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  • Burst mode resolution of EAS and PAS will provide fastest thermal distributions recorded at different radial distances in the solar wind. At high cadence, test:
  • how anisotropic and irregular are proton and electron distributions? This can test whether resonant heating or stochastic heating is the dominant heating mechanism.
  • how does the anisotropy change in time / space?
  • how are distributions related to local turbulence and global expansion?