Physics
Scientific paper
May 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992kosis..30..368l&link_type=abstract
Kosmicheskie Issledovaniya (ISSN 0023-4206), vol. 30, no. 3, p. 368-377.
Physics
Energetic Particles, Proton Energy, Solar Activity, Solar Protons, Solar Wind Velocity, Satellite Observation, Shock Wave Interaction, Solar Cycles
Scientific paper
Recurrent enhancements of energetic particle fluxes recorded on board the space probes VEGA-1 and VEGA-2 during the first half of 1985 formed a long-lasting series of events during the decreasing phase of the 21st solar cycle. On the basis of intensity data for protons with energies of 1-2 MeV measured by the IMP-7 and IMP-8 spacecraft, it is found that the series spans 26 solar rotations. During recurrent events the flux of 0.04-1.0 MeV protons and ions reaches a maximum several hours earlier than particles greater than 1 MeV particles. The last ten enhancements of the series are associated with a coronal hole on the sun.
Gringauz K.
Kecskemety Károly
Klimenko I.
Logachev Yu.
Somogyi Andrea
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