Physics
Scientist
Kazanskii Gosudarstvennyi Universitet, Kazan, USSR
A steady-state model for the planetary distribution of aerosol particles in the upper atmosphere
Allowing for the Effect of the Antenna Radiation Pattern along the Azimuth and for the Uneven Distribution of the Radiants of Meteors when Determining the Average Wind Velocity
Seasonal variations in the semi-diurnal tide in the upper atmosphere as determined from radio meteor observations
Seasonal variations of solar and lunar tides in the meteor zone
Vertical Characteristics of Wind Velocity Spectra in the Meteor Region of the Atmosphere
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