Physics
Scientific paper
Apr 1976
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976natur.260..491m&link_type=abstract
Nature, vol. 260, Apr. 8, 1976, p. 491-495. Research supported by the Science Research Council.
Physics
10
Interplanetary Magnetic Fields, Muons, Particle Energy, Periodic Variations, Primary Cosmic Rays, Interstellar Magnetic Fields, Multipolar Fields, Northern Hemisphere, Solar Activity Effects, Solar Magnetic Field
Scientific paper
The apparent sidereal variation in the intensity of muons generated by cosmic rays with energies greater than 10 to the 11th eV showed a marked change in phase at Northern Hemisphere stations at the time of the recent reversal in sign of the general solar magnetic field. No corresponding change was observed at rather lower energies at Hobart, Tasmania. By adopting a particular model of the large scale interplanetary field, it is possible to account for this behavior of the sidereal variation in terms of a primary cosmic ray anisotropy which is related to the local direction of the galactic magnetic field.
Elliot H.
Hynds R. J.
Marsden Richard G.
Thambyahpillai T.
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