activity
20192021
most citedMetis: the Solar Orbiter visible light and ultraviolet coronal imager

190 citations · 414 across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.SR202132 cited

Exploring the Solar Wind from its Source on the Corona into the Inner Heliosphere during the First Solar Orbiter - Parker Solar Probe Quadrature

Daniele Telloni, Vincenzo Andretta, Ester Antonucci +68

This Letter addresses the first Solar Orbiter (SO) -- Parker Solar Probe (PSP) quadrature, occurring on January 18, 2021, to investigate the evolution of solar wind from the extend…

astro-ph.SR20218 cited

Effects of the chromospheric Lyα line profile shape on the determination of the solar wind HI outflow velocity using the Doppler dimming technique

G. E. Capuano, S. Dolei, D. Spadaro +15

The determination of solar wind outflow velocity is fundamental in order to probe the mechanisms of wind acceleration in the corona. We aim to study, via the Doppler dimming techni…

astro-ph.SR202150 cited

First light observations of the solar wind in the outer corona with the Metis coronagraph

M. Romoli, E. Antonucci, V. Andretta +65

The investigation of the wind in the solar corona initiated with the observations of the resonantly scattered UV emission of the coronal plasma obtained with UVCS-SOHO, designed to…

astro-ph.IM20212 cited

Progress on the Astrometric Gravitation Probe design

Mario Gai, Alberto Vecchiato, Alberto Riva +13

The Astrometric Gravitation Probe mission is a modern version of the 1919 Dyson-Eddington-Davidson experiment, based on a space-borne telescope with a permanent built-in eclipse, p…

astro-ph.IM20214 cited

The ASTRA project: a doorway to future astrometry

Mario Gai, Zhaoxiang Qi, Mario G. Lattanzi +15

Astrometric Science and Technology Roadmap for Astrophysics (ASTRA) is a bilateral cooperation between China and Italy with the goal of consolidating astrometric measurement concep…

astro-ph.IM20216 cited

RAFTER: Ring Astrometric Field Telescope for Exo-planets and Relativity

Alberto Riva, Mario Gai, Alberto Vecchiato +5

High precision astrometry aims at source position determination to a very small fraction of the diffraction image size, in high SNR regime. One of the key limitations to such goal…