• pp.48.2-48.2
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• 2016

The wide-field and the round-the clock operation capabilities of the KMTNet enables the discovery, astrometry and follow-up physical characterization of asteroids and comets in a most efficient way. We collectively refer to the team members, partner organizations, the dedicated software subsystem, the computing facility and research activities as Deep Ecliptic Patrol of the Southern Sky (DEEP-South). Most of the telescope time for DEEP-South is devoted to targeted photometry of Near Earth Asteroids (NEAs) to push up the number of the population with known physical properties from several percent to several dozens of percent, in the long run. We primarily adopt Johnson R-band for lightcurve study, while we employ BVI filters for taxonomic classification and detection of any possible color variations of an object at the same time. In this presentation, the progress and new findings since the last KAS meeting will be outlined. We report DEEP-South preliminary lightcurves of several dozens of NEAs obtained at three KMTNet stations during the first year runs. We also present a physical model of asteroid (5247) Krylov, the very first Non principal Axis (NPA) rotator that has been confirmed in the main belt (MB). A new asteroid taxonomic classification scheme will be introduced with an emphasis on its utility in the LSST era. The progress on the current version of automated mover detection software will also be summarized.