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Type II Burst-Sources as Low-VA Regions in the Corona ‘Illuminated’ by Flare-Induced MHD Shocks
Published online by Cambridge University Press: 25 May 2016
Abstract
(Solar Phys.). The author has proposed a hypothesis that the type II burst-sources may be due to the local enhancement of the flare-produced MHD fast-mode shock wave on encountering the pre-existing low Alfvén velocity regions in the corona (Uchida, 1973). The purpose of the present paper is to show that this may actually be the case by comparing the behavior of the computor-simulated propagation and strengthening of MHD fast-mode (weak) shock with the observed characteristics of type II burst-sources.
- Type
- Part III Shock Waves and Plasma Ejection
- Information
- Symposium - International Astronomical Union , Volume 57: Coronal Disturbances , 1974 , pp. 383 - 385
- Copyright
- Copyright © Reidel 1974