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

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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
329.39 Ca IV - -
330.94 Ca V - -
331.44 Ca IV - -
331.99 Ca IV - -
332.53 Ca IV - -
332.81 Ca IV - -
333.44 Ca V - -
333.57 Ca V - -
334.55 Ca V - -
335.34 Ca V - -
336.55 Ca V - -
337.54 Ca V - -
338.06 Ca V - -
338.83 Ca IV - -
339.79 Ca IV - -
340.29 Ca IV - -
341.29 Ca IV - -
341.46 Ca IV - -
342.45 Ca IV - -
343.19 Ca IV - -
343.44 Ca IV - -
343.64 Ca V - -
343.93 Ca IV - -
344.96 Ca IV - -
345.13 Ca IV - -
352.92 Ca V - -
356.25 Ca V - -
357.98 Ca III 585 - 3s2.3p6 1S0 0 3s2.3p5.3d 11 279353.64
363.08 Ca X - - 2p6.4p 21/2 899290 2p6.5s 2S1/2 1174710
365.62 Ca X - - 2p6.4p 23/2 901200 2p6.5s 2S1/2 1174710
371.883 Ca IX - - 3s.3p 30 143176 3s.3d 3D1 412078
373.809 Ca IX - - 3s.3p 31 144675 3s.3d 3D2 412191
373.967 Ca IX - - 3s.3p 31 144675 3s.3d 3D1 412078
374.74 Ca IV - -
377.18 Ca V - -
378.082 Ca IX - - 3s.3p 32 147912 3s.3d 3D3 412405
378.388 Ca IX - - 3s.3p 32 147912 3s.3d 3D2 412191
378.39 Ca XVI - - 2s2.2p 23/2 36520 2s.2p2 4P5/2 300800
378.55 Ca IX - - 3s.3p 32 147912 3s.3d 3D1 412078
387.08 Ca V - -
395.024 Ca IX - - 3s.3p 11 214482 3s.3d 1D2 467631
403.724 Ca III 210 - 3s2.3p6 1S0 0 3s2.3p5.4s 11 247696.39
409.954 Ca III 120 - 3s2.3p6 1S0 0 3s2.3p5.4s 31 243930.44
411.694 Ca X - - 2p6.3p 21/2 174213 2p6.3d 2D3/2 417112
419.754 Ca X - - 2p6.3p 23/2 179287 2p6.3d 2D5/2 417522
420.477 Ca X - - 2p6.3p 23/2 179287 2p6.3d 2D3/2 417112
425. Ca V - -
432. Ca XVI - - 2s2.2p 23/2 36520 2s.2p2 4P1/2 267990
434.57 Ca IV - -
437.27 Ca IV - -
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