Solar Radio Emission Observations at “Orbita” Radio Polygon

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, (ionos.kz/) and are also available through the Kazakhstan Space Weather Portal (ssa.fai.kz/, registration required), which additionally offers interactive visualizations and graphs.