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


Cite item

Full Text

Open Access Open Access
Restricted Access Access granted
Restricted Access Subscription Access

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

Supplementary files

Supplementary Files
Action
1. JATS XML

Copyright (c) 2017 Pleiades Publishing, Ltd.