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
320.2926 He I 30 - 1s.2p 32 169086.7664725 2p2 3P0,1,2 481301.5
505.61 He I 10 - 1s2 1S0 0 1s.15p 11 197823.79
505.75 He I 15 - 1s2 1S0 0 1s.14p 11 197751.82
505.9 He I 20 - 1s2 1S0 0 1s.13p 11 197662.63
506.31 He I 25 - 1s2 1S0 0 1s.12p 11 197550.24
506.56 He I 40 - 1s2 1S0 0 1s.11p 11 197405.87
507.08 He I 55 - 1s2 1S0 0 1s.10p 11 197216.0895622
507.71 He I 80 - 1s2 1S0 0 1s.9p 11 196959.692816
508.63 He I 105 - 1s2 1S0 0 1s.8p 11 196601.400247
509.97 He I 135 - 1s2 1S0 0 1s.7p 11 196079.0875698
512.07 He I 195 - 1s2 1S0 0 1s.6p 11 195274.908466
515.596 He I 270 - 1s2 1S0 0 1s.5p 11 193942.462294
522.186 He I 555 - 1s2 1S0 0 1s.4p 11 191492.711909
537.0293 He I 2500 - 1s2 1S0 0 1s.3p 11 186209.36494
584.3339 He I 10000 - 1s2 1S0 0 1s.2p 11 171134.896946
591.4121 He I 555 - 1s2 1S0 0 1s.2p 31 169086.8428979
Page:
1

Privacy Policy | Back to interactive spectra

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