• 지구물리와물리탐사
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• 제25권1호
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• pp.1-13
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• 2022

포항분지 천부가스 탐사를 위해 육상과 해상이 연결되는 전이대에서 탄성파 탐사 방법을 제안하고 탐사를 수행하였다. 해저면 환경, 육상 탐사 환경을 고려하여 탐사를 설계하였다. 육상노드 수진기는 육상에만 설치하였고 육상에서는 바이브로사이스 음원을, 해양에서는 에어건 음원을 이용하여 자료를 취득하였다. 전이대에서 취득한 탄성파 탐사자료의 경우 육상탐사와 해상탐사 간의 정확한 연계를 위해 신중한 자료 취득과 처리 과정이 필요하다. 음원 종류에 따른 진폭과 위상변화를 고려하고, 음원위치에 따른 정적보정을 적용한 자료처리를 통해 지층단면도에서 반사파 연속성이 유지되게 하였다. 자료처리 결과 육상과 해상의 지층구조가 연결된 탄성파 지층단면도를 확보하고 포항분지 천부 가스층 탐사에 활용하고자 하였다. 전이대에서 탄성파 탐사는 천부가스뿐만 아니라 연안지역 단층대 조사에도 활용할 수 있을 것으로 기대된다.

• 한국조경학회지
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• 제27권4호
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• pp.59-64
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• 1999

This study is about gaining orientation through anchorage act of a group of ferryman. In addition, a point acquisition and character of landmark that is closely realated to a point acquisition would be clarified by studying the form of configuration of the earth and object which is used landmark for anchorage. There are 13 anchorage points in the north part of Pusan harbor. 12 anchorage points are used to anchor. A ferryman let a ship which is temporarily anchoring move safely and speedily at the anchorage point. At that time, he uses landmarks by a technique of Overlay View. Between landmarks and viewer would be formed exquisite location combination. A mountain peak, a peak of island, nature configuration of land such as intermitent rock and location, size and form of buildings or structures of a city were variously appeared as landscape elements which were used landmarks. Looking at conditions to be easily captured as a target object, 1. A particular point of a mountain ridge line which was not shield by buildings. 2. In case objects have similar form, the building which was located in the front or the highest. 3. In case of a singular object, whatever there is physical elements, that would be a target object. Through this study a configuration of the ground such as a mountain peak which is become the background of harbor landscape is very important element to find anchorage point in configuration of the ground and object. So, the continuous preservation of the contour line of mountain is needed to do safe and effective anchorage act.

• 지구물리와물리탐사
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• 제7권1호
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• pp.7-13
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• 2004

In this paper, we demonstrate that Common Mid-Point (CMP) cross-correlation gathers of multi-channel and multi-shot surface waves give accurate phase-velocity curves, and enable us to reconstruct two-dimensional (2D) velocity structures with high resolution. Data acquisition for CMP cross-correlation analysis is similar to acquisition for a 2D seismic reflection survey. Data processing seems similar to Common Depth-Point (CDP) analysis of 2D seismic reflection survey data, but differs in that the cross-correlation of the original waveform is calculated before making CMP gathers. Data processing in CMP cross-correlation analysis consists of the following four steps: First, cross-correlations are calculated for every pair of traces in each shot gather. Second, correlation traces having a common mid-point are gathered, and those traces that have equal spacing are stacked in the time domain. The resultant cross-correlation gathers resemble shot gathers and are referred to as CMP cross-correlation gathers. Third, a multi-channel analysis is applied to the CMP cross-correlation gathers for calculating phase velocities of surface waves. Finally, a 2D S-wave velocity profile is reconstructed through non-linear least squares inversion. Analyses of waveform data from numerical modelling and field observations indicate that the new method could greatly improve the accuracy and resolution of subsurface S-velocity structure, compared with conventional surface-wave methods.

