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Edge Sensors for the Schwarzschild-Couder Telescopes David Hanna McGill University UCLA AGIS Meeting...

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Edge Sensors for the Schwarzschild-Couder Telescopes David Hanna McGill University UCLA AGIS Meeting June 26-27, 2008
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Page 1: Edge Sensors for the Schwarzschild-Couder Telescopes David Hanna McGill University UCLA AGIS Meeting June 26-27, 2008.

Edge Sensors for the Schwarzschild-Couder Telescopes

David HannaMcGill University

UCLA AGIS MeetingJune 26-27, 2008

Page 2: Edge Sensors for the Schwarzschild-Couder Telescopes David Hanna McGill University UCLA AGIS Meeting June 26-27, 2008.

The Requirement:

facets on the S-C telescopes need to be positioned to a tolerance of the order of 10 microns

light-weight optical support structure will undergodeformations of at least this scale while tracking sources

a system of actuators to dynamically correct the facets’ positions and orientations is planned

a related system to measure the facets’ positions and orientations must be developed

Page 3: Edge Sensors for the Schwarzschild-Couder Telescopes David Hanna McGill University UCLA AGIS Meeting June 26-27, 2008.

Edge Sensors

to measure the displacement of one mirror facet with respect to its neighbour we plan to use a system of position-sensitive detectors (PSDs) illuminated by diode lasers or collimated LEDs.

relative motion of the two facets causes the position of the beam spot on the PSD to be displaced; the job of the actuatorsis to move the facets in order to put the spot back to itsnominal position

light sourcePSD

beam

Mirror 1 Mirror 2

Page 4: Edge Sensors for the Schwarzschild-Couder Telescopes David Hanna McGill University UCLA AGIS Meeting June 26-27, 2008.

for the PSD, we are evaluating a lateral-effect photodiodeof the pin-cushion type ( Hamamatsu S5991).

- electrodes on the edges of the silicon photodiodecollect charges produced by the illumination of the PSD.

- ratios of currents from electrodes on opposite sides are used to calculate the centroid of the light pool.

- thus the device is non-imaging.

- shaped electrodes increase linearity near the edges and produce the pin-cushion-shaped sensitive area.

figure from Circuit Cellar(www.circuitcellar.com)

Position Sensitive Detectors (PSDs)

Page 5: Edge Sensors for the Schwarzschild-Couder Telescopes David Hanna McGill University UCLA AGIS Meeting June 26-27, 2008.

15 mm

- this PSD model is available for $30 each in large quantities.

- resolution is 1.5 m

Hamamatsu S5991

Page 6: Edge Sensors for the Schwarzschild-Couder Telescopes David Hanna McGill University UCLA AGIS Meeting June 26-27, 2008.

Light Sources:

we have two options: laser diode and light-emitting diode (LED)

LED – blue(465 nm) Optek Technology ~ $0.70

(shown here with collimator, 1 mm diameter 10 mm long)

LASER diode- red (650 nm) BEA lasers ~ $60

The LED can be made bright enough for our purposes but the forward current(80 mA) is larger than the suggested maximum (20 mA)

Probably OK since - collimator acts as a very effective heat sink- we can use the LED in a low-duty-cycle mode (needs study)

Page 7: Edge Sensors for the Schwarzschild-Couder Telescopes David Hanna McGill University UCLA AGIS Meeting June 26-27, 2008.

Hamamatsu provides a circuit for reading out the PSD.

We have carried out tests on accuracy and stability using the setup shown at the right;

the collimated LED is attachedto an X-Y-Z translation devicewhich is used to make controlledscans across the PSD

- the blue spot below the PSDshows the size of the beam spot obtained using the simple collimator

System Evaluation

Page 8: Edge Sensors for the Schwarzschild-Couder Telescopes David Hanna McGill University UCLA AGIS Meeting June 26-27, 2008.

Scan in x and y

use micrometer translator to change laser spot position on PSD

compare PSD reading with translator position

repeat to test for reproducibility

Page 9: Edge Sensors for the Schwarzschild-Couder Telescopes David Hanna McGill University UCLA AGIS Meeting June 26-27, 2008.

Overnight Stability Test

leave LED on for 16 hours

record x, y and current

sunrise

+/- 10 um

Page 10: Edge Sensors for the Schwarzschild-Couder Telescopes David Hanna McGill University UCLA AGIS Meeting June 26-27, 2008.

Electronics Developments

single PSD circuit

op-amps turn currents into voltages for ADCsto digitize

Page 11: Edge Sensors for the Schwarzschild-Couder Telescopes David Hanna McGill University UCLA AGIS Meeting June 26-27, 2008.

4-PSD op-amp board

Page 12: Edge Sensors for the Schwarzschild-Couder Telescopes David Hanna McGill University UCLA AGIS Meeting June 26-27, 2008.

Present status and future plans

PSDs and op-amp circuits now at UCLA awaiting tests on mechanical setup

new circuit which puts ADC near the op-amp (ie send digital information over cables to improve noise rejection) to be developed this summer at McGill


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