Small-scale inhomogeneities in the solar
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D. B. Melrose
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Article
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1975
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Springer
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English
โ 517 KB
A number of inconsistencies between simple theory and observations of solar radio bursts indicate that mode-mode coupling in the solar corona is much stronger than predicted. The inconsistencies include the absence of predicted reversal of the sense of polarization in a type 1 storm at CMP, and the