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Arrival directions of cosmic rays of E .4 EeVThe anisotropy of cosmic rays observed by the Utah Fly's Eye detector has been studied. Emphasis has been placed on examining distributions of events in galactic coordinates. No statistically significant departure from isotropy has been observed for energies greater than 0.4 EeV (1 EeV = 10 to the 18th power eV). Results of the standard harmonic analysis in right ascension are also presented.
Document ID
19850025758
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Baltrusaitis, R. M. (Utah Univ. Salt Lake City, UT, United States)
Cady, R. (Utah Univ. Salt Lake City, UT, United States)
Cassiday, G. I. (Utah Univ. Salt Lake City, UT, United States)
Cooper, R. (Utah Univ. Salt Lake City, UT, United States)
Elbert, J. W. (Utah Univ. Salt Lake City, UT, United States)
Gerhardy, P. R. (Utah Univ. Salt Lake City, UT, United States)
Ko, S. (Utah Univ. Salt Lake City, UT, United States)
Loh, E. C. (Utah Univ. Salt Lake City, UT, United States)
Mizumoto, Y. (Utah Univ. Salt Lake City, UT, United States)
Salamon, M. H. (Utah Univ. Salt Lake City, UT, United States)
Date Acquired
August 12, 2013
Publication Date
August 1, 1985
Publication Information
Publication: 19th Intern. Cosmic Ray Conf - Vol. 2
Subject Category
Space Radiation
Report/Patent Number
OG-5.3-4
Accession Number
85N34071
Funding Number(s)
CONTRACT_GRANT: NSF PHY-82-01089
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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IDRelationTitle19850025693Collected WorksNinteenth International Cosmic Ray Conference. OG Sessions, Volume 2
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