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2009 Olin Student Projects. Keith Gendreau [email protected] 301-286-6188 Phil Deines-Jones [email protected] 301-286-6884 Jeff Livas [email protected] 301-286-7289. 2009 Student Projects with contacts. Continuation of MCA Keith Gendreau

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2009 olin student projects l.jpg

2009 Olin Student Projects

Keith Gendreau

[email protected]

301-286-6188

Phil Deines-Jones

[email protected]

301-286-6884

Jeff Livas

[email protected]

301-286-7289


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2009 Student Projects with contacts

  • Continuation of MCA

    • Keith Gendreau

  • XACT Sounding Rocket Optical Bench Alignment System

    • Keith Gendreau, Phil Deines-Jones

  • UV flux monitor

    • Keith Gendreau

  • Super Webcam microscope

    • Jeff Livas

  • USB Bit Error Rate Measuring Tool

    • Jeff Livas


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Continuation of MCA project from 2008

  • In 2008, I asked the Olin students to make a “$25 MCA” to measure pulseheights and record times of X-ray events from a detector.

  • System nearly worked, but not quite…


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A PIC Microcontroller Based Pulse Detection and Measurement System

Take an input analog signal, look for pulses above a threshold, detect the peak voltage of each pulse, digitize the peak voltage, write to a file the pulse time and peak pulse height, continue….

Build on last year’s “Flux Meter”, if possible.


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X-ray Detection and Pulses System

X-ray photons

Vsignal

X-ray Detector

Amplifier

X-rays pack a lot of energy. X-ray detectors see individual X-ray photons. If the detectors and electronics are good enough, they can determine the energy of the photon.

Science is to be gained by knowing the energy of the photons and when they arrived.


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Pulses on an analog signal (from an X-ray detector) System

V

vpulse

Vpulse is proportional

to Energy of photon

Pulse widths: ~25 ns- 2µsec

t

tpulse

V

Noise pulses?

vthresh

t

Pulse#1

Pulse#2

Pulse#3


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Desired Layout: Top view System

Computer

With Olin

Software

To display/save

Events

Olin Pulse

Height Box

Analog signal

From X-ray

Detector

On a BNC

Connector

USB Output

Any type of computer, PC or Mac

(I prefer Mac, but whatever is doable)

Knob for

Lower Voltage

Threshold

Knob for

Additional

gain


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Requirements System

  • Must handle pulses ranging from ~< 100 nsec to ~ 100 microsec wide

    • Loosen requirement: Require 1-50 microseconds with a goal of 100 nsec to 100 microseconds

  • Goal of achieving ~106 counts per second (typically, it is much less than this, I’d be happy with ~104 cps)

    • Loosen requirement to ~1000 cps with a goal of 105 cps

  • Should be able to handle pulseheights ranging from ~0 to 10 volts (positive).


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Output Desires System

  • ASCII file with time and pulseheight for each event above threshold

  • Plot with histogram of pulseheights

  • Flux vs time (like on the flux meter)

  • Be creative.

  • TCP/IP port?

    • eg, The computer reading the instrument can make the data available as a server to others as client computers via a TCP/IP Sockets protocol

    • Would be an extremely useful feature for beamline work.


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For 2009 System

  • I will send you home with a detector

  • We could not get the software to work from last year.

  • Last year’s board broke at the USB connection and we now have a flaky USB board on one of our computers… (QA)


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Project #2, XACT Optical Bench Alignment System

  • We are in the initial phases of designing and building a suborbital rocket payload to do astrophysics

  • Science is realized when optics can direct photons to detectors about 3 meters away.

  • An optical bench separates the optics and the detectors…

    • Can we measure the relative alignment of these?

      • Tip/Tilt and X/Y offsets


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XACT Payload and Rocket System

Nose Cone & Recovery System

X-ray Polarimeters, Electronics, & MXS

Telemetry and ACS

Systems

Aft Cone & Door

Optical Bench

Black Brant VC

X-ray Concentrators & Star Tracker

Terrier Mk70

Overall Payload Length: 3.26 m

Payload Diameter: 52 cm*

Payload Mass: 80.2 kg (include ST)

A 1st approximation of complete XACT rocket


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Alignment System

  • X-ray optics must not shift laterally more than ~1 mm from a line connecting the source to the detector

    • Measure to 0.1 mm

  • Optics must not tilt relative to detector more than ~ 2 arcminutes

    • Measure to 1/5 arcminute


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Laser System

Position Sensitive Photodiodes

BeamSplitters


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Laser System

Lateral Shift Part

Position Sensitive Photodiodes

BeamSplitters

Tilt Part


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Components System

  • Position Sensitive Photodiodes

    • Produces analog voltage proportional to position of light centroid

    • Made by Pacific Silicon Sensor

  • Laser

  • Mirrors

  • Beamsplitters

  • “the Smarts”

