• CO5BOLD non-magnetic K2 V comparison model: Emergent continuum intensity (Salhab, Steiner, Steffen 2017)
  d3t50g45rsn01_448x448x276_int01B3_R_030-040.mpg

• CO5BOLD non-magnetic K2 V comparison model: "Line wing" intensity showing reversed granulation (Salhab, Steiner, Steffen 2017)
  d3t50g45rsn01_448x448x276_int03B3_R_030-040.mpg

• CO5BOLD magneto-convection in an K2 V dwarf atmosphere with <Bz>=50 G: Emergent continuum intensity (Salhab, Steiner, Steffen 2017)
  d3t50g45v50rsn01_448x448x276_int01B3_R_060-070.mpg

• CO5BOLD magneto-convection in an K2 V dwarf atmosphere with <Bz>=50 G: "Line wing" intensity showing reversed granulation ( Salhab, Steiner, Steffen 2017)
  d3t50g45v50rsn01_448x448x276_int03B3_R_060-070.mpg

• CO5BOLD magneto-convection in an K2 V dwarf atmosphere with <Bz>=100 G: Emergent continuum intensity (Salhab, Steiner, Steffen 2017)
  d3t50g45v100rsn01_448x448x276_int01B3_R_070-080.mpg

• CO5BOLD magneto-convection in an K2 V dwarf atmosphere with <Bz>=100 G: "Line wing" intensity showing reversed granulation (Salhab, Steiner, Steffen 2017)
  d3t50g45v100rsn01_448x448x276_int03B3_R_070-080.mpg

• CO5BOLD magneto-convection in an K2 V dwarf atmosphere with <Bz>=100 G: Magnetic field strength |B| in vertical slice (Salhab, Steiner, Steffen 2017)
  d3t50g45v100rsn01_448x448x276_bfield_070-080.mpg