Computer Science
Scientific paper
Aug 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....5..198m&link_type=abstract
In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 5 p 198-201 (SEE N85-34991 23-93)
Computer Science
Cosmic Rays, Energy Spectra, Galactic Radiation, Solar Activity, Helium, Pioneer 10 Space Probe, Protons, Temporal Distribution, Time Dependence
Scientific paper
Radial gradients for relativistic galactic cosmic rays (E > 70 MeV) remained nearly constant at ≡2.5%/AU from 1978 - 84, which includes the period of maximum solar modulation in 1981 - 82. For energies 30 - 70 MeV/n, gradients decreased at solar maximum to values of 1%/AU (protons) and 4%/AU (helium), and appear to be increasing again in 1983 - 84 toward the values found for solar minimum. The anomalous helium component has not reappeared, either at 1 AU or at Pioneer 10 at R > 34 AU.
McKibben Bruce R.
Pyle Roger K.
Simpson André J.
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