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Context. The generation of the slow solar wind remains an open problem in heliophysics. One of the current theories among those aimed at explaining the injection of coronal plasma in the interplanetary medium is based on interchange reconnection. It assumes that the exchange of magnetic connectivity between closed and open fields allows the injection of coronal plasma in the interplanetary medium to travel along the newly reconnected open field. However, the exact mechanism underlying this effect is still poorly understood. ...
Published by: \aap Published on: jul
YEAR: 2023   DOI: 10.1051/0004-6361/202245611
Published by: \apj Published on: 01/2017
YEAR: 2017   DOI: 10.3847/1538-4357/834/1/62