OS23C:
Modeling of Gas Hydrate–Related Systems I


Submit an Abstract to this Session


Session ID#: 57539

Session Description:
Gas hydrates are widely distributed along the world’s continental margins and in permafrost regions. Natural gas hydrate is of great interest for its potential role in the global carbon cycle and climate change, in submarine slope stability, as a drilling hazard, and as a potential energy resource and in many other industry applications. All of these processes are highly coupled to hydrate formation and dissociation, which is a sophisticated process involving many fundamental phenomena. These phenomena include gas generation (biogenic or thermogenic); macro-scale fluid flow, bubble migration and gas transport; micro-scale hydrate nucleation, growth and dissociation; and hydraulic, petrophysical, biogeochemical and geomechanical changes in sediments over time. Modeling efforts spanning the nano-scale, pore-scale, reservoir-scale and basin-scale provide indispensable tools for better understanding these fundamental processes. We welcome any type of modeling studies, from various perspectives and spanning different spatial or time scales, which illuminate these fundamental processes in hydrate systems.
Primary Convener:  Kehua You, University of Texas at Austin, Austin, TX, United States
Conveners:  Ewa Burwicz, MARUM - University of Bremen, Bremen, Germany, Yoshihiro Konno, Department of Ocean Technology, Policy, and Environment, The University of Tokyo, Japan, Kashiwa, Japan and Michael Nole, Sandia National Labs, Albuquerque, NM, United States
Primary Liaison:  Michael Nole, Sandia National Labs, Albuquerque, NM, United States
Chairs:  Kehua You, University of Texas at Austin, Austin, TX, United States and Michael Nole, Sandia National Labs, Albuquerque, NM, United States
OSPA Liaison:  Michael Nole, Sandia National Labs, Albuquerque, NM, United States

Cross-Listed:
  • B - Biogeosciences
  • H - Hydrology
Index Terms:

3004 Gas and hydrate systems [MARINE GEOLOGY AND GEOPHYSICS]

Abstracts Submitted to this Session:

Li Wei1, Ann Cook1, Michael Nole2, Alberto Malinverno3, Hugh Daigle4, Aggeliki Georgiopoulou5, Philip Barnes6, Ingo Andreas Pecher7, Leah LeVay8, IODP Expedition 372 Scientists9 and IODP Expedition 375 Scientists9, (1)Ohio State University Main Campus, Columbus, OH, United States, (2)Sandia National Labs, Albuquerque, NM, United States, (3)Lamont -Doherty Earth Observatory of Columbia University, Palisades, NY, United States, (4)University of Texas at Austin, Hildebrand Department of Petroleum and Geosystems Engineering, Austin, TX, United States, (5)University College Dublin, Dublin, Ireland, (6)National Institute of Water & Atmospheric Research, Wellington, New Zealand, (7)University of Auckland, Auckland, New Zealand, (8)Texas A&M University, International Ocean Discovery Program, College Station, TX, United States, (9)Texas A&M University, College Station, TX, United States
Jess Irene Tsahai Hillman1, Gareth James Crutchley2 and Karsten Friedrich Kroeger2, (1)GNS Science, Lower Hutt, New Zealand, (2)GNS Science-Institute of Geological and Nuclear Sciences Ltd, Lower Hutt, New Zealand
Hugh Daigle, University of Texas at Austin, Hildebrand Department of Petroleum and Geosystems Engineering, Austin, TX, United States
Christian Stranne, Matt O'Regan and Martin Jakobsson, Stockholm University, Department of Geological Sciences, Stockholm, Sweden
Shilong Shang, Peking University, College of Engineering, Beijing, China, Hailong Lu, School of Earth and Space Sciences, Peking University, Beijing, China and Yihua Teng, Peking University, Beijing, China
Hyun Chul Yoon1, Jihoon Kim1 and Joo Yong Lee2, (1)Texas A&M University College Station, College Station, TX, United States, (2)Korea Institute of Geoscience and Mineral Resources, Deajeon, South Korea

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