[en] In the 3200-5600 A region the limb-darkening coefficients of the solar disk in the integral spectrum (i.e. in the continuum with all the absorption lines) have been calculated. In the calculations, the continuum limb-darkening coefficients and the estimates for the behaviour of lines of different intensity categories in the transition from the centre of the disk to the limb have been used. The complete sums of equivalent widths of all the lines in centre and at the limb, and separate ones for strong (the equivalent width is more than 250 m A) lines are given. The limb-darkening coefficients have been tabulated. Their root-mean-square error is estimated to be about 3-5 per cent