activity
20052023
most citedMetis: the Solar Orbiter visible light and ultraviolet coronal imager

190 citations · 470 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.IM2023★ 1 cited

The Critical Coronal Transition Region: A Physics-framed Strategy to Uncover the Genesis of the Solar Wind and Solar Eruptions

Angelos Vourlidas, Amir Caspi, Yuan-Kuen Ko +10

Our current theoretical and observational understanding suggests that critical properties of the solar wind and Coronal Mass Ejections (CMEs) are imparted within 10 Rs, particularl…

astro-ph.SR2021★ 32 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.SR2021★ 50 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.SR2019★ 190 cited

Metis: the Solar Orbiter visible light and ultraviolet coronal imager

Ester Antonucci, Marco Romoli, Vincenzo Andretta +100

Metis is the first solar coronagraph designed for a space mission capable of performing simultaneous imaging of the off-limb solar corona in both visible and UV light. The observat…

astro-ph.SR2019★ 103 cited

Element Abundances: A New Diagnostic for the Solar Wind

J. Martin Laming, Angelos Vourlidas, Clarence Korendyke +11

We examine the different element abundances exhibited by the closed loop solar corona and the slow speed solar wind. Both are subject to the First Ionization Potential (FIP) Effect…

astro-ph.SR2014★ 93 cited

The Role of Turbulence in Coronal Heating and Solar Wind Expansion

S. R. Cranmer, M. Asgari-Targhi, M. P. Miralles +4

Plasma in the Sun's hot corona expands into the heliosphere as a supersonic and highly magnetized solar wind. This paper provides an overview of our current understanding of how th…