DOI: 10.1016/S1387-6473(00)00010-5
关键词: Turbulence 、 Current (fluid) 、 Drop (liquid) 、 Magnetic field 、 Viscosity 、 Physics 、 Magnetohydrodynamic turbulence 、 Astrophysics 、 Observable 、 Astronomy 、 Accretion disc
摘要: Abstract We describe the α prescription of Shakura and Sunyaev discuss constraints placed on it by observable phenomena in time varying discs. explain why hydrodynamic turbulence alone cannot be source viscosity introduction a weak magnetic field changes this so that magnetohydrodynamic is effective. recent numerical simulations suggest MHD might drop to zero during dwarf-nova quiescence consider consequences for outbursts. speculate part played secondary star's own field.