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Estimate of cosmic-ray latitudinal gradients in 1981-1982

Journal Article · · Astrophys. J., Lett. Ed.; (United States)
DOI:https://doi.org/10.1086/184238· OSTI ID:6675648
We report an analysis of greater than 70 MeV galactic cosmic-ray proton gradients measured by Voyager 1 and Voyager 2 during the 17 month period from early 1981 through mid-1982. This period coincides with the initial phase of cosmic-ray recovery following a minimum reached in late 1980 to early 1981. During this interval, the two spacecraft remain within 4/sup 0/ of one another in heliolongitude, with Voyagers 1 and 2 moving in helioradius from 9.8 to 13.2 Au and 8.2 to 10.1 AU respectively. The Voyagers increase their heliolatitude separation from 3/sup 0/ to 16/sup 0/ as Voyager 1 moves from 2/sup 0/ south to 13/sup 0/ north of the helioequatorial plane at the rate of 1.5 per month following its encounter with Saturn in late 1980. We find that the intensity difference between the two spacecraft is consistent with either a positive radial gradient of approximately 2% per AU (assuming zero heliolatitude gradient), or a small heliolatiatude gradient of approximately 0.4% per degree (assuming zero helioradial gradient). At present, we are unable to make an unambiguous separation between the radial and latitudinal effects.
Research Organization:
Applied Physics Laboratory, The Johns Hopkins University
OSTI ID:
6675648
Journal Information:
Astrophys. J., Lett. Ed.; (United States), Journal Name: Astrophys. J., Lett. Ed.; (United States) Vol. 278:2; ISSN AJLEA
Country of Publication:
United States
Language:
English