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Spectral parameters consistent with UARS and EOS

More accurate forward model

Reduced effects due to noise, jitter, and spacecraft motion by averaging scan pairs

Use of all scans and samples. Original processing used only 1/6 of scans and 1/4 of samples (I.E. 1/24 of data)

Better Vertical resolution by using all scan samples with interleave approach

Bore sight alignment (twist) through data analysis

Aerosol effects accounted for using SAGE and HALOE results

Better H2O and NO2 results by matching temperature resolution

Rigorous evaluation of FOV effects