The formation and structure of a strongly magnetized corona above a weakly magnetized accretion disk

Physics & Astronomy

• accretion disks 93%
• coronas 89%
• scale height 59%
• orbitals 9%
• buoyancy 6%
• approximation 6%
• Mach number 6%
• escape 6%
• neutron stars 6%
• energy 5%
• dissipation 5%
• shock 4%
• simulation 4%
• turbulence 4%
• saturation 4%
• cooling 4%
• heating 4%
• estimates 3%
• curves 3%
• magnetic fields 3%
• temperature 1%

Earth & Environmental Sciences

• corona 100%
• accretion 84%
• toroidal field 18%
• energy 16%
• amplification 10%
• buoyancy 10%
• dissipation 10%
• outflow 10%
• magnetic field 9%
• simulation 9%
• turbulence 8%
• timescale 8%
• saturation 8%
• cooling 8%
• heating 8%
• temperature 4%
• rate 3%