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Ramesh GOVIND and John DAWSON

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use of the IERS2000 diurnal and semi-diurnal Earth Orientation model; ... Microcosm. Cneq/Solve. Slv2snx. Normal Point Data. NEQ combination. Format Translation ... – PowerPoint PPT presentation

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Title: Ramesh GOVIND and John DAWSON


1
ILRS AWG Pilot Project POSEOP
  • Ramesh GOVIND and John DAWSON

01/0000
2
ILRS AWG Pilot Project POSEOP
  • Analysis for
  • Lageos1, Lageos2,
  • Etalon1, Etalon2
  • ILRS AWG options A, B1 and B2

3
Changes Implemented
  • use of the IERS2000 diurnal and semi-diurnal
    Earth Orientation model
  • a revised time and range bias estimation scheme
  • use of the Mendes FCUL mapping function for
    atmospheric refraction

4
Data Set
  • Only stations that observed 30 or more
    observations during each 28 day solution were
    included in the analysis.

5
Series A Global SLR data.
6
Series B Global SLR data.
7
Analysis Procedure
8
Multi-Arc NEQ Combination
9
Computation Procedure
  • Data Weighting
  • 1.0 CM GOOD STATIONS,
  • 5.0 CM POOR STATIONS
  • Centre of Mass
  • L1 AND L2 0.251
  • E1 AND E2 0.558 FOR ALL STATIONS

10
Estimated Parameters
  • STATION COORDINATES
  • DAILY X, Y AND TAI-UT1 RATES
  • LAGEOS 1 AND 2
  • SATELLITE ELEMENTS PER 28 DAY ARC
  • SOLAR RADIATION PRESSURE SCALE (once per arc)
  • ALONG TRACK ACCELERATION CONSTANT AND
    ONCE-PER-REVOLUTION SINE/COSINE EVERY 7 DAYS
  • CROSS TRACK ONCE-PER-REVOLUTION SINE/COSINE
    EVERY 7 DAYS RANGE
    BIAS PER STATION EVERY 7 DAYS

11
Estimated Parameters
  • ETALON 1 AND 2
  • SATELLITE ELEMENTS PER 28 DAY ARC
  • SOLAR RADIATION PRESSURE SCALE FACTOR EVERY
    28 DAYS
  • ALONG TRACK ACCELERATION CONSTANT AND
    ONCE-PER-REVOLUTION SINE/COSINE EVERY 28 DAYS
  • CROSS TRACK ONCE-PER-REVOLUTION SINE/COSINE
    EVERY 28 DAYS

12
CONSTRAINTS
  • ORBIT UNCONSTRAINED
  • RANGE BIAS 1 M
  • X/Y POLE 20 MAS, UT 2 MS
  • X/Y POLE RATE 10 MAS/DAY, LOD 0.2 MS
  • STATION COORDINATES 1 M OR 10 M

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20
Work in progress
  • upgrade of our computation, combination and SINEX
    output software to include the ability to
    estimate and output EOP rates, i.e. xpole/ypole
    rate and Length of Day (LOD)

21
CONCLUSIONS
  • No significant improvement in station coordinate
    solution with the inclusion of sparse/limited
    Etalon data. Lageos dominate the solution.
  • Marginal improvement in the EOP solution with the
    inclusion of the Etalon data -- more stations /
    more data still required to see any impact.
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