Laser Rangefinder Update 9/5/03 Experiment - PowerPoint PPT Presentation

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Laser Rangefinder Update 9/5/03 Experiment

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December 3-4, Green Bank. GBT PTCS In Progress Review. Laser Rangefinder ... focus at source near NCP 'Track' at 360 ... parts nearing obsolesence (IRIG, ... – PowerPoint PPT presentation

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Title: Laser Rangefinder Update 9/5/03 Experiment


1
Laser Rangefinder Update9/5/03 Experiment
  • K. Constantikes

2
Experiment
  • Designed to correlate thermal, astrometric data
    with LRF data
  • 24 hours of
  • Point/focus at source near NCP
  • Track at 360, 38 for 2 minutes
  • LRFs running continously, 15 sec sample interval
  • 11 targets, some with 4 rangefinders designated
    (FA tip, el bearing)
  • Zero points for each instrument
  • Leakages for each instrument
  • Weather data , 10 sec sample interval
  • LRFs had pointing optimized for all target at
    this GBT pose

3
Range data processing
  • Zero points and leakages smoothed 75 sec median
  • Group refractive index smoothed 120 sec median
  • LRF integration time 1 sec
  • SNR gt 10 Phase estimate noise lt200 ?m
  • Selected low SNR to get more range data
  • RMS range residual in trilateration will ID noisy
    range data
  • 97F Fem model used for range prediction and
    resolving range uncertainty
  • Ranges corrected for glass offset, GRI, monument
    and rangefinder geometry
  • For 4 el bearing targets (2 each side) and 2 FA
    tip targets
  • Select last 60 secs of data (up to 4 ranges, 4
    rangefinders), GBT at 360, 38 ?1
  • lt 650 ?m FA y, lt 250 ?m FA x,z
  • lt 125 ?m el bearing x,y

4
EMS Flowgraph
5
Bounding actual FA position errors
2.4 0.8mm at FA tip
6
Bounding actual el bearing position errors
3 at el bearing 0.4mm
7
ZAG736D The best
  • 1900 outage due to SW failure
  • Some trend visible in X
  • No data after 2130
  • LRF pointing
  • Dew, fog
  • Expectation of 1s range error 40mm
  • 3 rangefinders
  • Consistent PTCS/PN/8

8
ZAG736D The best
25 minutes
  • - Dispersion of range error broader due to low
    SNR threshold.
  • 40mm PDOP 300mm total position error SHORT
    TERM (60 secs) ?
  • Actual 1s total position error 2mm, 1s y error
    0.7mm, or 6 azimuth pointing error equiv.

9
ZEG41040L Monument errors
  • No data after 2100
  • Position jumps due to redundant ranging (4 LRFs)
    and monument posn errors
  • Consistent with 1 mm monument posn error.

X (mm)
Number of LRFS
10
ZY107 Erratic pointing
  • Very high SNR occasionally, but long outages

11
ZY102 Low laser power?
  • Consistent SNR
  • Degrade after sundown-
  • Dew?
  • Thermal pointing shift?
  • SNR would be still be adequate _at_ 0.1sec
    integration
  • 1900 outage was software

12
ZY103 Inadequate laser power, poor pointing
  • Laser power too low for 0.1 sec integration time
  • Pointing erratic too

13
Data quality statistics
  • 6 Targets, 20 hours, 4 ranges per minute
  • 2 retros per el bearing, 2 FA tip retros
  • Possible 20x60x4 4800 trilaterations
  • About half lost due to fog, dew
  • Others lost to pointing/SNR issues (even though
    SNR10 threshold used)
  • Total good trilaterations, percent excluding
    fog/dew
  • ZAG731D .210 or 10 ZAG731P .142 or
    5 ZAG736D .611 or 25 ZAG736P .44
    or 0 ZEG41040L .241 or 10 ZEG41040R
    337 or 15

14
Reliability
  • Out of six experiments, not one case where all 12
    ground LRFs were operational
  • one week preparation time each case.
  • Pointing problems most common, but also
  • Oscillator failures
  • Servo failures
  • Computer (ZY and ZIY) failures

15
Fixes
  • LRF outgoing and incoming beams need to be
    broadened, pointing errors identified
  • Some laser diodes replaced (obsolete, will
    require mechanical retrofits
  • Other parts nearing obsolesence (IRIG,
    Oscillators)
  • 360 Degree retros to improve ground geometry
  • Beam split and track to ameliorate detector group
    delay issues (centriod and carrier density)?
  • How to ameliorate dew problem?
  • More lab characterization to ensure were ready
  • Major, time consuming, expensive undertaking

16
Summary
  • Not only are there fundamental issues-
  • Geometry and group refractive index
  • And major system design issues-
  • E.g., LRFs on feed arm
  • But also suitability, usability, cost, and
    schedule issues.
  • And we know how to fix them
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