TY - GEN
T1 - Comparison of Collisionless Plasma Plume Expansions Under Different External Magnetic Fields
AU - Vatansever, D.
AU - Levin, D.
N1 - Publisher Copyright:
© 2025, American Institute of Aeronautics and Astronautics Inc, AIAA. All rights reserved.
PY - 2025
Y1 - 2025
N2 - Three-dimensional (3-D), fully kinetic particle-in-cell (PIC) simulations using the CHAOS code are conducted to investigate the expansion dynamics of magnetized mesothermal plasma plumes under various magnetic field topologies. The simulations incorporate static magnetic fields, including divergent and axially uniform configurations, mapped onto the Electric Forest of Trees (E-FOT) grids in CHAOS to explore their effects on plasma plume collimation. This study examines the influence of field strength and topology on plume behavior by tracking the plume front’s time evolution, analyzing macroparameters across cross-sections, evaluating electron thermal energy losses, and characterizing non-Maxwellian electron velocity distribution functions (EVDFs). The study demonstrates that uniform magnetic fields with strengths exceeding 150 G significantly enhance plume collimation, resulting in plume front speeds at least one ion acoustic speed (1 cs0) higher than those observed in unmagnetized or diverging field cases. Additionally, improved collimation in uniform fields reduces electron thermal energy losses by 50% and 60% compared to the losses observed in diverging field and unmagnetized cases, respectively.
AB - Three-dimensional (3-D), fully kinetic particle-in-cell (PIC) simulations using the CHAOS code are conducted to investigate the expansion dynamics of magnetized mesothermal plasma plumes under various magnetic field topologies. The simulations incorporate static magnetic fields, including divergent and axially uniform configurations, mapped onto the Electric Forest of Trees (E-FOT) grids in CHAOS to explore their effects on plasma plume collimation. This study examines the influence of field strength and topology on plume behavior by tracking the plume front’s time evolution, analyzing macroparameters across cross-sections, evaluating electron thermal energy losses, and characterizing non-Maxwellian electron velocity distribution functions (EVDFs). The study demonstrates that uniform magnetic fields with strengths exceeding 150 G significantly enhance plume collimation, resulting in plume front speeds at least one ion acoustic speed (1 cs0) higher than those observed in unmagnetized or diverging field cases. Additionally, improved collimation in uniform fields reduces electron thermal energy losses by 50% and 60% compared to the losses observed in diverging field and unmagnetized cases, respectively.
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U2 - 10.2514/6.2025-2491
DO - 10.2514/6.2025-2491
M3 - Conference contribution
AN - SCOPUS:105001261126
SN - 9781624107238
T3 - AIAA Science and Technology Forum and Exposition, AIAA SciTech Forum 2025
BT - AIAA Science and Technology Forum and Exposition, AIAA SciTech Forum 2025
PB - American Institute of Aeronautics and Astronautics Inc, AIAA
T2 - AIAA Science and Technology Forum and Exposition, AIAA SciTech Forum 2025
Y2 - 6 January 2025 through 10 January 2025
ER -