Shallow gas accumulations and fluid flow in the vicinity of the Goliat field, SW Barents Sea

This thesis focuses on the Goliat area located in the Hammerfest Basin, SW Barents Sea. The overall aim of this study is to increase the understanding of fluid flow processes between deeper thermogenic sources, and shallow gas accumulations. Indications of an active fluid flow system has been observ...

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Main Author: Paulsen, Renate Strugstad
Format: Master Thesis
Language:English
Published: UiT Norges arktiske universitet 2017
Subjects:
Online Access:https://hdl.handle.net/10037/11075
id ftunivtroemsoe:oai:munin.uit.no:10037/11075
record_format openpolar
spelling ftunivtroemsoe:oai:munin.uit.no:10037/11075 2023-05-15T15:38:27+02:00 Shallow gas accumulations and fluid flow in the vicinity of the Goliat field, SW Barents Sea Paulsen, Renate Strugstad 2017-05-15 https://hdl.handle.net/10037/11075 eng eng UiT Norges arktiske universitet UiT The Arctic University of Norway https://hdl.handle.net/10037/11075 openAccess Copyright 2017 The Author(s) VDP::Mathematics and natural science: 400::Geosciences: 450::Marine geology: 466 VDP::Matematikk og Naturvitenskap: 400::Geofag: 450::Marin geologi: 466 Barents Sea Fluid flow Shallow gas Polygonal faults pockmarks GEO-3900 Master thesis Mastergradsoppgave 2017 ftunivtroemsoe 2021-06-25T17:55:17Z This thesis focuses on the Goliat area located in the Hammerfest Basin, SW Barents Sea. The overall aim of this study is to increase the understanding of fluid flow processes between deeper thermogenic sources, and shallow gas accumulations. Indications of an active fluid flow system has been observed throughout the southwestern Barents Sea. Much of the fluid flow from deep hydrocarbon reservoirs has been associated with the denudation history of the Barents Sea. Well-known fluid flow features like pipes or pockmarks appear on seismic images and multibeam bathymetry data and provide evidence for fluid migration. A single seismic data set from the Goliat field area, provided by Eni Norge, has been interpreted for possible indications of fluid flow features and shallow gas accumulation. This study focusses mostly on the sedimentary formations above the Base Cretaceous Unconformity (BCU). Two main sets of faults are categorized: deep-seated faults extending downwards from the BCU and into the Permian strata, and shallow faults affecting the Kolmule and Torsk Formations. Within the shallow faults, two different sets of polygonal faults are interpreted. One polygonal fault system affecting only a small interval within the lower Kolmule Formation, and the other is a set of reactivated polygonal faults affecting both the Kolmule and Tosk Formations. As the SW Barents Sea has undergone several phases of uplift and erosion, different sets of faults have been active at different times. The change and orientation of lithospheric stress causes different sets of faults to be open as potential fluid migration pathways. This makes it possible for fluids to migrate and accumulate at different stratigraphic levels in the subsurface. Pockmarks and fluid flow features above the upper regional unconformity (URU) implies an active fluid flow system after the Plio-Pleistocene glaciation. Amplitude anomalies are often associated with the presence of free gas in the subsurface. The presence and distribution of amplitude anomalies in this work indicates that there is a relation between the deeper-lying hydrocarbon reservoirs and both deep-seated and shallow faults. The observation of pockmarks on the seafloor increases the possibility of free gas to be present in the area. Master Thesis Barents Sea Hammerfest Hammerfest Basin University of Tromsø: Munin Open Research Archive Barents Sea
institution Open Polar
collection University of Tromsø: Munin Open Research Archive
op_collection_id ftunivtroemsoe
language English
topic VDP::Mathematics and natural science: 400::Geosciences: 450::Marine geology: 466
VDP::Matematikk og Naturvitenskap: 400::Geofag: 450::Marin geologi: 466
Barents Sea
