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- W2726155031 abstract "An updated report is given of observations of galactic cosmic ray intensity to heliocentric radial distances of 8.6 and 18.4 AU with Pioneer 11 and Pioneer 10, respectively. Solar activity via the magnetic structure of the interplanetary medium continues to modulate the intensity out to the greatest distance reached thus far. During the period 1972-1979, aperiodic temporal variations of intensity by about a factor of two and on a time scale of the order of a year are observed as are quasi-persistent cyclic variations of 26-day period and amplitude of a few percent. The latter are associated with fast-slow solar wind streams, not with toward-away magnetic field sectors. For protons of energy E/sub P/ > 80 MeV, there is a fairly consistent heliocentric radial gradient of +2.1 (+- 0.3) percent per AU in intensity until April-May 1978, at which time a substantial disruption of the distribution of cosmic rays in the heliosphere occurred. The radius of the heliosphere is estimated to be of the order of 80 AU." @default.
- W2726155031 created "2017-07-14" @default.
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- W2726155031 date "1979-08-01" @default.
- W2726155031 modified "2023-09-27" @default.
- W2726155031 title "Galactic cosmic-ray intensity to a heliocentric distance of 18 AU. Progress report. [Pioneer 10 and 11]" @default.
- W2726155031 hasPublicationYear "1979" @default.
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