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LCLV and Adaptive Optics
Amar
IUCAA
Advisor: Prof. Ramprakash
AO Test Bench Flowchart
Sky simulator
Atmospheric
distortion
simulator
Telescope
simulator
Laser
guide star
Tip-tilt
open/close
loop
DM open/close
loop, higher
order
correction
Science
instrument
The AO test bench
(correct this schematic)
LCLV as a prospective AO
substitute
Stating the problem for higher order
corrections
•  The writing light has intensity variations
and this intensity variations is transformed
into phase variations in the reading side.
•  Need to convert the phase changes to
intensity changes effectively.
Who are the proposed candidates
•  Brewster angle concept.
•  Internal reflection concept.
•  Moire’ and Fourier transformation concept.
Whom do I prefer
•  Moire’ and Fourier transformation concept.
Brewster angle and internal
reflection concept
Moire’ and Fourier concept to
convert the phase in a 2D wavefront
into intensity variations.
What is needed ??
For a wave front with no
higher order aberrations
Transformation
Intensity
What is needed ??
For a wave front with
higher order aberrations
Transformation
Intensity
Trying Moire’ and Fourier concepts
Incident LGS
wavefront with
distortions
This is the image plane
Trying Moire’ and Fourier concepts
Reference
wavefront
Spatial negative grid
This is the image plane
Trying Moire’ and Fourier concepts
Superimpose
A Break
A Micro Channel Plate
The setup
LGS wavefront
Reference
wavefront in
lab
Superimposed
output
Low
intensity High intensity
suitable for
LCLV write sideMCP
Optics
How does the flow chart look now
AO Test Bench Flowchart
Sky simulator
Atmospheric
distortion
simulator
Telescope
simulator
Laser
guide star
Tip-tilt
open/close
loop
DM open/close
loop, higher
order
correction
Science
instrument
Reference
laser
wavefront
1
2 3 4 5
6
7
8
9
10
MCP
Science
11
16
15
13
14
23
24
25
26
27
28
29
30
31
32
17
18
19
20
2122
12
(1)  Sky Simulator Screen
(2)  Optics
(3)  Wedge
(4)  Transparency sheet or a hot plate
(5)  Optics
(6)  Optics
(7)  LGS mirror
(8)  Cassegrain secondary mirror
(9)  Cassegrain primary mirror
(10)  Folding mirror
(11)  Reference laser
(12)  Optics for reference laser
(13)  Narrow band laser frequency filter
(14)  Optics
(15)  Spatial grid
(16)  Spatial negative grid
(17)  Superimposing optics
(18)  Wavefront with local phase distortions shown up as
intensity distortions.
(19)  Microchannel Plate for light amplification suitable for
LCLV system.
(20)  Wavefront with optimum light amplification for
LCLV system
(21)  Optics
(22)  LCLV system
(23)  Folding mirror
(24)  Tip-tilt mirror
(25)  Optics
(26)  Off axis optics to shift the target light
(27)  Fold mirror
(28)  Tip-Tilt sensor
(29) Electronics for algorithm
(30) Optics
(31) Optics
(33) Fold mirror
Thank You

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LCLV front end optics

  • 1. LCLV and Adaptive Optics Amar IUCAA Advisor: Prof. Ramprakash
  • 2. AO Test Bench Flowchart Sky simulator Atmospheric distortion simulator Telescope simulator Laser guide star Tip-tilt open/close loop DM open/close loop, higher order correction Science instrument
  • 3. The AO test bench (correct this schematic)
  • 4.
  • 5. LCLV as a prospective AO substitute
  • 6. Stating the problem for higher order corrections •  The writing light has intensity variations and this intensity variations is transformed into phase variations in the reading side. •  Need to convert the phase changes to intensity changes effectively.
  • 7. Who are the proposed candidates •  Brewster angle concept. •  Internal reflection concept. •  Moire’ and Fourier transformation concept. Whom do I prefer •  Moire’ and Fourier transformation concept.
  • 8. Brewster angle and internal reflection concept
  • 9. Moire’ and Fourier concept to convert the phase in a 2D wavefront into intensity variations.
  • 10. What is needed ?? For a wave front with no higher order aberrations Transformation Intensity
  • 11. What is needed ?? For a wave front with higher order aberrations Transformation Intensity
  • 12. Trying Moire’ and Fourier concepts Incident LGS wavefront with distortions This is the image plane
  • 13. Trying Moire’ and Fourier concepts Reference wavefront Spatial negative grid This is the image plane
  • 14. Trying Moire’ and Fourier concepts Superimpose
  • 17. The setup LGS wavefront Reference wavefront in lab Superimposed output Low intensity High intensity suitable for LCLV write sideMCP Optics
  • 18. How does the flow chart look now
  • 19. AO Test Bench Flowchart Sky simulator Atmospheric distortion simulator Telescope simulator Laser guide star Tip-tilt open/close loop DM open/close loop, higher order correction Science instrument Reference laser wavefront
  • 20. 1 2 3 4 5 6 7 8 9 10 MCP Science 11 16 15 13 14 23 24 25 26 27 28 29 30 31 32 17 18 19 20 2122 12
  • 21. (1)  Sky Simulator Screen (2)  Optics (3)  Wedge (4)  Transparency sheet or a hot plate (5)  Optics (6)  Optics (7)  LGS mirror (8)  Cassegrain secondary mirror (9)  Cassegrain primary mirror (10)  Folding mirror (11)  Reference laser (12)  Optics for reference laser (13)  Narrow band laser frequency filter (14)  Optics (15)  Spatial grid (16)  Spatial negative grid (17)  Superimposing optics (18)  Wavefront with local phase distortions shown up as intensity distortions. (19)  Microchannel Plate for light amplification suitable for LCLV system. (20)  Wavefront with optimum light amplification for LCLV system (21)  Optics (22)  LCLV system (23)  Folding mirror (24)  Tip-tilt mirror (25)  Optics (26)  Off axis optics to shift the target light (27)  Fold mirror (28)  Tip-Tilt sensor (29) Electronics for algorithm (30) Optics (31) Optics (33) Fold mirror