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| author | Jörg Frings-Fürst <debian@jff-webhosting.net> | 2016-10-02 19:25:17 +0200 |
|---|---|---|
| committer | Jörg Frings-Fürst <debian@jff-webhosting.net> | 2016-10-02 19:25:17 +0200 |
| commit | c2ca7be5a751879159f3cb591a64bb9568b79762 (patch) | |
| tree | 04e38d4f4a2aad4d789bda0a65b7abb80a3439a2 /doc/FWA.html | |
| parent | 45c152c326d87478fbf41714b4b8e2f7b57a282b (diff) | |
| parent | 3db384424bd7398ffbb7a355cab8f15f3add009f (diff) | |
Updated version 1.9.1+repack from 'upstream/1.9.1+repack'
with Debian dir 98a996367aa69ae41accf9c6d369f600bc94de80
Diffstat (limited to 'doc/FWA.html')
| -rw-r--r-- | doc/FWA.html | 7 |
1 files changed, 4 insertions, 3 deletions
diff --git a/doc/FWA.html b/doc/FWA.html index c6b1f4b..e83a64f 100644 --- a/doc/FWA.html +++ b/doc/FWA.html @@ -225,9 +225,10 @@ instruments provide an illuminant measurement capability over the visible spectrum, for FWA compensation it is desirable to know the Ultra Violet (UV) component of the illuminant. Few color instruments - are capable of reading to such short wavelengths though. Argyll - provides an indirect way of estimating the UV component of an - illuminant using its <a href="illumread.html">illumread</a> + are capable of reading to such short wavelengths though (the <a + href="instruments.html#specbos">JETI specbos 1211</a> is an + exception). Argyll provides an indirect way of estimating the UV + component of an illuminant using its <a href="illumread.html">illumread</a> utility. Using illumread in combination with FWA compensation is the recommended approach to modelling real world appearance of paper containing FWA.<br> |