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Moving the diffraction grating to the backside of the lens adapter, I was able to make the spectra appear closer to the source. It seems possible to use the camera as an imaging spectrometer for various sources- here's the sun:
[PLAIN]http://img828.imageshack.us/img828/6797/dsc6607.jpg
and streetlights:
[PLAIN]http://img202.imageshack.us/img202/5695/dsc6629r.jpg
Both of these were taken with the 15mm, and the solar image also contains the secondary spectrum. As expected, the sun provides a continuum while the Hg streetlamps have discrete spectra.
Using the 400mm, I was able to capture the spectrum of Polaris:
[PLAIN]http://img811.imageshack.us/img811/2498/dsc6632d.jpg
IIRC, this was a 1s exposure. On the original, faint spectra from other stars can be seen, but I need to work a little bit to improve things.
It's not clear if I can extract quantitative spectral information from these, but it would be interesting if I could see differences in stars, or measure atmospheric attenuation.
[PLAIN]http://img828.imageshack.us/img828/6797/dsc6607.jpg
and streetlights:
[PLAIN]http://img202.imageshack.us/img202/5695/dsc6629r.jpg
Both of these were taken with the 15mm, and the solar image also contains the secondary spectrum. As expected, the sun provides a continuum while the Hg streetlamps have discrete spectra.
Using the 400mm, I was able to capture the spectrum of Polaris:
[PLAIN]http://img811.imageshack.us/img811/2498/dsc6632d.jpg
IIRC, this was a 1s exposure. On the original, faint spectra from other stars can be seen, but I need to work a little bit to improve things.
It's not clear if I can extract quantitative spectral information from these, but it would be interesting if I could see differences in stars, or measure atmospheric attenuation.
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