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
Download CSV

  |««     «     ‹   Page:   ›     »»|  
λ, Å E. Sp.# Rel.Int. EVB Lower Config Lower Term+J Lower Level Upper Config Upper Term+J Upper Level
5974.72 Hf I 120 98
5978.66 Hf I 330 262
5992.96 Hf I 120 102
6016.79 Hf I 540 417
6054.17 Hf I 555 417
6098.67 Hf I 540 380
6185.13 Hf I 675 409
6210.7 Hf I 345 205
6216.82 Hf I 240 140
6238.58 Hf I 135 76
6248.95 Hf II 480 269
6299.54 Hf I 150 78
6311.85 Hf I 150 76
6318.33 Hf I 95 46
6338.1 Hf I 135 61
6380.19 Hf I 70 29
6386.23 Hf I 210 90
6409.52 Hf I 50 19
6556.5 Hf I 45 12
6587.23 Hf I 50 13
6644.6 Hf II 660 139
6647.06 Hf II 285 58
6659.4 Hf I 15 3
6713.48 Hf I 390 67
6754.61 Hf II 660 97
6769.95 Hf I 135 19
6789.27 Hf I 795 101
6818.94 Hf I 1000 124
6826.56 Hf I 135 15
6850.07 Hf I 450 46
6858.7 Hf I 375 36
6911.4 Hf I 840 67
6926.19 Hf I 375 27
6979.59 Hf I 30 2
6980.91 Hf II 300 17
7019.25 Hf I 40 2
7030.33 Hf II 600 28
7035.13 Hf I 40 2
7061.9 Hf I 105 4
7062.87 Hf I 50 2
7063.83 Hf I 345 14
7094.4 Hf I 50 2
7100.54 Hf I 50 2
7119.52 Hf I 165 5
7131.81 Hf I 870 25
7237.1 Hf I 1000 16 5d2.6s2 a 3F4 4567.64 5d2.6s.(b 2D).6p z 3D°3 18381.49
7240.87 Hf I 810 12
7262.62 Hf I 20 -
7267.58 Hf IV 35 -
7320.05 Hf I 225 2
  |««     «     ‹   Page:   ›     »»|  
13

Privacy Policy | Back to interactive spectra

These tables are Public Domain/CC0 (https://creativecommons.org/publicdomain/zero/1.0/).