Whistler mode chorus is an important magnetospheric wave emission playing a major role in radiation belt dynamics, where it contributes to both the acceleration and loss of relativistic electrons. In
Dataset accompanying manuscript titled "Reconstructing magnetotail reconnection events using data mining is feasible and repeatable" Abstract: Recently, Stephens et al. (2023) utilized a data mining
This dataset contains 3D Proton distributions (particle phase space density) from the CIS-CODIF instrument on the Cluster C4 spacecraft in High-Sensitivity.
This is the dataset created for the JGR paper "Multi-Point Observations of Quasiperiodic Emission Intensification and Effects on Energetic Electron Precipitation"
