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+ | <catlist -forceHeadTitle -exclupage -sortAscending -hideNotFoundMsg -columns:1 -maxDepth:1 -noHead -noAddPageButton -ACLhideNs> | ||
+ | ---- | ||
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====== INFRARED [COLLAGE] ====== | ====== INFRARED [COLLAGE] ====== | ||
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===== HSDL-1001 ===== | ===== HSDL-1001 ===== | ||
- | * {{ :documentation: | + | * {{ documentation: |
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+ | ====== FAR IR / NEAR IR ====== | ||
+ | |||
+ | < | ||
+ | sensing and thermal imaging - this has a wavelength range of about 6 to 10 µm, and is not detected | ||
+ | at all my photodiodes or phototransistors. At these wavelengths glass absorbs, so any lenses have to | ||
+ | be made of exotic materials and are expensive. No source of illumination is needed, the heat of objects | ||
+ | is enough to radiate. | ||
+ | |||
+ | "near IR" is close to the visible range of light, say 0.7 to 1.5µm (700 to 1500nm) range, and most | ||
+ | photo diodes and photo transistors have peak sensitivity in this range, typically 780 or 850nm. Such | ||
+ | near IR behaves like light and can go through glass lenses (for instance). For seeing at night in near | ||
+ | IR you need a source of (near IR) illumination. Most visible light sources also put out near IR, so | ||
+ | a white flame will, but a blue flame probably gives out nothing in near IR, but loads and loads in | ||
+ | far IR.</ |