Can we dual-purpose the laser optics for imaging? Glenn - - PowerPoint PPT Presentation

can we dual purpose the laser optics for imaging
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Can we dual-purpose the laser optics for imaging? Glenn - - PowerPoint PPT Presentation

Can we dual-purpose the laser optics for imaging? Glenn Horton-Smith 2019-08-13 Preliminary design Typically these mirrors are narrowband dichroic for high UV efficiency and suppression of longer wavelengths. But the other optics dont


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Can we dual-purpose the laser

  • ptics for imaging?

Glenn Horton-Smith 2019-08-13

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Preliminary design

Slide 7 from from Jose Maneira “laser coverage calculations” https://indico.fnal.gov/event/20979/

Typically these mirrors are narrowband dichroic for high UV efficiency and suppression of longer wavelengths. But the other optics don’t have to be narrowband. The mirror at the bottom could be broadband dielectric.

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actuator

If we can introduce an insertable/retractable mirror immediately after the upper laser

  • ptics, and have a 25 mm aperature

down to the lower mirror, we could get useful images of the interior of the cryostat with a compact, high- QE camera. A photo of an actual Prosilica low light camera with lens is shown with correct scale at right. (Closeup view next page.)

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200 mm Mirror actuator 2 9 m m 7 5 m m

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200 mm Mirror actuator 2 9 m m 7 5 m m This is drawn to scale, and the camera shown actually has an ok

  • lens. But we can do better.
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Better optics

  • Something like Orion’s CT80 80mm Compact

Refractor Telescope Optical Tube

https://www.telescope.com/Orion/Astrophotography/Astrophotography-Telescopes/

Orion-CT80-80mm-Compact-Refractor-Telescope-Optical-Tube/rc/2160/pc/-1/c/4/sc/19/p/118189.uts

– Mount vertically, with another flat diagonal.

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SLIDE 7

Image resolution

Airy disk size: θA=1.22λ/D=26 microradians Field of view: θV=D/L=6.7milliradians Radians per pixel: θp=7.0microradians Pixels per Airy disk: 3.7 (~2 times oversample) Feature resolution for object 15 m from mirror: (15 m+3.7 m) ⋅θA=0.49mm Position resolution for line or edge 15 m from mirror: (15 m+3.7 m) ⋅θp=0.13mm

Assume 532 nm wavelength, 25 mm mirror at bottom, 3.7 m from camera to mirror, 1280x960 pixel camera, field of view restricted by lower mirror, fills image. The resolution meets the inspection camera requirement. Although field of view is small in any given image, the mirror scan system would make it possible acquire multiple overlapping images to form a mosaic.

?

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Uses

  • As inspection camera:

HV surfaces: CPA, FC, etc.

Mechanical alignment check.

Surface of liquid argon seen from below, inside and outside

APA check (viewing from outside endwall only, as central ports are too close to APAs)

Interior and exterior views!

  • As laser system aid for aligning and steering the laser on small target

(e.g., for photoelectron target studies)

25 mm restriction at top and bottom of vertical path means camera image is somewhat well aligned with laser if camera can see anything.

View from camera in laser being set up serves as “viewfinder”.

One camera can also watch the targeting of another laser. If one system shines a green alignment beam (like MicroBooNE), the camera on the

  • ther system can look from a different angle and see exactly where it

hits as the system is steered.

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SLIDE 9

Light gathering power of system is low, need suitable camera

  • Many possibilities.
  • One idea would be to use an astro-imaging camera from

Orion, Celestron, SkyBig, or similar well-known company. ($200~$500)

Ex: Celestron Skyris https://www.celestron.com/products/skyris-236m

  • In addition to working at low light with good focal

properties, these often come with software designed to correct for frame to frame image shifts and blurring caused by viewing through a moving fluid.

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SLIDE 10

A couple of examples

1.25 in 5 m m 5 m m 60 mm 1.25 " 2 " 2.25 "

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Example optics

(shorter and higher quality can be obtained, but this could be adequate for purpose)