NASA NTRS · 19730029150
The solar EUV-emitting plasma.
Abstract
The extreme ultraviolet (EUV), covering a decade in wavelength from about 300 A to about 3000 A, is considered. The general characteristics of the quiet solar atmosphere are reviewed, with emphasis on how the observed emission may be used as a tool to infer this structure. Many of the same techniques are applied to the study of overall properties of active regions.
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Noyes, R. W., Withbroe, G. L.. 1972-11-01. The solar EUV-emitting plasma.. https://ntrs.nasa.gov/citations/19730029150
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