In the spectrum of hydrogen atom which of the spectral lines falls in visible region.
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Four of the Balmer lines are in the technically "visible" part of the spectrum, with wavelengths longer than 400 nm and shorter than 700 nm. Parts of the Balmer series can be seen in the solar spectrum. H-alpha is an important line used in astronomy to detect the presence of hydrogen.
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Explanation:
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Transition from higher states to n=2 lead to emission of radiation with wavelengths 656.3nm and 365.0nm. These wavelengths fall in the visible region and constitute the Balmer series.
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