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A New Installation for Studying the Sidereal Anisotropy of Cosmic Rays

Published online by Cambridge University Press:  25 April 2016

A. G. Fenton ,
K. B Fenton ,
J. E. Humble ,
R. M. Jacklyn ,
A. Vrana ,
K. Murakami ,
Z. Fijii ,
T. Yamada ,
S. Sakakibara  and
K. Fujimoto
...Show all authors
A. G. Fenton
Affiliation:
Physics Department, University of Tasmania
K. B Fenton
Affiliation:
Physics Department, University of Tasmania
J. E. Humble
Affiliation:
Physics Department, University of Tasmania
R. M. Jacklyn
Affiliation:
Antarctic Division, Hobart
A. Vrana
Affiliation:
Antarctic Division, Hobart
K. Murakami
Affiliation:
Nagoya University, Japan
Z. Fijii
Affiliation:
Nagoya University, Japan
T. Yamada
Affiliation:
Nagoya University, Japan
S. Sakakibara
Affiliation:
Nagoya University, Japan
K. Fujimoto
Affiliation:
Nagoya University, Japan
H. Ueno
Affiliation:
Nagoya University, Japan
N. Nagashima
Affiliation:
Nagoya University, Japan
I. Kondo
Affiliation:
University of Tokyo, Japan
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Extract

It is now firmly established that a small anisotropy of the galactic cosmic rays exists, observable from Earth as a variation of intensity in sidereal time. The problem now is to determine more clearly the characteristics of the anisotropy and, in particular, its detailed spatial structure and how it depends upon the energy and composition of the cosmic rays. This is a very difficult task and, in the final analysis, may not be fully achievable from Earth-based observations. The purpose of the present paper is to describe briefly an installation now operating in Tasmania to provide further information on the spatial structure of the anisotropy.

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Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 4 , Issue 4 , 1982 , pp. 456 - 458
Copyright
Copyright © Astronomical Society of Australia 1982

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References

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