A Comparison of the Minimum Current Corona to a Magnetohydrodynamic Simulation of Quasi‐Static Coronal Evolution [PDF]
, 2004 D. W. Longcope, Tetsuya Magara
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Dynamical Inference from Polarized Light Curves of Sagittarius A*
The Astrophysical JournalPolarimetric light curves of Sagittarius A* (Sgr A*) sometimes exhibit loops in the Stokes Q and U plane over time, often interpreted as orbiting hotspot motion. In this work, we apply the differential geometry of planar curves to develop a new technique
Angelo Ricarte +5 more
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Probing Physics of Magnetohydrodynamic Turbulence Using Direct Numerical Simulation
, 1998 Mahendra K. Verma, Gaurav Dar
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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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Magnetohydrodynamic Simulations of the Formation of Cold Fronts in Clusters of Galaxies Including Heat Conduction [PDF]
, 2004 N. Asai, Naoya Fukuda, Ryōji Matsumoto
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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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