gronod/argyllcms
1
0
Fork 0
Code Issues Pull Requests Actions Packages Projects Releases 11 Wiki Activity
Files
main
argyllcms/doc/instruments.html
T
gronod 45bdf51201 Initial commit of v3.5.0
2026-08-20 20:28:40 +01:00

7757 lines
121 KiB
HTML
Executable File
Raw Permalink Blame History

<!DOCTYPE html PUBLIC "-//W3C//DTD HTML 4.01 Transitional//EN">
<html>
<head>
<title>Operation of particular instruments</title>
<meta http-equiv="content-type" content="text/html;
charset=windows-1252">
</head>
<body>
<h2><u>Operation of particular instruments</u></h2>
<span style="font-weight: bold;">Please note that instruments are
being driven by ArgyllCMS drivers, and that any problems or
queries regarding instrument<br>
operation </span><span style="font-weight: bold;">should be
directed to the Argyll's author(s) or the Argyll mailing list, and
not to any</span> <span style="font-weight: bold;">other party.</span><span
style="font-weight: bold;"></span><br>
<br>
The following instruments are directly supported:<br>
(Please <span style="font-weight: bold;">note</span> the <a
href="Installing.html">installation instructions</a> for each
platform - they contain important information for getting your
instruments working.)<br>
<br>
JETI:<br>
<br>
&nbsp;&nbsp;&nbsp; <a href="#specbos">specbos 1211 &amp; 1201</a>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
- Tele-Spectro-Radiometer<br>
&nbsp;&nbsp;&nbsp; <a href="#spectraval">spectraval 1511&amp; 1501</a>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
&nbsp; - Tele-Spectro-Radiometer<br>
&nbsp;&nbsp;&nbsp; <a href="#specbos2501" moz-do-not-send="true">specbos
2501</a>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
&nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;&nbsp; -
Tele-Spectro-Radiometer<br>
<br>
Image Engineering:<br>
<br>
&nbsp;&nbsp;&nbsp; <a href="#ex1">EX1</a>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
- Tele-Spectro-Radiometer<br>
<br>
Klein:<br>
<br>
&nbsp;&nbsp;&nbsp; <a href="#k10a">K10-A</a>&nbsp;&nbsp;
&nbsp;&nbsp;&nbsp; &nbsp;&nbsp;&nbsp; &nbsp;&nbsp;&nbsp;
&nbsp;&nbsp;&nbsp; &nbsp;&nbsp;&nbsp; &nbsp;&nbsp;&nbsp;
&nbsp;&nbsp;&nbsp; &nbsp;&nbsp;&nbsp; &nbsp;&nbsp;&nbsp;
&nbsp;&nbsp;&nbsp; - Display Colorimeter. Reported also to work with
the K-1, K-8 and&nbsp; K-10<br>
<br>
X-Rite &amp; Calibrite:<br>
&nbsp;&nbsp;&nbsp; <a href="#DTP20">DTP20 "Pulse"</a>&nbsp;
&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
- "swipe" type reflective spectrometer, that can be used untethered.<br>
&nbsp;&nbsp;&nbsp; <a href="#DTP22">DTP22 Digital Swatchbook</a>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
- spot type reflective spectrometer.<br>
&nbsp;&nbsp;&nbsp; <a href="#DTP41">DTP41</a>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
- spot and strip reading reflective spectrometer.<br>
&nbsp;&nbsp;&nbsp; <a href="#DTP41">DTP41T</a> &nbsp; &nbsp; &nbsp;
&nbsp; &nbsp; &nbsp; &nbsp; &nbsp;&nbsp;
&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
- spot and strip reading reflective/transmissive spectrometer.<br>
&nbsp;&nbsp;&nbsp; <a href="#dtp51">DTP51</a>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
- strip reading reflective colorimeter.<br>
&nbsp;&nbsp;&nbsp; <a href="#DTP92">DTP92</a>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
- CRT display colorimeter.<br>
&nbsp;&nbsp;&nbsp; <a href="#DTP94">DTP94</a> <font size="-1">"Optix
XR"</font> or "Optix XR2" or "Optix Pro"- display colorimeter.<br>
<a href="#ColorMunki"><span style="text-decoration: underline;"></span></a>&nbsp;&nbsp;&nbsp;
<a href="#ColorMunki"><span style="text-decoration: underline;">ColorMunki</span></a>
Design or Photo or i1Studio, ColorChecker Studio.<br>
&nbsp;&nbsp;&nbsp; &nbsp;&nbsp;&nbsp; &nbsp;&nbsp;&nbsp;
&nbsp;&nbsp;&nbsp; &nbsp;&nbsp;&nbsp; &nbsp;&nbsp;&nbsp;
&nbsp;&nbsp;&nbsp; &nbsp;&nbsp;&nbsp; &nbsp;&nbsp;&nbsp;
&nbsp;&nbsp;&nbsp; &nbsp;&nbsp;&nbsp; &nbsp; &nbsp; &nbsp;&nbsp;
&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; - spot and "swipe"
reflective/emissive spectrometer (UV cut only).<br>
&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
[ The OEM&nbsp; XEROX PhaserMeter is also reported to work. ] <br>
&nbsp;&nbsp;&nbsp; <a href="#i1d"><span style="text-decoration:
underline;">ColorMunki</span></a> Create or Smile&nbsp;&nbsp;
&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; - display
colorimeter. (Similar to an Eye-One Display 2)<br>
&nbsp;&nbsp;&nbsp; <a href="#Huey">Lenovo W</a> &nbsp; &nbsp;
&nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;
&nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; - built in laptop
Huey display colorimeter.<br>
&nbsp;&nbsp;&nbsp; <a href="#i1d3">Eye-One Display 3</a> &nbsp;
&nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;
&nbsp; &nbsp; - i1 DisplayPro, DisplayPro Plus and ColorMunki
Display/i1Display Studio<br>
&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
Calibrite ColorChecker Display/Pro/Plus<br>
&nbsp;&nbsp;&nbsp; &nbsp;&nbsp;&nbsp; &nbsp;&nbsp;&nbsp;
&nbsp;&nbsp;&nbsp; &nbsp;&nbsp;&nbsp; &nbsp;&nbsp;&nbsp;
&nbsp;&nbsp;&nbsp; &nbsp;&nbsp;&nbsp; &nbsp;&nbsp;&nbsp;
&nbsp;&nbsp;&nbsp; &nbsp;&nbsp;&nbsp; &nbsp;&nbsp;&nbsp;
&nbsp;&nbsp;&nbsp; &nbsp;&nbsp;&nbsp;&nbsp;&nbsp; [ Other branded
i1d3's are also reported to work.]<br>
&nbsp; &nbsp; <a href="#i1p2">i1Pro2</a> "EFI ES-2000"&nbsp;&nbsp;
&nbsp;&nbsp;&nbsp;&nbsp;
&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
- spot and "swipe" reflective/emissive spectrometer.<br>
&nbsp; &nbsp; <a href="#i1p3">i1Pro3</a> and <b>i1Pro3 Plus</b>&nbsp;
&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
- spot and "swipe" reflective/emissive spectrometer.<br>
<br>
Gretag-Macbeth (now X-Rite):<br>
&nbsp; &nbsp; <a href="#sl">Spectrolino</a> &nbsp; &nbsp; &nbsp;
&nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;
&nbsp; &nbsp; &nbsp; &nbsp; &nbsp; - spot reflective/emissive
spectrometer<br>
&nbsp; &nbsp; <a href="#ss">SpectroScan</a> &nbsp; &nbsp; &nbsp;
&nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;
&nbsp; &nbsp; &nbsp; &nbsp; - spot reflective/emissive, XY table
reflective spectrometer&nbsp; <br>
&nbsp; &nbsp; <a href="#ss">SpectroScanT</a> &nbsp; &nbsp; &nbsp;
&nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;
&nbsp; &nbsp; &nbsp; - spot reflective/emissive/transmissive, XY
table reflective spectrometer<br>
&nbsp; &nbsp; <a href="#i1p">Eye-One Pro</a> "EFI ES-1000" &nbsp;
&nbsp; &nbsp; &nbsp; &nbsp; - spot and "swipe" reflective/emissive
spectrometer<br>
&nbsp; &nbsp; <a href="instruments.html#i1m">Eye-One Monitor</a>
&nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;
&nbsp; &nbsp; &nbsp; &nbsp; - spot and "swipe" emissive spectrometer<br>
&nbsp;&nbsp;&nbsp; <a href="#i1d">Eye-One Display 1 or 2&nbsp; or
LT</a>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; - display
colorimeter<br>
&nbsp;&nbsp;&nbsp; <a href="instruments.html#i1d">HP DreamColor or
APS</a>&nbsp;
&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
- display colorimeter. (Treated as a Eye-One Display 2)<br>
&nbsp;&nbsp;&nbsp; <a href="#i1d">CalMAN X2</a>
&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
- display colorimeter. (Treated as a Eye-One Display 2)<br>
&nbsp;&nbsp;&nbsp; <a href="#Huey">Huey</a> &nbsp; &nbsp; &nbsp;
&nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;
&nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;
&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; - display colorimeter<br>
<br>
Sequel imaging (Now X-Rite):<br>
&nbsp;&nbsp;&nbsp;&nbsp; <a href="#mox">MonacoOPTIX</a> &nbsp;
&nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;&nbsp;
&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; - display colorimeter (Treated
as an Eye-One Display 1)<br>
&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
[The Sequel Chroma 4 &amp; 5, and Sencore ColorPro V, IV &amp; III
also work.]<br>
<br>
Lacie Blue
Eye:&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
- see <a href="#i1d">Eye-One Display</a><br>
<br>
DataColor ColorVision:<br>
&nbsp;&nbsp;&nbsp;&nbsp; <a href="#spyd2">Spyder 2</a> &nbsp;
&nbsp; &nbsp; &nbsp;&nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;
&nbsp; &nbsp; &nbsp; &nbsp;&nbsp;
&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; - display colorimeter (Note
that the user must <a href="oeminst.html">supply</a> firmware)<br>
&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
[The Spyder 1 also seems to work.]<br>
&nbsp;&nbsp;&nbsp;&nbsp; <a href="#spyd3">Spyder 3</a> &nbsp;
&nbsp; &nbsp; &nbsp;&nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;
&nbsp; &nbsp; &nbsp; &nbsp;&nbsp;
&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; - display colorimeter.<br>
&nbsp;&nbsp;&nbsp;&nbsp; <a href="#spyd4">Spyder 4</a> &nbsp;
&nbsp; &nbsp; &nbsp;&nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;
&nbsp; &nbsp; &nbsp; &nbsp;&nbsp;
&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; - display colorimeter (Note
that the user must <a href="oeminst.html">supply</a> calibration
data)<br>
&nbsp;&nbsp;&nbsp;&nbsp; <a href="#spyd5">Spyder 5</a> &nbsp;
&nbsp; &nbsp; &nbsp;&nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;
&nbsp; &nbsp; &nbsp; &nbsp;&nbsp;
&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; - display colorimeter (Note
that the user must <a href="oeminst.html">supply</a> calibration
data)<br>
&nbsp;&nbsp;&nbsp;&nbsp; <a href="#spydX">SpyderX</a> &nbsp; &nbsp;
&nbsp; &nbsp;&nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;
&nbsp; &nbsp; &nbsp;&nbsp;
&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; - display colorimeter<br>
&nbsp;&nbsp;&nbsp;&nbsp; <a href="#spydX2" moz-do-not-send="true">SpyderX2</a>
&nbsp; &nbsp; &nbsp; &nbsp;&nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;
&nbsp; &nbsp; &nbsp; &nbsp; &nbsp;&nbsp;
&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; - display colorimeter<br>
&nbsp;&nbsp;&nbsp;&nbsp; <a href="#spyd2024" moz-do-not-send="true">Spyder
&amp; SpyderPRO (2024)</a> &nbsp; &nbsp;&nbsp; - display
colorimeter<br>
<br>
Other:<br>
&nbsp;&nbsp;&nbsp; <span class="titre"><a href="#HCFR">Colorimètre
HCFR</a>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
- display colorimeter<br>
</span>&nbsp;&nbsp;&nbsp; <a href="#ColorHug">ColorHug</a> &amp;
ColorHug2&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
- display colorimeter<span class="titre"></span><br>
&nbsp;&nbsp;&nbsp; <a href="#SMCube">Palette/SwatchMate Cube</a>
&nbsp;&nbsp; &nbsp; &nbsp;&nbsp; &nbsp;&nbsp;&nbsp; - reflective
colorimeter<br>
<br>
Other instruments can be supported indirectly, since patch result
files created by other packages can be imported into Argyll.<br>
<span class="titre"><br>
General information about:<br>
<br>
&nbsp;&nbsp;&nbsp; <a href="#strip">Strip reading instruments</a><br>
</span>&nbsp;&nbsp;&nbsp; <a href="#xy">X-Y Table instruments</a><br>
&nbsp;&nbsp;&nbsp; <a href="#spot">Spot reading instruments</a><br>
<span style="font-weight: bold;"></span><br>
<br>
There is a <a href="ccsss.html">list of contributed</a> <span
style="font-weight: bold;">ccss</span> (Colorimeter Correction
Spectral Sample) files.<br>
There is a <a href="ccmxs.html">list of contributed</a> <span
style="font-weight: bold;">ccmx</span> (Colorimeter Correction
Matrix) files.<br>
<br>
<hr style="width: 100%; height: 2px;">
<h3><a name="strip"></a>Strip reading instruments</h3>
When used with a <span style="font-weight: bold;">DT20</span>, <span
style="font-weight: bold;">DTP41</span>, <span
style="font-weight: bold;">DTP51</span>, <span
style="font-weight: bold;">Eye-One Pro<span style="font-weight:
bold;"> </span></span>or <span style="font-weight: bold;">ColorMunki</span>
strip reading instrument, chartread will first establish
communications with the instrument, and then set it up ready to read
the strips. The strips are labeled A to ZZ, and for each strip it
will prompt:<br>
<br>
&nbsp;&nbsp;&nbsp; About to read strip XX&nbsp; :<br>
<br>
where XX is the strip label, and this is followed by the available
options to navigate, read the strip, or finish. Note that the normal
(forward) direction of strip reading is one that starts at the strip
label.<br>
<br>
For the <span style="font-weight: bold;">DTP51</span> you should
feed the strip into the instrument, and the microswitch will trigger
the read.<br>
<br>
For the <span style="font-weight: bold;">DTP41</span> you should
line the appropriate strip up in the machine, and press its button.<br>
<br>
For the <span style="font-weight: bold;">Eye-One Pro</span> you
should set the guide to the appropriate strip, place the instrument
<span style="text-decoration: underline;">ahead</span> of the first
patch on blank paper, and then press and hold the instruments
button. When you hear a beep from the computer, you can then move
the instrument steadily over the patches, releasing the button after
the instrument is past the last patch. Moving the instrument too
fast or changing speeds may cause a mis-read, or a scan with few
samples read per patch.<br>
<br>
For the <span style="font-weight: bold;">ColorMunki</span> with the
default chart, the patches are the same width as the silver portion
of body (white version), or the textured portion of the body (black
