Gas hydrate stability zone of the Barents Sea and Kara Sea region

Published version. Source at http://dx.doi.org/10.1016/j.egypro.2016.10.005 In this study we assess the present-day gas hydrate stability zone for the Barents Sea and Kara Sea region. Thereby, we make use of a data-based 3D lithosphere-scale pressure and thermal model. The resulting gas hydrate stab...

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Bibliographic Details
Published in:Energy Procedia
Main Authors: Klitzke, Peter, Luzi-Helbing, Manja, Schicks, Judith M., Cacace, Mauro, Jacquey, Antoine B., Scheck-Wenderoth, Magdalena, Faleide, Jan Inge
Format: Article in Journal/Newspaper
Language:English
Published: Elsevier 2016
Subjects:
gas hydrate stability zone
3D modelling
Barents Sea
Kara Sea
VDP::Teknologi: 500::Berg‑ og petroleumsfag: 510::Petroleumsteknologi: 512
VDP::Technology: 500::Rock and petroleum disciplines: 510::Petroleum engineering: 512
Online Access:https://hdl.handle.net/10037/10455
https://doi.org/10.1016/j.egypro.2016.10.005
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Summary:Published version. Source at http://dx.doi.org/10.1016/j.egypro.2016.10.005 In this study we assess the present-day gas hydrate stability zone for the Barents Sea and Kara Sea region. Thereby, we make use of a data-based 3D lithosphere-scale pressure and thermal model. The resulting gas hydrate stability zone varies within >1km across the study area and strongly correlates with the local geological settings and the corresponding geothermal gradient. Gas hydrates containing hydrocarbons from a thermogenic source (CH4+C2H3+C3H8) are potentially more widespread than previously assumed. The corresponding thermogenic feed gas may have derived from leaking petroleum systems during late Cenozoic basin inversion.

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