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A New Determination of Muon Directional Coupling Coefficients

Published online by Cambridge University Press:  25 April 2016

D. J. Cooke  and
A. G. Fenton
D. J. Cooke
Affiliation:
Department of Physics, University of Tasmania
A. G. Fenton
Affiliation:
Department of Physics, University of Tasmania
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Extract

Primary cosmic rays passing through the solar system carry with them valuable information about solar and astrophysical phenomena in the form of intensity and spectral variations. In order that this information be efficiently extracted from observations of the directional cosmic-ray flux at the surface of the Earth, it is essential to have accurate information available to enable the relating of the observed secondary cosmic-ray directions of motion and intensity to those outside the range of the disturbing terrestrial influences.

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 1 , Issue 4 , December 1968 , pp. 154 - 157
Copyright
Copyright © Astronomical Society of Australia 1968

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References

1 Dorman, L. I., Cosmic Ray Variations, State Publishing House for Technical and Theoretical Physics, Moscow 1957.Google Scholar
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