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Commands can be entered as a script in the same way that they would be entered into the Command Window. m extension, then the commands can be executed by simply typing the name of the script. m can be executed by typing test in the Command Window. For some scripts it can be useful to place the command clear as the first line in the script so that MATLAB script is started from a clean environment. Of course, it is important to be careful to avoid using names for M-files that clash with any of MATLAB’s built-in functions or M-file functions.
11), x ¼ Wx ðlÞ=½Wy ðlÞ þ Wy ðlÞ þ Wz ðlÞ, y ¼ Wy ðlÞ=½Wx ðlÞ þ Wy ðlÞ þ Wz ðlÞ. 11) can be replaced by the colour-matching functions and in this case the chromaticity coordinates are computed for the appropriate observer and for the equal-energy illuminant (illuminant E). 11) and the tables of weights at 10-nm intervals. In order to generate a smooth spectral locus 5-nm intervals or less are required. 8)] to a reflectance vector. 083; n = length(P); for i=2:n-1 cP(i) = -a*P(i-1) + (1 + 2*a)*P(i) - a*P(i+1); end cP(1) = (1 + a)*P(1) - a*P(2); cP(n) = (1 + a)*P(n) - a*P(n-1); The format for this function is [cp] = cband(p) where p is an n61 or 16n matrix.
The default option is a linear interpolation in which the y points are simply connected by straight lines. This works surprisingly well for many reflectance curves given that the sampling interval is 20 nm or less. Other options include ‘cubic’ and ‘spline’. The cubic fit performs cubic interpolation piecemeal in the way stipulated by the CIE. 2. , 2000) at 10nm intervals were sub-sampled to generate data at 20-nm intervals. 1487) 10-nm intervals. The original and interpolated spectra were compared and rootmean-square (rms) errors computed for each sample.