version). Place aperture of the the instrument (located at its
center) in the white space ahead of the first patch, and then press
and hold the instruments button. When you hear a beep from the
computer, you can then move the instrument steadily over the
patches, releasing the button after the instrument is past the last
patch. Moving the instrument too fast or changing speeds may cause a
mis-read, or a scan with few samples read per patch. For the <span
style="font-weight: bold;">high density</span> ColorMunki chart (<a
href="printtarg.html#h">printtarg -h</a>), the patches are
arranged so that three rows are exactly the width of the&nbsp; body
of the instrument. If you are careful you can use this to guide the
center of the instrument over each row, or you may prefer to use
something like a plastic ruler to help guide the instrument.<br>
<br>
Using the <span style="font-weight: bold;">DTP20</span> or the <span
style="font-weight: bold;">Eye-One Pro</span> or <span
style="font-weight: bold;">ColorMunki</span> with a randomized
chart layout, the strip may be scanned from either direction. If a
randomized chart layout has not been used for the <span
style="font-weight: bold;">Eye-One Pro</span> or <span
style="font-weight: bold;">ColorMunki</span>, then the chart
should only be read in the one direction (use <a
href="chartread.html#B">chartread -B</a>).<br>
<br>
Note that you may have to check that system alert sounds are enabled
and at a suitable volume to in order to hear the beep prompt. For
the Eye-One Pro and ColorMunki, a second beep will sound after a
successfully read strip, or a double beep will sound,&nbsp;
indicating a failure or warning that needs attention. See also the
note on Linux in <a href="Installing_Linux.html">installation</a>.<br>
<br>
If the strip is read successfully there will be a single "success"
beep, and the line will be followed with:<br>
<br>
&nbsp;&nbsp;&nbsp; Ready to read strip&nbsp; XX&nbsp; : <br>
&nbsp;&nbsp;&nbsp; Strip read OK<br>
<br>
If there is an error of some sort there will be a double "fail"
beep, and a message will be issued, and you will be asked whether to
abort the chart reading, or retry the<br>
failed strip:<br>
<br>
&nbsp;&nbsp;&nbsp; Ready to read strip XX&nbsp; : <br>
&nbsp;&nbsp;&nbsp; Strip read failed due to misread (Not enough
patches)<br>
<br>
&nbsp;&nbsp;&nbsp; Hit Esc to give up, any other key to retry:<br>
<br>
If you are unable to successfully read a strip after several
retries, you can skip that strip using the <span
style="font-weight: bold;">'n'</span> key, and save<br>
the chart readings without that strip.<br>
<br>
If the strip is read successfully, but the patches values don't seem
to be what is expected, you will get a double "fail" beep&nbsp; and
the following type of warning:<br>
<br>
&nbsp;&nbsp;&nbsp; Ready to read strip&nbsp; XX&nbsp; :<br>
&nbsp;&nbsp;&nbsp; (Warning) Seem to have read strip&nbsp; YY&nbsp;
rather than&nbsp; XX !<br>
&nbsp;&nbsp;&nbsp; Hit Return to use it anyway, any other key to
retry, Esc, ^C or Q to give up:<br>
<br>
This could be because you have accidentally read the wrong strip (a
common mistake), or it could be that the device response is so
different from what is expected that warning is erroneous, or you
may get a lot of these sorts of warnings if you are accidentally
reading the wrong chart. You may also get this sort of warning if
you are not using bi-direction reading (chartread -B), and read the
strip from the wrong end.<br>
If you are absolutely sure you lined up the correct strip, then hit
return, otherwise line the appropriate strip up again, and hit some
other key (ie. space).<br>
Erroneous warnings are less likely if a previous profile for a
device was given to <span style="font-weight: bold;">targen</span>
to set more accurate expectations.<br>
<br>
You may also see the following type of warning:<br>
<br>
&nbsp;&nbsp;&nbsp; Ready to read strip&nbsp; XX&nbsp; :<br>
&nbsp;&nbsp;&nbsp; (Warning) Patch error YY.YYY (&gt;35 not good,
&gt;95 bad)<br>
&nbsp;&nbsp; There is at least one patch with an very unexpected
response!<br>
&nbsp;&nbsp;&nbsp; Hit Return to use it anyway, any other key to
retry, Esc, ^C or Q to give up:<br>
<br>
Similar to the previous warning, this indicates that while the right
strip appears to have been read, one of the patch readings is quite
different to what is expected. This may indicate an error of some
sort (ie. damaged test chart, or bad instrument positioning), or may
be erroneous if the actual device response is quite different to the
expectation. Erroneous warnings are less likely if a previous
profile for a device was given to <span style="font-weight: bold;">targen</span>
to set more accurate expectations.<br>
<br>
You can also navigate the next strip to be read using the <span
style="font-weight: bold;">'f'</span> key to move forward and the
<span style="font-weight: bold;">'b'</span> keys<span
style="font-weight: bold;"></span><span style="font-weight: bold;"></span>
to move backwards. The prompt will indicate whether this strip has
already been read or not, or whether all strips have been read. You
can also use <span style="font-weight: bold;">'n'</span> to move
forward to the next unread strip. After each successful reading it
will move forward to the next unread strip. When you are finished,
use the <span style="font-weight: bold;">'d'</span> to indicate
that you are done. You can choose to finish before all the strips
are read, and the patches that have been read will be saved to the
.ti3 file. This is useful if you are unable to read a particular
strip successfully, or if you are unable to finish the chart in one
session, and you can later <span style="text-decoration:
underline;">resume</span> reading the chart by using the <span
style="font-weight: bold;">chartread -r</span> flag. [You could
resume reading the chart patch by patch using the <span
style="font-weight: bold;">chartread -r -p</span> if you are
unable to read a strip successfully.]<br>
<br>
When reading in patch by patch mode, there are a few additional
navigation options, such as <span style="font-weight: bold;"><span
style="font-weight: bold;">F</span></span> to move forward 10
patches, <span style="font-weight: bold;">B</span> to move
backwards 10 patches, and <span style="font-weight: bold;">g</span>
to go to a specific patch.<br>
<br>
You can abort the whole process at any time by hitting Escape, and
the readings will not be saved.<br>
<br>
<hr style="width: 100%; height: 2px;">
<h3><a name="xy"></a>X-Y Table instruments</h3>
When you are using an XY table type instrument, such as a Gretag <span
style="font-weight: bold;">SpectroScan</span>, &nbsp;chartread
will first establish communications with the instrument, and then
set it up ready to read the chart. You will be prompted for each
sheet with a message such as:<br>
<br>
&nbsp;&nbsp;&nbsp; Please make sure that the white reference is in
slot 1, then<br>
&nbsp;&nbsp;&nbsp; place sheet 1 of 4 on table, then<br>
&nbsp;&nbsp;&nbsp; hit return to continue, Esc to give up<br>
<br>
After hitting return you will be prompted to line up three squares
on the sheet, one at a time:<br>
<br>
&nbsp;&nbsp;&nbsp; Using the XY table controls, locate patch A1 with
the sight,<br>
&nbsp;&nbsp;&nbsp; then hit return to continue, Esc to give up<br>
<br>
On completing this, the instrument will commence reading each sheet.<br>
<br>
<hr style="width: 100%; height: 2px;">
<h3><a name="spot"></a>Spot reading instruments</h3>
When used with a <span style="font-weight: bold;">DT22</span> or <span
style="font-weight: bold;">SpectroLino</span> or use the patch by
patch reading mode (<span style="font-weight: bold;">chartread -p</span>)
with the <span style="font-weight: bold;"></span> <span
style="font-weight: bold;">Eye-One Pro<span style="font-weight:
bold;"> </span></span>or <span style="font-weight: bold;">ColorMunki</span>
instrument, or use the external values mode (<span
style="font-weight: bold;">chartread -x</span>), chartread will
first establish communications with the instrument, and then set it
up ready to read the patches. The patches are typically labeled by
column A to ZZ, and row 1-999. Each patch will prompt:<br>
<br>
&nbsp;&nbsp;&nbsp; Ready to read patch 'XX'&nbsp; :<br>
<br>
where XX is the patch label, and this is followed by the available
options to navigate, read the strip, or finish.<br>
<br>
Place the instrument on the indicated patch, and trigger a reading
using one of the available methods (typically using the instrument
switch of pressing a key).<br>
<br>
There should be an audible prompt on a successful or failed reading.
<br>
<br>
Note that you may have to check that system alert sounds are enabled
and at a suitable volume to in order to hear the beep prompt. For
the Eye-One Pro and ColorMunki, a second beep will sound after a
successfully read strip, or a double beep will sound,&nbsp;
indicating a failure or warning that needs attention. See also the
note on Linux in <a href="Installing_Linux.html">installation</a>.<br>
<br>
If the patch is read successfully, the line will be completed with:<br>
<br>
&nbsp;&nbsp;&nbsp; Ready to read patch&nbsp; XX&nbsp; :<br>
&nbsp;&nbsp;&nbsp; Patch read OK<br>
<br>
If there is an error of some sort, a message will be issued, and you
will be asked whether to abort the chart reading, or retry the<br>
failed patch:<br>
<br>
&nbsp;&nbsp;&nbsp; Ready to read patch XX&nbsp; : read_strip
returned 'Strip misread' (Bad reading)<br>
<br>
&nbsp;&nbsp;&nbsp; Strip read failed due to misread<br>
&nbsp;&nbsp;&nbsp; Hit Esc to give up, any other key to retry:<br>
<br>
You can navigate the next patch to be read using the <span
style="font-weight: bold;">'f'</span> key to move forward and the
<span style="font-weight: bold;">'b'</span> keys<span
style="font-weight: bold;"></span><span style="font-weight: bold;"></span>
to move backwards, while <span style="font-weight: bold;">'F'</span>
and <span style="font-weight: bold;">'B'</span> will move forward
and backwards by 10 patches. The prompt will indicate whether this
patch has already been read or not, or whether all patches have been
read. You can also use <span style="font-weight: bold;">'n'</span>
to move forward to the next unread patch. When you are finished, use
the <span style="font-weight: bold;">'d'</span> to indicate that
you are done. You can choose to finish before all the patches are
read, and they will be saved to the .ti3 file. This is useful if you
are unable to finish the chart in one session, and you can later <span
style="text-decoration: underline;">resume</span> reading the
chart by using the <span style="font-weight: bold;">chartread -r</span>
flag.<br>
<br>
You can abort the whole process at any time by hitting Escape, and
the readings will not be saved.<br>
<br>
<span style="font-weight: bold;"></span>
<hr style="width: 100%; height: 2px;">
<h3><a name="displaytype"></a>Display Type<br>
</h3>
Many of the colorimeters have a <span style="font-weight: bold;">display
type</span> selection parameter. Depending on the instrument, this
may combine two related functions: 1) Changing the measurement mode
to suite either refresh-type, or non-refresh displays, and 2)
Changing the calibration to suite a particular displays spectral
characteristics.<br>
<br>
A refresh type display uses a technology that presents different
portions of the image at different times, doing so at a high enough
rate that this is normally imperceptible. This time varying
characteristic can interfere with measuring a display color unless
the instrument makes allowances for it, typically by making its
measurement period a multiple of the display refresh period. Display
types that <span style="font-weight: bold;">refresh</span> are CRT
(Cathode Ray Tube), Single chip DLP (Digital Light Processing) and
Plasma displays. An example of a <span style="font-weight: bold;">non-refresh</span>
display technology is LCD (Liquid Crystal Display), although is a
few cases the back-light illumination may have a low enough
frequency flicker to benefit from the refresh mode.<br>
<br>
Instruments in which the display type selection only changes the
measurement mode (i.e. i1d3), will typically have some other
independent option to set the calibration type. Simpler instruments
combine the measurement mode with a calibration selections,
typically refresh+CRT and non-refresh+LCD. Some instruments are a
hybrid of both (Spyder4), where the display type can select between
generic refresh/non-refresh that can then use a .CCSS to set the
calibration type, or a combined selection of non-refresh and a
particular display type.<br>
<br>
See <a
href="http://en.wikipedia.org/wiki/Comparison_of_display_technology">Comparison_of_display_technology</a>
for some background on different display technologies.<br>
<br>
<hr width="100%" size="2"><br>
<h3><a name="refreshmeasurement"></a>Refresh Rate Measurement</h3>
<p>Most of the colorimeters that have a refresh display type
selection, also have an ability to measure the refresh rate of a
display. Some of the spectrometers also have a display refresh
rate measurement capability when in an emissive measurement mode,
even though they don't use this to support a refresh display mode.
