spectral imaging of the coronal environment (spice)

22
Spectral Imaging of the Coronal Environment (SPICE) Caitlyn Quinn Summer 2010 Gregory Woytko, 547

Upload: oki

Post on 02-Feb-2016

26 views

Category:

Documents


0 download

DESCRIPTION

Spectral Imaging of the Coronal Environment (SPICE). Caitlyn Quinn Summer 2010 Gregory Woytko, 547. What is SPICE?. Imaging coronal spectrograph One of ten instruments to fly on the ESA/NASA Solar Orbiter mission in 2017 Will orbit the sun at closest distances ever attempted, around 1/4 AU - PowerPoint PPT Presentation

TRANSCRIPT

Page 1: Spectral Imaging of the Coronal Environment (SPICE)

Spectral Imaging of the Coronal Environment

(SPICE)

Spectral Imaging of the Coronal Environment

(SPICE)

Caitlyn QuinnSummer 2010

Gregory Woytko, 547

Caitlyn QuinnSummer 2010

Gregory Woytko, 547

Page 2: Spectral Imaging of the Coronal Environment (SPICE)

What is SPICE?What is SPICE?

Imaging coronal spectrograph

One of ten instruments to fly on the ESA/NASA Solar Orbiter mission in 2017

Will orbit the sun at closest distances ever attempted, around 1/4 AU

SPICE instrument currently in Phase A

Imaging coronal spectrograph

One of ten instruments to fly on the ESA/NASA Solar Orbiter mission in 2017

Will orbit the sun at closest distances ever attempted, around 1/4 AU

SPICE instrument currently in Phase A

Page 3: Spectral Imaging of the Coronal Environment (SPICE)

Solar Orbiter Mission GoalsSolar Orbiter Mission Goals

Evaluate plasma properties and composition of the sun with unprecedented spatial and spectral resolution

Improve our understanding of the Sun’s effects on Earth and the solar system

Better understand CME and space weather

Evaluate plasma properties and composition of the sun with unprecedented spatial and spectral resolution

Improve our understanding of the Sun’s effects on Earth and the solar system

Better understand CME and space weather

Page 4: Spectral Imaging of the Coronal Environment (SPICE)

OrbitOrbit

.23 AU

Page 5: Spectral Imaging of the Coronal Environment (SPICE)

The InstrumentThe Instrument

Sun’s light comes in through entrance aperture

Ray hits primary mirror and series of optics

Pre-slit deflects excess radiation

Ray passes through slit mechanism; four slits of varying width

Detectors interpret incoming EUV light

Sun’s light comes in through entrance aperture

Ray hits primary mirror and series of optics

Pre-slit deflects excess radiation

Ray passes through slit mechanism; four slits of varying width

Detectors interpret incoming EUV light

Page 6: Spectral Imaging of the Coronal Environment (SPICE)

The Detector (Housing and Door)The Detector (Housing and Door)

Page 7: Spectral Imaging of the Coronal Environment (SPICE)

The DetectorThe Detector

Spring-loaded door2 detector stacks

Spring-loaded door2 detector stacks

MCP

HAS FOC

Page 8: Spectral Imaging of the Coronal Environment (SPICE)

Detector StacksDetector Stacks Micro Channel Plates

(MCP) High voltage

Fiber Optic Coupler (FOC) Transmits/focuses image

HAS chip Intensified active pixel

sensors Off-centered active area

Components in stack connected by epoxy bond lines

Micro Channel Plates (MCP) High voltage

Fiber Optic Coupler (FOC) Transmits/focuses image

HAS chip Intensified active pixel

sensors Off-centered active area

Components in stack connected by epoxy bond lines FOCHAS

MCP

Page 9: Spectral Imaging of the Coronal Environment (SPICE)

The DetectorThe Detector

Door opens, EUV radiation hits MCPs

MCPs are supplied a high voltage, detect and amplify incoming radiation

Radiation and voltage transmit through FOC to HAS chip

High voltage activates HAS pixels, which record incoming signal

Door opens, EUV radiation hits MCPs

MCPs are supplied a high voltage, detect and amplify incoming radiation

Radiation and voltage transmit through FOC to HAS chip

High voltage activates HAS pixels, which record incoming signal

Page 10: Spectral Imaging of the Coronal Environment (SPICE)

