k Fraunhofer lines, illustration Fraunhofer lines. Illustration of the Suns spectrum, showing a set of dark absorption lines known as Fraunhofer lines. These are named after the German physicist Joseph von Fraunhofer 17871826, who discovered them in 1814. The spectrum is shown ranging from blue left to red right, with the wavelength in nanometres across bottom. The absorption lines indicate the presence of certain elements in the Suns atmosphere. Stock Photo - Afloimages
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Fraunhofer lines, illustration Fraunhofer lines. Illustration of the Sun s spectrum, showing a set of dark absorption lines known as Fraunhofer lines. These are named after the German physicist Joseph von Fraunhofer  1787 1826 , who discovered them in 1814. The spectrum is shown ranging from blue  left  to red  right , with the wavelength in nanometres across bottom. The absorption lines indicate the presence of certain elements in the Sun s atmosphere.
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Fraunhofer lines, illustration

Fraunhofer lines. Illustration of the Sun's spectrum, showing a set of dark absorption lines known as Fraunhofer lines. These are named after the German physicist Joseph von Fraunhofer (1787-1826), who discovered them in 1814. The spectrum is shown ranging from blue (left) to red (right), with the wavelength in nanometres across bottom. The absorption lines indicate the presence of certain elements in the Sun's atmosphere.

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