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Exercise:
In astrophysics so called radio recombination lines i.e. transitions from high n states to lower states are routinely observed. The observed spectral lines for hydrogen are labelled Hnalpha for transitions nto n-. vspacemm Calculate the wavelength for the Halpha line.

Solution:
The photon energy is E_gamma E_leftfracn^-fracn-^ right E_fracn-^-n^n^n-^ E_ frac-n+nn+^ frachclambda Solving for the wavelength yields lambda laF frachcEgr times fracntimesn+^-timesn+ resultlaP-
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Exercise:
In astrophysics so called radio recombination lines i.e. transitions from high n states to lower states are routinely observed. The observed spectral lines for hydrogen are labelled Hnalpha for transitions nto n-. vspacemm Calculate the wavelength for the Halpha line.

Solution:
The photon energy is E_gamma E_leftfracn^-fracn-^ right E_fracn-^-n^n^n-^ E_ frac-n+nn+^ frachclambda Solving for the wavelength yields lambda laF frachcEgr times fracntimesn+^-timesn+ resultlaP-
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quantum physics
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energy level, hydrogen, photon, wavelength
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(2, default)
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Language
ENG (English)
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Calculative / Quantity
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