GNSS Replication Data for: \"On the production of ionospheric irregularities via Kelvin-Helmholtz instability associated with cusp flow channels\"

The files contain data recorded on 30.11.2014 by four NovAtel GPStation-6 GNSS Ionospheric Scintillation and TEC Monitors located in Svalbard, and used in the publication Spicher et al. (2020). Each receiver operates more or less continuously and outputs both 60 second reduced data (Total Electron Content and scintillation indices), 1 second Total Electron Content data, and 50 Hz raw data (power and phase). The data processing is described in the following scientific publications: Oksavik, K., C. van der Meeren, D. A. Lorentzen, L. J. Baddeley, and J. Moen (2015), Scintillation and loss of signal lock from poleward moving auroral forms in the cusp ionosphere, J. Geophys. Res. Space Physics, 120, 9161–9175, doi:10.1002/2015JA021528. [Available at https://agupubs.onlinelibrary.wiley.com/doi/full/10.1002/2015JA021528] van der Meeren, C., K. Oksavik, D. A. Lorentzen, M. T. Rietveld, and L. B. N. Clausen (2015), Severe and localized GNSS scintillation at the poleward edge of the nightside auroral oval during intense substorm aurora, J. Geophys. Res. Space Physics, 120, 10,607–10,621, doi:10.1002/2015JA021819. [Available at https://agupubs.onlinelibrary.wiley.com/doi/full/10.1002/2015JA021819] Uploaded by A.S. Notice: This dataset has been superseded by the content of the newer UiB GNSS data collection, which users can access here: K. Oksavik (2020), The University of Bergen Global Navigation Satellite System Data Collection, DataverseNO, https://doi.org/10.18710/AJ4S-X394.