Provided by: argyll_1.5.1-5ubuntu1_amd64 
NAME
Convert - Convert spectral .ti3 file.
SYNOPSIS
spec2cie [options] input.ti3 output.ti3
DESCRIPTION
Convert spectral .ti3 file, Version 1.5.1 Author: Gerhard Fuernkranz, licensed under the
AGPL Version 3
-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
-n Don't output spectral values
-p Plot each values spectrum
input.ti3
Measurement file
output.ti3
Converted measurement file
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
-n Don't output spectral values
-p Plot each values spectrum
input.ti3
Measurement file
output.ti3
Converted measurement file