diff options
| author | Jörg Frings-Fürst <debian@jff-webhosting.net> | 2015-05-01 16:24:15 +0200 |
|---|---|---|
| committer | Jörg Frings-Fürst <debian@jff-webhosting.net> | 2015-05-01 16:24:15 +0200 |
| commit | a30ba67504ffd12c4db499adbb5ce47a7d1f6036 (patch) | |
| tree | 9ae1a7e3849dda6bbb5c578232f6f2fa5b2e7e7e /doc/spotread.html | |
| parent | 89e99e8a827859729729dfc92d74be4a8f96f1a4 (diff) | |
| parent | 094535c010320967639e8e86f974d878e80baa72 (diff) | |
New release 1.7.0
Diffstat (limited to 'doc/spotread.html')
| -rw-r--r-- | doc/spotread.html | 436 |
1 files changed, 406 insertions, 30 deletions
diff --git a/doc/spotread.html b/doc/spotread.html index aaac0a1..f3964f5 100644 --- a/doc/spotread.html +++ b/doc/spotread.html @@ -3,14 +3,18 @@ <head> <title>spotread</title> <meta http-equiv="content-type" content="text/html; - charset=ISO-8859-1"> + charset=windows-1252"> <meta name="author" content="Graeme Gill"> </head> <body> <h2><b>spectro/spotread</b></h2> <h3>Summary</h3> Use an instrument to read a single color value. This can be a useful - diagnostic aid. + diagnostic aid.<br> + <br> + [ A commercial tool that does much of what spotread does and more, + is the <a href="http://www.argyllpro.com.au/">ArgyllPRO ColorMeter</a>. + ]<br> <h3>Usage Summary</h3> <small><span style="font-family: monospace;">spotread [-options] [logfile]</span><br style="font-family: monospace;"> @@ -34,6 +38,14 @@ + + + + + + + + Verbose mode</span><br style="font-family: monospace;"> <span style="font-family: monospace;"></span><span @@ -58,6 +70,14 @@ + + + + + + + + Print spectrum for each reading.</span></small><br style="font-family: monospace;"> <small><span style="font-family: monospace;"></span><span @@ -87,6 +107,14 @@ + + + + + + + + Set COM port, 1..4 (default 1)</span><span style="font-family: monospace;"></span><span style="font-family: monospace;"><br style="font-family: monospace;"> @@ -110,6 +138,14 @@ + + + + + + + + Use transmission measurement mode</span><br style="font-family: monospace;"> <span style="font-family: monospace;"> </span><a style=" @@ -133,6 +169,14 @@ + + + + + + + + Use emissive measurement mode (absolute results)<br> </span></small><small><span style="font-family: monospace;"> </span><a style=" font-family: monospace;" href="#eb">-eb</a><span @@ -155,11 +199,27 @@ + + + + + + + + Use display white brightness relative measurement mode<br> </span></small><small><span style="font-family: monospace;"> </span><a style=" font-family: monospace;" href="#ew">-ew</a><span style="font-family: monospace;"> + + + + + + + + Use display white point relative chromatically adjusted mode<br> </span></small><small><span style="font-family: monospace;"> </span><a style=" font-family: monospace;" href="#p">-p</a><span @@ -182,6 +242,14 @@ + + + + + + + + Use telephoto measurement mode (absolute results)<br> </span></small><small><span style="font-family: monospace;"> </span><a style=" font-family: monospace;" href="#pb">-pb</a><span @@ -204,6 +272,14 @@ + + + + + + + + Use </span></small><small><span style="font-family: monospace;">projector</span></small><small><span style="font-family: monospace;"> white brightness relative measurement mode<br> @@ -228,6 +304,14 @@ + + + + + + + + Use </span></small><small><span style="font-family: monospace;">projector</span></small><small><span style="font-family: monospace;"> </span></small><small><span style="font-family: monospace;">white point relative @@ -253,6 +337,14 @@ + + + + + + + + Use ambient measurement mode (absolute results)<br> <a href="#f">-f</a> @@ -272,6 +364,14 @@ + + + + + + + + Use ambient flash measurement mode (absolute results)<br> </span></small><font size="-1"><span style="font-family: monospace;"> <a href="#y">-y X</a> @@ -293,6 +393,14 @@ + + + + + + + + Display type - instrument specific list to choose from.