LF radiowave propagation effects of meteoric ionization

Details LF radiowave propagation effects of meteoric ionization LF radiowave propagation effects of meteoric ionization

Apr 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979p%26ss...27..533b&link_type=abstract

Planetary and Space Science, vol. 27, Apr. 1979, p. 533-535.

Computer Science

Atmospheric Ionization, Low Frequencies, Meteor Trails, Radio Transmission, Radio Meteors, Radio Navigation, Signal Fading

Scientific paper

LF signal fading noted during one year's observations of 280-kHz signals received both day and night over paths of 110 and 1000 km from navigational beacon transmitters has been ascribed by Sen and Saha (1977) to absorption due to meteoric ionization deposited below the signal reflection height. However, it is shown that the model of a meteoric plasma column used by Sen and Saha to explain the LF radiowave fading is not compatible with the observed properties of meteor trains.

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