Occupancy Transition in Methane Hydrate II at High Pressure
收藏ESRF Portal2028-01-01 更新2026-04-23 收录
下载链接：
https://doi.esrf.fr/10.15151/ESRF-ES-2250354653
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资源简介：
Methane hydrate is a prominent substance in our solar system as both of its constituents (end members) are abundant on Earth, icy moons and on the outer ice giants (Uranus and Neptune). In this proposal we aim to determine accurately the methane occupancy of the water cages in phase II of methane hydrate at ~1.3 GPa, and explore whether MH-II increases its methane occupancy at this pressure. To achieve this we plan single crystal x-ray diffraction studies.
提供机构：
University of Edinburgh, Centre for Science at Extreme Conditions, Erskine Williamson Building Kings Buildings Mayfield Road, EH9 3JZ, Edinburgh, UNITED KINGDOM; University of Edinburgh, Centre for Science at Extreme Conditions, Erskine Williamson Building, Kings Buildings Mayfield Road, Eh9 3jz Edinburgh, United Kingdom; University of Edinburgh, School of Physics, The Kings Buildings Mayfield Road, EH9 3JZ, Edinburgh, UNITED KINGDOM
创建时间：
2028-01-01
