Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
8141990 | Planetary and Space Science | 2018 | 8 Pages |
Abstract
In the given work, the data of meteor radar observation from August to November of 1986 are resulted. The conditions of observation have defined some types of orbits: internal orbits with aphelion distance Qâ¼1 AU and with a wide spectrum of perihelion distances and external orbits with perihelion distance qâ¼1 AU and with a wide spectrum of aphelion distances. The majority of all observed orbits are close to circular orbits for which Qâ¼1 AU and qâ¼1 AU. Three-dimensional maps of meteor microstream distribution and numbers of meteors in them by perihelion, by aphelion distances and by inclinations are constructed. Orbital parameters of the most significant meteor streams that have been found out are presented.
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Geophysics
Authors
S. Kalabanov, O. Sherstyukov, A. Karpov, R. Ishmuratov,