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Title: Electromagnetic wave propagation through an overdense magnetized collisional plasma layer

Journal Article · · Journal of Applied Physics
DOI:https://doi.org/10.1063/1.3195085· OSTI ID:21361773
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  1. Voss Scientific LLC, Albuquerque, New Mexico 87108 (United States)

The results of investigations into the feasibility of using a magnetic window to propagate electromagnetic waves through a finite-sized overdense plasma slab are described. We theoretically calculate the transmission coefficients for right- and left-handed circularly polarized plane waves through a uniform magnetized plasma slab. Using reasonable estimates for the plasma properties expected to be found in the ionized shock layer surrounding a hypersonic aircraft traveling in the earth's upper atmosphere (radio blackout conditions), and assuming a 1 GHz carrier frequency for the radio communications channel, we find that the required magnetic field for propagation of right-handed circularly polarized, or whistler, waves is on the order of a few hundred gauss. Transmission coefficients are calculated as a function of sheath thickness and are shown to be quite sensitive to the electron collision frequency. One-dimensional particle-in-cell simulations are shown to be in good agreement with the theory. These simulations also demonstrate that Ohmic heating of the electrons can be considerable. Two- and three-dimensional particle-in-cell simulations using a simplified waveguide and antenna model illustrate the same general transmission behavior as the theory and one-dimensional simulations. In addition, a net focusing effect due to the plasma is also observed in two and three dimensions. These simulations can be extended to design and analyze more realistic waveguide and antenna models.

OSTI ID:
21361773
Journal Information:
Journal of Applied Physics, Vol. 106, Issue 4; Other Information: DOI: 10.1063/1.3195085; (c) 2009 American Institute of Physics; ISSN 0021-8979
Country of Publication:
United States
Language:
English