Issue |
A&A
Volume 686, June 2024
|
|
---|---|---|
Article Number | C5 | |
Number of page(s) | 1 | |
Section | The Sun and the Heliosphere | |
DOI | https://doi.org/10.1051/0004-6361/202450907e | |
Published online | 18 June 2024 |
Study of solar brightness profiles in the 18–26 GHz frequency range with INAF radio telescopes
II. Evidence of coronal emission (Corrigendum)
1
INAF – Cagliari Astronomical Observatory, Via della Scienza 5, 09047 Selargius (CA), Italy
e-mail: marco.marongiu@inaf.it
2
INAF – Institute of Radio Astronomy, Via Gobetti 101, 40129 Bologna, Italy
3
INAF – Astrophysical Observatory of Arcetri, Largo Enrico Fermi 5, 50125 Firenze, Italy
4
University of Florence, Department of Physics and Astronomy, Via Giovanni Sansone 1, 50019 Sesto Fiorentino (FI), Italy
5
ASI – c/o Cagliari Astronomical Observatory, Via della Scienza 5, 09047 Selargius (CA), Italy
6
Los Alamos National Laboratory, Bikini Atoll Rd, Los Alamos, NM 87545, USA
7
INAF – Catania Astrophysical Observatory, Via Santa Sofia 78, 95123 Catania, Italy
8
ASTRON – The Netherlands Institute for Radio Astronomy, Oude Hoogeveensedijk 4, 7991 PD Dwingeloo, The Netherlands
9
INAF – Turin Astrophysical Observatory, Via Osservatorio 20, 10025 Pino Torinese (TO), Italy
10
INAF – Trieste Astronomical Observatory, Via Giambattista Tiepolo 11, 34131 Trieste, Italy
11
Department of Physics, University of Trieste, Via Alfonso Valerio 2, 34127 Trieste, Italy
12
NRAO – Central Development Laboratory, 1180 Boxwood Estate Rd, Charlottesville, VA 22903, USA
13
INAF – Astronomical Observatory of Capodimonte, Salita Moiariello 16, 80131 Napoli, Italy
Key words: methods: data analysis / Sun: atmosphere / Sun: chromosphere / Sun: corona / Sun: photosphere / errata / addenda
An error occurred during the production process. Some units have been mistakenly changed in the text: each “mm” (millimeter) unit should read “Mm” (megameter).
© The Authors 2024
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