You can do a display refresh rate measurement in <a
href="spotread.html">spotread</a> using the <b>'F' </b>key.
The particular instruments have a range of accuracy when making
this measurement. A rough guide is as follows:<br>
<br>
</p>
<table width="372" height="230" cellspacing="2" cellpadding="2"
border="1">
<tbody>
<tr>
<td valign="top"><b>Instrument</b></td>
<td valign="top"><b>Typical error in Hz.</b></td>
</tr>
<tr>
<td valign="top">spectrobos 1211/1201/1501/1511/2501<br>
</td>
<td valign="top">0.05<br>
</td>
</tr>
<tr>
<td valign="top">Klein K10-A<br>
</td>
<td valign="top">0.05<br>
</td>
</tr>
<tr>
<td valign="top">DTP92<br>
</td>
<td valign="top">0.1<br>
</td>
</tr>
<tr>
<td valign="top">i1 Display 2<br>
</td>
<td valign="top">0.5<br>
</td>
</tr>
<tr>
<td valign="top">Spyder 2<br>
</td>
<td valign="top">0.7<br>
</td>
</tr>
<tr>
<td valign="top">Spyder 3<br>
</td>
<td valign="top">3<br>
</td>
</tr>
<tr>
<td valign="top">Spyder 4<br>
</td>
<td valign="top">3<br>
</td>
</tr>
<tr>
<td valign="top">i1 Display Pro<br>
</td>
<td valign="top">0.05<br>
</td>
</tr>
<tr>
<td valign="top">i1 Pro Spectro.<br>
</td>
<td valign="top">0.05<br>
</td>
</tr>
<tr>
<td valign="top">ColorMunki Spectro.<br>
</td>
<td valign="top">0.05<br>
</td>
</tr>
</tbody>
</table>
<p><br>
</p>
<hr width="100%" size="2">
<p><span style="font-weight: bold;"><a name="specbos"></a><span
style="font-weight: bold;">specbos 1211 and 1201
Tele-Spectro-Radiometer<br>
</span></span></p>
<img alt="JETI specbos 1211" src="JETI_1211.jpg" width="257"
height="254">
<p><span style="font-weight: bold;"><br>
</span><span style="font-weight: bold;">Availability:<br>
<br>
</span>The <span style="font-weight: bold;">specbos 1211</span><span
style="font-weight: bold;"> </span>and <b>1201</b> from <a
href="http://www.jeti.com/">JETI</a>&nbsp; are currently
available instruments. These are reference grade instruments
capable of emissive and ambient measurements, and are often used
for monitor, projector and cinema calibration &amp;
characterization, lighting measurement and colorimeter
calibration, amongst many other uses.<br>
</p>
<p>The <b>JETI</b> specbos <span style="font-weight: bold;">1211</span><span
style="font-weight: bold;"> </span>and <b>1201</b> makes use
of the FTDI FT232R Virtual COM Port Drivers (VCP), that may need
installing for your operating system. See <a
href="Installing.html">installation instructions</a>. </p>
<br>
<hr width="100%" size="2">
<p><span style="font-weight: bold;"><a name="spectraval"></a><span
style="font-weight: bold;">spectraval 1511 and 1501
Tele-Spectro-Radiometer<br>
</span></span></p>
<img alt="JETI spectraval 1501" src="JETI_1501.jpg" width="167"
height="253"> <span style="font-weight: bold;"><br>
</span><span style="font-weight: bold;">Availability:<br>
<br>
</span>The <span style="font-weight: bold;">spectraval 1511</span><span
style="font-weight: bold;"> </span>and <b>1501</b> from <a
href="http://www.jeti.com/">JETI</a>&nbsp; are currently available
instruments. These are high grade instruments capable of emissive
measurements, and are often used for monitor, projector and cinema
calibration &amp; characterization and colorimeter calibration,
amongst many other uses.<br>
<br>
The <b>JETI</b> specbos <span style="font-weight: bold;">1511</span><span
style="font-weight: bold;"> </span>and <b>1501</b> makes use of
the newer FTDI FT231XS Virtual COM Port Drivers (VCP), that may need
installing for your operating system. See <a href="Installing.html">installation
instructions</a>.<br>
<br>
<b>Bluetooth:</b> These instruments can be operated via Bluetooth by
first pairing the instrument with your computer and enabling the
Bluetooth serial port, and then allowing the ArgyllCMS tools to
identify the instrument over the serial port. <br>
<br>
<hr width="100%" size="2">
<p><span style="font-weight: bold;"><a name="specbos2501"></a><span
style="font-weight: bold;">specbos 2501
Tele-Spectro-Radiometer<br>
</span></span></p>
<img alt="JETI specbos 2501" src="JETI_2501.jpg"
moz-do-not-send="true" width="300" height="200">&nbsp;&nbsp;
&nbsp;
<p><span style="font-weight: bold;"><br>
</span><span style="font-weight: bold;">Availability:<br>
<br>
</span>The <span style="font-weight: bold;">specbos </span><b>2501</b>
from <a href="http://www.jeti.com/">JETI</a>&nbsp; are currently
available instruments. These are reference grade instruments
capable of emissive measurements, and are often used for monitor,
projector and cinema calibration &amp; characterization, lighting
measurement and colorimeter calibration, amongst many other uses.<br>
</p>
<p>The <b>JETI</b> specbos <span style="font-weight: bold;">25</span><b>01</b>
makes use of the FTDI FT232R Virtual COM Port Drivers (VCP), that
may need installing for your operating system. See <a
href="Installing.html" moz-do-not-send="true">installation
instructions</a>. </p>
<br>
<hr width="100%" size="2">
<p><span style="font-weight: bold;"><br>
<a name="ex1"></a><span style="font-weight: bold;">Image
Engineering EX1<br>
</span></span></p>
<img alt="Image Engineering EX1" src="EX1.jpg" width="253"
height="158"> <span style="font-weight: bold;"><br>
</span><span style="font-weight: bold;"><br>
Availability:<br>
<br>
</span>The <a
href="http://www.image-engineering.de/iq-products/iq-tools/measurement-devices/ex1">Image
Engineering EX1</a> is a currently available instruments. This is
a high resolution spectrometer intended for the measurement of light
sources.
<p> </p>
<p><br>
</p>
<hr width="100%" size="2">
<p><span style="font-weight: bold;"><a name="k10a"></a><span
style="font-weight: bold;">Klein K10-A Colorimeter<br>
</span></span></p>
<img alt="Klein K10-A" src="K10A.jpg" width="267" height="236"><br>
<p><span style="font-weight: bold;"><br>
</span><span style="font-weight: bold;">Availability:<br>
<br>
</span>The <span style="font-weight: bold;">Klein K10-A </span>from
<a href="http://www.kleininstruments.com/">Klein Instruments</a>&nbsp;
is a currently available instrument. It is noted for it's speed,
high precision, and ability to measure to very low light
levels.This is a high end instruments capable of contact and tele
- emissive, and ambient measurements, and are often used for
monitor, projector and cinema calibration and characterization. <br>
</p>
<p>Note that unlike the operation of other instruments, the Ambient
mode is purely manual - the diffuser must be fitted and then the
appropriate calibration setting chosen (Typically with "Lux" in
the name).<br>
</p>
<p>By default, more measurements are taken and averaged together
when the light level is low. This can be disabled and a single
measurement taken per reading, to gain maximum speed by using the
-Y A flag.<br>
</p>
<p>The <b>K-1</b>, <b>K-8</b> and&nbsp; <b>K-10</b> are also
reported to work.<br>
</p>
<p>The&nbsp; <b>Klien K10A</b> makes use of the FTDI FT232R Virtual
COM Port Drivers (VCP), that may need installing for your
operating system. See <a href="Installing.html">installation
instructions</a>.</p>
<p> </p>
<hr width="100%" size="2">
<p><br>
</p>
<span style="font-weight: bold;"></span><br>
<span style="font-weight: bold;"><a name="ColorMunki"></a><span
style="font-weight: bold;">ColorMunki </span>Design or Photo,
i1 Studio <span style="font-weight: bold;">reflective/emissive
spectrometer<br>
</span> <br>
<img style="width: 272px; height: 243px;" alt="" title="ColorMunki
(White)" src="ColorMunki.jpg">&nbsp;&nbsp; <br>
<br>
</span><span style="font-weight: bold;">Availability:<br>
<br>
</span>The <span style="font-weight: bold;">ColorMunki</span> <span
style="font-weight: bold;">Design or Photo </span>or <b>i1
Studio</b> from <a href="http://www.xrite.com/">X-Rite</a>&nbsp;
is currently available in two different packages from the
manufacturer. These packages differ in what features the
manufacturers software provides, as well as cosmetic differences
between the instrument (white and black). This comparison <a
href="http://www.colormunki.com/product/show?page=2">chart</a>
illustrates the differences (Note that the ColorMunki Design comes
with <b>Pantone</b> libraries). Used with Argyll, there are no
differences in operation of a ColorMunki instrument, irrespective of
which package it came with. The ColorMunki Design has the lowest
RRP, but the Photo package may be cheaper with discounting .<br>
<br>
<span style="font-weight: bold;">Limitations &amp; Features:</span><br>
<br>
Unlike the Eye-One Pro, the ColorMunki only operates in a U.V. Cut
(ie. equivalent to "Ultra Violet filtered") measurement mode, due to
it using a white LED as an illuminant. This means that it is not
suitable for use with the&nbsp; Fluorescent Whitener Additive
Compensation option in Argyll (see <a href="FWA.html">here</a> for
a discussion about what FWA compensation is).<br>
<br>
It has a much larger minimum integration time than the i1Pro, and
hence has a much lower maximum brightness capability. This may
become evident in measuring very bright displays, or attempting to
measure outdoor ambient light.<br>
<br>
Like the Eye-One Pro, this instrument does support the <a
href="spotread.html#H">high resolution</a> spectral mode when used
with the ArgyllCMS driver.<br>
<br>
There are some OEM versions of this instrument around too, and
the&nbsp;<a href="http://www.office.xerox.com/latest/78XDS-03U.PDF">XEROX
PhaserMeter</a> instruments (part of the Xerox PhaserMatch 5.0
package) are also reported to work.<br>
<br>
<span style="font-weight: bold;">OS X and X-Rite drivers</span><br>
<br>
Please note the installation <a
href="Installing_OSX.html#ColorMunki">instructions</a>.<br>
<br>
<span style="font-weight: bold;">Tips &amp; Tricks:<br>
<br>
</span>In handling the instrument when about to make a reading, be
very careful not to accidentally press the switch - it is large and
easily pressed by accident. A guide of some sort (ie. a plastic
ruler) can help a lot in&nbsp; keeping the instrument over a line
of&nbsp; patches. <br>
<br>
<span style="font-weight: bold;">Patch recognition:</span><br>
<br>
For the best chances of good patch recognition, the instrument
should be drawn smoothly and not too rapidly over the strip. (This
can be a little tricky due to the two small rubber feet on the
bottom of the device that aid its spot reading guide.) If there is a
misread, try slowing down slightly. Generally a higher quality set
of readings will result if slower scans are used, since there will
then be more samples averaged for each patch. <br>
<br>
In <a href="chartread.html">chartread</a>, the -<span
style="font-weight: bold;">T ratio</span> argument modifies the
patch consistency tolerance threshold for the ColorMunki. In
recognizing patches in a strip, the instrument takes multiple
readings as the strip is read, and then divide the readings up into
each patch. It then check the consistency of the multiple readings
corresponding to each patch, and reject the measurement if they are
too inconsistent. For some media (ie. a coarser screens, fabric
etc.) the default tolerance may be unreasonably tight, so the <span
style="font-weight: bold;">-T ratio</span> argument can be used to
modify this criteria. To loosen the tolerance, use a number greater
than 1.0 (ie. 1.5, 2.0). <br>
<br>
Note that <a href="printtarg.html">printtarg</a> provides the <a
href="printtarg.html#h">-h</a> option that allows the choice of
two different patch row widths with ColorMunki test charts. [Some
people have successfully used the i1Pro patch layout with the
ColorMunki, by making a guide to keep it over the much narrower
patchs.]<br>
<br>
<b>Native Calibration Standard:</b><br>
<br>
Reflection measurements are natively X-Rite <a href="XRGA.html">XRGA</a>.<br>
<span style="font-weight: bold;"></span><br>
<span style="font-weight: bold;"><span style="font-weight: bold;"></span></span><span
style="font-weight: bold;"></span><br>
<span style="font-weight: bold;"><span style="font-weight: bold;"></span></span>
<hr style="width: 100%; height: 2px;"><span style="font-weight:
bold;"><br>
<a name="DTP20"></a></span><span style="font-weight: bold;">DTP20
"Pulse" reflective spectrometer<br>
<br>
</span><span style="font-weight: bold;"><img title="DTP20" alt=""
src="DTP20.jpg" style="width: 304px; height: 210px;"><br>
<br>
</span><span style="font-weight: bold;">Availability:<br>
<br>
</span>The <span style="font-weight: bold;">DTP20</span> from <a
href="http://www.xrite.com/">X-Rite</a> was discontinued during
2007, but may still be available from old stock or second hand. <br>
<br>
<span style="font-weight: bold;">Special features:</span><br>
<br>
The <span style="font-weight: bold;">DTP20</span> has a couple of
unique features that Argyll can take advantage of. One is that it
can operate un-tethered (off line). A whole chart can be read
un-tethered by first clearing any previous readings in the
instrument, then reading the chart TID strip, before reading all the
other strips. The instrument can then be connected up to <span
style="font-weight: bold;">chartread</span>, which will recognize
the chart, and download all the measurements.<br>
If there is no chart in the instrument when chartread connects to
it, then it will use the strip by strip tethered mode, just like the
other strip instruments. If the right number of spot readings are
present in the instrument, these will be used by <span
style="font-weight: bold;">chartread</span> too.<br>
<br>
Un-tethered spot measurements can also be read in using&nbsp; <span
style="font-weight: bold;">spotread</span>, which will notice the
stored readings, and offer to print them out, or they can be
ignored, and tethered readings taken. This will clear any saved spot
readings.<br>
<br>
<span style="font-weight: bold;">Note</span> that tethered (on-line)
strip reading will only work if the firmware in the device is
version 1.03 or greater. You can check the firmware version by
running with the verbose option: <span style="font-weight: bold;">-v<br>
<br>
Chart printing:<br>
<span style="font-weight: bold;"><br>
</span></span>Because the DTP20 measures exact distances using the
markings on its ruler, it's critical that the chart be printed out
exactly the right size. If the chart gets re-sized at all in the
process of printing it, the DTP20 is likely to fail in reading it.
