Atomic chemistry in turbulent astrophysical media. I. effect of atomic cooling

Physics & Astronomy

• astrophysics 100%
• chemistry 99%
• cooling 78%
• solar simulation 67%
• direct numerical simulation 38%
• Mach number 37%
• magnesium 36%
• sodium 34%
• grids 31%
• helium 30%
• turbulence 29%
• ionization 26%
• carbon 25%
• products 24%
• hydrogen 23%
• oxygen 23%
• estimates 22%
• simulation 14%
• temperature 11%

Earth & Environmental Sciences

• cooling 82%
• simulation 50%
• recombination 42%
• ionization 37%
• magnesium 33%
• hydrogen 29%
• turbulence 29%
• sodium 28%
• effect 27%
• oxygen 24%
• carbon 21%
• product 18%
• temperature 14%