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16. Some aspects of the creation of meteor trains and radio-wave scattering from them

Published online by Cambridge University Press:  14 August 2015

K. V. Kostylev
K. V. Kostylev*
Affiliation:
Radio Astronomy Department, Kazan University, U.S.S.R.

Extract

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Small meteor particles are considered, which produce meteors with magnitudes between +3m and +10m to +12m, and for which the thermal conductivity may be assumed infinite. Fragmentation and air cap effects are neglected. The derivation is made taking into account radiation losses and temperature variation during the evaporation time. The temperature variation of the meteoroid is defined in this case by the equation:

Type
Session 3
Information
Symposium - International Astronomical Union , Volume 33: Physics and Dynamics of Meteors , 1968 , pp. 169 - 174
Copyright
Copyright © Reidel 1968 

References

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