HAS: Off-Centered Active AreaHAS: Off-Centered Active Area

Page 11: Spectral Imaging of the Coronal Environment (SPICE)

Bonding the Detector TogetherBonding the Detector Together

Epotek 310M Epoxy Plastic adhesive Transparent, maintains

maximum strength down to 10-12 m

Connection between HAS and fiber optic coupler is CRITICAL Determines resolution of

images captured

Epotek 310M Epoxy Plastic adhesive Transparent, maintains

maximum strength down to 10-12 m

Connection between HAS and fiber optic coupler is CRITICAL Determines resolution of

images capturedCRITICAL bond line

Page 12: Spectral Imaging of the Coronal Environment (SPICE)

Critical Bond: FOC to HASCritical Bond: FOC to HAS

FOC focus: 4 m HAS pixels: 18 m Light refracts 30° on

either side of ray from the FOC to epoxy

Distance between FOC and HAS (i.e. bond thickness) determines spread Smaller spread, better

resolution

FOC focus: 4 m HAS pixels: 18 m Light refracts 30° on

either side of ray from the FOC to epoxy

Distance between FOC and HAS (i.e. bond thickness) determines spread Smaller spread, better

resolution

Page 13: Spectral Imaging of the Coronal Environment (SPICE)

Critical Bond: FOC to HASCritical Bond: FOC to HAS

Worst case scenario: bond line 12 m, single focused ray spreads over multiple HAS pixels

Page 14: Spectral Imaging of the Coronal Environment (SPICE)

Issues With BondingIssues With Bonding

ESD sensitivity of HAS Accuracy, precision

How to ensure precise placement of FOC in active area despite slight variations in HAS chips?

2 bonds on one FOC Expense of HAS

Only get “one shot” to do it right during actual fabrication

Solution??

ESD sensitivity of HAS Accuracy, precision

How to ensure precise placement of FOC in active area despite slight variations in HAS chips?

2 bonds on one FOC Expense of HAS

Only get “one shot” to do it right during actual fabrication

Solution??

Page 15: Spectral Imaging of the Coronal Environment (SPICE)

Bonding FixtureBonding Fixture Grounded metal plate with

HAS-shaped pocket Outer holes to secure

fixture and ground plate Holes around pocket for

T-shaped alignment bars (adjustable)

HAS is removable after bonding is achieved

Drawings approved, quote received, solid models in the making!

Grounded metal plate with HAS-shaped pocket

Outer holes to secure fixture and ground plate

Holes around pocket for T-shaped alignment bars (adjustable)

HAS is removable after bonding is achieved

Drawings approved, quote received, solid models in the making!

Page 16: Spectral Imaging of the Coronal Environment (SPICE)

SPICE: General IssuesSPICE: General Issues

Ability of instrument to withstand wide range of temperatures

Will the detector and bonds withstand testing: vibration, thermal, acoustic, etc?

Passing upcoming CDRDelayed execution of instrument (>3 yrs)

Ability of instrument to withstand wide range of temperatures

Will the detector and bonds withstand testing: vibration, thermal, acoustic, etc?

Passing upcoming CDRDelayed execution of instrument (>3 yrs)

Page 17: Spectral Imaging of the Coronal Environment (SPICE)

Other Experiences at NASAOther Experiences at NASA

Working alongside engineers, scientists, machinists

Clean room training

Disassembling hardware

Machine Shop ESDM 5-axis milling Metrology, FARO arms Rapid prototyping: SLA

Working alongside engineers, scientists, machinists

Clean room training

Disassembling hardware

Machine Shop ESDM 5-axis milling Metrology, FARO arms Rapid prototyping: SLA

Page 18: Spectral Imaging of the Coronal Environment (SPICE)

2 in.

Page 19: Spectral Imaging of the Coronal Environment (SPICE)
Page 20: Spectral Imaging of the Coronal Environment (SPICE)
Page 21: Spectral Imaging of the Coronal Environment (SPICE)
Page 22: Spectral Imaging of the Coronal Environment (SPICE)

Questions?Questions?