Erratum: Study of solar brightness profiles in the 18-26 GHz frequency range with INAF radio telescopes: II. Evidence of coronal emission (Astronomy and Astrophysics (2024) 684 (A123) DOI: 10.1051/0004-6361/202348770)

Marongiu, M.; Pellizzoni, A.; Righini, S.; Mulas, S.; Nesti, R.; Burtovoi, A.; Romoli, M.; Serra, G.; Valente, G.; Egron, E.; Murtas, G.; Iacolina, M. N.; Melis, A.; Guglielmino, S. L.; Loru, S.; Zucca, P.; Zanichelli, A.; Bachetti, M.; Bemporad, A.; Buffa, F.; Concu, R.; Deiana, G. L.; Karakotia, C.; Ladu, A.; Maccaferri, A.; Marongiu, P.; Messerotti, M.; Navarrini, A.; Orfei, A.; Ortu, P.; Pili, M.; Pisanu, T.; Pupillo, G.; Romano, P.; Saba, A.; Schirru, L.; Tiburzi, C.; Abbo, L.; Frassati, F.; Giarrusso, M.; Jerse, G.; Landini, F.; Pancrazzi, M.; Russano, G.; Susino, C. Sasso And R.

doi:10.1051/0004-6361/202450907e

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Erratum: Study of solar brightness profiles in the 18-26 GHz frequency range with INAF radio telescopes: II. Evidence of coronal emission (Astronomy and Astrophysics (2024) 684 (A123) DOI: 10.1051/0004-6361/202348770) / M. Marongiu, A.P.. - In: ASTRONOMY & ASTROPHYSICS. - ISSN 1432-0746. - ELETTRONICO. - 686:(2024), pp. C5.0-C5.0. [10.1051/0004-6361/202450907e]