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Spectroscope focused on a Bunsen flame

Spectroscope focused on a Bunsen flame. The sodium flame test. The Sun. Atoms in the cooler gas mantle around the Sun absorb the background hotter radiation we see at specific wavelengths.

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Spectroscope focused on a Bunsen flame

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  1. Spectroscope focused on a Bunsen flame

  2. Thesodiumflame test

  3. The Sun

  4. Atoms in the cooler gas mantle around the Sun absorb the background hotter radiation we see at specific wavelengths

  5. Fraunhofer’s original drawn lines overlayed on the visible spectrum - NB with red to the left (modern convention is blue to the left)

  6. G F E D C B A 500 600 700 nm 400 Fraunhofer mapped out the puzzling dark lines in the solar spectrum labelling them A B C D… from the red end

  7. 3P3/2 Sodium D Lines 3P1/2 589.0 nm 589.6 nm 2S1/2 0.597 nm

  8. Fraunhofer Absorption Lines in the Sun’s Spectrum Na D lines Orange street lamps contain sodium

  9. 3P3/2 Sodium D Lines 3P1/2 589.0 nm 589.6 nm 2S1/2 0.597 nm

  10. Fraunhofer – the Father of Astrophysics

  11. Thomson Higher Education

  12. Commemorated by the German Stamp

  13. G F E D C B 500 600 700 nm 400

  14. Noting that the solar spectrum was crossed by "innumerable" dark lines, Fraunhofer mapped their relative positions with precision.  He developed an alphabetic system for labeling selected reference lines, assigning A to a line near the red end of the spectrum, D to the pair of dark lines associated with the bright orange streak he had observed in flame spectra, H to a line near the end of the visible violet, and I to a line in the ultraviolet.  Fraunhofer's lines puzzled practitioners and theorists alike for over four decades after the publication of his spectral maps.

  15. Noting that the solar spectrum was crossed by "innumerable" dark lines, Fraunhofer mapped their relative positions with precision.  He developed an alphabetic system for labeling selected reference lines, assigning A to a line near the red end of the spectrum, D to the pair of dark lines associated with the bright orange streak he had observed in flame spectra, H to a line near the end of the visible violet, and I to a line in the ultraviolet.  Fraunhofer's lines puzzled practitioners and theorists alike for over four decades after the publication of his spectral maps.

  16. Fraunhofer Absorption Lines in the Sun’s Spectrum Na D lines Orange street lamps contain sodium Harry Kroto 2004

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