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- W2104350321 abstract "The last few years have seen great advances in the instrumentation used to obtain X-ray spectra of the Sun. These new observations reveal a wealth of multiplet structure containing many lines which allow us to understand more of the nature of the coronal plasma. Three areas of interest are examined. (1) The temperature sensitive satellite lines to helium —like resonance lines. (2) The strong lines of neon —like iron, Fexvii. (3) The combination of high spectral and high spatial resolution (Skylab) observations." @default.
- W2104350321 created "2016-06-24" @default.
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- W2104350321 date "1976-05-06" @default.
- W2104350321 modified "2023-09-27" @default.
- W2104350321 title "A Discussion on the physics of the solar atmosphere - High resolution x-ray spectra of the Sun" @default.
- W2104350321 doi "https://doi.org/10.1098/rsta.1976.0035" @default.
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