</span></font><br> <small><span style="font-family: monospace;"> </span><a style="font-family: monospace;" href="spotread.html#I">-I illum</a><span @@ -312,6 +420,14 @@ M0, + + + + + + + + M1, M2, A, D50 (def.), D50M2, D65, F5, F8, F10 or file.sp</span></small><br style="font-family: monospace;"> <small><span style="font-family: monospace;"></span><span @@ -319,7 +435,7 @@ M0, style="font-family: monospace;" href="#i">-i illum</a><span style="font-family: monospace;"> Choose illuminant for computation of - CIE XYZ from spectral data & FWA:</span><br + CIE XYZ from spectral reflectance & FWA:</span><br style="font-family: monospace;"> <span style="font-family: monospace;"> @@ -348,6 +464,14 @@ D50 + + + + + + + + D50M2, D65, F5, F8, F10 or file.sp</span><br style="font-family: monospace;"> <span style="font-family: monospace;"> </span><a style=" @@ -374,6 +498,14 @@ D50 + + + + + + + + </span></small><small><span style="font-family: monospace;">1931_2 </span></small><small><span style="font-family: monospace;"> (def.)</span></small><small><span @@ -399,6 +531,14 @@ D50 + + + + + + + + Set filter configuration:<br> n @@ -419,6 +559,14 @@ D50 + + + + + + + + None<br> p @@ -439,6 +587,14 @@ D50 + + + + + + + + Polarising filter<br> 6 @@ -459,6 +615,14 @@ D50 + + + + + + + + D65<br> u @@ -479,6 +643,14 @@ D50 + + + + + + + + U.V. Cut<br> <a href="#E">-E extrafilterfile</a> Apply extra filter compensation file<br> @@ -502,6 +674,14 @@ D50 + + + + + + + + Display Yxy instead of Lab<br> </span></font><font size="-1"><span style="font-family: monospace;"> <a href="#h">-h</a> @@ -523,6 +703,14 @@ D50 + + + + + + + + Display LCh instead of Lab</span></font><br> <font size="-1"><span style="font-family: monospace;"> <a href="#V">-V</a> @@ -544,6 +732,14 @@ D50 + + + + + + + + Show running average and std. devation from ref.</span></font><br> <font size="-1"><span style="font-family: monospace;"> <a href="#T">-T</a> @@ -565,6 +761,14 @@ D50 + + + + + + + + Display correlated color temperatures and CRI<br> </span></font><font size="-1"><span style="font-family: monospace;"> <a href="#N">-N</a> @@ -585,7 +789,44 @@ D50 + + + + + + + + Disable initial calibration of instrument if possible</span></font><br> + <font size="-1"><span style="font-family: monospace;"> <a + href="spotread.html#O">-O</a> + + + + + + + + + + + + + + + + + + + + + + + + + + + Do one cal. or measure and exit</span></font><br> <font size="-1"><span style="font-family: monospace;"> </span><a style="font-family: monospace;" href="#H">-H</a><span style="font-family: monospace;"> @@ -611,6 +852,14 @@ D50 + + + + + + + + Apply Colorimeter Correction Matrix</span></font><br> <span style="font-family: monospace;"> <a href="#X2">-X file.ccss</a> @@ -636,6 +885,14 @@ Samples + + + + + + + + for calibration</span><br> <font size="-1"><span style="font-family: monospace;"> </span><a style=" font-family: monospace;" href="#Yrn">-<font size="-1">Y</font> @@ -650,10 +907,26 @@ Samples + + + + + + + + Override refresh, non-refresh display mode</span></font><br> <tt> <a href="#YR">-Y R:<i>rate</i></a> + + + + + + + + Override measured refresh rate with rate Hz</tt><br> <font size="-1"><span style="font-family: monospace;"> </span><a style=" font-family: monospace;" href="#YA">-<font size="-1">Y </font>A</a><span @@ -688,6 +961,14 @@ none, + + + + + + + + h = HW, x = Xon/Xoff</span></font><br> <small><span style="font-family: monospace;"> </span><a style=" font-family: monospace;" href="#D">-D [level]</a><span @@ -713,6 +994,14 @@ none, + + + + + + + + Optional file to save reading results<br style="font-family: monospace;"> </span></font><small><span style="font-family: monospace;"></span><span @@ -736,6 +1025,64 @@ none, You must strike a key in the plot window to continue with another measurement.