Fluid flow
Shallow gas
Polygonal faults
pockmarks
GEO-3900
spellingShingle VDP::Mathematics and natural science: 400::Geosciences: 450::Marine geology: 466
VDP::Matematikk og Naturvitenskap: 400::Geofag: 450::Marin geologi: 466
Barents Sea
Fluid flow
Shallow gas
Polygonal faults
pockmarks
GEO-3900
Paulsen, Renate Strugstad
Shallow gas accumulations and fluid flow in the vicinity of the Goliat field, SW Barents Sea
topic_facet VDP::Mathematics and natural science: 400::Geosciences: 450::Marine geology: 466
VDP::Matematikk og Naturvitenskap: 400::Geofag: 450::Marin geologi: 466
Barents Sea
Fluid flow
Shallow gas
Polygonal faults
pockmarks
GEO-3900
description This thesis focuses on the Goliat area located in the Hammerfest Basin, SW Barents Sea. The overall aim of this study is to increase the understanding of fluid flow processes between deeper thermogenic sources, and shallow gas accumulations. Indications of an active fluid flow system has been observed throughout the southwestern Barents Sea. Much of the fluid flow from deep hydrocarbon reservoirs has been associated with the denudation history of the Barents Sea. Well-known fluid flow features like pipes or pockmarks appear on seismic images and multibeam bathymetry data and provide evidence for fluid migration. A single seismic data set from the Goliat field area, provided by Eni Norge, has been interpreted for possible indications of fluid flow features and shallow gas accumulation. This study focusses mostly on the sedimentary formations above the Base Cretaceous Unconformity (BCU). Two main sets of faults are categorized: deep-seated faults extending downwards from the BCU and into the Permian strata, and shallow faults affecting the Kolmule and Torsk Formations. Within the shallow faults, two different sets of polygonal faults are interpreted. One polygonal fault system affecting only a small interval within the lower Kolmule Formation, and the other is a set of reactivated polygonal faults affecting both the Kolmule and Tosk Formations. As the SW Barents Sea has undergone several phases of uplift and erosion, different sets of faults have been active at different times. The change and orientation of lithospheric stress causes different sets of faults to be open as potential fluid migration pathways. This makes it possible for fluids to migrate and accumulate at different stratigraphic levels in the subsurface. Pockmarks and fluid flow features above the upper regional unconformity (URU) implies an active fluid flow system after the Plio-Pleistocene glaciation. Amplitude anomalies are often associated with the presence of free gas in the subsurface. The presence and distribution of amplitude anomalies in this work indicates that there is a relation between the deeper-lying hydrocarbon reservoirs and both deep-seated and shallow faults. The observation of pockmarks on the seafloor increases the possibility of free gas to be present in the area.
format Master Thesis
author Paulsen, Renate Strugstad
author_facet Paulsen, Renate Strugstad
author_sort Paulsen, Renate Strugstad
title Shallow gas accumulations and fluid flow in the vicinity of the Goliat field, SW Barents Sea
title_short Shallow gas accumulations and fluid flow in the vicinity of the Goliat field, SW Barents Sea
title_full Shallow gas accumulations and fluid flow in the vicinity of the Goliat field, SW Barents Sea
title_fullStr Shallow gas accumulations and fluid flow in the vicinity of the Goliat field, SW Barents Sea
title_full_unstemmed Shallow gas accumulations and fluid flow in the vicinity of the Goliat field, SW Barents Sea
title_sort shallow gas accumulations and fluid flow in the vicinity of the goliat field, sw barents sea
publisher UiT Norges arktiske universitet
publishDate 2017
url https://hdl.handle.net/10037/11075
geographic Barents Sea
geographic_facet Barents Sea
genre Barents Sea
Hammerfest
Hammerfest Basin
genre_facet Barents Sea
Hammerfest
Hammerfest Basin
op_relation https://hdl.handle.net/10037/11075
op_rights openAccess
Copyright 2017 The Author(s)
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