If you have a problem with this, you might want to increase the page
margins using the <span style="font-weight: bold;">printtarg -m</span>
parameter, or find a printing path that preserves the test chart
size correctly.<br>
<br>
<span style="font-weight: bold;"><span style="font-weight: bold;"></span></span><span
style="font-weight: bold;">Operation:<br>
<br>
</span>When reading in tethered (on-line) mode, that the instrument
takes <span style="font-weight: bold;">several seconds</span> to
download the measurements after each strip, and that the indicator
will be in "rainbow" mode while this occurs. <span
style="text-decoration: underline;">Wait</span> until the
indicator turns solid green again before starting to measure the
next strip.<br>
<br>
To <span style="font-weight: bold;">reset</span> the instrument and
clear any stored readings: press the button three times in quick
succession. The indicator will turn solid blue. Then hold the button
down until the instrument beeps and the indicator goes out. Release
the button and the indicator should flash then return to solid green
(ready).<br>
<br>
To <span style="font-weight: bold;">calibrate</span> the
instrument, place it on its calibration tile, then press the button
three times in quick succession.The indicator will turn solid blue.
Click the button another three times in quick succession, and the
indicator should turn yellow. Then hold the button down until the
instrument beeps and the indicator goes out. Release the button and
the instrument should flash and then turn solid green.<br>
<br>
If the chart is particularly <span style="font-weight: bold;">small</span>,
the patches may end up printed very close to the edge of the chart,
and therefore it may be difficult to confine your scan to the chart,
and passing<br>
the instrument over the edge of the chart may prevent it reading
successfully. One way of working around this is to place the chart
on a larger piece of paper of the same type.<br>
<br>
The <span style="font-weight: bold;">speed</span> of scan can be
quite critical with this instrument. In particular, it doesn't work
very well if the scan is too <span style="font-weight: bold;">slow</span>.
You don't want to go too fast either, as this reduces the number of
samples per patch.<br>
<br>
<b>Native Calibration Standard:</b><br>
<br>
Reflection measurements are natively historical X-Rite standard
(XRDI).<br>
<br>
<span style="font-weight: bold;"><span style="font-weight: bold;"></span></span><span
style="font-weight: bold;"></span><br>
<span style="font-weight: bold;"><span style="font-weight: bold;"></span></span>
<hr style="width: 100%; height: 2px;"><span style="font-weight:
bold;"><br>
<a name="DTP22"></a></span><span style="font-weight: bold;">DTP22
Digital Swatchbook reflective spectrometer</span><br>
<span style="font-weight: bold;"><br>
<img alt="" src="DTP22.jpg" style="width: 222px; height: 193px;"><br>
<br>
</span><span style="font-weight: bold;">Availability:<br>
<br>
</span>The <span style="font-weight: bold;">DTP22</span> from <a
href="http://www.xrite.com/">X-Rite</a> is a discontinued
instrument.&nbsp; It may still be available second hand. It is
capable of reading colored patches one at a time.<br>
<br>
<b>Native Calibration Standard:</b><br>
<br>
Reflection measurements are natively historical X-Rite standard
(XRDI).<br>
<br>
<br>
<span style="font-weight: bold;"><span style="font-weight: bold;"></span></span>
<hr style="width: 100%; height: 2px;"><span style="font-weight:
bold;"><br>
<a name="DTP41"></a>DTP41 reflective, DTP41T
reflective/transmissive spectrometers<br>
<br>
<img alt="" src="DTP41.jpg" style="width: 263px; height: 298px;"><br>
<br>
</span><span style="font-weight: bold;">Availability:<br>
<br>
</span>The <span style="font-weight: bold;">DTP41</span> and <span
style="font-weight: bold;">DTP41T</span> from <a
href="http://www.xrite.com/">X-Rite</a> is a discontinued
instrument.&nbsp; It may still be available second hand. <br>
<br>
The series II instruments (<span style="font-weight: bold;">DTP41B</span>
and <span style="font-weight: bold;">DTP41TB</span>) offer both
serial and USB connection. Note that currently only serial operation
using Argyll is possible with these instruments.<br>
<br>
<b>Native Calibration Standard:</b><br>
<br>
Reflection measurements are natively historical X-Rite standard
(XRDI).<br>
<br>
<hr style="width: 100%; height: 2px;"><br>
<a name="dtp51"></a><span style="font-weight: bold;">DTP51
reflective colorimeter<br>
<br>
<img alt="" src="DTP51.jpg" style="width: 263px; height: 223px;"><br>
<br>
</span><span style="font-weight: bold;">Availability:<br>
<br>
</span>The <span style="font-weight: bold;">DTP51</span> from <a
href="http://www.xrite.com/">X-Rite</a> is a discontinued
instrument.&nbsp; It may still be available second hand. <br>
<br>
<span style="font-weight: bold;">Operation:</span><br>
<span style="font-weight: bold;"><span style="font-weight: bold;"><br>
</span></span>The DTP51's switch is triggered by inserting a strip
into the slot.<br>
<br>
<b>Native Calibration Standard:</b><br>
<br>
Reflection measurements are natively historical X-Rite standard
(XRDI).<br>
<br>
<br>
<span style="font-weight: bold;"><span style="font-weight: bold;"></span></span>
<hr style="width: 100%; height: 2px;"><span style="font-weight:
bold;"><br>
<a name="DTP92"></a>DTP92 CRT display colorimeter<br>
<br>
<img alt="" src="DTP92.jpg" style="width: 223px; height: 180px;"><br>
<br>
</span><span style="font-weight: bold;">Availability:<br>
<br>
</span>The <span style="font-weight: bold;">DTP92</span><span
style="font-weight: bold;"></span> from <a
href="http://www.xrite.com/">X-Rite</a> is a discontinued
instrument.&nbsp; It may still be available second hand. It will
only read CRT technology displays.<br>
<br>
<span style="font-weight: bold;">Operation:</span><br>
<br>
The Display Selections for this instrument are:<br>
<br>
&nbsp;&nbsp;&nbsp; <span style="font-weight: bold;">c</span>&nbsp;&nbsp;&nbsp;
CRT display&nbsp;&nbsp;&nbsp; &nbsp;&nbsp;&nbsp;&nbsp; A Cathode Ray
Tube display, that is of the Refresh type [Default, CB2].<br>
<br>
<hr style="width: 100%; height: 2px;"><br>
<span style="font-weight: bold;"><a name="DTP94"></a>DTP94, </span><font
size="-1">"Optix XR"</font> or "Optix XR2" or "Optix Pro" <span
style="font-weight: bold;">display colorimetrers</span><br>
<span style="font-weight: bold;"><br>
<img title="DTP94" alt="" src="DTP94.jpg" style="width: 138px;
height: 171px;"> &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;
&nbsp; &nbsp; <img alt="" title="Optix XR/Pro" src="moxxr.jpg"
style="width: 155px; height: 190px;"><br>
<br>
</span><span style="font-weight: bold;">Availability:<br>
<br>
</span>The <span style="font-weight: bold;">DTP94 </span>from <a
href="http://www.xrite.com/">X-Rite</a> is a discontinued
instrument, although it is still being supplied to OEMs.&nbsp; It
may still be available as old stock, or second hand. It was sold as
an instrument without software as the DTP94, and packaged with
software from the manufacturer as the "Optix XR" range.<br>
<br>
<span style="font-weight: bold;">Operation:</span><br>
<br>
The Display Selections for this instrument are:<br>
<br>
&nbsp;&nbsp;&nbsp; <span style="font-weight: bold;">l</span>&nbsp;&nbsp;&nbsp;&nbsp;
LCD display&nbsp;&nbsp;&nbsp; &nbsp;&nbsp;&nbsp;&nbsp; A Liquid
Crystal Display, that is of the Non-Refresh type [default, CB1].<br>
&nbsp;&nbsp;&nbsp; <span style="font-weight: bold;">c</span>&nbsp;&nbsp;&nbsp;
CRT display&nbsp;&nbsp;&nbsp; &nbsp;&nbsp;&nbsp;&nbsp; A Cathode Ray
Tube display, that is of the Refresh type [CB2].<br>
&nbsp;&nbsp;&nbsp; <b>g</b>&nbsp;&nbsp;&nbsp;
Generic&nbsp;&nbsp;&nbsp;
&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; Generic
display [CB3]<br>
&nbsp;&nbsp; <br>
<br>
<span style="font-weight: bold;"></span>
<hr style="width: 100%; height: 2px;"><span style="font-weight:
bold;"><br>
<a name="sl"></a>Spectrolino reflective/emissive spectrometer<br>
<br>
<img alt="" src="sl.jpg" style="width: 239px; height: 200px;"><br>
<br>
</span><span style="font-weight: bold;">Availability:<br>
<br>
</span>The <span style="font-weight: bold;">Spectrolino </span>from
Gretag
MacBeth (Now X-Rite) is a discontinued instrument. It is often
available second hand. If buying it second hand, make sure it comes
with all it's accessories, including white reference, spot reading
adapter, display reading adapters, filters (UV, polarizing, D65),
serial cable adapter and power supply.<br>
<br>
<b>Native Calibration Standard:</b><br>
<br>
Reflection measurements are natively historical Gretag MacBeth
standard (GMDI).<br>
<span style="font-weight: bold;"><br>
</span>
<hr style="width: 100%; height: 2px;"><span style="font-weight:
bold;"><br>
<a name="ss"></a>SpectroScan reflective/emissive and SpectroScanT
reflective/emissive/transmissive spectrometers<br>
<br>
<img style="width: 336px; height: 294px;" alt="" src="ss.jpg"><br>
<br>
</span><span style="font-weight: bold;">Availability:<br>
<br>
</span>The <span style="font-weight: bold;">SpectroScan</span> and
<span style="font-weight: bold;">SpectroScanT</span> from Gretag
MacBeth (Now X-Rite) is a discontinued instrument. It is the
combination of an X-Y table and the <span style="font-weight:
bold;">Spectrolino</span> instrument. The <span
style="font-weight: bold;">SpectroScanT</span> is capable of
measuring transparency. It is often available second hand. If buying
it second hand, make sure it comes with all it's accessories,
including white reference, spot reading adapter, display reading
adapters, filters (UV, polarizing, D65) and power supply.<br>
<br>
If measuring transparencies using a SpectroScanT, the <b>Enter</b>
key on the instrument may be used to trigger each reading. It will
be recognized after each previous reading has been completed.<br>
<br>
<b>Native Calibration Standard:</b><br>
<br>
Reflection measurements are natively historical Gretag MacBeth
standard (GMDI).<br>
<br>
<br>
<hr style="width: 100%; height: 2px;"><span style="font-weight:
bold;"><br>
<a name="i1p3"></a>i1Pro3:</span><span style="font-weight: bold;"><br>
<br>
<img src="i1Pro3.jpg" alt="i1 Pro 3" width="429" height="295"><br>
<br>
</span><span style="font-weight: bold;">Availability:<br>
<br>
</span> The <span style="font-weight: bold;">i1Pro3 </span>(standard
aperture) and <b>i1Pro3 Plus</b> (large aperture, polarizing
filter) from&nbsp; <a href="http://www.xrite.com/">X-Rite</a> are
currently available instruments. They are available in several
packages from the manufacturer. These packages differ partly in what
accessories come with the instrument, but primarily in what features
the manufacturers software provides. Used with ArgyllCMS, there are
no differences in operation of an i1Pro3 instrument, irrespective of
which package it came with. The lowest cost package is the <a
href="https://www.xrite.com/categories/calibration-profiling/i1basic-pro-3">i1
Basic Pro 3</a>. The lowest cost large aperture instrument is the
<a
href="https://www.xrite.com/categories/calibration-profiling/i1basic-pro-3-plus">i1
Basic Pro3 Plus</a>.<br>
<br>
All features of the i1Pro3 are supported by the ArgyllCMS driver:<br>
<br>
&nbsp;&nbsp;&nbsp; Reflective spot &amp; scan Measurement mode.<br>
&nbsp;&nbsp;&nbsp; Emissive/Display spot &amp; scan Measurement
mode.<br>
&nbsp;&nbsp;&nbsp; Transmission spot &amp; scan Measurement mode
when used with a light table or equivalent.<br>
&nbsp;&nbsp;&nbsp; Ambient spot &amp; flash Measurement mode.<br>
&nbsp;&nbsp;&nbsp; Zebra ruler assisted scan measurement.<br>
<br>
For reflective measurement, filters none/M0 (default, flag -Fn),
D50/M1 (flag -F5) and UV cut/M2 (flag -Fu) are supported.<br>
For the i1Pro3 Plus, Polarized spot &amp; scan measurement mode
(flag -Fp) mode is also supported.<br>
When used with the zebra ruler, a scan can be repeated several times
to increase the total number of measurements per patch.<br>
<br>
In addition, these ArgyllCMS specific features are supported:<br>
<br>
&nbsp;&nbsp;&nbsp; High-resolution mode for all measurement modes
except reflection measurement.<br>
&nbsp;&nbsp;&nbsp; Refresh rate measurement.<br>
&nbsp;&nbsp;&nbsp; Display update delay measurement.<br>
<br>
Agreement between the CIE values from the ArgyllCMS driver and the
Manufacturers driver is typically within 0.05 delta E or better.<br>
Note that for the highest accuracy and agreement with the
Manufacturers CIE measurement values, standard resolution mode
should be used.<br>
High resolution mode is most useful in the context of spectral
plots.<br>
<br>
There are a number of OEM Eye-One Pro3's (i.e. The EFI ES-3000)<b>,</b>
but beware that they may may be missing features that are standard
in the retail version of the instrument. <br>
<br>
See <a href="instruments.html#i1p">Eye-One Pro reflective/emissive
spectrometer</a><span style="font-weight: bold;"> </span>below
for details on the operation of this type of instrument.<br>
<br>
<hr style="width: 100%; height: 2px;"><span style="font-weight:
bold;"><br>
<a name="i1p2"></a>i1Pro2:</span><span style="font-weight: bold;"><br>
<br>
</span> <img style=" width: 357px; height: 234px;" alt="Eye-One Pro
2" src="i1pro2.jpg"><br>
<br>
<span style="font-weight: bold;">Availability:<br>
<br>
</span> The <span style="font-weight: bold;">i1Pro2 </span>(AKA
Eye-One Pro Rev E) from&nbsp; <a href="http://www.xrite.com/">X-Rite</a>
is a discondinued instrument, but may be available second hand. It
was available in several packages from the manufacturer. These
packages differ partly in what accessories come with the instrument,
but primarily in what features the manufacturers software provides.
