Fully Exploiting 3D-3V Phase Space to Understand Plasma Heating and Particle Acceleration in Collisionless Shocks
ORAL
Abstract
In weakly collisional plasmas, the physical mechanisms by which the plasma species are heated and particles are accelerated are governed by collisionless interactions between the electromagnetic fields and individual particles. The recently developed field-particle correlation technique was devised to identify and characterize the mechanisms that energize particles in the six-dimensional (3D-3V) phase space of kinetic plasmas, mechanisms underlying the fundamental plasma processes of kinetic turbulence, collisionless magnetic reconnection, and collisionless shocks. Here we present an overview of how the field-particle correlation method can be applied to gain deeper insight into the kinetic plasma processes that govern how particles are energized at collisionless shocks. Requiring only single-point measurements in space, the technique can be used to identify well-known acceleration mechanisms, such as shock drift acceleration and shock surfing acceleration. In addition, it shows promise to be able to separate the energization mediated by micro-instabilities arising in the shock transition from that due to the macroscopic shock fields.
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Publication: A Field-Particle Correlation Analysis of a Perpendicular Magnetized Collisionless Shock;<br>Juno, J., Howes, G. G., TenBarge, J. M., Wilson, L. B., III, Spitkovsky, A. Caprioli, D., Klein, K. G., and Hakim, A.;<br>J. Plasma Phys., 87, 905870316 (2021).
Presenters
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Gregory G Howes
University of Iowa
Authors
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Gregory G Howes
University of Iowa
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James L Juno
The University of Iowa, University of Iowa
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Collin R Brown
University of Iowa
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Colby C Haggerty
University of Hawaii
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Jason M TenBarge
Princeton University
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Damiano Caprioli
University of Chicago
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Anatoly Spitkovsky
Princeton University
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Lynn B Wilson
NASA Goddard Space Flight Center