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XSIQ
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Physics - Absorption spectra
Absorption spectra
When light of a wide range of frequencies (e.g. from the sun) passes
through a pure substance (e.g. a gas), only photons with energies_ (hf)_
equal to energy differences between electron levels will be absorbed. If
the light is then spread into a spectrum, [1] there will be dark lines
corresponding to these absorbed frequencies.
Absorption spectrum for the element hydrogen
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