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Hyperspectral Imager Program Development Allan Hollinger Manager, Sensors

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Manager, Sensors & Signal Processing. Spacecraft Payloads ... External Baffles. Mechanisms. Telescope. Attitude Orbit Control System. Spectrometers VISNIR SWIR ... – PowerPoint PPT presentation

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Title: Hyperspectral Imager Program Development Allan Hollinger Manager, Sensors


1
Hyperspectral ImagerProgram DevelopmentAllan
HollingerManager, Sensors Signal
ProcessingSpacecraft Payloads
2
Why Hyperspectral Remote Sensing? Canadian
National Working Groups Recommendations
  • Geoscience Working Group
  • Develop a spectral library representative of
    materials in the Canadian tundra
  • Software and algorithm development to help
    industry to use hyperspectral data
  • Agriculture Working Group
  • Identify the potential of hyperspectral data for
    precision farming
  • Environment Working Group
  • Applications for the identification of
    bio-indicators and indexes
  • Emphasis should be placed upon the simpler cases
    of data representation, data integration
    (especially the merging of fine resolution data
    with RADARSAT data), information extraction and
    product delivery

3
Overview of Canadian Capabilities in
Hyperspectral Remote Sensing Program Objectives
  • To develop advanced hyperspectral technologies as
    partner in foreign missions
  • To satisfy Canadian needs for high quality
    hyperspectral data products, and to provide
    better access to data for Canadian users
  • To provide advanced hyperspectral information
    products for
  • exploration geology and prospecting
  • management of mine wastes
  • assessment of environmental stress in ecosystems
    and coastal zones
  • monitoring of water resources and aquaculture
  • management of forests and agriculture

4
Canadian Investment in Hyperspectral activities
5
Canadian Expert Support Laboratory for MERIS
  • MERIS is a 15 band imager (designed as a
    visible imaging spectrometer) primarily for
    ocean/water monitoring ? 300 m footprint) and
    3 day revisit cycle
  • Simulate and evaluate MERIS data in diverse
    Canadian landscape and seasons
  • Develop and test product generation algorithms
    for MERIS
  • Evaluate benefits of information products and
    initiate a science framework for Canada
  • Canadians have responded to the MERIS AO
    successfully

6
Canadian Expert Support Laboratory for MERIS
  • 2 Land Projects
  • L1 (ISTS) -forest change
  • L2 (U.Sherbrooke) -atmosphere correction (Land)
  • 6 Water Projects
  • W1 (Borstad) -FLH algorithm develop
  • W2 (Borstad) -FLH algorithm test
  • W3 (NWRI) -lake water optical parameters
  • W4 (Borstad-BIO) -primary productivity
  • W5 (Satlantic) -coastal water variability
  • W6 (MDA) -sensitivity of atmospheric effects over
    water
  • 4 Infrastructure Projects
  • I1 (MDA) -project communications atm. corr.
    (water)
  • I2 (ISTS) -intra project instrument calibration
  • I3 (MDA) -management
  • I4 (MDA) -MERIS ground station study

7
Overview of Canadian Capabilities in
Hyperspectral Remote Sensing
  • Hyperspectral Mission
  • CSA and CCRS are providing a coordinated approach
    to facilitate access to hyperspectral missions
    and related opportunities
  • Current activities
  • Prepare options for Canadian participation in a
    hyperspectral mission
  • Data and instrument simulation to ensure that
    mission meets Canadian users needs and to
    influence payload design
  • Demonstration of applications to ensure that
    Canadian users can take full advantage of the
    data when a satellite is operational

8
Hyperspectral Imager Technology Assessment
Objectives
  • Examine Canadian participation in all aspects of
    satellite based program and provide critical
    assessment of
  • Technical constraints
  • Schedule
  • Budget
  • Leading to
  • detailed design and fabrication
  • user application studies and user development

9
Hyperspectral SensorFunctional Block Diagram
Control Flight Computers
Command Telemetry
Instrument Control Electronics
Scene
Attitude Orbit Control System
Optical Calibration Subsystem
Fore-Optics
Telescope
Mechanisms
External Baffles
Timing Synchronisation
Data Handling Electronics
Sensor Subsystems
Raw Data Buffer
FPAs Pan Imager VISNIR SWIR
Signal Conditioning Analog to Digital Converter
Spectrometers VISNIR SWIR
On-board Calibration Processor (Radiometric
Correction)
Lossless Compression
Housekeeping Headers
Instrument Control Status
EDAC Downlink Electronics
Data Recorder incl. EDAC
Data Formatting Electronics
10
Hyperspectral Imager Technology Assessment
11
Hyperspectral Imager Technology Assessment
12
Software Tools for Hyperspectral Imagers
  • Goals
  • 1. Datacube management
  • 2. Spectral interpretation (match to known or
    identify unknown)
  • 3. Combining spectral-spatial algorithms
  • 4. Visualization tools
  • 5. Browse, archive, retrieval and dissemination
  • Some Developers (algorithms, proprietary and COTS
    tools)
  • - CCRS (ISDAS)
  • - CSA (SIDMF)
  • - MDA (Geobox, Hawkeye, MIMCOM, etc.)
  • - Borstad
  • - Itres
  • - Universities

