Distribution of the gas hydrate stability zone in the Ross Sea, Antarctica
ABSTRACT The theoretical gas hydrates stability zone (GHSZ) in the Ross Sea area was evaluated by mean of a steady state simple approach by using bathymetric data, sea bottom temperature, a variable geothermal gradient and assuming that the natural gas is methane. The results from our study suggest...
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Servicio Nacional de Geología y Minería (SERNAGEOMIN)
2018
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oai:scielo:S0718-710620180001000782018-02-22Distribution of the gas hydrate stability zone in the Ross Sea, AntarcticaGiustiniani,MichelaTinivella,UmbertaSauli,ChiaraDella Vedova,Bruno Gas hydrates stability zone Ross sea Modeling ABSTRACT The theoretical gas hydrates stability zone (GHSZ) in the Ross Sea area was evaluated by mean of a steady state simple approach by using bathymetric data, sea bottom temperature, a variable geothermal gradient and assuming that the natural gas is methane. The results from our study suggest that bathymetry and distribution of the GHSZ are correlated; in fact, the GHSZ reaches a maximum (ca. 400 m) in the basins, where the water temperature is the lowest, and decreases in the banks with thickness ranging between 7 and <100 m. On the other hand, the existence and dynamics of the gas hydrate distribution is strictly related to the existence and evolution of the shallow geological and geomorphological features below the sea floor, as suggested in the past by several authors.info:eu-repo/semantics/openAccessServicio Nacional de Geología y Minería (SERNAGEOMIN)Andean geology v.45 n.1 20182018-01-01text/htmlhttp://www.scielo.cl/scielo.php?script=sci_arttext&pid=S0718-71062018000100078en10.5027/andgeov45n1-2989 |
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Scielo Chile |
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Scielo Chile |
language |
English |
topic |
Gas hydrates stability zone Ross sea Modeling |
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Gas hydrates stability zone Ross sea Modeling Giustiniani,Michela Tinivella,Umberta Sauli,Chiara Della Vedova,Bruno Distribution of the gas hydrate stability zone in the Ross Sea, Antarctica |
description |
ABSTRACT The theoretical gas hydrates stability zone (GHSZ) in the Ross Sea area was evaluated by mean of a steady state simple approach by using bathymetric data, sea bottom temperature, a variable geothermal gradient and assuming that the natural gas is methane. The results from our study suggest that bathymetry and distribution of the GHSZ are correlated; in fact, the GHSZ reaches a maximum (ca. 400 m) in the basins, where the water temperature is the lowest, and decreases in the banks with thickness ranging between 7 and <100 m. On the other hand, the existence and dynamics of the gas hydrate distribution is strictly related to the existence and evolution of the shallow geological and geomorphological features below the sea floor, as suggested in the past by several authors. |
author |
Giustiniani,Michela Tinivella,Umberta Sauli,Chiara Della Vedova,Bruno |
author_facet |
Giustiniani,Michela Tinivella,Umberta Sauli,Chiara Della Vedova,Bruno |
author_sort |
Giustiniani,Michela |
title |
Distribution of the gas hydrate stability zone in the Ross Sea, Antarctica |
title_short |
Distribution of the gas hydrate stability zone in the Ross Sea, Antarctica |
title_full |
Distribution of the gas hydrate stability zone in the Ross Sea, Antarctica |
title_fullStr |
Distribution of the gas hydrate stability zone in the Ross Sea, Antarctica |
title_full_unstemmed |
Distribution of the gas hydrate stability zone in the Ross Sea, Antarctica |
title_sort |
distribution of the gas hydrate stability zone in the ross sea, antarctica |
publisher |
Servicio Nacional de Geología y Minería (SERNAGEOMIN) |
publishDate |
2018 |
url |
http://www.scielo.cl/scielo.php?script=sci_arttext&pid=S0718-71062018000100078 |
work_keys_str_mv |
AT giustinianimichela distributionofthegashydratestabilityzoneintherossseaantarctica AT tinivellaumberta distributionofthegashydratestabilityzoneintherossseaantarctica AT saulichiara distributionofthegashydratestabilityzoneintherossseaantarctica AT dellavedovabruno distributionofthegashydratestabilityzoneintherossseaantarctica |
_version_ |
1714205856753516544 |