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- W1799286 abstract "The solar corona is an extremely hot (106 K or about 0.1 keV), almost fully ionised plasma which extends from a few thousand km above the Sun’s visible surface or photosphere (6000 K) to where it freely expands into the solar system as the solar wind. The exact reasons for its high temperature are still being debated despite more than 50 years of research, but magnetic fields are believed to be responsible for this heating. This article reviews some recent progress in our understanding, using data from spacecraft (Yohkoh, SOHO and TRACE) and from ground-based eclipse observations." @default.
- W1799286 created "2016-06-24" @default.
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- W1799286 date "2003-01-01" @default.
- W1799286 modified "2023-10-18" @default.
- W1799286 title "The Solar Corona" @default.
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- W1799286 doi "https://doi.org/10.1007/3-540-36963-5_8" @default.
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