13
Hyperspectral Imager Technology Assessment
14
1 Optical Technology Advancement
  • Demonstrate fabrication capabilities for a
    three-mirror anastigmatic (TMA) fore-optics and
    on-board calibration subsystem optical elements
  • Build and test breadboard optical components
  • Perform fabrication and materials trade-offs
  • Advance TMA and calibration-subsystem optical
    designs, considering e.g. straylight, scatter,
    opto-mechanical methods

15
2 System Studies for a Hyperspectral Imager
  • Establish system-level and instrument-level
    requirements, based on applications needs
  • Develop system modeling tools, including
    applications algorithms, lumped-parameter models
    (LPMs) and data-flow models (DFMs)
  • Perform systems analysis using LPMs and DFMs
  • Models and analyses to include Cal/val
    requirements and functional performance
  • Application algorithms should be well
    benchmarked including ground truth to
    distinguish instrument error from algorithm error

16
3 Predictors for Lossless Compression of
Hyperspectral Data
  • Investigate and Select optimum predictor for a
    satellite HSI program, considering performance
    and ease of hardware implementation
  • Assess predictors performance, using
    Hyperspectral datasets from a variety of
    available scenes and sensors
  • Examine benefits of on-board calibration to
    compression
  • Consokidate buffering and compreesion electronics
    design identify critical components and
    implementation issues

17
ESA Explorer Core MissionLand Surface Processes
and Interaction Mission
  • Designed to meet research goals
  • Relies on intensive study of partiular sites
  • Examines BRDF algorithms and Remote Sensing
    Science
  • Phase A study benefits from ESA Payload
    technology studies (HRIS and pre-phase A on
    PRISM)
  • Alcatel/Aerospatiale won the competitive contract
  • Completion expected June 1999

18
Partnership Options
  • Ongoing discussions with
  • Australia - ARIES
  • European options
  • ESA Earth Explorer
  • Land Surface Processes and Interaction Mission
    (Core Mission)
  • SIMSA (German led Opportunity Mission)
  • Smart Spectral (Dornier led commercial mission)

19
Earth Explorer Opportunity Mission Issues and
Process at ESA
  • Stage 1 Submission of Preliminary SIMSA
    proposal?
  • Stage 2 Submission of Full Proposal Dec 1/98 ?
  • Scientific Proposal
  • Technical Proposal
  • Feasible cost and schedule
  • Technical maturity and understanding of key
    technologies requiring customization or
    development
  • Programmatic benefits and alignment of SIMSA
    and LSPIM
  • Selection of Proposals for Phase A/B - June 1999
    est
  • Stage 3 ESA ITT to Industry
  • Current Meeting provides an opportunity for
    forming a preliminary industrial team

20
SIMSA Conclusions Nov 16-17/98
  • Initiatives for EEOM Phase A/B or bilateral
    hyperspectral programmes
  • Science programme description and definition
  • Harmonisation of science programme for selected
    applications
  • Baseline mission, satellite and instrument
    definition

21
Status of ARIES
  • ARIES Phase A and pre-Phase B completed by
    current partners
  • Australian Tax Office ruling critical to ARIES
    funding
  • Written ruling expected shortly Phase B set to
    start June 1999
  • Preliminary discussions between Canada and ARIES
    in March and December 1997
  • Major joint workshop held in June 1998
  • Work package alternatives discussed
  • Data rights discusses
  • Meeting with ARIES held Jan/99
  • Follow up meetings planned for spring 1999

22
ARIES Consortium
  • Currently there are three partners
  • Auspace (a wholly owned subsidiary of MMS-UK)
  • CSIRO (DEM)
  • ACRES
  • ARIES Operating Company (to be created)
  • Finances operations through data sales
  • Investors TBD
  • Responsibility
  • Space Segment Prime
  • Applications Prime
  • Ground Segment Prime
  • Owns Satelliteand Data
  • Contracts with AUSPACE, CSIRO and ACRES for
    satellite development and operation

23
Australian Resource Information and
Environmental Satellite
  • Goal to develop and operate a commercially
    sustainable resource information satellite using
    the latest hyperspectral sensing technology
  • Outcome of 20 years of collaborative RD between
    Australias leading research agency (CSIRO) and
    the mining industry
  • ARIES-1 Project Office created in October 1995
  • ARIES-1 feasibility study completed in March 1997
  • ARIES-1 launch in 2002 with operation starting in
    2003
  • Australian consortium CSIRO, ACRES, Auspace Ltd.
  • Other partners
  • International groups of mining and exploration
    companies
  • Australian and European Geological Surveys
    consortia
  • UK Natural Environment Research Council
  • Canada Centre for Remote Sensing (with the
    participation of CSA)

24
Australian Resource Information and
Environmental Satellite
  • Satellite
  • Australian design and weight less than 500 kg
  • Polar, sun synchronous 500 km above the Earth's
    surface
  • Design life 5 years
  • Sensor
  • 32 contiguous bands in the VNIR (400 to 1100nm)
  • 32 contiguous bands in the SWIR (2000-2500nm)
  • Optional coverage of 1000-2000nm range with
    emphasis on atmospheric correction and
    calibration
  • Spatial resolution Spectrometer - 30 metres at
    nadir Panchromatic - 10 metres at nadir
  • Ground swath 15 km at nadir
  • Off-track pointing to 30 degrees off vertical
  • Revisit time 7 days at 30 degrees look angle
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