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Abstract: Comparing the instantaneous energy transfer rates of plasmoid/flux rope and reconnection magnetic topologies in solar wind turbulence as seen by Cluster (AGU25)

Comparing the instantaneous energy transfer rates of plasmoid/flux rope and reconnection magnetic topologies in solar wind turbulence as seen by Cluster

Sandra C Chapman1, Bogdan Hnat2, Nicholas Wynn Watkins1,3 and Conan Liptrott1, (1)University of Warwick, CFSA, Physics, Coventry, United Kingdom, (2)University of Warwick, Coventry, United Kingdom, (3)London School of Economics, London, United Kingdom