Radial and latitudinal gradients of anomalous oxygen during 1977 - 1985

Details Radial and latitudinal gradients of anomalous oxygen during 1977 - 1985 Radial and latitudinal gradients of anomalous oxygen during 1977 - 1985

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....5..172w&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 5 p 172-175 (SEE N85-34991 23-93)

Physics

Cosmic Rays, Energy Spectra, Latitude, Oxygen, Radial Distribution, Radiant Flux Density, Solar Magnetic Field, Annual Variations, Magnetic Anomalies, Protons, Temporal Distribution, Voyager Project

Scientific paper

The authors find that the radial gradient of anomalous O remains constant during 1977 - 85 at ≡10 - 15%/AU although the intensity changes by more than a factor of 100. These results can be used to deduce that most of the modulation of the intensities of these particles is occurring beyond 27 AU. Evidence for a latitudinal gradient of ≡+3%/degree at low energies (7.1 - 10.6 MeV/nuc) is also found.

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