gpstec

Calibrated GPS total electron content (TEC) from NovAtel GPStation-6 and other dual-frequency receivers.

Website: https://dipanjanbanerjee.github.io/gpstec/

gpstec turns a raw GPStation-6 .GPS file (or any RINEX 2/3 observation file) into calibrated slant and vertical TEC, with a user-chosen elevation cut-off. It writes daily data files and publication-quality figures in one command:

gpstec run -c station.toml -o results  2242_0_00_skbu.GPS

Why

Many GPStation-6 users go through the chain .GPS → RTKLIB → RINEX → a closed calibration program → .Cmn files. That chain has three problems:

• Wrong station position. RTKCONV 2.4.2 writes latitude, longitude and height into the APPROX POSITION XYZ header field, which expects Earth-centred coordinates. A program that trusts the header then places the station near the centre of the Earth, so every elevation, pierce point and VTEC is wrong. gpstec always takes the position from your configuration file.
• No elevation cut-off. Low-elevation rays need a mapping function that fails near the equatorial anomaly. gpstec lets you choose the cut-off (50° by default) and keeps all lower data out of the products.
• No way to check the calibration. gpstec reports independent checks for every day: the CODE global ionosphere map, a midnight continuity test, and a calibration uncertainty band.

Install

Python 3.9 or newer:

pip install gpstec
gpstec install-convbin        # only needed for .GPS input: builds RTKLIB convbin (needs git, gcc, make)
gpstec init                   # writes station.toml: put your antenna position in it

On Ubuntu/Debian, sudo apt install git build-essential provides the build tools for install-convbin. On Windows, use the convbin.exe that comes with RTKLIB and set its path in station.toml.

Use

gpstec run -c station.toml -o results  /data/2242_*.GPS        # a week of receiver files
gpstec run -c station.toml -o results  skbu3590.22o            # RINEX (.22n next to it)
gpstec run -c station.toml -o results  skbu3590.22o --elev 40  # another elevation cut-off
gpstec --version

Satellite bias files (CODE .DCB) and global ionosphere maps (CODE IONEX) are downloaded automatically into dcb/ and gim/. If your network blocks the download, put the files there yourself. gpstec picks them up by date and prints the exact file names it needs.

Method

1. .GPS → RINEX with RTKLIB convbin -r nov. The correct station position is written into the header.
2. Geometry. Satellite positions come from the broadcast ephemeris (or SP3 precise orbits with --sp3). Azimuth, elevation and pierce points are computed on a thin shell at 350 km.
3. Slant TEC.
   • Code: P4 = P2 − C1.
   • Carrier phase: L4 = L1·λ1 − L2·λ2.
   • Each continuous satellite pass is levelled to the code with an elevation-weighted mean above 20° (Ciraolo et al., 2007).
   • Passes that continue across midnight are levelled as one pass.
4. Biases: STEC = STEC_measured + B_sat + B_rx.
   • B_sat comes from CODE monthly DCBs (P1−P2, plus P1−C1 for C1 receivers) or from Bias-SINEX files.
   • B_rx is estimated for each day from that day's night-time data alone. It is a least-squares fit of STEC = VTEC(t, pierce point)/M(el) − B_rx, in which VTEC may vary north–south and east–west. That matters near the anomaly crest, where minimum-scatter methods drift.
   • The receiver bias is never allowed to make VTEC negative.
5. VTEC. VTEC = STEC · √(1 − (Re·cos E / (Re + h))²), using only satellites above the elevation cut-off.
6. Station VTEC curve. All satellites above the cut-off are fitted together as V0(t) + Gn(t)·Δlat + Ge(t)·Δlon with smooth splines. The curve therefore does not jump when a satellite rises or sets, and the horizontal gradients are saved as well.

Checks you get for every day

• CODE global ionosphere map at the station, drawn on the plot. Its night-time difference from the station is saved, typically within 2–3 TECU.
• Calibration uncertainty band: the spread of independent receiver-bias estimates.
• Midnight continuity. Day X's file ends at 00:00:00 and the next file starts at 00:00:01, so the same satellites are seen at the same moment. gpstec compares them and splits any jump into the part caused by the receiver-bias change and the part left over from processing.

Outputs

Per day, in results/YYYY-MM-DD/:

For multi-day runs, results/ also gets:

• all days in one CSV;
• an overlay figure, a day × UT map and the midnight continuity figure;
• calibration_summary.csv and midnight_continuity.csv.

Figures

The figures are made for papers:

• vector PDF with embedded, editable fonts, plus 300 dpi PNG;
• legends outside the data area;
• a colour-blind-safe palette.

The test suite checks automatically that no two pieces of text touch. In station.toml you can change:

• the formats (png, pdf, svg, eps, tiff);
• the width (figure_width_in = 3.5 for one journal column);
• whether titles are drawn (figure_titles = false when the caption goes in the paper).

Citing

If you use gpstec in published work, please cite it (see CITATION.cff; GitHub shows a "Cite this repository" button):

Banerjee, D. (2026). gpstec: calibrated GPS total electron content from GPStation-6 receivers (version 1.0.0). https://github.com/dipanjanbanerjee/gpstec

References

• Ciraolo, L., Azpilicueta, F., Brunini, C., Meza, A., & Radicella, S. M. (2007). Calibration errors on experimental slant total electron content (TEC) determined with GPS. Journal of Geodesy, 81, 111–120.
• Ma, G., & Maruyama, T. (2003). Derivation of TEC and estimation of instrumental biases from GEONET in Japan. Annales Geophysicae, 21, 2083–2093.
• Schaer, S. (1999). Mapping and predicting the Earth's ionosphere using the Global Positioning System. PhD thesis, University of Bern.
• Seemala, G. K., & Valladares, C. E. (2011). Statistics of total electron content depletions observed over the South American continent for the year 2008. Radio Science, 46, RS5019.

Author and license

Copyright © 2026 Dipanjan Banerjee. Released under the license in LICENSE.

Bug reports and questions: GitHub issues.