diff options
Diffstat (limited to 'doc/dispcal.html')
| -rwxr-xr-x[-rw-r--r--] | doc/dispcal.html | 226 |
1 files changed, 220 insertions, 6 deletions
diff --git a/doc/dispcal.html b/doc/dispcal.html index ff96ff2..4a8e9c3 100644..100755 --- a/doc/dispcal.html +++ b/doc/dispcal.html @@ -70,6 +70,10 @@ + + + + Verbose mode<br>
</span></font><font size="-1"><span style="font-family:
@@ -137,6 +141,10 @@ for + + + + VideoLUT access.</span></font><br>
<font size="-1"><span style="font-family: monospace;"> <a
@@ -195,6 +203,10 @@ list + + + + 1)</span></font><br>
<span style="font-family: monospace;"> <a href="#dweb">-dweb[:port]</a> @@ -243,6 +255,10 @@ list + + + + Display via a web server at port (default 8080)</span><br>
<span style="font-family: monospace;"> <a href="#dmadvr">-dmadvr</a>
@@ -276,6 +292,10 @@ list + + + + [MSWin] Display via MadVR Video Renderer</span><br>
<tt> </tt><tt><a href="#dcc">-dcc[:n]</a> @@ -288,6 +308,10 @@ list + + + + </tt><tt>Display via n'th ChromeCast (default 1, ? for list)</tt><br
style="font-family: monospace;">
@@ -342,10 +366,14 @@ list + + + + listno</a><span style="font-family: monospace;">
- Set communication port from
- the following list (default 1)<br>
+ Choose instrument from the
+ following list (default 1)<br>
</span></small><font size="-1"><span style="font-family:
monospace;"> </span><a style="font-family: monospace;"
href="#r">-r</a><span style="font-family: monospace;">
@@ -420,6 +448,10 @@ list + + + + Fast ICC Profile Description string (Default "outfile")<br>
<a href="#u">-u</a> @@ -477,6 +509,10 @@ ICC + + + + profile VideoLUTs</span><span style="font-family: monospace;"></span><span
style="font-family: monospace;"></span><br style="font-family:
@@ -530,6 +566,10 @@ ICC + + + + Quality - Low, Medium (def), High<br>
<a href="#p">-p</a> @@ -568,6 +608,10 @@ ICC + + + + Use telephoto mode (ie. for a projector) (if available)<br>
</span></font><font size="-1"><span style="font-family:
@@ -619,6 +663,10 @@ ICC + + + + Display type - instrument specific list to choose from.</span></font><font
size="-1"><span style="font-family: monospace;"><br
@@ -680,6 +728,10 @@ in + + + + deg. K (deflt.)<br>
</span></font><font size="-1"><span style="font-family:
@@ -739,6 +791,10 @@ temperaturee + + + + in deg. K</span></font><br style="font-family: monospace;">
<font size="-1"><span style="font-family: monospace;"></span><span
@@ -791,6 +847,10 @@ temperaturee + + + + Set the target white point as chromaticity coordinates</span><br
style="font-family: monospace;">
@@ -843,6 +903,10 @@ temperaturee + + + + Set the target white brightness in cd/m^2</span><br
style="font-family: monospace;">
@@ -895,6 +959,10 @@ temperaturee + + + + Set the target response curve gamma (Def. 2.4)</span><br
style="font-family: monospace;">
@@ -945,6 +1013,10 @@ temperaturee + + + + Use "-gl" for L*a*b* curve</span><br style="font-family:
monospace;">
@@ -995,6 +1067,10 @@ temperaturee + + + + Use "-gs" for sRGB curve<br>
@@ -1052,6 +1128,10 @@ use + + + + -a as well!)<br>
@@ -1101,6 +1181,10 @@ use + + + + Use "-g240" for SMPTE 240M curve </span></font><font size="-1"><span
style="font-family: monospace;">(should use -a as well!)</span></font><br>
@@ -1151,6 +1235,10 @@ use + + + + Use "-G2.4 -f0" for BT.1886</span></font> @@ -1192,6 +1280,10 @@ use + + + + <br>
<font size="-1"><span style="font-family: monospace;"> </span><a
@@ -1254,6 +1346,10 @@ output + + + + offset (default all output offset)<br>
<a href="#a">-a ambient</a> @@ -1303,6 +1399,10 @@ output + + + + Use viewing condition adjustment for ambient in Lux<br>
</span></font><font size="-1"><span style="font-family:
@@ -1322,6 +1422,10 @@ output + + + + Use forced black point hack<br>
</span></font> <font size="-1"><span style="font-family:
@@ -1373,6 +1477,10 @@ output + + + + Set the target black brightness in cd/m^2</span></font><br
style="font-family: monospace;">
@@ -1426,6 +1534,10 @@ output + + + + Run n verify passes on final curves<br>
</span></font><font size="-1"><span style="font-family:
@@ -1479,6 +1591,10 @@ output + + + + Run only verify pass on installed calibration curves</span></font><br
style="font-family: monospace;">
@@ -1541,6 +1657,10 @@ center, + + + + = right/bottom etc.</span><br style="font-family: monospace;">
<span style="font-family: monospace;"> @@ -1598,6 +1718,10 @@ normal, + + + + = double etc.<br>
</span></font><font size="-1"><span style="font-family:
@@ -1635,6 +1759,10 @@ normal, + + + + ss,vs: = optional horizontal, vertical scale.</span></font><br>
<font size="-1"><span style="font-family: monospace;"> <a
