activity
20162026
most citedObservation of Magnetic Switchback in the Solar Corona

56 citations · 215 across the 17 of their papers we have counts for

collaborators

17 papers

astro-ph.SR2026

PRICM3: A novel Polarization Ratio framework for three-dimensional CME reconstruction

Yara De Leo, Manuela Temmer, Fernando M. López +15

Coronal mass ejections (CMEs) are inherently three-dimensional (3D), but traditional white-light coronagraphs provide only two-dimensional (2D) projections. While the Polarization…

astro-ph.SR2026

A view of the evolution of a CME and the associated wave-trains at high spatial and temporal resolution

G. Russano, Y. De Leo, F. Frassati +13

Context. Studying the kinematic and dynamic evolution of fast eruptive events from the middle to high solar corona is a primary objective of the Metis coronagraph on Solar Orbiter.…

astro-ph.SR2025

Metis Observations of Alfvénic Outflows Driven by Interchange Reconnection in a Pseudostreamer

P. Romano, P. Wyper, V. Andretta +33

This study presents observations of a large pseudostreamer solar eruption and, in particular, the post-eruption relaxation phase, as captured by Metis onboard the Solar Orbiter on…

astro-ph.SR2024

Study of solar brightness profiles in the 18-26 GHz frequency range with INAF radio telescopes II. Evidence for coronal emission

M. Marongiu, A. Pellizzoni, S. Righini +43

One of the most important objectives of solar physics is the physical understanding of the solar atmosphere, the structure of which is also described in terms of the density (N) an…

astro-ph.SR2023

Eruptive events with exceptionally bright emission in HI Ly-alpha observed by the Metis coronagraph

G. Russano, V. Andretta, Y. De Leo +29

Metis, the coronagraph on board Solar Orbiter, provides for the first time coronagraphic imaging in the ultraviolet HI Ly-alpha line and, simultaneously, in polarized visible light…

astro-ph.SR2023

Coronal Heating Rate in the Slow Solar Wind

Daniele Telloni, Marco Romoli, Marco Velli +59

This Letter reports the first observational estimate of the heating rate in the slowly expanding solar corona. The analysis exploits the simultaneous remote and local observations…

astro-ph.SR2023★ 15 cited

In-flight validation of Metis Visible-light Polarimeter Coronagraph on board Solar Orbiter

A. Liberatore, S. Fineschi, M. Casti +21

Context. The Metis coronagraph is one of the remote-sensing instruments of the ESA/NASA Solar Orbiter mission. Metis is aimed at the study of the solar atmosphere and solar wind by…

astro-ph.SR2022★ 6 cited

Three-dimensional reconstruction of type U radio bursts: a novel remote sensing approach for coronal loops

S. Mancuso, D. Barghini, A. Bemporad +5

Type U radio bursts are impulsive coherent radio emissions produced by the Sun that indicate the presence of subrelativistic electron beams propagating along magnetic loops in the…

astro-ph.SR2022★ 56 cited

Observation of Magnetic Switchback in the Solar Corona

Daniele Telloni, Gary P. Zank, Marco Stangalini +49

Switchbacks are sudden, large radial deflections of the solar wind magnetic field, widely revealed in interplanetary space by the Parker Solar Probe. The switchbacks' formation mec…

astro-ph.SR2022★ 18 cited

A Coronal Mass Ejection followed by a prominence eruption and a plasma blob as observed by Solar Orbiter

A. Bemporad, V. Andretta, R. Susino +26

On February 12, 2021 two subsequent eruptions occurred above the West limb, as seen along the Sun-Earth line. The first event was a typical slow Coronal Mass Ejection (CME), follow…

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★ 13 cited

Combining White Light and UV Lyman-alpha Coronagraphic Images to determine the Solar Wind Speed: the Quick Inversion Method

Alessandro Bemporad, Silvio Giordano, Luca Zangrilli +1

This work focuses on the combination of White Light (WL) and UV (Ly-alpha) coronagraphic images to demonstrate the capability to measure the solar wind speed in the inner corona di…

astro-ph.SR2021★ 12 cited

Radio evidence for a shock wave reflected by a coronal hole

S. Mancuso, A. Bemporad, F. Frassati +4

We report the first unambiguous observational evidence in the radio range of the reflection of a coronal shock wave at the boundary of a coronal hole. The event occurred above an a…

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.IM2021★ 10 cited

Cosmic-ray flux predictions and observations for and with Metis on board Solar Orbiter

C. Grimani, V. Andretta, P. Chioetto +41

The Metis coronagraph is one of the remote sensing instruments hosted on board the ESA/NASA Solar Orbiter mission. Metis is devoted to carry out the first simultaneous imaging of t…

astro-ph.SR2021★ 1 cited

SWELTO -- Space WEather Laboratory in Turin Observatory

A. Bemporad, L. Abbo, D. Barghini +20

SWELTO -- Space WEather Laboratory in Turin Observatory is a conceptual framework where new ideas for the analysis of space-based and ground-based data are developed and tested. Th…

astro-ph.SR2016★ 2 cited

Measuring coronal magnetic fields with remote sensing observations of shock waves

Alessandro Bemporad, Roberto Susino, Federica Frassati +1

Recent works demonstrated that remote sensing observations of shock waves propagating into the corona and associated with major solar eruptions can be used to derive the strength o…