MAGNETIC DIRECTION DEPENDENCE OF THE VLF PHASE VELOCITY FOR THE FIRST TWO WAVEGUIDE MODES.

Abstract

The methods previously reported for the computation of the complex propagation constant for the dominant VLF waveguide mode (n=1) are extended to the second mode (n=2). A stratified cylindrical ionosphere model with axial magnetic field is ued to determine the wave impedances needed in the subsequent iterative procedure which yields the modal propagation constants in the magnetic East to West (EW) and magnetic West to East (WE) directions. The predictions for phase velocity differences between modes n=1 and n=2 can account for the recently reported observations on the magnetic direction dependence of the distance D between interference minima of these modes propagating below the nighttime ionosphere. The individual height variations of the components of the conductivity tensor should be considered, and ionosphere models of exponential height variation of conductivity are not adequate. The phase velocity difference between the two modes is less than one per cent, but it is smallest for EW propagation, so that the mode interference distance is 1000 to 2000 km greater for EW propagation than for WE propagation. (Author)

Document Details

Document Type
Technical Report
Publication Date
Jun 01, 1966
Accession Number
AD0635939

Entities

People

  • J. Galejs

Organizations

  • Sylvania Electric Products

Tags

Communities of Interest

  • Advanced Electronics

DTIC Thesaurus Topics

  • Computations
  • Conductivity
  • Impedance
  • Ionosphere
  • Magnetic Fields
  • Observation
  • Phase Velocity
  • Physical Properties
  • Waveguides

Fields of Study

  • Physics

Readers

  • Electromagnetic Wave Scattering and Antenna Radiation Engineering
  • Space/Atmospheric Physics.