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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

Created by Yannis Zouganelis, last modified on 05 Feb, 2023

Identify and characterise the solar wind reconnection physics in current sheets with thickness down to the ion scales and smaller (Huttunen et al., 2007; Chen et al., 2007). [not necessarily at pelihelion]

Relevant SOOPs: I_DEFAULT