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Cosmic ray intensity gradients in the outer solar system measured by Pioneer 10 and 11Earlier results are extended to include data from Pioneer 10 to a radial range of 11.3 AU, and from Pioneer 11 inward from 5 AU to 3.75 AU after Jupiter encounter, and to a maximum heliographic latitude of 17 deg. The data include the period from March 1972 through October 1976, during which time the neutron monitor cosmic ray intensity was, except for a few significant excursions, near solar minimum level. It is shown that the radial gradients of all particle species considered are small and positive throughout the period of study. On a shorter time scale, the data indicate transient decreases in the value of the differential gradient associated with major decreases in the cosmic ray intensity in the inner solar system. The observations are consistent with a modulating region whose radius is large compared to 11 AU. The 'anomalous' helium component, present since 1972 at earth orbit, is observed continuously at all radial distances.
Document ID
19790053409
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Mckibben, R. B.
(Chicago Univ. Chicago, IL, United States)
Ogallagher, J. J.
(Chicago Univ. Chicago, IL, United States)
Pyle, K. R.
(Chicago Univ. Chicago, IL, United States)
Simpson, J. A.
(Chicago, University Chicago, Ill., United States)
Date Acquired
August 9, 2013
Publication Date
January 1, 1978
Subject Category
Space Radiation
Meeting Information
Meeting: International Cosmic Ray Conference
Location: Plovdiv
Country: Bulgaria
Start Date: August 13, 1977
End Date: August 26, 1977
Accession Number
79A37422
Funding Number(s)
CONTRACT_GRANT: NSF ATM-75-20407
CONTRACT_GRANT: NAS2-6551
Distribution Limits
Public
Copyright
Other

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