Distribution of Lyrid meteoroids in a large range of echo durations

Details Distribution of Lyrid meteoroids in a large range of echo durations Distribution of Lyrid meteoroids in a large range of echo durations

May 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988baicz..39..165p&link_type=abstract

Astronomical Institutes of Czechoslovakia, Bulletin (ISSN 0004-6248), vol. 39, May 1988, p. 165-168.

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Mass Distribution, Meteoroid Showers, Radar Echoes, Comets, Radar Data

Scientific paper

Radar observations of the Lyrid meteor stream made at the Ondřejov Observatory in 1980 - 1985, are analyzed and discussed from the viewpoint of determining the mass distribution exponent for overdense echoes in the range of 0.4 - 50 s. The mass exponent proved to be almost constant over the whole range of echo durations with s ≡ 1.58. The contribution of larger particles, as compared with other meteor streams, was found to be more significant for the Lyrids. The almost constant value of s indicates a still active contribution of fresh cometary material to the stream.

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