laser production for nasa's global ecosystem dynamics ...€¦ · qs = q-switch 1/4 wp = 1/4...

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Laser Production for NASA's Global Ecosystem Dynamics Investigation (GEDI) Lidar SPIE DSS April 19, 2016 Paul R. Stysley , D. Barry Coyle, Greg B. Clarke, Erich Frese, Gordon Blalock, Peter Morey, Richard B. Kay, Demetrios Poulios, Michael Hersh NASA-Goddard Space Flight Center 1 https://ntrs.nasa.gov/search.jsp?R=20160005285 2020-06-02T15:15:47+00:00Z

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Page 1: Laser Production for NASA's Global Ecosystem Dynamics ...€¦ · QS = Q-Switch 1/4 WP = 1/4 wave plate GRM = gradient (Gaussian) reflective mirror 1. HR mirror prescription change

Laser Production for NASA's Global Ecosystem Dynamics

Investigation (GEDI) Lidar

SPIE DSS April 19, 2016

Paul R. Stysley , D. Barry Coyle, Greg B. Clarke, Erich Frese, Gordon Blalock, Peter Morey, Richard B. Kay,

Demetrios Poulios, Michael Hersh

NASA-Goddard Space Flight Center

1

https://ntrs.nasa.gov/search.jsp?R=20160005285 2020-06-02T15:15:47+00:00Z

Page 2: Laser Production for NASA's Global Ecosystem Dynamics ...€¦ · QS = Q-Switch 1/4 WP = 1/4 wave plate GRM = gradient (Gaussian) reflective mirror 1. HR mirror prescription change

• NASA Earth Ventures Instrument (EVI) program

• $90 M , cost capped, “PI-Led” mission

• Class C, 1-2 year mission

• Multi-beam waveform lidarinstrument with 10 ground tracks

• Launch Vehicle: Space-X Falcon 9/Dragon or equivalent

• Platform: International Space Station,

• Japanese Experiment Module Exposed Facility, Site: EFU#6

• Orbit: 415 km average; 51.6 degrees

• Payload Allocations (TBR): 600 Kg., 887 W, 5.4 Mbps

• Science and Mission Operations Ground System, B.32 GSFC

2

GEDI Mission Overview

2015 2016 2017 2018 2019 2020

SRR

6-15

PDR

4-16

CDR

1-17

PER

8-17

PSR

5-18

LRD

8-18

Primary Mission:

365 Days of

Science Collection

Extended Mission

to Account for ISS

Induced Downtime

Page 3: Laser Production for NASA's Global Ecosystem Dynamics ...€¦ · QS = Q-Switch 1/4 WP = 1/4 wave plate GRM = gradient (Gaussian) reflective mirror 1. HR mirror prescription change

3

Science Goal

GEDI provides the Earth’s first comprehensive

and high-resolution data set of ecosystem structure

C A R B O N C Y C L E B I O D I V E R S I T Y

Characterize the effects of

changing climate and land use on ecosystem

structure and dynamics

Page 4: Laser Production for NASA's Global Ecosystem Dynamics ...€¦ · QS = Q-Switch 1/4 WP = 1/4 wave plate GRM = gradient (Gaussian) reflective mirror 1. HR mirror prescription change

• Sole GEDI observable is the lidar waveform

- Provide ground elevation, canopy height, canopy cover and various vertical profiles and metrics

4

Lidar Measurement

Page 5: Laser Production for NASA's Global Ecosystem Dynamics ...€¦ · QS = Q-Switch 1/4 WP = 1/4 wave plate GRM = gradient (Gaussian) reflective mirror 1. HR mirror prescription change

• GEDI is self-contained laser altimeter

• 3 lasers produce a total of 10 ground tracks

• Precise ranging, attitude & position sensors enable precise geo-location of each laser footprint (10-m knowledge)

• Active Pointing Control Mechanism (PCM) provides even distribution and complete coverage of ground tracks (225-m control)

5

GEDI Laser Ground Track Coverage

Canopy Coverage

Laser

Dense Canopy Laser

60 m

Canopy Coverage

Laser

5.4 km600 m

1 2 3 4 5 6 7 8 9 10

Page 6: Laser Production for NASA's Global Ecosystem Dynamics ...€¦ · QS = Q-Switch 1/4 WP = 1/4 wave plate GRM = gradient (Gaussian) reflective mirror 1. HR mirror prescription change

