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- W61621854 abstract "Abstract X-ray images have revealed the corona to comprise four basic morphologies. In order of X-ray luminosity these structures are: (1) Bright, relatively short, X-ray loops in active regions, (2) Less bright and larger X-ray structures of the so-called quiet corona, (3) X-ray bright points, and (4) Coronal holes. The soft X-ray telescope (SXT) on Yohkoh provides good angular resolution with much improved time resolution and continuity of coverage as compared to the earlier observations. In the SXT movies these structures often appear to be interacting and change appearance on time scales from seconds to weeks. Flare, flare-like, and eruptive processes continuously alter the general structure of the corona. This paper will comment on the structure, changes and heating of the X-ray corona as revealed by the Yohkoh observations." @default.
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- W61621854 date "1994-01-01" @default.
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- W61621854 title "General Structure of the X-ray Corona" @default.
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- W61621854 doi "https://doi.org/10.1017/s0252921100025021" @default.
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