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Solar Prominence Observed by Young

  • Pl. XII

  • 1872 (Published)

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Prominences represented in their natural colors, as seen through a large telescope when the slit of the spectroscope was open wide and directed on to the red C-line. These prominences are characteristic of the a nebulous form.

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  • 662 pages
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  • Courtesy of Science History Institute

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Schellen, Heinrich. “Solar Prominence Observed by Young.” Spectrum Analysis in Its Application to Terrestrial Substances, and the Physical Constitution of the Heavenly Bodies. London, England: M. & N. Hanhart (Printers), 1872. https://digital.sciencehistory.org/works/3197xn19c.

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