Laboratory evidence of dynamo amplification of magnetic fields in a turbulent plasma
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D. Lamb | R. Bingham | J. Ross | J. Foster | C. Graziani | C. Forest | D. Ryutov | C. Li | M. Koenig | B. Remington | D. Ryu | F. Miniati | A. Schekochihin | A. Casner | D. Froula | H. Park | A. Bell | J. Ross | B. Reville | E. Churazov | G. Gregori | P. Tzeferacos | T. White | F. Fiuza | F. Cattaneo | J. Emig | R Bingham | M Koenig | A Casner | H-S Park | D H Froula | C B Forest | B A Remington | J. Meinecke | P Tzeferacos | D Q Lamb | A R Bell | G Gregori | A. Rigby | J. Katz | A A Schekochihin | A. Bott | J. Foster | C.K. Li | R. Petrasso | C Graziani | J Emig | J Meinecke | J S Ross | F Fiuza | D Ryutov | A Rigby | A F A Bott | F Cattaneo | E M Churazov | J Foster | J Katz | C-K Li | R Petrasso | D Ryu | T G White | B Reville | F Miniati
[1] D. Lamb,et al. Proton imaging of stochastic magnetic fields , 2017, Journal of Plasma Physics.
[2] D. Lamb,et al. Numerical modeling of laser-driven experiments aiming to demonstrate magnetic field amplification via turbulent dynamo , 2017, 1702.03015.
[3] D. Lamb,et al. Inferring morphology and strength of magnetic fields from proton radiographs. , 2016, The Review of scientific instruments.
[4] Klaus Weide,et al. FLASH MHD simulations of experiments that study shock-generated magnetic fields , 2015 .
[5] F. Miniati,et al. The generation and amplification of intergalactic magnetic fields in analogue laboratory experiments with high power lasers , 2015 .
[6] Francesco Miniati,et al. Self-similar energetics in large clusters of galaxies , 2015, Nature.
[7] Robert Crowston,et al. Developed turbulence and nonlinear amplification of magnetic fields in laboratory and astrophysical plasmas , 2015, Proceedings of the National Academy of Sciences.
[8] Petros Tzeferacos,et al. Collisionless shock experiments with lasers and observation of Weibel instabilities , 2015 .
[9] C. Ott,et al. Implicit large eddy simulations of anisotropic weakly compressible turbulence with application to core-collapse supernovae , 2015, 1501.03169.
[10] C. Federrath,et al. THE TURBULENT DYNAMO IN HIGHLY COMPRESSIBLE SUPERSONIC PLASMAS , 2014, 1411.4707.
[11] Klaus Weide,et al. THE BIERMANN CATASTROPHE IN NUMERICAL MAGNETOHYDRODYNAMICS , 2014, 1408.4161.
[12] Anthony Scopatz,et al. Turbulent amplification of magnetic fields in laboratory laser-produced shock waves , 2014, Nature Physics.
[13] S. Allen,et al. THE RELATION BETWEEN GAS DENSITY AND VELOCITY POWER SPECTRA IN GALAXY CLUSTERS: QUALITATIVE TREATMENT AND COSMOLOGICAL SIMULATIONS , 2014, 1404.5306.
[14] D. Nagai,et al. The relation between gas density and velocity power spectra in galaxy clusters: High-resolution hydrodynamic simulations and the role of conduction , 2014, 1404.5302.
[15] D. Ryutov,et al. Collisional effects in the ion Weibel instability for two counter-propagating plasma streams , 2014 .
[16] B. Reville,et al. SCALING OF MAGNETO-QUANTUM-RADIATIVE HYDRODYNAMIC EQUATIONS: FROM LASER-PRODUCED PLASMAS TO ASTROPHYSICS , 2014, 1401.7880.
[17] F. Krause,et al. The Inverse Scattering Transformation and the Theory of Solitons. By W. ECKHAUS and A. VAN HARTEN. North-Holland, 1981. 222pp. $31.75. , 1982, Journal of Fluid Mechanics.
