Hostname: page-component-848d4c4894-2xdlg Total loading time: 0 Render date: 2024-07-08T01:30:52.047Z Has data issue: false hasContentIssue false
  • English
  • Français

Trajectories of Sublimating Interplanetary Dust Grains

Published online by Cambridge University Press:  14 August 2015

G. H. Schwehm
G. H. Schwehm*
Affiliation:
Ruhr-Universitat Bochum, F.R.G.

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 equation of motion for interplanetary dust particles close to the Sun has been solved numerically taking into consideration the interaction with the radiation field of the Sun and the temperature distribution as a function of grain size and heliocentric distance for different materials.

Type
III: The Interplanetary Dust Complex 1. Sources, Evolution, and Dynamics
Information
Symposium - International Astronomical Union , Volume 90: Solid Particles in the Solar System , 1980 , pp. 319 - 320
Copyright
Copyright © Reidel 1980 

References

MacQueen, R.M.: 1968, Astrophys. J. 154, pp. 1059–1076 CrossRefGoogle Scholar