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The Stokes profiles of Fe I lines in the photosphere of the Sun arecalculated within the Unno-Beckers-Landi-Dagl`Innocenti theory. Estimates ofthe magnetic strengthening of the lines were obtained. The changes in theStokes profiles depending on the excitation potential, wavelength, equivalentwidth, Lande factor, micro-macroturbulent velocities, radial velocity, dampingconstant, atmospheric model, magnetic field strength and direction areconsidered. The graphically presented variations of the Stokes profiles make itpossible to determine the initial values of the input parameters for solvingthe problems of magnetic field vector reconstruction by the inversion method.The presented dependencies of the magnetic strengthening on the line parameterswill help to correctly select magnetically sensitive lines for theinvestigation of sunspots, flux tubes, plages, and other magnetic features.

The influence of the medium physical conditions and atomic constants on the Stokes profiles of absorption lines in the solar spectrum