Chromosphere

Definition and stakes

Portrait of David P. Todd David P. Todd,  Astronomy: The Science of the Heavenly Bodies

“ Beneath the corona we meet the projecting prominences, to which parts of the corona are certainly related, and beneath them the first true layer or atmosphere of the sun known as the chromosphere, its average depth being about one-hundredth part of the sun's diameter. Beneath the chromosphere is the layer of the sun from which emanates the light by which we see it, called the photosphere. ”
Source: Gutenberg

George C. Comstock,  A Text-Book of Astronomy

“ Fig. 78.—A solar prominence.—Hale.
124. The chromosphere.—Between the corona and the photosphere there is a thin separating layer called the chromosphere (Greek, color sphere) , because when seen at an eclipse it shines with a brilliant red light quite unlike anything else upon the sun save the prominences which are themselves only parts of the chromosphere temporarily thrown above its surface, as in a fountain a jet of water is thrown up from the basin and remains for a few moments suspended in mid-air.
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Source: Gutenberg

John Lubbock,  Popular Science Monthly (1882)

“ The body of the sun, or photosphere, is intensely brilliant; round it lies the solar atmosphere of comparatively cool gases, which cause the dark lines in the spectrum; thirdly, a chromosphere—a sphere principally of hydrogen, jets of which are said sometimes to reach to a height of 100,000 miles or more, into the outer coating or corona, the nature of which is still very doubtful. ”
Source: Wikisource

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