Results 11 to 20 of about 5,169 (254)
RADIATIVE MAGNETOHYDRODYNAMIC SIMULATION OF SUNSPOT STRUCTURE [PDF]
The Astrophysical Journal, 2009 Results of a three-dimensional MHD simulation of a sunspot with a photospheric size of about 20 Mm are presented. The simulation has been carried out with the MURaM code, which includes a realistic equation of state with partial ionization and radiative transfer along many ray directions.
M. Rempel, M. Schüßler, M. Knölker
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Stream-aligned Magnetohydrodynamics for Solar Wind Simulations [PDF]
The Astrophysical Journal, 2021 Abstract We present a reduced magnetohydrodynamic (MHD) mathematical model describing the dynamical behavior of highly conducting plasmas with frozen-in magnetic fields, constrained by the assumption that there exists a frame of reference, where the magnetic field vector,
Igor V. Sokolov +2 more
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Simulations of Incompressible Magnetohydrodynamic Turbulence [PDF]
The Astrophysical Journal, 2001 We simulate incompressible MHD turbulence using a pseudospectral code. Our major conclusions are: (1) MHD turbulence is most conveniently described in terms of counterpropagating shear Alfven and slow waves. Shear Alfven waves control the cascade dynamics. Slow waves play a passive role and adopt the spectrum set by the shear Alfven waves.
Maron, Jason, Goldreich, Peter
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SIMULATIONS OF ELECTRON MAGNETOHYDRODYNAMIC TURBULENCE
The Astrophysical Journal, 2009 We present numerical simulations of electron magnetohydrodynamic (EMHD) and electron reduced MHD (ERMHD) turbulence. Comparing scaling relations, we find that both EMHD and ERMHD turbulence show similar spectra and anisotropy. We develop new techniques to study anisotropy of EMHD turbulence.
Cho, Jungyeon, Lazarian, A.
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RESISTIVE MAGNETOHYDRODYNAMIC SIMULATIONS OF RELATIVISTIC MAGNETIC RECONNECTION [PDF]
The Astrophysical Journal, 2010 published in ...
Zenitani, Seiji +2 more
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General relativistic magnetohydrodynamical simulations of the jet in M87 [PDF]
, 2016 (abridged) The connection between black hole, accretion disk, and radio jet can be best constrained by fitting models to observations of nearby low luminosity galactic nuclei, in particular the well studied sources Sgr~A* and M87.
Falcke, Heino +2 more
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Striped Jets in Post–Neutron Star Merger Systems
The Astrophysical Journal, 2023 Models invoking magnetic reconnection as the particle acceleration mechanism within relativistic jets often adopt a gradual energy dissipation profile within the jet. However, such a profile has yet to be reproduced in first-principles simulations.
Emma Kaufman +4 more
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MAGNETOHYDRODYNAMIC SIMULATIONS OF HOT JUPITER UPPER ATMOSPHERES [PDF]
The Astrophysical Journal, 2014 accepted at ...
Trammell, George B. +2 more
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The Astrophysical Journal, 2023 Nonequilibrium ionization (NEI) is essentially required for astrophysical plasma diagnostics once the plasma status departs from the assumption of ionization equilibrium.
Chengcai Shen +2 more
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The Formation of Star-forming Disks in the TNG50 Simulation
The Astrophysical Journal, 2023 We investigate the disk formation process in the TNG50 simulation, examining the profiles of SFR surface density (Σ _SFR ), gas inflow and outflow, and the evolution of the angular momentum of inflowing gas particles.
Enci Wang, Simon J. Lilly
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