5.10.7 How do the combined electron strahl and composition signatures vary across reconnecting solar wind current sheets? Are these consistent with expectations of interchange reconnection models? What are the combined signatures in other solar wind structures (e.g. shocks, CIRs, CMEs), and how definitive are these in determining solar origins and/or defining processes occurring in the solar wind? 



 

Required observations:

  • SWASWA Normal Mode, a few tens of minutes around an event, other instruments: MAG, RPW.

Duration:

  • A few tens of minutes around an event.

Other constraints: