Results 101 to 110 of about 1,800,884 (153)
Simulations of cosmic ray propagation. [PDF]
Hanasz M, Strong AW, Girichidis P.
europepmc +1 more source
16 pages, Accepted in A&A 04/08/2006We present the first-ever simulations of non-ideal magnetohydrodynamical (MHD) stellar magnetospheric winds coupled with disc-driven jets where the resistive and viscous accretion disc is self-consistently described ...
C. Sauty +5 more
core +1 more source
The Interaction of a Supernova Remnant with Background Interstellar Turbulence
Supernova explosions are among the most energetic events in the Universe. After the explosion, the material ejected by the supernova expands throughout the interstellar medium (ISM), forming what is called a supernova remnant (SNR). The shocks associated
Giuseppe Prete +4 more
doaj +1 more source
Cosmic-Ray Acceleration of Galactic Outflows in Multiphase Gas
We investigate the dynamical interaction between cosmic rays (CRs) and the multiphase interstellar medium (ISM) using numerical magnetohydrodynamic (MHD) simulations with a two-moment CR solver and TIGRESS simulations of star-forming galactic disks.
Lucia Armillotta +3 more
doaj +1 more source
The Impact of Enhanced Extreme-ultraviolet Flux on the Upper Atmosphere of Earth-like Exoplanets
Identifying Earth-like planets outside our solar system is a leading research goal in astronomy, but determining if candidate planets have atmospheres, and more importantly if they can retain atmospheres, is still out of reach.
Lukas Hanson +3 more
doaj +1 more source
Odd Radio Circles Modeled by Shock-bubble Interactions
The physical nature and origins of the newly discovered class of Odd Radio Circles (ORCs) remain unclear. We investigate a model whereby ORCs are synchrotron-emitting vortex rings formed by the Richtmyer–Meshkov instability (RMI) when a shock interacts ...
Yiting Wang, Sebastian Heinz
doaj +1 more source
Effects of Dynamo-generated Large-scale Magnetic Fields on the Surface Gravity (f) Mode
By modeling the upper layers of the Sun in terms of a two-layer setup where a free surface exists within the computational domain, we numerically study the interaction between the surface gravity, or the fundamental ( f ) mode, and the magnetic fields ...
Rajesh Mondal, Nishant K. Singh
doaj +1 more source
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 +9 more
core +1 more source
Context.We present a detailed study of localised magnetohydrodynamical (MHD) instabilities occurring in two-dimensional magnetized accretion disks. Aims.We model axisymmetric MHD disk tori, and solve the equations governing a two-dimensional ...
Keppens, R. +5 more
core +1 more source

