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The Lyman series is one of the spectral line series produced by hydrogen atoms. These series are related sequences of wavelengths emitted by energized atoms, and when viewed through a spectroscope, they appear as lines that become closer together toward the shortest wavelength, known as the series limit.1

The Lyman series specifically lies in the ultraviolet region of the electromagnetic spectrum. Its wavelengths can be calculated using a formula similar to the Balmer series, but with a constant term that is the reciprocal of 1 squared, and the integer n begins at 2. This series corresponds to electron transitions from higher energy states down to the ground state (n=1) of the hydrogen atom.12

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