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• W2945784416 abstract "Filaments (when seen in absorption on the solar disk) or prominences (when seen in emission above the limb) reveal the location of the magnetic neutral line in active regions and often represent progenitors of CMEs. What mainly distinguishes filaments from ordinary coronal loops or flux tubes is that their temperature is much cooler, and their density is much higher than the surrounding corona, and thus they are likely to be fed by upflows of heated dense chromospheric plasma that cools off by condensation." @default.
• W2945784416 created "2019-05-29" @default.
• W2945784416 creator A5075355111 @default.
• W2945784416 date "2019-01-01" @default.
• W2945784416 modified "2023-09-23" @default.
• W2945784416 title "Filaments and Prominences" @default.
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• W2945784416 doi "https://doi.org/10.1007/978-3-030-13956-8_11" @default.
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