(Solved): Extra Credit 1 ( 2 points): Write your own matlab code that normalizes your spectra (that is, calcu ...
Extra Credit 1 ( 2 points): Write your own matlab code that normalizes your spectra (that is, calculates relative changes in intensity based on a reference as the spectrometer software does). To do this, you need to determine the usable non-zero spectra of the lamp. See below for example script (some? need to be filled in) 888888888888889888888888888887 8 Example matlab script HReference Intensity is so theference wavelength is LO. sone test spectra is s tone test wavelength is L. 10LL30 the data is redundant, dim=size (S0,?); 8 number of spectrometer points Bchreshold value below there isn't enough light thresh =?; start_i=sum (SO (:, int (dim/2)0?=10(, start_i:fin_i); struncated relevant wavelengths St0 = SO (, , start_i:fin_i); \$truncated relevant spectras St=S(:,start_i:fin_i); ftruncated test spectra plot (Lt0, St0./St) 888888888888888888888888838888