• CO5BOLD non-magnetic F5 V comparison model: Emergent continuum intensity (Salhab, Steiner, Steffen 2017)
  d3t65g45rsn01_466x466x268int01B3_R_070-080.mpg

• CO5BOLD non-magnetic F5 V comparison model: Line wing intensity showing reversed granulation (Salhab, Steiner, Steffen 2017)
  d3t65g45rsn01_466x466x268int03B3_R_070-080.mpg

• CO5BOLD magneto-convection in an F5 V dwarf atmosphere with <Bz>=50 G: Emergent continuum intensity (Salhab, Steiner, Steffen 2017)
  d3t65g45v50rsn01_466x466x268int01B3_R_070-080.mpg

• CO5BOLD magneto-convection in an F5 V dwarf atmosphere with <Bz>=50 G: Line wing intensity showing reversed granulation (Salhab, Steiner, Steffen 2017)
  d3t65g45v50rsn01_466x466x268int03B3_R_070-080.mpg

• CO5BOLD magneto-convection in an F5 V dwarf atmosphere with <Bz>=50 G: Magnetic field strength |B| in vertical slice (Salhab, Steiner, Steffen 2017)
  d3t65g45v50rsn01_466x466x268_bfield_070-080_blue.mpg

• CO5BOLD magneto-convection in an F5 V dwarf atmosphere with <Bz>=100 G: Emergent continuum intensity (Salhab, Steiner, Steffen 2017)
  d3t65g45v100rsn01_466x466x268int01B3_R_059-068.mpg

• CO5BOLD magneto-convection in an F5 V dwarf atmosphere with <Bz>=100 G: Line wing intensity showing reversed granulation (Salhab, Steiner, Steffen 2017)
  d3t65g45v100rsn01_466x466x268int03B3_R_059-068.mpg

• CO5BOLD magneto-convection in an F5 V dwarf atmosphere with <Bz>=100 G: Magnetic field strength |B| in vertical slice (Salhab, Steiner, Steffen 2017)
  d3t65g45v100rsn01_466x466x268_bfield_059-068_blue.mpg