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Coherent Effect in the Preferential Acceleration of Relativistic Solar Heavy Cosmic Ray Nuclei

Published online by Cambridge University Press:  25 May 2016

Shahinaz M. A. Yousef
Shahinaz M. A. Yousef*
Affiliation:
Astronomy Dept., Cairo University, Cairo, Egypt

Abstract

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(Solar Phys.). The observed enrichment of heavy nuclei in the composition of relativistic cosmic rays including solar, may be explained on the basis of a coherent accelerating mechanism. This mechanism requires the existence of high intensity relativistic electron beams or preferably blobs (with number density ≥1011 electrons cm−3) in the accelerating solar regions. The radius of each blob should be less than its plasma wavelength, i.e. of the order of cm.

Type
Part IV Acceleration, Containement and Emission of High-Energy Flare Particles
Information
Symposium - International Astronomical Union , Volume 57: Coronal Disturbances , 1974 , pp. 477 - 478
Copyright
Copyright © Reidel 1974