Simulating the Propagation of Infrasonic Waves and Estimating the Energy of the Chelyabinsk Meteoroid Explosion Observed on February 15, 2013
- Authors: Kulichkov S.N.1, Popov O.Y.1, Avilov K.V.1, Chunchuzov I.P.1, Chkhetiani O.G.1, Smirnov A.A.2, Dubrovin V.I.2, Mishenin A.A.1
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Affiliations:
- Obukhov Institute of Atmospheric Physics
- Institute of Geophysical Research
- Issue: Vol 54, No 3 (2018)
- Pages: 293-303
- Section: Article
- URL: https://journals.rcsi.science/0001-4338/article/view/148557
- DOI: https://doi.org/10.1134/S0001433818030106
- ID: 148557
Cite item
Abstract
Results obtained from simulating the propagation of infrasonic waves from the Chelyabinsk meteoroid explosion observed on February 15, 2013, are given. The pseudodifferential parabolic equation (PDPE) method has been used for calculations. Data on infrasonic waves recorded at the IS31 station (Aktyubinsk, Kazakhstan), located 542.7 km from the likely location of the explosion, have been analyzed. Six infrasonic arrivals (isolated clearly defined pulse signals) were recorded. It is shown that the first “fast” arrival (F) corresponds to the propagation of infrasound in a surface acoustic waveguide. The rest of the arrivals (T1–T5) are thermospheric. The agreement between the results of calculations based on the PDPE method and experimental data is satisfactory. The energy E of the explosion has been estimated using two methods. One of these methods is based on the law of conservation of the acoustic pulse I, which is a product of the wave profile area S/2 of the signal under analysis and the distance to its source EI [kt] = 1.38 × 10–10 (I [kg/s])1.482. The other method is based on the relation between the energy of explosion and the dominant period T of recorded signal ET [kt] = 1.02 × (T [s]2/σ)3/2, where σ is the dimensionless distance determining the degree of nonlinear effects during the propagation of sound along ray trajectories. According to the data, the explosion energy EI,T ranges from 1.87 to 32 kt TNT.
About the authors
S. N. Kulichkov
Obukhov Institute of Atmospheric Physics
Author for correspondence.
Email: snik1953@gmail.com
Russian Federation, Moscow, 119017
O. Ye. Popov
Obukhov Institute of Atmospheric Physics
Email: snik1953@gmail.com
Russian Federation, Moscow, 119017
K. V. Avilov
Obukhov Institute of Atmospheric Physics
Email: snik1953@gmail.com
Russian Federation, Moscow, 119017
I. P. Chunchuzov
Obukhov Institute of Atmospheric Physics
Email: snik1953@gmail.com
Russian Federation, Moscow, 119017
O. G. Chkhetiani
Obukhov Institute of Atmospheric Physics
Email: snik1953@gmail.com
Russian Federation, Moscow, 119017
A. A. Smirnov
Institute of Geophysical Research
Email: snik1953@gmail.com
Kazakhstan, Kurchatov, 071100
V. I. Dubrovin
Institute of Geophysical Research
Email: snik1953@gmail.com
Kazakhstan, Kurchatov, 071100
A. A. Mishenin
Obukhov Institute of Atmospheric Physics
Email: snik1953@gmail.com
Russian Federation, Moscow, 119017