Results 131 to 140 of about 1,046 (208)

The prevalence of pseudo-bulges in the Auriga simulations [PDF]

We study the galactic bulges in the Auriga simulations, a suite of 30 cosmological magnetohydrodynamical zoom-in simulations of late-type galaxies in Milky Way sized dark matter haloes performed with the moving-mesh code AREPO.
Gómez, FA, Monachesi, A, Grand, RJJ, Tissera, P, Gargiulo, ID, Pakmor, R, White, SDM, Marinacci, F, Bell, EF, Fragkoudi, F   +9 more
core   +1 more source

Resistive Magnetohydrodynamics Simulation of Fusion Plasmas [PDF]

, 2001
Tang, X.Z., Fu, G. Y., Jardin, S. C., Lowe, L. L., Park, W., Strauss, H. R.   +5 more
openaire   +2 more sources

Magnetohydrodynamic Simulation of a Coronal Mass Ejection Observed during the Near-radial Alignment of Solar Orbiter and Earth

The Astrophysical Journal
Interplanetary coronal mass ejections (ICMEs) are the primary sources of geomagnetic storms at Earth. The negative out-of-ecliptic component ( B _z ) of magnetic field in the ICME or its associated sheath region is necessary for it to be geoeffective ...
Talwinder Singh, Dinesha V. Hegde, Tae K. Kim, Nikolai V. Pogorelov   +3 more
doaj   +1 more source

The parametrization of gas flows in discs in the Auriga simulations [PDF]

We study the radial motions of cold, star-forming gas in the secular evolution phase of a set of 14 magnetohydrodynamical cosmological zoom-in simulations of Milky Way-mass galaxies.
Okalidis, P, Grand, RJJ, Yates, RM, Kauffmann, G   +3 more
core   +1 more source

Radiative Cooling Changes the Dynamics of Magnetically Arrested Disks

The Astrophysical Journal Letters
We study magnetically arrested disks (MADs) around rotating black holes (BHs) under the influence of radiative cooling. We introduce a critical value of the mass accretion rate ${\dot{M}}_{{\rm{crit}}}$ for which the cooling by the synchrotron process ...
Akshay Singh, Damien Bégué, Asaf Pe’er   +2 more
doaj   +1 more source

Neutron star merger remnants. [PDF]

Gen Relativ Gravit, 2020
Bernuzzi S.
europepmc   +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

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, Krumholz MR, Di Teodoro EM.   +2 more
europepmc   +1 more source

Three-dimensional Magnetohydrodynamic Simulations of Periodic Variations of Ganymede’s Footprint

The Astrophysical Journal
Alfvénic power is generated through the interaction between the mini-magnetosphere of Ganymede and the corotating flow of the Jovian plasma, contributing to the formation of the Ganymede auroral footprint at Jupiter’s ionosphere.
Tao Yan, Binzheng Zhang, Junjie Chen, Zhiqi Zheng, Ziyi Yang, Shengyi Ye, Jun Cui   +6 more
doaj   +1 more source

Investigating Turbulence Effects on Magnetic Reconnection Rates Through High-Resolution Three-Dimensional Resistive Magnetohydrodynamical Simulations

We investigate the impact of turbulence on magnetic reconnection through high-resolution 3D MHD simulations, covering Lundquist numbers from $S=10^3$ to $10^6$.
Kowal, Grzegorz, Vicentin, Giovani H., Lazarian, Alex, Pino, Elisabete M. de Gouveia Dal   +3 more
core