Energetic particle recurrence and escape during solar cycle 20

Details Energetic particle recurrence and escape during solar cycle 20 Energetic particle recurrence and escape during solar cycle 20

Oct 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980icrc....5...46g&link_type=abstract

In: International Cosmic Ray Conference, 16th, Kyoto, Japan, August 6-18, 1979, Conference Papers. Volume 5. (A81-12386 02-93) T

Computer Science

Energetic Particles, Proton Flux Density, Solar Cosmic Rays, Solar Cycles, Solar Protons, Solar Wind, Interplanetary Magnetic Fields, Proton Energy, Solar Corona, Solar Wind Velocity

Scientific paper

Low-energy solar particle data have been combined from a multi-spacecraft near-earth data set covering most of solar cycle 20 (1966-1976). Particle intensity profiles have been ordered in the natural heliographic coordinate system of the estimated high coronal connection longitude of the foot point of the interplanetary field line. The recurrence trends of approximately 1-MeV solar particles become more apparent in this coordinate system than when plotted versus time, and thereby extend the evidence for regions of continual injection and escape from the corona. Intercomparison of solar particles and solar wind streams in heliographic longitude suggests that the origin of stream-associated spatial particle events seen at 1 AU is solar rather than interplanetary.

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