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- Q2613048 subject Q7173499.
- Q2613048 subject Q7215740.
- Q2613048 subject Q8529487.
- Q2613048 abstract "The emission spectrum of atomic hydrogen is divided into a number of spectral series, with wavelengths given by the Rydberg formula. These observed spectral lines are due to the electron making transitions between two energy levels in the atom. The classification of the series by the Rydberg formula was important in the development of quantum mechanics. The spectral series are important in astronomical spectroscopy for detecting the presence of hydrogen and calculating red shifts.".
- Q2613048 thumbnail Hydrogen_spectrum.svg?width=300.
- Q2613048 wikiPageExternalLink index.php?option=com_content&view=category&layout=blog&id=50&Itemid=221.
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- Q2613048 wikiPageWikiLink Q7173499.
- Q2613048 wikiPageWikiLink Q7215740.
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- Q2613048 wikiPageWikiLink Q8529487.
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- Q2613048 wikiPageWikiLink Q944.
- Q2613048 wikiPageWikiLink Q970745.
- Q2613048 comment "The emission spectrum of atomic hydrogen is divided into a number of spectral series, with wavelengths given by the Rydberg formula. These observed spectral lines are due to the electron making transitions between two energy levels in the atom. The classification of the series by the Rydberg formula was important in the development of quantum mechanics. The spectral series are important in astronomical spectroscopy for detecting the presence of hydrogen and calculating red shifts.".
- Q2613048 label "Hydrogen spectral series".
- Q2613048 depiction Hydrogen_spectrum.svg.