Investigating the formation of post-coronal mass ejection plasmoids observed by the Metis coronagraph on board Solar Orbiter

Coronal mass ejections (CMEs) are complex transient solar phenomena often associated with solar flares, large-scale current sheets (CS), and the formation of dense plasma structures, known as plasmoids or plasma blobs. Multiwavelength observations are required to study the properties, onset, and evolution of these structures. We studied the properties of multiple plasma blobs that are likely related with magnetic reconnection that continues after the transit of a CME over the solar west limb on