The Effect of Ionospheric Scintillations Fading on Aircraft-to-Satellite Communications.

Abstract

Ionospheric scintillation fading on a UHF earth-to-satellite communication link has a strong dependence on season, time-of-day, and geographic location. In the equatorial region + or - 20 deg. from the magnetic equator, 20 to 30 dB fades can be expected 1 to 2 hours after sunset during the equinox period. Airborne terminals may experience fade rates as fast as 1 fade per second to as slow as 1 fade in 90 seconds, depending on the direction of flight. The amplitude fading follows a power low distribution with a rate of F-2 to F-4 depending on fade rate. In the polar region an airborne terminal may experience ionospheric scintillation more often than near the equator but usually with less amplitude. Polar fading of 10 dB or less may occur 10 to 30% of the time. In the mid latitudes occasional random ionospheric scintillation may occur, but the fade depth and occurrence are so small as to pose only a minor annoyance to an airborne satellite communication system. (Author)

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Document Details

Document Type
Technical Report
Publication Date
Feb 01, 1979
Accession Number
ADA068758

Entities

People

  • Allen J. Johnson

Organizations

  • Air Force Research Laboratory

Tags

Communities of Interest

  • Space

DTIC Thesaurus Topics

  • Air
  • Air Force
  • Aircrafts
  • Artificial Satellites
  • Communication Systems
  • Cross Correlation
  • Electrons
  • Equatorial Regions
  • Ground Stations
  • High Latitudes
  • Ionospheric Scintillation
  • Magnetic Fields
  • Measurement
  • Polar Regions
  • Power Spectra
  • Satellite Communications
  • Scintillation

Fields of Study

  • Environmental science

Readers

  • Aviation Science / Aeronautics.
  • Radio communications and signal processing.
  • Space/Atmospheric Physics.

Technology Areas

  • Space