In the present work, we evaluate the accuracy of the Solar Quiet Reference Field (SQRF) model for forecasting and predicting the geomagnetic solar quiet (Sq) daily field variation in the South America Magnetic Anomaly (SAMA) region. The model simulates the monthly average horizontal field of the geomagnetic quiet (Sq-H) daily variation solving a set of functional fitting equations for the specified geographic coordinates. We carried out two comparisons between the simulated and observational data of the Sq-H field. The first part attempts to evaluate the accuracy for predicting the Sq-H field over Medianeira (25.30°S, 54.11°W, dip angle: -33.45°) by using linear interpolation on the SQRF coefficients. The second part of the analysis attempts to evaluate the accuracy for forecasting the quiet daily field variation over Cachoeira Paulista (22.70°S, 45.01°W, dip angle: -38.48°). The results of the simulation for both locations show that this empirical model presents a good agreement with the Sq-H field obtained from the magnetic field data. The accuracy of the SQRF model (high correlation, r>0.9) provides a high potential for estimating and forecasting geomagnetic quiet daily field variation for space weather applications. Therefore, this model could be useful in the Sq-H field regions near of SAMA.