Structure of the quadrantid stream from radar observations

Details Structure of the quadrantid stream from radar observations Structure of the quadrantid stream from radar observations

Mar 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984baicz..35..123b&link_type=abstract

Astronomical Institutes of Czechoslovakia, Bulletin (ISSN 0004-6248), vol. 35, March 1984, p. 123-126.

Astronomy and Astrophysics

Astronomy

3

Quadrantid Meteoroids, Radar Astronomy, Radar Tracking, Spatial Distribution, Flux Density, Particle Size Distribution, Periodic Variations

Scientific paper

Variations of the flux density and the mass exponent S for the Quadrantid meteor stream are obtained from radar observations made at the Engelhardt Observatory over a period of eight years. A method of avoiding the uncertainty of an aerial diagram is proposed. The stability of the shower from year to year is established. The standard deviation of random variations of the maximum flux density does not exceed ten per cent.

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