Numerical simulation data for submission to Geophysical Research Letters: 'Flow Channels and the Generation of Alfvénic Turbulence along Storm-time Inner Magnetospheric Field-lines', C. C. Chaston 2022

Contains data from 3-D numerical simulation of inner magnetospheric flow channels: <br> 1. 2-D data including the stream function, vector potential and normalized density from an equatorial slice through the 3-D simulation volume as a function of time. <br> 2. 3-D data of the normalized density variation within the simulation volume. <br> 3. Time arrays corresponding to the data above <br> All variables and spatial grids are defined in the manuscript under review from September 2022 with Geophysical Research Letters.