MAIHEM is built with FLASH (version 4.4) and tracks ionizations, recombinations, and species by species radiative cooling for hydrogen, helium, carbon, nitrogen, oxygen, neon, sulfur, calcium, and iron. For more information on MAIHEM, see Turbulent Astrophysical Media I and Turbulent Astrophysical Media II.
Works in the Arizona State University School of Earth and Space Exploration and worked on developing MAIHEM.
Currently an Astrophysicist at the University of Michigan and worked on developing MAIHEM.
A graduate student attending Arizona State University and is using MAIHEM to understand the role of turbulence in elemental abundances.
Evan Scannapieco: email@example.com
William Gray: firstname.lastname@example.org
Edward Buie II: email@example.com