MagAO Commissioning Day 11: A calibration riddle

Here’s a riddle for all you AO fans out there:

What aberration can be sensed but not corrected?

Usually an AO system has the opposite problem: There are aberrations you can correct but not measure.  And of course, there are all sorts of aberrations you can neither measure nor correct, like the very highest spatial frequencies. (And if you don’t have enough stroke, you can saturate your attempt to correct an aberration — but that wasn’t the case today.)

Contemplating and debating the riddle

But today while we were making our interaction matrices, we found we had 3 high spatial frequency dots in our pupil images (a couple times the size of an actuator) and we spent some time trying to track down whether they were phase or amplitude, and whether it was a dirty optic, scattered light, or misalignment.

Pato takes Enrico up in the scissor lift to inspect the optics

Jared had to power-cycle the CRO controller, and so he and Armando went up on the scissor lift to check if the CRO was in the right position and to inspect the optics.

Jared and Armando on the scissor lift, checking if the CRO motors are working properly

When we closed the loop, these “dots” could not be corrected.  We tried shifting some optics to see if we could move the spots, and we concluded they weren’t an amplitude error (too bright).  Finally, we tried setting the ASM back to an older flat shape — and the dots disappeared!  This means that these phase errors were somehow introduced to the system at the time we were calibrating the interaction matrices.  So then when we closed the loop, we were driving toward that shape — not toward a true flat.

So the answer to the riddle is, the shape you can measure but not correct is an error in your null!

Now that we’ve solved the riddle, tomorrow we’ll re-do our interaction matrices with a flatter null.

Vizzy contemplates the calibration riddle from her perch

Yesterday:

Simone: “Hey, I think we should try taking the pyramid out.”
Laird: “No.”
Armando: “No.”
Phil: “No.”
Jared: “No.”
Katie: “What? Is he serious???”

Today:

Laird: “Hey, maybe we should try taking the pyramid out.”
Simone: “No.  The last thing we want to do is take the pyramid out!”

MagAO pupils and Fourier optics

Today we are going to explore the MagAO pupils and their corresponding transforms in the image plane, courtesy of Fourier optics.

So let’s have a look at the pupil.  Here is a photo of the ASM, taken with a digital camera.  This was from before Clio was mounted, so that we just stood on the Nasmyth platform and put the digital camera where Clio is now.  The light source is the sky, and the light path is primary + secondary + tertiary.

ASM image, from before Clio was mounted. You can see bird poop on the tertiary, a splotch at about 11:00 in this image, and the lollipop-shaped "slot" is at 9:00.

The main features of the pupil are the outer diameter of the mirror, the inner diameter of the secondary obscuration, the support spiders holding up the secondary, and the slot.  Here, then, is the pupil mask:

Pupil mask

Since we know what the pupil looks like, we can create simulated images of the focal plane by taking the Fourier transform modulus squared:

What the PSF will look like in the image plane (log scale)

If we really stretch the color table, you can see the diffraction off the spiders, but it is not a big effect.  Also, I couldn’t find the diffraction off the slot, so it is negligible:

Stretching the color table to saturate the inner part of the PSF allows you to see the diffraction spikes off the spiders, but they are very faint

Now, Clio is an infrared camera, going out to 5 um, and so it has its own pupil mask, a cold stop.  So let’s look at the pupil through Clio, by taking a pupil image (which we did after Clio was mounted).  Here is an image of the pupil plane through the whole system, taken with Clio by putting in a powered lens to the focal plane to make a pupil image:

Clio pupil image, 3.4 um

It’s pretty cool because you can see the 2 spiders holding up the secondary obscuration on the cold stop, but you can also see the 4 telescope spiders and the ASM slot!  Here’s just the Clio cold stop pupil mask:

Pupil mask - Clio cold stop

And here is its Fourier-transform-modulus-squared: The simulated PSF:

Simulated PSF for Clio cold stop (log scale). Diffraction off the spiders is a little bit visible here, since they are slightly wider than the telescope spiders.

