Astronomical Spectra L200 Spectrograph
Bench Testing
The astronomical Spectra L200 spectrograph is a kit designed and sold by Ken Harrison. A Littrow spectroscope kit, the Spectra-L200 is for amateurs moving from the basic Star Analyser/ Rainbow Optic grating to their first slit spectroscope. It is only available to members of the astronomical spectroscopy Y! group.
Ken Harrison is the owner of the  Yahoo! 
astronomical_spectroscopy Astronomical Spectroscopy for Amateurs group. 
This web page shows work-in-progress of building and testing the Spectra L200.  Below are photos of the unpainted Spectra L200 that was put together to check mechanical fit and optical alignment.
- R=3000+
 - The 30mm x 30mm diffraction gratings is an Optometrics 600 l/mm ruled 500 nm blaze.
 - Adjustable slit mechanism
 - For use with telescopes above f7 (f7 to f12)
 - For bench testing the objective lens is a 
Mini Borg 45ED
 f/ 7.2 (focal length 325) refractor. 
 - The Orion flip mirror is used as a finder. 
 - The astronomical spectrograph snaps on a tripod with the Bogen-Manfrotto RC4 Low Profile Rectangular Rapid Connect Adapter.
 - The astronomical spectrograph mounts on a telescope mount with a Vixen dovetail.
 

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  Major Components Mounted on the Spectra L200 Spectrograph
Going from the left side to the right side:
 
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The above test spectrum is dark rain clouds taken from inside the house with the Spectra L200 pointing out an open door.
 
- Screen capture of a uncalibrated spectrum image.
 - Shorter wavelenghts are on the right side of the spectrum.
 - H-alpha absorption line is the dark line at the far right where the white vertical tick is.  
 - The exposure time was 120 seconds. 
 - The white dots in the spectrum image are the hot pixels. Dark calibration will remove them.
 - Dark round shadow in the spectrum image is dust on the CCD. Flat calibration should remove it.
 - Horizontal tilted bands are from the uneven slit. Need to clean the slit with the tooth picks that came with the Spectra L200.
 - The above screen capture image is half the spectrum image resolution.
 - The CCD camera was aligned so the spectrum lines are vertical. 
 - Micrometer setting is 21.145.
 - Spectrum order is 1st.
 - Camera control software is Diffraction Limited MaxIm DL V5.07.
 

Spectra L200 Spectrograph

© 1998-2011 David Haworth