Hostname: page-component-cd9895bd7-dk4vv Total loading time: 0 Render date: 2024-12-27T07:06:11.279Z Has data issue: false hasContentIssue false

Interaction of the Planets through the Solar Wind

Published online by Cambridge University Press:  25 April 2016

E. G. Bowen*
Affiliation:
Division of Radiophysics, CSIRO, Sydney

Extract

It is usual to describe the motion of the planets around the sun in terms only of the gravitational forces between them. The purpose of this note is to point out that another form of interaction between bodies in the solar system is possible through the medium of the solar wind.

Type
Invited Papers
Copyright
Copyright © Astronomical Society of Australia 1967

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

1 Bigg, E. K., J. Geophys. Res. 68, 4099 (1963).Google Scholar
2 Sucksdorff, E., Geophysica (Helsinki) 5 (2), 95 (1956).Google Scholar
3 Houtgast, J., and van Sluiters, A., Nature 196, 462 (1962).Google Scholar
4 Stolov, H. L., and Cameron, A. G. W., J. Geophys. Res. 69, 4975 (1964).Google Scholar
5 Bell, B., and Defouw, R. J., J. Geophys. Res. 69, 3169 (1964).Google Scholar
6 Slipher, E. C., ‘Mars’ (Sky Publishing Corporation, Cambridge, Massachusetts, 1962).Google Scholar
7 Bigg, E. K., Nature 203, 1008 (1964).Google Scholar
8 Ness., N. P., Scearce, C. S., and Seek, J. B., J. Geophys. Res. 69, 3531 (1964).CrossRefGoogle Scholar