Hostname: page-component-8448b6f56d-qsmjn Total loading time: 0 Render date: 2024-04-25T04:33:30.487Z Has data issue: false hasContentIssue false

4.4 The Heliocentric Distribution of the Meteor Bodies at the Vicinity of the Earth’S Orbit

Published online by Cambridge University Press:  12 April 2016

V.V. Andreev
Affiliation:
Engelhardt Astronomical Observatory, Kazan/U.S.S.R.
O.I. Belkovich
Affiliation:
Engelhardt Astronomical Observatory, Kazan/U.S.S.R.
V.S. Tokhtas’ev
Affiliation:
Engelhardt Astronomical Observatory, Kazan/U.S.S.R.

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

A determination of velocity distributions of sporadic meteor bodies and distributions of their radiants over the celestial sphere corrected for the motion and attraction of the earth is one of the main problem of the meteor astronomy. An analytical model of these distributions has certain interest.

Type
4 Meteors and their Relation to Interplanetary Dust
Copyright
Copyright © Springer-Verlag 1976