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19942023
most citedThe Protogalactic Origin for Cosmic Magnetic Fields

456 citations · 8.7k across the 154 of their papers we have counts for

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6 papers · 1 filter

astro-ph2000★ 1 cited

Winds and Shocks in Galaxy Clusters: Shock Acceleration on an Intergalactic Scale

T. W. Jones, Francesco Miniati, Dongsu Ryu +1

We review the possible roles of large scale shocks as particle accelerators in clusters of galaxies. Recent observational and theoretical work has suggested that high energy charge…

astro-ph2000★ 117 cited

The Magnetohydrodynamic Kelvin-Helmholtz Instability: A Three-Dimensional Study of Nonlinear Evolution

Dongsu Ryu, T. W. Jones, Adam Frank

We investigate through high resolution 3D simulations the nonlinear evolution of compressible magnetohydrodynamic flows subject to the Kelvin-Helmholtz instability. We confirm in 3…

astro-ph2000★ 25 cited

The Parker Instability in a Thick Gaseous Disk II: Numerical Simulations in 2D

Alfredo Santillan, Jongsoo Kim, Jose Franco +3

We present 2D, ideal-MHD numerical simulations of the Parker instability in a multi-component warm disk model. The calculations were done using two numerical codes with different a…

astro-ph2000

3-D MHD Numerical Simulations of Cloud-Wind Interactions

G. Gregori, Francesco Miniati, Dongsu Ryu +1

We present results from three-dimensional (3-D) numerical simulations investigating the magnetohydrodynamics of cloud-wind interactions. The initial cloud is spherical while the ma…

astro-ph2000

Acceleration of CR at Large Scale Shocks and Their Cosmological Role for Structure Formation in the Universe

Francesco Miniati, Dongsu Ryu, T. W. Jones +1

We investigate the dynamical importance of a newly recognized possible source of significant feedback generated during structure formation; namely cosmic ray (CR) pressure. We pres…

astro-ph2000★ 281 cited

Properties of Cosmic Shock Waves in Large Scale Structure Formation

Francesco Miniati, Dongsu Ryu, Hyesung Kang +3

We have examined the properties of shock waves in simulations of large scale structure formation for two cosmological scenarios (a SCDM and a LCDM with Omega =1). Large-scale shock…