• 지구물리와물리탐사
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• 제8권1호
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• pp.73-77
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• 2005

전도성 지질에서 얻어진 지표 핵자기 공명(SNMR) 자료를 올바르게 역산하고 해석하기 위해서는 기하의 전기전도도 분포에 대한 정확한 추정이 필요하다. 이러한 추정 결과는 SNMR 수직탐사를 수행하기 이전에 전도도 구조가 지하수 탐지를 방해할 것인지에 대해 결정하는데 유용할 것이다 이 논문에서는 SNMR 모델링을 이용하여 지하 전기전도도 구조가 주어졌을 때, 대부분의 SNMR 신호를 발생하는 심도 범위를 결정하는 방법을 서술하였다. 이 논문에서는 반무한 공간에서 SNMR침투 심도를 추정하는 방법을 사용하였으며 전도성 반무한 공간(<10 ohm-m)에서는 침투심도가 50 m 이내라는 것을 보였다. 또한 이러한 반an한 공간 모델에서는 동일위치 방식의 loop 크기를 늘리더라도 침투심도를 뚜렷이 증가시키지 못함도 알 수 있었다. 이러한 결과는 좀 더 복잡한 1 차원 전도도 구조에 대한 반무한 공간 근사를 통해 전도성 지층에서 신호가 얻어질 수 있는 심도 범위를 합리적으로 추정하는데 사용될 수 있을 것이다.

• 한국지구물리탐사학회:학술대회논문집
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• 한국지구물리탐사학회 2009년도 특별 심포지엄
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• pp.73-87
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• 2009

Geophysical survey for unconformity-type uranium deposit applied to this study area in Athabaska Basin, Canada were carried out airborne TEM and magnetic, resistivity-induced polarization (DC-IP), puser seismic reflection and well-logging method. The results of airborne survey interpreted the lithological boundary, geological structures, and conductors. Also, these results decided to main targets for ground DC-IP survey. The Low resistivity and the high chargeability slices of 3D modeling interpreted from DC-IP survey response for conductors related to hydrothermal alteration zones and fault-controlled graphitic zones occurring at the unconformity-type uranium deposit, and they confirmed by diamond drilling. Seismic results interpreted to lake bottom surface, alluvium layer and intra-sandstone faults. We suggest the resonable field data acquisition of DC-IP method on the land or the lake in Athabaska Basin.

• 지구물리와물리탐사
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• 제7권1호
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• pp.33-40
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• 2004

Numerical and laboratory studies have been conducted to test the ability of Electrical Resistance Tomography-a technique used to map the electrical resistivity of the subsurface-to delineate contaminant plumes. Two-dimensional numerical models were created to investigate survey design and resolution. Optimal survey design consisted of both downhole and surface electrode sites. Resolution models revealed that while the bulk fluid flow could be outlined, small-scale fingering effects could not be delineated. Laboratory experiments were conducted in a narrow glass tank to validate theoretical models. A visual comparison of fluid flow with ERT images also showed that, while the bulk fluid flow could be seen in most instances, fine-scale effects were indeterminate.

• 건축역사연구
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• 제24권5호
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• pp.49-58
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• 2015

The purpose of this study is to analyze the overall condition of the foundation for the three storied stone pagoda of Bulguksa temple in GyeongJu. As a research method, exploration of the electrical resistivity, refraction seismic, surface wave exploration, GPR exploration, Reputation loading test. The results of the investigation, the range of the foundation was formed in foundation stone outskirts of 1.5 ~ 2.0m. It was confirmed to be about 2.0m depth. The depth of the foundation becomes shallower from the base portion to the outside. And the bearing capacity of foundation was sufficient conditions to weight. It can sufficiently support the weight of pagoda. And, the result of this investigation becomes basis data for repair work.

• 한국건축시공학회:학술대회논문집
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• 한국건축시공학회 2022년도 봄 학술논문 발표대회
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• pp.103-104
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• 2022

Cracks may occur in reinforced concrete (RC) structures due to various physical and chemical factors, and the growth of cracks causes deterioration of the structure's performance. It is important to prevent the expansion of cracks through periodic diagnosis of cracks in structures. In order to enable free crack exploration even in a narrow space, a construction robot using a Mecanum wheel that can move up, down, left and right and rotate in place was designed. High-quality crack images were periodically collected through the camera, and the image fragments stored during the exploration were combined into a single photo after the exploration was completed. The robot detected cracks with a width of 0.2 mm or more on the concrete probe surface with an accuracy of about 90% or more.

