{"status":"ok","message-type":"work","message-version":"1.0.0","message":{"indexed":{"date-parts":[[2023,11,28]],"date-time":"2023-11-28T20:59:08Z","timestamp":1701205148083},"reference-count":20,"publisher":"Institute of Electrical and Electronics Engineers (IEEE)","issue":"5","license":[{"start":{"date-parts":[[2018,9,1]],"date-time":"2018-09-01T00:00:00Z","timestamp":1535760000000},"content-version":"vor","delay-in-days":0,"URL":"https:\/\/ieeexplore.ieee.org\/Xplorehelp\/downloads\/license-information\/IEEE.html"},{"start":{"date-parts":[[2018,9,1]],"date-time":"2018-09-01T00:00:00Z","timestamp":1535760000000},"content-version":"stm-asf","delay-in-days":0,"URL":"https:\/\/doi.org\/10.15223\/policy-029"},{"start":{"date-parts":[[2018,9,1]],"date-time":"2018-09-01T00:00:00Z","timestamp":1535760000000},"content-version":"stm-asf","delay-in-days":0,"URL":"https:\/\/doi.org\/10.15223\/policy-037"}],"content-domain":{"domain":[],"crossmark-restriction":false},"short-container-title":["Comput. Sci. Eng."],"published-print":{"date-parts":[[2018,9]]},"DOI":"10.1109\/mcse.2018.05329811","type":"journal-article","created":{"date-parts":[[2018,8,30]],"date-time":"2018-08-30T18:38:42Z","timestamp":1535654322000},"page":"8-17","source":"Crossref","is-referenced-by-count":4,"title":["Simulating Stellar Hydrodynamics at Extreme Scale"],"prefix":"10.1109","volume":"20","author":[{"given":"Paul R.","family":"Woodward","sequence":"first","affiliation":[{"name":"University of Minnesota"}],"role":[{"role":"author","vocabulary":"crossref"}]},{"given":"Falk","family":"Herwig","sequence":"additional","affiliation":[{"name":"University of Victoria"}],"role":[{"role":"author","vocabulary":"crossref"}]},{"given":"Ted","family":"Wetherbee","sequence":"additional","affiliation":[{"name":"Fond du Lac Tribal and Community College"}],"role":[{"role":"author","vocabulary":"crossref"}]}],"member":"263","reference":[{"key":"ref10","doi-asserted-by":"crossref","first-page":"2991","DOI":"10.1093\/mnras\/stw2783","article-title":"Idealized Hydrodynamic Simulations of Turbulent Oxygen-Burning Shell Convection in $4\\pi$ Geometry","volume":"465","author":"jones","year":"2017","journal-title":"Monthly Notices of the Royal Astronomical Society"},{"key":"ref11","doi-asserted-by":"crossref","first-page":"2l","DOI":"10.1051\/0004-6361\/201527171","article-title":"The Growth of Helium-Burning Cores","volume":"582","author":"spruit","year":"2015","journal-title":"Astronomy and Astrophysics"},{"key":"ref12","doi-asserted-by":"crossref","first-page":"3l","DOI":"10.1088\/2041-8205\/792\/1\/L3","article-title":"Global Non-Spherical Oscillations in 3-D $4\\pi$ Simulations of the H-Ingestion Flash","volume":"792","author":"herwig","year":"2014","journal-title":"Astrophysical J Letters"},{"key":"ref13","article-title":"Simulating Turbulent Mixing from Richtmyer-Meshkov and Rayleigh-Taylor Instabilities in Converging Geometries using Moving Cartesian Grids","author":"woodward","year":"0","journal-title":"Proc NECDC2012 LA-UR-13-20949 (NECDC 12)"},{"key":"ref14","article-title":"In-Core Volume Rendering for Cartesian Grid Fluid Dynamics Simulations","author":"wetherbee","year":"0","journal-title":"Proc XSEDE Conf Scientific Advancements Enabled by Enhanced Cyberinfrastructure (XSEDE 15)"},{"key":"ref15","article-title":"The PPM Compressible Gas Dynamics Scheme","author":"woodward","year":"2007","journal-title":"Implicit Large-Eddy Simulation Computing Turbulent Fluid Dynamics"},{"key":"ref16","doi-asserted-by":"publisher","DOI":"10.1088\/0004-637X\/798\/1\/49"},{"key":"ref17","doi-asserted-by":"crossref","first-page":"174","DOI":"10.1016\/0021-9991(84)90143-8","article-title":"The Piecewise-Parabolic Method (PPM) for Gas Dynamical Simulations","volume":"54","author":"colella","year":"1984","journal-title":"J Computational Physics"},{"key":"ref18","article-title":"Scaling the Multifluid PPM Code on Blue Waters and Intel