Actually, calibration is not really the correct term. Calibratinga monitor would mean that you measure the response of the monitor and thencompensate for non-ideal behavior elsewhere, for example in the video-carddriver. Here, you are supposed to change the properties of the monitoritself to let it approach the ideal better. But then, who cares whether youcall it monitor adjustment or monitor calibration...

DisplayCAL (formerly known as dispcalGUI) is a display calibration and profiling solution with a focus on accuracy and versatility (in fact, the author is of the honest opinion it may be the most accurate and versatile ICC compatible display profiling solution available anywhere). At its core it relies on ArgyllCMS, an advanced open source color management system, to take measurements, create calibrations and profiles, and for a variety of other advanced color related tasks.


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Calibrate and characterize your display devices using one of many supported measurement instruments, with support for multi-display setups and a variety of available options for advanced users, such as verification and reporting functionality to evaluate ICC profiles and display devices, creating video 3D LUTs, as well as optional CIECAM02 gamut mapping to take into account varying viewing conditions. Other features include:

Alternatively, if you don't mind trying out development code, browse the SVN[8] repository of the latest development version (or do a full checkout using svn checkout svn://svn.code.sf.net/p/dispcalgui/code/trunk displaycal). But please note that the development code might contain bugs or not run at all, or only on some platform(s). Use at your own risk.

If the pre-compiled extension module that is included in the sources does not work for you (in that case you'll notice that the movable measurement window's size does not closely match the size of the borderless window generated by ArgyllCMS during display measurements) or you want to re-build it unconditionally, run python2 setup.py build_ext -i to re-build it from scratch (you need to satisfy the requirements for compiling the C extension module first).

If your measurement device is a i1 Display 2, i1 Display Pro, ColorMunki Display, DTP94, Spyder2/3/4/5, you'll want to import the colorimeter corrections that are part of the vendor software packages, which can be used to better match the instrument to a particular type of display. Note: The full range of measurement modes for the Spyder4/5 are also only available if they are imported from the Spyder4/5 software.

These instruments greatly reduce the amount of work needed to match them to a display because they contain the spectral sensitivities of their filters in hardware, so only a spectrometer reading of the display is needed to create the correction (in contrast to matching other colorimeters to a display, which needs two readings: One with a spectrometer and one with the colorimeter).

That means anyone with a particular screen and a spectrometer can create a special Colorimeter Calibration Spectral Set (.ccss) file of that screen for use with those colorimeters, without needing to actually have access to the colorimeter itself.

Here, you can load a preset, or a calibration (.cal) or ICC profile (.icc / .icm) file from a previous run. This will set options to those stored in the file. If the file contains only a subset of settings, the other options will automatically be reset to defaults (except the 3D LUT settings, which won't be reset if the settings file doesn't contain 3D LUT settings, and the verification settings which will never be reset automatically).

Many displays, be it CRT, LCD, Plasma or OLED, have a default response characteristic close to a gamma of approx. 2.2-2.4 (for CRTs, this is the actual native behaviour; and other technologies typically try to mimic CRTs). A target response curve for calibration that is reasonably close to the native response of a display should help to minimize calibration artifacts like banding, because the adjustments needed to the video card's gamma tables via calibration curves will not be as strong as if a target response farther away from the display's native response had been chosen.

Note that if you use this method of displaying test patches, then colors will be displayed with 8 bit per component precision, and any screen-saver or power-saver will not be automatically disabled. You will also be at the mercy of any color management applied by the web browser, and may have to carefully review and configure such color management.

Note that if you want to create a 3D LUT for a display that is directly connected (e.g. for Resolve's GUI viewer), you should not use the Resolve pattern generator, and select the actual display device instead which will allow for quicker measurements (Resolve's pattern generator has additional delay).

White level drift compensation tries to counter luminance changes of a warming up display device. For this purpose, a white test patch is measured periodically, which increases the overall time needed for measurements.

Black level drift compensation tries to counter measurement deviations caused by black calibration drift of a warming up measurement device. For this purpose, a black test patch is measured periodically, which increases the overall time needed for measurements. Many colorimeters are temperature stabilised, in which case black level drift compensation should not be needed, but spectrometers like the i1 Pro or ColorMunki Design/Photo/i1Studio are not temperature compensated.

Normally a delay of 200 msec is allowed between changing a patch color in software, and that change appearing in the displayed color itself. For some instuments (i.e. i1 Display Pro, ColorMunki Display, i1 Pro, ColorMunki Design/Photo/i1Studio, Klein K10-A) ArgyllCMS will automatically measure and set an appropriate update delay during instrument calibration. In rare situations this delay may not be sufficient (ie. some TV's with extensive image processing features turned on), and a larger delay can be set here.

Normally the display technology type determines how long is allowed between when a patch color change appears on the display, and when that change has settled down, and as actually complete within measurement tolerance. A CRT or Plasma display for instance, can have quite a long settling delay due to the decay characteristics of the phosphor used, while an LCD can also have a noticeable settling delay due to the liquid crystal response time and any response time enhancement circuit (instruments without a display technology type selection such as spectrometers assume a worst case).

The display settle time multiplier allows the rise and fall times of the model to be scaled to extend or reduce the settling time. For instance, a multiplier of 2.0 would double the settling time, while a multiplier of 0.5 would halve it.

Full field pattern insertion can help with displays that employ ASBL (automatic static brightness limiting), like some types of OLED and HDR displays. A full field pattern is shown every few seconds (the minimum interval can be set with the respective control) for a given duration, at a given signal level, if this option is enabled.

Allows setting the target white point locus to the equivalent of a daylight or black body spectrum of the given temperature in degrees Kelvin, or as chromaticity co-ordinates. By default the white point target will be the native white of the display, and it's color temperature and delta E to the daylight spectrum locus will be shown during monitor adjustment, and adjustments will be recommended to put the display white point directly on the Daylight locus. If a daylight color temperature is given, then this will become the target of the adjustment, and the recommended adjustments will be those needed to make the monitor white point meet the target. Typical values might be 5000 for matching printed output, or 6500, which gives a brighter, bluer look. A white point temperature different to that native to the display may limit the maximum brightness possible.

Set the target brightness of white in cd/m2. If this number cannot be reached, the brightest output possible is chosen, consistent with matching the white point target. Note that many of the instruments are not particularly accurate when assessing the absolute display brightness in cd/m2. Note that some LCD screens behave a little strangely near their absolute white point, and may therefore exhibit odd behavior at values just below white. It may be advisable in such cases to set a brightness slightly less than the maximum such a display is capable of.

To allow for the non-zero black level of a real display, by default the target curve values will be offset so that zero input gives the actual black level of the display (output offset). This ensures that the target curve better corresponds to the typical natural behavior of displays, but it may not be the most visually even progression from display minimum. This behavior can be changed using the black output offset option (see further below).

As explained for the tone curve settings, often colors are encoded in a situation with viewing conditions that are quite different to the viewing conditions of a typical display, with the expectation that this difference in viewing conditions will be allowed for in the way the display is calibrated. The ambient light level option is a way of doing this. By default calibration will not make any allowances for viewing conditions, but will calibrate to the specified response curve, but if the ambient light level is entered or measured, an appropriate viewing conditions adjustment will be performed. For a gamma value or sRGB, the original viewing conditions will be assumed to be that of the sRGB standard viewing conditions, while for REC 709 and SMPTE 240M they will be assumed to be television studio viewing conditions.

By specifying or measuring the ambient lighting for your display, a viewing conditions adjustment based on the CIECAM02 color appearance model will be made for the brightness of your display and the contrast it makes with your ambient light levels. ff782bc1db

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