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- W2105991888 abstract "Over the past 2 decades our observational understanding of the outer layers of the solar atmosphere has increased dramatically. We now know that the solar chromosphere, transition region, and corona are highly structured and dynamic. Magnetic fields, rooted in the subphotospheric layers, provide the structure that channels the plasma in the upper layers of the solar atmosphere." @default.
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- W2105991888 date "1990-07-10" @default.
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- W2105991888 title "Dynamic modeling of the solar atmosphere" @default.
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- W2105991888 doi "https://doi.org/10.1029/90eo00229" @default.
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