Mathematical model of accumulation of gas hydrates associated with deep-sea mud volcanoes


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A new model that can account for accumulations of gas hydrates associated with submarine mud volcanoes and based on the available data on these gas hydrates is proposed. This model permits us to predict the evolution of gas-hydrate saturation by depth and time, depending on the geophysical conditions on the ocean floor in zones of mud volcanoes.

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R. Zhostkov

Schmidt Institute of Physics of the Earth

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Email: shageraxcom@yandex.ru
俄罗斯联邦, Moscow, 123810

A. Sobisevich

Schmidt Institute of Physics of the Earth

Email: shageraxcom@yandex.ru
俄罗斯联邦, Moscow, 123810

E. Suetnova

Schmidt Institute of Physics of the Earth

Email: shageraxcom@yandex.ru
俄罗斯联邦, Moscow, 123810

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