6

GEDI Instrument

+Z_GEDI

+Y_GEDI

+X_GEDIGPS Antenna

Star Tracker #2

Star Tracker #3

Star Tracker #1

FRGF

H Fixture

PIU

SpaceXPassive FSE x 4

Page 7: Laser Production for NASA's Global Ecosystem Dynamics ...€¦ · QS = Q-Switch 1/4 WP = 1/4 wave plate GRM = gradient (Gaussian) reflective mirror 1. HR mirror prescription change

7

GEDI – Internal Views

Pointing Control Mechanism

PIU

4X Accumulator

3X Laser

3X BDU 3X TOA

Sun Shade

Deployed Aperture Cover

Star Tracker #1 Star Tracker #3

Star Tracker #2

Page 8: Laser Production for NASA's Global Ecosystem Dynamics ...€¦ · QS = Q-Switch 1/4 WP = 1/4 wave plate GRM = gradient (Gaussian) reflective mirror 1. HR mirror prescription change

8

GEDI Optical Bench

Star Tracker # 2

Star Tracker # 3

Star Tracker # 1

Laser # 2

Laser # 1

Laser # 3

BDU #1

BDU #2

BDU #3

TOA #3

TOA #2

TOA #1

RTA

Page 9: Laser Production for NASA's Global Ecosystem Dynamics ...€¦ · QS = Q-Switch 1/4 WP = 1/4 wave plate GRM = gradient (Gaussian) reflective mirror 1. HR mirror prescription change

Laser Optical Design Overview

HR(2.5 mROC)

RisleyPair

TCL

Nd:YAG Slab(7x4 bar LDAs)

22 bounce2.68 thick x 26.5o tip angle

RisleyPair

Q-Switch

TFP1/4 WP

GRM(-2.37 mROC)

40 cm

HR(1.0 mROC)

RisleyPair

TCL

Nd:YAG Slab(7x4 bar LDAs)

22 bounce2.68 thick x 26.5o tip angle

RisleyPair

Q-Switch

TFP1/4 WP

GRM(-2.37 mROC)

GEDI Pre-SRR /HOMER-2

GEDI-Laser

HR = high reflective mirrorTCL = thermal compensation lensTFP = thin film polarizerQS = Q-Switch1/4 WP = 1/4 wave plateGRM = gradient (Gaussian) reflective mirror

1. HR mirror prescription change 2.5 mCC to 1.0 mCC

2. The TCL focal length is “adjusted” for each cavity or slab

installed, to best match thermal lensing. (TCLs ordered

at a range anyway)

3. Mini-BX added to adjust for change in divergence

4. Reduction in output power from 17 mJ to 10 mJ to

maintain same damage margins

5. Reduction of power allocation from 50 W to 40 W

12

9

17 mJ

10 mJ

34

5

BX

Page 10: Laser Production for NASA's Global Ecosystem Dynamics ...€¦ · QS = Q-Switch 1/4 WP = 1/4 wave plate GRM = gradient (Gaussian) reflective mirror 1. HR mirror prescription change

10

HOMER Class Heritage and Philosophy

Design:-Model-Best practices-Margins

Bread Board:• Confirm basic performance• Confirm “laser physics” margins• COTS parts

Hardened bread boards/EDUs:• Confirm mechanical margins• Environmental/Life Testing

ETUs:• Flight-like procedures• Test to flight levels• Life testing

To FlightAny change to laser is checked for impact to performance and margins

HOMER Breadboard

HOMER-1

HOMER-2

GEDI Laser

Page 11: Laser Production for NASA's Global Ecosystem Dynamics ...€¦ · QS = Q-Switch 1/4 WP = 1/4 wave plate GRM = gradient (Gaussian) reflective mirror 1. HR mirror prescription change

11

HOMER TRL-6 Performance Summary

Titanium Flexures (X3)

HRM

Sealed Enclosure w/Dual Monitoring Windows

GRM Laser HeadActive Q-Switch

Optical Bench Truss, Removable for FullOut-of-Box Alignment

F(cyl) = -62cm Lens

Conductive Thermal Control

Flexure bonding LDA pedestal to optical bench

Zoom

Single Mode Far Field ImageDx/Dy = 0.99/0.96 mRad

Laser Settings:

• Diode Pulse = 65us

• I = 48 A (~55% derated)

• F = 241 Hz

HR mirror Near Field Image Wx/Wy = 1.8/2.12 mm

Laser Output:

• E = 16 mJ

• Q-switch pulse ~11ns

• Fluence < 2.5 J/cm2

Reported 01/06/2010

Parameter HOMER Output

Energy 20 - 15 mJ

Pulse Width 12 +/- 1 ns

Rep Rate 250 -100 Hz

LDA Current 48-80 A

LDA Derating 50%

TRL 6 Mass 6 kg

Total QS Shots

HOMER Design15+ Billion

Page 12: Laser Production for NASA's Global Ecosystem Dynamics ...€¦ · QS = Q-Switch 1/4 WP = 1/4 wave plate GRM = gradient (Gaussian) reflective mirror 1. HR mirror prescription change

