As a rule, when analyzing the mechanism of quasi continuous fragmentation (QCF) it is assumed that fragments separated from the parent meteoroid (PM) are of equal initial mass. In reality, this may not be so. A major difficulty is the lack of observational data on the function of the fragment initial mass distribution and so one must resort to theoretical modeling. A discrete distribution is considered which excluded to a certain extent some mathematical difficulties. The calculation results are given and discussed
This paper is concerned with a meteoroid shape estimation technique based on statistical laws of dis...
Atmospheric entry of meteoroids poses danger to humans in the form of blast-wave overpressure, impac...
The dynamic fragmentation of meteoroids during their flight in the atmosphere is described. The exam...
Photographic observations of meteors carried out in Dushanbe by the method of instantaneous exposure...
Different fragmentation models are applied to a number of events, including the entry of TC3 2008 as...
Detailed analysis of the fragmentation of the Morávka meteoroid during the atmospheric entry is pres...
Meteors with peak magnitudes fainter than +2 are typically called faint meteors, resulting from the ...
To model the interaction with the atmosphere of fragments of a disrupted asteroid, which move indepe...
Context. Meteoroids are pieces of asteroids and comets. They serve as unique probes to the physical ...
Faint meteors observed with Super-Schmidt cameras are re-examined in order to assess whether their d...
The calculation results of Sikhote-Alinian meteorite interaction with the Earth atmosphere are prese...
Everyday thousands of meteoroids enter the Earth's atmosphere. The vast majority burn up harmlessly ...
Abstract–In this study, we conduct a detailed analysis of the Košice meteorite fall (February28, 201...
There has been much interest in the meteor physics community recently regarding the form that meteor...
The explicit solution of the drag and ablation equations of a single nonfragmenting meteoroid moving...
This paper is concerned with a meteoroid shape estimation technique based on statistical laws of dis...
Atmospheric entry of meteoroids poses danger to humans in the form of blast-wave overpressure, impac...
The dynamic fragmentation of meteoroids during their flight in the atmosphere is described. The exam...
Photographic observations of meteors carried out in Dushanbe by the method of instantaneous exposure...
Different fragmentation models are applied to a number of events, including the entry of TC3 2008 as...
Detailed analysis of the fragmentation of the Morávka meteoroid during the atmospheric entry is pres...
Meteors with peak magnitudes fainter than +2 are typically called faint meteors, resulting from the ...
To model the interaction with the atmosphere of fragments of a disrupted asteroid, which move indepe...
Context. Meteoroids are pieces of asteroids and comets. They serve as unique probes to the physical ...
Faint meteors observed with Super-Schmidt cameras are re-examined in order to assess whether their d...
The calculation results of Sikhote-Alinian meteorite interaction with the Earth atmosphere are prese...
Everyday thousands of meteoroids enter the Earth's atmosphere. The vast majority burn up harmlessly ...
Abstract–In this study, we conduct a detailed analysis of the Košice meteorite fall (February28, 201...
There has been much interest in the meteor physics community recently regarding the form that meteor...
The explicit solution of the drag and ablation equations of a single nonfragmenting meteoroid moving...
This paper is concerned with a meteoroid shape estimation technique based on statistical laws of dis...
Atmospheric entry of meteoroids poses danger to humans in the form of blast-wave overpressure, impac...
The dynamic fragmentation of meteoroids during their flight in the atmosphere is described. The exam...