From c0b89ac5bfb90835ef01573267020e42d4fe070c Mon Sep 17 00:00:00 2001 From: =?UTF-8?q?J=C3=B6rg=20Frings-F=C3=BCrst?= Date: Sun, 23 Aug 2015 12:17:05 +0200 Subject: Imported Upstream version 1.8.0 --- doc/spec2cie.html | 14 +++++++++++++- 1 file changed, 13 insertions(+), 1 deletion(-) mode change 100644 => 100755 doc/spec2cie.html (limited to 'doc/spec2cie.html') diff --git a/doc/spec2cie.html b/doc/spec2cie.html old mode 100644 new mode 100755 index d25b0a0..7911948 --- a/doc/spec2cie.html +++ b/doc/spec2cie.html @@ -16,6 +16,7 @@ spec2cie [options] input.ti3 + output.ti3
 
-v            @@ -23,6 +24,7 @@  -I illum   +    Override actual instrument illuminant in .ti3 file:
           @@ -31,6 +33,7 @@                 + (only used in conjunction with -f)
   -o observ  +    Choose CIE Observer for spectral data:
                 + 1931_2
(def.), - 1964_10, S&B 1955_2, shaw, J&V 1978_2
+ 1964_10, S&B 1955_2, shaw, J&V 1978_2 or file.cmf
 -n             Don't output + spectral values
 -p             @@ -73,10 +80,12 @@ output Measurement + file
 output.ti3     + Converted measurement file

Comments

This program takes the (usually reflective) spectral data in a .ti3 @@ -129,6 +138,7 @@ Measurement computation illuminant used for FWA (see -i below). See + colprof -f for a fuller explanation.

The -i parameter allows specifying a @@ -185,6 +195,8 @@ Measurement   shaw selects the Shaw and Fairchild 1997 2 degree observer

+ or a .cmf file can be provided as an argument.
+
Note that if an observer other than 1931 2 degree is chosen, the resulting ICC profile will not be standard, and cannot be freely interchanged with other profiles that that us the standard 1931 2 -- cgit v1.2.3