12

GEDI Laser Interface and Functional Overview

TelemetryTemperature x5

Pressure x2 QS Voltage

808 nm

~3.5 kV at 242 Hz

12 VTrigger 242Hz

LEU

ISS Flow/TEC35 +/- 2 °C

To BDU

~10 mJ/1064 nm

> 16 ns

0 to 50 A40 -100 us

Trigger 242 Hz

Q-switch Driver

Laser Enclosure

Laser Optical Bench Laser Pump Module

Start Pulse

Pickoff

The Laser module consists of:

1. Laser Cavity (pump module, laser bench)

2. Pressurized Mechanical Housing

3. Q-Switch Drive Electronics

Mini Beam ExpanderTi Flexures

Page 13: Laser Production for NASA's Global Ecosystem Dynamics ...€¦ · QS = Q-Switch 1/4 WP = 1/4 wave plate GRM = gradient (Gaussian) reflective mirror 1. HR mirror prescription change

13

GEDI Laser Mechanical Overview

GRM

RisleyPair

¼ Waveplate

KD*P Q-Switch

Laser Head“Bridge”

HR

Cyl Lens

RisleyPair

Laser Diode Array“Pedestal”

Tool Access

Optical Bench

Thin FilmPolarizer

40 cm Cavity Length from mirror to mirror

• Incorporating all opto-mechanical lessons learned from HOMER-2, LOLA, MLA,

CALIPSO, DESDYNI, & ESA’s ALADIN

• Modular design allows complete laser assembly, alignment, and substantial

performance without the enclosure if necessary

• Preliminary leak rate, structural, and thermal analysis performed and will be tested

20.5 ” 9.125 ”

6.25 ”

Page 14: Laser Production for NASA's Global Ecosystem Dynamics ...€¦ · QS = Q-Switch 1/4 WP = 1/4 wave plate GRM = gradient (Gaussian) reflective mirror 1. HR mirror prescription change

BDU Design Overview

KD*P Pockels cell mounts with pitch, yaw, and roll adjustments

Rotatable 1064nm half-wave plate mount

Rotatable/lockable YVO4

wedge mount

Enclosure Model

Fused SiO2 AR-coated windows

BDU enclosure

Open Model

CBE Total Mass: ~1.81 kgAll optics, mounts, sensors, and seals (except the wedge) are either directly using or leveraging parts already being using in the HOMER laser

Telemetry:IEU- Tempe x2

LEU- Pressure x2 LEU- QS Monitor

LEU: 12 VTrigger 242Hz (DU)

Q-Switch Driver

3.5 kV at 242 Hz

10 mJ from Laser

Page 15: Laser Production for NASA's Global Ecosystem Dynamics ...€¦ · QS = Q-Switch 1/4 WP = 1/4 wave plate GRM = gradient (Gaussian) reflective mirror 1. HR mirror prescription change

Side Lobe Description Summary

X-axis

Y-axis

The image file is imported into a gaussian analysis model to integrate over the profiles, the quantify % energy in side lobe.

Beam Image of Slab Exit:

A few rays at “top” of Y-axis travel a different path.

This produces a clipping effect, or “lobe” at the

slab output end.

This creates problems for science differentiating

between sloped ground and tree height.

To remove this you can either:

1) Clip off the side lobes outside the cavity

2) Make the beam smaller

3) Make the slab bigger

All options were explored and GEDI selected

option 2 by changing HR Mirror curvature.

Options were reviewed externally by NESC supervised laser team from 554, 562, and expert from NGS.See GEDI-LAS-REVW-0004

Side lobes

Page 16: Laser Production for NASA's Global Ecosystem Dynamics ...€¦ · QS = Q-Switch 1/4 WP = 1/4 wave plate GRM = gradient (Gaussian) reflective mirror 1. HR mirror prescription change

Laser Testing Performance Summary

Parameter Value Unit

AverageEnergy

10.2 mJ

Frequency 242 Hz

Pump Width 71-77 μs

Current 55 A

1000m470m

Inspection Point

2000m

Calibration Point

470m330m 700m 1000m

220m

3200m2700mLDA Turned Up

3200m

HOMER-1 1 mCC HRM Life Assessment Testing

No additional damage found

HOMER-1 sensitive to temperature

10 mJ example beam with

no side lobes from GEDI-

LAS-RPT-0029

Parametric Testing :• Thermal lensing• Diode distance• End mirror tolerance

Page 17: Laser Production for NASA's Global Ecosystem Dynamics ...€¦ · QS = Q-Switch 1/4 WP = 1/4 wave plate GRM = gradient (Gaussian) reflective mirror 1. HR mirror prescription change

ETU Diode Life Test Results

Energy measurements were corrected for the LDA temperature change. Efficiency of the LDA decreases as the temperature increases.

