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- W3211943666 abstract "The ion-Weibel instability is a leading candidate mechanism for the formation of collisionless shocks observed in may astrophysical systems. Experimental and computational studies have shown that the ion-Weibel instability drives current filamentation in interpenetrating plasma flows 1 , 2 with the capability to mediate collisionless shock formation and subsequent particle acceleration 3 in the lab. The present work focuses on the study of nonlinear ion-Weibel evolution under various plasma conditions through utilization of different ion species and experimental geometries. Temporally varying plasma condition are determined using benchmarked FLASH simulations. Path-integrated B-field distributions are retrieved from experimental proton images in all cases and Fourier analyzed to quantify the dominant filament scale-size and estimate the B-field strength. This new analysis methodology demonstrates that the first ~400ps of plasma interpenetration sets the spectral characteristics of ion-Weibel filamentation, and that underlying plasma conditions later in time do not significantly alter nonlinear filament evolution." @default.
- W3211943666 created "2021-11-22" @default.
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- W3211943666 date "2021-09-12" @default.
- W3211943666 modified "2023-09-26" @default.
- W3211943666 title "Nonlinear Evolution of the Ion-Weibel Instability in Interpenetrating Plasmas of CH, Al, and Cu" @default.
- W3211943666 doi "https://doi.org/10.1109/icops36761.2021.9588627" @default.
- W3211943666 hasPublicationYear "2021" @default.
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