Results 101 to 110 of about 45,937 (210)
Finding Local Parallel Electric Fields in Magnetotail Reconnection Using a Two‐Spacecraft Method
Abstract We investigate the use of a novel two‐spacecraft Liouville‐mapping method using data from the Magnetospheric Multiscale mission to determine local magnetic‐field‐aligned (parallel) electric fields in the Earth's magnetotail. The method detects the presence of local acceleration potentials by mapping phase‐space density between electron ...
J. D. White +4 more
wiley +1 more source
Relativistic Particle-In-Cell Simulation Studies of Prompt and Early Afterglows from GRBs
Nonthermal radiation observed from astrophysical systems containing relativistic jets and shocks e.g. gamma-ray bursts (GRBs) active galactic nuclei (AGNs) and microquasars commonly exhibit power-law emission spectra.
David Palmer +7 more
core +1 more source
Simulations of Relativistic Jets with Genesis [PDF]
6 pages, 2 figures, to appear in the proceedings of the conference "Godunov methods: theory and applications", Oxford, October ...
Aloy, Miguel A. +4 more
openaire +2 more sources
High--Resolution 3D Simulations of Relativistic Jets
We have performed high-resolution 3D simulations of relativistic jets with beam flow Lorentz factors up to 7, a spatial resolution of 8 cells per beam radius, and for up to 75 normalized time units to study the morphology and dynamics of 3D relativistic ...
E. Müller +8 more
core +1 more source
Relativistic Hydrodynamic Flows Using Spatial and Temporal Adaptive Structured Mesh Refinement
Astrophysical relativistic flow problems require high resolution three-dimensional numerical simulations. In this paper, we describe a new parallel three-dimensional code for simulations of special relativistic hydrodynamics (SRHD) using both spatially ...
Gingold R. A. +4 more
core +1 more source
Transverse stability of relativistic two-component jets
Context: Astrophysical jets from various sources seem to be stratified, with a fast inner jet and a slower outer jet. As it is likely that the launching mechanism for each component is different, their interface will develop differential rotation, while ...
Biretta +24 more
core +2 more sources
Synchrotron-limited Particle Acceleration in Relativistic Shearing Flows
Fermi-type shear particle acceleration is a promising mechanism for sustaining ultrarelativistic particles along the kiloparsec scale jets in active galactic nuclei.
Frank M. Rieger, Peter Duffy
doaj +1 more source
Parsec-scale Properties of Brightest Cluster Galaxies
We present new VLBI observations at 5 GHz of a complete sample of Brightest Cluster Galaxies (BCGs) in nearby Abell Clusters (distance class
Augusto +128 more
core +1 more source
POWERFUL RELATIVISTIC JETS IN SPIRAL GALAXIES [PDF]
The discovery of high-energy (E > 100 MeV) γ rays from Narrow-Line Seyfert 1 Galaxies (γ-NLS1s) has confirmed the presence of powerful relativistic jets in this class of active galactic nuclei (AGN). Although the jet emission is similar to that of blazars and radio galaxies, γ-NLS1s have some striking differences: relatively small masses (106-8 M⊙),
openaire +2 more sources
A Simulation Study of Low-power Relativistic Jets: Flow Dynamics and Radio Morphology of FR-I Jets
Radio galaxies are classified into two primary categories based on their morphology: center-brightened FR-I and edge-brightened FR-II. It is believed that the jet power and interactions with the ambient medium govern the deceleration and decollimation of
Ayan Bhattacharjee +3 more
doaj +1 more source

