Magnetohydrodynamics in Astrophysics
Magnetohydrodynamics (MHD) is the simplest but sufficient approximation to describe many large-scale low-frequency phenomena in astrophysical plasma: regular and turbulent dynamo, plasma motions driven by strong magnetic fields, accreation disks, and relativistic jets.
KeywordsBlack Hole Accretion Disk White Dwarf Active Galactic Nucleus Secondary Star
Unable to display preview. Download preview PDF.