From a0442ed58dee48a521ea053083ea967894507898 Mon Sep 17 00:00:00 2001 From: =?UTF-8?q?J=C3=B6rg=20Frings-F=C3=BCrst?= Date: Wed, 11 Jul 2018 22:19:56 +0200 Subject: New upstream version 2.0.1+repack --- doc/spec2cie.html | 24 ++++++++++++++++++++++++ 1 file changed, 24 insertions(+) (limited to 'doc/spec2cie.html') diff --git a/doc/spec2cie.html b/doc/spec2cie.html index d973289..4554531 100755 --- a/doc/spec2cie.html +++ b/doc/spec2cie.html @@ -22,6 +22,7 @@ + EMISINPUT (See the description of the .ti3 format. This would have to be done manually, as no ArgyllCMS tools generate such @@ -38,12 +39,14 @@ + output.[ti3|sp]
 -v                        + Verbose mode
 -A NN|AX|AG|XA|XG|GA|GX   XRGA conversion (default NN)
@@ -58,10 +61,12 @@ +                + Override actual instrument illuminant in .ti3 or .sp file:
                         @@ -70,6 +75,7 @@ +          (only used in conjunction with -f)
 -f [illum] @@ -77,23 +83,27 @@ + 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:
           @@ -110,10 +120,12 @@ +              +   Choose CIE Observer for spectral data:
              @@ -121,10 +133,12 @@ +          1931_2 (def.), 1964_10, 2012_2, + 2012_10, S&B 1955_2, shaw, J&V 1978_2 or file.cmf
 -n                        @@ -140,6 +154,7 @@ output + spectral values
 -p                        @@ -148,6 +163,7 @@ output + Plot each values spectrum
  input.[ti3|sp]            @@ -239,6 +255,7 @@ output + colprof -f for a fuller explanation.

The -i parameter allows specifying a @@ -281,6 +298,13 @@ output should generally be linked with other profiles that have the same illuminant and observer.

+ If a non D50 illuminant is used, then an extra set of L*a*b* output + fields will be created in the resulting CGATS file, containing + values relative to the illuminant white point. These will be + labelled XXXLAB_L etc, where XXX is the name of the illuminant. + These are informational only, and are not used by any ArgyllCMS + tools.
+
The -o flag allows specifying a tristimulus observer, and is used to compute PCS (Profile Connection Space) tristimulus values. The following choices are available:
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