• Journal of Astronomy and Space Sciences
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• 제40권4호
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• pp.237-245
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• 2023

Laser communication has been considered as a novel method for earth observation satellites with generation of high data volume. It offers faster data transmission speeds compared to conventional radio frequency (RF) communication due to the short wavelength and narrow beam divergence. However, laser beams are refracted due to atmospheric turbulence between the ground and the satellite. Refracted laser beams, upon reaching the receiver, result in angle-of-arrival (AoA) fluctuation, inducing image dancing and wavefront distortion. These phenomena hinder signal acquisition and lead to signal loss in the course of laser communication. So, precise alignment between the transmitter and receiver is essential to guarantee effective and reliable laser communication, which is achieved by pointing, acquisition, and tracking (PAT) system. In this study, we simulate the effectiveness of tip/tilt compensation for more efficient laser communication in the satellite-ground downlink. By compensating for low-order terms using tip/tilt mirror, we verify the alleviation of AoA fluctuations under both weak and strong atmospheric turbulence conditions. And the performance of tip/tilt correction is analyzed in terms of the AoA fluctuation and collected power on the detector.

• Journal of Astronomy and Space Sciences
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• 제15권1호
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• pp.183-196
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• 1998

SAR(Synthetic Aperture Radar) 영상과 수치지형표고모형(DEM: Digital Elevation Model)을 이용하여 3차원 입체영상지도를 만드는 과정이 소개된다. 영상좌표와 DEM의 지리적 좌표 계를 이어주기 위해서는 그 연결고리로써 위성의 궤도결정과 자세결정의 방법을 이용하여 영상신호 취득 기하를 정밀하게 모형 화하는 작업이 요구된다. 이를 위해 사례연구 대상으로 삼은 RADARSAT의 궤도결정과 자세결정을 수행하였다. 궤도결정을 위해서는 영상신호 취득 시 관측된 영도 플러(zero Doppler) 경사거리를 이용하며, 자세결정을 위해서는 도플러 중심주파수(Doppler centriod)를 이용한다. 엄밀한 영상신호 취득기하를 확립함으로써 위성중심의 정밀한 영상 자리 매김 과정이 소개된다. 기존의 영상자리 매김이 순방향(영상좌표 계에서 지리적 좌표 계)으로 이루어진 것과는 반대로 영상 내에 지형 보정을 동시에 실시하기 위해서 DEM을 이용하여 역 방향(지리적 좌표 계에서 영상좌표 계)으로 수행하였다. 위성과 지상목표물간의 운동은 지구중심 관성좌표 계에서 기술된다.

• 지구물리와물리탐사
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• 제21권1호
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• pp.41-53
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• 2018

전통적인 탄성파 탐사 자료처리 분야에서 겹반사파(multiple)는 잡음으로 취급되어 제거한 후 자료처리를 수행한다. 그러나 최근 겹반사파를 잡음이 아닌 하나의 신호로 인식하고 이를 영상화에 이용하는 연구가 많이 이루어지고 있다. 겹반사파는 일차 반사파(primary reflection)가 도달하지 못하는 지점까지 도달할 수 있어 적은 수의 송신원과 수신기로도 더 넓은 범위를 영상화 할 수 있다. 이를 검증하기 위해 본 연구에서는 영상화 기법 중 하나인 거꿀시간 참반사 보정(reverse-time migration)을 이용하여 겹반사파 자료를 영상화한 후 일차 반사파를 사용한 전통적인 거꿀시간 참반사 보정 결과와 비교하였다. 겹반사파를 독립적으로 사용하기 위해 자유면 기인 겹반사파 제거(surface-related multiple elimination; SRME)기법을 사용해 탄성파 자료에서 겹반사파를 분리하였다. 수치 예제를 통해 겹반사파를 이용한 참반사 보정 결과가 일차 반사파를 이용한 전통적인 참반사 보정 결과보다 더 넓은 범위를 영상화 할 수 있음을 확인하였고, 특히 천부 지층에서 두드러진 효과가 나타나는 것을 알 수 있었다. 또한 겹반사파를 이용한 참반사 보정은 자료취득 흔적(acquisition footprint)에 의한 영상 왜곡이 제거됨을 확인할 수 있었다.

