Disk–jets connection during the 2006 and 2009–10 outbursts. The top panel compares their B-LCs shifted to their maxima (vertical bar). The second panel shows evolution of average fluxes of jets, ﹩{F}_{\mathrm{jets}}=({F}_{{{\rm{S}}}^{+}}+{F}_{{{\rm{S}}}^{-}})/2﹩ (data from Tomov et al. 2007; Skopal et al. 2009, and our Table 2). The third panel plots the evolution of the effective radius, ﹩{R}_{\mathrm{WD}}^{\mathrm{eff}}﹩, of the warm pseudophotosphere, and the bottom panel displays radial velocities of the absorption component in the Hα profile (crosses are values corrected for the orbital motion of the hot component according to elements of Fekel et al. 2000).