    • Combines the outputs of the photodiodes and puts out 4 types of data: X and Y offset, Tip and Tilt angle



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Olin Student Job for XACT Alignment System System

  • Design full system- including the “smarts”

  • Build a prototype system using two optical benches separated by ~ 3 meters

  • Test

  • Document


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Olin student Project #4: UV flux monitor System

  • Our new modulated X-ray source uses UV light to generate photoelectrons which are accelerated into high voltage targets to make X-rays

  • We like to have absolute control of the X-ray flux, which is driven by absolute control of the UV light (from LEDs)

  • We have found some evidence of UV LED instability

  • Need a way to monitor UV flux and record it on a computer with time stamps.


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The World’s First Fully Controllable Modulated X-ray Source

  • Characteristics:

    • Rugged- no moving parts or fragile filaments- perfect for space flight.

    • Modulates x-rays at same rate that one can modulate an LED

  • Major NASA Uses:

    • Timing Calibration

    • A “flagged” in-flight Gain Calibration Source: Have calibration photons only when you want them and increase your sensitivity by reducing the background associated with the calibration photons


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Unpolarized MXS Prototype for XACT Source

HV FEED- THROUGH

QUARTZ WINDOWS (2)

BE WINDOW

UV LEDs


Slide22 l.jpg

~3 days Source


Slide23 l.jpg

Computer which reads and records data at regular intervals, or at times when there is a change.

Electronics with a UV photodiode (Mouser has several) and circuit to read it.

USB


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Objectives for Olin Summer UV Flux monitor Project 2009 or at times when there is a change.

  • Design and build UV Photodiode circuit

  • Build a USB interface

  • Write software to record data- perhaps triggered by changes in flux

  • Calibrate


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Olin student Project: $75 Diffraction-limited microscope or at times when there is a change.

“Simple” Microscope

webcam

Protective tube

Single lens


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Olin student Project: $75 Diffraction-limited microscope or at times when there is a change.

“Compound” Microscope: 2 lenses

Webcam: pixel size will limit resolution

Add on another Single lens

And maybe a support tube


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Olin student Project: $75 Diffraction-limited microscope or at times when there is a change.

  • Requirements

    • Approximately 1 micron resolution (~ 2 !)

    • Reasonable working distance (~ 10 mm)

    • Built-in calibration capability?


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Olin student Project: $75 Diffraction-limited microscope or at times when there is a change.

  • Tasks

    • Figure out single lens focal length

    • Work out required additional lens

    • Figure best-possible resolution based on number of pixels, diffraction, etc

    • Prove it!

      • http://en.wikipedia.org/wiki/1951_USAF_Resolution_Test_Chart


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0.005” = 127 or at times when there is a change.m

Olin student Project: $75 Diffraction-limited microscope

  • Out of the box:

    • Roughly 5 mils is easy

    • 1.3 Mpixel is 640 x 480 color

      • 640 x 480 x 4 = 1.3 Mpixels

  • From picture

    • guess 127 um is 1/10 x 480 = 48 pixels, or 2.6 pixels/micron (color)

Shim stock on edge


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Olin Objectives for Microscope Project: or at times when there is a change.

  • Design add on optic for current microscope

  • Build and Test

  • Update software to transfer calibration to images


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Olin student Project: Bit Error Rate (BER) Test System or at times when there is a change.

  • Idea: quantitatively measure the performance of a comm link

  • Concept: Go digital!

    • Send a pattern out with the transmitter

    • At the receiver, recover the pattern

      • May be difficult to find if many errors

      • Overall time shift not important

      • May be inverted

    • Count the errors

      • Accumulate statistics on type of error, etc


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1 or at times when there is a change.

0

0110010111

1

Error

0

Error

Olin student Project: Bit Error Rate (BER) Test System

Error types

Clock

Rx

  • Concept: Go digital!

    • Send a pattern out with the transmitter

    • At the receiver, recover the pattern

      • May be difficult to find if many errors

      • Overall time shift not important

      • May be inverted

    • Count the errors

      • Accumulate statistics on type of error

Tx

Transmitter

Noisy Channel

Noise

Receiver

0110010101

Clock recovery


Slide33 l.jpg

1 or at times when there is a change.

0

0110010111

1

Error

0

Error

Olin student Project: Bit Error Rate (BER) Test System

Error types

Clock

Rx

  • Concept: Go digital!

