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Cosmic ray north-south anisotropy: The role of the interplanetary magnetic field

Journal Article · · J. Geophys. Res.; (United States)
Nucleonic intensity data from the north and south polar stations Thule and McMurdo are analyzed to determine the nature of periodicities in the north-south asymmetry of relativistic galactic cosmic rays. The 24-hour average intensity differences of individual days range from 0 to +- 1.5%, and the most prominent time variation is recurrence tendency with a period consistent with the 27-day solar rotation period. A recently developed procedure for evaluating the statistical significance of quasipersistent data has been utilized to establish the reality of the 27-day signal disclosed by superposed epoch analysis of the north-south asymmetry data. Analyses of various components of the interplanetary magnetic field reveal that the IMF component B-bar/sub ..mu../ (parallel to the nominal garden hose direction) also displays a 27-day variation with maximum amplitude. Furthermore, a significant relationship between B-bar/sub ..mu../ and the north-south asymmetry is established by Chree analysis. On the basis of this relationship, it is suggested that the 27-day variation in the north-south asymmetry arises from the B-bar/sub ..mu../ x del-bar(n) drift, where del-bar(n) represents the radial gradient of cosmic rays.
Research Organization:
Bartol Research Foundation of the Franklin Institute University of Delaware, Newark, Delaware 19711
OSTI ID:
6249767
Journal Information:
J. Geophys. Res.; (United States), Journal Name: J. Geophys. Res.; (United States) Vol. 87:A12; ISSN JGREA
Country of Publication:
United States
Language:
English

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