This Letter reports the first observation of the onset of fully developed turbulence in the solar
corona. Long time series of white-light coronal images, acquired by Metis aboard Solar …

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 …

The unexpected observation of a sudden expulsion of mass through the solar corona in
1971 opened up a new field of interest in solar and stellar physics. The discovery came from …

Aims We aim to investigate and characterize the morphology and dynamics of small-scale
coronal plasma density inhomogeneities detected as brighter, denser features propagating …

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 …

This paper addresses the first direct investigation of the energy budget in the solar corona.
Exploiting joint observations of the same coronal plasma by Parker Solar Probe and the …

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 …

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 …

Context. Ultraviolet (UV) emission from coronal mass ejections can provide information on
the evolution of plasma dynamics, temperature, and elemental composition, as …

Context. The Metis coronagraph is one of the remote sensing instruments of the ESA-NASA
Solar Orbiter mission. The goal for the instrument is to enable the study of the solar …