<br> <br> + The Graph plots light wavelength on the X axis, and either absolute + or relative level on the Y axis. <br> + <br> + <table cellpadding="0" cellspacing="0" border="1" height="153" + width="200"> + </table> + <table cellpadding="0" cellspacing="0" border="1"> + <tbody> + <tr> + <th valign="top"> Measurement Mode <br> + </th> + <th valign="top">Y Units<br> + </th> + </tr> + <tr> + <td align="center" valign="top">Emission<br> + </td> + <td align="center" valign="top">mW/(m<sup>2</sup>.sr.nm)</td> + </tr> + <tr> + <td align="center" valign="top">Ambient<br> + </td> + <td align="center" valign="top">mW/(m<sup>2</sup>.nm)<br> + </td> + </tr> + <tr> + <td align="center" valign="top">Emission Flash<br> + </td> + <td align="center" valign="top"> mW/(m<sup>2</sup>.sr.nm.s) + + + + + + <br> + </td> + </tr> + <tr> + <td align="center" valign="top">Ambient Flash<br> + </td> + <td align="center" valign="top">mW/(m<sup>2</sup>.nm.s)<br> + </td> + </tr> + <tr> + <td align="center" valign="top">Reflective<br> + </td> + <td align="center" valign="top">%/nm<br> + </td> + </tr> + <tr> + <td align="center" valign="top">Transmissive<br> + </td> + <td align="center" valign="top">%/nm<br> + </td> + </tr> + </tbody> + </table> + <br> <a name="c"></a> The instrument is assumed to communicate through a USB or serial communication port, and the port can be selected with the <b>-c</b> option, if the instrument is not connected to the @@ -833,29 +1180,33 @@ none, and how this works, see <a href="instruments.html">Operation of particular instruments</a>. <b>3)</b> Any installed CCSS files (if applicable), or CCMX files. These files are typically created - using <a href="ccxxmake.html">ccxxmake</a>, - and installed using <a - href="oeminst.html">oeminst</a>. The - default and Base Calibration types will be indicated in the usage.<br> + using <a href="ccxxmake.html">ccxxmake</a>, and installed using <a + href="oeminst.html">oeminst</a>. The default and Base Calibration + types will be indicated in the usage.<br> <br> <a name="I"></a>The <b>-I</b> parameter allows specifying a - standard or custom illumination spectrum to be used as the similated - instrument illuminant when FWA compensation is used during - measurement, overriding the default <b>D50</b> or CIE computation - illuminant used for FWA (see <b>-i</b> below<b>). </b>See <a - href="colprof.html#f">colprof -f</a> for a fuller explanation. <br> + standard or custom illumination spectrum to be used as the simulated + reflectance instrument illuminant when FWA compensation is used + during <u>measurement</u>, overriding the default <b>D50</b> or + CIE computation illuminant used for FWA (see <b>-i</b> below<b>). </b>If + + using <b>M0</b>, <b>M1</b> or <b>M2</b>, then the <b>-i</b> + option is <b>not</b> normally used. See <a href="colprof.html#f">colprof + + -f</a> for a fuller explanation. <br> <br> <a name="i"></a>The <b>-i</b> parameter allows specifying a - standard or custom illumination spectrum applied to <span + standard or custom reflectance illumination spectrum applied to <span style="text-decoration: underline;">reflective</span> or <u>transmissive</u> - spectral data to compute CIE tristimulus values. <b>A</b>, <b>D50</b>, - <b>D50M2, D65</b>, <b>F5</b>, <b>F8</b>, <b>F10</b> are a - selection of standard illuminant spectrums, with <b>D50</b> being - the default. If a filename is specified instead, it will be assumed - to be an Argyll specific <a href="File_Formats.html#.sp">.sp</a> - spectrum file. If FWA compensation is used during measurement, this - illuminant will be used by default as the simulated instrument - illuminant.