• 한국지반공학회:학술대회논문집
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• 한국지반공학회 1996년도 가을 학술발표회 논문집
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• pp.209-218
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• 1996

• 한국우주과학회:학술대회논문집(한국우주과학회보)
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• 한국우주과학회 2009년도 한국우주과학회보 제18권1호
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• pp.37.1-37.1
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• 2009

• 지구물리와물리탐사
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• 제16권4호
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• pp.203-210
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• 2013

화천 시추공 지진관측소의 부지특성을 살펴보기 위해 지표와 시추공 자료에 기록된 배경잡음과 지진신호의 특성을 분석하였다. 배경잡음을 분석한 결과, 비교적 잡음유입이 적은 밤 시간대에 비하여 낮 시간대에서 지표/시추공 잡음에너지 비가 약 15배 높게 나타났으며, 저주파에서 고주파로 갈수록 지표/시추공 스펙트럼 비가 크게 나타났다. 지진신호에 대해서는 P파와 SH파의 우세주파수 양상을 비교하였는데, 진앙거리가 가깝고, 규모가 작은 국내지진은 지표자료에서 8 Hz와 46 Hz에서 우세주파수를 보이며 시추공 자료와 다른 값을 나타내었다. 이는 수평/수직 스펙트럼 비 분석으로 구한 퇴적층의 공명주파수(7.4 Hz, 46 Hz)와 일치하며 상부 퇴적층에 영향을 받아 증폭현상이 나타나고 있음을 시사한다. 이번 연구를 통해 지표 관측소에 비하여 시추공 관측소에서는 배경잡음이 최대 20,000배 이상 감소되고, 상부퇴적층에 의한 증폭현상이 나타나지 않아 양질의 자료를 획득하여 지진관측능력이 향상될 수 있음을 알 수 있었다.

• Journal of Astronomy and Space Sciences
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• 제40권4호
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• pp.131-148
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• 2023

Lunar permanently shadowed regions (PSRs) never see direct sunlight and are illuminated only by secondary illumination - light reflected from nearby topography. The ShadowCam imaging experiment onboard the Korea Pathfinder Lunar Orbiter is acquiring images of these PSRs. We characterize and discuss the nature of secondary illumination for the Shackleton PSR from ShadowCam radiance-calibrated images. We also use modeling to understand the magnitude and direction of the secondary illumination. Results from our analysis highlight the non-homogeneous, dynamic, and complex nature of PSR secondary lighting. Knowledge of the direction of the secondary illumination is crucial for reli-able interpretation of contrasts observed in ShadowCam images. This preliminary analysis of the floor of Shackleton crater from images acquired over multiple secondary illumination conditions does not reveal indications of exposed surface ice, even though temperatures are constantly below 110K.

• 천문학회보
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• 제43권1호
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• pp.32.1-32.1
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• 2018

Searching for low surface brightness (LSB) dwarf galaxies in low density environments (isolated and group) can help us resolve the discrepancy between observation and theory known as the 'missing satellite' problem. They are also important to study the evolution of low mass galaxies in these environments. Although the number of dwarfs in such environments is rapidly increasing in many recent studies, it is still not easy to characterize their general properties. Motivated by this, we present preliminary results of our search for LSB dwarf galaxies around 60 nearby galaxies (D<50Mpc) using deep optical images. Imaging data from Maidanak Astronomical Observatory (MAO) in Uzbekistan as a part of Intensive Monitoring Survey of Nearby Galaxies (IMSNG; Im in prep.) and other archival data are used to find previously unknown LSB dwarf galaxies. Extended LSB sources (central surface brightness ${\mu}_0$ > $23mag/arcsec^2$) are first selected in the ${\mu}_0$ - magnitude plane (Rines & Geller 2008). The dwarf galaxy candidates are chosen by visual inspection. We discuss whether these candidates are actual satellite galaxies, by measuring the projected number densities in group environments and in the field. Also, their structural and photometric properties are compared with those of previously discovered dwarf galaxies in the literature.