• 한국광물학회지
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• 제29권2호
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• pp.73-78
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• 2016

점토 광물의 구조 내에 들어 있는 철의 산화수는 퇴적환경의 산화/환원 조건에 대한 정보를 제공하여 준다. 이러한 광물형성의 메커니즘을 밝히기 위해서는 고해상도를 가진 전자현미경을 이용한 나노 스케일 분석이 불가피하다. 투과전자현미경에 장착되어있는 전자에너지 손실분광 분석법(EELS)을 이용하여 정량적 철 산화수 분석을 논트로나이트 점토광물 구조 내 철의 환원으로 인한 K-논트로나이트의 형성의 예를 들어 설명하고자 한다. 철 산화/환원의 정량적 분석을 통하여 퇴적물의 위치에 따른 철 산화도 측정은 광물변화에 대한 연구를 용이하게 해준다. 따라서 본 논문은 전자에너지 손실분광의 분석방법 및 장점을 소개함을 목적으로 한다.

• 천문학회지
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• 제38권4호
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• pp.445-462
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• 2005

In a companion paper, we have presented so-called Spatio-Spectral Maximum Entropy Method (SSMEM) particularly designed for Fourier-Transform imaging over a wide spectral range. The SSMEM allows simultaneous acquisition of both spectral and spatial information and we consider it most suitable for imaging spectroscopy of solar microwave emission. In this paper, we run the SSMEM for a realistic model of solar microwave radiation and a model array resembling the Owens Valley Solar Array in order to identify and resolve possible issues in the application of the SSMEM to solar microwave imaging spectroscopy. We mainly concern ourselves with issues as to how the frequency dependent noise in the data and frequency-dependent variations of source size and background flux will affect the result of imaging spectroscopy under the SSMEM. We also test the capability of the SSMEM against other conventional techniques, CLEAN and MEM.

• 천문학회지
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• 제39권2호
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• pp.51-56
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• 2006

We report the development of a semi-VLBI observation system operating at 21 cm and present the measurement of visibility function toward the sun using this system. The system consists of two 2.3 meter antennas with a maximum separation of 35 meter, a conventional high speed data acquisition system, and a set of programs for software correlation. Since two local oscillators of receiver modules are independent, data had to be fringe-fitted to yield the visibility amplitude. It is found that the visibility amplitude decreases and then bounces back as baseline increases. We confirm that solar disk with brighter limb best explains the measured visibility amplitude.

• 천문학회보
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• 제36권2호
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• pp.93.2-93.2
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• 2011

Japan Aerospace Exploration Agency (JAXA) has measured space environment and its effects on spacecraft and astronaut since 1987. At present, we have operated space environment monitors onboard one GEO spacecraft, one QZO spacecraft, and two LEO spacecrafts. The obtained space environment data has been gathered into the Space Environment and Effects System database (SEES, http://sees.tksc.jaxa.jp/). In this presentation, measurement result of space environment in low earth orbit obtained by the Daichi satellite from 2006 through 2011 is reported as well as recent activities in space environment engineerings in JAXA. The Technical Data Acquisition Equipment (TEDA) on board the Daichi satellite (Advanced Land Observing Satellite: ALOS) had been operated in low earth orbit at 700 km altitude with 98 degree inclination from February 2006 until April 2011. The TEDA consists of the Light Particle Telescope and the Heavy Ion Telescope. The operation period of the Daichi satellite was through the solar-activity minimum period. The space radiation environment around the Daichi satellite had been almost stable. However, large solar flares followed by CMEs sometimes disturbed the space radiation environment in the orbit of the Daichi satellite. In addition, high speed solar wind often flowed and modulated the electron flux in the horn region. On the other hand, a little variation was seen in the SAA region.