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NASA NTRS · 19800037013

Acceleration of energetic protons by interplanetary shocks

Abstract

The University of Iowa instrument aboard Pioneer 11 detected 69 energetic proton events (EPE) (in the 0.6-3.4 MeV energy range) during 1973-1974 in the heliocentric radial range 1-5 AU. Sixty percent of the EPE peak within plus or minus 5 hours of a corotating interaction region (CIR) boundary, while 19% peak inside and 21% peak outside the interaction regions. Of the CIR boundaries at which an EPE peaks with plus or minus 5 hours, 80% have associated shocks. The observed intensities and pitch angle distributions of protons near shock fronts are consistent with a theoretical simulation of the acceleration of protons by a drift in the electric field at the shock front.

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BibTeXRIS

Pesses, M. E., Tsurutani, B. T., Smith, E. J., Van Allen, J. A.. 1979-12-01. Acceleration of energetic protons by interplanetary shocks. https://ntrs.nasa.gov/citations/19800037013

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