There are no files associated with this item.
Full metadata record
DC Field | Value | Language |
---|---|---|
dc.citation.number | 4 | - |
dc.citation.startPage | 041404 | - |
dc.citation.title | PHYSICS OF PLASMAS | - |
dc.citation.volume | 24 | - |
dc.contributor.author | Tzeferacos, P. | - |
dc.contributor.author | Rigby, A. | - |
dc.contributor.author | Bott, A. | - |
dc.contributor.author | Bell, A. R. | - |
dc.contributor.author | Bingham, R. | - |
dc.contributor.author | Casner, A. | - |
dc.contributor.author | Cattaneo, F. | - |
dc.contributor.author | Churazov, E. M. | - |
dc.contributor.author | Emig, J. | - |
dc.contributor.author | Flocke, N. | - |
dc.contributor.author | Fiuza, F. | - |
dc.contributor.author | Forest, C. B. | - |
dc.contributor.author | Foster, J. | - |
dc.contributor.author | Graziani, C. | - |
dc.contributor.author | Katz, J. | - |
dc.contributor.author | Koenig, M. | - |
dc.contributor.author | Li, C. -K. | - |
dc.contributor.author | Meinecke, J. | - |
dc.contributor.author | Petrasso, R. | - |
dc.contributor.author | Park, H. -S. | - |
dc.contributor.author | Remington, B. A. | - |
dc.contributor.author | Ross, J. S. | - |
dc.contributor.author | Ryu, Dongsu | - |
dc.contributor.author | Ryutov, D. | - |
dc.contributor.author | Weide, K. | - |
dc.contributor.author | White, T. G. | - |
dc.contributor.author | Reville, B. | - |
dc.contributor.author | Miniati, F. | - |
dc.contributor.author | Schekochihin, A. A. | - |
dc.contributor.author | Froula, D. H. | - |
dc.contributor.author | Gregori, G. | - |
dc.contributor.author | Lamb, D. Q. | - |
dc.date.accessioned | 2023-12-21T22:18:57Z | - |
dc.date.available | 2023-12-21T22:18:57Z | - |
dc.date.created | 2017-05-26 | - |
dc.date.issued | 2017-04 | - |
dc.description.abstract | The universe is permeated by magnetic fields, with strengths ranging from a femtogauss in the voids between the filaments of galaxy clusters to several teragauss in black holes and neutron stars. The standard model behind cosmological magnetic fields is the nonlinear amplification of seed fields via turbulent dynamo to the values observed. We have conceived experiments that aim to demonstrate and study the turbulent dynamo mechanism in the laboratory. Here, we describe the design of these experiments through simulation campaigns using FLASH, a highly capable radiation magnetohydrodynamics code that we have developed, and large-scale three-dimensional simulations on the Mira supercomputer at the Argonne National Laboratory. The simulation results indicate that the experimental platform may be capable of reaching a turbulent plasma state and determining the dynamo amplification. We validate and compare our numerical results with a small subset of experimental data using synthetic diagnostics. | - |
dc.identifier.bibliographicCitation | PHYSICS OF PLASMAS, v.24, no.4, pp.041404 | - |
dc.identifier.doi | 10.1063/1.4978628 | - |
dc.identifier.issn | 1070-664X | - |
dc.identifier.uri | https://scholarworks.unist.ac.kr/handle/201301/21995 | - |
dc.identifier.url | http://aip.scitation.org/doi/10.1063/1.4978628 | - |
dc.identifier.wosid | 000400390700008 | - |
dc.language | 영어 | - |
dc.publisher | AMER INST PHYSICS | - |
dc.title | Numerical modeling of laser-driven experiments aiming to demonstrate magnetic field amplification via turbulent dynamo | - |
dc.type | Article | - |
dc.description.isOpenAccess | FALSE | - |
dc.relation.journalWebOfScienceCategory | Physics, Fluids & Plasmas | - |
dc.relation.journalResearchArea | Physics | - |
dc.description.journalRegisteredClass | scie | - |
dc.description.journalRegisteredClass | scopus | - |
dc.subject.keywordPlus | STAGGERED MESH SCHEME | - |
dc.subject.keywordPlus | SIMULATIONS | - |
dc.subject.keywordPlus | SATURATION | - |
dc.subject.keywordPlus | GENERATION | - |
dc.subject.keywordPlus | FLASH | - |
dc.subject.keywordPlus | INDUCTION | - |
dc.subject.keywordPlus | CLUSTERS | - |
dc.subject.keywordPlus | CRITERIA | - |
dc.subject.keywordPlus | PLASMA | - |
Items in Repository are protected by copyright, with all rights reserved, unless otherwise indicated.
Tel : 052-217-1404 / Email : scholarworks@unist.ac.kr
Copyright (c) 2023 by UNIST LIBRARY. All rights reserved.
ScholarWorks@UNIST was established as an OAK Project for the National Library of Korea.