Results 141 to 150 of about 4,916 (215)

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

Three‐dimensional Magnetohydrodynamic Simulations of an Accretion Disk with Star‐Disk Boundary Layer [PDF]

, 2002
Adriane Steinacker, J. C. B. Papaloizou
openalex   +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

OpenMP Parallelism for Multi-dimensional Grid-Adaptive Magnetohydrodynamic Simulations [PDF]

, 2002
Rony Keppens, Gábor Tóth
openalex   +1 more source

Forming Prominences Accounting for Partial Ionization Effects

The Astrophysical Journal
One of the most striking structures in the solar atmosphere are prominences, predominantly coronal structures, with thermodynamic conditions that vary from chromospheric internally to the corona that surrounds them.
V. Jerčić, B. Popescu Braileanu, R. Keppens   +2 more
doaj   +1 more source

Magnetic Flux Plays an Important Role during a Black Hole X-Ray Binary Outburst in Radiative Two-temperature General Relativistic Magnetohydrodynamic Simulations

The Astrophysical Journal
Black hole (Bh) X-ray binaries cycle through different spectral states of accretion over the course of months to years. Although persistent changes in the Bh mass accretion rate are generally recognized as the most important component of state ...
M. T. P. Liska, N. Kaaz, K. Chatterjee, Razieh Emami, G. Musoke   +4 more
doaj   +1 more source

Photoelectric Heating and [Cii] Cooling in Translucent Clouds: Results for Cloud Models Based on Simulations of Compressible Magnetohydrodynamic Turbulence [PDF]

, 2003
M. Juvela, Paolo Padoan, Raúl Jiménez
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

Three‐dimensional Magnetohydrodynamic Simulations of Radiatively Inefficient Accretion Flows [PDF]

, 2003
I. V. Igumenshchev, Ramesh Narayan, M. A. Abramowicz   +2 more
openalex   +1 more source

Neutron star merger remnants. [PDF]

Gen Relativ Gravit, 2020
Bernuzzi S.
europepmc   +1 more source