PROJECT TITLE :
A Hyperspectral Camera in the UVA Band
We have a tendency to present a hyperspectral camera primarily based on a Fabry–Pérot interferometer designed to work in the UVA range (315–four hundred nm). The measured hypercube contains concerning pixels, for a complete of one hundred sixty 00zero spectra. Every spectrum contains a spectral resolution of concerning 5 nm at the wavelength of 315 nm. Spatial and spectral discrimination capability has been demonstrated by imaging a target with 5 completely different ultraviolet (UV) lightweight-emitting diodes. Spectral resolution is demonstrated by aiming at the sky and observing spectral features of the diffused solar light-weight in the UV. A doable application of the hyperspectral camera is the measurement of the UVA content of the subtle lightweight of the entire sky.
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