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François Piché August 16, 1999 Introduction Procedure Results Conclusions Acknowledgements 1. Introduction
This is a short report on the work performed on setting piston of the HET mirror. It
also presents data taken to test the accuracy of the final product. This work was performed between February 9th to February 14th, 1999. The spherometer has been upgraded by replacing the dial indicator with a Chicago Dial digital indicator with RS-232 data download capability. We set the indicator resolution to 5 μm throughout the alignment. Most of the segments were measured with a hanging operator, some measurements of edge segments were done with the operator standing on the truss. Prior to start, the state of the mirror was as follows:
The segments were left in a stacked status at the end of the previous night work. The dome was conditioned until piston alignment was performed in the afternoon. It is estimated that the stack alignment remained within 5 arcseconds (mirror) during piston alignment (i.e a possible influence of 12.5 μm on piston measurements). Segments were measured with respect to only one of their neighbor with little cross-checking. Whenever cross checking was performed the piston measured was within the ±25 μm requirement specs. 3. Results
Figure 1 shows the measurements pattern used and the piston adjustments that
were applied. The RMS value of the piston adjustments applied as measured from rings 1 to 3
segments (minus segment 16) was ±150 μm RMS. We do not include ring 4 - 5 segments
in this calculation as the number of segments that needed to be roughed in would
distort the statistics and are unreliable of how the mirror is holding piston
alignment. It seems fairly safe to ascertain that once properly pistoned the
mirror holds
its piston figure to within ±200 μm
RMS over extended period of time (months). As can be noted from the underlined numbers distribution in Fig. 1, it was surprising to find at least 6 segments that had been previously pistoned, had not been re-installed, and still needed roughing-in. A possible explanation for this state of affair is that all six segments sit next to a solid month segment. It is plausible that during installation of the solid mount segments, these neighboring segments were disturbed somehow.
Another item of note is that when performing large piston moves (i.e. 300 to
500 μm), it was often found
that applying a correction of the same size as the measured piston misalignment
would actually overshoot by approximately 5%. This might indicate a need to alter
the lever arm
ratio number in SPS. At the completion of piston alignment, the mirror piston figure is approximately ±50
μm
RMS (±100 μm RMS if one wants to be conservative). This should contribute only
about
0.12” (0.23”) to sky imaging quality (not taking into account possible systematic global
asphericity of the primary mirror figure).
Again thanks to everybody that was involved in this effort: Grant Hill, Matthew
Shetrone, Craig Nance, Paul Worthington, Jim Fowler, and Jerry Martin.
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