Abstract
MANY observers have reported Doppler-effect heterodynes in the background of received high-frequency broadcast signals. The accepted explanation of the whistles is that waves received after reflexion from ionized meteor trails have undergone a frequency-shift, relative to the waves received by a more direct path. Usually, the pitch of the heterodyne descends to zero. Chamanlal and Venkataraman1 suggested, in 1941, that the descending pitch was the result of the meteor being rapidly retarded in velocity. More recently, Sir Edward Appleton and Mr. R. Naismith2 proposed an alternative explanation of the change of pitch, which is ascribed to the reduction of the difference between the two path-lengths that occurs as the meteor, travelling tangentially to the observer, approaches the minimum distance.
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References
Chamanlal and Venkataraman, Nature, 149, 416 (1942); summary of article in Electrotechnics (Bangalore, Nov. 1941).
Appleton, Sir Edward, and Naismith, R., Proc. Phys. Soc, 59, 461 (1947).
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GRIFFITHS, H., MARTINGELL, S. & BAYLIFF, R. Meteor Whistles. Nature 161, 478–479 (1948). https://doi.org/10.1038/161478a0
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DOI: https://doi.org/10.1038/161478a0
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