MIC","author":"woodward","year":"0","journal-title":"Extreme Scaling Workshop"},{"key":"ref19","doi-asserted-by":"publisher","DOI":"10.1016\/j.jpdc.2016.04.005"},{"key":"ref4","doi-asserted-by":"crossref","first-page":"37l","DOI":"10.1093\/mnrasl\/slx190","article-title":"Pop III i-Process Nucleosynthesis and the Elemental Abundances of SMSS J0313-6708 and the Most Iron-Poor Stars","volume":"474","author":"clarkson","year":"2018","journal-title":"Monthly Notices of the Royal Astronomical Society"},{"key":"ref3","doi-asserted-by":"crossref","first-page":"1l","DOI":"10.1093\/mnrasl\/slx126","article-title":"Convective-Reactive Nucleosynthesis of K, Sc, Cl, and P-Process Isotopes in O-C Shell Mergers","volume":"474","author":"ritter","year":"2018","journal-title":"Monthly Notices of the Royal Astronomical Society"},{"key":"ref6","doi-asserted-by":"crossref","first-page":"6l","DOI":"10.1051\/0004-6361\/201015428","article-title":"Evolution and Nucleosynthesis of Extremely Metal-Poor and Metal-Free Low- and Intermediate-Mass Stars","volume":"522","author":"campbell","year":"2010","journal-title":"Astronomy and Astrophysics"},{"key":"ref5","doi-asserted-by":"crossref","first-page":"377","DOI":"10.1086\/380989","article-title":"Flash?Driven Convective Mixing in Low?Mass, Metal?deficient Asymptotic Giant Branch Stars: A New Paradigm for Lithium Enrichment and a Possible s?Process","volume":"602","author":"iwamoto","year":"2004","journal-title":"Astrophysical J"},{"key":"ref8","doi-asserted-by":"crossref","first-page":"89","DOI":"10.1088\/0004-637X\/727\/2\/89","article-title":"Convective-reactive Proton-12C Combustion in Sakurai's Object (V4334 Sagittarii) and Implications for the Evolution and Yields from the First Generations of Stars","volume":"727","author":"herwig","year":"2011","journal-title":"Astrophysical J"},{"key":"ref7","doi-asserted-by":"crossref","first-page":"435","DOI":"10.1146\/annurev.astro.43.072103.150600","article-title":"Evolution of Asymptotic Giant Branch Stars","volume":"43","author":"herwig","year":"2005","journal-title":"Ann Rev Astronomy and Astrophysics"},{"key":"ref2","doi-asserted-by":"crossref","first-page":"3848","DOI":"10.1093\/mnras\/stv2488","article-title":"H Ingestion into He-Burning Convection Zones in Super-AGB Stellar Models as a Potential Site for Intermediate Neutron-Density Nucleosynthesis","volume":"455","year":"2016","journal-title":"Monthly Notices of the Royal Astronomical Society"},{"key":"ref1","doi-asserted-by":"crossref","first-page":"651","DOI":"10.1086\/425419","article-title":"Evolution and Yields of Extremely Metal?poor Intermediate?Mass Stars","volume":"155","author":"herwig","year":"2004","journal-title":"Astrophysical J Suppl"},{"key":"ref9","first-page":"497","article-title":"Hydrodynamical Models of Stellar Convection","volume":"313","author":"freytag","year":"1996","journal-title":"Astronomy and Astrophysics"},{"key":"ref20","first-page":"33","article-title":"mPPM Viewed as a Co-Design Effort","author":"woodward","year":"0","journal-title":"Proc 1st Int'l Workshop on Hardware-Software Co-Design for HPC (Co-HPC 14)"}],"container-title":["Computing in Science & Engineering"],"original-title":[],"link":[{"URL":"http:\/\/xplorestaging.ieee.org\/ielx7\/5992\/8452043\/08452054.pdf?arnumber=8452054","content-type":"unspecified","content-version":"vor","intended-application":"similarity-checking"}],"deposited":{"date-parts":[[2022,5,3]],"date-time":"2022-05-03T19:57:53Z","timestamp":1651607873000},"score":1,"resource":{"primary":{"URL":"https:\/\/ieeexplore.ieee.org\/document\/8452054\/"}},"subtitle":[],"short-title":[],"issued":{"date-parts":[[2018,9]]},"references-count":20,"journal-issue":{"issue":"5"},"URL":"https:\/\/doi.org\/10.1109\/mcse.2018.05329811","relation":{},"ISSN":["1521-9615","1558-366X"],"issn-type":[{"value":"1521-9615","type":"print"},{"value":"1558-366X","type":"electronic"}],"subject":[],"published":{"date-parts":[[2018,9]]}}}