And here is the zoomed-out, saturated version so that you can better see the diffraction spikes:

Clio cold stop PSF -- scaled to bring out the diffraction spikes.

Summary:

Top: ASM slot + telescope spiders pupil image and mask. Bottom: Clio cold stop image + pupil mask.
Top: ASM slot + telescope spiders PSF. Bottom: Clio cold stop PSF.

The two simulated PSFs look very similar, and diffraction off the spiders and slot has a very minimal effect compared to the Airy rings.

For Alan

Alan Uomoto has been teaching us about the power supply at LCO.  Rather than calling it clean and dirty, the actual difference between the different circuitry is whether they go direct (white outlets) or through an un-interuptable power supply (UPS) (orange outlets).  Alan, this one’s for you!
Before Alan
After Alan

(And — despite how it looks from the outlets — we really are in Chile!  The observatory is highly USA-compatible.  I haven’t even used my plug adaptor yet!)

Update: And here is the MagAO-certified power protector I made to keep people from stepping on the plugs and cords above:

Power cords protector, standing around the plugs imaged above

MagAO Commissioning Day 9 – Nighttime Edition: Incorporating Clio

Today was a busy day, and we began splitting MagAO’ers into day and night crew.  See Derek’s awesome post for the bulk of the day’s tasks: aligning the CRO and ASM.

The next major happening was mounting Clio to the NAS.  Even though we didn’t play the theme from Top Gun as we did it (sorry Phil!), it was an exciting moment.  This is the first time our infrared camera officially met our optical camera and our AO system!  They are together at the telescope at last!

Clio, VisAO, W-unit, Nas, ASM, Clay: So happy together!

Here’s how it happened:

Removing Clio from the support cart with the crane — under PI Phil's watchful care
Attaching Clio to the NAS ring — under Phil's watchful care
Clio at the Nas, flanked by Phil and Katie
Left: Phil and Clio instrument. Right: Clio electronics rack and Phil.

Phil, Katie, and Laird then aligned Clio’s cold pupil stops to the ASM.

Heave-ho: Shimming Clio to align the cold stops
How's it look, Phil?

LCO crew were busy as always, making everything work smoothly for the run.  Here, Mauricio brings up LN2 to fill Clio’s dewar, and Pato optimizes the PID loop that rotates the Nas while the telescope tracks and slews:

Mauricio brings up LN2 to the Nas platform to fill the Clio dewar
Pato feels for vibrations as he optimizes the PID loop tracking and slewing the Nas rotater

 

Quotes:
Alfio: “What is this mirror cover?”
Laird: “Oh you’re so cute Alfio.”

Phil:  “I don’t lean on Clio.”

Phil:  “Used to be, we only had 1 actuator.”

Povilas: “Can 14 mm be considered a shim? That’s more like a structural member.”

Simone has a key to Galileo's house.

Katie: “Hey Jared, how’s it going with the CRO?”
Jared: “I dunno. It’s all in Italian.”

Jared: “The number of Illuminati asking me questions is daunting.” (That would be Simone Esposito himself, as well as suspected members Laird, Phil, and Armando — see our paper for more info.)

 

Armandino

Jared: “I’m pretty sure I would throw myself off the catwalk if Armando thought it would help.

MagAO Commissioning Day 8: Shim shine.

Today was the first day with all the big guns:

From left: Laird Povilas Simone Phil Armando

We shimmed the ASM to put it in the middle of the range for collimation and focus.

Laird checking the shim calculations

Alfio and Jared tested the Bayside stages for collisions with the telescope — all clear.

Screen shot of VisAO working on the Clay telescope. This is our 1 micron PSF behind our occulting spot.

Phil has been checking Clio out in the clean room, testing the motors, homing, and taking internal pinhole images.

ASM (upper left) and as viewed through the NAS

Tonight – Povilas is working on the pointing model for the telescope.

This is to satisfy requests from our various mothers to see the dorms.

Quotes:

Derek: And then we make a real-time Zemax model.  I was born for this.

Laird: Hey Jared… while you’re looking at the blog… remember to look at your data!