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dc.contributor.authorTilmes, Simone
dc.contributor.authorEmmons, Louisa
dc.contributor.authorLamarque, Jean-François
dc.contributor.authorCameron-Smith, Philip
dc.contributor.authorBrown-Steiner, Benjamin E
dc.contributor.authorSelin, Noelle E
dc.contributor.authorPrinn, Ronald G
dc.date.accessioned2019-01-29T20:02:41Z
dc.date.available2019-01-29T20:02:41Z
dc.date.issued2018-10
dc.date.submitted2018-08
dc.identifier.issn1991-9603
dc.identifier.issn1991-959X
dc.identifier.urihttp://hdl.handle.net/1721.1/120143
dc.description.abstractWhile state-of-the-art complex chemical mechanisms expand our understanding of atmospheric chemistry, their sheer size and computational requirements often limit simulations to short lengths or ensembles to only a few members. Here we present and compare three 25-year present-day offline simulations with chemical mechanisms of different levels of complexity using the Community Earth System Model (CESM) Version 1.2 CAM-chem (CAM4): the Model for Ozone and Related Chemical Tracers, version 4 (MOZART-4) mechanism, the Reduced Hydrocarbon mechanism, and the Super-Fast mechanism. We show that, for most regions and time periods, differences in simulated ozone chemistry between these three mechanisms are smaller than the model-observation differences themselves. The MOZART-4 mechanism and the Reduced Hydrocarbon are in close agreement in their representation of ozone throughout the troposphere during all time periods (annual, seasonal, and diurnal). While the Super-Fast mechanism tends to have higher simulated ozone variability and differs from the MOZART-4 mechanism over regions of high biogenic emissions, it is surprisingly capable of simulating ozone adequately given its simplicity. We explore the trade-offs between chemical mechanism complexity and computational cost by identifying regions where the simpler mechanisms are comparable to the MOZART-4 mechanism and regions where they are not. The Super-Fast mechanism is 3 times as fast as the MOZART-4 mechanism, which allows for longer simulations or ensembles with more members that may not be feasible with the MOZART-4 mechanism given limited computational resources.en_US
dc.description.sponsorshipUnited States. Department of Energy (Grant DE-FG02-94ER61937)en_US
dc.publisherCopernicus GmbHen_US
dc.relation.isversionofhttp://dx.doi.org/10.5194/gmd-11-4155-2018en_US
dc.rightsCreative Commons Attribution 4.0 International licenseen_US
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/en_US
dc.sourceCopernicusen_US
dc.titleEvaluating simplified chemical mechanisms within present-day simulations of the Community Earth System Model version 1.2 with CAM4 (CESM1.2 CAM-chem): MOZART-4 vs. Reduced Hydrocarbon vs. Super-Fast chemistryen_US
dc.typeArticleen_US
dc.identifier.citationBrown-Steiner, Benjamin et al. “Evaluating Simplified Chemical Mechanisms Within Present-Day Simulations of the Community Earth System Model Version 1.2 with CAM4 (CESM1.2 CAM-Chem): MOZART-4 Vs. Reduced Hydrocarbon Vs. Super-Fast Chemistry.” Geoscientific Model Development 11, 10 (October 2018): 4155–4174 © 2018 Author(s)en_US
dc.contributor.departmentMassachusetts Institute of Technology. Center for Global Change Scienceen_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciencesen_US
dc.contributor.departmentMassachusetts Institute of Technology. Institute for Data, Systems, and Societyen_US
dc.contributor.departmentMassachusetts Institute of Technology. Joint Program on the Science & Policy of Global Changeen_US
dc.contributor.mitauthorBrown-Steiner, Benjamin E
dc.contributor.mitauthorSelin, Noelle E
dc.contributor.mitauthorPrinn, Ronald G
dc.relation.journalGeoscientific Model Developmenten_US
dc.eprint.versionFinal published versionen_US
dc.type.urihttp://purl.org/eprint/type/JournalArticleen_US
eprint.statushttp://purl.org/eprint/status/PeerRevieweden_US
dc.date.updated2019-01-18T16:34:04Z
dspace.orderedauthorsBrown-Steiner, Benjamin; Selin, Noelle E.; Prinn, Ronald; Tilmes, Simone; Emmons, Louisa; Lamarque, Jean-François; Cameron-Smith, Philipen_US
dspace.embargo.termsNen_US
dc.identifier.orcidhttps://orcid.org/0000-0002-6396-5622
dc.identifier.orcidhttps://orcid.org/0000-0001-5925-3801
mit.licensePUBLISHER_CCen_US


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