gnssanalysis

The package encompasses various GNSS-related functionality such as efficient reading and writing GNSS files (e.g. SINEX, SP3, CLK, IONEX and many others), advanced analysis and comparison, various coordinate transformations including geodetic frame rotations, predictions and combinations. Package Solver.

Install

bash pip install gnssanalysis

File formats supported

• BLQ
• BSX/BIA
• CLK
• ERP
• IONEX
• NANU
• RINEX
• SINEX (including discontinuity, post-seismic file formats)
• SP3
• TROP
• GINAN proprietary formats: PEA partials, POD output, STEC and TRACE

Standalone utilities

There is a set of standalone utilities installed together with the module module which are build on top of gnssanalysis.

diffutil

A utility originally created for automated testing of the computed GNSS files relative to the known good solution files. The simplest use case for the diffutil is to call it with two GNSS files specified after -i: bash diffutil -i file1 file2 diffutil parses files' extensions and automatically calls a command needed, e.g. sp3 for file.sp3. It is also possible to specify the command manually in case file extensions are non-standard or missing.

bash diffutil -i file1 file2 sp3 # sp3 is a command inside diffutil

snxmap

Reads any number of sinex files given, specifically the SITE/ID block and creates an interactive html map with all the stations plotted. Every file will get a unique color marker, with decreasing size for each additional marker, constructing "lollipops" at common stations. This allows seeing intersections of stations within files to be easily seen. The sinex files may also be compressed (either .Z or .gz)

How to use: bash snxmap snxfile1 snxfile2.Z snxfile3.gz -o path_to_output

sp3merge

Merges any number of sp3 files together creating sp3 file of any length. Could also accept clk files to populate merged sp3 with clock offset values.

How to use: bash sp3merge -s file1.sp3 file2.sp3.Z file3.sp3.gz -c file1.clk file2.clk.Z file3.clk.gz

log2snx

A utility to parse collection of igs-format station files and create a sinex file with required station information - location, station hardware etc.

How to use: bash log2snx -l "~/logfiles/*/*log"

trace2mongo (needs update)

Converts tracefile to the mongo database that is compatible with Ginan's mongo output for EDA

gnss-filename

Determines appropriate filename for GNSS based on the content

orbq

Compares two sp3 files and outputs statistics to the terminal window.

How to use: bash orbq -i IGS2R03FIN_20191990000_01D_05M_ORB.SP3 TUG0R03FIN_20191990000_01D_05M_ORB.SP3 Result: ``` PRN RRMS ARMS CRMS dXRMS dYRMS dZRMS 1DMEAN 3DRMS E01 0.01429 0.00629 0.0077 0.01116 0.00894 0.00993 0.01001 0.01741 E02 0.01931 0.01063 0.01009 0.01564 0.01332 0.01288 0.01395 0.02424 E03 0.0207 0.01334 0.00935 0.0139 0.01909 0.01168 0.01489 0.02634

...

