Modeling of motion of a disrupted meteoric body motion in the atmosphere (Q1584164)
From MaRDI portal
| This is the item page for this Wikibase entity, intended for internal use and editing purposes. Please use this page instead for the normal view: Modeling of motion of a disrupted meteoric body motion in the atmosphere |
scientific article; zbMATH DE number 1524065
| Language | Label | Description | Also known as |
|---|---|---|---|
| English | Modeling of motion of a disrupted meteoric body motion in the atmosphere |
scientific article; zbMATH DE number 1524065 |
Statements
Modeling of motion of a disrupted meteoric body motion in the atmosphere (English)
0 references
31 October 2000
0 references
The authors present the results of comparison of the trajectories of the disrupting meteoric bodies in the atmosphere for two models of disruption. It is established that the motion of the parts of the meteoric bodies depends on the adopted model of disruption. The obtained results may be applied in the solution of the inverse problem of meteoric physics, namely, the determination of the meteoric bodies parameters using the observation data.
0 references
disruption of the meteoric bodies
0 references
disruption models
0 references
0.9160911
0 references
0.8801118
0 references
0.8512467
0 references
0.8391528
0 references
0.83259195
0 references
0.83100545
0 references