THE NUMBER DENSITY OF METEOR TRAILS OBSERVABLE BY THE FORWARD-SCATTERING OF RADIO WAVES

1 October 1956

journal article
Published by Canadian Science Publishing in Canadian Journal of Physics

Vol. 34 (10) , 997-1004
https://doi.org/10.1139/p56-110

Abstract

The number of meteor trails which can be detected by the forward-scattering of radio waves varies with the region of the sky under observation. The number density is determined theoretically, as a function of position relative to the transmitter and receiver.

Keywords

NUMBER DENSITY
FUNCTION
SKY
THEORETICALLY
METEOR TRAILS OBSERVABLE
DENSITY OF METEOR

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