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Multispectral & Scientific Imaging

When multispectral capture goes wrong, work through it in physical order — lighting, geometry, exposure, calibration, then processing — because a fault early in that chain masquerades as something else later. The fastest single check is to flat-field with fresh white and dark references and confirm the bands are registered; that resolves the majority of "the data looks broken" reports. This guide is the end-to-end triage I run in the imaging room, with the concrete symptom-to-fix mapping for each stage.

Why won't my bands align? ​

Misregistration is the most common and most damaging fault: each waveband is a separate exposure, so any movement of the camera, the page or the focus ring shifts a band by a pixel or more, and false-colour or PCA then paints colour ghosts along every stroke.

Fixes, in order of impact:

  • Lock focus and aperture before the first band; never refocus mid-sequence.
  • Use a rigid copy stand and a book cradle that does not creep.
  • Trigger remotely to avoid touching the rig.
  • Register in software afterward with Linear Stack Alignment with SIFT (Fiji) or phase cross-correlation to absorb residual drift.

Why is one band darker or brighter than the others? ​

Because exposure must be set per waveband. A halogen lamp and a silicon sensor are far more sensitive in the visible than in the UV or deep IR, so a single fixed exposure clips some bands and buries others in noise. Set each band's exposure so the white reference reads near 90% of full scale without clipping:

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per band:  expose so white-ref ≈ 0.9 * max,  no pixels at saturation
then:      corrected = (raw - dark) / (white - dark)

The flat-field divide is what makes bands comparable afterwards.

How do I get rid of glare and hotspots? ​

Specular reflections off parchment, gilding or a glass platen show up as blown-out patches that destroy any text underneath. The standard answer is cross-polarisation: a polarising sheet on each light, a polarising filter on the lens, rotated 90 degrees to the lights. Combined with diffuse, even illumination at ~45 degrees, this removes the mirror reflection while keeping the diffuse signal that carries information.

SymptomCauseFix
Bright blown patchSpecular glareCross-polarisation
Bright edge near gutterRaking angle too steepLower light angle, diffuse
Sheen over gildingMetallic reflectionPolarise + reposition lights

What causes banding or a grid pattern? ​

Two unrelated culprits. Light flicker — cheap LED or fluorescent sources pulsing at mains frequency — beats against a short exposure to produce horizontal banding; cure it with a flicker-free source and an exposure longer than one mains cycle. Fixed-pattern sensor noise produces a static grid; subtract a dark frame captured at the same exposure and temperature to remove it.

Why do good-looking images fail in analysis? ​

This is the quiet killer. The image looks fine because your screen applied an automatic stretch, but the saved master was 8-bit or JPEG-compressed, throwing away the faint differences the whole technique depends on. Rules that prevent it:

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- Save masters as 16-bit linear TIFF (no gamma, no JPEG).
- Flat-field every band against white and dark references.
- Apply contrast stretches only to derivative copies.
- Keep the raw and the calibration frames.

How do I separate a real feature from an artefact? ​

Reproduce it. Re-capture the region and check whether the faint mark survives flat-fielding and registration and appears in the bands physics predicts. Artefacts are fragile — change the light angle, re-flat-field, or re-register and they shift or vanish. A genuine palimpsest stroke or faded line is stubbornly repeatable across captures and behaves consistently across wavebands. Document each test so the conclusion is defensible.

Key Takeaways ​

  • Troubleshoot in physical order: lighting, geometry, exposure, calibration, processing.
  • Misregistration is the top fault — lock focus, use a rigid stand, and align bands in software.
  • Set exposure per band so the white reference sits near 90% without clipping.
  • Kill glare with cross-polarisation and diffuse 45-degree lighting.
  • Banding comes from light flicker or fixed-pattern noise; use flicker-free sources and dark-frame subtraction.
  • Save 16-bit linear masters and flat-field; never analyse a JPEG or 8-bit copy.
  • Validate faint features by reproducing them across re-captures and expected bands.

Frequently Asked Questions ​

Why are my multispectral bands not aligning? ​

The page or camera moved between exposures, or focus shifted. Lock focus and aperture for the whole sequence, use a sturdy copy stand and a book cradle, and register the bands in software afterwards to absorb any residual sub-pixel drift.

Why is one band much darker or brighter than the rest? ​

Exposure was not balanced per waveband. Each band needs its own exposure because lamps and sensor sensitivity vary with wavelength; set exposure so the white reference sits near 90% without clipping in every band, then flat-field.

What causes glare or hotspots on the page? ​

Specular reflection from raking or frontal light, common on glossy parchment and gilding. Use cross-polarisation (polarising filters on both lights and lens) and even, diffuse illumination at roughly 45 degrees to kill the hotspots.

Why do I see banding or a grid pattern in the image? ​

Usually flicker from LED or fluorescent lighting beating against the exposure, or fixed-pattern sensor noise. Use a flicker-free light source, lengthen exposure past one mains cycle, and subtract a dark frame to remove fixed-pattern noise.

My results look fine on screen but fail in analysis — why? ​

You probably skipped flat-fielding or saved a lossy/8-bit version. Keep 16-bit linear masters, flat-field with white and dark references, and only stretch contrast in a derivative copy, never in the master.

How do I tell a real faint feature from an artefact? ​

Reproduce it. Re-capture the region, check it survives flat-fielding and registration, and confirm it appears consistently across the expected bands. A true feature is repeatable; an artefact usually moves or vanishes when you change one capture variable.