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Evolutionary Relation between Type I Storm Activity and the S-Component at Centimetre Wavelengths
Published online by Cambridge University Press: 25 April 2016
Extract
Type I storms are the most frequently observed solar phenomena at metre and decimetre wavelengths. Since the first identification of the emission of this type with a large sunspot group a great many type I storms have been recorded with radio-spectrographs, polarimeters and interferometers (see, for example, Wild, Smerd and Weiss, Kundu, Wild). Nevertheless, we can offer no satisfactory answers to the most fundamental questions about type I storms: ‘What kind of disturbances supply energy to a localized coronal region to maintain the storm activity for up to several days?’; ‘What is the emission mechanism responsible for the peculiar features observed in type I storms?’.
- Type
- Contributions
- Information
- Publications of the Astronomical Society of Australia , Volume 2 , Issue 4 , October 1973 , pp. 217 - 219
- Copyright
- Copyright © Astronomical Society of Australia 1973
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