Simulation results for the coronal structure of the Sun during activity minimum (CR 1922). The upper panels contain the distribution of the magnetic energy density (ε_{B r}, left), the number density (n, middle) and temperature (T, right). For the last two quantities, the distribution over the plane y = 0 is presented. The sphere represents the stellar surface and selected 3D magnetic field lines are shown in white. Note the change of scale for ε_{B r} in this case. The lower images correspond to synthetic coronal emission maps in EUV (blue/171 Å, green/195 Å, and yellow/284 Å) and SXR (red/2−30 Å). The perspective is preserved in all panels, with an inclination angle of i = 90 °.