Voltage drop change

Took diodes off for 1B Shot inspection and DPA

Voltage drop correction

Diodes re-inpsected several times thru testing. No damage or unexpected change in performance

Page 18: Laser Production for NASA's Global Ecosystem Dynamics ...€¦ · QS = Q-Switch 1/4 WP = 1/4 wave plate GRM = gradient (Gaussian) reflective mirror 1. HR mirror prescription change

18

Cavity Fluence Estimates

HR

RisleyPair

TCL

Nd:YAG Slab

RisleyPair

QS

TFP1/4 WP

GRM

… To get the operational damage margin for each optic:

MD =jLIDT /jcalc

HR RisleyPair

TCL Slab Face

Slab TIR Slab Face

TFP QS ¼ WP

RisleyPair

GRM

Meas LIDT (J/cm2)

11.5 44 25 >10 12* >10 20 >10 >10 44 4

Calc Fluence(J/cm2)

1.75 1.95 2.08 2.37(1/2.23)

2.37*(1/1.56)

2.37(1/2.23)

2.22 2.69 2.85 3.06 3.24

Margin MD 4.2 22.6 15.3 >9.4 6.1* >9.4 9.0 >3.7 >3.5 14.4 1.23

Sigma 0.32 0.36 0.37 <0.43 0.43* <0.43 0.4 0.48 0.51 0.55 0.58

jLIDT

jcalc

RGRM =1

pa2× R0 ×

0

a

ò0

2p

ò exp-2r2

w 2

é

ëê

ù

ûú ×r ×dr ×dq

Ein = Eout ×(1+ RGRM )

(1- RGRM )

Energy (avg) Inside laser cavity with output coupler reflectivity ROC= RGRM:

But our reflectivity changes with beam size on the GRM, so we have to estimate:

jcalc = Ein ×2

p ×w calc

2

So we can calculate the fluence on each optic:

*worst case:round beam at GRM-end of slab

Page 19: Laser Production for NASA's Global Ecosystem Dynamics ...€¦ · QS = Q-Switch 1/4 WP = 1/4 wave plate GRM = gradient (Gaussian) reflective mirror 1. HR mirror prescription change

GEDI Laser Requirements VerificationID Requirement Values FT CPT Life test Technique Used

1 Laser Wavelength1064.5 nm ± 0.2 nm

in vacuumx O

Pickoff beam. Use built in software to calibrate measurement for vac. Take vacuum and air values

2* Laser Output Energy10 mJ +5% fully

captured beam at the output

x x C

Measuring Total Output Energy using energy meter with 10ms integration time. CPT - energy meter put at the end of the snout to get full output. Used to calibrate pickoff measurement as wellFT/Lifetest - calibrated pickoff

3*Far-Field Divergence of the Central Lobe

0.6 mrad ±0.08mrad1/e2 div. x x C

Spiricon camera (raw beam data) 5-10 capturesComputer Analysis and post processing for side lobes FT-50 cm lensCPT - Rayleigh Range

6Laser Output

Polarization Ratio≥ 200:1 x O

Measure by hand using wave-plate/hi ratio polarizer configuration

9 Pulse Repetition Rate 242 ± 2 Hz x x CConfirm pulse with Tektonix 2024C and use e-drive output reading for continuous measurement

10 Pulse Width

<16ns

ns Full-width and half-

maxx x C

FT- 200 MHz Oscilloscope Average of 16 captures of laser pulsesCPT -2 GHz scope. High speed Oscilloscope compiling 10,000 shots with histogram through computer analysis and post processing. LMB will be measured as well.

