Vis enkel innførsel

dc.contributor.advisorAndreassen, Karin
dc.contributor.advisorWinsborrow, Monica
dc.contributor.advisorVadakkeyambatta, Sunil
dc.contributor.authorLøvaas, John Sverre
dc.date.accessioned2016-07-05T09:38:47Z
dc.date.available2016-07-05T09:38:47Z
dc.date.issued2016-05-24
dc.description.abstractSeismic evidence of shallow gas anomalies are prominent at Ververis Dome structure and Hoop Fault Complex in Bjarmeland Platform. Ubiquitous high amplitude anomalies at the same depth as these shallow gas anomalies infer a possible relation to gas hydrates. A wide range of fluid flow structures within the two study areas have previously been discovered and reported, and may possibly feed the base of the gas hydrate stability zone (BGHSZ) with upward migrating thermogenic gas. This thesis focuses on seismic interpretation of gas hydrate-related bottom simulating reflectors (BSR) from high resolution 3D seismic data and high resolution 2D P-cable seismic data, as well as numerical modelling of gas hydrate stability conditions based on analyzed gas samples from geochemical data reports from well 7226/2-1 and 7324/8-1. Numerical modelling of present day gas hydrate stability conditions indicate favorable conditions for gas hydrate stability both in Ververis and Hoop Fault Complex. Furthermore, the estimated depth of gas hydrate stability from numerical modelling coincides with the interpreted BSRs in both study areas. As such, confidence is built in the interpretation and mapping of gas hydrates in the study areas. By using the results from ongoing work at Centre for arctic gas hydrate, environment and climate (CAGE) on numerical modelling of the ice sheet and isostatic conditions during the last glaciation, modelling of gas hydrate stability conditions indicate stable conditions for gas hydrates as deep as 618 m sub bottom depth in Ververis and 412 m sub bottom depth in Hoop Fault Complex during Last Glacial Maximum (LGM). The modelled gas hydrate stability zone in both study areas is thinning through deglaciation, possibly caused by unloading of vast ice sheets and the increasing bottom water temperatures.en_US
dc.identifier.urihttps://hdl.handle.net/10037/9376
dc.identifier.urnURN:NBN:no-uit_munin_8937
dc.language.isoengen_US
dc.publisherUiT The Arctic University of Norwayen_US
dc.publisherUiT Norges arktiske universiteten_US
dc.rights.accessRightsopenAccess
dc.rights.holderCopyright 2016 The Author(s)
dc.rights.urihttps://creativecommons.org/licenses/by-nc-sa/3.0en_US
dc.rightsAttribution-NonCommercial-ShareAlike 3.0 Unported (CC BY-NC-SA 3.0)en_US
dc.subject.courseIDEOM-3901
dc.subjectVDP::Matematikk og Naturvitenskap: 400::Geofag: 450en_US
dc.subjectVDP::Mathematics and natural science: 400::Geosciences: 450en_US
dc.titlePossible gas hydrates on the Bjarmeland Platform; seismic expression and stability modellingen_US
dc.typeMaster thesisen_US
dc.typeMastergradsoppgaveen_US


Tilhørende fil(er)

Thumbnail
Thumbnail

Denne innførselen finnes i følgende samling(er)

Vis enkel innførsel

Attribution-NonCommercial-ShareAlike 3.0 Unported (CC BY-NC-SA 3.0)
Med mindre det står noe annet, er denne innførselens lisens beskrevet som Attribution-NonCommercial-ShareAlike 3.0 Unported (CC BY-NC-SA 3.0)