Line Tables

These tables give observed air wavelengths for the 2000-20000 Å range for spectra other than Fr I. Outside of the 2000-20000 Å range, the wavelengths are vacuum wavelengths. Lines of Fr I are extrapolated vacuum wavelengths from known energy levels. All observed lines are from NIST ASD. All energy level information is from NIST ASD. Wavelengths from MIT Wavelength Tables have been omitted as this publication appears to still be under copyright. However, in some cases, the exact same wavelength is given by NIST and MIT; in that case, the line is included.

Line intensities have been adjusted in the visible region to match photographed visible spectra. Line intensities of Rn have been adjusted to match the Grotrian diagram of Rn I. Line intensities in the infrared and ultraviolet are less reliable, but every effort was made to estimate them as accurately as possible. The elements He, O, Cl, Ar, Kr, and Xe have had their NIR lines photographed out to roughly 11000 Å. The intensities of the "brightest" several IR lines of each of these elements, in the 7000-10000 Å range, can be trusted. For the range of 3800-8000 Å, estimated visual brightnesses (EVB) are given. A dash in either of the intensity columns means the line intensity would be less than one relative to other lines of the same spectrum.

All Spectra

H   He
Li Be   B C N O F Ne
Na Mg   Al Si P S Cl Ar
K Ca   Sc Ti V Cr Mn Fe Co Ni Cu Zn Ga Ge As Se Br Kr
Rb Sr   Y Zr Nb Mo Tc Ru Rh Pd Ag Cd In Sn Sb Te I Xe
Cs Ba La Ce Pr Nd Pm Sm Eu Gd Tb Dy Ho Er Tm Yb Lu Hf Ta W Re Os Ir Pt Au Hg Tl Pb Bi Po At Rn
Fr Ra Ac Th Pa U Np Pu Am Cm Bk Cf Es Fm Md No Lr Rf Db Sg Bh Hs Mt Ds Rg Cn Nh Fl Mc Lv Ts Og

Entire Range | 2000-10000 Å | Visible Region | Si CCD/CMOS Region | Thermal IR | Vacuum UV
Specific Wavelength (rounded):  Å  nm
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λ, Å E. Sp.# Rel.Int. EVB Lower Config Lower Term+J Lower Level Upper Config Upper Term+J Upper Level
5795.78 Ra I 65 62 7s.7p 31 13999.3569 7p2? 3P1 31248.61
5811.58 Ra I 70 64 7s.6d 3D1 13715.779 6d.7p 12 30918.01
5813.63 Ra II 990 921 7p 23/2 26208.8538 8s 2S1/2 43405.05
5823.49 Ra I 30 28 7s.6d 3D3 14707.29 7s.8p 32 31874.25
5907.2 Ra I 25 20 7s.6d 3D2 13993.94 6d.7p 12 30918.01
5957.17 Ra I 30 24
5957.67 Ra I 120 103
6151.19 Ra I 210 139 7s.7p 32 16688.54 7p2? 3P2 32941.2
6158.73 Ra II 10 7 8p 21/2 50606.29 10s 2S1/2 66838.72
6167.03 Ra I 525 328 7s.6d 3D3 14707.29 6d.7p 12 30918.01
6200.3 Ra I 8000 4718 7s.6d 3D2 13993.94 6d.7p 33 30117.72
6247.16 Ra II 420 231 8p 23/2 52392.02 9d 2D5/2 68394.87
6298.56 Ra II 10 5 8p 23/2 52392.02 9d 2D3/2 68264.07
6336.9 Ra I 4500 2145 7s.6d 1D2 17081.31 7s.8p 11 32857.537
6438.9 Ra I 300 110 7s.7p 32 16688.54 7p2? 1D2 32214.76
6446.2 Ra I 10000 3576 7s.7p 32 16688.54 7s.7d 3D3 32197.27
6474.47 Ra I 150 51
6487.32 Ra I 10000 3268 7s.6d 3D3 14707.29 6d.7p 33 30117.72
6528.92 Ra I 150 44 7s.7p 32 16688.54 7s.7d 3D1 32000.78
6532.08 Ra I 300 88 7s.7p 32 16688.54 7s.7d 3D2 31993.4
6545.93 Ra I 300 84
6585.41 Ra I 540 133
6593.34 Ra II 5500 1357 5f 25/2 48987.86 5g 2G7/2,9/2 64150.49
6599.47 Ra I 330 80 7s.6d 1D2 17081.31 6d.7p 31 32229.89
6645.95 Ra I 180 38
6653.33 Ra I 195 39
6719.32 Ra II 7000 1126 5f 27/2 49272.14 5g 2G7/2,9/2 64150.49
6758.2 Ra I 705 101 7s.6d 1D2 17081.31 7s.8p 32 31874.25
6903.1 Ra I 315 26 7s.6d 1D2 17081.31 7s.8p 31 31563.4
6920.11 Ra II 10 1 8p 23/2 52392.02 10s 2S1/2 66838.72
6980.22 Ra I 7500 443 7s.6d 3D1 13715.779 6d.7p 32 28038
7078.02 Ra II 375 14 6d 2D3/2 12084.2721 7p 23/2 26208.8538
7118.5 Ra I 4500 139 7s.6d 3D2 13993.94 6d.7p 32 28038
7141.2167 Ra I 9000 236 7s2 1S0 0 7s.7p 31 13999.3569
7225.16 Ra I 4000 62 7s.6d 1D2 17081.31 6d.7p 12 30918.01
7310.27 Ra I 2000 18 7s.7p 30 13078.4 7s.8s 3S1 26754.02
7468.21 Ra I 5 -
7499.87 Ra I 50 -
7565.49 Ra I 10 -
7836.09 Ra I 10 -
7838.12 Ra I 390 - 7s.7p 31 13999.3569 7s.8s 3S1 26754.02
7877.08 Ra I 10 -
7896.43 Ra I 25 -
8005.13 Ra I 25 -
8019.25 Ra I 10 -
8019.7 Ra II 765 - 6d 2D5/2 13742.99 7p 23/2 26208.8538
8177.31 Ra I 40 - 7s.7p 11 20715.6142 7p2? 3P2 32941.2
8248.7 Ra I 25 -
8269.03 Ra I 25 -
8335.07 Ra I 25 -
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