[HTML][HTML] Rome Precision Solar Photometric Telescope: precision solar full-disk photometry during solar cycles 23–25

I Ermolli, F Giorgi, T Chatzistergos - Frontiers in Astronomy and Space …, 2022 - frontiersin.org
The Rome Precision Solar Photometric Telescope (Rome/PSPT) is a ground-based
telescope engaged in precision solar photometry. It has a 27-year database of full-disk …

2-D multiline spectroscopy of the solar photosphere

F Berrilli, G Consolini, E Pietropaolo, B Caccin… - Astronomy & …, 2002 - aanda.org
The structure and dynamics of the photosphere are investigated, with time series of
broadband and monochromatic images of quiet granulation, at the solar disk center. Images …

Height-dependent velocity structure of photospheric convection in granules and intergranular lanes with Hinode/SOT

T Oba, Y Iida, T Shimizu - The Astrophysical Journal, 2017 - iopscience.iop.org
The solar photosphere is the visible surface of the Sun, where many bright granules,
surrounded by narrow dark intergranular lanes, are observed everywhere. The granular …

Time series of high resolution photospheric spectra in a quiet region of the Sun-II. Analysis of the variation of physical quantities of granular structures

KG Puschmann, BR Cobo, M Vázquez… - Astronomy & …, 2005 - aanda.org
From the inversion of a time series of high resolution slit spectrograms obtained from the
quiet sun, the spatial and temporal distribution of the thermodynamical quantities and the …

Using the infrared iron lines to probe solar subsurface convection

I Milić, HN Smitha, A Lagg - Astronomy & Astrophysics, 2019 - aanda.org
Context. Studying the properties of solar convection using high-resolution
spectropolarimetry began in the early 1990s with the focus on observations in the visible …

Occurrence and persistence of magnetic elements in the quiet Sun

F Giannattasio, F Berrilli, G Consolini… - Astronomy & …, 2018 - aanda.org
Context. Turbulent convection efficiently transports energy up to the solar photosphere, but
its multi-scale nature and dynamic properties are still not fully understood. Several works in …

Scaling properties of magnetic field fluctuations in the quiet Sun

F Giannattasio, G Consolini, F Berrilli… - Astronomy & …, 2022 - aanda.org
Context. The study of the dynamic properties of small-scale magnetic fields in the quiet
photosphere is important for several reasons:(i) it allows us to characterise the dynamic …

The complex nature of magnetic element transport in the quiet Sun: The Lévy-walk character

F Giannattasio, G Consolini, F Berrilli… - The Astrophysical …, 2019 - iopscience.iop.org
The study of the dynamic properties of small-scale magnetic fields in the solar photosphere
(magnetic elements, MEs) provides a fundamental tool to investigate some still unknown …

Stellar turbulent convection: the multiscale nature of the solar magnetic signature

S Scardigli, F Berrilli, D Del Moro, L Giovannelli - Atmosphere, 2021 - mdpi.com
The multiscale dynamics associated with turbulent convection present in physical systems
governed by very high Rayleigh numbers still remains a vividly disputed topic in the …

Time series of high resolution photospheric spectra in a quiet region of the sun-I. Analysis of global and spatial variations of line parameters

K Puschmann, M Vázquez, JA Bonet, BR Cobo… - Astronomy & …, 2003 - aanda.org
A 50 min time series of one-dimensional slit-spectrograms, taken in quiet sun at disk centre,
observed at the German Vacuum Tower Telescope (Observatorio del Teide), was used to …