Astronomy and Astrophysics – Astronomy
Scientific paper
Sep 1974
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974soph...38..227a&link_type=abstract
Solar Physics, vol. 38, Sept. 1974, p. 227-256. Research supported by the National Academy of Science
Astronomy and Astrophysics
Astronomy
2
Anisotropy, Interplanetary Magnetic Fields, Magnetic Field Configurations, Solar Cosmic Rays, Solar Flares, Solar Protons, Explorer 34 Satellite, Explorer 41 Satellite, Lines Of Force, Proton Energy, Satellite Observation, Spaceborne Astronomy, Statistical Analysis
Scientific paper
Data was obtained from instrumentation on Explorers 34 and 41 on cosmic-ray anisotropy and magnetic field vectors during five solar flare events. The analysis was conducted in the energy range from 0.7 to 7.6 MeV, of the late decay phase, to evaluate the dependence of net cosmic-ray anisotropy vector amplitude and direction on the magnetic field azimuth. Results showed that in the late decay phase the direction of the net cosmic-ray anisotropy vector was invariant in relation to the direction of the magnetic field, particle energy, and species. Within the statistical error of the available data the invariant direction was perpendicular to the mean magnetic field direction.
Allum F. R.
Fairfield Donald H.
Gleeson Leo John
McCracken K. G.
Palmeira A. R. R.
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