The reflection of radio waves from irregularly ionized meteor trains

Details The reflection of radio waves from irregularly ionized meteor trains The reflection of radio waves from irregularly ionized meteor trains

Aug 1969

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1969p%26ss...17.1519j&link_type=abstract

Planetary and Space Science, Volume 17, Issue 8, p. 1519-1526.

Physics

Scientific paper

A theory of the reflection process of radio waves from irregularly ionized meteor trains has been developed which predicts a scatterin the decay time of underdense radio meteors. The magnitude of this scatter is close to that deduced previously by a numerical method, and is shown to be wavelength dependent. Application of the theory to available data indicates that irregularities in the electron line density with scale lengths between 300 and 500 m are less than 20 per cent of the mean electron line density while those with scale lengths between 500 m and 6 km are less than 43 per cent of the mean.

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