The populations and orbits of double-station TV meteors

Details The populations and orbits of double-station TV meteors The populations and orbits of double-station TV meteors

Mar 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984baicz..35...46h&link_type=abstract

Astronomical Institutes of Czechoslovakia, Bulletin (ISSN 0004-6248), vol. 35, no. 1, 1984, p. 46-64.

Astronomy and Astrophysics

Astronomy

22

Meteoroids, Orbits, Television Cameras, Trajectory Analysis, Faint Object Camera, Image Analysis, Radio Meteors, Tables (Data), Video Data

Scientific paper

The atmospheric trajectories, velocities, brightnesses and orbits of double-station TV-meteors, 3 magnitudes fainter than those photographed by Super-Schmidt cameras are given. The beginning heights of A and C meteors found in photographic observations are compared with the TV-meteor data. The strongest component of the TV-meteors forms a natural continuation of the C1 group of the Super-Schmidt meteors. A new well populated C3 group with randomly-inclined short period orbits is revealed and its presence among the brighter meteors is investigated. A mass-selective evolution of C2-type orbits into C3-type orbits is consistent with the observations. A brief discussion of showers and associated orbits is given. Theoretical beginning heights are briefly mentioned.

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