Mathematical model of accumulation of gas hydrates associated with deep-sea mud volcanoes
- Authors: Zhostkov R.A.1, Sobisevich A.L.1, Suetnova E.I.1
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Affiliations:
- Schmidt Institute of Physics of the Earth
- Issue: Vol 474, No 1 (2017)
- Pages: 604-606
- Section: Geophysics
- URL: https://bakhtiniada.ru/1028-334X/article/view/189989
- DOI: https://doi.org/10.1134/S1028334X17050282
- ID: 189989
Cite item
Abstract
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.
About the authors
R. A. Zhostkov
Schmidt Institute of Physics of the Earth
Author for correspondence.
Email: shageraxcom@yandex.ru
Russian Federation, Moscow, 123810
A. L. Sobisevich
Schmidt Institute of Physics of the Earth
Email: shageraxcom@yandex.ru
Russian Federation, Moscow, 123810
E. I. Suetnova
Schmidt Institute of Physics of the Earth
Email: shageraxcom@yandex.ru
Russian Federation, Moscow, 123810
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