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The Balmer series refers to a set of spectral lines in the visible region of the electromagnetic spectrum that are emitted by energized hydrogen atoms. In 1885, Swiss mathematician Johann Balmer discovered a formula that accurately described the wavelengths of these lines. This formula, which uses the Rydberg constant, was a significant step in the development of atomic theory and the field of spectroscopy. Later, Niels Bohr's theory of discrete energy states within the atom explained why Balmer's formula worked. Other spectral line series for hydrogen, like the Lyman, Paschen, Brackett, and Pfund series, exist in the ultraviolet and infrared regions.12

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