The influence of the local solar wind structures on the propagation of low energy particles

Details The influence of the local solar wind structures on the propagation of low energy particles The influence of the local solar wind structures on the propagation of low energy particles

Nov 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984esasp.207..293a&link_type=abstract

In ESA Plasma Astrophys. p 293-296 (SEE N85-22270 12-90)

Astronomy and Astrophysics

Astrophysics

Astronomical Models, Electron Emission, Solar Activity Effects, Solar Wind, Confinement, Rotating Environments, Twenty-Seven Day Variation

Scientific paper

The authors investigate the role that the high speed solar wind streams (HSS) may play in the confinement and propagation of low energy particles. They find that there exists a good correlation between the electron quiet time increases at 1 AU (QTI) and the HSS. The authors therefore propose that confinement and propagation in the local solar wind structures can in principle explain the morphology of the QTI without invoking source effects as current models do. Finally the authors test this interpretation by using data from the corotating nuclei events.

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