Solar Radio Emission Observations at “Orbita” Radio Polygon
Short Name:
solar_flux data
Date:
12 Dec 2024 19:58:36
Publisher:
Fesenkov Astrophysical Institute
Description:
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:
- **timestamp**: The time of observation at the detector.
- **SFU**: The solar flux unit measurement, representing the intensity of solar radio emission in SFU (Solar Flux Units).
The data is collected and provided by the Institute of Ionosphere (https://ionos.kz/).
