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Evidence of Directivity of Solar Type III Radio Burst Storm Emission
Published online by Cambridge University Press: 25 April 2016
Extract
Solar type III radio bursts often occur for prolonged periods (≳ 1 hour) with small time intervals (≲ 1 minute) between bursts. Such phenomena usually are confined to decametre wavelengths (frequency ≲ 100 MHz) and are called ‘type III storms’ (e.g. Stewart and Labrum 1972).
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- Copyright © Astronomical Society of Australia 1980
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