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authorJörg Frings-Fürst <debian@jff-webhosting.net>2018-07-11 22:20:14 +0200
committerJörg Frings-Fürst <debian@jff-webhosting.net>2018-07-11 22:20:14 +0200
commit7beb00cd8d28c3d5893ce3db907a828d64afdea9 (patch)
tree395a3dee2fe197b8284dee02c5f527889df78413 /doc/spec2cie.html
parente2d30e0583c047a4bedf4c8d0c86320f1b3fd8ed (diff)
parenta0442ed58dee48a521ea053083ea967894507898 (diff)
Update upstream source from tag 'upstream/2.0.1+repack'
Update to upstream version '2.0.1+repack' with Debian dir 6edb5dd2df9aca152662fc4a8f72bd6d86f8552e
Diffstat (limited to 'doc/spec2cie.html')
-rwxr-xr-xdoc/spec2cie.html24
1 files changed, 24 insertions, 0 deletions
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 @@
+
<span style="font-weight: bold;">EMISINPUT</span> (See the <a
href="ti3_format.html">description of the .ti3 format</a>. This
would have to be done manually, as no ArgyllCMS tools generate such
@@ -38,12 +39,14 @@
+
output.[ti3|sp]<br>
&nbsp;</span></small></tt><tt><small>-v
&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
+
Verbose mode<br>
&nbsp;<a href="A">-A NN|AX|AG|XA|XG|GA|GX</a>&nbsp;&nbsp; XRGA
conversion (default NN)<br>
@@ -58,10 +61,12 @@
+
&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
+
Override actual instrument illuminant in .ti3 or .sp file:<br>
&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
&nbsp; &nbsp;&nbsp;&nbsp;&nbsp;&nbsp; &nbsp; &nbsp; &nbsp;
@@ -70,6 +75,7 @@
+
&nbsp; &nbsp; &nbsp; &nbsp;&nbsp; (only used in conjunction
with <span style="font-weight: bold;">-f</span>)<br>
</small></small></tt><tt><small><small>&nbsp;<a href="#f">-f [<i>illum</i>]</a>
@@ -77,23 +83,27 @@
+
Use Fluorescent Whitening Agent compensation [simulated inst.
illum.:<br>
&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
+
&nbsp; &nbsp; &nbsp; &nbsp; M0, M1, M2, A, C, D50 (def.),
D50M2, D65, F5, F8, F10 or file.sp]<br>
</small></small></tt><tt><small><small><small>&nbsp;<a href="#i">-i
+
<i>illum</i></a>&nbsp;&nbsp;
&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
+
Choose illuminant for computation of CIE XYZ from spectral
data &amp; FWA:<br>
&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
@@ -110,10 +120,12 @@
+
&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
+
&nbsp; Choose CIE Observer for spectral data:<br>
&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
&nbsp;
@@ -121,10 +133,12 @@
+
&nbsp; &nbsp; &nbsp; &nbsp;&nbsp; 1931_2 </small></tt><tt><small>
(def.)</small></tt><tt><small>, 1964_10, </small></tt><tt><small><tt><small>2012_2,
+
2012_10, </small></tt>S&amp;B 1955_2, shaw, J&amp;V 1978_2
or file.cmf<br>
&nbsp;<a href="#p">-n</a>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
@@ -140,6 +154,7 @@ output
+
spectral values<br>
</small></tt><tt><small>&nbsp;<a href="#p">-p</a>
&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
@@ -148,6 +163,7 @@ output
+
Plot each values spectrum</small></tt><tt><br>
</tt><tt> </tt><tt><small>&nbsp;<span style="font-style: italic;">input.[ti3|sp]</span>
&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
@@ -239,6 +255,7 @@ output
+
<a href="colprof.html#f">colprof -f</a> for a fuller explanation. <br>
<br>
<a name="i"></a>The <b>-i</b> parameter allows specifying a
@@ -281,6 +298,13 @@ output
should generally be linked with other profiles that have the same
illuminant and observer.<br>
<br>
+ 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.<br>
+ <br>
<a name="o"></a> The <b>-o</b> flag allows specifying a tristimulus
observer, and is used to compute PCS (Profile Connection Space)
tristimulus values. The following choices are available:<br>