Upper panel: figure adopted from Coriat et al. (2011, Fig. 5): “standard” correlation between radio and X-ray luminosity , defined by the black hole binaries GX 339-4 and V404 Cyg (dashed lines indicate dispersion) and data for H1743-322, typical of the so-called outliers on the lower track. Red line: fit to the high luminosity data of H1743-322; data for the outburst 2008a marked by horizontal slashes. Lower panel: “standard” correlation between radio and X-ray luminosity and fit to the data for H1743-322 as in upper panel; blue lines: X-ray luminosity including additional luminosity caused by the photons of an underlying disk, ΔL_X/L_Edd = 0.0025, 0.005 and 0.01); horizontal lines: the increase required for the red line fit to the data of H1743-322.