Hostname: page-component-586b7cd67f-tf8b9 Total loading time: 0 Render date: 2024-11-28T23:05:44.174Z Has data issue: false hasContentIssue false
  • English
  • Français

A Medium Rigidity Muon Experiment for the South Pole Station

Published online by Cambridge University Press:  25 April 2016

M. L. Duldig ,
R. M. Jacklyn  and
M. A. Pomerantz
M. L. Duldig
Affiliation:
Antarctic Division, Department of Science
R. M. Jacklyn
Affiliation:
Antarctic Division, Department of Science
M. A. Pomerantz
Affiliation:
Bartol Research Foundation, University of Delaware
Get access Rights & Permissions [Opens in a new window]

Abstract

A proposal for a medium rigidity muon telescope system to be installed at the U.S. South Pole Station for observations of time variations of cosmic ray intensity is at present being prepared by Professor Pomerantz, Director of the Bartol Research Foundation, University of Delaware and Drs Jacklyn and Duldig of the Cosmic Ray Section, Antarctic Division, Department of Science. A novel approach to medium energy cosmic ray observations viewing in equatorial to mid-latitude directions is described. The absorber depth required for the proposed 50-1000 GV rigidity range would be achieved by locating the telescope system at a depth of approximately 7 metres water equivalent (MWE) in the ice and viewing at high zenith angles. Optimization techniques used in the telescope design are presented together with the unique advantages of the location. Justification for the experiment and comparison with important observatories in this rigidity range are also discussed.

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 6 , Issue 1 , 1985 , pp. 48 - 52
Copyright
Copyright © Astronomical Society of Australia 1985

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

Cooke, D. J., 1975, Proc. 14th Int. Cosmic Ray Conf, Munich, 4, 1492.Google Scholar
Jacklyn, R. M., and Duldig, M. L., 1983, Proc. Astron. Soc. Aust. 5, 262.CrossRefGoogle Scholar
Jacklyn, R. M. and Pomerantz, M. A., 1983, Proc. 18th Int. Cosmic Ray Conf., Bangalore, 3, 206.Google Scholar
Jacklyn, R. M., Duldig, M. L., and Pomerantz, M. A., 1984a, Proc. Astron. Soc. Aust., 5, 581.CrossRefGoogle Scholar
Jacklyn, R. M., Duldig, M. L., and Pomerantz, M. A., 1984b, Proc. Int. Symp. on Cosmic Ray Modulation in the Heliosphere, Morioka, p 76.Google Scholar
Nagashima, K., Sakakibara, S., Fenton, A. G., and Humble, J. E., 1984, Planet. Space Sci. (in press).Google Scholar
Pomerantz, M. A., Duggal, S. P., Owens, A. J., Tolba, M. F., and Tsao, C. H., 1982, J. Geophys. Res., 87, 10325.CrossRefGoogle Scholar
Swinson, D. B., 1983, Proc. 18th Int. Cosmic Ray Conf., Bangalore, 10, 55.Google Scholar
Winkler, J. R., and Stroud, W. G., 1949, Phys. Rev. 76, 1012 CrossRefGoogle Scholar