V. Penza

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

B. Caccin, D. Del Moro, D. Moro, 2004 .

2-D multiline spectroscopy of the solar photosphere

Ermanno Pietropaolo, B. Caccin, Francesco Berrilli, 2002 .

Comparison of model calculations and photometric observations of bright magnetic regions

B. Caccin, Mauro Centrone, Ilaria Ermolli, 2004 .

Statistical behaviour of a proxy of the entropy production rate of the solar photosphere

Francesco Berrilli, Giuseppe Consolini, D. Del Moro, 2019 .

Line-Depth and Teff Variations with the Solar Cycle due to Possible Size-Changes of Photospheric Granulation

V. Penza, Bruno Caccin, 2000 .