- 1.1.4.1.1 Interchange reconnection between open and closed field lines and its role in slow wind generation
- 1.1.4.1.2 Identify coronal reconnection sites by measuring impulsive event material
- 1.1.4.1.3 Identify reconnection exhausts in the solar wind
- 1.1.4.1.4 Current sheets inferred by determining the magnetic field geometries at local chromospheric heating sites
- 1.1.4.1.5 Identify and characterise the solar wind reconnection physics in current sheets with thickness down to the ion scales and smaller
- 1.1.4.1.6 Photospheric reconnection
- 1.1.4.1.7 Electron acceleration in coronal reconnection regions
- 1.1.4.1.8 Formation of flux ropes/CMEs via magnetic reconnection in the corona
Overview
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