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Radial transport of energetic solar flare particles from 1 to 6 AU

Journal Article · · J. Geophys. Res.; (United States)
The Pioneer 10 and 11 missions to Jupiter and beyond have provided the first opportunity to observe solar flare acclerated particles at distances of several astronomical units from the sun. The intensity-time profiles out to at least 6 AU ae consistent with mainly diffusive interplanetary propagation. No obvious effects of a free escape boundary have been observed, which implies that the outer boundary of the diffusion region is beyond to AU. Four solar particle events are discussed in detail. These are events during which azimuthal propagation and corotation effects played a relatively minor role at least until the time of maximum intensity. Their intensity-time profiles, which were observed simultaneously at two or three well-separated radial positions (with Imp 6 or Imp 8 at I AU and with Pioneer 10 and/or Pioneer 11 at 2.7-6.1 AU), are used to study the radial transport of energetic particles in interplanetary space. The events are interpreted in terms of a spherically symmetric propagation model which includes the effects of diffusion, convection, and adiabatic deceleration and which assumes that the particles are impulsively injected at the sun.
Research Organization:
Enrico Fermi Institute and Department of Physics, University of Chicago, Chicago, Illinois 60637
OSTI ID:
7110003
Journal Information:
J. Geophys. Res.; (United States), Journal Name: J. Geophys. Res.; (United States) Vol. 82:16; ISSN JGREA
Country of Publication:
United States
Language:
English