[18] R. P. Drake,et al. Observation of magnetic field generation via the Weibel instability in interpenetrating plasma flows , 2013, Nature Physics.
[19] A. Lazarian,et al. Astrophysical Hydromagnetic Turbulence , 2013, 1307.5496.
[20] Dongwook Lee,et al. A solution accurate, efficient and stable unsplit staggered mesh scheme for three dimensional magnetohydrodynamics , 2013, J. Comput. Phys..
[21] Klaus Weide,et al. Modeling HEDLA magnetic field generation experiments on laser facilities , 2013 .
[22] Y. Zakharov. Comment on “Studying astrophysical collisionless shocks with counterstreaming plasmas from high power lasers” , 2012 .
[23] R. P. Drake,et al. Self-organized electromagnetic field structures in laser-produced counter-streaming plasmas , 2012, Nature Physics.
[24] Moscow,et al. A Mexican hat with holes: calculating low-resolution power spectra from data with gaps , 2012, 1207.5825.
[25] J. Frenje,et al. Source characterization and modeling development for monoenergetic-proton radiography experiments on OMEGA. , 2012, The Review of scientific instruments.
[26] R. P. Drake,et al. DESIGN CONSIDERATIONS FOR UNMAGNETIZED COLLISIONLESS-SHOCK MEASUREMENTS IN HOMOLOGOUS FLOWS , 2012 .
[27] D. Sokoloff,et al. Current Status of Turbulent Dynamo Theory , 2012, 1203.6195.
[28] R. P. Drake,et al. Studying astrophysical collisionless shocks with counterstreaming plasmas from high power lasers , 2012 .
[29] R. P. Drake,et al. Generation of scaled protogalactic seed magnetic fields in laser-produced shock waves , 2012, Nature.
[30] D. Ryutov,et al. Invited article: Relation between electric and magnetic field structures and their proton-beam images. , 2012, The Review of scientific instruments.
[31] Wojciech Rozmus,et al. Characterizing counter-streaming interpenetrating plasmas relevant to astrophysical collisionless shocks , 2011 .
[32] H. Boehringer,et al. X-ray surface brightness and gas density fluctuations in the Coma cluster , 2011, 1110.5875.
[33] A. Beresnyak. Universal nonlinear small-scale dynamo. , 2011, Physical review letters.
[34] Hamburg,et al. Mach number dependence of turbulent magnetic field amplification: solenoidal versus compressive flows. , 2011, Physical review letters.
[35] J. F. Williams,et al. An efficient approach for the numerical solution of the Monge-Ampère equation , 2011 .
[36] R. Klessen,et al. THE GENERATION OF STRONG MAGNETIC FIELDS DURING THE FORMATION OF THE FIRST STARS , 2010, 1008.3481.
[37] D. Lamb,et al. Inertial range Eulerian and Lagrangian statistics from numerical simulations of isotropic turbulence , 2010, Journal of Fluid Mechanics.
[38] Andrew Siegel,et al. Extensible component-based architecture for FLASH, a massively parallel, multiphysics simulation code , 2009, Parallel Comput..
[39] D. Ryu,et al. Turbulence and Magnetic Fields in the Large-Scale Structure of the Universe , 2008, Science.
[40] D. Lamb,et al. Intermittency and universality in fully developed inviscid and weakly compressible turbulent flows. , 2007, Physical review letters.
[41] J. McWilliams,et al. Fluctuation dynamo and turbulent induction at low magnetic Prandtl numbers , 2007, 0704.2002.
[42] J. Pinton,et al. Generation of a magnetic field by dynamo action in a turbulent flow of liquid sodium. , 2007, Physical review letters.
[43] J. R. Rygg,et al. Measuring E and B fields in laser-produced plasmas with monoenergetic proton radiography. , 2006, Physical review letters.
[44] A. Schekochihin,et al. Turbulence, magnetic fields, and plasma physics in clusters of galaxies , 2006, astro-ph/0601246.