    • Send a pattern out with the transmitter

    • At the receiver, recover the pattern

      • May be difficult to find if many errors

      • Overall time shift not important

      • May be inverted

    • Count the errors

      • Accumulate statistics on type of error

Tx

Transmitter

Noisy Channel

Noise

Receiver

0110010101

Clock recovery


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Block Diagram or at times when there is a change.

Olin Electronics box that produces test pattern and sends it out a BNC. Box also has a BNC for the receive end

Computer with Olin Student software that prepares the test pattern for transmission, issues transmit command, and compares received to transmitted. Finally produces a BER figure

USB

BNC In

BNC out

“comm Link”


Slide35 l.jpg

Olin student Project: Bit Error Rate (BER) Test System or at times when there is a change.

  • Tasks

    • Choose test patterns, build generator

    • Develop clock recovery (PLL)

    • Develop “pattern recognition”

      • Cross-correlation based often best

    • Time shift by bits to find best fit

    • Accumulate error statistics

    • BER = number of errors/total bits sent


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Projects we probably wont do this year or at times when there is a change.


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“i-Heliograph” or at times when there is a change.

  • Can we make a low power data transmitter to send “lots” of data from the moon to the earth using a 19th century idea enhanced with 21st century technology?

  • How does such a system compare to laser communication?


Slide39 l.jpg

Replace this guy with a avalanche photodiode and an ethernet port..

Replace this guy with a high speed optical modulator and an ethernet port.


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Replacing the guy wiggling the mirror port..

  • Voltage Controlled LCD displays (KHz Speeds?)

  • Acoustic Optical Modulators (speeds up to 100 MHz)



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There should be a power savings compared to Laser Comm receive end

  • Lasers are ~10% efficient on producing optical output from electricity it gathers from ~25% efficient solar cells.

    • Total efficiency from sun = 0.25 * 0.1 = 2.5%

  • Mirrors are ~90% reflective


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Other factors in comparison receive end

  • Mass to moon

    • Do solar cells and power system with Laser weigh more than a mirror and heliostat?

  • Reliability

    • Solar panels, motors, AOMs…

    • Is dust an issue?


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2009 Olin Job receive end

  • Build a Heliostat to capture the sun

  • Pipe the light from the Heliostat through either an accoustic optical modulator or a LCD retarder

  • Build a simple pulse frequency modulator to drive the AOM or LCD retarder

  • Build a demodulator to read the output of an APD

  • Predict performance and compare to Laser Comm.


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GSFC will provide receive end

  • A telescope base to make a heliostat

  • An AOM to modulate light

  • A Circuit design to produce a FM Pulse train

  • A Telescope for the receive end

  • An APD (maybe dual use the one for the MCA project)

  • The demodulator design.



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Lunar Laser Ranging Background receive end

  • First suggested by R. H. Dicke in early 1950s.

  • MIT and soviet Union bounced laser light off lunar surface in 1960s.

  • Retroreflectors proposed for Surveyor missions but not flown.

  • Retroreflectors flown on 3 Apollo missions.


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Science of LLR receive end

Lunar ephemerides are a product of the LLR analysis used by current and future spacecraft missions.

Lunar ranging has greatly improved knowledge of the Moon's orbit, enough to permit accurate analyses of solar eclipses as far back as 1400 B.C.

Gravitational physics:

Tests of the Equivalence principle

Accurate determination of the PPN parameter β,γ,

Limits on the time variation of the gravitational constant G,

Relativistic precession of lunar orbit (geodetic precession).

Lunar Science:

Lunar tides

Interior structure (fluid core)


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Optical Communications receive end

With an optical link it is natural to use it for communications in addition to ranging.

Potentially higher capacity over large distances than RF communications.

Several methods currently under development at GSFC.


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Other applications receive end

Collision avoidance

Robotics

Delay estimation


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1 receive end

0

0110010111

1

Error

0

Error

Olin student Project: Ranging System

Clock

Rx

Tx

  • Concept: Nominally same as for BER

    • Send a pattern out with the transmitter

    • At the receiver, recover the pattern

      • May be difficult to find if many errors

      • BUT - Overall time shift IS important

      • May be inverted

    • Count the errors

      • Accumulate statistics on type of error

Transmitter

Noise

Receiver

0110010101

Clock recovery


Slide52 l.jpg

Olin student Project: Ranging System receive end

  • Tasks

    • Choose test patterns, build generator

    • Develop clock recovery (PLL)

    • Develop “pattern recognition”

      • Cross-correlation based often best

    • Time shift by bits to find best fit

    • Measure time shift to get range


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