(66g) Probing the Effect of Stirring on Natural Gas Hydrate Formation-a Future Energy Fuel
AIChE Spring Meeting and Global Congress on Process Safety
2018
2018 Spring Meeting and 14th Global Congress on Process Safety
6th International Conference on Upstream Engineering and Flow Assurance
Gas Hydrates, Wax and Asphaltenes II
Tuesday, April 24, 2018 - 2:14pm to 2:36pm
In order to avoid liquefaction cost, the scientists are trying to study gas hydrates as potential mode of natural gas transportation and storage in future. Gas hydrates are crystalline compounds, formed of water and gas molecules. One volume of hydrate can store up to 180 volumes of natural gas at STP (standard temperature and pressure). Therefore, the development of hydrate production plants holds particular importance in future.
In this experimental based work, the formation rate of gas hydrates in a high pressure cell has been studied at different stirring rates using a magnetic stirrer. In the first stage, the system was first cooled from 20 o C to 2 o C at constant pressure for 18 hours. Then in second stage, the system was left stable at 2 o C for another 18 hours at constant stirring rate. The stirring rates were varied between 100-1400 Rpm (Rotations per minute) for each experiment and the gas hydrate crystal formation was observed by calculating pressure drop across the high pressure cell during the second stage.
The experimental result shows that for a chosen high pressure cell, the stirring rate has a significant effect on the rate of gas hydrate crystal formation. The maximum gas hydrate crystal formation was observed within the stirring range of 550-750 RPM. It was found that there exists a threshold stirring limit, above or below which little or no hydrate crystal formation takes place. This fundamental study is a significant step forward and it can be useful for modeling purposes and designing of a pilot scale hydrate production plant to study the economical and safety factors associated with natural gas hydrate storage and transportation phenomena.
Acknowledgement
This work was made possible by NPRP grant # 6-330-2-140 and GSRA # 2-1-0603-14012 from the Qatar National Research Fund (a member of Qatar Foundation). The statements made herein are solely the responsibility of the authors.