    R_RMS   A_RMS   C_RMS   dX_RMS  dY_RMS  dZ_RMS  1D_MEAN 3D_RMS

AVG 0.01155 0.01536 0.01346 0.01504 0.01443 0.01277 0.01408 0.02485 STD 0.01045 0.02978 0.01767 0.02065 0.02253 0.01809 0.02017 0.03522 RMS 0.01553 0.03334 0.02212 0.02543 0.02663 0.02205 0.02449 0.04292

```

clkq

Compares two clk files and outputs statistics to the terminal window. How to use: bash clkq -i IGS2R03FIN_20191990000_01D_30S_CLK.CLK COD0R03FIN_20191990000_01D_30S_CLK.CLK Result: ``` INFO:root:filtering using 10.00 hard cutoff on the detrended data. [99.99% data left] INFO:root:filtering using 3.00*sigma cut on the detrended data. [99.99% data left] INFO:root:clkq CODE AVG STD RMS E01 3.6127 0.0469 3.613 E02 3.5929 0.0469 3.5932 E03 3.6221 0.042 3.6224

...

GNSS AVG STD RMS E 3.6075 0.0595 3.608 G -0.0621 0.0663 0.0909 R 6.1658 0.3282 6.1746 ```

Reject satellites

You are able to provide a regex to reject satellites, e.g.: bash clkq -i IGS2R03FIN_20191990000_01D_30S_CLK.CLK COD0R03FIN_20191990000_01D_30S_CLK.CLK --reject "G18" Result: NFO:root:Excluding satellites based on regex expression: 'G18' INFO:root:Removed the following satellites from first file: '['G18']' INFO:root:Removed the following satellites from second file: '['G18']' INFO:root:filtering using 10.00 hard cutoff on the detrended data. [100.00% data left] INFO:root:filtering using 3.00*sigma cut on the detrended data. [100.00% data left] INFO:root:clkq CODE AVG STD RMS E01 3.6127 0.0469 3.613 E02 3.5929 0.0469 3.5932 ...

Normalisation Procedure

And you are also able to provide a normalisation parameter to choose how the data is normalised (daily, epoch), e.g.: bash clkq -i IGS2R03FIN_20191990000_01D_30S_CLK.CLK COD0R03FIN_20191990000_01D_30S_CLK.CLK --norm "daily" Result: INFO:root::_clk_compare:using ['daily'] clk normalization INFO:root:---removing common mode from clk 1--- INFO:root:Using daily offsets for common mode removal INFO:root:---removing common mode from clk 2--- INFO:root:Using daily offsets for common mode removal INFO:root:filtering using 10.00 hard cutoff on the detrended data. [99.99% data left] INFO:root:filtering using 3.00*sigma cut on the detrended data. [99.99% data left] INFO:root:clkq CODE AVG STD RMS E01 -0.1216 0.0469 0.1303 E02 -0.1214 0.0469 0.1302 E03 -0.1216 0.042 0.1286 ... These can also be stacked: bash clkq -i IGS2R03FIN_20191990000_01D_30S_CLK.CLK COD0R03FIN_20191990000_01D_30S_CLK.CLK --norm "daily" --norm "epoch" Result: INFO:root::_clk_compare:using ['daily', 'epoch'] clk normalization INFO:root:---removing common mode from clk 1--- INFO:root:Using daily offsets for common mode removal INFO:root:Using epoch normalization (mean gnss) offsets for common mode removal INFO:root:---removing common mode from clk 2--- INFO:root:Using daily offsets for common mode removal INFO:root:Using epoch normalization (mean gnss) offsets for common mode removal INFO:root:filtering using 10.00 hard cutoff on the detrended data. [99.99% data left] INFO:root:filtering using 3.00*sigma cut on the detrended data. [99.99% data left] INFO:root:clkq CODE AVG STD RMS E01 -0.0 0.0149 0.0149 E02 -0.0 0.0191 0.0191 E03 -0.0 0.0076 0.0076 ...

Some usage examples

Combination of sinex solutions files

Combination of with a frame file projected to a midday of a date of interest Usage examples:

• Daily comnination with frameofday centered at midday python from gnssanalysis import gn_combi daily_comb_neq = gn_combi.addneq(snx_filelist=_glob.glob('/data/cddis/2160/[!sio][!mig]*0.snx.Z'),frame_of_day=frame_of_day)

• Weekly combination with frameofday centered at week's center: python weekly_comb_neq = gn_combi.addneq(snx_filelist=_glob.glob('/data/cddis/2160/[!sio][!mig]*.snx.Z'),frame_of_day=frame_of_day)

The frame of day could be generated using a respective function from gn_frame module: ```python from gnssanalysis import gnframe, gndatetime

framedatetime = gndatetime.gpsweeksec2datetime(2160,43200)

frameofday = gnframe.getframeofday(dateorj2000=framedatetime, itrfpathordf = '/data/cddis/itrf2014/ITRF2014-IGS-TRF.SNX.gz',disconpathordf='/data/cddis/itrf2014/ITRF2014-soln-gnss.snx',psdpathordf='/data/cddis/itrf2014/ITRF2014-psd-gnss.snx') ```