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dc.contributor.authorLecoanet, Daniel
dc.contributor.authorLe Bars, Michael
dc.contributor.authorVasil, Geoffrey M.
dc.contributor.authorBrown, Benjamin P.
dc.contributor.authorQuataert, Eliot
dc.contributor.authorOishi, Jeffrey S.
dc.contributor.authorBurns, Keaton James
dc.date.accessioned2015-07-01T15:22:55Z
dc.date.available2015-07-01T15:22:55Z
dc.date.issued2015-06
dc.date.submitted2015-04
dc.identifier.issn1539-3755
dc.identifier.issn1550-2376
dc.identifier.urihttp://hdl.handle.net/1721.1/97601
dc.description.abstractWater's density maximum at 4[superscript ∘]C makes it well suited to study internal gravity wave excitation by convection: an increasing temperature profile is unstable to convection below 4[superscript ∘]C, but stably stratified above 4[superscript ∘]C. We present numerical simulations of a waterlike fluid near its density maximum in a two-dimensional domain. We successfully model the damping of waves in the simulations using linear theory, provided we do not take the weak damping limit typically used in the literature. To isolate the physical mechanism exciting internal waves, we use the spectral code dedalus to run several simplified model simulations of our more detailed simulation. We use data from the full simulation as source terms in two simplified models of internal-wave excitation by convection: bulk excitation by convective Reynolds stresses, and interface forcing via the mechanical oscillator effect. We find excellent agreement between the waves generated in the full simulation and the simplified simulation implementing the bulk excitation mechanism. The interface forcing simulations overexcite high-frequency waves because they assume the excitation is by the “impulsive” penetration of plumes, which spreads energy to high frequencies. However, we find that the real excitation is instead by the “sweeping” motion of plumes parallel to the interface. Our results imply that the bulk excitation mechanism is a very accurate heuristic for internal-wave generation by convection.en_US
dc.description.sponsorshipKavli Institute for Astrophysics and Space Research (Graduate Fellowship)en_US
dc.description.sponsorshipNational Science Foundation (U.S.). Graduate Research Fellowship (Grant 1122374)en_US
dc.publisherAmerican Physical Societyen_US
dc.relation.isversionofhttp://dx.doi.org/10.1103/PhysRevE.91.063016en_US
dc.rightsArticle is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use.en_US
dc.sourceAmerican Physical Societyen_US
dc.titleNumerical simulations of internal wave generation by convection in wateren_US
dc.typeArticleen_US
dc.identifier.citationLecoanet, Daniel, Michael Le Bars, Keaton J. Burns, Geoffrey M. Vasil, Benjamin P. Brown, Eliot Quataert, and Jeffrey S. Oishi. "Numerical simulations of internal wave generation by convection in water." Phys. Rev. E 91, 063016 (June 2015). © 2015 American Physical Societyen_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Physicsen_US
dc.contributor.mitauthorBurns, Keaton Jamesen_US
dc.relation.journalPhysical Review Een_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.updated2015-06-30T22:00:05Z
dc.language.rfc3066en
dc.rights.holderAmerican Physical Society
dspace.orderedauthorsLecoanet, Daniel; Le Bars, Michael; Burns, Keaton J.; Vasil, Geoffrey M.; Brown, Benjamin P.; Quataert, Eliot; Oishi, Jeffrey S.en_US
dc.identifier.orcidhttps://orcid.org/0000-0003-4761-4766
mit.licensePUBLISHER_POLICYen_US
mit.metadata.statusComplete


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