Mathematical model of accumulation of gas hydrates associated with deep-sea mud volcanoes
- Авторлар: Zhostkov R.A.1, Sobisevich A.L.1, Suetnova E.I.1
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Мекемелер:
- Schmidt Institute of Physics of the Earth
- Шығарылым: Том 474, № 1 (2017)
- Беттер: 604-606
- Бөлім: Geophysics
- URL: https://bakhtiniada.ru/1028-334X/article/view/189989
- DOI: https://doi.org/10.1134/S1028334X17050282
- ID: 189989
Дәйексөз келтіру
Аннотация
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.
Авторлар туралы
R. Zhostkov
Schmidt Institute of Physics of the Earth
Хат алмасуға жауапты Автор.
Email: shageraxcom@yandex.ru
Ресей, Moscow, 123810
A. Sobisevich
Schmidt Institute of Physics of the Earth
Email: shageraxcom@yandex.ru
Ресей, Moscow, 123810
E. Suetnova
Schmidt Institute of Physics of the Earth
Email: shageraxcom@yandex.ru
Ресей, Moscow, 123810
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