12

Laser Pulse Energy Concentration in Far-

Field Outside of Central Lobe

≤ 0.5% of 1/e2 Central Lobe per energy concentration

x OSpiricon camera (raw beam data) 5-10 capturesComputer Analysis and post processing

13*Number of Laser

Shots for Life Testing3.2 billion shots x x C

GSE shot counter will monitor shots for every test. ETU life time shot count will be monitored continuously

24LDA OperatingTemperature

35 +/- 2 °C x C .Internal 10k thermistors read by EGSE

O = Occasional C = Continuous X = One Time Measurement

19

Page 20: Laser Production for NASA's Global Ecosystem Dynamics ...€¦ · QS = Q-Switch 1/4 WP = 1/4 wave plate GRM = gradient (Gaussian) reflective mirror 1. HR mirror prescription change

GEDI Laser Test Matrix GEDI-SYS-PLAN-0019

• Environmental Testing performed on ETU and Flight units

- ETU: Vibration, TVAC, EMC, and life test

- Flight: Vibration, TVAC, EMI/C (at instrument level)

- CPTs before and after each test (or specific cycles)

• Interface testing: BDU, LEU, DOE

20

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Page 21: Laser Production for NASA's Global Ecosystem Dynamics ...€¦ · QS = Q-Switch 1/4 WP = 1/4 wave plate GRM = gradient (Gaussian) reflective mirror 1. HR mirror prescription change

Laser GSE Functional Diagram

Page 22: Laser Production for NASA's Global Ecosystem Dynamics ...€¦ · QS = Q-Switch 1/4 WP = 1/4 wave plate GRM = gradient (Gaussian) reflective mirror 1. HR mirror prescription change

Optical Setup – Laser Lifetest w/BDU

Page 23: Laser Production for NASA's Global Ecosystem Dynamics ...€¦ · QS = Q-Switch 1/4 WP = 1/4 wave plate GRM = gradient (Gaussian) reflective mirror 1. HR mirror prescription change

ETU Laser Development Flow

GSE

Optical Parts

Procurement

Start

Build

Acceptance

Testing

Bonding

Kitting &

Inspection

Preparation 1/16 Sub-Assembly 3/16

Pump

Module

Optical

Bench

Enclosure

Integrate Pump

Module and

Optical Bench

Integrate

Electronics

Test Cavity

Performance

Integrate

Enclosure

CPT

LEGEND

Parts Ordered Parts Delivered

Paperwork Release Complete Task

Complete

Monitor - no tech/cost/schd impact

Monitor - tech/cost/schd impact

On PlanLaser Module

Assembly 4/16

TRR

Vibration/CP

T

Environmental

Testing 5/16

EMC

TVAC/CPT

Start Life

Testing 5/16

Mechanical

Fabrication

Electrical

Harnessing

SLAC

Repair

Interface

Test

Special

Testing*

*Special testing includes pressure and temperature cycling

Pre-Qual 1/16

Q-switch

Spare

Enclosure

Seal Test

Q-switch

Driver

23

Page 24: Laser Production for NASA's Global Ecosystem Dynamics ...€¦ · QS = Q-Switch 1/4 WP = 1/4 wave plate GRM = gradient (Gaussian) reflective mirror 1. HR mirror prescription change

Laser Assembly Flow

Assemble bucket:• Flexures• QSD• Harness

Workmanship Test Seals (Qualify on ETU)

Add Pump Module:• Safe-to-mate GSE• Test Fire Diodes

24

Page 25: Laser Production for NASA's Global Ecosystem Dynamics ...€¦ · QS = Q-Switch 1/4 WP = 1/4 wave plate GRM = gradient (Gaussian) reflective mirror 1. HR mirror prescription change

25

Laser Assembly Flow

Functional Test:LASER-2,3,9,10,11

Comprehensive Performance Test:LASER-1,2,3,4,5,6,7,8,9,10,11,12,15,18,19,20,21Special Test:• Lab Pressure Test• FT min/nom/max pressure

Special Test:• Lab Temp Cycle• FT every 0.5 C

Add Laser Optical Bench & Bench Optics

Seal Enclosure

Special Test:• Lab Temp Cycle• FT every 0.5 C

Environmental& Interface Testing

Page 26: Laser Production for NASA's Global Ecosystem Dynamics ...€¦ · QS = Q-Switch 1/4 WP = 1/4 wave plate GRM = gradient (Gaussian) reflective mirror 1. HR mirror prescription change

Laser ETU Bucket and Driver Assembly

“Bucket” Enclosure

Q-switch Driver

Titanium Flexure

26

Page 27: Laser Production for NASA's Global Ecosystem Dynamics ...€¦ · QS = Q-Switch 1/4 WP = 1/4 wave plate GRM = gradient (Gaussian) reflective mirror 1. HR mirror prescription change

Laser ETU Diode and Bench Assembly

Laser Diodes Laser Optical Bench

27

Page 28: Laser Production for NASA's Global Ecosystem Dynamics ...€¦ · QS = Q-Switch 1/4 WP = 1/4 wave plate GRM = gradient (Gaussian) reflective mirror 1. HR mirror prescription change

28

BDU ETU Assembly Test Configuration

Q-switches

Crystal

Functional Test Platform

TVAC Testing