Stochastic Heating of Electrons in Partially Magnetized Plasmas

POSTER

Abstract

In partially magnetized E x B discharges, there are many instabilities that occur, like electron cyclotron drift instability and modified two stream instability. Such instabilities occur along the E x B drift direction, creating a plasma wave. As electrons undergo gyromotion and drift motion, they interact with the plasma wave, sometimes behaving stochastically depending on the Hall parameter. When the electrons behave stochastically, this leads to a net increase of temperature perpendicular to the magnetic field and anomalous cross-field transport. The conditions under which stochasticity arises will be demonstrated and verified using Hamiltonian mechanics. The effect of electron-neutral collisions will also be incorporated into the model to demonstrate the transition from a plasma in a range of Hall parameters.

*This work was supported by a NASA Space Technology Graduate Research Opportunity, under Grant No. 80NSSC21K1273 and NASA through the Joint Advanced Propulsion Institute, a NASA Space Technology Research Institute under Grant No. 80NSSC21K1118.

Presenters

  • Andrew Christopher Denig

    • Stanford University

Authors

  • Andrew Christopher Denig

    • Stanford University
  • Kae Heller

    • Stanford University
  • Kentaro Hara

    • Stanford University