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- W3100663095 abstract "Here, we report on the unique observation of flaring coronal loops at the solar limb using high-resolution imaging spectropolarimetry from the Swedish 1 m Solar Telescope. The vantage position, orientation, and nature of the chromospheric material that filled the flare loops allowed us to determine their magnetic field with unprecedented accuracy using the weak-field approximation method. Our analysis reveals coronal magnetic field strengths as high as 350 G at heights up to 25 Mm above the solar limb. These measurements are substantially higher than a number of previous estimates and may have considerable implications for our current understanding of the extended solar atmosphere." @default.
- W3100663095 created "2020-11-23" @default.
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- W3100663095 date "2019-03-29" @default.
- W3100663095 modified "2023-10-15" @default.
- W3100663095 title "Mapping the Magnetic Field of Flare Coronal Loops" @default.
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- W3100663095 doi "https://doi.org/10.3847/1538-4357/ab08e9" @default.
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