DOI: https://doi.org/10.18524/1810-4215.2015.28.70333

ABOUT THE NATURE OF METEOR FLARES

V. A. Smirnov

Анотація


Whereas at development of the meteoric phenomenon there are processes in different temporary scales (more slow processes heat conductivity, mechanical rotation, destruction) and considerably faster (fluctuations of brightness of radiating plasma is like gas-dynamical laser), the observable flares of meteors differ in nature, and in appearance caused by character of radiation. Continuing development of the meteoric phenomena in the Earth's atmosphere has been described by Astapovich I.S. (Astapovich I.S. 1958). The classification of meteor flashes which depends on the physical nature of the phenomenon is given below and the formulas of a physical theory representing these processes while moving the meteor are presented here.

Ключові слова


Flares; Meteor stream; Gas-dynamical laser; Ambipolar diffusion; Kinetics of meteor plasma

Повний текст:

PDF (English)

Посилання


Abe S., Ebizuka N., Yano H., Watanabe J., Borovicka J.: 2007, Adv. Space Res., 39, 4, 538-543.

Astapovich I.S. Meteor Phenomena in the Land Atmosphere. Fizmatgiz, Moscow, 1958.

Biberman L.M., Vorobjov V.S., Jakubov I.T. The Kinetics of Non-equilibrium Low-temperature plasma. Science. Moscow, 1982.

Chudnovsky A.F. Heat-physics of Soils. Science, Moscow, 1976.

Smirnov V.A.: 2007, Adv. Space Res., 39, 4, 526-532.

Smirnov V.A. The Speсtra of Transient Atmospheric Luminous Phenomena: Meteors. Physico-Mathematical Literature, Moscow, 1994.

Smirnov V.A.: 2000, Proc. of IMC Frasso Sabino, International Meteor Organization, 59-71.

Smirnov V.A.: 2003, in: Proc. of IMC Frombork /eds. Olech A., Zloczewski K., Mularczyk K., Poland 26 - 29 September 2002. International Meteor Organization, 119-124.




Copyright (c) 2015 Odessa Astronomical Publications

Creative Commons License
Ця робота ліцензована Creative Commons Attribution-NonCommercial 4.0 International License.