Physics
Scientific paper
Dec 1976
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976soph...50..491s&link_type=abstract
Solar Physics, vol. 50, Nov.-Dec. 1976, p. 491-500.
Physics
5
Interplanetary Magnetic Fields, Magnetic Effects, Proton Energy, Solar Flares, Solar Protons, Astronomical Catalogs, Histograms, Proton Flux Density, Solar Corona
Scientific paper
Onsets of some 40 to 45 low-energy proton events during the years 1957-1969 coincided in time with transits of well-defined sector boundaries across the earth. These events can be interpreted as long-lived proton streams filling up some of the magnetic sectors, indicating an acceleration of protons which is not associated with typical proton-producing flares. The sharp onsets of these particle streams, as well as a deficiency of flare-associated particle events shortly before the boundary transit, indicate that in some cases magnetic sector boundaries can inhibit transverse propagation of low-energy particles in the solar corona or in interplanetary space.
Dodson-Prince H. W.
Fritzova-Svestkova L.
Hedeman Ruth E.
Nolte J. T.
Svestka Zdenek
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