Procedures were developed for extracting low resolution spectra while correcting for halation effects and scattered light within the instrument. To correct for halation, the spectra were extracted from the line-by-line images. Perpendicular scans of the image were fitted using an iterative least squares procedure with a known form function. The fitting function was a linear combination of a Gaussian with a Lorentz function. Correction for light scattered from the gratings employed a guess and test method. A priori choices of schematic spectral distributions were used to compute different sets of scattered light coefficients. Satisfactory results are shown for both methods.