On the influence of fragmentation on estimating bulk densities of meteoroids

Details On the influence of fragmentation on estimating bulk densities of meteoroids On the influence of fragmentation on estimating bulk densities of meteoroids

Dec 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990baicz..41..387n&link_type=abstract

Astronomical Institutes of Czechoslovakia, Bulletin (ISSN 0004-6248), vol. 41, Dec. 1990, p. 387-391.

Statistics

Computation

1

Astronomical Models, Computerized Simulation, Density Distribution, Meteoroids, Radio Meteors, Astronomical Photography, Atmospheric Ionization, Fragmentation

Scientific paper

The solution presently obtained for a model problem for meteoroid break-up, single-event crumbling, and gradual crumbling and husking, indicates that the neglect of meteoroid fragmentation characteristics can result in erroneous bulk-density estimates for bodies generating radar meteors. All parameters encompassed by the present computations were identical with those of Bibarsov and Cheboratev (1972). It is shown that the neglect of husking can lead to large bulk density errors.

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