"Exploring Coronal Holes Through K-Band Radio Observations (18-26 GHz ) with INAF Radio Telescopes" (Marongiu et al., Solar Physics, 301, 117, 2026)
"Correlation between active regions’ spectra at high radio frequencies and solar flare occurrences" (Mulas et al., Scientific Reports, 2026)
"Study of solar brightness profiles in the 18-26 GHz frequency range with INAF radio telescopes. II. Evidence of coronal emission" (Marongiu et al., A&A, 2024, 684-A123)
"Study of solar brightness profiles in the 18-26 GHz frequency range with INAF radio telescopes. I. Solar radius" (Marongiu et al., A&A,, 2024, 684-A122)
"A new method for accurate calibration of solar disk emission in the radio band" (Mulas et al., ASI Technical Report, RS-UCS-2022-007, 2022)
"Solar observations with single-dish INAF radio telescopes: continuum imaging in the 18 – 26 GHz range" (Pellizzoni et al., Solar Physics, 297, 86, 2022)
"A dedicated pipeline to analyse solar data with INAF radio telescopes: SUNPIT (SUNdish PIpeline Tool)" (Marongiu et al., INAF Technical Reports, 137, 2022)
"A Python approach for solar data analysis: SUNDARA (SUNDish Active Region Analyser), preliminary development" (Marongiu et al., INAF Technical Reports, 81, 2021)
"Imaging of the solar atmosphere in the centimetre-millimetre band through single-dish observations" (Pellizzoni et al., NCimC, 42, 9P, 2019)
"Current state and perspective of Space Weather science in Italy" (Plainaki et al., J. Space Weather Space Clim., 10, 6 2020)
"High-Resolution Imaging of the Solar Chromosphere in the Centimetre-Millimetre Band through Single-Dish Observations" (Pellizzoni et al., 2nd URSI AT-RASC, Gran Canaria, 28 May – 1 June 2018 ).
"Testing technological and astronomical SDSA/SRT capabilities for solar and near-Sun observations" (Iacolina et al., IAC 2019, Washington, 21-25 October 2019)