The efficiency of second-order fermi acceleration by weakly compressible magnetohydrodynamic turbulence

Physics & Astronomy

• magnetohydrodynamic turbulence 100%
• solar wind 48%
• pitch (inclination) 42%
• scattering 37%
• distribution functions 28%
• heating 22%
• turbulence 18%
• cooling 16%
• protons 15%
• particle acceleration 14%
• plasma waves 13%
• encounters 12%
• mean free path 12%
• field strength 10%
• tuning 9%
• expansion 7%
• estimates 7%
• magnetic fields 5%

Earth & Environmental Sciences

• magnetohydrodynamics 94%
• turbulence 55%
• scattering 49%
• solar wind 41%
• particle 35%
• power law 29%
• heating 22%
• plasma 16%
• timescale 14%
• cooling 14%
• distribution 11%
• parameter 10%
• rate 10%
• magnetic field 9%