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
4127.8 Hf II 495 47
4145.76 Hf I 615 83
4162.36 Hf II 405 64
4162.69 Hf I 390 62
4174.34 Hf I 330 62 5d2.6s2 a 3F3 2356.68 5d2.6s.(a 4F).6p z 53 26305.78
4190.95 Hf I 435 106
4206.58 Hf II 990 299
4209.7 Hf I 495 151
4228.08 Hf I 150 54
4232.44 Hf II 375 132
4260.98 Hf I 615 254
4263.39 Hf I 615 256
4272.85 Hf II 645 277
4294.79 Hf I 1000 543
4318.14 Hf I 315 145
4330.27 Hf I 210 100
4336.66 Hf II 750 353
4350.51 Hf II 495 231
4356.33 Hf I 555 265
4367.9 Hf II 1500 675
4370.97 Hf II 2500 1271
4417.35 Hf II 720 342
4417.91 Hf I 360 171
4438.04 Hf I 1000 562
4457.34 Hf I 300 141
4461.18 Hf I 285 135
4540.93 Hf I 915 454
4565.94 Hf I 1500 700
4598.8 Hf I 390 201
4620.86 Hf I 735 396
4655.19 Hf I 990 556
4699.01 Hf I 615 356
4782.74 Hf I 1000 658
4800.5 Hf I 1005 651
4859.24 Hf I 435 303
4975.25 Hf I 540 419
5018.2 Hf I 270 213
5021.75 Hf I 55 42
5040.82 Hf II 2000 1682
5047.45 Hf I 195 153
5079.65 Hf II 2000 1480
5112.13 Hf I 435 367
5128.53 Hf II 1000 861
5157.96 Hf I 450 388
5167.42 Hf I 105 91
5170.18 Hf I 330 284
5181.86 Hf I 645 568
5186.84 Hf I 85 77
5187.75 Hf II 630 561
5243.99 Hf I 165 154
  |««     «     ‹   Page:   ›     »»|  
11

Privacy Policy | Back to interactive spectra

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