Abstract

Natural gas hydrates (GHs) filling sand layer pores are the most promising GHs that can be produced via conventional mechanisms in deep-sea environments. However, the seismic tracking of such thin GH-bearing sand layers is subject to certain limitations. For example, because most GH-bearing sand layers are thin and sparsely interbedded with mud layers, conventional seismic data with a maximum resolution of ~10 m are of limited use for describing their spatial distribution. The 2010 Ulleung Basin drilling expedition identified a relatively good GH reservoir at the UBGH2-6 site. However, the individual GH-bearing sand layers at this site are thin and cannot therefore be reliably tracked using conventional seismic techniques. This study presents a new thin layer tracking method using stepwise seismic inversion and 3D seismic datasets with two different resolutions. The high-resolution acoustic impedance volume obtained is then used to trace thin layers that cannot be harnessed with conventional methods. Moreover, we estimate the high-resolution regional GH distribution based on GH saturation derived from acoustic impedance at UBGH2-6. The thin GH layers, previously viewed as a single layer because of limited resolution, are further subdivided, traced, and characterized in terms of lateral variation.

Highlights

  • IntroductionPublisher’s Note: MDPI stays neutral with regard to jurisdictional claims in published maps and institutional affiliations

  • To overcome the low-resolution problem, the present study proposes a new method of generating high-resolution acoustic impedance volume by performing stepwise seismic inversion using well-log data and two 3D seismic datasets acquired from sources with different frequency ranges

  • If the high-resolution impedance volume can be derived from the data, the uncertainty owing to resolution limitations can be reduced

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Summary

Introduction

Publisher’s Note: MDPI stays neutral with regard to jurisdictional claims in published maps and institutional affiliations. Gas hydrates (GHs) are solid clathrates consisting of water and hydrocarbon gas (mainly methane). Natural GHs form in permafrost regions or in deep (≥500 m) marine environments offering adequate temperature, pressure, and gas concentration conditions [1]. Interest in natural GHs has increased in recent decades because of their potential as a future energy source, the possibility of related submarine geohazards, and their impact on global climate change [2,3,4,5]

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