• CO5BOLD non-magnetic K8 V comparison model: Emergent continuum intensity (Salhab, Steiner, Steffen 2017)
  d3t40g45rsn01_526x526x176_int01B3_R_070-080.mpg

• CO5BOLD non-magnetic K8 V comparison model: "Line wing" intensity showing reversed granulation (Salhab, Steiner, Steffen 2017)
  d3t40g45rsn01_526x526x176_int03B3_R_070-080.mpg

• CO5BOLD magneto-convection in an K8 V dwarf atmosphere with <Bz>=50 G: Emergent continuum intensity (Salhab, Steiner, Steffen 2017)
  d3t40g5v50rsn01_526x526x176_int01B3_R_070-080.mpg

• CO5BOLD magneto-convection in an K8 V dwarf atmosphere with <Bz>=50 G: "Line wing" intensity showing reversed granulation (Salhab, Steiner, Steffen 2017)
  d3t40g45v50rsn01_526x526x176_int03B3_R_070-080.mpg

• CO5BOLD magneto-convection in an K8 V dwarf atmosphere with <Bz>=100 G: Emergent continuum intensity (Salhab, Steiner, Steffen 2017)
  d3t40g45v100rsn01_526x526x176_int01B3_R_070-080.mpg

• CO5BOLD magneto-convection in an K8 V dwarf atmosphere with <Bz>=100 G: "Line wing" intensity showing reversed granulation (Salhab, Steiner, Steffen 2017)
  d3t40g45v100rsn01_526x526x176_int03B3_R_070-080.mpg