Curvature Wavefront Sensor Arbitrary Waveform Generator Kenyan Kawauchi Subaru Telescope (NAOJ)...

14
Curvature Wavefront Curvature Wavefront Sensor Arbitrary Sensor Arbitrary Waveform Generator Waveform Generator Kenyan Kawauchi Kenyan Kawauchi Subaru Telescope (NAOJ) Subaru Telescope (NAOJ) Mentor: Stephen Colley Mentor: Stephen Colley

Transcript of Curvature Wavefront Sensor Arbitrary Waveform Generator Kenyan Kawauchi Subaru Telescope (NAOJ)...

Page 1: Curvature Wavefront Sensor Arbitrary Waveform Generator Kenyan Kawauchi Subaru Telescope (NAOJ) Mentor: Stephen Colley.

Curvature Wavefront Sensor Curvature Wavefront Sensor Arbitrary Waveform GeneratorArbitrary Waveform Generator

Kenyan KawauchiKenyan Kawauchi

Subaru Telescope (NAOJ)Subaru Telescope (NAOJ)

Mentor: Stephen ColleyMentor: Stephen Colley

Page 2: Curvature Wavefront Sensor Arbitrary Waveform Generator Kenyan Kawauchi Subaru Telescope (NAOJ) Mentor: Stephen Colley.

Subaru Adaptive OpticsSubaru Adaptive Optics

Earth’s atmospheredistorts light

Telescopeimages blurred

Removes effectsof atmospheric

distortion

Image resolutionimproved

Without AO With AO

Page 3: Curvature Wavefront Sensor Arbitrary Waveform Generator Kenyan Kawauchi Subaru Telescope (NAOJ) Mentor: Stephen Colley.

AO System ComponentsAO System Components

Page 4: Curvature Wavefront Sensor Arbitrary Waveform Generator Kenyan Kawauchi Subaru Telescope (NAOJ) Mentor: Stephen Colley.

Wavefront SensorWavefront Sensor

Visible light reflectsoff one sideof membrane

Measure lightintensity

APDs count photonsin each lenslet

Calculate wavefrontphase shift

Page 5: Curvature Wavefront Sensor Arbitrary Waveform Generator Kenyan Kawauchi Subaru Telescope (NAOJ) Mentor: Stephen Colley.

What vibrates membrane?What vibrates membrane?

Other side of membrane

Page 6: Curvature Wavefront Sensor Arbitrary Waveform Generator Kenyan Kawauchi Subaru Telescope (NAOJ) Mentor: Stephen Colley.

ProblemProblem

Page 7: Curvature Wavefront Sensor Arbitrary Waveform Generator Kenyan Kawauchi Subaru Telescope (NAOJ) Mentor: Stephen Colley.

SolutionSolution

• Design your own AWG!

• Use DAC40 board

• Field Programmable Gate Array (FPGA)

• Digital-to-Analog Converters (DACs)

Page 8: Curvature Wavefront Sensor Arbitrary Waveform Generator Kenyan Kawauchi Subaru Telescope (NAOJ) Mentor: Stephen Colley.

AWG SpecificationAWG Specification Range of period – 100 Hz to 4 kHzRange of period – 100 Hz to 4 kHz Number of points – 1000Number of points – 1000 Voltage resolution – 14 bits (DAC40 DACs) Voltage resolution – 14 bits (DAC40 DACs) Update rate for new waveforms – 0.1 seconds Update rate for new waveforms – 0.1 seconds

(10 Hz)(10 Hz)

Voltage Amplitude

Time

Page 9: Curvature Wavefront Sensor Arbitrary Waveform Generator Kenyan Kawauchi Subaru Telescope (NAOJ) Mentor: Stephen Colley.

Logic Block DiagramLogic Block Diagram

AWG

Timing Memory

A B

Page 10: Curvature Wavefront Sensor Arbitrary Waveform Generator Kenyan Kawauchi Subaru Telescope (NAOJ) Mentor: Stephen Colley.

Implement using Quartus IIImplement using Quartus II

Page 11: Curvature Wavefront Sensor Arbitrary Waveform Generator Kenyan Kawauchi Subaru Telescope (NAOJ) Mentor: Stephen Colley.

Design FlowDesign FlowDesign Entry

(VHDL)Compilation Simulation

ProgramDevice

Page 12: Curvature Wavefront Sensor Arbitrary Waveform Generator Kenyan Kawauchi Subaru Telescope (NAOJ) Mentor: Stephen Colley.

Simulate DesignSimulate DesignDesign Entry

(VHDL)Compilation Simulation

ProgramDevice

Page 13: Curvature Wavefront Sensor Arbitrary Waveform Generator Kenyan Kawauchi Subaru Telescope (NAOJ) Mentor: Stephen Colley.

ConclusionConclusion

Dual-stroke waveform conceptDual-stroke waveform conceptEfficient – Only 1 wavefront sensorEfficient – Only 1 wavefront sensorAstronomical objects appear 2.5X brighterAstronomical objects appear 2.5X brighter

In the FutureIn the Future- Interface DAC40 to oscilloscopeInterface DAC40 to oscilloscope- Test AWGTest AWG- Implement in next generation AO systemImplement in next generation AO system

Page 14: Curvature Wavefront Sensor Arbitrary Waveform Generator Kenyan Kawauchi Subaru Telescope (NAOJ) Mentor: Stephen Colley.

AcknowledgementsAcknowledgements

Stephen ColleyStephen ColleyOlivier Guyon – Subaru AstronomerOlivier Guyon – Subaru AstronomerHideki Takami – AO Project ManagerHideki Takami – AO Project ManagerSubaru Telescope (NAOJ)Subaru Telescope (NAOJ)Center for Adaptive OpticsCenter for Adaptive Optics Funding provided through the Center for Adaptive Funding provided through the Center for Adaptive

Optics, a National Science Foundation Science and Optics, a National Science Foundation Science and Technology Center (STC), AST-987683Technology Center (STC), AST-987683