carrier plus: a sensor payload for living with a star space environment testbed … ·  ·...

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To be presented at SPIE Conf. 5167 “Focal Plane Arrays for Space Telescopes” August 6, 2003 1 Carrier Plus: A Sensor Payload for Living With a Star Space Environment Testbed (LWS/SET) Cheryl Marshall 1 , Steven Moss 2 , Regan Howard 3 , Kenneth LaBel 1 , Tom Grycewicz 4 , Janet Barth 1 , and Dana Brewer 5 NASA Goddard Space Flight Center The Aerospace Corporation Orbital Sciences Corporation Defense Threat Reduction Agency NASA Headquarters SPIE Conf. 5167 “Focal Plane Arrays for Space Telescopes” August 6, 2003

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To be presented at SPIE Conf. 5167 “Focal Plane Arrays forSpace Telescopes” August 6, 2003

1

Carrier Plus: A Sensor Payload for Living With a

Star Space Environment Testbed (LWS/SET)

Cheryl Marshall1, Steven Moss2, Regan Howard3,

Kenneth LaBel1, Tom Grycewicz4, Janet Barth1, and

Dana Brewer5

• NASA Goddard Space Flight Center• The Aerospace Corporation• Orbital Sciences Corporation• Defense Threat Reduction Agency• NASA Headquarters

SPIE Conf. 5167 “Focal Plane Arrays for Space Telescopes” August 6, 2003

To be presented at SPIE Conf. 5167 “Focal Plane Arrays forSpace Telescopes” August 6, 2003

2

Outline

• Living With a Star (LWS) Program

– Space Environment Testbed (SET)

– Natural Space Environment

• Carrier Plus

– Goals and Benefits

• On-Orbit Sensor Measurements

• Carrier Plus Architecture

• Participation in Carrier Plus

To be presented at SPIE Conf. 5167 “Focal Plane Arrays forSpace Telescopes” August 6, 2003

3

Living With a Star (LWS) Program:a pure and applied science program with an

engineering application

• Program Goal – Perform investigations in space tounderstand solar variability & its effects leading to areliable predictive capability of solar variability (i.e.,space weather)

– Continuous program started in FY01

• Science Missions: the what’s and why’s of the solarvariant environment

• Theory and Modeling and Data Analysis: theenvironment models and tools developed fromsolar-variant data

• Space Environment Testbeds (SETs): Improve theengineering approach to accommodate and/ormitigate the effects of solar variability on spacecraftdesign & operations

To be presented at SPIE Conf. 5167 “Focal Plane Arrays forSpace Telescopes” August 6, 2003

4

Trapped ParticlesProtons, Electrons, Heavy Ions

Galactic Cosmic Rays

Solar Protons&

Heavier Ions

The Natural Space Radiation Environment

• Particles trapped in the Van Allen Belts

– Energetic proton, electrons and heavy ions

• Transient radiation

– Galactic cosmic ray particles

– Particles from solar events

• Particles from solar events

can drive the total ionizing

dose, displacement damage

and single event transient

effects of a sensor

To be presented at SPIE Conf. 5167 “Focal Plane Arrays forSpace Telescopes” August 6, 2003

5

SET Technologies

• SET provides opportunities for flightvalidation experiments on technologies– Microelectronics– Photonics– Materials– Sensors

• These investigations focus on– Demonstration of environment

tolerance• Radiation hardening approaches

– Validation of technology ground testmethods and performance predictiontechniques

• Investigations must require exposure tosolar-variant environment

Space Technology ResearchVehicle 1-d

with NASA experiments

To be presented at SPIE Conf. 5167 “Focal Plane Arrays forSpace Telescopes” August 6, 2003

6

SET Services Provided to Experiments

Exp 1

Exp 2

Exp N-1

Exp N

PowerConversion &Distribution

AnalogInterface

RS-422or other

28V

Data

DOSE

TEMP

Command

Power

Host S/C

SETProcessor

SET Payload

Exp = ExperimentCarrier Electronics

Card or Box

(mechanical, thermal,etc. not shown)

CorrelativeEnvironment

Monitor(s)

Data

Commands

To be presented at SPIE Conf. 5167 “Focal Plane Arrays forSpace Telescopes” August 6, 2003

7

Why a Sensor SET Payload?

• UV/Visible focal plane array (FPA) technologies identified as critical to

the NASA mission yet they are inherently sensitive to radiation

– NASA Office of Space Science roadmapping effort

– Charge coupled devices (CCDs) will remain important as well as

newer technologies such as active pixel sensors (APS), p-CCDs, Si

hybrids, etc.

• Science instruments push the state-of-the-art for signal detectibility

and precision even in the absence of radiation!

– Unfortunately, the greater the performance, the greater the

sensitivity to radiation

– CCDs with charge transfer efficiencies (CTEs) in excess of 0.999999

transfer electrons over inches of pristine Si

To be presented at SPIE Conf. 5167 “Focal Plane Arrays forSpace Telescopes” August 6, 2003

8

Benefits of Carrier Plus

• Unlike most microelectronic devices, sensors are highly susceptible

to displacement damage effects

– Protons and secondaries create carrier traps that increase the

dark current, reduce CTE, and produce hot pixels and transients

– Secondaries are produced in the heavy shielding often required

for sensor survivability on-orbit

• Models used to predict displacement damage effects have not been

validated by careful comparison with on-orbit performance

• Hence large radiation design margins (RDM) for a soft technology.

