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-rw-r--r--doc/spec2cie.html10
1 files changed, 5 insertions, 5 deletions
diff --git a/doc/spec2cie.html b/doc/spec2cie.html
index 192ee64..c928f9a 100644
--- a/doc/spec2cie.html
+++ b/doc/spec2cie.html
@@ -19,7 +19,7 @@
          
Verbose mode</small></tt><br>
<tt><small><small>&nbsp;<a
- href="file:///D:/src/argyll/doc/spec2cie.html#I">-I <i>illum</i></a>&nbsp;&nbsp;
+ href="spec2cie.html#I">-I <i>illum</i></a>&nbsp;&nbsp;
&nbsp;&nbsp; Override
actual instrument illuminant
in .ti3 file:<br>
@@ -31,14 +31,14 @@
(only
used in conjunction with <span style="font-weight: bold;">-f</span>)<br>
</small></small></tt><tt><small><small>&nbsp;<a
- href="file:///D:/src/argyll/doc/colprof.html#f">-f [<i>illum</i>]</a>
+ href="colprof.html#f">-f [<i>illum</i>]</a>
&nbsp;&nbsp; Use Fluorescent Whitening Agent compensation
[simulated inst. illum.:<br>
&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
M0, M1, M2, A, C, D50 (def.), D50M2, D65, F5, F8, F10 or
file.sp]<br>
</small></small></tt><tt><small><small><small>&nbsp;<a
- href="file:///D:/src/argyll/doc/spec2cie.html#i">-i <i>illum</i></a>&nbsp;&nbsp;
+ href="spec2cie.html#i">-i <i>illum</i></a>&nbsp;&nbsp;
&nbsp;&nbsp; Choose illuminant for computation of CIE XYZ
from spectral data &amp; FWA:<br>
&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
@@ -93,7 +93,7 @@ Measurement
bold;">-f</span>
flag. If a
filename is specified instead, it will be assumed to be an Argyll
- specific <a href="file:///D:/src/argyll/doc/File_Formats.html#.sp">.sp</a>
+ specific <a href="File_Formats.html#.sp">.sp</a>
custom spectrum file.
Illuminant details are:<br>
<br>
@@ -130,7 +130,7 @@ Measurement
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:///D:/src/argyll/doc/File_Formats.html#.sp">.sp</a>
+ href="File_Formats.html#.sp">.sp</a>
custom spectrum file. This only works if spectral data is available.
Illuminant details are:<br>
<br>