From f6b8e0eae4374f339487a33e3e4fe5462d5816e1 Mon Sep 17 00:00:00 2001 From: =?UTF-8?q?J=C3=B6rg=20Frings-F=C3=BCrst?= Date: Sat, 25 Nov 2017 10:16:00 +0100 Subject: New upstream version 2.0.0 --- doc/mpplu.html | 382 ++++++++++++++++++++++++++++++--------------------------- 1 file changed, 203 insertions(+), 179 deletions(-) mode change 100644 => 100755 doc/mpplu.html (limited to 'doc/mpplu.html') diff --git a/doc/mpplu.html b/doc/mpplu.html old mode 100644 new mode 100755 index 8d4e755..68f985b --- a/doc/mpplu.html +++ b/doc/mpplu.html @@ -1,182 +1,206 @@ - - mpplu - - - - -

xicc/mpplu

-

Summary

-Lookup individual color values though an MPP profile. Also -create MPP gamut files or X3DOM -views.
-

Usage

-mpplu [-v level] [-f func] -[-i intent] [-o order] profile.mpp
--v             -Verbose
--f function    f = forward, b = -backwards
--p oride       x -= XYZ_PCS, l = -Lab_PCS, y = Yxy, s = spectral,
--l limit       override -default -ink limit, 1 - N00%
--i illum       Choose -illuminant for -print/transparency spectral data:
-            -     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
--u         -    Use Fluorescent Whitening Agent compensation
--g         -    Create gamut output
--w         -    Create gamut X3DOM as well
--n             -Don't add X3DOM axes
--a n           Gamut -transparency level
--d -n           Gamut -surface detail level
--t num     -    Invoke debugging test code -"num" 1..n
-            -     1 - check partial derivative for device -input
-            -     2 - create overlap diagnostic X3DOM gamut -surface
-profile.mpp   Profile to be -used
-
-    The colors to -be translated should be fed into -standard input,
-    one input -color per line, white space separated.
-    A line -starting with a # will be ignored.
-    A line not -starting with a number will terminate the -program. -
-

Usage Details and Discussion

-This is an analogous tool to icclu , but -applying -to MPP profile, rather than ICC profiles. Because MPP profiles -can also contain a spectral description of device behavior, there are -extra options in mpplu to describe how to convert spectral values into -CIE tristimulus values.
-Some additional functionality is included in mpplu, analogous to iccgamut, allowing gamut files and images to -be generated from MPP profiles.
-
-The -v flag causes extra information about the profile to be -printed.
-
-The -f flag is experimental, and should be ignored.
-
-Normally L*a*b* is displayed, but this can be changed using the the -p -flag and XYZ, Yxy, or spectral values to be be displayed.
-
-If an illuminant, observer or Fluorescent Whitening Agent compensation -is selected, then the CIE tristimulus values will be computed from the -spectral information in the MPP profile (if present).
-
-The -l flag overrides any default ink limit (Total Area -Coverage) recorded in the profile. The ink limit has an effect on the -results of a gamut -generated from the profile.
-
-The -i flag allows specifying a standard or custom illumination -spectrum, applied to reflective spectral profile data to compute CIE -tristimulus -values. A, D50, D65, F5, F8, F10 -are a selection of standard illuminant spectrums, with D50 -being the -default. If a filename is specified instead, it will be assumed to be -an -Argyll specific .sp spectrum file.
-
- The -o flag allows specifying a tristimulus -observer, and is used to compute PCS (Profile Connection Space) -tristimulus values. The following choices are available:
-  1931_2 selects the standard CIE 1931 2 degree observer. -The default.
-  1964_10 selects the standard CIE 1964 10 degree observer.
-  1955_2 selects the Stiles and Birch 1955 2 degree -observer
-  1978_2 selects the Judd and Voss 1978 2 degree observer
-  shaw selects the Shaw and Fairchild 1997 2 degree -observer
-
-The -u flag enables Fluorescent Whitening Agent compensation, -which compensates for the effect a different illuminant will have, on -any Fluorescent Whitening Agent present in the reflective media.
-
-The -g flag causes mpplu to simply generate a gamut surface -description from the profile, creating a .gam file with the same base name as -the given profile.
-
-The -w flag causes the gamut surface to be generated in X3DOM format -as well as .gam format.
-
-The -n flag suppresses the X3DOM axes.
-
-The -a n parameter sets a transparency -level in the X3DOM surface.
-
-The -d parameter controls the level of detail displayed in the -gamut surface. The parameter roughly corresponds to a deltaE value, so -smaller values give greater detail. The default value is around 10, and -is a good place to start. Small values may take a lot of time to -generate, and will produce big files.
-
-The -t parameter invokes special MPP test and diagnostic output.
-
-
-
-
- + + mpplu + + + + +

xicc/mpplu

+

Summary

+ Lookup individual color values though an MPP profile. Also create MPP + gamut files or X3DOM + views.
+

