Gas Hydrates 1: Fundamentals, Characterization and Modeling
Gas hydrates, or clathrate hydrates, are crystalline solids resembling ice, in which small (guest) molecules, typically gases, are trapped inside cavities formed by hydrogen-bonded water (host) molecules. They form and remain stable under low temperatures – often well below ambient conditions – and...
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ftarchimer:oai:archimer.ifremer.fr:56506 2023-05-15T16:37:44+02:00 Gas Hydrates 1: Fundamentals, Characterization and Modeling Broseta, Daniel Ruffine, Livio Desmedt, Arnaud 2017-08-14 application/pdf https://archimer.ifremer.fr/doc/00453/56506/58852.pdf https://archimer.ifremer.fr/doc/00453/56506/58853.pdf https://archimer.ifremer.fr/doc/00453/56506/58854.pdf https://doi.org/10.1002/9781119332688 https://archimer.ifremer.fr/doc/00453/56506/ eng eng https://archimer.ifremer.fr/doc/00453/56506/58852.pdf https://archimer.ifremer.fr/doc/00453/56506/58853.pdf https://archimer.ifremer.fr/doc/00453/56506/58854.pdf doi:10.1002/9781119332688 https://archimer.ifremer.fr/doc/00453/56506/ ISTE Ltd 2017 info:eu-repo/semantics/openAccess restricted use text Book info:eu-repo/semantics/book 2017 ftarchimer https://doi.org/10.1002/9781119332688 2021-09-23T20:31:29Z Gas hydrates, or clathrate hydrates, are crystalline solids resembling ice, in which small (guest) molecules, typically gases, are trapped inside cavities formed by hydrogen-bonded water (host) molecules. They form and remain stable under low temperatures – often well below ambient conditions – and high pressures ranging from a few bar to hundreds of bar, depending on the guest molecule. Their presence is ubiquitous on Earth, in deep-marine sediments and in permafrost regions, as well as in outer space, on planets or comets. In addition to water, they can be synthesized with organic species as host molecules, resulting in milder stability conditions: these are referred to as semi-clathrate hydrates. Clathrate and semi-clathrate hydrates are being considered for applications as diverse as gas storage and separation, cold storage and transport and water treatment. This book is the first of two edited volumes, with chapters on the experimental and modeling tools used for characterizing and predicting the unique molecular, thermodynamic and kinetic properties of gas hydrates (Volume 1) and on gas hydrates in their natural environment and for potential industrial applications (Volume 2). Book Ice permafrost Archimer (Archive Institutionnelle de l'Ifremer - Institut français de recherche pour l'exploitation de la mer) Hoboken, NJ, USA |
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Archimer (Archive Institutionnelle de l'Ifremer - Institut français de recherche pour l'exploitation de la mer) |
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ftarchimer |
language |
English |
description |
Gas hydrates, or clathrate hydrates, are crystalline solids resembling ice, in which small (guest) molecules, typically gases, are trapped inside cavities formed by hydrogen-bonded water (host) molecules. They form and remain stable under low temperatures – often well below ambient conditions – and high pressures ranging from a few bar to hundreds of bar, depending on the guest molecule. Their presence is ubiquitous on Earth, in deep-marine sediments and in permafrost regions, as well as in outer space, on planets or comets. In addition to water, they can be synthesized with organic species as host molecules, resulting in milder stability conditions: these are referred to as semi-clathrate hydrates. Clathrate and semi-clathrate hydrates are being considered for applications as diverse as gas storage and separation, cold storage and transport and water treatment. This book is the first of two edited volumes, with chapters on the experimental and modeling tools used for characterizing and predicting the unique molecular, thermodynamic and kinetic properties of gas hydrates (Volume 1) and on gas hydrates in their natural environment and for potential industrial applications (Volume 2). |
format |
Book |
author |
Broseta, Daniel Ruffine, Livio Desmedt, Arnaud |
spellingShingle |
Broseta, Daniel Ruffine, Livio Desmedt, Arnaud Gas Hydrates 1: Fundamentals, Characterization and Modeling |
author_facet |
Broseta, Daniel Ruffine, Livio Desmedt, Arnaud |
author_sort |
Broseta, Daniel |
title |
Gas Hydrates 1: Fundamentals, Characterization and Modeling |
title_short |
Gas Hydrates 1: Fundamentals, Characterization and Modeling |
title_full |
Gas Hydrates 1: Fundamentals, Characterization and Modeling |
title_fullStr |
Gas Hydrates 1: Fundamentals, Characterization and Modeling |
title_full_unstemmed |
Gas Hydrates 1: Fundamentals, Characterization and Modeling |
title_sort |
gas hydrates 1: fundamentals, characterization and modeling |
publishDate |
2017 |
url |
https://archimer.ifremer.fr/doc/00453/56506/58852.pdf https://archimer.ifremer.fr/doc/00453/56506/58853.pdf https://archimer.ifremer.fr/doc/00453/56506/58854.pdf https://doi.org/10.1002/9781119332688 https://archimer.ifremer.fr/doc/00453/56506/ |
genre |
Ice permafrost |
genre_facet |
Ice permafrost |
op_relation |
https://archimer.ifremer.fr/doc/00453/56506/58852.pdf https://archimer.ifremer.fr/doc/00453/56506/58853.pdf https://archimer.ifremer.fr/doc/00453/56506/58854.pdf doi:10.1002/9781119332688 https://archimer.ifremer.fr/doc/00453/56506/ |
op_rights |
ISTE Ltd 2017 info:eu-repo/semantics/openAccess restricted use |
op_doi |
https://doi.org/10.1002/9781119332688 |
op_publisher_place |
Hoboken, NJ, USA |
_version_ |
1766028043513495552 |