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chara:discussion_of_alignment_procedures [2024/07/10 19:03] gail_stargazer |
chara:discussion_of_alignment_procedures [2024/07/10 19:35] (current) gail_stargazer |
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* If coma and astigmatism high, create sky flat on bright star - Turn off **[DM]**, **[SV FLT]**, **[FLATEN]**, | * If coma and astigmatism high, create sky flat on bright star - Turn off **[DM]**, **[SV FLT]**, **[FLATEN]**, | ||
* For IR combiners, move beacon flat to align star to STST. | * For IR combiners, move beacon flat to align star to STST. | ||
- | * For SPICA, move beacon flat to align star on SPICA FTT. <font inherit/ | + | * For SPICA, move beacon flat to align star on SPICA FTT. <font inherit/ |
- | * <font inherit/ | + | * <font inherit/ |
+ | * Star Acquired. | ||
+ | | ||
==== Proposed Revisions to Current Alignment Sequence ==== | ==== Proposed Revisions to Current Alignment Sequence ==== | ||
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Note that we went back and redid all of the alignments of W1 at stow with M7 and flats set to default, just to confirm that the vignetting mentioned above was not the result of moving dichroic vs M7. | Note that we went back and redid all of the alignments of W1 at stow with M7 and flats set to default, just to confirm that the vignetting mentioned above was not the result of moving dichroic vs M7. | ||
- | Here is a pdf with some screenshots: | + | Here is a pdf with some screenshots: |
Gail | Gail | ||
+ | |||
+ | __**Engineering Report from UT 2024May16**__ | ||
+ | * E1 - AO engineering + obsgtk integration | ||
+ | * Comparison of M7 vs Dichroic alignment tests with SPICA | ||
+ | * UT 04:24 HD 113226, EL 64 deg, AZ 150 deg - M7 alignment (adjust boxes) | ||
+ | * UT 06:00 - dichroic alignment | ||
+ | * UT 07:20 HD 113226, EL 53, AZ 239 deg - realign at stow, go back to M7 align | ||
+ | * video of telao on and off | ||
+ | |||
+ | First night with AO running on all 6 telescopes (after W2 DM installation): | ||
+ | |||
+ | **Notes from Gail:** | ||
+ | |||
+ | We took a short video last night comparing the spots on the Six Telescope Star Tracker (J-band) with the AO on versus AO off. There' | ||
+ | |||
+ | The video starts with AO on. Then the AO servo' | ||
+ | |||
+ | **Notes from Denis:** | ||
+ | |||
+ | I have posted some SPICA images recorded during the same engineering tests. They can be viewed on this link: | ||
+ | |||
+ | [[https:// | ||
+ | |||
+ | For all sequences, we have, from left to right, E1-W2-W1-S2-S1-E1. Images are 10ms exposure and the gifs are ' | ||
+ | |||
+ | * 04-56-44: initial situation after opening and standard alignment. Large residual static aberrations on W2W1 clearly. Flux on E's is much less than others. Flat on W1, W2 does not improve the situation. | ||
+ | * 06-31-05: We did a stow, then M7 to default, and then dichroic alignment. Situation is better (but seeing may have evolved in the meantime). | ||
+ | * 07-15-03: BF/M7 alignment. The TopLeft-BottomRight elongation is related to the atmospheric refraction (zenithal distance ~40°). | ||
+ | * 07-30-33: same record close loop | ||
+ | * 07-34-41: record open loop | ||
+ | |||
+ | From the last record, it can be seen that the seeing was really poor. The encircled energy computation goes from 3% (open loop) to 7-8% in close loop. We are still far from 25% as expected but the atmospheric refraction (not yet compensated) is also a limitation of course, as well as the seeing conditions. Many beams have residual static aberrations, | ||
+ | |||
+ | Qualitatively and with these conditions, I do not see obvious difference between the two methods of alignment for the AO performance. It's great to have all 6 AO working now. | ||