Physics
Scientific paper
Feb 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005pimo.conf...71s&link_type=abstract
Proceedings of the International Meteor Conference, Varna, Bulgaria, 23-26 September, 2004, Eds.: Triglav-Čekada, M., Kac, J.; M
Physics
Scientific paper
In this article the characteristics of meteor radiation are investigated. The character of the radiating spectrum depends first of all on the speed of the meteor, and also on the chemical and mechanical structure of the meteoroid. The spectrum of the meteor changes along its atmospheric path according to the Wien's law. For fast meteors the final flares occur due to the particular conditions of the power interaction between the meteoric plasma and particles of the atmosphere. Such features confirm that the meteor plasma can radiate at a speed in excess of 60~km/s in flares, by the mechanism of cascade radiation, which is similar to the radiation of gas-dynamic lasers.
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