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 800-8000 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

  ‹   Page:
λ, Å E. Sp.# Rel.Int. EVB Lower Config Lower Term+J Lower Level Upper Config Upper Term+J Upper Level
10031.16 He I 1 - 1s.3d 1D2 186104.9666893 1s.7f 13 196071.18106496
10138.42358 He I - - 1s.3p 11 186209.36494 1s.7d 1D2 196070.12838342
10311.22108 He I 2 - 1s.3p 32 185564.56192 1s.6d 3D1 195260.07720298
10311.2269 He I 2 - 1s.3p 32 185564.56192 1s.6d 3D2 195260.07173649
10311.2273 He I 2 - 1s.3p 32 185564.56192 1s.6d 3D3 195260.07135803
10311.24445 He I 2 - 1s.3p 31 185564.583895 1s.6d 3D1 195260.07720298
10311.25027 He I 2 - 1s.3p 31 185564.583895 1s.6d 3D2 195260.07173649
10311.5323 He I - - 1s.3p 30 185564.85454 1s.6d 3D1 195260.07720298
10667.66205 He I - - 1s.3p 32 185564.56192 1s.6s 3S1 194936.119697
10667.68706 He I - - 1s.3p 31 185564.583895 1s.6s 3S1 194936.119697
10829.09114 He I 35 - 1s.2s 3S1 159855.9743297 1s.2p 30 169087.8308131
10830.2501 He I 120 - 1s.2s 3S1 159855.9743297 1s.2p 31 169086.8428979
10830.33977 He I 240 - 1s.2s 3S1 159855.9743297 1s.2p 32 169086.7664725
10912.92 He I 1 - 1s.3d 3D2 186101.5486891 1s.6f 33 195262.42421684
10913.05 He I 1 - 1s.3d 3D1 186101.5928903 1s.6f 32 195262.42837301
10917.1 He I - - 1s.3d 1D2 186104.9666893 1s.6f 13 195262.43178436
  ‹   Page:

Privacy Policy | Back to interactive spectra

These tables are Public Domain/CC0 (