Comparison of the location of the coronal holes for the PFSS (top left panel), WP (top right panel), and WP-AW model (bottom left panel) with EUV observations by SDO/AIA 193 (background). We show the comparison with EUV data from Carrington Rotation 2240. Just for the WP-AW model, we also show the comparison with Carrington rotation 2241 (bottom right panel). Results extracted from observations are shown with white contours, while results obtained from numerical simulations are shown in color. The coronal holes corresponding to the simulation performed using the magnetic map from February 15 without the AR are shown in blue, while the ones using the magnetic map from February 22 with the AR are shown in yellow. We also indicate the longitude corresponding to the AR on the far-side with a red line, and the longitude corresponding to the central meridian as seen from the Earth with a green line.