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srb_000007/0000

Charisma - J_Dyer_G_Verri_and_J_Cupitt_Multispectral

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192
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Presentations of MSI conference in Serbia
srb_000007/0183
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srb_000007/0183

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align.82 align.83 S{ a1] cx Position line along edge of reflectance standard in visible-induced IR humin... [013 | specden.os4 [xs] fől {20 | viscalil,C35, matrix 031] C33.matrix gag |89.7991 [95.4605 | 105.74 Enclose the reflectance standard with box O| first } Extract from row: o S| number | Extract this many rows: 1 Matrix_extract_item,Rows_item.action 030 S/n 23.3865 [24.5863 |26.702 frst | Extract from row: o S| number Extract this many rows: 1 Rotate the reflectance standard to get white at the bottom-left Matrix_extract_item.Rows_item.action 031 28) v| @ Vector Q39.value?0 3 {oss | | angle [Rotate by: | 90 degrees clockwise rotate_widget 0 box, NULL == default v] 98 label JR reflectance Patches across chart; 8 targets 23.3685 26.7702 17.9647 | 18.9009 14.4442 15.1969 | 16.5468 11.9687 (12.5924 = 13.7109 5.09087 3.63785 | 3.82742 3.51932 | 3.70272 1.45406 | 1.52983 weal 6900) oh) Bulle) or) owffe~ hu) ale ely) ol Wo] ol we) = Figure 3-88 ~ i o| ] label | visible~induced IR luminescence, stray light removed arch Desktop (0B RWS B & 12:19 <> a sa label | visible-induced IR luminescence, stray light removed targets <> & A input.Pair (Q1.label ++ ", stray light removed") (Q1.targets - Q3.targets) (Q1.object - 03.object) Figure 3-89 28) Figure 3-90 shows a comparison of the images before (right) and after subtraction of the ambient stray radiation (left). 29) The sRGB (or RGB16) VIL images corrected for ambient stray radiation can be viewed and saved in the “results” tab. Images of the mathematically reconstructed ambient stray radiation are also available in this column of the “results” tab (see later). Correcting for the “pigment-binder’” interaction (Kubelka-Munk) 30) Click on the “vilkm” tab (Figure 3-91). Column J] uses the corrected VIS, IRR and VIL images (automatically carried over from the “viscalib”, “specden” and “vilstray” tabs, respectively) to calculate y, a function which expresses the extent to which the pigment particles absorb the light emitted by the luminescent materials (for more details see Chapter 1). Version No. 1.0 176 Date : 14/10/2013

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