wpo - spectra - without a spectroscope!
The CD, as a simple reflective diffraction grating, is now joined by
a transmission version via the cover disk from a stack of blank CDs and
useful for testing deepsky and pollution filters.

At
some stage most 'discover' that by tilting a reflective grating, CD or
DVD so sunlight just skims the ruled surface - the absorption lines in
the spectrum are clearly visible to the unaided eye brought close to the
grating surface.
Domestic fluorescent tubes [Hg = mercury], energy saving lamps and mercury and sodium street lighting will also produce a spectrum via a CD as below.
The spectrum image can be captured onto film/digital camera by replicating the eye's position with the lens focused on the target light.
*credited to Phillip Pendred-Brittany

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Solar spectra below were taken with a digital still camera at full zoom and 600g/mm grating in 2nd order spectrum and yield a dispersion of 1A/pixel i.e. about the same as the pro-standard SBIG stellar spectrograph! Raw images have been resampled vertically to remove artefacts.
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Diffraction effects can also be seen in surfaces with regular small scale patterns like CCDs pixels to estimate the pixel size/shape in both X and Y axes.
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images/text copyright - Maurice Gavin - Sept 2001/ Feb 2002/Feb 2005