A method for the determination of the systematic errors of Harrick's formulas is proposed. The method is based on the expansion of the expressions for the optical density into a Maclaurin series in terms of the extinction coefficient of the medium under study. Using numerical calculations, it is shown that, under conditions of weak absorption, it is sufficient to consider only the first two terms of this series, with the relative systematic errors of Harrick's formulas being determined in this case by dividing the first term of the series by the second. The behavior of the relative systematic errors for perpendicular and parallel polarizations is compared. These errors are shown to decrease monotonically with an increase in the angle of incidence and have finite limits both for angles of incidence tending to the critical value and at grazing incidence of probe radiation.