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Past and recent observations of the solar upper atmosphere at vacuum-ultraviolet wavelengths
DOI: 10.1016/S1364-6826(02)00285-7
Bibcode: 2003JASTP..65..167W
Wilhelm, Klaus
Our understanding of the high-temperature solar atmosphere is to a large extent based on spectroscopic observations of emission lines and continuum radiation in the vacuum-ultraviolet (VUV) wavelength range of the electromagnetic spectrum. In addition, important contributions stem from soft X-ray measurements. The VUV radiation is produced by tran…
2003
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Journal of Atmospheric and Solar-Terrestrial Physics
SOHO
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