VLF AND ELF PROPAGATION DURING SUDDEN IONOSPHERIC DISTURBANCES,

Abstract

The study presents the results of a theoretical analysis of the propagation of electromagnetic waves in the very-low-frequency (VLF) and extremely-low-frequency (ELF) ranges in the earth-ionosphere cavity during solar flares. The calculations, which are based upon nominal models of ambient conditions and solar-flare x-ray fluxes and spectra, result in mode-attenuation coefficients which are in good general agreement with observations. The propagation is enhanced relative to ambient conditions at ELF and upper VLF frequencies but is degraded in the lower VLF range. This general behavior is quite insensitive to the details of the assumed x-ray spectrum, the main requirement being a sufficient concentration of x-ray energy in the 1 - 8 A wavelength band. This class of spectrum tends to cause a moderate lowering of the D-region accompanied by an increase in the height gradient of conductivity in the reflection region; this in turn causes the observed phenomena at ELF and VLF during sudden ionospheric disturbances. (Author)

Document Details

Document Type
Technical Report
Publication Date
Sep 01, 1969
Accession Number
AD0697754

Entities

People

  • E. C. Field

Organizations

  • RAND Corporation

Tags

DTIC Thesaurus Topics

  • Extremely Low Frequency
  • Frequency
  • Ionospheric Disturbances
  • Solar Flares
  • Spectra
  • Very Low Frequency
  • X Ray Spectra
  • X Rays

Fields of Study

  • Physics

Readers

  • Astronomy and Astrophysics.
  • Plasma Physics / Magnetohydrodynamics
  • Solar Physics