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. Pellizzoni; S. Righini; S. Mulas; R. Nesti; A. Burtovoi; M. Romoli; G. Serra; G. Valente; E. Egron; G. Murtas; M. N. Iacolina; A. Melis; S. L. Guglielmino; S. Loru; P. Zucca; A. Zanichelli; M. Bachetti; A. Bemporad; F. Buffa; R. Concu; G. L. Deiana; C. Karakotia; A. Ladu; A. Maccaferri; P. Marongiu; M. Messerotti; A. Navarrini; A. Orfei; P. Ortu; M. Pili; T. Pisanu; G. Pupillo; P. Romano; A. Saba; L. Schirru; C. Tiburzi; L. Abbo; F. Frassati; M. Giarrusso; G. Jerse; F. Landini; M. Pancrazzi; G. Russano; C. Sasso and R. Susino;
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)
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Italy
- University of Florence Italy
- Los Alamos National Laboratory United States
- University of Trieste Italy
- National Institute for Astrophysics Italy
- Osservatorio Astrofisico di Catania Italy
methods: data analysis; Sun: atmosphere; Sun: chromosphere; Sun: corona; Sun: photosphere; errata; addenda
methods: data analysis; Sun: atmosphere; Sun: chromosphere; Sun: corona; Sun: photosphere; errata; addenda
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This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
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This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
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