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This study shows that large biases can occur if subgrid cell variability is ignored, where bias is defined as the difference between the average of fluxes computed at high resolution within a model cell and the flux computed with the average surface and cloud properties within the cell. The dependence of the downwelling shortwave and longwave radiation flux bias on cloud fraction, cloud optical depth and solar zenith angle (shortwave only) is described, and a method for correcting the bias that implicitly accounts for small-scale variability is presented. Results indicate that for low cloud amounts the shortwave flux is overestimated and the longwave flux is underestimated; high cloud amounts have the opposite effect. Cloud optical depth is also important in estimating the radiative fluxes in that the larger the cloud optical depth, the larger the flux biases. The biases are nearly scale-invariant, especially for the downwelling longwave flux. A simple regression approach to correcting the fluxes for errors that result from horizontal variability was found to reduce the average bias by up to 80%. The correction can be easily implemented in numerical models.