The coagulation process in meteor trails

Details The coagulation process in meteor trails The coagulation process in meteor trails

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988avest..22..340b&link_type=abstract

Astronomicheskii Vestnik (ISSN 0320-930X), vol. 22, Oct.-Dec. 1988, p. 340-344. In Russian.

Astronomy and Astrophysics

Astronomy

Coagulation, Meteor Trails, Particle Collisions, Aerosols, Atmospheric Entry, Brownian Movements, Secondary Emission

Scientific paper

The structure of meteors and the processes behind the collision of particles formed after the interaction of meteoritic matter with the earth's atmosphere are described. An equation describing coagulation in meteor trails is obtained. It is shown that primary and secondary particles of meteoritic origin exist in the meteor zone which are sources of semidisperse aerosol.

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