diff options
Diffstat (limited to 'doc/spec2cie.html')
-rwxr-xr-x | doc/spec2cie.html | 24 |
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> </span></small></tt><tt><small>-v + Verbose mode<br> <a href="A">-A NN|AX|AG|XA|XG|GA|GX</a> XRGA conversion (default NN)<br> @@ -58,10 +61,12 @@ + + Override actual instrument illuminant in .ti3 or .sp file:<br> @@ -70,6 +75,7 @@ + (only used in conjunction with <span style="font-weight: bold;">-f</span>)<br> </small></small></tt><tt><small><small> <a href="#f">-f [<i>illum</i>]</a> @@ -77,23 +83,27 @@ + Use Fluorescent Whitening Agent compensation [simulated inst. illum.:<br> + M0, M1, M2, A, C, D50 (def.), D50M2, D65, F5, F8, F10 or file.sp]<br> </small></small></tt><tt><small><small><small> <a href="#i">-i + <i>illum</i></a> + Choose illuminant for computation of CIE XYZ from spectral data & FWA:<br> @@ -110,10 +120,12 @@ + + Choose CIE Observer for spectral data:<br> @@ -121,10 +133,12 @@ + 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&B 1955_2, shaw, J&V 1978_2 or file.cmf<br> <a href="#p">-n</a> @@ -140,6 +154,7 @@ output + spectral values<br> </small></tt><tt><small> <a href="#p">-p</a> @@ -148,6 +163,7 @@ output + Plot each values spectrum</small></tt><tt><br> </tt><tt> </tt><tt><small> <span style="font-style: italic;">input.[ti3|sp]</span> @@ -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> |