Coronal and interplanetary transport of solar energetic protons and electrons

Details Coronal and interplanetary transport of solar energetic protons and electrons Coronal and interplanetary transport of solar energetic protons and electrons

Sep 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989soph..124..353w&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 124, no. 2, 1989, p. 353-392.

Physics

28

Coronal Loops, Interplanetary Medium, Solar Corona, Solar Electrons, Solar Protons, Helios 1, Helios 2, Magnetic Field Configurations, Prognoz Satellites, Solar Wind, Transport Properties

Scientific paper

Data from the Helios 1 and 2 and the Prognoz 6 spacecraft are used to separate coronal and interplanetary propagation effects for two solar particle events on December 27, 1977 and January 1, 1978. The results confirm the concept of two different coronal propagation regimes. In both regimes electrons are transported more efficiently than protons. Possible explanations for the fast transport of electrons and the different behavior of electrons and protons are considered.

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