Particle acceleration and magnetic field amplification by relativistic shocks in inhomogeneous media
K Morikawa, Y Ohira, T Ohmura - The Astrophysical Journal …, 2024 - iopscience.iop.org
Particle acceleration and magnetic field amplification in relativistic shocks propagating in
inhomogeneous media are investigated by three-dimensional magnetohydrodynamical …
inhomogeneous media are investigated by three-dimensional magnetohydrodynamical …
Shock-Turbulence Interactions in Star Formation
MM Foley - 2024 - dash.harvard.edu
Multiscale processes in the interstellar medium (ISM) can be modeled as shocks
encountering turbulent gas. Much of the gas in the ISM is characterized by supersonic …
encountering turbulent gas. Much of the gas in the ISM is characterized by supersonic …