Show simple item record

Authordc.contributor.authorShaffer, Gary 
Authordc.contributor.authorFernández Villanueva, Esteban 
Authordc.contributor.authorRondanelli Rojas, Roberto 
Authordc.contributor.authorPepke Pedersen, Jens Olaf 
Authordc.contributor.authorMalskr Olsen, Steffen 
Authordc.contributor.authorHuber, Matthew 
Admission datedc.date.accessioned2018-06-18T14:13:26Z
Available datedc.date.available2018-06-18T14:13:26Z
Publication datedc.date.issued2017
Cita de ítemdc.identifier.citationGeosci. Model Dev., 10, 4081–4103, 2017es_ES
Identifierdc.identifier.other10.5194/gmd-10-4081-2017
Identifierdc.identifier.urihttps://repositorio.uchile.cl/handle/2250/148933
Abstractdc.description.abstractGeological records reveal a number of ancient, large and rapid negative excursions of the carbon-13 isotope. Such excursions can only be explained by massive injections of depleted carbon to the Earth system over a short duration. These injections may have forced strong global warming events, sometimes accompanied by mass extinctions such as the Triassic-Jurassic and end-Permian extinctions 201 and 252 million years ago, respectively. In many cases, evidence points to methane as the dominant form of injected carbon, whether as thermogenic methane formed by magma intrusions through overlying carbon-rich sediment or from warming-induced dissociation of methane hydrate, a solid compound of methane and water found in ocean sediments. As a consequence of the ubiquity and importance of methane in major Earth events, Earth system models for addressing such events should include a comprehensive treatment of methane cycling but such a treatment has often been lacking. Here we implement methane cycling in the Danish Center for Earth System Science (DCESS) model, a simplified but well-tested Earth system model of intermediate complexity. We use a generic methane input function that allows variation in input type, size, timescale and ocean-atmosphere partition. To be able to treat such massive inputs more correctly, we extend the model to deal with ocean suboxic/anoxic conditions and with radiative forcing and methane lifetimes appropriate for high atmospheric methane concentrations. With this new model version, we carried out an extensive set of simulations for methane inputs of various sizes, timescales and ocean-atmosphere partitions to probe model behavior. We find that larger methane inputs over shorter timescales with more methane dissolving in the ocean lead to ever-increasing ocean anoxia with consequences for ocean life and global carbon cycling. Greater methane input directly to the atmosphere leads to more warming and, for example, greater carbon dioxide release from land soils. Analysis of synthetic sediment cores from the simulations provides guidelines for the interpretation of real sediment cores spanning the warming events. With this improved DCESS model version and paleo-reconstructions, we are now better armed to gauge the amounts, types, timescales and locations of methane injections driving specific, observed deep-time, global warming events.es_ES
Patrocinadordc.description.sponsorshipFONDECYT (Chile) 1150913 Chilean ICM grant NC120066es_ES
Lenguagedc.language.isoenes_ES
Publisherdc.publisherCopernicus Publicationses_ES
Type of licensedc.rightsAttribution-NonCommercial-NoDerivs 3.0 Chile*
Link to Licensedc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/3.0/cl/*
Sourcedc.sourceGeoscientific Model Developmentes_ES
Títulodc.titleImplementation of methane cycling for deep-time global warming simulations with the DCESS Earth system model (version 1.2)es_ES
Document typedc.typeArtículo de revista
Catalogueruchile.catalogadortjnes_ES
Indexationuchile.indexArtículo de publicación ISIes_ES


Files in this item

Icon

This item appears in the following Collection(s)

Show simple item record

Attribution-NonCommercial-NoDerivs 3.0 Chile
Except where otherwise noted, this item's license is described as Attribution-NonCommercial-NoDerivs 3.0 Chile