This comparison <a
href="http://www.xrite.com/product_overview.aspx?ID=812">chart</a>
illustrates the differences. Used with Argyll, there are no
differences in operation of an Eye-One Pro instrument, irrespective
of which package it came with. The lowest cost package is the <a
href="http://www.xrite.com/categories/calibration-profiling/i1basic-pro-2">i1
Basic Pro 2</a>.<br>
<br>
There is support for some of the new features of the Eye-One Pro2
(also known as the Eye-One Pro Rev E), in particular the&nbsp; Rev E
measurement mode, spectrometer stray light reduction, wavelength
calibration, and improved black level tracking. Note that there is
no support currently for using the Eye-One Pro2 Ultra Violet
measurement mode, since ArgyllCMS can simulate M0/M1/M2 measurement
modes using both older (Rev A-D) and newer instruments without this.
The new support can be disabled and an Eye-One Pro2 operated in
legacy mode by setting the environment variable
ARGYLL_DISABLE_I1PRO2_DRIVER. See <a href="instruments.html#i1p">Eye-One
Pro reflective/emissive spectrometer</a><span style="font-weight:
bold;"> </span>below for details on the operation of this type of
instrument.<br>
<br>
<b>OEM models:<br>
<br>
</b>The retail Eye-One Pro2 has the part number <b>EO2-XR-ULZW</b>,
but there are a number of OEM Eye-One Pro2's (i.e. The EFI ES-2000)
that appear from time to time with the part number <b>EO2-XR-UF</b>
that are missing most of the features that are new to this model. In
particular they are fitted with an Ultra Violet filter and therefore
can only make M2 measurements, they are missing Ambient light
measurement capabilities, they are missing the UV illumination LED
(which would be useless given the UV filter anyway), they are
missing the Zebra stripe ruler sensor needed to make use of the UV
LED, and they are missing the automatic Wavelength Calibration
capability. They appear to be replacement models for the original
Eye-One Pro Rev A-D OEM models. If you are buying an Eye-One Pro2
second hand, be aware of which model you are getting - you should be
paying a lot less for the <b>EO2-XR-UF</b> compared to the full
retail model.<br>
<b></b> <br>
<b>Native Calibration Standard:</b><br>
<br>
Reflection measurements are natively X-Rite <a href="XRGA.html">XRGA</a>.<span
style="font-weight: bold;"></span><br>
<br>
<hr style="width: 100%; height: 2px;"><br>
<span style="font-weight: bold;"><a name="i1p"></a>Eye-One Pro
reflective/emissive spectrometer<br>
<br>
<img alt="" src="i1p.jpg" style="width: 347px; height: 234px;"><br>
<br>
</span><span style="font-weight: bold;">Availability:<br>
<br>
</span>The <span style="font-weight: bold;">Eye-One Pro</span> from
<a href="http://www.xrite.com/">X-Rite</a> (was Gretag MacBeth) is a
discontinued instrument, but may be available second hand.<br>
<br>
The EFI ES-1000 (which is a re-badged Eye-One Pro) is also reported
to work with Argyll, but may be missing certain accessories, and may
not support Ambient mode. It may or may not be a UV cut instrument.<br>
<br>
Unless you know what you're doing, and have a very specific reason
to buy an instrument fitted with a UV (Ultra Violet) filter, make
sure that you buy an instrument without the filter. A UV filtered
instrument can't deal intelligently with FWA (Fluorescent Whitener
Additive) effects in paper. (Look <a href="FWA.html">here</a> for
more information about FWA compensation.) Using FWA compensation you
can make measurements using ISO 13655:2009 M0, M1 and M2 conditions.
The M2 condition emulates a UV cut instrument.<br>
<br>
There have been four revisions of the Eye-One Pro, Rev. A, B, D and
E (AKA Eye-One Pro2 - see above). The rev B, D and E are capable of
sampling twice as fast as the Rev. A version of the instrument, and
are also available with an ambient light reading capability.<br>
<br>
<span style="font-weight: bold;">NOTE</span> for those running on
older versions of Linux with a Rev. D, there was a problem with the
Linux USB stack that causes the instrument to stop working once it
has been used. The only workaround is to unplug and replug the
instrument in again, whereupon it can be used one time again. A fix
for this problem was in the&nbsp; Linux 2.6.26 kernel release.<br>
<br>
See also <a href="i1proDriver.html">How can I have confidence in
the i1pro Driver ?</a><br>
<br>
<span style="font-weight: bold;">Patch recognition:</span><br>
<br>
For the best chances of good patch recognition, the instrument
should be drawn smoothly and not too rapidly over the strip. If
there is a misread, try slowing down slightly. The Rev A and B.
instruments have a slower sampling rate than the latter revision
instruments, and hence must be used a bit more slowly. Generally a
higher quality set of readings will result if slower scans are used,
since there will then be more samples averaged for each patch.<br>
<br>
In <a href="chartread.html">chartread</a>, the -<span
style="font-weight: bold;">T ratio</span> argument modifies the
patch consistency tolerance threshold for the Eye-One Pro. In
recognizing patches in a strip, the instrument takes multiple
readings as the strip is read, and then divide the readings up into
each patch. It then check the consistency of the multiple readings
corresponding to each patch, and reject the measurement if they are
too inconsistent. For some media (ie. a coarser screens, fabric
etc.) the default tolerance may be unreasonably tight, so the <span
style="font-weight: bold;">-T ratio</span> argument can be used to
modify this criteria. To loosen the tolerance, use a number greater
than 1.0 (ie. 1.5, 2.0). <span style="font-weight: bold;"></span><br>
<br>
<b>Native Calibration Standard:</b><br>
<br>
Reflection measurements are natively historical Gretag MacBeth
standard (GMDI) for RevA-D,<br>
and&nbsp; natively X-Rite <a href="XRGA.html">XRGA</a> for Rev E.<br>
<br>
<span style="font-weight: bold;">Special features:</span><br>
<br>
A feature unique to Argyll when used with the Eye-One Pro, is the
high resolution spectral mode. This returns spectral measurements at
3.333 nm spacing, rather than the default 10nm spacing, and also
extends the range of wavelengths very slightly. This high resolution
may assist in giving better accuracy for "peaky" emissive sources
such as illuminants and displays. The high resolution mode is
selected by using the <span style="font-weight: bold;">-H</span>
flag on the command line to <span style="font-weight: bold;">dispcal</span>,
<span style="font-weight: bold;">dispread</span>, <span
style="font-weight: bold;">chartread</span>, and <span
style="font-weight: bold;">spotread</span>. It can also be toggled
on and off within <span style="font-weight: bold;">spotread</span>
using the <span style="font-weight: bold;">h</span> key.<br>
<br>
Note that while finer spectral resolution will worsen the signal to
noise ratio of the individual spectral values, the signal to noise
ratio of the resulting tri-stimulus color values will be identical
to normal resolution mode, since the same overall integration is
performed. <br>
<br>
See <a href="i1proHiRes.html">Does the i1pro High Resolution mode
improve accuracy ?</a><br>
<br>
<img alt="High res. and standard res. spectrum."
src="Fluorescent.jpg" style="width: 750px; height: 375px;"><br>
<br>
<img alt="C.R.T high res. and standard res. spectrum."
