Physics
Scientific paper
Aug 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....4..347m&link_type=abstract
In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 4 p 347-350 (SEE N85-34729 23-92)
Physics
Interplanetary Space, Solar Cosmic Rays, Solar Flares, Transport Properties, Cosmic Ray Showers, Energy Spectra, International Sun Earth Explorers, Models, Spatial Distribution, Temporal Distribution
Scientific paper
Time intensity profiles of solar flare energetic particle events carry information on the particle injection processes at the Sun, as well as the transport of particles in interplanetary space. However, in order to help identify the individual processes of injection versus transport it is necessary to use observations taken at more than one radial location. Results of such a study concerning the 22 November 1977 solar particle event, observed with instruments at 1.0 and 1.55 AU are presented. The observations are for particles of energies near 1 MeV/nucleon, considerably less than the approx. 10 to 20 MeV/nucleon energies typical of previous radial transport studies. Thus, in the present work it is possible to examine the validity of transport models to considerably lower energies than in previous work.
Gloeckler George
Hamilton Douglas C.
Klecker Berndt
Mason Glenn M.
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