Shallow gas and gas hydrates

2009 ◽  
pp. 163-188 ◽  
Author(s):  
Alan Judd ◽  
Martin Hovland
Keyword(s):  
2012 ◽  
Vol 32 (5-6) ◽  
pp. 407-417 ◽  
Author(s):  
Jeffrey Poort ◽  
Oleg M. Khlystov ◽  
Lieven Naudts ◽  
Albert D. Duchkov ◽  
Hitoshi Shoji ◽  
...  

2014 ◽  
Vol 1010-1012 ◽  
pp. 1719-1722
Author(s):  
Zhi Li Hua ◽  
Zhong Hai Zhou

Plume is closely related to the presence of gas hydrates which can often be found in plume development area. By acoustic detection, plumes of bubbles in the seawater from shallow gas have been found by marine surveying instruments in some areas over the world. Based on the existed theory of plume porosity, acoustic echo profile of sedbed seep plumes are numerically calculated. Within the simulation results, according to the pattern of gas bubble change and movement in the seawater, process of methane plumes generation is simulated and directs the distribution of bubble radius and plume boundary as depth. Acoustic features of plume bubbles seeping from shallow gas are shown to be consistent with the field results.


Geosciences ◽  
2019 ◽  
Vol 9 (3) ◽  
pp. 134 ◽  
Author(s):  
Claudio Argentino ◽  
Stefano Conti ◽  
Chiara Fioroni ◽  
Daniela Fontana

The occurrence of seep-carbonates associated with shallow gas hydrates is increasingly documented in modern continental margins but in fossil sediments the recognition of gas hydrates is still challenging for the lack of unequivocal proxies. Here, we combined multiple field and geochemical indicators for paleo-gas hydrate occurrence based on present-day analogues to investigate fossil seeps located in the northern Apennines. We recognized clathrite-like structures such as thin-layered, spongy and vuggy textures and microbreccias. Non-gravitational cementation fabrics and pinch-out terminations in cavities within the seep-carbonate deposits are ascribed to irregularly oriented dissociation of gas hydrates. Additional evidences for paleo-gas hydrates are provided by the large dimensions of seep-carbonate masses and by the association with sedimentary instability in the host sediments. We report heavy oxygen isotopic values in the examined seep-carbonates up to +6‰ that are indicative of a contribution of isotopically heavier fluids released by gas hydrate decomposition. The calculation of the stability field of methane hydrates for the northern Apennine wedge-foredeep system during the Miocene indicated the potential occurrence of shallow gas hydrates in the upper few tens of meters of sedimentary column.


2004 ◽  
Vol 2004 (1) ◽  
pp. 1-4 ◽  
Author(s):  
Hai Zhu ◽  
Ingo A. Pecher ◽  
Stuart A. Henrys ◽  
Guy Maslen

2003 ◽  
Vol 90 (6) ◽  
pp. 273-276 ◽  
Author(s):  
Stefan Sommer ◽  
Wilko Ahlrichs ◽  
Olaf Pfannkuche ◽  
Erik Gutzmann
Keyword(s):  

2021 ◽  
Vol 42 (1) ◽  
Author(s):  
Yin-Sheng Huang ◽  
Shu-Kun Hsu ◽  
Chih-Chieh Su ◽  
Andrew Tien-Shun Lin ◽  
Pai-Sen Yu ◽  
...  

AbstractWe have collected two shallow gas hydrate samples at two sites having different geological settings off southwest Taiwan during the cruise MD214 in 2018. The first core site, MD18-3542, is on the South Yuan-An East Ridge at ~ 1200 m water deep, where a structural unconformity covered by fine-silt sediments appears at ~ 5.5 m below the seafloor. The second core site, MD18-3543, is close to the Good-Weather Ridge at ~ 1100 m water deep, where a gas-related pockmark structure and authigenic carbonates are present at shallow strata with fine-silt sediments near the seafloor. Sediment properties of core MD18-3542 are distinctively different above and below the layer corresponding to the unconformity. Both cores show obvious gaps or voids in the lower core halves. The core features could be linked to the dissociated methane upward migrating from deep strata. Core site settings with upwelling methane would favor the formation of shallow gas hydrates. At site MD18-3542, the shallow hydrate could be formed due to high concentration methane kept beneath the unconformity covered by fine-silt sediments. At site MD18-3543, the shallow hydrate could be formed due to an extremely high flux of upwelling methane trapped either beneath the authigenic carbonates or fine-silt sediments.


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