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- W2004368344 abstract "We study a possible connection of moving magnetic features (MMFs) and the overlying atmosphere using several sets of multiwavelength observations of sunspot areas from the photosphere to the corona. We find that as a collective phenomenon, very intense MMF formation anticorrelates with the presence of large-scale stable coronal loops: such loops are rooted at the side of sunspots with no or few MMFs rather than at the side of the penumbra/moat highly populated by MMFs. Conjectures to help understand the observed correlation between the preferable site of coronal loops and the deficiency of MMFs are discussed." @default.
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- W2004368344 date "2007-01-19" @default.
- W2004368344 modified "2023-09-27" @default.
- W2004368344 title "Anticorrelation between Moving Magnetic Features and Coronal Loop Formation" @default.
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- W2004368344 doi "https://doi.org/10.1086/512184" @default.
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