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Unusual Absorption of a Solar Type II Burst by ‘Shadow’ Type III Bursts
Published online by Cambridge University Press: 25 May 2016
Abstract
(Proc. Astron. Soc. Australia). The Hα-flare on 1968 August 23d23h45m was followed by a short-lived type II burst. The radio spectrograph record obtained at Culgoora is shown in Figure 1. The type II burst was of split-band structure with unusual spectral features in each component of the split band. The most remarkable one is an absorption feature between 23h52m02s and 23h52m10s: suppression of the bright type II emission along an ‘inverted U’ (between 120 and 85 MHz).
- Type
- Part II The Flash Phase of Solar Flares
- Information
- Symposium - International Astronomical Union , Volume 57: Coronal Disturbances , 1974 , pp. 245 - 248
- Copyright
- Copyright © Reidel 1974