<br> + spectral data to <u>compute</u> CIE tristimulus values. <b>A</b>, + <b>D50</b>, <b>D50M2, D65</b>, <b>F5</b>, <b>F8</b>, <b>F10</b> + are a selection of standard illuminant spectrums, with <b>D50</b> + being the default. If using <b>-I M0</b>, <b>M1</b> or <b>M2</b>, + then this <b>-i</b> option is <b>not</b> normally used. If a + filename is specified instead, it will be assumed to be an Argyll + specific <a href="File_Formats.html#.sp">.sp</a> spectrum file. If + FWA compensation is used during measurement, this illuminant will be + used by default as the simulated instrument illuminant.<br> <br> <a name="Q"></a> The <b>-Q</b> flag allows specifying a tristimulus observer, and is used to compute PCS (Profile Connection Space) @@ -930,6 +1281,11 @@ none, computer. It is advisable to only use this option on the second and subsequent measurements in a single session.<br> <br> + <a name="O"></a><b>-O</b> Do a calibration or a single measurement + and exit. To take a measurement with an instrument that always does + a calibration first, calibrate it and then use -O with -N. The -O + option is intended to simplify scripted use of spotread.<br> + <br> <a name="H"></a> The -<span style="font-weight: bold;">H</span> option turns on high resolution spectral mode, if the instrument supports it. See <a href="instruments.html">Operation of particular @@ -970,6 +1326,14 @@ a + + + + + + + + colorimeters accuracy for a particular type of display.<br> <br> <a name="Yrn"></a> The -<span style="font-weight: bold;">Y r </span>and @@ -982,6 +1346,14 @@ a + + + + + + + + <b>-Y n</b> options overrides the refresh display mode set by the <a href="#y">-y display type selection</a>, with <b>-Y</b><span style="font-weight: bold;"> r</span> forcing refresh display mode, @@ -997,12 +1369,12 @@ a <br> <a name="YA"></a> The -<span style="font-weight: bold;">Y A</span> option uses a non-adaptive integration time emission measurement - mode, if the instrument supports it, such as the Eye-One Pro or - ColorMunki. By default an adaptive integration time measurement mode - will be used for emission measurements, but some instruments support - a fixed integration time mode that can be used with display devices. - This may give increased consistency and faster measurement times, - but may also give less accurate low level readings.<br> + mode, if the instrument supports it, such as the Eye-One Pro, + ColorMunki, i1d3 or K10. By default an adaptive integration time + measurement mode will be used for emission measurements, but some + instruments support a fixed integration time mode that can be used + with display devices. This may give faster measurement times, but + may also give less accurate low level readings.<br> <br> <a name="W"></a>The <b>-W</b> <span style="font-weight: bold;">n|h|x</span> parameter overrides the default serial communications flow control @@ -1041,9 +1413,13 @@ a the range 0 .. 100 for reflective or transmissive readings, and absolute cd/m^2 for display, emissive and ambient readings.<br> <br> - The L*a*b* values are computed relative to a D50 100 scale white - point. (Note that using display white relative mode makes the L*a*b - relative to the display white point.)<br> + By default the L*a*b* values are computed relative to a fixed D50 + 100 scale white point, so values for emissive sources are not + particularly useful.<br> + Using the display white relative mode uses a Bradford chromatic + transform to transform from the measured white to a D50 white (the + same as ArgyllCMS ICC profile deals a display white), and then + computes the D50 L*a*b from that.<br> <br> If Fluorescent Whiter Additive (FWA) compensated readings are to be made, then this needs to be enabled with the correct command line |