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Defining the middle corona
The middle corona, the region roughly spanning heliocentric distances from 1.5 to 6 solar
radii, encompasses almost all of the influential physical transitions and processes that …
radii, encompasses almost all of the influential physical transitions and processes that …
The Imprint of Intermittent Interchange Reconnection on the Solar Wind
The solar wind is known to be highly structured in space and time. Observations from Parker
Solar Probe have revealed an abundance of so-called magnetic switchbacks within the near …
Solar Probe have revealed an abundance of so-called magnetic switchbacks within the near …
In-flight radiometric calibration of the Metis Visible Light channel using stars and comparison with STEREO-A/COR2 data
Y De Leo, A Burtovoi, L Teriaca, M Romoli… - Astronomy & …, 2023 - aanda.org
Context. We present the results for the in-flight radiometric calibration performed for the
Visible Light (VL) channel of the Metis coronagraph on board Solar Orbiter. Aims. The …
Visible Light (VL) channel of the Metis coronagraph on board Solar Orbiter. Aims. The …
Recurrent solar density transients in the slow wind observed with the Metis coronagraph
Aims We aim to investigate and characterize the morphology and dynamics of small-scale
coronal plasma density inhomogeneities detected as brighter, denser features propagating …
coronal plasma density inhomogeneities detected as brighter, denser features propagating …
Coronal heating rate in the slow solar wind
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 of the …
solar corona. The analysis exploits the simultaneous remote and local observations of the …
Space weather-related activities and projects on-going at INAF-Turin Observatory
Abstract The Solar Physics Group at the INAF-Turin Astrophysical Observatory (OATo) is
actually involved in different Space Weather (SW) projects and missions. In particular, this …
actually involved in different Space Weather (SW) projects and missions. In particular, this …
The first coronal mass ejection observed in both visible-light and UV HI Ly-α channels of the Metis coronagraph on board Solar Orbiter
Context. The Metis coronagraph on board Solar Orbiter offers a new view of coronal mass
ejections (CMEs), observing them for the first time with simultaneous images acquired with a …
ejections (CMEs), observing them for the first time with simultaneous images acquired with a …
Possible evidence for shear-driven Kelvin–Helmholtz instability along the boundary of fast and slow solar wind in the corona
This paper reports the first possible evidence for the development of the Kelvin–Helmholtz
(KH) instability at the border of coronal holes separating the associated fast wind from the …
(KH) instability at the border of coronal holes separating the associated fast wind from the …
Coronal mass ejection followed by a prominence eruption and a plasma blob as observed by Solar Orbiter
Context. On 2021 February 12, two subsequent eruptions occurred above the western limb
of the Sun, as seen along the Sun-Earth line. The first event was a typical slow coronal mass …
of the Sun, as seen along the Sun-Earth line. The first event was a typical slow coronal mass …
Eruptive events with exceptionally bright emission in HI Ly-α observed by the Metis coronagraph
G Russano, V Andretta, Y De Leo, L Teriaca… - Astronomy & …, 2024 - aanda.org
Context. Ultraviolet (UV) emission from coronal mass ejections can provide information on
the evolution of plasma dynamics, temperature, and elemental composition, as …
the evolution of plasma dynamics, temperature, and elemental composition, as …