Luminosity of Meteoric Trains

Details Luminosity of Meteoric Trains Luminosity of Meteoric Trains

Nov 1936

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1936natur.138..933k&link_type=abstract

Nature, Volume 138, Issue 3500, pp. 933-934 (1936).

Physics

Scientific paper

IT is well known that the portion constituting nearly, but not quite,
the end part of a meteoric train is generally brighter and more
persistently visible than the rest of it. Charles P. Olivier also refers
to it in his book on meteors. The phenomenon may be explained as due to:

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