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Interaction of the Planets through the Solar Wind

Published online by Cambridge University Press:  25 April 2016

E. G. Bowen
E. G. Bowen*
Affiliation:
Division of Radiophysics, CSIRO, Sydney
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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
Information
Publications of the Astronomical Society of Australia , Volume 1 , Issue 1 , January 1967 , pp. 5 - 6
Copyright
Copyright © Astronomical Society of Australia 1967

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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