Introduction

20
VieVS User Workshop 7 – 9 September, 2010 Vienna Introduction Johannes Böhm

description

Introduction. Johannes Böhm. Occam. Occam 6.1 LSM had some weaknesses equinox-based transformation between TRS and CRS only piecewise linear rates starting with the first observation old Fortran with COMMON blocks. Occam. Occam 6.1 LSM had some weaknesses no graphical interface - PowerPoint PPT Presentation

Transcript of Introduction

Page 1: Introduction

VieVS User Workshop7 – 9 September, 2010

Vienna

IntroductionJohannes Böhm

Page 2: Introduction

VieVS User Workshop 2010 2

OccamOccam 6.1 LSM had some weaknesses

equinox-based transformation between TRS and CRS onlypiecewise linear rates starting with the first observationold Fortran with COMMON blocks

Page 3: Introduction

VieVS User Workshop 2010 3

OccamOccam 6.1 LSM had some weaknesses

no graphical interface no handbookdevelopers separated by 10.000 km / 12 h...

Page 4: Introduction

VieVS User Workshop 2010 4

First idea to use Matlab ..goes back to Thomas Hobiger in 2005

Page 5: Introduction

VieVS User Workshop 2010 5

Why Matlab?our students are experts in Matlab, but not in Fortran or C++nor are weIt is expensive, but there are non-commercial alternatives or we can provide executables

Page 6: Introduction

VieVS User Workshop 2010 6

Why did we develop VieVS?to have VLBI software for students

to get them involved with bachelor, diploma and ph.d. thesesthey can add their own tools

to have a clear structurenew modules can be added rather easily

Page 7: Introduction

VieVS User Workshop 2010 7

Why did we develop VieVS?easy functional model with piecewise linear offsets at integer hours in the sense of GGOSnon-rotating origin right from the beginning (no equinox-based transformation)

Page 8: Introduction

VieVS User Workshop 2010 8

Why did we develop VieVS?

Page 9: Introduction

VieVS User Workshop 2010 9

PolicyAvailable for registered users

easier to get feedbackto be able to report bugs to the users

We are open for co-operationnew modules developed at other institutes(e.g. co-authorship in VieVS handbook)

Page 10: Introduction

VieVS User Workshop 2010 10

PolicyOPT and outlier files will not be generally made available

these make the solutions different

Page 11: Introduction

VieVS User Workshop 2010 11

Outlook

Page 12: Introduction

VieVS User Workshop 2010 12

Data formatNew IVS WG4 data format to be implemented (netcdf)

Page 13: Introduction

VieVS User Workshop 2010 13

Troposphere delaysfrom external files

ray-traced delays, VMF1, site pressure, NWM pressure, ...

only GMF/GPT internally

Page 14: Introduction

VieVS User Workshop 2010 14

VieVS Face-liftingone interface

Page 15: Introduction

VieVS User Workshop 2010 15

SINEXResults in SINEX formatgetting operational in Vienna

Page 16: Introduction

VieVS User Workshop 2010 16

Close gap with raw observationsdetermination of ambiguities(delay-rate) solutionphase solution for VLBI2010?software correlator for short sessions???

Page 17: Introduction

VieVS User Workshop 2010 17

Kalman Filterand equivalent classical least-squares adjustment

Page 18: Introduction

VieVS User Workshop 2010 18

SystemTest Octave and executables

Page 19: Introduction

VieVS User Workshop 2010 19

Source structureVolunteers?

Page 20: Introduction

VieVS User Workshop 2010 20

Documentation!!