New processing examples - Bernese GNSS Software

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Example for a BPE_CLN–script R. Dach et al.: Bernese GNSS Software: Processing Examples in Version 5.2 Document compiled: Bern, July 2, 2013 # Get variables # ------------- my ($yyssssm30, $ssssm30, $taskId, $dirBpePrt, $dirBpeLog, $extBpePrt, $extBpeLog) = $bpe->getKeys( ’$YSS-(30)’, ’$S-(30)’, ’TASKID’, ’DIR_BPEPRT’, ’DIR_BPELOG’, ’EXT_BPEPRT’, ’EXT_BPELOG’); # Delete PRT/LOG and BPE files # ---------------------------- my @delLst = ("${dirBpePrt}${taskId}${yyssssm30}__.${extBpePrt}", "${dirBpeLog}${taskId}${yyssssm30}__.${extBpeLog}", "${dirBpePrt}${ssssm30}.BPE"); map { unlink(glob($_)) } @delLst; Slide 23 of 86 Astronomical Institute, University of Bern AIUB Closing Remarks on the Scripts to Realize the Dataflow • To modify the list of result files or their target directory needs adaptions in the XXX_SAV–script. R. Dach et al.: Bernese GNSS Software: Processing Examples in Version 5.2 Document compiled: Bern, July 2, 2013 • If you have another structure in your datapool you need to revise the source directories in the XXX_COP–script. • The scripts shall be as generic as possible, it means in particular use variables where all variables are used in the BPE processing. • The deletion scripts are very important and must be kept consistent with the processing part. No left–overs from the processing are allowed for a permanently running process! • To finish a BPE with a DUMMY script at PID 999 is beneficial to check whether the processing has successfully finished. Slide 24 of 86 Astronomical Institute, University of Bern AIUB
Consequences from the Example Dataflow The full intended dataflow is now realized in the processing examples of Version 5.2. R. Dach et al.: Bernese GNSS Software: Processing Examples in Version 5.2 Document compiled: Bern, July 2, 2013 The consequence is that a few additional tools need to be installed before the processing examples can be started: • extracting UNIX-compressed files • RINEX Hatanaka compression tools Potential sources are listed at http://www.bernese.unibe.ch/download/#TLS. Our assumption is that these (or at least equivalent) tools are needed anyhow if you want to process GNSS data. This means that this does not imply any additional work load to the users. Slide 25 of 86 Astronomical Institute, University of Bern AIUB The Processing Examples in Version 5.2 R. Dach et al.: Bernese GNSS Software: Processing Examples in Version 5.2 Document compiled: Bern, July 2, 2013 The Processing Examples in Version 5.2 The Examples BPEs Characteristics of the Examples BPEs Slide 26 of 86 Astronomical Institute, University of Bern AIUB
Page 1 and 2: Bernese GNSS Software: Processing E
Page 3 and 4: Directory Structure Main Directorie
Page 5 and 6: Populating the DATAPOOL area Let us
Page 7 and 8: Populating the DATAPOOL area Let us
Page 9 and 10: Realization of the Example Dataflow
Page 11: Example for a XXX_SAV-script: R2S_S
Page 15 and 16: What Applications Shall be Covered
Page 17 and 18: Processing Example: CLKDET.PCF R. D
Page 19 and 20: Example Dataset R. Dach et al.: Ber
Page 21 and 22: Standard-Variables for the Dataflow
Page 23 and 24: Defining Standard Processing Files
Page 25 and 26: Defining the Reference Frame BPE-va
Page 27 and 28: Selecting Orbit/Clock Products R. D
Page 29 and 30: Example BPE: Specific Aspects R. Da
Page 31 and 32: BPE-specific Variables (PPP) R. Dac
Page 33 and 34: BPE-specific Variables (RNX2SNX) R.
Page 35 and 36: BASTST-Example PCFile name: ${U}/PC
Page 37 and 38: BPE-specific Variables (CLKDET) Int
Page 39 and 40: Preparing the Campaign You have to
Page 41 and 42: Filling the DATAPOOL Put the needed
Page 43: Generate Project Related Files A se

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