Simulation results for the coronal structure of HD 22049 driven by the ZDI large-scale magnetic field map. 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 equatorial plane (z = 0) is presented. The sphere represents the stellar surface and selected 3D magnetic field lines are shown in white. 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 and colour scales are preserved in all panels, with an inclination angle of i = 45°.