Convert spectral .ti3 file, Version 1.8.3 Author: Gerhard Fuernkranz, licensed under the AGPL Version 3 Usage: spec2cie [options] input.ti3 output.ti3 -v Verbose mode -I illum Override actual instrument illuminant in .ti3 file: A, C, D50, D50M2, D65, F5, F8, F10 or file.sp (only used in conjunction with -f) -f [illum] Use Fluorescent Whitening Agent compensation [simulated inst. illum.: M0, M1, M2, A, C, D50 (def.), D50M2, D65, F5, F8, F10 or file.sp] -i illum Choose illuminant for computation of CIE XYZ from spectral data & FWA: A, C, D50 (def.), D50M2, D65, F5, F8, F10 or file.sp -o observ Choose CIE Observer for spectral data: 1931_2 (def), 1964_10, S&B 1955_2, shaw, J&V 1978_2 or file.cmf -n Don't output spectral values -p Plot each values spectrum input.ti3 Measurement file output.ti3 Converted measurement file

Convert spectral .ti3 file, Version 1.8.3 Author: Gerhard Fuernkranz, licensed under the AGPL Version 3 Usage: spec2cie [options] input.ti3 output.ti3 -v Verbose mode -I illum Override actual instrument illuminant in .ti3 file: A, C, D50, D50M2, D65, F5, F8, F10 or file.sp (only used in conjunction with -f) -f [illum] Use Fluorescent Whitening Agent compensation [simulated inst. illum.: M0, M1, M2, A, C, D50 (def.), D50M2, D65, F5, F8, F10 or file.sp] -i illum Choose illuminant for computation of CIE XYZ from spectral data & FWA: A, C, D50 (def.), D50M2, D65, F5, F8, F10 or file.sp -o observ Choose CIE Observer for spectral data: 1931_2 (def), 1964_10, S&B 1955_2, shaw, J&V 1978_2 or file.cmf -n Don't output spectral values -p Plot each values spectrum input.ti3 Measurement file output.ti3 Converted measurement file