• 제목/요약/키워드: Duho Formation

검색결과 14건 처리시간 0.019초

포항분지 제3기 두호층 이암의 크리프 거동 (Creep behaviour of mudstone in the tertiary Duho Formation at Pohang basin)

  • 김광식;김교원
    • 지질공학
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    • 제13권2호
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    • pp.227-238
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    • 2003
  • 암석의 점탄성적 성질에 기인하는 크리프 특성에 대한 이해는 일정하중 하에서 시간에 대한 변형으로 장기적인 지반거동을 예측할 수 있는 중요한 요소이다. 포항지역에 분포하는 제3기 두호층 이암의 크리프 특성을 파악하기 위하여 암석의 기본적인 물성, 역학적 특성 및 크리프 시험을 실시하였다. 대상 이암은 illite 및 chlorite 등 점토광물을 26% 함유하고 있어 큰 크리프 변형을 보였으며, 평균 일축압축강도는 $462{\;}kg/\textrm{cm}^2$ 이었는데, 크리프 시험은 일축압축강도의 40-70% 일정 응력수준에서 수행하였다. 시험 결과 얻어진 시간-변형률 곡선으로부터 암석의 크리프 특성을 규정하는 다양한 경험식 및 이론식의 크리프 상수를 도출하였는데, 그 중 Griggs 경험식 및 Burger 모델의 이론식이 이암의 크리프 특성을 가장 잘 반영하는 것으로 평가되었다. 또, 순간탄성변형률은 응력수준에 정비례하여 증가하였으나, 1차 크리프의 변형률 속도는 응력의 크기와 무관하게 시간 경과에 따라 비슷한 양상으로 감소하였다.

한반도의 제3기 분지와 포항분지내 지질구조 연구 (Tertiary basin in Korean peninsula and the study of geologic structure at Pohang basin)

  • 이병주
    • 한국지반공학회:학술대회논문집
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    • 한국지반공학회 2002년도 암반역학위원회 학술세미나 논문집
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    • pp.3-17
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    • 2002
  • Tertiary Pohang basin distributed in south weatern part of the korean peninsula, is composed of Chunbuk formation as the basal conglomerate, Hakjon formation, Duho formation and intrusive basalt which is 15 Ma by absolute age data. The basement of the basin is represented by Cretaceous sedimentary rocks, Hakjon welded tuff and Chilpo welded tuff and rhyolite. The fault systems at the basement of the Pohang basin are consist of NNE direction fault, WNW to EW trend fault. NNE fault is not only strike-slip fault but also normal fault. n fault has sinistral strike-slip sene and the EW fault is strike-slip and normal fault. In the Tertiary basin, the fault system is represented by nm strike-slip fault, EW normal fault and NNE thrust fault. By these fault relationships and geometries, it is interpreted that NNE sinistral strike-slip fault and nomal fault have acted at Creceous times. At Tertiary tines, NNE dextralstrike-slip fault and EW normal fault has created. Progressively Tertiary Pohang basin was influenced by the trenspression to make thrust fault and fold, namely as inversion tectonics.

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포항분지내 지각변형 해석 (Interpretation of geologic structure in Tertiary Pohang basin, Korea)

  • 이병주;송교영
    • 자원환경지질
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    • 제28권1호
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    • pp.69-77
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    • 1995
  • Tertiary Pohang basin distributed in south western part of the Korean peninsula, is composed of Chunbuk formation as the basal conglomerate, Hakjon formation, Duho formation and intrusive basalt having 15 Ma by absolute age data. The basement of the basin is represented to Cretaceous sedimentary rocks, Hakjon welded tuff and Chilpo welded tuff and rhyolite. The fault systems in the basement of Tertiary Pohang basin are consist of $N20^{\circ}E$ fault, $N60^{\circ}W$ and E-W trend. NNE fault is not only strike-slip but also normal dip-slip. WNW fault has sinistral strike-slip sense and the geometry of E-W fault is strike-slip and normal faults. In the basin, the fault system is represented to $N20^{\circ}E$ strike-slip, E-W normal and NNE thrust faults. By these fault relationship and geometry, it is interpreted that NNE sinistral strike-slip fault and N-S normal faults have acted at the Cretaceous basement. After Miocene NNE dextral strike-slip fault has acted and created E-W normal fault. Progressively Tertiary basin was influenced by the transpression to make thrust and fold, namely inversion tectonics.

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Infrared Medium-Deep Survey: Overview

  • Im, Myungshin;Pak, Soojong;Park, Won-Kee;Kim, Ji Hoon;Kim, Jae-Woo;Lee, Seong-Kook J.;Karouzos, Marios;Jeon, Yiseul;Choi, Changsu;Jun, Hyunsung;Kim, Dohyeong;Hong, Jueun;Kim, Duho;Hyun, Minhee;Yoon, Yongmin;Taak, Yoon Chan;Kim, Yongjung;Baek, Giseon;Jeong, Hyeonju;Lim, Juhee;Kim, Eunbin;Choi, Nahyun;Lee, Hye-In;Bae, K.M.;Chang, Seunghyuk
    • 천문학회보
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    • 제38권2호
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    • pp.68.1-68.1
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    • 2013
  • Infrared Medium-Deep Survey is a near-infrared imaging survey geared toward understanding the formation and the evolution of quasars and galaxies at high redshift, and studying transient and time-variable objects such as gamma-ray bursts, supernovae, and young stellar objects. The survey uses a multi-tier structure, with deep imaging survey of 100 $deg^2$ using UKIRT to the depth of 23 AB mag, and a shallower imaging of interesting sources using the CQUEAN camera on the 2.1m telescope at McDonald observatory. This talk will give an overview of the survey strategy, the instrument development, and science highlights. The science highlights will include the discovery of high redshift quasars, high redshift galaxy clusters, GRBs, and other interesting sources. At the end of the talk, we will also present the future prospects of our study.

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