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Evolution and Influences of Plasma Turbulence in the Heliosphere (Matthaeus/ Parashar/Chasapis)
Friday July 28, 930 am SHINE 2017, July 23-28, 2017 Manor Saint-Sauveur, QC Canada
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Focus on kinetic physics and response of kinetic scales and particle VDFs to turbulence cascade
How kinetic physics, especially particle vdfs, respond to turbulence Heating Exchange of energy with E/M field Microscopic flows Scale to scale cascade What MMS can tell us in SW magnetosheath
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Scene setters and themes for discussion
Yan Yang (Peking U., U of Delaware): Channels of energy transfer, exchange & dissipation Theory and simulations Clarify the role of J.E, “p-theta” and “Pi-D” and other effects that MMS can measure! Alex Chasapis (U. of Delaware): MMS observations Magnetic fields, pressure tensors, currents, stress tensors Sergio Servidio (U. of Calabria): velocity space cascade and analysis Hermite representation MMS in magnetosheath V-space cascade observation and theory
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