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• W2492017265 abstract "PreviousNext No AccessGeophysical Characterization of Gas Hydrates13. Gas Hydrates and Magnetism: Surveying and Diagenetic AnalysisAuthors: L. EstebanT. S. HamiltonR. J. EnkinC. LoweI. NovoselL. G. BenningR. T. WilkinH. L. BarnesR. A. BernerA. BoetiusK. RavenschlagC. J. SchubertD. RickertF. WiddelA. GiesekeR. AmannB. B. Joøslash;rgensenU. WitteO. PfannkucheW. S. BorowskiC. K. PaullW. UsslerT. A. BrentM. RiedelM. CaddelT. S. CollettS. R. DallimoreS. R. DallimoreT. S. CollettD. E. CanfieldR. RaiswellS. H. BottrellN. R. ChapmanJ. GettrustR. WaliaD. HannayG. D. SpenceW. WoodR. D. HyndmanT. S. CollettM. W. LeeS. R. DallimoreW. F. AgenaS. R. DallimoreT. UchidaT. S. CollettT. S. CollettR. E. LewisS. R. DallimoreS. R. DallimoreT. S. CollettS. R. DallimoreT. S. CollettS. R. DallimoreT. S. CollettR. DayM. D. FullerV. A. SchmidtR. DumontM. CoyleD. OneschukJ. PotvinR. DumontM. CoyleD. OneschukJ. PotvinR. DumontM. CoyleD. OneschukJ. PotvinR. DumontM. CoyleD. OneschukJ. PotvinD. J. Dunlopö. ÖzdemirR. EnkinJ. BakerD. NourgalievP. IassonovT. S. HamiltonR. C. ErdH. T. EvansD. H. RichterM. E. EvansF. HellerM. E. FleetM. E. FleetP. N. FroelichG. P. KlinkhammerM. L. BenderN. A. LuedtkeG. R. HeathD. CullenP. DauphinD. HammondB. HartmanV. MaynardJ. F. L. GarmingU. BleilN. RiedingerM. B. GoldhaberI. R. KaplanE. D. GoldbergR. M. HabererK. MangelsorfV. DieckmannA. FuhrmannH. WilkesB. HorsfieldS. R. DallimoreT. S. CollettV. HoffmannH. StanjekE. MuradC. S. HorngK. H. ChenB. A. HousenR. J. MusgraveK. A. JennerS. R. DallimoreI. D. ClarkD. ParéB. E. MedioliS. R. DallimoreT. UchidaT. S. CollettJ. K. JertzJ. D. RimstidtS. J. KaoC. S. HorngA. P. RobertsK. K. LiuH. E. KingC. T. PrewittM. KrsF. NovákM. KrsováP. PrunerL. KouklíkováJ. JansaR. E. KruppJ. C. LarrasoanaE. GràciaM. GarcésR. J. MusgraveE. PineroF. Martinez-RuizM. E. VegaA. M. TréhuG. BohrmannM. E. TorresF. S. ColwellJ. C. LarrasoanaA. P. RobertsR. J. MusgraveE. GràciaE. PineroM. VegaF. Martínez-RuizC. LoweR. J. EnkinJ. BakerS. R. DallimoreS. R. DallimoreT. S. CollettB. E. MedioliN. WilsonS. R. DallimoreD. ParéP. Brennan-AlpertH. OdaS. R. DallimoreT. S. CollettJ. B. MurowchickH. L. BarnesR. J. MusgraveY. HirokiC. K. PaullR. MatsumotoP. J. WallaceW. P. DillonC. NiewohnerC. HensenS. KastenM. ZabelH. D. SchulzI. NovoselG. D. SpenceR. D. HyndmanC. PetersM. J. DekkersM. PósfaiP. R. BuseckD. A. BazylinskiR. B. FrankelA. V. PowellP. VaqueiroK. S. KnightL. C. ChaponR. D. SanchezM. RiedelG. D. SpenceR. N. ChapmanR. D. HyndmanM. RiedelG. D. SpenceR. D. HyndmanN. R. ChapmanM. RiedelT. S. CollettM. J. MaloneN. RiedingerK. PfeiferS. KastenJ. F. L. GarmingC. VogtC. HensenA. P. RobertsM. A. A. SchoonenH. L. BarnesR. SkálaI. CisarovaM. DrabekB. J. SkinnerR. C. ErdR. F. GrimaldiR. E. SweeneyI. R. KaplanA. M. TréhuG. BohrmannF. R. RackM. E. TorresA. WasedaT. UchidaS. R. DallimoreT. S. CollettG. K. WestbrookB. CarsonR. J. MusgraveR. T. WilkinH. L. BarnesM. R. WolthersS. J. Van der GaastD. RickardM. R. WolthersL. CharletP. R. Van der LindeD. RickardC. H. Van der WeijdenL. EstebanGeological Survey of Canada, Sidney, British Columbia, CACamosun College, Victoria, British Columbia, CAGeological Survey of Canada, Sidney, British Columbia, CAGeological Survey of Canada, Sidney, British Columbia, CAShell International Exploration and Production Inc., Houston, TX, USSearch for more papers by this author, T. S. HamiltonGeological Survey of Canada, Sidney, British Columbia, CACamosun College, Victoria, British Columbia, CAGeological Survey of Canada, Sidney, British Columbia, CAGeological Survey of Canada, Sidney, British Columbia, CAShell International Exploration and Production Inc., Houston, TX, USSearch for more papers by this author, R. J. EnkinGeological