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, was supported in part by the Israel Science Foundation (grant no. 368/14). C.T.R. was supported through NASA's Magnetospheric Multiscale mission. A.P.D. was supported by the Swedish Civil Contingencies Agency (MSB) (grant no. 2016-2102). C.C. acknowledges the Cluster FGM (grant no. ST/P003427/1) from UKSA/STFC. N.G. acknowledges financial support from NASA grant 80NSSC17K0015 and NSF grant 1663770. Author contributions: M.A.B. performed the initial analysis and motivation for the study. A.P.D. analyzed the data and wrote the first draft of the manuscript together with, were funded by the Academy of Finland (grant nos. 288472 and 267073/2013). Y.V.K. was supported by the Swedish Research Council
Competing interests: The authors declare that they have no competing interests. Data and materials availability: All data needed to evaluate the conclusions in the paper are present in the paper and/or the Supplementary Materials. Additional data related to this paper may be requested from the authors. We acknowledge the Cluster FGM, DWP, EFW, and CIS instrument teams and also the Cluster Science Archive. The data used in this study are openly available through the Cluster Science Archive ,
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