src="CRTspectrum.jpg" style="width: 750px; height: 375px;"><br>
<br>
<hr style="width: 100%; height: 2px;"><br>
<span style="font-weight: bold;"><a name="i1m"></a>Eye-One Monitor
emissive spectrometer<br>
<br>
<img alt="" src="i1m.jpg" style="width: 347px; height: 234px;"><br>
<br>
</span><span style="font-weight: bold;">Availability:<br>
<br>
</span>The <span style="font-weight: bold;">Eye-One Monitor</span>
from <a href="http://www.xrite.com/">X-Rite</a> (was Gretag
MacBeth) is a discontinued instrument. It was a lower cost version
of the <span style="font-weight: bold;">Eye-One Pro</span> without
reflective measurement capability. See <a href="#i1p">Eye-One Pro
reflective/emissive spectrometer</a><span style="font-weight:
bold;"> </span>for details on the operation of this instrument.<br>
<br>
<br>
<hr style="width: 100%; height: 2px;"><br>
<span style="font-weight: bold;"><a name="i1d"></a>Eye-One Display
1, Eye-One Display 2, Eye-One Display LT, ColorMunki Create,
ColorMunki Smile colorimeters,<br>
<br>
<img style=" width: 124px; height: 168px;" alt="ColorMunki Smile"
src="Smile.jpg"><img alt="Eye-One Display 2" src="i1d.jpg"
style="width: 145px; height: 168px;"> <img style="width: 133px;
height: 168px;" alt="ColorMunki Create"
src="ColorMunkiCreate.jpg"><br>
<br>
Instrument Availability:<br>
<br>
</span>The <span style="font-weight: bold;">ColorMunki Smile</span>
colorimeter is a currently available instrument.<br>
The <span style="font-weight: bold;">Eye-One Display LT</span> and
<span style="font-weight: bold;">Eye-One Display 2</span> are
discontinued products, although they may still be available from
some retailers, second hand, and may still be shipped with some
displays as part of their calibration capability.<br>
The <span style="font-weight: bold;">ColorMunki Create</span>
colorimeter is a discontinued product, although they may still be
available from some retailers or second hand,can also be used. They
will appear as an i1Display2 colorimeter.<br>
The <span style="font-weight: bold;">HP DreamColor</span>
colorimeter can also be used, and will appear as an i1Display2
colorimeter [note that it is calibrated for the DreamColor display].<br>
The <span style="font-weight: bold;">HP APS</span> (Advanced
Profiling Solution) colorimeter is also reported to work, and will
appear as an i1Display2.<br>
The <span style="font-weight: bold;">CalMAN X2</span> colorimeter
is also reported to work, and will appear as an i1Display2
colorimeter.<br>
The&nbsp; <span style="font-weight: bold;">Lacie Blue Eye</span> <span
style="font-weight: bold;"></span> colorimeter is also reported to
work, and will appear as an i1Display2 colorimeter.<br>
<br>
<span style="font-weight: bold;"></span>The <span
style="font-weight: bold;">Eye-One Display 1</span> is a
discontinued instrument. <br>
<br>
The Eye-One Display LT came with a less expensive<span
style="text-decoration: underline;"></span> package with more
limited software from the manufacture.<br>
The Eye-One Display 2 package came with more software
features,&nbsp; but the instruments are virtually identical, and
will operate identically using Argyll.<br>
The ColorMunki Create<span style="text-decoration: underline;"></span>
package is another alternative, and will operate identically using
Argyll.<br>
<br>
<span style="font-weight: bold;">Operation:</span><br>
<br>
The Display Selections for the <span style="font-weight: bold;">ColorMunki
Smile</span> are:<br>
<br>
&nbsp;&nbsp;&nbsp; <span style="font-weight: bold;">f</span>
&nbsp;&nbsp; LCD with CCFL back-light&nbsp;&nbsp;&nbsp;
&nbsp;&nbsp;&nbsp;&nbsp; A Liquid Crystal display that uses a Cold
Cathode Fluorescent back lighting. [Default, CB1]<br>
&nbsp;&nbsp;&nbsp; <span style="font-weight: bold;">e</span>&nbsp;&nbsp;&nbsp;
LCD with LED back-light&nbsp;&nbsp;&nbsp;
&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; A Liquid Crystal display that uses
Light Emitting Diode back lighting.<br>
<br>
other instruments will offer:<br>
<br>
&nbsp;&nbsp;&nbsp; <span style="font-weight: bold;">l</span>&nbsp;&nbsp;&nbsp;&nbsp;
LCD display&nbsp;&nbsp;&nbsp; &nbsp;&nbsp;&nbsp;&nbsp; A Liquid
Crystal Display, that is of the Non-Refresh type. [Default, CB1]<br>
&nbsp;&nbsp;&nbsp; <span style="font-weight: bold;">c</span>&nbsp;&nbsp;&nbsp;
CRT display&nbsp;&nbsp;&nbsp; &nbsp;&nbsp;&nbsp;&nbsp;&nbsp; A
Cathode Ray Tube display, that is of the Refresh type. [CB2]<br>
<br>
<br>
<hr style="width: 100%; height: 2px;"><br>
<span style="font-weight: bold;"><a name="i1d3"></a></span>&nbsp; <span
style="font-weight: bold;">i1 DisplayPro and ColorMunki Display<span
style="font-weight: bold;"> colorimeters (i1 Display 3)</span><br>
<br>
<img alt="i1 Display Pro" src="i1d3_1.jpg" style="width: 194px;
height: 223px;"> <img style="width: 176px; height: 222px;"
alt="ColorMunki Display" src="i1d3_2.jpg"><br>
<br>
Instrument Availability:<br>
<br>
</span>Both instruments are currently available.<br>
<br>
The ColorMunki Display is a less expensive <a
href="http://xritephoto.com/ph_product_overview.aspx?id=1513&amp;catid=149">package</a>
with more limited software from the manufacture, and has hardware
that takes a noticeably longer time to make most measurements (a
minimum of 1 second), but both instruments will take longer for very
dark samples, and under these conditions the speed difference is
less significant. Because of the measurement speed limitation, the
measurement of display refresh rate and synchronization of its
measurements to a refresh display is not possible with the
ColorMunki Display. <br>
<br>
The i1Display Pro <a
href="http://xritephoto.com/ph_product_overview.aspx?id=1454&amp;catid=109">package</a>
comes with i1Profiler, and the instrument is generally faster than
the ColorMunki Display, but other than this and the software
package, the instruments appear to be virtually identical. (Note
though that the ColorMunki Display is <u>unable</u> to measure the
refresh period, so is less repeatable in this mode than the
i1Display Pro).<br>
<br>
Both instruments are capable of using CCSS (<a
href="File_Formats.html#ccss">Colorimeter Calibration Spectral
Sample</a>) files, and this also gives the instrument the
capability of using a non-default standard observer. CCSS files can
be created using the <a href="ccxxmake.html">ccxxmake</a> tool, and
installed or translated from the .EDR files that are provided with
the instrument CD using the <a href="oeminst.html">oeminst</a>
utility using a spectrometer as a reference.<br>
<br>
There are some OEM versions of this instrument around too, and the <a
href="http://www.spectracal.com/">SpectraCal OEM i1Display</a>, <a
href="http://www.chromapure.com/">ChromaPure</a>, <a
href="http://www.necdisplay.com/p/sensors/mdsvsensor3">NEC
SpectraSensor Pro</a>, <a
href="http://www8.hp.com/us/en/products/oas/product-detail.html?oid=5225568">HP
DreamColor</a> and <a
href="https://us-store.wacom.com/Catalog/Accessories/wacom-color-manager">Wacom
Color Manager</a> instruments are also reported to work. They will
appear as a be a the same as the i1Display Pro. There are
unconfirmed reports that the ASUS branded instrument will also work.<br>
<span style="font-weight: bold;">[Note</span> that if you have an
OEM version of this instrument, it's worth checking if they come
with any extra .edr files, that can then be translated for use with
ArgyllCMS using <a href="oeminst.html">oeminst</a>.]<br>
<br>
On MSWindows, if you have installed the Manufacturers applications,
you may have to shut the i1Profiler tray application down before
Argyll can open the instrument.<br>
<br>
<span style="font-weight: bold;">Operation:</span><br>
<br>
The Display Selections for this instrument are:<br>
<br>
&nbsp;&nbsp;&nbsp; <span style="font-weight: bold;">n</span><span
style="font-weight: bold;"></span>&nbsp;&nbsp;&nbsp;&nbsp; A
non-refresh type display [Default, CB1].<br>
&nbsp;&nbsp;&nbsp; <span style="font-weight: bold;">r</span>
&nbsp;&nbsp;&nbsp; A refresh type display&nbsp; - The refresh period
is measured, and the integration time adjusted appropriately. [CB2]<br>
<br>
With the manufacturers .edr files &amp; reference Argyll .ccss files
installed, the following selections are:<br>
<br>
&nbsp;&nbsp;&nbsp; <span style="font-weight: bold;">n</span><span
style="font-weight: bold;"></span>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; A
non-refresh type display [Default, CB1].<br>
&nbsp;&nbsp;&nbsp; <span style="font-weight: bold;">r</span>
&nbsp;&nbsp;&nbsp;&nbsp; A refresh type display&nbsp; - The refresh
period is measured, and the integration time adjusted appropriately.
[CB2]<br>
&nbsp;&nbsp;&nbsp; <b>c</b>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; CRT
(Hitachi CM2112MET, Diamond View 1772ie)<br>
&nbsp;&nbsp;&nbsp; <b>l</b> &nbsp;&nbsp;&nbsp;&nbsp;&nbsp; LCD CCFL
IPS (CCFL AC EIZO HP with CORRECTION)<br>
&nbsp;&nbsp;&nbsp; <b>L</b>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; LCD CCFL
Wide Gamut IPS (WG CCFL NEC241 271)<br>
&nbsp;&nbsp;&nbsp; <b>b&nbsp;</b>&nbsp;&nbsp;&nbsp;&nbsp; LCD RGB
LED IPS (RGBLED HP SOYO)<br>
&nbsp;&nbsp;&nbsp; <b>e</b>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; LCD White
LED IPS (WLED AC LG Samsung)<br>
&nbsp;&nbsp;&nbsp; <b>p</b>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; Projector
(Marantz HP Panasonic Projectors Hybrid EDR)<br>
<br>
By default the integration time is adaptive, taking longer when the
light level is low. This can be disabled and a fixed integration
time used to gain maximum speed at the cost of greatly reduced low
light accuracy, by using the -Y A flag.<br>
<br>
<b>Note when measuring CRT displays:<br>
</b><br>
The small magnet in the ambient light cover used to signal what
position it is in, can interfere in the operation of the CRT
display, particularly if the ambient cover is in it's natural
position at 180 degrees away from the measuring lens. One way of
minimizing this is to swing the cover down so that it touches the
display adjacent to the lens, thereby moving the magnet away from
the display surface. A more thorough but inconvenient way of
avoiding this problem is to unclip the ambient light cover and slide
it down the cable.<br>
<br>
<hr style="width: 100%; height: 2px;"><br>
<span style="font-weight: bold;"><a name="Huey"></a>Huey colorimeter<br>
<br>
<img alt="" src="Huey.jpg" style="width: 128px; height: 202px;"><br>
<br>
Availability:<br>
<br>
</span>The <span style="font-weight: bold;">Huey </span>and <b>Huey
Pro</b> are discontinued instruments. They may still be available
as old stock, or second hand. <br>
<span style="font-weight: bold;"></span><br>
<span style="font-weight: bold;">Operation:</span><br>
<br>
The Display Selections for this instrument are:<br>
<br>
&nbsp;&nbsp;&nbsp; <span style="font-weight: bold;">l</span>&nbsp;&nbsp;&nbsp;&nbsp;
LCD display&nbsp;&nbsp;&nbsp; &nbsp;&nbsp;&nbsp;&nbsp; A Liquid
Crystal Display, that is of the Non-Refresh type. [Default, CB1]<br>
&nbsp;&nbsp;&nbsp; <span style="font-weight: bold;">c</span>&nbsp;&nbsp;&nbsp;
CRT display&nbsp;&nbsp;&nbsp; &nbsp;&nbsp;&nbsp;&nbsp; A Cathode Ray
Tube display, that is of the Refresh type. [CB2]<br>
<br>
<br>
<hr style="width: 100%; height: 2px;"><br>
<span style="font-weight: bold;"><a name="mox"></a>MonacoOPTIX
colorimeters<br>
<br>
<img alt="" src="mox.jpg" style="width: 115px; height: 147px;">
&nbsp; &nbsp; &nbsp; &nbsp; &nbsp; <img alt="" src="Chroma4.jpg"
style="width: 135px; height: 146px;"><br>
<br>
Instrument Availability:<br>
</span><br>
<span style="font-weight: bold;">Availability:<br>
<br>
</span>The <span style="font-weight: bold;">MonacoOPTIX</span> from
Monaco Soft is a discontinued instrument.&nbsp; It may still be
available as old stock, or second hand. It was sold packaged with
software from the manufacturer. The Sequel Chroma 4 appears to be a
similar instrument, and both seem to operate as if they were an
Eye-One Display 1 using Argyll.<br>
<br>
<span style="font-weight: bold;">Operation:</span><br>
<br>
The Display Selections for this instrument are:<br>
<br>
&nbsp;&nbsp;&nbsp; <span style="font-weight: bold;">c</span>&nbsp;&nbsp;&nbsp;
CRT display&nbsp;&nbsp;&nbsp; &nbsp;&nbsp;&nbsp;&nbsp; A Cathode Ray
Tube display, that is of the Refresh type.<br>
&nbsp;&nbsp;&nbsp; <span style="font-weight: bold;">l</span>&nbsp;&nbsp;&nbsp;&nbsp;
LCD display&nbsp;&nbsp;&nbsp; &nbsp;&nbsp;&nbsp;&nbsp; A Liquid
Crystal Display or alternate Calibration, that is of the Non-Refresh
type.<br>
<br>
<hr style="width: 100%; height: 2px;"><br>
<span style="font-weight: bold;"><a name="spyd2"></a>Spyder 2
colorimeter<br>
<br>
<img alt="" src="Spyd2.jpg" style="width: 218px; height: 232px;"><br>
<br>
</span><span style="font-weight: bold;">Availability:<br>
<br>
</span>The <span style="font-weight: bold;">Spyder 2 </span><span
style="font-weight: bold;"></span>has been superseded by the
Spyder 5 and SpyderX, but may be available second hand.<br>
[The Spyder 1 has also been reported as working, but this has not
been confirmed.]<br>
<span style="font-weight: bold;"><br>
</span><span style="font-weight: bold;">Operation:<br>
</span><br>
<span style="font-weight: bold;">Important Note </span>about the
ColorVision Spyder 2 instrument support:<br>
<br>
This instrument cannot function without the driver software having
access to the vendor supplied PLD firmware pattern for it.<br>
This firmware is not provided with Argyll, since it is not available
under a compatible license.<br>
<br>
The purchaser of a Spyder 2 instrument should have received a copy
of this firmware along with their instrument, and should therefore
be able to enable the Argyll driver for this instrument by using the
<a href="oeminst.html">oeminst</a> tool.<span style="font-weight:
bold;"></span><br>
<br>
The Display Selections for this instrument are:<br>
<br>
&nbsp;&nbsp;&nbsp; <span style="font-weight: bold;">l</span>&nbsp;&nbsp;&nbsp;&nbsp;
LCD display&nbsp;&nbsp;&nbsp; &nbsp;&nbsp;&nbsp; A Liquid Crystal
Display, that is of the Non-Refresh type. [Default, CB1]<br>
&nbsp;&nbsp;&nbsp; <span style="font-weight: bold;">c</span>&nbsp;&nbsp;&nbsp;
CRT display&nbsp;&nbsp;&nbsp; &nbsp;&nbsp;&nbsp;&nbsp; A Cathode Ray
Tube display, that is of the Refresh type. [CB2]<br>
<br>
<br>
<span style="font-weight: bold;">Linux USB hub problems:<br>
<br>
</span>Note that the Spyder doesn't appear to operate at all well on
Linux if attached to a secondary USB hub. You may have such a
secondary hub built into your motherboard. If Argyll has difficulty
in reliably talking to the Spyder, try connecting it directly to the
computer rather than via a usb hub, or try using a USB port on your
computer that connects directly to a root hub. This is probably due
to a bug in the Linux EHCI driver, and a fix is due to appear in the
Linux kernel sometime after July 2011. The name of the fix is "EHCI:
fix direction handling for interrupt data toggles".<br>
<br>
<hr style="width: 100%; height: 2px;"><br>
<span style="font-weight: bold;"><a name="spyd3"></a>Spyder 3
colorimeter<br>
<br>
<img style="width: 262px; height: 220px;" alt="Spyder3"
src="Spyd3.jpg"> <img style="width: 193px; height: 220px;"
alt="Spyder3Express" src="Spyd3x.jpg"><br>
<br>
</span><span style="font-weight: bold;">Availability:<br>
<br>
</span>The <span style="font-weight: bold;">Spyder3Elite</span>, <span
style="font-weight: bold;">Spyder3Pro</span> and <span
style="font-weight: bold;">Spyder3Express</span> have being
superseded by the Spyder 5 and SpyderX, but may still stocked by
some dealers, and may be available second hand. The <span
style="font-weight: bold;">Spyder3Elite</span> and <span
style="font-weight: bold;">Spyder3Pro</span> appear to be
identical hardware with different software from the manufacturer.
