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- W3106433910 abstract "Context. Extreme UV (EUV) and X-ray loops in the solar corona connect regions of enhanced magnetic activity, but they are not usually rooted in the dark umbrae of sunspots because the strong magnetic field found there suppresses convection. This means that the Poynting flux of magnetic energy into the upper atmosphere is not significant within the umbra as long as there are no light bridges or umbral dots." @default.
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- W3106433910 date "2016-02-12" @default.
- W3106433910 modified "2023-10-16" @default.
- W3106433910 title "A closer look at a coronal loop rooted in a sunspot umbra" @default.
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- W3106433910 doi "https://doi.org/10.1051/0004-6361/201527340" @default.
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