Structural peculiarities of the Quadrantid meteor shower

Details Structural peculiarities of the Quadrantid meteor shower Structural peculiarities of the Quadrantid meteor shower

Aug 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987maph...25..351i&link_type=abstract

In International Council of Scientific Unions, Middle Atmosphere Program. Handbook for MAP, Volume 25 p 351-355 (SEE N88-14502 0

Physics

Annual Variations, Meteoroid Showers, Particle Flux Density, Quadrantid Meteoroids, Radar Tracking, Radiometric Resolution, Solar Longitude, Spatial Distribution

Scientific paper

Systematic radio observations to investigate the Quadrantid meteor shower structure are regularly carried out. They have now been conducted annually in the period of its maximum activity, January 1 to 6, since 1966. The latest results of these investigations are presented, on the basis of 1981 to 1984 data obtained using new equipment with a limiting sensitivity of +7.7m which make it possible to draw some conclusions on the Quadrantids shower structure both for transverse and lengthwise directions.

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