activity
20212026
most citedObservation of Magnetic Switchback in the Solar Corona

56 citations · 113 across the 10 of their papers we have counts for

collaborators

10 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.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★ 3 cited

Does Turbulence along the Coronal Current Sheet Drive Ion Cyclotron Waves?

Daniele Telloni, Gary P. Zank, Laxman Adhikari +32

Evidence for the presence of ion cyclotron waves, driven by turbulence, at the boundaries of the current sheet is reported in this paper. By exploiting the full potential of the jo…

astro-ph.SR2023★ 17 cited

Slow wind belt in the quiet solar corona

E. Antonucci, C. Downs, G. E. Capuano +16

The slow solar wind belt in the quiet corona, observed with the Metis coronagraph on board Solar Orbiter on May 15, 2020, during the activity minimum of the cycle 24, in a field of…

astro-ph.SR2022★ 1 cited

Connecting Solar Orbiter remote-sensing observations and Parker Solar Probe in-situ measurements with a numerical MHD reconstruction of the Parker spiral

Ruggero Biondo, Alessandro Bemporad, Paolo Pagano +21

As a key feature, NASA's Parker Solar Probe (PSP) and ESA-NASA's Solar Orbiter (SO) missions cooperate to trace solar wind and transients from their sources on the Sun to the inner…

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.SR2021★ 4 cited

Measuring the F-corona intensity through time correlation of total and polarized visible light images

A. Burtovoi, G. Naletto, S. Dolei +4

We present a new correlation method for deriving the F-corona intensity distribution, which is based on the analysis of the evolution of the total and polarized visible light (VL)…

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…