Variations of galactic cosmic rays with heliolatitude in the outer heliosphere

Details Variations of galactic cosmic rays with heliolatitude in the outer heliosphere Variations of galactic cosmic rays with heliolatitude in the outer heliosphere

Aug 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986georl..13..781m&link_type=abstract

Geophysical Research Letters (ISSN 0094-8276), vol. 13, Aug. 1986, p. 781-784.

Astronomy and Astrophysics

Astronomy

25

Galactic Cosmic Rays, Heliosphere, Interplanetary Medium, Spaceborne Astronomy, Flux Quantization, Kinetic Energy, Latitude, Voyager 1 Spacecraft, Voyager 2 Spacecraft

Scientific paper

On 1 January 1986, Voyager 1 was at a heliolatitude of 30° above the
ecliptic plane at a radial distance of 25.4 AU. The galactic cosmic ray
latitudinal gradients in the outer heliosphere measured at that time
were found to be negative, ≡ 1 - 2%/AU, show no strong energy
dependence and are approximately half the radial gradient.

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