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Publications of the Astronomical Society of Australia Publications of the Astronomical Society of Australia

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Enhanced Cosmic Ray Diurnal Variations in Mawson and Hobart Neutron Monitor and Underground Data Records

Published online by Cambridge University Press:  25 April 2016

M. L. Duldig  and
J. E. Humble
M. L. Duldig
Affiliation:
Australian Antarctic Division, c/o Physics Department, University of Tasmania
J. E. Humble
Affiliation:
Physics Department, University of Tasmania, PO Box 252C, Hobart, Tas 7001
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Abstract

Analysis of surface and underground detector data from Mawson and Hobart for the period 1982 to 1988 has revealed a number of episodes of enhanced diurnal variation lasting more than 5 days. A preliminary study of these enhancements shows that variations in the rigidity spectrum and in the upper limiting rigidity must be present to explain the phenomenon.

Type
High Energy Astrophysics
Information
Publications of the Astronomical Society of Australia , Volume 8 , Issue 3 , 1990 , pp. 268 - 273
Copyright
Copyright © Astronomical Society of Australia 1990

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References

Alania, M. V., Aslamazashvili, R. G. and Djapiashvili, T. V., 1981, Proc. 17th Int. Cosmic Ray Conf., Paris, 4, 64.Google Scholar
Baker, C. P., Duldig, M. L. and Humble, J. E., 1989, Proc. Astron. Soc. Aust., 8, 55.CrossRefGoogle Scholar
Forbush, S. E., 1969, J. Geophys. Res., 74, 3451.CrossRefGoogle Scholar
Fujimoto, K., Inoue, A., Murakami, K. and Nagashima, K., 1984, Rep. No. 9, Cosmic Ray Res. Lab., Nagoya, Japan.Google Scholar
Humble, J. E., Duldig, M. L., Fenton, K. B. and Fenton, A. G., A.N.A.R.E. Research Note (in press).Google Scholar
Iucci, N., Parisi, M., Storini, M. and Villoresi, G., 1981, Proc. 17th Int. Cosmic Ray Conf., Paris, 10, 238.Google Scholar
Iucci, N., Parrisi, M., Storini, M. and Villoresi, G., 1983, Proc. 18th Int. Cosmic Ray Conf., Bangalore, 3, 354.Google Scholar
Jacklyn, R. M. and Humble, J. E., 1965, Aust. J. Phys., 18, 451.CrossRefGoogle Scholar
Jacklyn, R. M. and Humble, J. E., 1981, Proc. 17th Int. Cosmic Ray Conf., Paris, 4, 134.Google Scholar
Kota, J., 1985, Proc. 19th Int. Cosmic Ray Conf., La Jolla, 9, 275.Google Scholar
Levy, E. H., 1976, J. Geophys. Res., 81, 2082.CrossRefGoogle Scholar
Mishra, B. L. and Agrawal, S. P., 1987, Proc. 20th Int. Cosmic Ray Conf., Moscow, 4, 172.Google Scholar
Mori, S., Yasue, S., Ichinose, M. and Manakata, Y., 1975, Proc. 14th Int. Cosmic Ray Conf., Munich, 4, 1463.Google Scholar
Murayama, T., 1981, Proc. 17th Int. Cosmic Ray Conf., Paris, 4, 155.Google Scholar
Riker, J.F. and Ahluwalia, H. S., 1987, Planet. Space Sci., 35, 1111.CrossRefGoogle Scholar
Somogyi, A. J., 1981, Proc. 17th Int. Cosmic Ray Conf., Paris, 13, 227.Google Scholar
Swinson, D.B., 1981, Proc. 17th Int. Cosmic Ray Conf., Paris, 4, 138.Google Scholar
Yasue, S., Mori, S., Sakakibara, S. and Nagashima, K., 1982, Rep. No. 7, Cosmic Ray Res. Lab., Nagoya, Japan.Google Scholar

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