Solar flares are an impulsive increase of emissions as a result of impetuous release of
magnetic free energy. This paper will present the recent progress on circular-ribbon flares …

Context. Most observations of the solar corona beyond 2 R⊙ consist of broadband visible
light imagery carried out with coronagraphs. The associated diagnostics mainly consist of …

For the first time the evolution of the coronal reconfiguration after a coronal mass ejection
(CME) was observed by the multichannel Metis Coronagraph on board the ESA–Solar …

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

Based on observations from the Solar Dynamics Observatory (SDO) and the Solar and
Heliospheric Observatory (SOHO), we investigate 30 apparent current sheets during 1999 …

Context. The Solar Orbiter Heliospheric Imager (SoloHI) instrument of the Solar Orbiter
mission is a next-generation heliospheric imager. New observations from SoloHI …

The current sheet is a characteristic structure of magnetic energy dissipation during the
magnetic reconnection process. So far, the width and depth of the current sheet are still …

We have carried out a comprehensive study of the temperature structure of plasmoids, which
successively occurred in recurrent active region jets. The multithermal plasmoids were seen …

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 …

Introduction: Large-scale solar eruptive activities have a close relationship with coronal
magnetic flux ropes. Previous numerical studies have found that the equilibrium of a coronal …