Results 151 to 160 of about 5,169 (254)

THREE-DIMENSIONAL MAGNETOHYDRODYNAMIC SIMULATIONS OF CIRCUMBINARY ACCRETION DISKS: DISK STRUCTURES AND ANGULAR MOMENTUM TRANSPORT [PDF]

, 2012
Ji-Ming Shi, Julian H. Krolik, Stephen H. Lubow, John F. Hawley   +3 more
openalex   +1 more source

Comparative Analysis of Hall Effect Implementations in Hall Magnetohydrodynamics

The Astrophysical Journal
There is no standard numerical implementation of the Hall effect, which is one of the nonideal magnetohydrodynamic (MHD) effects. Numerical instability arises when a simple implementation is used, in which the Hall electric field is added to the electric
Kazunari Iwasaki, Kengo Tomida
doaj   +1 more source

Over 20‐Year Global Magnetohydrodynamic Simulation of Earth's Magnetosphere [PDF]

, 2022
Ilja Honkonen, Max van de Kamp, Theresa Hoppe, Kirsti Kauristie   +3 more
openalex   +1 more source

Fast Magnetoacoustic Wave Behavior within Gravitationally Stratified, Magnetically Inhomogeneous Media

The Astrophysical Journal
The nature of MHD waves within inhomogeneous media is fundamental to understanding and interpreting wave behavior in the solar atmosphere. We investigate fast magnetoacoustic wave behavior within gravitationally stratified, magnetically inhomogeneous ...
Ryan T. Smith, James A. McLaughlin, Gert J. J. Botha   +2 more
doaj   +1 more source

Comparative statistics of selected subgrid-scale models in large-eddy simulations of decaying, supersonic magnetohydrodynamic turbulence [PDF]

, 2017
Philipp Grete, D. G. Vlaykov, W. Schmidt, D. R. G. Schleicher   +3 more
openalex   +1 more source

Global Non-ideal Magnetohydrodynamic Simulations of Protoplanetary Disks with Outer Truncation [PDF]

, 2021
Haifeng Yang, Xue‐Ning Bai
openalex   +1 more source

Turbulent Diffuse Molecular Media with Nonideal Magnetohydrodynamics and Consistent Thermochemistry: Numerical Simulations and Dynamic Characteristics

The Astrophysical Journal
Turbulent diffuse molecular clouds can exhibit complicated morphologies caused by the interactions among radiation, chemistry, fluids, and fields.
Nannan Yue, Lile Wang, Thomas Bisbas, Donghui Quan, Di Li   +4 more
doaj   +1 more source

Oscillatory disintegration of a trans-Alfvénic shock: A magnetohydrodynamic simulation [PDF]

, 2000
S. A. Markovskii, S. L. Skorokhodov
openalex   +1 more source

A Data-constrained Magnetohydrodynamic Simulation of the X1.0 Solar Flare of 2021 October 28 [PDF]

, 2022
Daiki Yamasaki, Satoshi Inoue, Yumi Bamba, Jeongwoo Lee, Haimin Wang   +4 more
openalex   +1 more source

Cosmic-Ray Feedback on Bistable Interstellar Medium Turbulence

The Astrophysical Journal
While cosmic rays ( E ≳ 1 GeV) are well coupled to a galaxy’s interstellar medium (ISM) at scales of L > 100 pc, adjusting stratification and driving outflows, their impact on small scales is less clear.
Roark Habegger, Ka Wai Ho, Ka Ho Yuen, Ellen G. Zweibel   +3 more
doaj   +1 more source