Collision of expanding plasma clouds: Mixing, flow morphology, and instabilities

Abstract

The collision of two expanding plasma flows is investigated with an emphasis on the mixing flow. The study adheres to laboratory experiments where two Ohmically exploding parallel wires launch hot plasma coronas toward each other. The interpenetration and mixing of the coronas is followed by the collision and mixing of the slowly moving phases of the melted wires. In a recent publication [M. A. Malkov and V. I. Sotnikov, Phys. Plasmas 25(10), 102108 (2018)], a stationary flow that emerges from interpenetrating coronas and plasma microinstabilities in the mixing region had been studied analytically. In this present work, using two-dimensional numerical simulations, we investigate the time evolution of the flow, compare its patterns resulting from collisions of the rarefied coronas and dense wire material, and examine the macroscopic stability of the flow. The stability of the mixing layer with respect to the so-called thin-shell instability is specifically addressed.

Document Details

Document Type
Pub Defense Publication
Publication Date
Dec 01, 2020
Source ID
10.1063/5.0024615

Entities

People

  • A. Hamilton
  • Mikhail A. Malkov
  • V. I. Sotnikov

Organizations

  • Air Force Office of Scientific Research
  • Air Force Research Laboratory
  • University of California, San Diego

Tags

Fields of Study

  • Physics

Readers

  • Fluid Dynamics.
  • Plasma Physics / Magnetohydrodynamics
  • Pulsed Power and Plasma Physics.