2010
DOI: 10.1029/2009jb007078
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Evidence from three‐dimensional seismic tomography for a substantial accumulation of gas hydrate in a fluid‐escape chimney in the Nyegga pockmark field, offshore Norway

Abstract: [1] In recent years, it has become evident that features commonly called gas chimneys provide major routes for methane to pass through the methane-hydrate stability zone in continental margins and escape to the ocean. One of many such chimneys lying beneath pockmarks in the southeastern Vøring Plateau off Norway was investigated with a high-resolution seismic experiment employing a 2-D array of sixteen 4-component ocean bottom seismic recorders at approximately 100 m separation and a dense network of shots to … Show more

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Cited by 66 publications
(81 citation statements)
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“…Seismic anisotropy may also exist in regions where vertical to subvertical, fluid-filled fractures and micro-cracks are present . The Nyegga pockmarks region exhibits a sub-horizontal stratigraphy (Kjeldstad et al 2003) as seen from extensive seismic reflection data Berndt et al 2003;Westbrook et al 2008;Plaza-Faverola et al 2010. The underlying chimney-like and pipe structures cut vertically through the horizontal layers Berndt et al 2003;Plaza-Faverola et al 2011).…”
Section: Anisotropy At Cne03mentioning
confidence: 99%
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“…Seismic anisotropy may also exist in regions where vertical to subvertical, fluid-filled fractures and micro-cracks are present . The Nyegga pockmarks region exhibits a sub-horizontal stratigraphy (Kjeldstad et al 2003) as seen from extensive seismic reflection data Berndt et al 2003;Westbrook et al 2008;Plaza-Faverola et al 2010. The underlying chimney-like and pipe structures cut vertically through the horizontal layers Berndt et al 2003;Plaza-Faverola et al 2011).…”
Section: Anisotropy At Cne03mentioning
confidence: 99%
“…Both Vp representations start at the seafloor (∼727 m below sea-surface) and extend to a depth of 1000 m (line 1, S to N) and 1050 m (line 2, NW to SE), below sea-surface. The velocities in the first and the second layer (727-750 m, and 750-800 m) are poorly constrained at the chimney interior and the flanks, due to a low density of seismic-ray impact points in this region (Plaza-Faverola et al 2010). The model shows an increased seismic velocity along the pipe structure compared with the surrounding strata, most probably resulting from the presence of hydrate in the pores of the host sediments within the GHSZ (Figs 3a and c).…”
Section: D Seismic Tomographymentioning
confidence: 99%
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