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dc.contributor.authorSchillo, Kevin
dc.contributor.authorCassibry, Jason
dc.contributor.authorRodriguez, Mitchell
dc.contributor.authorThompson, Seth
dc.date.accessioned2019-09-18T09:05:48Z
dc.date.available2019-09-18T09:05:48Z
dc.date.copyright7/19/2019 12:00:00 AM
dc.date.issued2019
dc.identifier.issn2332-8983
dc.identifier.otherners_005_04_042201
dc.identifier.urihttp://yetl.yabesh.ir/yetl1/handle/yetl/4258806
dc.description.abstractThree-dimensional (3D) modeling of magneto-inertial fusion (MIF) is at a nascent stage of development. A suite of test cases relevant to plasma liner formation and implosion is presented to present the community with some exact solutions for verification of hydrocodes pertaining to MIF confinement concepts. MIF is of particular interest to fusion research, as it may lead to the development of smaller and more economical reactor designs for power and propulsion. The authors present simulated test cases using a new smoothed particle hydrodynamic (SPH) code called SPFMax. These test cases consist of a total of six problems with analytical solutions that incorporate the physics of radiation cooling, heat transfer, oblique-shock capturing, angular-momentum conservation, and viscosity effects. These physics are pertinent to plasma liner formation and implosion by merging of a spherical array of plasma jets as a candidate standoff driver for MIF. An L2 norm analysis was conducted for each test case. Each test case was found to converge to the analytical solution with increasing resolution, and the convergence rate was on the order of what has been reported by other SPH studies.
dc.publisherAmerican Society of Mechanical Engineers (ASME)
dc.titleSuite for Smooth Particle Hydrodynamic Code Relevant to Spherical Plasma Liner Formation and Implosion
dc.typeJournal Paper
dc.journal.volume5
dc.journal.issue4
dc.journal.titleJournal of Nuclear Engineering and Radiation Science
dc.identifier.doi10.1115/1.4042710
dc.journal.fristpage42201
dc.journal.lastpage042201-13
dc.treeJournal of Nuclear Engineering and Radiation Science:;2019:;volume( 005 ):;issue: 004
dc.contenttypeFulltext


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