Investigation of the disintegration of three-dimensional meteoric bodies in the upper atmospheric layers

Details Investigation of the disintegration of three-dimensional meteoric bodies in the upper atmospheric layers Investigation of the disintegration of three-dimensional meteoric bodies in the upper atmospheric layers

Nov 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979kosis..17..866a&link_type=abstract

Kosmicheskie Issledovaniia, vol. 17, Nov.-Dec. 1979, p. 866-874. In Russian.

Astronomy and Astrophysics

Astronomy

1

Atmospheric Effects, Atmospheric Entry, Mathematical Models, Meteoroids, Particle Motion, Upper Atmosphere, Aerodynamic Characteristics, Astrodynamics, Atmospheric Heating, Conductive Heat Transfer, Equations Of Motion, Kinematic Equations, Molecular Flow

Scientific paper

The mathematical model proposed in the present paper for the motion of a meteoric body of arbitrary configuration in the upper atmosphere makes allowance for internal heating, evaporation, and ablation. Numerical calculations are carried out for initially ellipsoidal bodies with different semiaxes ratios, different initial velocities, and different atmospheric entry angles. The ablation, temperature, luminescence, and the electron concentration in the meteor train are determined.

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