🔧На сайте запланированы технические работы
25.12.2025 в промежутке с 18:00 до 21:00 по Московскому времени (GMT+3) на сайте будут проводиться плановые технические работы. Возможны перебои с доступом к сайту. Приносим извинения за временные неудобства. Благодарим за понимание!
🔧Site maintenance is scheduled.
Scheduled maintenance will be performed on the site from 6:00 PM to 9:00 PM Moscow time (GMT+3) on December 25, 2025. Site access may be interrupted. We apologize for the inconvenience. Thank you for your understanding!

 

Simulation of the Conditions for the Formation and Dissociation of Methane Hydrate over the Last 130 000 Years


如何引用文章

全文:

开放存取 开放存取
受限制的访问 ##reader.subscriptionAccessGranted##
受限制的访问 订阅存取

详细

The thermobaric conditions of the formation, stability, and dissociation of continental gas hydrates were determined by simulation of the thermal state of the permafrost. The calculations covered the period over the last 130 000 years, taking into account the various paleo-settings, including continental glaciation, marine transgression, and high geothermal fluxes. According to the numerical calculations, relict gas hydrates may currently exist in the metastable state in the permafrost at depths of less than 100–150 m.

作者简介

M. Arzhanov

Obukhov Institute of Atmospheric Physics

编辑信件的主要联系方式.
Email: arzhanov@ifaran.ru
俄罗斯联邦, Moscow, 119017

V. Malakhova

Institute of Computational Mathematics and Mathematical Geophysics, Siberian Branch

Email: arzhanov@ifaran.ru
俄罗斯联邦, Novosibirsk, 630090

I. Mokhov

Obukhov Institute of Atmospheric Physics; Moscow State University

Email: arzhanov@ifaran.ru
俄罗斯联邦, Moscow, 119017; Moscow, 119991

补充文件

附件文件
动作
1. JATS XML

版权所有 © Pleiades Publishing, Ltd., 2018