The “Orbita” Radio Polygon at an altitude of 2750 meters
conducts solar radio emission observations using
state-of-the-art equipment. This includes instruments for
monitoring solar radio flux at frequencies of 1 GHz and 2.8 GHz,
as well as the Callisto solar radio spectrograph, which is part
of the international e-Callisto network. These tools enable the
detection of solar radio bursts of types II, III, IV, and V, and
provide valuable insights for forecasting the geo-effectiveness
of solar flare activity.
The provided dataset consists of daily tables, where each table
corresponds to a single observation day. The data includes two columns:
- Obs_time: The time of observation at the detector (UTC).
- Flux [SFU]: The solar flux unit measurement, representing the intensity of solar radio emission in SFU (Solar Flux Units).
The data are collected and provided by the Institute of Ionosphere,
(https://ionos.kz/) and are also available through the Kazakhstan
Space Weather Portal (https://ssa.fai.kz/, registration required),
which additionally offers interactive visualizations and graphs.
