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3D Inversion of Aeromagnetic Data In an Area of Geumsan

금산지구 항공 자력탐사 자료의 3차원 역산

  • Ko, Kwang-Beom (Technology Innovation Team, Technology Management division, KORES) ;
  • You, Young-Jun (Technology Planning Team, Technology Management division, KORES)
  • 고광범 (한국광물자원공사 기술경영본부 선도기술팀) ;
  • 유영준 (한국광물자원공사 기술경영본부 기술기획팀)
  • Received : 2013.03.28
  • Accepted : 2014.05.15
  • Published : 2014.05.31

Abstract

3D magnetic inversion, based on the assemblage of 2D forward modeling and inversion as a practical technique to reflect the a priori information, was conducted to investigate the spatial distribution features of black-shale related and pyrometamorphic uranium deposit and several lithological units of Ogcheon Super Group in an area of Geumsan. By using the 3D visualization technique with suitable susceptibility interval and horizontal slice map, the spatial distribution of magnetic susceptibility corresponded to the black shale related uranium bearing lithological units, Black Slate member was well coincided with a information of uranium deposit. Also, even though it is indirect indicator for the detetction of uranium deposits interbedded in Gray Hornfels member, spatial susceptibility distribution which shows the south-east magnetic linearment corresponding to the Majeon-ri formation and Dark Gray Slate were matched well. From this investigation, we inferred that maximum depth extension which Black Slate member can be separately recognized with respect to adjacent Dark Gray Slate with strong magnetic susceptibility anomaly is about 150m with reference elevation level of 306m. In addition, Majeon-ri formation located south of Black Slate member revels relatively high magnetic susceptibility range but shows high spatial susceptibility fluctation. And, as an intrusive rocks, Jurassic Biotite Granite shows relatively low magnetic susceptibility characteristics. On the contrary, Cretaceous granite distributed in soutthern part of the study area shows the relatively high susceptibility distribution.

금산지역 항공 자력자료에 대하여 2차원 수치모델링 및 역산조합으로 구한 사전정보를 이용하는 3차원 자력역산을 수행하고 지질정보와 대비하여 함우라늄 층과 여타 옥천누층군 단위 암상에 대응하는 자기감수율의 공간적 분포특성을 고찰하였다. 체적당 자기감수율 분포 및 수평 슬라이스 시각화를 통해 흑색셰일형 함우라늄층인 흑색 점판암과 대응하는 자력이상 값은 우라늄 광화대와 전체적으로 양호한 상관관계를 보여주었다. 회색 혼펠스층 우라늄 광화대의 간접 지시자인 마전리층 및 암회색 점판암층 역시 석영반암 경계에서부터 동남쪽으로 발달하는 자력선구조 특성을 잘 보여주었다. 인접한 강한 자기감수율 이상을 보여주는 암회색 점판암과 분리하여 인지 가능한 함우라늄 흑색 점판암층의 최대 깊이는 고도 306m 기준으로 약 150m 안팎으로 판단하였다. 한편, 흑색 점판암층 남쪽의 마전리층은 다소 높은 자기감수율 분포를 보여주나 자기감수율의 공간적 변동이 심한 특징을 보이며 관입암인 주라기 화강암은 낮은 자기감수율 특성을 보여주는 반면, 백악기 화강암은 상대적으로 높은 자기감수율 특성을 나타내었다.

Keywords

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