new and future models

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3/6/09 New and Future Models Matt King, Newcastle University, UK

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New and Future Models. Matt King, Newcastle University, UK. New: Effects of New Models on Tropo Estimates. Several consistent global reprocessing solutions (1995-2007) ‏ In turn, examine effect of Abs Phase Centres VMF1 Improved Hydrostatic Zenith Delay Thomas et al (in prep) ‏. - PowerPoint PPT Presentation

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Page 1: New and Future Models

3/6/09

New and Future Models

Matt King, Newcastle University, UK

Page 2: New and Future Models

3/6/09

New: Effects of New Models on Tropo Estimates

• Several consistent global reprocessing solutions (1995-2007)

• In turn, examine effect of

– Abs Phase Centres

– VMF1

– Improved Hydrostatic Zenith Delay

• Thomas et al (in prep)

Page 3: New and Future Models

3/6/09

Tropo Estimates

• Respective models influence is location dependant)

Page 4: New and Future Models

3/6/09

Near future: Higher order ionospheric effects

• Examine effect of 2nd+3rd order ionosphere on consistent reprocessing (1995-2007, every 2nd day)

• Also effect of geomagnetic model (simple dipole vs International Geomagnetic Reference Field)

• Petrie et al (in prep), and invited talk at EGU

Page 5: New and Future Models

3/6/09

2nd and 3rd order iono

Transformation to ITRF2005

Effect of modelling terms

Difference between dipole and IGRF modelPeriodogram for dTZ

Page 6: New and Future Models

3/6/09

2nd and 3rd order

1996-2000

2001-2005

1996-2005

Page 7: New and Future Models

3/6/09

Needed: Improved MP model

• Simulation MP model of Elosegui et al (1995) on long time series

– Static MP field is sampled by time-variable satellite constellation

– Time-variable propagation effect?

Page 8: New and Future Models

3/6/09

Possible MP effect

Presuming clear horizon

Page 9: New and Future Models

3/6/09

Possible MP effect

Page 10: New and Future Models

3/6/09

Conclusions

• Recent models improve GPS TZD estimates dramatically

• Higher Order iono important for global reference frame

• MP simulations

– Gives feel for likely MP effect at each site

– Model too simplistic – e.g., no azimuthal variation, technically only applies in far field

– Need advances here to model and mitigate the effect