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PSR Section 7

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Validation of Wedged Filter Approach for Spacecraft Instrumentation ... Difficult to differentiate High Albedo from Specular Reflection ... – PowerPoint PPT presentation

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Title: PSR Section 7


1
Section 7 Atmospheric Corrector
. . . Dennis Reuter EO-1 LEISA Atmospheric
Corrector
2
LEISA Atmospheric Corrector (LAC) Contribution to
EO-1
  • Validation of Wedged Filter Approach for
    Spacecraft Instrumentation
  • Atmospheric correction for ALI Multispectral
    images
  • Atmospheric correction for Landsat-7 images
    (Formation Flying)
  • Direct study of Spatial Resolution Degradation
    (cross-comparison with Hyperion)
  • Retrieved atmospheric parameters
  • Cross-comparison with MODIS

3
LAC BLOCK DIAGRAM
28 V
Lenses
power
Power Conversion
digital
RS 422
Digital Buffers and
Formatting
SPACECRAFT
bias
1773
1773 Interface, Array
Control and TEC Control
clock
TEC
ELECTRONICS
l
MODULE
3 Wedged Filter/ Array Assemblies
OPTICS MODULE
4
LAC Characteristics
  • High Spectral - Moderate Spatial Resolution
    Hyperspectral Imager using Wedged Filter
    Technology (LVE).
  • Spectral Coverage 0.9 - 1.6 mm 256 Bands
    Selected for optimal correction of High Spatial
    Resolution Images.
  • Spectral Resolution 35 cm-1 (Dl 3 nm _at_ 0.9 mm,
    9 nm _at_ 1.6 mm)
  • Swath Width 185 km Matches Landsat.
  • Spatial Resolution (pixel) 356 mradian (250
    meter _at_ 705 Km).
  • Three 256 x 256 Element InGaAs Arrays TEC
    Stabilized (lt285 K).
  • Three 15 Degree FOV 3 Element Lenses.
  • Two Modules Bolt-onOptics Module and
    Electronics Module.
  • Mass 10.5 kg (EM, 4.4 kg OM 3.9 kg Cable 2.2
    kg).
  • Power 48 W (Peak) lt15 W (Orbital Average).

5
Performance Testing
  • Box Level
  • Cards Simulated on an Individual Basis
  • TECs Tested with Engineering Backplane (Focal
    Plane)
  • Focal Plane Timing Tested with Multiplexers
  • Subsystem Level
  • OM Limited Set of Images Obtained with EM
    Simulator
  • Engineering Model Vibration Tested
  • EM Operation Tested by Interface to OM Simulator
  • Instrument Level
  • Vibration and Thermal-Vacuum
  • Radiometric, Spectral Calibration and Alignment
  • EMI/EMC

6
LAC Test Descriptions
  • Vibration
  • Individual modules tested to proto-flight level
    (1.25 x expected maximum flight loads)
  • Instrument mounted on Spacecraft and tested to
    flight level
  • Thermal Vacuum (Pre-Spacecraft Integration)
  • Four cycles to survival levels (-10C to 50C
    Range expected on orbit 20C? 10C)
  • Operation from 0C to 30C (Orbital Predict
    20C, 30C worst case)
  • Images Obtained Using LAC GSE
  • Thermal Vacuum (Integrated with Spacecraft)
  • Four Cycles
  • Operation from 0 C to 30 C (No Operation at 40
    C)
  • Images Using Spacecraft System (WARP, XBPAA,
    etc.)

7
LAC Test Descriptions
  • EMI/EMC
  • Instrument Level Tests Conducted and Radiated
    Emissions, and Radiated Susceptibility
  • Alignment
  • Orientation of Arrays with respect to Alignment
    Cube using Theodolites
  • LAC Alignment to ALI on Spacecraft Using
    Theodolites
  • Optical Calibration
  • Wavelength and Instrumental Shape Grating
    Monochrometer 1 to 100 nm Steps
  • Radiometric Calibrated Black-body (all 4 TEC
    Settings)
  • Flat Field Diffuse Source Illuminating Lenses
    and Solar Calibrators

8
LAC Test Results / Actions
  • Vibration (Proto-flight, Module Level)
  • OM Arrays contacted by LVE some damage to
    arrays and LVEs wire bonds broken on one array
  • Incorrect assembly of LVE mount
  • Wire bonds repaired on array
  • One LVE replaced with flight spare
  • LVE mount re-assembled correctly
  • Module re-vibrated with no damage
  • EM 1773 Fiber Alignment Cylinder Cracked
  • Failure mode observed in other 1773 interface
    applications
  • Cylinder replaced
  • Module re-tested with no damage
  • Vibration (Satellite, Instrument Level) No
    damage

9
LAC Test Results /Actions
  • EMI/EMC
  • Excessive radiated / conducted Emissions (20 - 30
    dB in some places)
  • Interpoint Power Supply filtering
  • Additional Filter Assembly mounted on EM
  • Filter reduces excess emissions to at most 5 dB -
    waiver granted
  • Components destroyed during conducted
    Susceptibility Test
  • Incorrect test conditions
  • Components replaced
  • Test was not repeated - waiver granted

10
LAC Test Results /Actions
  • Thermal Vacuum (before Spacecraft integration)
  • Instrument operated for approximately 10 hours
  • Mount temperatures lt 25 C, continuous operation
    for 1 hour
  • Mount temperature 30 C, Digital Board overheated
    in 40 minutes
  • No modification Maximum operating time in-flight
    20 minutes
  • Thermal Vacuum (Spacecraft)
  • Instrument operated for approximately 20 hours
  • Dark current consistent with previous results
  • Mount 40 C Power Board reached Red-Limit temp
    in lt 5 minutes
  • Power board Red-Limit set for mount temperature
    at lt 30 C Models indicate Red-Limit can be
    increased 20 C
  • Excellent TEC control

11
LAC Test Results /Actions
  • Optical Calibration
  • Radiometric
  • Initial results consistent with models
  • Offset error limits dynamic range to 11 bits.
    Difficult to differentiate High Albedo from
    Specular Reflection
  • Unexpected temperature dependence of Quantum
    Efficiency
  • Spectral
  • Filters have excellent spectral characteristics
  • Alignment Within 2 arc-min of ALI Track --
    achieved 1
  • Flat Field Solar Calibrators consistent with
    Diffuse Illumination

12
Modifications
  • Software
  • Red-Limits on currents eliminated
  • TEC set-points lowered to reflect improved
    thermal results on Spacecraft
  • Hardware
  • No additional hardware modifications required
  • NO SIGNIFICANT OPEN ISSUES INSTRUMENT HAS RUN
    SEVERAL HUNDRED HOURS 50 TROUBLE-FREE
  • REQUIRED ORBITAL OPERATION 50 HOURS

13
Waivers and NCRs
  • 5 waivers
  • 3 EMI / EMC
  • Parts tracability
  • Degraded performance of TEC 3 during instrument
    T/V
  • Not apparent in Spacecraft T/V tests
  • 9 NCRs
  • Waivers and NCRs available in GSFC system
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