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Fine Structure in Type IV Solar Radio Bursts
Published online by Cambridge University Press: 25 May 2016
Abstract
(Solar Phys.). The fine structure in solar type IV radio bursts was studied using the 169 MHz Nançay radioheliograph and the 60 channel radiospectrograph at Utrecht (160–320 MHz). The observed fine structure includes pulsating structure, zebra patterns (parallel drifting bands) and intermediate drift bursts. All are considered as modulation of high frequency radiation by low frequency oscillations or as the result of up conversion of low frequency oscillations to higher frequencies (Rosenberg, 1973).
- Type
- Part II The Flash Phase of Solar Flares
- Information
- Symposium - International Astronomical Union , Volume 57: Coronal Disturbances , 1974 , pp. 291 - 292
- Copyright
- Copyright © Reidel 1974