New processing examples - Bernese GNSS Software

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BPE–specific Variables (CLKDET) R. Dach et al.: Bernese GNSS Software: Processing Examples in Version 5.2 Document compiled: Bern, July 2, 2013 BPE–variables for clustering of parallel BPE jobs: (CLKDET.PCF) • V_CLU (default: depends on your computer system) Specifies how many files (stations/baselines) are processed together in one of the parallel running BPE jobs. • V_CLUCOD (default: depends on your computer system) Number of clusters for pre-processing the code measurements in regional clusters for residual screening. • V_CLUPRP (default: depends on your computer system) The number of clusters for steps (MKCLUSAP/TIMEST P with options CLK ED0 and CLK EDT). Slide 71 of 86 Astronomical Institute, University of Bern AIUB BPE–specific Variables (CLKDET) R. Dach et al.: Bernese GNSS Software: Processing Examples in Version 5.2 Document compiled: Bern, July 2, 2013 BPE–variables for clustering of parallel BPE jobs: (CLKDET.PCF) • V_CLUSOL (default: “1”) The final solution (MKCLUSAP/TIMEST P with options CLK RES) may also be computed in clusters if many stations are included. • V_MAXSOL (default: depends on your application) For the final solution a maximum number of stations per cluster may be specified. This option limits the number of stations in the final solution in conjunction with the number of clusters. Slide 72 of 86 Astronomical Institute, University of Bern AIUB
BPE–specific Variables (CLKDET) Introduce a CRD/TRP solution: (CLKDET.PCF) It is possible that the results from an external solution may be introduced to compute a clock solution consistent to those results: R. Dach et al.: Bernese GNSS Software: Processing Examples in Version 5.2 Document compiled: Bern, July 2, 2013 • V_FIXPTH (default: “${S}/RNX2SNX/$Y+0”) Path from where the external coordinate/troposphere solution files are copied. • V_FIXCRD (default: “F1_$YSS+0”) Name of the coordinate solution file to be introduced: {V_FIXPTH}/STA/{V_FIXCRD}.CRD • V_FIXTRP (default: “F1_$YSS+0”) Name of the troposphere solution file to be introduced: {V_FIXPTH}/ATM/{V_FIXTRP}.TRP Slide 73 of 86 Astronomical Institute, University of Bern AIUB LEOPOD–Example PCFile name: ${U}/PCF/LEOPOD.PCF Description: ${U}/PCF/LEOPOD.README R. Dach et al.: Bernese GNSS Software: Processing Examples in Version 5.2 Document compiled: Bern, July 2, 2013 PRECISE ORBIT DETERMINATION FOR LOW EARTH ORBITER Purpose: This BPE performs reduced-dynamic and kinematic orbit determinations for one LEO. The following results are obtained: • screened carrier phase observation files • reduced-dynamic orbit solution with piece-wise constant accelerations as empirical parameters • kinematic orbit solution • orbit comparison between both orbit solutions Slide 74 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 and 12: Example for a XXX_SAV-script: R2S_S
Page 13 and 14: Consequences from the Example Dataf
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: BASTST-Example PCFile name: ${U}/PC
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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