29/09/2026
This International Team - led by R. D'Amicis & M. Velli - is investigating the solar sources ☀️ and evolution of the Alfvénic slow wind.
Using observations from Parker Solar Probe and Solar Orbiter, together with next-generation models, the team is studying how waves and turbulence help the solar wind escape the Sun’s magnetic field and form the heliosphere.
Their results show that while fast solar-wind streams are broadly similar, slower streams differ depending on where and how they originate. Alfvénic slow wind is linked to small, rapidly expanding open magnetic regions, whereas non-Alfvénic slow wind can escape through magnetic instabilities and reconnection.
➡️ https://teams.issibern.ch/alfvenicslowwind/