Usage

+ mpplu [-v level] [-f + func] [-i intent] [-o order] profile.mpp
+ -v             + + Verbose
+ -f function    f = forward, + b = backwards
+ -p oride       + + x = XYZ_PCS, l = Lab_PCS, y = Yxy, s = spectral,
+ -l limit       + override default ink limit, 1 - N00%
+ -i illum       + Choose illuminant for print/transparency spectral data:
+             +  + +    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, 2012_2, 2012_10, S&B +1955_2, + + shaw, J&V 1978_2 or file.cmf
+ -u         +  + +   Use Fluorescent Whitening Agent compensation
+ -g         +  + +   Create gamut output
+ -w         +  + +   Create gamut X3DOM as well
+ -n             +Don't + + add X3DOM axes
+ -a n           + Gamut transparency level
+ -d + n           Gamut + surface detail level
+ -t + num         Invoke debugging test + code "num" 1..n
+             +  + +    1 - check partial derivative for device input
+             +  + +    2 - create overlap diagnostic X3DOM gamut surface
+ profile.mpp   Profile + to be used
+
+     The + colors to be translated should be fed into standard input,
+     one input + color per line, white space separated.
+     A line + starting with a # will be ignored.
+     A line + not starting with a number will terminate the program. +
+

Usage Details and Discussion

+ This is an analogous tool to icclu , but + applying to MPP profile, rather + than ICC profiles. Because MPP + profiles can also contain a spectral description of device behavior, + there are extra options in mpplu to describe how to convert spectral + values into CIE tristimulus values.
+ Some additional functionality is included in mpplu, analogous to iccgamut, allowing gamut files and + images to be generated from MPP profiles.
+
+ The -v flag causes extra information about the profile to be + printed.
+
+ The -f flag is experimental, and should be ignored.
+
+ Normally L*a*b* is displayed, but this can be changed using the the + -p flag and XYZ, Yxy, or spectral values to be be displayed.
+
+ If an illuminant, observer or Fluorescent Whitening Agent + compensation is selected, then the CIE tristimulus values will be + computed from the spectral information in the MPP profile (if + present).
+
+ The -l flag overrides any default ink limit (Total Area + Coverage) recorded in the profile. The ink limit has an effect on + the results of a gamut generated from the profile.
+
+ The -i flag allows specifying a standard or custom + illumination spectrum, applied to reflective spectral profile data + to compute CIE tristimulus values. A, D50, D65, + F5, F8, F10 are a selection of standard + illuminant spectrums, with D50 being the default. If a + filename is specified instead, it will be assumed to be an Argyll + specific .sp spectrum file.
+
+ The -o flag allows specifying a tristimulus + observer, and is used to compute PCS (Profile Connection Space) + tristimulus values. The following choices are available:
+   1931_2 selects the standard CIE 1931 2 degree + observer. The default.
+   1964_10 selects the standard CIE 1964 10 degree + observer.
+   2012_2 selects the proposed CIE 2012 2 degree observer
+   2012_10 selects the proposed CIE 2012 10 degree + observer
+   1955_2 selects the Stiles and Birch 1955 2 degree + observer
+   1978_2 selects the Judd and Voss 1978 2 degree + observer
+   shaw selects the Shaw and Fairchild 1997 2 degree + observer
+   file.cmf selects an observer specified by the + given .cmf file.
+
+ The -u flag enables Fluorescent Whitening Agent + compensation, which compensates for the effect a different + illuminant will have, on any Fluorescent Whitening Agent present in + the reflective media.
+
+ The -g flag causes mpplu to simply generate a gamut surface + description from the profile, creating a .gam file with the same base + name as the given profile.
+
+ The -w flag causes the gamut surface to be generated in X3DOM format as well as .gam format.
+
+ The -n flag suppresses the X3DOM + axes.
+
+ The -a n parameter sets a + transparency level in the X3DOM surface.
+
+ The -d parameter controls the level of detail displayed in + the gamut surface. The parameter roughly corresponds to a deltaE + value, so smaller values give greater detail. The default value is + around 10, and is a good place to start. Small values may take a lot + of time to generate, and will produce big files.
+
+ The -t parameter invokes special MPP test and diagnostic + output.
+
+
+
+
+ -- cgit v1.2.3