Cosmic ray gradients in the outer heliosphere

Details Cosmic ray gradients in the outer heliosphere Cosmic ray gradients in the outer heliosphere

Aug 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983icrc....3...55w&link_type=abstract

International Cosmic Ray Conference, 18th, Bangalore, India, Aug. 22-Sept. 3, 1983, Paper. 4 p.

Physics

Heliosphere, Pioneer Space Probes, Solar Cosmic Rays, Cerenkov Counters, Energy Spectra, Least Squares Method, Solar Cycles

Scientific paper

Launched in 1972 and 1973 respectively, the Pioneer 10 and 11 spacecraft are now probing the outer heliosphere on their final escape from the sun. The data in this paper extend for almost an entire solar cycle from launch to early 1983, when Pioneer 10 was at a heliocentric distance of 29 AU and Pioneer 11, 13 AU. The UCSD instruments on board were used to study the gradient, and to look at the time and spatial variations of the cosmic ray intensities.

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