.\" DO NOT MODIFY THIS FILE!  It was generated by help2man 1.43.3.
.TH CONVERT "1" "August 2013" "Convert spectral .ti3 file, Version 1.5.1" "User Commands"
.SH NAME
Convert \- Convert spectral .ti3 file.
.SH SYNOPSIS
.B spec2cie
[\fIoptions\fR] \fIinput.ti3 output.ti3\fR
.SH DESCRIPTION
Convert spectral .ti3 file, Version 1.5.1
Author: Gerhard Fuernkranz, licensed under the AGPL Version 3
.TP
\fB\-v\fR
Verbose mode
.TP
\fB\-I\fR illum
Override actual instrument illuminant in .ti3 file:
.IP
A, C, D50, D50M2, D65, F5, F8, F10 or file.sp
(only used in conjunction with \fB\-f\fR)
.TP
\fB\-f\fR [illum]
Use Fluorescent Whitening Agent compensation [simulated inst. illum.:
.IP
M0, M1, M2, A, C, D50 (def.), D50M2, D65, F5, F8, F10 or file.sp]
.TP
\fB\-i\fR illum
Choose illuminant for computation of CIE XYZ from spectral data & FWA:
A, C, D50 (def.), D50M2, D65, F5, F8, F10 or file.sp
.TP
\fB\-o\fR observ
Choose CIE Observer for spectral data:
.IP
1931_2 (def), 1964_10, S&B 1955_2, shaw, J&V 1978_2
.TP
\fB\-n\fR
Don't output spectral values
.TP
\fB\-p\fR
Plot each values spectrum
.TP
input.ti3
Measurement file
.TP
output.ti3
Converted measurement file
.PP
Author: Gerhard Fuernkranz, licensed under the AGPL Version 3
.PP
Usage: spec2cie [options] input.ti3 output.ti3
.TP
\fB\-v\fR
Verbose mode
.TP
\fB\-I\fR illum
Override actual instrument illuminant in .ti3 file:
.IP
A, C, D50, D50M2, D65, F5, F8, F10 or file.sp
(only used in conjunction with \fB\-f\fR)
.TP
\fB\-f\fR [illum]
Use Fluorescent Whitening Agent compensation [simulated inst. illum.:
.IP
M0, M1, M2, A, C, D50 (def.), D50M2, D65, F5, F8, F10 or file.sp]
.TP
\fB\-i\fR illum
Choose illuminant for computation of CIE XYZ from spectral data & FWA:
A, C, D50 (def.), D50M2, D65, F5, F8, F10 or file.sp
.TP
\fB\-o\fR observ
Choose CIE Observer for spectral data:
.IP
1931_2 (def), 1964_10, S&B 1955_2, shaw, J&V 1978_2
.TP
\fB\-n\fR
Don't output spectral values
.TP
\fB\-p\fR
Plot each values spectrum
.TP
input.ti3
Measurement file
.TP
output.ti3
Converted measurement file