The <span style="font-weight: bold;">Spyder3Express</span> lacks
the ambient sensor.<br>
<br>
[Note that this instrument doesn't seem particularly suited to
measuring CRT displays, since it no longer seems to synchronise its
readings to a CRT refresh, and you can no longer remove the LCD
filter, reducing its sensitivity compared to the Spyder 2 in CRT
mode. The Spyder 2 or one of the other instruments may be a better
choice if you particularly need to measure CRTs or Refresh
displays.]<br>
<span style="font-weight: bold;"><br>
</span><span style="font-weight: bold;">Operation:<br>
</span><br>
The ambient light sensor can be used with the <span
style="font-weight: bold;">Spyder3Elite</span> and <span
style="font-weight: bold;">Spyder3Pro</span> instruments, but is
only capable of monochrome readings.<span style="font-weight: bold;"><br>
</span><br>
The Display Selections for this instrument are:<br>
<br>
&nbsp;&nbsp;&nbsp; <span style="font-weight: bold;">n</span> | <span
style="font-weight: bold;">l</span>&nbsp;&nbsp;&nbsp;&nbsp; A
non-refresh type display [Default, CB1]<br>
&nbsp;&nbsp;&nbsp; <span style="font-weight: bold;">r | c</span>
&nbsp;&nbsp;&nbsp; A refresh type display. [CB2]<br>
<br>
<br>
<hr style="width: 100%; height: 2px;"><br>
<span style="font-weight: bold;"><a name="spyd4"></a>Spyder 4
colorimeter<br>
<br>
<img style=" width: 262px; height: 220px;" alt="Spyder4"
src="Spyd4.jpg"> <br>
<br>
</span><span style="font-weight: bold;">Availability:<br>
<br>
</span>The <span style="font-weight: bold;">Spyder4Elite</span>, <span
style="font-weight: bold;">Spyder4Pro</span> and <span
style="font-weight: bold;">Spyder4Express</span> have being
superseded by the Spyder 5 and SpyderX, but may still stocked by
some dealers, and may be available second hand.&nbsp; The <span
style="font-weight: bold;">Spyder4Elite</span> and <span
style="font-weight: bold;">Spyder4Pro</span> appear to be
identical hardware with different software from the manufacturer.
The <span style="font-weight: bold;">Spyder4Express</span> lacks
the ambient sensor.<br>
<span style="font-weight: bold;"><br>
</span><span style="font-weight: bold;">Operation:<br>
</span><br>
These instruments are capable of using using CCSS (<a
href="File_Formats.html#ccss">Colorimeter Calibration Spectral
Sample</a>) files, and this also gives the instrument the
capability of using a non-default standard observer. CCSS files can
be created using the <a href="ccxxmake.html">ccxxmake</a> tool
using a spectrometer as a reference.<br>
<br>
<span style="font-weight: bold;">Important Note </span>about the
DataColor Spyder 4 vendor display type/calibration support:<br>
<br>
This instrument does not have a full range of display type
calibration selections available without the vendor supplied
calibration data for it.<br>
This calibration data is not provided with Argyll, since it is not
available under a compatible license.<br>
You can use CCSS files as an alternative (see above), or as the
purchaser of a Spyder 4 instrument you should have received a copy
of the calibration data along with the instrument, and should
therefore be able to enable the full range of display type
selections in Argyll by using the <a href="oeminst.html">oeminst</a>
tool.<br>
<br>
The Display Selections for this instrument are:<br>
<br>
&nbsp;&nbsp;&nbsp; <span style="font-weight: bold;">n</span> | <span
style="font-weight: bold;">l</span>&nbsp;&nbsp; &nbsp;
&nbsp;&nbsp; A non-refresh type display with a generic calibration
[Default, CB1].<br>
&nbsp;&nbsp;&nbsp; <span style="font-weight: bold;">r | c</span> <span
style="font-weight: bold;"></span> &nbsp; &nbsp; &nbsp;&nbsp; A
refresh type display with a generic calibration.[CB2]<br>
<br>
The Display Selections for this instrument when the manufacturers
calibration information has been installed is:<br>
<br>
&nbsp;&nbsp;&nbsp; <span style="font-weight: bold;">n&nbsp;&nbsp; </span><span
style="font-weight: bold;"></span>&nbsp;&nbsp; &nbsp;
&nbsp;&nbsp;&nbsp;&nbsp; A non-refresh type display with a generic
calibration [Default, CB1].<br>
&nbsp;&nbsp;&nbsp; <span style="font-weight: bold;">r</span> <span
style="font-weight: bold;"></span> &nbsp; &nbsp; &nbsp;&nbsp;
&nbsp;&nbsp;&nbsp;&nbsp; A refresh type display with a generic
calibration.[CB2]<br>
&nbsp;&nbsp;&nbsp; <span style="font-weight: bold;">f &nbsp;&nbsp;
&nbsp;&nbsp;&nbsp; </span>&nbsp;&nbsp;&nbsp;&nbsp; LCD, CCFL
Backlight&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
- normal gamut Liquid Crystal Display with standard Cold Cathode
Fluorescent Lamp backlight.<br>
&nbsp;&nbsp;&nbsp; <span style="font-weight: bold;">L</span>&nbsp;
&nbsp;&nbsp;&nbsp; &nbsp;&nbsp;&nbsp; &nbsp; Wide Gamut LCD, CCFL
Backlight&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; - wide gamut Liquid Crystal
Display with Cold Cathode Fluorescent Lamps backlight.<br>
&nbsp;&nbsp;&nbsp; <span style="font-weight: bold;">e</span>
&nbsp;&nbsp; &nbsp;&nbsp;&nbsp; &nbsp;&nbsp;&nbsp;&nbsp; LCD, White
LED Backlight&nbsp;&nbsp;&nbsp; &nbsp;&nbsp;&nbsp;
&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; - normal
gamut Liquid Crystal Display with a White LED backlight.<br>
&nbsp;&nbsp;&nbsp; <span style="font-weight: bold;">B</span>&nbsp;&nbsp;
&nbsp;&nbsp;&nbsp; &nbsp;&nbsp;&nbsp;&nbsp; Wide Gamut LCD, RGB LED
Backlight - wide gamut Liquid Crystal Display with RGB LED
backlight.<br>
&nbsp;&nbsp;&nbsp; <span style="font-weight: bold;">x</span>
&nbsp;&nbsp; &nbsp;&nbsp;&nbsp; &nbsp;&nbsp;&nbsp;&nbsp; LCD, CCFL
Type 2
Backlight&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
- normal gamut Liquid Crystal Display with alternative Cold Cathode
Fluorescent Lamp backlight (Laptop ?)<br>
<br>
The ambient light sensor can be used with the <span
style="font-weight: bold;">Spyder4Elite</span> and <span
style="font-weight: bold;">Spyder4Pro</span> instruments, but is
only capable of monochrome readings.<span style="font-weight: bold;"></span><br>
<br>
<br>
<hr style="width: 100%; height: 2px;"><br>
<span style="font-weight: bold;"><a name="spyd5"></a>Spyder 5
colorimeter<br>
<br>
<img style="width: 262px; height: 220px;" alt="Spyder5"
src="Spyd5.jpg" width="449" height="350"> <br>
<br>
</span><span style="font-weight: bold;">Differences:<br>
<br>
</span>The <span style="font-weight: bold;">Spyder5Elite</span> and
<span style="font-weight: bold;">Spyder5Pro</span> appear to be
identical hardware with different software from the manufacturer.
The <span style="font-weight: bold;">Spyder5Express</span> lacks
the ambient sensor.<br>
<span style="font-weight: bold;"><br>
</span><span style="font-weight: bold;">Operation:<br>
</span><br>
These instruments are capable of using using CCSS (<a
href="File_Formats.html#ccss">Colorimeter Calibration Spectral
Sample</a>) files, and this also gives the instrument the
capability of using a non-default standard observer. CCSS files can
be created using the <a href="ccxxmake.html">ccxxmake</a> tool
using a spectrometer as a reference.<br>
<br>
<span style="font-weight: bold;">Important Note </span>about the
DataColor Spyder 5 vendor display type/calibration support:<br>
<br>
This instrument does not have a full range of display type
calibration selections available without the vendor supplied
calibration data for it.<br>
This calibration data is not provided with Argyll, since it is not
available under a compatible license.<br>
You can use CCSS files as an alternative (see above), or as the
purchaser of a Spyder 5 instrument you should have received a copy
of the calibration data along with the instrument or have been
directed to download it from the manufacturers website, and should
therefore be able to enable the full range of display type
selections in Argyll by using the <a href="oeminst.html">oeminst</a>
tool.<br>
<br>
The Display Selections for this instrument are:<br>
<br>
&nbsp;&nbsp;&nbsp; <span style="font-weight: bold;">n</span> | <span
style="font-weight: bold;">l</span>&nbsp;&nbsp; &nbsp;
&nbsp;&nbsp; A non-refresh type display with a generic calibration
[Default, CB1].<br>
&nbsp;&nbsp;&nbsp; <span style="font-weight: bold;">r | c</span> <span
style="font-weight: bold;"></span> &nbsp; &nbsp; &nbsp;&nbsp; A
refresh type display with a generic calibration.[CB2]<br>
<br>
The Display Selections for this instrument when the manufacturers
calibration information has been installed is:<br>
<br>
&nbsp;&nbsp;&nbsp; <span style="font-weight: bold;">n&nbsp;&nbsp; </span><span
style="font-weight: bold;"></span>&nbsp;&nbsp; &nbsp;
&nbsp;&nbsp;&nbsp;&nbsp; A non-refresh type display with a generic
calibration [Default, CB1].<br>
&nbsp;&nbsp;&nbsp; <span style="font-weight: bold;">r</span> <span
style="font-weight: bold;"></span> &nbsp; &nbsp; &nbsp;&nbsp;
&nbsp;&nbsp;&nbsp;&nbsp; A refresh type display with a generic
calibration.[CB2]<br>
&nbsp;&nbsp;&nbsp; <span style="font-weight: bold;">f &nbsp;&nbsp;
&nbsp;&nbsp;&nbsp; </span>&nbsp;&nbsp;&nbsp;&nbsp; LCD, CCFL
Backlight&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
- normal gamut Liquid Crystal Display with standard Cold Cathode
Fluorescent Lamp backlight.<br>
&nbsp;&nbsp;&nbsp; <span style="font-weight: bold;">L</span>&nbsp;
&nbsp;&nbsp;&nbsp; &nbsp;&nbsp;&nbsp; &nbsp; Wide Gamut LCD, CCFL
Backlight&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; - wide gamut Liquid Crystal
Display with Cold Cathode Fluorescent Lamps backlight.<br>
&nbsp;&nbsp;&nbsp; <span style="font-weight: bold;">e</span>
&nbsp;&nbsp; &nbsp;&nbsp;&nbsp; &nbsp;&nbsp;&nbsp;&nbsp; LCD, White
LED Backlight&nbsp;&nbsp;&nbsp; &nbsp;&nbsp;&nbsp;
&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; - normal
gamut Liquid Crystal Display with a White LED backlight.<br>
&nbsp;&nbsp;&nbsp; <span style="font-weight: bold;">B</span>&nbsp;&nbsp;
&nbsp;&nbsp;&nbsp; &nbsp;&nbsp;&nbsp;&nbsp; Wide Gamut LCD, RGB LED
Backlight - wide gamut Liquid Crystal Display with RGB LED
backlight.<br>
&nbsp;&nbsp;&nbsp; <span style="font-weight: bold;">x</span>
&nbsp;&nbsp; &nbsp;&nbsp;&nbsp; &nbsp;&nbsp;&nbsp;&nbsp; LCD, CCFL
Type 2
Backlight&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
- normal gamut Liquid Crystal Display with alternative Cold Cathode
Fluorescent Lamp backlight (Laptop ?)<br>
<br>
The ambient light sensor can be used with the <span
style="font-weight: bold;">Spyder5Elite</span> and <span
style="font-weight: bold;">Spyder5Pro</span> instruments, but is
only capable of monochrome readings.<br>
<br>
<hr style="width: 100%; height: 2px;"><span style="font-weight:
bold;"><a name="spydX"></a>SpyderX colorimeter<br>
<br>
<img alt="SpydeX" src="SpydX.jpg" width="250" height="249"> <br>
<br>
</span><span style="font-weight: bold;">Differences:<br>
<br>
</span>The <span style="font-weight: bold;">SpyderX Pro</span> and
<span style="font-weight: bold;">SpyderX Elite</span> appear to be
identical hardware with different software from the manufacturer.<br>
<span style="font-weight: bold;"><br>
</span><span style="font-weight: bold;">Operation:<br>
<br>
</span>This instrument has a black point that varies with
temperature, so it is advisable to first acclimatize it on the
display to be measured for 10-15 minutes before doing a black
calibration and then starting measurements.<span style="font-weight:
bold;"><br>
<br>
</span>The instrument appears to be sensitive to light polarization,
so the angle it is at may affect measurements of LCD based displays.<span
style="font-weight: bold;"><br>
</span><br>
The Display Selections for this instrument are:<br>
<br>
&nbsp;&nbsp; <b>l</b>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
General
[Default,CB1]&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
- i.e. LCD with CCFL backlight<br>
&nbsp;&nbsp; <b>e</b>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
Standard
LED&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
- i.e. LCD with white LED backlight<br>
&nbsp;&nbsp;<b> b</b>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
