Quote:
Originally Posted by multiweb
Edmund optics had a 5" deformable mirror with electronics and SDK a couple of years ago. But you have to do everything yourself.
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Was this advertised on April 1st?
With the demise of CCD's sadly things are going one step forward and two back, as often happens when accountants influence engineering.
The original SBIG AO was not as Bill suggests ".... commercial AO boxes that only correct for mount imperfections"
When its control software ran under DOS, the system could achieve 40Hz tip-tilt corrections to the incoming wavefront.
This is the first order AO correction that even higher order professional systems must apply.
These finely calibrated units often cost $$ to send back for correcting "defects" purely due to rough handling by FedEx/UPS etc. hence commercially had issues from the get go.
The introduction of Windoze95 slowed it down a tad, with 30Hz being more
typical. Then the design was made more robust by the use of a refractive element, but that slowed corrections by a factor of two i.e. 15Hz.
That said, 15Hz guiding can and does improve FWHM's by a good 30%
First order AO works well on nights of "slow seeing". But when guide-stars start to look like fuzzballs, sure the system has few practical benefits.
It's also worth noting, it would nigh impossible to guide a telescope + mount at 15Hz.
I regularly watch the atmosphere bounce around guide stars in Ra and Dec, that my AO-X quickly calms....
but to get 150Kg of Telescope/Mount/Counterweights etc. to ignore inertia and move at the same rate and be passed off as "mount imperfections"
sorry...I simply can't agree as being an accurate description of the physical reality