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Perturbation theory for electromagnetic radiation in magnetoplasma

Perturbation theory for electromagnetic radiation in magnetoplasma

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A new perturbation technique is developed for resolving electromagnetic-radiation problems in a magnetoplasma with a weak anisotropy. The technique provides the capability of computing the full-wave fields in analytically closed form. Each successive term in the iterative solution is smaller than the preceding one by a small parameter of the anisotropy. As an example, the technique is used to calculate the Green function for a δ function source oriented parallel to the static magnetic field.

References

    1. 1)
      • T.N.C. Wang , T.E. Bell . Radiation resistance of a short dipole in a magnetoplasma. Radio Sci. , 167 - 177
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      • J.A. Ratcliffe . (1959) , The magneto-ionic theory and its applications to the ionosphere.
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      • W.P. Allis , S.J. Buchsbaum , A. Bers . (1963) , Waves in anisotropic plasmas.
    4. 4)
      • P.C. Clemmow . The theory of electromagnetic waves in a simple anisotropic medium. Proc. IEE , 1 , 101 - 106
    5. 5)
      • E. Arbel , L.B. Felson , E.C. Jordan . (1963) Theory of radiation from source in anisotropic madia, Symposium on electromagnetic theory and antennas—Pt. I.
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