Speaker
Description
Combined observations from the Metis coronagraph and EUI/FSI on board Solar Orbiter, together with recent results, will be presented to focus on future scientific objectives of the JEDI (Joint EUV coronal Diagnostic Investigation) instrument on Vigil.
In particular, we discuss the potential of multi-band coronal observations
(Metis in visible light and UV, and FSI at 174 Å and 304 Å, both on-disk and in coronagraphic mode) to provide a unique opportunity to infer the physical parameters of the streamer belt, where the sources of the slow solar wind are located.
This is fundamental for studying the key processes that connect coronal sources of outflows with the heliosphere and for constraining coronal models characterizing the mechanisms responsible for plasma heating and acceleration.
| Do you plan to attend in-person or online? | In-person |
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