output = SPDToLinSPD(input,B)

Find the best fitting spectrum within a linear model.

output - spectrum within the linear model
(n-wavelengths by number-of-lights)
input - source spectral power distribution
(n-wavelengths by number-of-lights)
B - linear model for spectral power distributions
(number-of-wavelengths by n-dimension)

30/11/07 Change call to non-existent SPDToLinWgts.m into call to
FindModelWeights.m, as suggested by Mickey Rowe. (MK)

Path   Retrieve current version from GitHub | View changelog