A view of the solar granulation at 200 nm
Results of a 3D radiation hydrodynamics simulation of solar surface convection
M.Steffen, Astrophysikalisches Institut Potsdam & S. Wedemeyer, Institut für Theoretische Physik und Astrophysik, Universität Kiel

chro3D06fw_2000_00b chro3D06fw_2000_0_56b chro3D06fw_2000_0_76b chro3D06fw_2000_0_88b
Quiet solar granulation at 200.0 nm, assuming pure continuum opacities Quiet solar granulation at 200.0 nm, assuming a line haze due to FeI (0 ev) depressing the true continuum by 56% Quiet solar granulation at 200.0 nm, assuming a line haze due to FeI (0 ev) depressing the true continuum by 76% Quiet solar granulation at 200.0 nm, assuming a line haze due to FeI (0 ev) depressing the true continuum by 88%
chro3D06fw_4445_00r chro3D06fw_2000_5_48b chro3D06fw_2000_5_68b chro3D06fw_2000_5_83b
Quiet solar granulation at 444.5 nm, assuming pure continuum opacities Quiet solar granulation at 200.0 nm, assuming a line haze due to FeI (5 ev) depressing the true continuum by 48% Quiet solar granulation at 200.0 nm, assuming a line haze due to FeI (5 ev) depressing the true continuum by 68% Quiet solar granulation at 200.0 nm, assuming a line haze due to FeI (5 ev) depressing the true continuum by 83%
Alternative color table Model chro3D06fw: non-grey radiative transfer, chromosphere Back to main page