Astronomy and Astrophysics – Astronomy
Scientific paper
Aug 1987
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987maph...25..272b&link_type=abstract
In International Council of Scientific Unions, Middle Atmosphere Program. Handbook for MAP, Volume 25 p 272-279 (SEE N88-14502 0
Astronomy and Astrophysics
Astronomy
Astronomical Photometry, Meteoritic Composition, Meteoroid Showers, Particle Flux Density, Diurnal Variations, Mass Distribution, Mathematical Models, Meteor Trails, Particle Density (Concentration)
Scientific paper
Studies of meteor showers permit the solving of some principal problems of meteor astronomy: to obtain the structure of a stream in cross section and along its orbits; to retrace the evolution of particle orbits of the stream taking into account gravitational and nongravitational forces and to discover the orbital elements of its parent body; to find out the total mass of solid particles ejected from the parent body taking into account physical and chemical evolution of meteor bodies; and to use meteor streams as natural probes for investigation of the average characteristics of the meteor complex in the solar system. A simple and effective method of determining the flux density and mass exponent parameter was worked out. This method and its results are discussed.
Belkovich Oleg I.
Suleimanov N. I.
Tokhtasjev V. S.
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