Physics
Scientific paper
Aug 1987
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987maph...25..222o&link_type=abstract
In International Council of Scientific Unions, Middle Atmosphere Program. Handbook for MAP, Volume 25 p 222-227 (SEE N88-14502 0
Physics
Air, Meteor Trails, Meteoroid Showers, Particle Collisions, Radiation Spectra, Afterglows, Line Spectra, Luminosity, Radiative Lifetime
Scientific paper
Meteor radiation appears as a result of collisions between meteoroid atoms and air molecules. Depending on duration, this radiation is usually divided into the following types: radiation of the meteor head; radiation of a coma surrounding or immediately following the meteor head; radiation of a trail formed as a result of fragments lagging behind or by the afterglow; and radiation of a meteor train forming from a tail as a result of various chemical and dynamical processes. To investigate physical processes caused by each of the above types, it is necessary to obtain the corresponding experimental data. The physical processes of the radiation and the measurement of the experimental data is discussed.
Maltsev N. V.
Mukhamednazarov S.
Ovezgeldyev O. G.
Shafiev R. I.
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