• Carrier Plus is expected to reduce the RDMs thereby allowing sensor

operation in a scientifically more useful orbit or for a longer mission.

To be presented at SPIE Conf. 5167 “Focal Plane Arrays forSpace Telescopes” August 6, 2003

9

Benefits of Carrier Plus, cont.

• Provides heritage for new sensor technologies.

• Validation of ground test based predictions of on-orbit performance.

– On–orbit measurements will correspond with ground testing.

– On-orbit dosimetry is critical for calibration with ground testing.

• Better understanding of space radiation effects can help mission

planning (key observations tend to be degraded first)

– Hubble loses ~10% observing time due to monthly anneals to reduce hot

pixel counts, and CTE loss is a significant problem.

To be presented at SPIE Conf. 5167 “Focal Plane Arrays forSpace Telescopes” August 6, 2003

10

Carrier Plus Measurement Suite

• Sensor dark current

– Both the average and dark current nonuniformity will be characterized

between -20 to +20°C +/- 0.02°C.

– Pixel by pixel dark current histograms acquired

• Temperature dependent CTE measurements.

– Extended edge pixel response (EPER). First pixel response (FPR), cosmic

ray tails, and possibly pinhole centroiding measurements.

– Lower temperatures will permit CTE measurements of damaged FPAs.

– Diagnostic signals can be generated using dark current for biweekly

characterizations

• Proton and heavy ion transient frames captured

• Photometrics may be possible using LED light sources

To be presented at SPIE Conf. 5167 “Focal Plane Arrays forSpace Telescopes” August 6, 2003

11

Focal Plane Array

FPA Support Electronics

ThermalManagement

Unit

To heat sink

ClocksPower

Control

Frame Data

Temperature Control

Frame Data + SensorHousekeeping Telemetry

Command & Telemetry

Heat

Secondary Power

Optical Stimulus Unit

Power & Control

Optical Sensor Head Block Diagram

To be presented at SPIE Conf. 5167 “Focal Plane Arrays forSpace Telescopes” August 6, 2003

12

Optical Sensor Head Block Diagram

CommandDecoder

Bias Supplies

ThermalManagement Unit

Focal Plane Array

Clock Generator

H/K TelemetryGenerator

A/D A/D

~

Selector

DataMux

A/D **

Discrete telemetrypoints

Sensor HeadAnalog Telemetry

PointsFrame

Transfer BusI/F

To frameProcessorOn the SET

LO HI

H/K Telemetry

pixelpixel,col,row,frame

Telemetry

To SET

Commands

From SET

Temperature set points

Bias voltage set points

Clock settings

Frame signal

frame

Dosimeter

Analog TelemetryDirectly to SET

Optical StimulusUnit (OSU)

Pulse width, amplitude and delay

OSU fire command

Heat

Light

OSU fire command

Correlated DoubleSampler

FPA Support Electronics

Passive Trim

Buffer C

ircuits

Circuit

pixel

To be presented at SPIE Conf. 5167 “Focal Plane Arrays forSpace Telescopes” August 6, 2003

13

Carrier Plus Data Processing Flow

SensorHeads

FrameProcessor Storage

HostSpacecraft

SETPayload

OperationsCenter

Experimenters

HostGroundSystem

SETCarrier

Frames &Sensor Head

Telemetry

Reduced

Frame Data

� Compressed subframes� Dark current histograms� Hot pixel lists

CCSDS SFDU

Host Telemetry Format

� Reduced Frame Data� Carrier HousekeepingTelemetry� Host Housekeeping Telemetry� Host Ephemerides

L0: ArchivalL1: Engineering Data Unit Processing

L2: Geometric Reduction

To be presented at SPIE Conf. 5167 “Focal Plane Arrays forSpace Telescopes” August 6, 2003

14

Flight Experiment Selection Process:Two methods

• NRA: a competitive action forinvestigations– Proposal process– Must demonstrate need to

fly in solar-variantenvironment

– Must have collateralground test and/or modeldevelopment program

– No technologydevelopment effortsfunded by this NRA

– Data is non-proprietary(may be ITAR)

– No funds exchanged withinternational entities

• Partnering– Partner may provide

investigation(s) outside ofthe NRA process inexchange for support ofthe LWS SET Program

• Funding• Launch opportunity• Infrastructure, etc…

– Data can be proprietary orsecure

 

To be presented at SPIE Conf. 5167 “Focal Plane Arrays forSpace Telescopes” August 6, 2003

15

Summary of Carrier Plus

• Carrier Plus Goals:– Validate ground test based prediction of on-orbit FPA performance.– Reduce uncertainties in methods used to predict on-orbit sensor

performance.– Provide on-orbit heritage of emerging FPA technologies.– Enhance understanding of various methods now used to assess CTE

behavior in flying instruments.

• Community participation is encouraged through NRAs.– Interest in a variety of FPAs including n-CCDs, p-CCDs, APS, Si hybrids, …

– Experimenters are responsible for ground test program.

– NASA may supply FPA support electronics board.

– For more information see http://lws-set.gsfc.nasa.gov and http://lws-set.gsfc.nasa.gov

• DTRA is our sensor partner and will identify half of the sensors flown

– For information see Tom Grycewicz at [email protected].