Institute of Radio Astronomy (IRA)
Author in the following contributions
- Probing the physical parameters of the solar chromosphere and the corona through radio observations in the 18-26 GHz frequency range
- Exploring the variable spectra and magnetic fields of the Active Regions in the chromosphere through high-frequency radio imaging: gyro-resonance emission and flare forecasting
- Monitoring of the solar atmosphere through radio imaging in the 18-100 GHz band: recent results and future challenges
