The separation of particles during meteor flares

Details The separation of particles during meteor flares The separation of particles during meteor flares

Dec 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989avest..23..339g&link_type=abstract

Astronomicheskii Vestnik (ISSN 0320-930X), vol. 23, Oct.-Dec. 1989, p. 339-343. In Russian.

Astronomy and Astrophysics

Astronomy

1

Fragmentation, Meteoroids, Astronomical Models, Light Curve, Micrometeoroids

Scientific paper

Levin's (1956) model of meteor fragmentation is used to estimate the number of terminal meteor flares leading up to the complete destruction of a meteor body. Using four meteors as examples, it is shown that during the terminal stage, a meteor fragments into particles with average masses between 0.00001 and 0.001 g and average radii of about 0.01 cm.

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