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hydrogen spectral series
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(physics) several series of spectral lines of hydrogen that correspond to quantum transitions between the various allowed energy levels of the hydrogen atom
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Astronomical spectroscopy Bohr model Hydrogen spectral series Lyman series Rydberg formula Stellar classification Theoretical and experimental justification for the Schrödinger equation Nave, C. R. (2006).
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The constant first arose as an empirical fitting parameter in the Rydberg formula for the hydrogen spectral series, but Niels Bohr later showed that its value could be calculated from more fundamental constants, explaining the relationship via his "Bohr model".
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The emission spectrum of atomic hydrogen has been divided into a number of spectral series, with wavelengths given by the Rydberg formula.
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Many spectral lines of atomic hydrogen also have designations within their respective series, such as the Lyman series or Balmer series.
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The spectral series are important in astronomical spectroscopy for detecting the presence of hydrogen and calculating red shifts.
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The Balmer series or Balmer lines in atomic physics, is the designation of one of a set of six named series describing the spectral line emissions of the hydrogen atom.
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The familiar red H-alpha spectral line of the Balmer series of atomic hydrogen, which is the transition from the shell n = 3 to the shell n = 2, is one of the conspicuous colours of the universe.
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As the first spectral lines associated with this series are located in the visible part of the electromagnetic spectrum, these lines are historically referred to as "H-alpha", "H-beta", "H-gamma" and so on, where H is the element hydrogen.
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8 sinne gevind in 3 ms. Hulle kom uit baie bronne en word nie nagegaan nie.