reprocessing the complete history of vlbi observations with vievs

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VieVS User Workshop 14 – 21 September, 2011 Vienna Reprocessing the complete history of VLBI observations with VieVS Sigrid Böhm

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Reprocessing the complete history of VLBI observations with VieVS. Sigrid Böhm. Why should one do that?. There are new solution methods/strategies. There is a new software. You would like to create a database with the optimal parameterization for each session. - PowerPoint PPT Presentation

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Page 1: Reprocessing the complete history of VLBI observations with VieVS

VieVS User Workshop

14 – 21 September, 2011

Vienna

Reprocessing the complete history of VLBI observations with VieVS

Sigrid Böhm

Page 2: Reprocessing the complete history of VLBI observations with VieVS

VieVS User Workshop 2011 2

Why should one do that?

There are new solution methods/strategies.

There is a new software.

You would like to create a database with the optimal parameterization for each session.

You are interested in time series of special parameters (such as ERP) covering the longest time span available.

Page 3: Reprocessing the complete history of VLBI observations with VieVS

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TS of special parameters - EOP

Which sessions to choose for processing?

Define exclusion/suitability criteriahttp://vlbi.geod.uni-bonn.de/IVS-AC/data/exclude.txt

No local or regional networks

No sessions with < 3 stations (except for dUT1 determination from Intensives)

No sessions with < 250 observations

Page 4: Reprocessing the complete history of VLBI observations with VieVS

Create a process listBasic list to start: e.g. use mk_list to get a list of intensive

sessions, add this int_list to exclude.txt and then use

mk_list with the option ‘ALL’ except ‘exclude.txt’.

Use preliminary list and process all sessions with a basic

parameterization

Then you can use the data in LEVEL3 to make an

extended exclude list according to the previously defined

criteria and find sessions which are not working properly

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Page 5: Reprocessing the complete history of VLBI observations with VieVS

Interesting parameters for the criteria and for “not working properly“

DATA/LEVEL3/SUBDIR/opt_sessname.mat:opt_.total_obs = number of observations

length(opt_.stat) = number of stations

opt_.mo = error of unit weight a posteriori

opt_.cond = condition number of N-matrix (a bit difficult to judge)

In Matlab: you can use diary(‘thisrun.log’) to store the output from the command window, diary off to stop the function

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Page 6: Reprocessing the complete history of VLBI observations with VieVS

e.g. log-file: search for “RCOND”

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Page 7: Reprocessing the complete history of VLBI observations with VieVS

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check “geometry“Take the information from the files stored in DATA/LEVEL1 and plot the network

Regional network

→ exclude the session

Page 8: Reprocessing the complete history of VLBI observations with VieVS

Other log-file “messages“Problems with tidal ocean loading at station VLBA85 3 Problems with tidal atmosphere loading at station VLBA85 3 Problems with non-tidal atmosphere loading at station VLBA85 3 Problems with thermal correction at station VLBA85 3 Problems with VMF1 at station VLBA85 3

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Page 9: Reprocessing the complete history of VLBI observations with VieVS

For the remaining sessions with high 0

There is no other way than … going through all of them individually

finding clock breaks, bad stations etc.

creating hundreds of OPT files

Most welcome alternative … write a module for the automatic detection of clock breaks and creation of OPT files

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Page 10: Reprocessing the complete history of VLBI observations with VieVS

Update process list

Add all sessions you have sorted out to the „exclude“-file and run mk_list again

Create an outlier file for each session with some simple parameterization

Decide about your final parameterization according to your needs

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Page 11: Reprocessing the complete history of VLBI observations with VieVS

Some rules for EOP estimation

Basic approach for daily resolution:Estimate all five EOP xp,yp,dUT1,dX,dY with 1440 min interval

Estimate station coordinates and apply NNR, NNT conditions

Polar motion with subdaily resolution:Do not estimate but fix nutation!!

Fix station coordinates

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Page 12: Reprocessing the complete history of VLBI observations with VieVS

R1 and R4 networks

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Page 13: Reprocessing the complete history of VLBI observations with VieVS

13VieVS User Workshop 2011

Comment on correlation coefficients

The Matlab function corrcoef works correctly but not for our purpose.

It does not take a covariance matrix as input! (Refer to Matlab Help for further info)

Correlation coefficient:

yyxx

xyxyr

Qxx = inv(atpa_.mat);varii = diag(Qxx);Rxy = Qxx./sqrt(varii*varii');

Page 14: Reprocessing the complete history of VLBI observations with VieVS

5 EOP 24 hours, NNR/NNT

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Page 15: Reprocessing the complete history of VLBI observations with VieVS

3 ERP 1h, nut 24 h, coord fix

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Page 16: Reprocessing the complete history of VLBI observations with VieVS

3 ERP 1h, nut fix, NNR/NNT

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Page 17: Reprocessing the complete history of VLBI observations with VieVS

3 ERP 1h, nut fix, coord fix

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