@@ -1686,6 +1814,10 @@ normal, + + + + Fill whole screen with black background</span></font><font
size="-1"><span style="font-family: monospace;"></span></font><br>
@@ -1717,6 +1849,10 @@ normal, + + + + </span></font><small><span style="font-family: monospace;">Video
encode output as (16-235)/255 "TV" levels</span></small><br
@@ -1779,6 +1915,10 @@ on + + + + test window<br>
</span></font><font size="-1"><span style="font-family:
@@ -1834,6 +1974,10 @@ on + + + + Disable initial calibration of instrument if possible</span></font><br>
<font size="-1"><span style="font-family: monospace;"> </span><a
@@ -1893,6 +2037,10 @@ on + + + + Apply Colorimeter Correction Matrix</span></font><br>
<span style="font-family: monospace;"> <a href="#X2">-X
@@ -1946,6 +2094,10 @@ Calibration + + + + Spectral Samples for calibration</span><font size="-1"><span
style="font-family: monospace;"><br>
@@ -2001,11 +2153,18 @@ Calibration + + + + 1931_2 </span></small><small><span
style="font-family: monospace;">(def.)</span></small><small><span
- style="font-family: monospace;">, 1964_10, S&B 1955_2, shaw,
- J&V 1978_2, 1964_10c<br>
+ style="font-family: monospace;">, 1964_10, </span></small><small><span
+ style="font-family: monospace;"><tt><small>2012_2, 2012_10, </small></tt>S&B + +
+ 1955_2, shaw, J&V 1978_2, 1964_10c or file.cmf<br>
<a href="#I">-I b|w</a> @@ -2053,6 +2212,10 @@ Calibration + + + + Drift compensation, Black: -Ib, White: -Iw, Both: -Ibw</span></small><br>
<small><span style="font-family: monospace;"><tt> <a href="#YR">-Y @@ -2071,6 +2234,10 @@ Calibration + + + + R:<i>rate</i></a> @@ -2088,6 +2255,10 @@ Calibration + + + + Override measured refresh rate with rate Hz<br>
</tt> </span></small><font size="-1"><span
@@ -2173,6 +2344,10 @@ none, + + + + h = HW, x = Xon/Xoff</span></font><font size="-1"><span
style="font-family: monospace;"></span></font><br>
@@ -2226,6 +2401,10 @@ none, + + + + Print debug diagnostics to stderr</span></font><br
style="font-family: monospace;">
@@ -2279,6 +2458,10 @@ none, + + + + </span><span style="font-family: monospace;">Base name for created
or updated </span></font><font size="-1"><a style="font-family:
@@ -2399,6 +2582,10 @@ none, + + + + 1,2</span> . Some experimentation may be needed using <a
href="dispwin.html">dispwin</a> on such systems, to discover what
@@ -2456,6 +2643,10 @@ none, falls back to the Default receiver (see <a href="Installing.html">installation + + + + instructions</a> for your platform).<br>
<br>
@@ -2714,6 +2905,10 @@ Set + + + + the target response curve gamma. This is normally an exponential
curve (output = input ^gamma), and defaults to 2.4 on MSWindows and
@@ -2770,6 +2965,10 @@ the + + + + L* curve, which is the response of the CIE L*a*b* perceptual
colorspace (<span style="font-weight: bold;">-gl</span>). the REC
@@ -2877,6 +3076,10 @@ As + + + + explained above, the gamma value provided to the <span
style="font-weight: bold;">-g</span> option is used to set and
@@ -3018,6 +3221,10 @@ If + + + + the black point is not being set completely to the same hue as the
white point (ie. because the <span style="font-weight: bold;">-k</span>
@@ -3178,7 +3385,9 @@ If information (ie. the X-Rite <span style="font-weight: bold;">i1d3</span>,
or the DataColor <span style="font-weight: bold;">Spyder4 &
Spyder 5</span>).This can improve a colorimeters accuracy for a
- particular type of display.<br>
+ particular type of display. A list of contributed <span
+ style="font-weight: bold;">ccss</span> files is <a
+ href="ccsss.html">here</a>.<br>
<br>
<a name="Q"></a> The <b>-Q</b> flag allows specifying a tristimulus
observer, and is used to compute PCS (Profile Connection Space)
@@ -3187,7 +3396,10 @@ If <b> 1931_2</b> selects the standard CIE 1931 2 degree
observer. The default.<br>
<b>1964_10</b> selects the standard CIE 1964 10 degree
- observer.<br>
+ observer<br>
+ <b> 2012_2</b> selects the proposed CIE 2012 2 degree observer<br>
+ <b>2012_10</b> selects the proposed CIE 2012 10 degree
+ observer<br>
<b>1955_2</b> selects the Stiles and Birch 1955 2 degree
observer<br>
<b>1978_2 </b>selects the Judd and Voss 1978 2 degree
@@ -3197,6 +3409,8 @@ If <b>1964_10c</b> selects a version of the CIE 1964 10 degree
observer that has been adjusted using a 3x3 matrix to better agree
with the 1931 2 degree observer.<br>
+ <i><b>file.cmf</b></i> selects an observer specified by the
+ given <a href="File_Formats.html#.cmf">.cmf</a> file.<br>
<br>
<span style="font-weight: bold;">NOTE</span> that if you select
anything other than the default 1931 2 degree observer, that the Y
|