The following five hydrogen lines were measured

PHYSICS · Multi-part · Fermi University Physics · Atomic, Molecular & Optical Physics · One-electron atoms and the origins of atomic structure · One-electron atoms and the origins of atomic structure

Reading the Spectrum, Ch Lines, series and the term diagram: what a spectrometer measures

Problem

The following five hydrogen lines were measured, the first in vacuum (air absorbs so far into the ultraviolet) and the other four in air: 121.567 nm121.567\,\mathrm{nm}, 656.280 nm656.280\,\mathrm{nm}, 486.130 nm486.130\,\mathrm{nm}, 434.050 nm434.050\,\mathrm{nm}, 1875.10 nm1875.10\,\mathrm{nm}. For the visible lines measured in air, use the vacuum correction λvac=1.000274 λair\lambda_{\rm vac} = 1.000274\,\lambda_{\rm air}. ((a)) State which series (Lyman, Balmer or Paschen) each line belongs to, giving your reasoning from the wavelength range alone. ((b)) Convert the three lines you assigned to the Balmer series to vacuum wavenumbers. ((c)) These three Balmer lines correspond to the upper levels n2=3,4,5n_2 = 3, 4, 5 (with n1=2n_1=2). Fit RHR_{\rm H} by computing ν~/(1/4−1/n22)\tilde\nu/(1/4 - 1/n_2^2) for each line and averaging. ((d)) Using your fitted RHR_{\rm H}, construct the term values Tn=RH/n2T_n = R_{\rm H}/n^2 for n=1,2,3,4n=1,2,3,4 in cm−1\mathrm{cm^{-1}}. Draw them as horizontal lines below a zero marking the ionisation limit, add an arrow for Hα\alpha between the two levels it joins, labelled with its measured wavenumber, and give the ionisation energy of hydrogen in eV.

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