DETERMINATION OF THE PARAMETERS OF SMALL METEORAL BODIES: COMPARISON OF POROUS AND SOLID BODY MODELS
https://doi.org/10.26006/29490995_2022_14_2_99
Abstract
The presented work proposes an ablation model describing the interaction of small meteoroids with the Earth's atmosphere, in which the meteoroid body is considered in two modifications: a solid and a porous body. An analysis is given of the obtained parameters for meteors with magnitudes from -2m to +2m obtained from optical observations.
About the Authors
V. V. Efremov
Sadovsky Institute of Geospheres Dynamics of Russian Academy of Sciences
Russian Federation
Russian Federation
O. P. Popova
Sadovsky Institute of Geospheres Dynamics of Russian Academy of Sciences
Russian Federation
Russian Federation
D. O. Glazachev
Sadovsky Institute of Geospheres Dynamics of Russian Academy of Sciences
Russian Federation
Russian Federation
A. P. Kartashova
Institute of Astronomy of Russian Academy of Sciences
Russian Federation
Russian Federation
Review
For citations:
Efremov V.V., Popova O.P., Glazachev D.O., Kartashova A.P. DETERMINATION OF THE PARAMETERS OF SMALL METEORAL BODIES: COMPARISON OF POROUS AND SOLID BODY MODELS. Dynamic Processes in Geospheres. 2022;14(2):99-105. (In Russ.) https://doi.org/10.26006/29490995_2022_14_2_99
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