Correlation between active regions’ spectra at high radio frequencies and solar flare occurrences

Abstract High radio frequencies observations with the Italian network of large single-dish radio telescopes resulted in $$\sim$$ 450 solar images between 2018 and 2023 in K-band frequency range (18–26 GHz). Solar radio mapping at these frequencies allows the probing of the Active Regions (ARs) chrom...

Celý popis

Podrobná bibliografie

Hlavní autoři:	Sara Mulas, Alberto Pellizzoni, Marco Marongiu, Adriana Marcucci, Simona Righini, Maria Noemi Iacolina, Elise Egron, Giulia Murtas, Matteo Bachetti, Francesco Berrilli, Alessandro Cabras, Roberto Caocci, Gian Luigi Deiana, Salvatore Luigi Guglielmino, Colby Haggerty, Adelaide Ladu, Sara Loru, Andrea Maccaferri, Pasqualino Marongiu, Andrea Melis, Alessandro Navarrini, Alessandro Orfei, Pierluigi Ortu, Mauro Pili, Tonino Pisanu, Giuseppe Pupillo, Andrea Saba, Luca Schirru, Giampaolo Serra, Caterina Tiburzi, Giuseppe Valente, Alessandra Zanichelli, Pietro Zucca, Mauro Messerotti
Médium:	Artigo
Jazyk:	Inglês
Vydáno:	Nature Portfolio 2026-01-01
Edice:	Scientific Reports
Témata:	Chromosphere Flares Magnetic Fields Radio Emission Sun
On-line přístup:	https://doi.org/10.1038/s41598-025-27776-2
Tagy:	Přidat tag Žádné tagy, Buďte první, kdo vytvoří štítek k tomuto záznamu!