Survey of Canada, Sidney, British Columbia, CACamosun College, Victoria, British Columbia, CAGeological Survey of Canada, Sidney, British Columbia, CAGeological Survey of Canada, Sidney, British Columbia, CAShell International Exploration and Production Inc., Houston, TX, USSearch for more papers by this author, C. LoweGeological Survey of Canada, Sidney, British Columbia, CACamosun College, Victoria, British Columbia, CAGeological Survey of Canada, Sidney, British Columbia, CAGeological Survey of Canada, Sidney, British Columbia, CAShell International Exploration and Production Inc., Houston, TX, USSearch for more papers by this author, I. NovoselGeological Survey of Canada, Sidney, British Columbia, CACamosun College, Victoria, British Columbia, CAGeological Survey of Canada, Sidney, British Columbia, CAGeological Survey of Canada, Sidney, British Columbia, CAShell International Exploration and Production Inc., Houston, TX, USSearch for more papers by this author, L. 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Van der WeijdenSearch for more papers by this authorhttps://doi.org/10.1190/1.9781560802197.ch13 SectionsAboutPDF/ePub ToolsAdd to favoritesDownload CitationsTrack CitationsPermissions ShareFacebookTwitterLinked InReddit Abstract Geochemical processes associated with gas-hydrate formation lead to the growth of iron sulphides, which have a geophysically measurable magnetic signature. Detailed magnetic investigation and complementary petrological observations were undertaken on cores from the permafrost setting Mackenzie Delta Mallik region (Northwest Territories) and the marine setting IODP Expedition 311 cores from the Cascadia margin off Vancouver Island. These magnetic measurements provide stratigraphic profiles, which reveal fine scale variations in lithology, magnetic grain size, and pore fluid geochemistry. The highest magnetic susceptibility values are observed in strata preserve high initial concentrations of detrital magnetite, such as glacial deposits. The lowest values of magnetic susceptibility are observed in which iron has been reduced to paramagnetic pyrite, formed in settings with high methane and sulphate flux such as at methane vents. Enhanced values of magnetic susceptibility characterize the introduction of the ferrimagnetic iron sulphide minerals greigite (Skinner et al., 1964) and smythite (Erd et al., 1957). These magnetic minerals are mostly found immediately adjacent to the sedimentary horizons, which host the gas hydrate, and their textures and compositions indicate rapid disequilibrium crystallization. These observations result from the unique physical and geochemical properties of the environment in which gas hydrates form; methane is available to fuel microbiological activity and pore water solutes concentrate during gas-hydrate formation. In these conditions, iron sulphides bacterially precipitate from solute rich brines. 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Willoughby, Michael Riedel, and Satinder Chopra21 March 2012 Geophysical Characterization of Gas HydratesISBN (print):978-1-56080-218-1ISBN (online):978-1-56080-219-8Copyright: 2010 Pages: 412 publication data© 2010 All rights reserved. No part of this publication may be reproduced or distributed in any form or by any means without written permission of the publisherPublisher:Society of Exploration Geophysicists HistoryPublished in print: 01 Jan 2010 CITATION INFORMATION L. Esteban, T. S. Hamilton, R. J. Enkin, C. Lowe, and I. Novosel, (2010), 13. Gas Hydrates and Magnetism: Surveying and Diagenetic Analysis, Geophysical Developments Series : 197-216. https://doi.org/10.1190/1.9781560802197.ch13 Plain-Language Summary PDF DownloadLoading ..." @default.
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