[45] K. Subramanian,et al. Evolving turbulence and magnetic fields in galaxy clusters , 2005, astro-ph/0505144.
[46] Imperial College London,et al. Simulations of the Small-Scale Turbulent Dynamo , 2003, astro-ph/0312046.
[47] R. Sunyaev,et al. Turbulence in clusters of galaxies and X-ray line profiles , 2003, astro-ph/0310737.
[48] N. Haugen,et al. Simulations of nonhelical hydromagnetic turbulence. , 2003, Physical review. E, Statistical, nonlinear, and soft matter physics.
[49] T. Ensslin,et al. The magnetic power spectrum in Faraday rotation screens , 2003, astro-ph/0302426.
[50] C. Carilli,et al. Cluster Magnetic Fields , 2001, astro-ph/0110655.
[51] B. Fryxell,et al. FLASH: An Adaptive Mesh Hydrodynamics Code for Modeling Astrophysical Thermonuclear Flashes , 2000 .
[52] M. Christen,et al. Magnetic field saturation in the Riga dynamo experiment. , 2000, Physical review letters.
[53] Gerbeth,et al. Detection of a flow induced magnetic field eigenmode in the riga dynamo facility , 1999, Physical review letters.
[54] S. Segre,et al. A review of plasma polarimetry—theory and methods , 1999 .
[55] K. Hurley,et al. An X-ray pulsar with a superstrong magnetic field in the soft γ-ray repeater SGR1806 − 20 , 1998, Nature.
[56] W. Gangbo,et al. The geometry of optimal transportation , 1996 .
[57] R. Cen,et al. The Protogalactic Origin for Cosmic Magnetic Fields , 1996, astro-ph/9607141.
[58] N. Kleeorin,et al. Magnetohydrodynamic turbulence in the solar convective zone as a source of oscillations and sunspots formation. , 1996 .
[59] Kleeorin,et al. Effective Ampère force in developed magnetohydrodynamic turbulence. , 1994, Physical review. E, Statistical physics, plasmas, fluids, and related interdisciplinary topics.
[60] A. Ruzmaikin,et al. Spectrum of the galactic magnetic fields , 1982 .
[61] U. Frisch,et al. Helical and Nonhelical Turbulent Dynamos , 1981 .
[62] L. Lucy. An iterative technique for the rectification of observed distributions , 1974 .
[63] A. P. Kazantsev. Enhancement of a magnetic field by a conducting fluid , 1968 .
[64] W. B. Thompson. Transport Processes in the Plasma , 1960 .
[65] E. Parker. Hydromagnetic Dynamo Models , 1955 .
[66] L. Biermann,et al. Cosmic Radiation and Cosmic Magnetic Fields. II. Origin of Cosmic Magnetic Fields , 1951 .
[67] G. Batchelor. On the spontaneous magnetic field in a conducting liquid in turbulent motion , 1950, Proceedings of the Royal Society of London. Series A. Mathematical and Physical Sciences.
[68] Brad Gallagher,et al. Terascale turbulence computation using the FLASH3 application framework on the IBM Blue Gene/L system , 2008, IBM J. Res. Dev..
[69] S. Owley,et al. Simulations of the Small-scale Turbulent Dynamo , 2008 .
[70] C. Heiles,et al. Magnetic fields in galaxies and beyond , 1997, Nature.
[71] Samuel A. Letzring,et al. Initial performance results of the OMEGA laser system , 1997 .
[72] R. Kulsrud. Important plasma problems in astrophysics , 1995 .
[73] Yu. B. Ponomarenko,et al. Theory of the hydromagnetic generator , 1973 .
[74] William H. Richardson,et al. Bayesian-Based Iterative Method of Image Restoration , 1972 .
[75] K. Papadopoulos,et al. SPONTANEOUS MAGNETIC FIELDS IN LASER-PRODUCED PLASMAS. , 1971 .
[76] D. Evans,et al. Laser light scattering in laboratory plasmas , 1969 .
[77] B. Trubnikov. Particle Interactions in a Fully Ionized Plasma , 1965 .