Radio-meteor heights and fragmentation of small meteoric bodies in the atmosphere

Details Radio-meteor heights and fragmentation of small meteoric bodies in the atmosphere Radio-meteor heights and fragmentation of small meteoric bodies in the atmosphere

Dec 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989avest..23..282k&link_type=abstract

Astronomicheskii Vestnik (ISSN 0320-930X), vol. 23, Oct.-Dec. 1989, p. 282-288. In Russian.

Other

Atmospheric Effects, Fragmentation, Radio Meteors, Altimetry, Chondrites, Mathematical Models, Radio Echoes, Stony Meteorites

Scientific paper

The bimodal distribution of the measured heights of slow radio meteors is analyzed, focusing on the composition, discrete distribution, and characteristics of the fine meteor particle complex. It is found that about half of the slow radio meteors give rise to nonfragmenting dense stony meteor bodies, while the other half fragments in the atmosphere, producing more friable bodies similar to C I carbonaceous chondrites.

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