The Astrophysical JournalMagnetohydrodynamic (MHD) simulations of the solar corona are often started from a potential field initial condition, which may be far from the true state of the coronal magnetic field. To test the sensitivity of the simulations to the initial condition,
Graham Barnes +2 more
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Temporal Properties of Compressible Magnetohydrodynamic Turbulence
The Astrophysical JournalDescribing the temporal properties of compressible magnetohydrodynamic (MHD) turbulence is a fundamental problem that has important implications for particle acceleration and transport in astrophysical plasmas.
Ka Ho Yuen, Hui Li, Huirong Yan
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The life cycle of the Central Molecular Zone - II. Distribution of atomic and molecular gas tracers. [PDF]
Mon Not R Astron Soc, 2020 Armillotta L +2 more
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General Relativistic Magnetohydrodynamic Simulations of Black Hole Accretion Disks [PDF]
, 2004 John F. Hawley +1 more
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Force Analysis of Venus’s Induced Magnetosphere: A Multifluid Hall–Magnetohydrodynamics Study
The Astrophysical JournalUnderstanding which processes control atmospheric escape and the loss of water from planetary environments is crucial. The ESA’s Venus Express spacecraft has observed a significant depletion in Venus’s upper atmosphere, driven by the solar wind.
Nihan Chen +10 more
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Three-Dimensional Magnetohydrodynamic Numerical Simulations of Coronal Loop Oscillations Associated with Flares [PDF]
, 2004 Takehiro Miyagoshi +2 more
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The Astrophysical JournalIn magnetar crusts, magnetic fields are sufficiently strong to confine electrons into a small to moderate number of quantized Landau levels. This can have a dramatic effect on the crust's thermodynamic properties, generating field-dependent de Haas–van ...
Peter B. Rau, Ira Wasserman
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Impeding Turbulence Decay in Self-gravitating Cloud Cores
The Astrophysical JournalTurbulence governs the fragmentation of molecular clouds and plays a pivotal role in star formation. The persistence of observed cloud turbulence suggests it does not decay significantly within the turnover timescale, implying a recurrent driving ...
Shibo Yuan, Hua-bai Li
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Three-Dimensional Magnetohydrodynamic Simulation of Nonlinear Magnetic Buoyancy Instability of Flux Sheets with Magnetic Shear [PDF]
, 2005 Satoshi Nozawa
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Second Core Formation and High-Speed Jets: Resistive Magnetohydrodynamic Nested Grid Simulations [PDF]
, 2006 Masahiro N. Machida +2 more
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