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학아가벌자,립원순삼,구보전륭이,서산영일랑,상촌채,내등호유,본전사기,급천신효,전촌팔주부,김전겸태랑,Tsuruga, Kayoko,Kasahara, Junzo,Kubota, Ryuji,Nishiyama, Eiichiro,Kamimura, Aya,Naito, Yoshihiro,Honda, Fuminori,Oikawa, Nobutaka,Tamura, Yasuo,Ni Korean Society of Earth and Exploration Geophysici 2008 지구물리와 물리탐사 Vol.11 No.1
We present a method for interpreting seismic records with arrivals and waveforms having characteristics which could be generated by extremely inhomogeneous velocity structures, such as non-typical oceanic crust, decollement at subduction zones, and seamounts in oceanic regions, by comparing them with synthetic waveforms. Recent extensive refraction and wide-angle reflection surveys in oceanic regions have provided us with a huge number of high-resolution and high-quality seismic records containing characteristic arrivals and waveforms, besides first arrivals and major reflected phases such as PmP. Some characteristic waveforms, with significant later reflected phases or anomalous amplitude decay with offset distance, are difficult to interpret using only a conventional interpretation method such as the traveltime tomographic inversion method. We find the best process for investigating such characteristic phases is to use an interactive interpretation method to compare observed data with synthetic waveforms, and calculate raypaths and traveltimes. This approach enables us to construct a reasonable structural model that includes all of the major characteristics of the observed waveforms. We present results here with some actual observed examples that might be of great help in the interpretation of such problematic phases. Our approach to the analysis of waveform characteristics is endorsed as an innovative method for constructing high-resolution and high-quality crustal structure models, not only in oceanic regions, but also in the continental regions.
지각 구조 연구에서 광각 탄성파 자료를 위한 대화식 분석 방법들
등강강,립원순삼,촌뢰규,망월공광,김전의행,Fujie, Gou,Kasahara, Junzo,Murase, Kei,Mochizuki, Kimihiro,Kaneda, Yoshiyuki Korean Society of Earth and Exploration Geophysici 2008 지구물리와 물리탐사 Vol.11 No.1
The analysis of wide-angle seismic reflection and refraction data plays an important role in lithospheric-scale crustal structure study. However, it is extremely difficult to develop an appropriate velocity structure model directly from the observed data, and we have to improve the structure model step by step, because the crustal structure analysis is an intrinsically non-linear problem. There are several subjective processes in wide-angle crustal structure modelling, such as phase identification and trial-and-error forward modelling. Because these subjective processes in wide-angle data analysis reduce the uniqueness and credibility of the resultant models, it is important to reduce subjectivity in the analysis procedure. From this point of view, we describe two software tools, PASTEUP and MODELING, to be used for developing crustal structure models. PASTEUP is an interactive application that facilitates the plotting of record sections, analysis of wide-angle seismic data, and picking of phases. PASTEUP is equipped with various filters and analysis functions to enhance signal-to-noise ratio and to help phase identification. MODELING is an interactive application for editing velocity models, and ray-tracing. Synthetic traveltimes computed by the MODELING application can be directly compared with the observed waveforms in the PASTEUP application. This reduces subjectivity in crustal structure modelling because traveltime picking, which is one of the most subjective process in the crustal structure analysis, is not required. MODELING can convert an editable layered structure model into two-way traveltimes which can be compared with time-sections of Multi Channel Seismic (MCS) reflection data. Direct comparison between the structure model of wide-angle data with the reflection data will give the model more credibility. In addition, both PASTEUP and MODELING are efficient tools for handling a large dataset. These software tools help us develop more plausible lithospheric-scale structure models using wide-angle seismic data.
압전순,구보전륭이,서산영일랑,안등윤,립원순삼,급천신효,Oshida, Atsushi,Kubota, Ryuji,Nishiyama, Eiichiro,Ando, Jun,Kasahara, Junzo,Nishizawa, Azusa,Kaneda, Kentaro Korean Society of Earth and Exploration Geophysici 2008 지구물리와 물리탐사 Vol.11 No.1
지각구조 연구에서 해저면 지진계(OBS)의 위치정보는 OBS-에어건 탄성파 탐사에 있어서 매우 중요한 변수들중의 하나이다. 이 변수의 정확도을 향상시키기 위해 우리는 이용 가능한 음향 트랜스폰더에 의한 거리 정보와 함께 에어건 발파 자료와 수심 자료를 이용하여 OBS 위치를 결정하는 새로운 방법을 개발하였다. 음향 트랜스폰더로 얻은 거리 자료가 3 지점 미만의 것일 때에는 에어건 발파에 의해 발생하여 OBS에 기록된 수중 직접파의 주시가 OBS 위치 결정에 매우 중요한 정보로 활용된다. 그 새로운 방법은 두 단계로 이루어져 있다. 첫 번째 단계에서는 광역 검색이 이루어지는데 이는 수심 격자상에서 에어건 발파로부터 나온 수중 직접파의 관측 주시와 트랜스폰더 시스템을 사용하여 얻은 음향 거리로 설명할 수 있는 가장 가까운 노드를 찾는 것이다. 만약 OBS가 위치한 해저면 지형이 매우 험하다면 정밀한 2D 수심 데이터의 사용이 가장 중요하다. 국부적으로 수렴하는 최소값에 빠지지 않기 위해 첫 번째 단계에서 얻은 노드의 위치는 두 번째 단계의 초기값으로 사용된다. 두 번째 단계에서는 비선형 역산법이 수행된다. 만일 OBS의 내부 시계가 큰 편차를 보인다면 이 방법을 사용한 최종 OBS 위치와 함께 내부 시계에 대한 보정 또한 이루어져야 한다. 우리는 여기에서 OBS 위치 결정에 사용한 각 측정값의 영향과 오차에 대해서도 토론하고자 한다.