Abstract

Summary form only given. The interaction of electromagnetic (EM) waves with magnetized plasmas is an active area of research. Most of the research so far have focused upon waves launched in the (k ∥ B <sub xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">o</sub> ) mode where the wave vector (k) is parallel to the static magnetic field (B <sub xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">o</sub> ), and B <sub xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">o</sub> is approximately uniform over the plasma volume with the dimension of the plasma much larger than the free space wavelength λ <sub xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">o</sub> , corresponding to the launched waves. There are only a few investigations in the k⊥B <sub xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">o</sub> mode.We study wave interaction with bounded plasmas in the k⊥B <sub xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">0</sub> mode where the waveguide cutoff wavelength λc is comparable [λc(≅14 cm) <sub xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">~</sub> λ <sub xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">0</sub> (≅12 cm)] to λ <sub xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">0</sub> . A high-density, radially inhomogeneous argon plasma is generated and confined in a cylindrically symmetric magnetostatic well (B <sub xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">0</sub> ∝ r <sup xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">3</sup> ), created by an octupole arrangement of permanent magnets surrounding the waveguide. In this work, the effect of the inhomogeneous, anisotropic magneto-plasma on the polarization of the penetrating waves is experimentally investigated. Polar measurement of the wave electric-field (E) intensity reveals that E is linearly polarized in the radial plane as expected. However, an asymmetry is observed in the lobes of the dipole-like .E-field polar intensity variation. The axis of polarization with respect to vacuum rotates with increase in plasma density and axial plasma interaction length (L <sub xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">0</sub> ). We found that for L <sub xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">0 ~</sub> 15 cm, the rotation angle Δφ <sub xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">~</sub> 10°. Such rotation hitherto unreported in laboratory bounded plasmas may be attributed to birefringence of the wave in the medium similar to optical crystals. Measurement of the wave vector k in the magnetoplasma by heterodyne technique is expected to shed further light on the nature of the birefringence.

Full Text
Paper version not known

Talk to us

Join us for a 30 min session where you can share your feedback and ask us any queries you have

Schedule a call

Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.