Hostname: page-component-cd9895bd7-7cvxr Total loading time: 0 Render date: 2024-12-26T05:14:22.643Z Has data issue: false hasContentIssue false
  • English
  • Français

4.6 Interplanetary Dust in the Vicinity of the Earth

Published online by Cambridge University Press:  12 April 2016

G.M. Teptin
G.M. Teptin*
Affiliation:
Kazan State University/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.

The characteristics of the flux density of the interplanetary small particles in the vicinity of the Earth are considered. From the results of the analysis of the characteristics of the suspended dusty particles in the turbulent upper atmosphere the density of flux is obtained. The radar meteor measurements of the turbulent intensity in the upper atmosphere allow to evaluate the flux density of the interplanetary dust as a function of the magnitude of the particles at the intervals of the sizes from ~ 1µ. to ~ 0.05µ. The comparison with the results of different experiments shows a good agreement.

Type
4 Meteors and their Relation to Interplanetary Dust
Information
International Astronomical Union Colloquium , Volume 31: Interplanetary Dust and Zodiacal Light , 1976 , pp. 389
Copyright
Copyright © Springer-Verlag 1976