First-authored, refereed papers of Valentina Penza

A list of first-authored, refereed publications of Valentina Penza, derived from the SAO/NASA Astrophysics Data System (ADS). The number in brackets after each title indicates the number of citations that the paper has received.

Orcid ID: 0000-0002-3948-2268

List of publications ordered by citations
Number of papers: 10
No. of citations: 113

2025

1. Investigating the Temperature Sensitivity of UV Line Ratios in the 280 nm Region of Solar-like Stars [0]
   Penza, Valentina, Criscuoli, Serena, Reda, Raffaele, Bertello, Luca, Bono, Giuseppe, Del Moro, Dario, D'Orazi, Valentina, Giovannelli, Luca, Nigro, Giuseppina & Berrilli, Francesco, ApJ, 982, 198

2024

1. Reconstruction of the Total Solar Irradiance During the Last Millennium [5]
   Penza, Valentina, Bertello, Luca, Cantoresi, Matteo, Criscuoli, Serena, Lucaferri, Lorenza, Reda, Raffaele, Ulzega, Simone & Berrilli, Francesco, ApJ, 976, 11

2023

1. Prediction of solar cycle 25: applications and comparison [8]
   Penza, Valentina, Bertello, Luca, Cantoresi, Matteo, Criscuoli, Serena & Berrilli, Francesco, Rendiconti Lincei. Scienze Fisiche e Naturali, 34, 663

2022

1. Total Solar Irradiance during the Last Five Centuries [23]
   Penza, Valentina, Berrilli, Francesco, Bertello, Luca, Cantoresi, Matteo, Criscuoli, Serena & Giobbi, Piermarco, ApJ, 937, 84

2021

1. Prediction of Sunspot and Plage Coverage for Solar Cycle 25 [18]
   Penza, Valentina, Berrilli, Francesco, Bertello, Luca, Cantoresi, Matteo & Criscuoli, Serena, ApJ, 922, L12

2014

1. Velocity and Temperature Response Functions of 61 Photospheric Lines in the Near-Infrared H Band (1500 - 1800 nm) - II [2]
   Penza, V. & Berrilli, F., Solar Physics, 289, 27

2012

1. Velocity and Temperature Response Functions of 77 Near-Infrared (800 - 1400 nm) Photospheric Lines - I [1]
   Penza, V. & Berrilli, F., Solar Physics, 277, 227

2006

1. Modeling the cyclic modulation of photospheric lines [22]
   Penza, V., Pietropaolo, E. & Livingston, W., A&A, 454, 349

2004

1. The sensitivity of the C I 538.0 nm Fe I 537.9 nm and Ti II 538.1 nm lines to solar active regions [17]
   Penza, V., Caccin, B. & Del Moro, D., A&A, 427, 345
2. Comparison of model calculations and photometric observations of bright ``magnetic'' regions [17]
   Penza, V., Caccin, B., Ermolli, I. & Centrone, M., A&A, 413, 1115