Numerical Simulations of Magnetized Astrophysical Jets and Comparison with Laboratory Laser Experiments

Abstract

The results of MHD numerical simulations of the formation and development of magnetized jets are presented. Similarity criteria for comparisons of the results of laboratory laser experiments and numerical simulations of astrophysical jets are discussed. The results of laboratory simulations of jets generated in experiments at the Neodim laser installation are presented.

arXiv comment21 pages, 19 figures, published in Astronomy reports 62, 162-188, 2018

References in corpus (8)

• A High Resolution X-ray Image of the Jet in M 87
• Chandra X-ray Imaging and Spectroscopy of the M87 Jet and Nucleus
• Structure of the X-ray Emission from the Jet of 3C 273
• Similarity Properties and Scaling Laws of Radiation Hydrodynamic Flows in Laboratory Astrophysics
• Propagation of Magnetized Neutron Stars Through the Interstellar Medium
• Spherical Bondi accretion onto a magnetic dipole
• Bondi-Hoyle Accretion onto Magnetized Neutron Star
• Creation of Magnetized Jet Using a Ring of Laser Beams

Cited by in corpus (3)

• Laboratory modeling of jets from young stars using plasma focus facilities
• Internal Structure of the Jets from Young Stars Simulated at Plasma Focus Facilities
• The collimated propagation causes of astrophysical and laboratory jets