Station GUR.AL has maintained continuous aurora frequency monitoring since commissioning in 1974. All observations are cataloged according to the Nordic Geomagnetic Index Protocol (NGIP-7) and cross-referenced with solar wind data from the Tromsø Geophysical Observatory.
Current detection array operates across 50 frequency bands in the visible spectrum, with primary sensitivity calibrated to oxygen emission lines at 557.7nm and 630.0nm.
Observation window: continuous, 24-hour cycle. Peak activity recorded during magnetic midnight ±3 hours.