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Jupiter's magnetosphere as a 'point source' for electrons propagating from 1 to 12 AUA profile of electron intensities in the interplanetary medium from 1 to 12 AU obtained from Pioneer 10 measurements of the 3-6 MeV Jovian electron flux shows recurring intensity peaks, the amplitude of which decreases with increasing distance from Jupiter both in the direction of the sun and away from it. Concurrent IMP-8 measurements of the 2-12 MeV electron flux revealed a series of 27-day recurrent intensity increases modulated with a period of about 13 months, beginning about four months before the probable magnetic field connection between earth and Jupiter. Amplitudes of the intensity increases reached a maximum near the time of best connection. These results are consistent with a three-dimensional interplanetary diffusion model with Jupiter as a continuously emitting point source.
Document ID
19790053512
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Chenette, D. L.
(Chicago Univ. Chicago, IL, United States)
Conlon, T. F.
(Chicago Univ. Chicago, IL, United States)
Pyle, K. R.
(Chicago, University Chicago, Ill., United States)
Simpson, J. A.
(Chicago Univ. Chicago, IL, 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
79A37525
Funding Number(s)
CONTRACT_GRANT: NSF ATM-75-20407
CONTRACT_GRANT: NAS2-6551
Distribution Limits
Public
Copyright
Other

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