Wide Gamut
LED&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
- i.e. LCD with RGB LED backlight<br>
&nbsp;<b>&nbsp; i&nbsp;</b>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
GB
LED&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
- i.e. LCD with GB-R Phosphor LED backlight<br>
<br>
The ambient light sensor is only capable of monochrome readings, but
seems rather inaccurate due to having a very directional
characteristic since it has no frosting on the collection lens, and
also seems to be quite spectrally inaccurate.<br>
<br>
<br>
<hr style="width: 100%; height: 2px;"><span style="font-weight:
bold;"><a name="spydX2"></a>SpyderX2 colorimeter<br>
<br>
<img alt="SpydeX" src="SpydX2.jpg" moz-do-not-send="true"
width="250" height="239"> <br>
<br>
</span><span style="font-weight: bold;">Availability:<br>
<br>
</span>The <span style="font-weight: bold;">Spyder X2 Pro</span>, <span
style="font-weight: bold;">Spyder X2 Elite</span> and <b>Spyder
X2 Ultra </b>may still be available instruments.<br>
<span style="font-weight: bold;"><br>
</span><span style="font-weight: bold;">Operation:<br>
<br>
</span>The ArgyllCMS driver has an optional black point calibration
for this instrument, although the black point seems much more stable
than the Spyder X.<span style="font-weight: bold;"><br>
<br>
</span><span style="font-weight: bold;"></span>The Display
Selections for this instrument are:<br>
<br>
&nbsp;&nbsp; <b>l</b>
&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
General
[Default,CB1]&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
- i.e. LCD with CCFL backlight<br>
&nbsp;&nbsp; <b>e</b>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
Standard
LED&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
- i.e. LCD with white LED backlight<br>
&nbsp;&nbsp;<b> b</b>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
Wide Gamut
LED&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
- i.e. LCD with RGB LED backlight<br>
&nbsp;<b>&nbsp; i&nbsp;</b>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
GB
LED&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
- i.e. LCD with GB-R Phosphor LED backlight<br>
&nbsp;<b>&nbsp; h </b>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
High Brightness&nbsp;
&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
- i.e. LCD with high maximum brightness<br>
<br>
The ambient light sensor is only capable of monochrome readings, but
seems rather inaccurate due to having a very directional
characteristic since it has no frosting on the collection lens, and
also seems to be quite spectrally inaccurate.<br>
<br>
<br>
<hr style="width: 100%; height: 2px;"><span style="font-weight:
bold;"><a name="spyd2024"></a>Spyder &amp; SpyderPro colorimeter<br>
<br>
<img alt="SpydeX" src="Spyd2024.jpg" moz-do-not-send="true"
width="250" height="239"> <br>
<br>
</span><span style="font-weight: bold;">Availability:<br>
<br>
</span>The year <span style="font-weight: bold;">2024 Spyder</span>
&amp; <b>SpyderPro </b>are a currently available instruments. The
hardware appears to be identical to the Spyder X2, but with updated
firmware.<br>
<span style="font-weight: bold;"><br>
</span><span style="font-weight: bold;">Operation:<br>
<br>
</span>The ArgyllCMS driver has an optional black point calibration
for this instrument, although the black point seems much more stable
than the Spyder X.<span style="font-weight: bold;"><br>
<br>
</span><span style="font-weight: bold;"></span>The Display
Selections for this instrument are:<br>
<br>
&nbsp;&nbsp; <b>l</b>
&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
General
[Default,CB1]&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
- i.e. LCD with CCFL backlight<br>
&nbsp;&nbsp; <b>e</b>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
Standard
LED&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
- i.e. LCD with white LED backlight<br>
&nbsp;&nbsp;<b> b</b>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
Wide Gamut
LED&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
- i.e. LCD with RGB LED backlight<br>
&nbsp;<b>&nbsp; i&nbsp;</b>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
GB
LED&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
- i.e. LCD with GB-R Phosphor LED backlight<br>
&nbsp;<b>&nbsp; h </b>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
High Brightness&nbsp;
&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
- i.e. LCD with high maximum brightness<br>
&nbsp;<b>&nbsp;
o&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
</b>OLED
&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
- i.e. direct Organic LED<br>
&nbsp;<b>&nbsp; m </b>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; &nbsp; &nbsp;
&nbsp; Mini-LED &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
&nbsp; &nbsp;&nbsp; - i.e. LCD with higher density RGB LED backlight<br>
<br>
The ambient light sensor is only capable of monochrome readings, but
seems rather inaccurate due to having a very directional
characteristic since it has no frosting on the collection lens, and
also seems to be quite spectrally inaccurate.<span
style="font-weight: bold;"></span><br>
<br>
<hr style="width: 100%; height: 2px;"><a name="HCFR"></a><span
style="font-weight: bold;" class="titre">Colorimètre HCFR
colorimeter<br>
<br>
<img alt="" src="HCFR.jpg" style="width: 203px; height: 194px;"><br>
<br>
</span><span style="font-weight: bold;">Availability:<br>
<br>
</span>The <span style="font-weight: bold;" class="titre">Colorimètre
HCFR Probe</span> is a kit instrument from <span
style="font-weight: bold;"></span> <a
href="http://www.homecinema-fr.com/colorimetre/index_en.php">HCFR</a>.
<br>
<br>
<span style="font-weight: bold;">OS X</span><br>
<br>
Please note the installation <a href="Installing_OSX.html#HCFR">instructions</a>.<br>
<br>
<span style="font-weight: bold;">Operation:</span><br>
<span style="font-weight: bold;"><span style="font-weight: bold;"></span></span><br>
The accuracy of this instrument does not seem to be comparable to
the commercial instruments when used for measuring displays,
particularly in the area of measuring dark colors, and I've seen the
best results when used with a CRT display. It may well give good
results in calibrating projectors, since this was what it was
designed to do.<br>
<br>
The Display Selections for this instrument are:<br>
<br>
&nbsp;&nbsp;&nbsp; <span style="font-weight: bold;">l</span>&nbsp;&nbsp;&nbsp;&nbsp;
LCD display&nbsp;&nbsp;&nbsp; &nbsp;&nbsp;&nbsp;&nbsp; A Liquid
Crystal Display [Default].<br>
&nbsp;&nbsp;&nbsp; <span style="font-weight: bold;">c</span>&nbsp;&nbsp;&nbsp;
CRT display&nbsp;&nbsp;&nbsp; &nbsp;&nbsp;&nbsp;&nbsp; A Cathode Ray
Tube display.<br>
&nbsp;&nbsp;&nbsp; <b>R</b> &nbsp; Raw&nbsp;
Reading&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; Raw sensor readings,
used for calibration [CB1]<br>
<br>
<hr style="width: 100%; height: 2px;"><a name="ColorHug"></a><span
style="font-weight: bold;" class="titre">ColorHug<br>
<br>
<img alt="" src="ColorHug.jpg" style="width: 203px; height:
194px;" width="552" height="623"><br>
<br>
</span><span style="font-weight: bold;">Availability:<br>
<br>
</span>The <span style="font-weight: bold;" class="titre">ColorHug</span>
is a low cost display colorimeter instrument from <span
style="font-weight: bold;"></span> <a
href="http://www.hughski.com/">Hughski</a>. <br>
ArgyllCMS will also work with the <a
href="http://www.hughski.com/colorhug2.html">ColorHug2</a>.<br>
<br>
<span style="font-weight: bold;">Operation:</span><br>
<span style="font-weight: bold;"><span style="font-weight: bold;"></span></span><br>
Due to the nature of its sensor, the ColorHug accuracy is quite
dependent on the instrument calibration matrix. (The <b>ColorHug2</b>
is much more forgiving though). A custom .CCMX will greatly assist
it's accuracy, although a workaround is to calibrate your display
using its native white point, rather than aiming for some absolute
white point such as D65.<br>
<br>
The Display Selections for this instrument are:<br>
<br>
&nbsp;&nbsp; <b>l</b>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
LCD, CCFL Backlight [Default]<br>
&nbsp;&nbsp; <b>c</b>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
CRT display<br>
&nbsp;&nbsp; <b>p</b>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
Projector<br>
&nbsp;&nbsp; <b>e</b>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
LCD, White LED Backlight<br>
&nbsp;&nbsp; <b>F</b>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
Factory matrix (For Calibration) [CB1]<br>
&nbsp;&nbsp;<b> R</b>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
Raw Reading (For Factory matrix Calibration) [CB2]<br>
<br>
<hr style="width: 100%; height: 2px;"><br>
<a name="SMCube"></a><span style="font-weight: bold;">Palette/SwatchMate
Cube<br>
<br>
<img alt="SwatchMate Cube" src="SMCube.jpg" width="169"
height="205"><br>
<br>
</span><span style="font-weight: bold;">Availability:<br>
<br>
</span>The Cube from <a href="http://palette.com/cube.html">Palette/SwatchMate</a>
is a currently available entry level Colorimeter, with <a
href="http://www.argyllcms.com/doc2/smcube/smcube1.html">somewhat
limited accuracy</a>. The ArgyllCMS driver provides two
alternative calibrations that noticably <a
href="http://www.argyllcms.com/doc2/smcube/smcube2.html">improve
this accuracy</a>.<br>
<br>
The Calibration Selections for this instrument are:<br>
<br>
&nbsp;&nbsp; <b>m</b>
&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
Matt surfaces [Default]<br>
&nbsp;&nbsp; <b>g</b>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
Gloss surfaces<br>
&nbsp;&nbsp; <b>N</b>
&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
Native Calibration<br>
<br>
The <b>Cube</b><b></b> makes use of the newer FTDI FT231XS Virtual
COM Port Drivers (VCP), that may need installing for your operating
system. See <a href="Installing.html">installation instructions</a>.<br>
<br>
<span style="font-weight: bold;">Operation:<br>
</span><br>
The Cube must be connected via USB for operation with ArgyllCMS, and
can be connected either by USB or using Bluetooth LE when used with
<a href="http://www.argyllpro.com.au/">ArgyllPRO ColorMeter</a> on
capable Android devices.<br>
<br>
The Cube goes to sleep fairly rapidly and must be woken up by
pressing the top of it before connecting via USB to be recognized by
ArgyllCMS, although once connected, and with an ArgyllCMS utility
running, it should stay awake.<br>
<br>
When connecting via Bluetooth to ColorMeter, the foreground
application will be the one that connects to it.<br>
<br>
The ability to measure values into its own memory and recover them
later is not supported, since it is not possible to use the
ArgyllCMS calibrations with this feature.<br>
<br>
<span style="font-weight: bold;">Calibration:</span><br>
<br>
As well as the normal white calibration step, the ArgyllCMS driver
offers two option supplemental calibration steps that can improve
accuracy, but both require appropriate calibration conditions. You
can use <a href="spotread.html">spotread</a> with the 'k' command
to trigger this calibration.<br>
<br>
The <b>black calibration</b> requires a light trap, and the easiest
way of providing this is to place the Cube in a location that is
dark (i.e. not illuminated directly by any light) and some distance
from any surface. A practical approach I have used is to place the
measuring end in a thick black sock, and hide it from direct
illumination while this calibration step is done.<br>
<br>
The <b>gloss calibration</b> requires a black glossy surface. I
have used a paint catalog gloss paint black sample square for this,
but some other completely black glossy surface of sufficient size
such as a glossy black plastic item or a smooth surface painted in
gloss black paint should also work.<br>
<br>
<br>
<br>
<br>
<br>
<br>
<br>
<br>
</body>
</html>
Reference in New Issue View Git Blame Copy Permalink