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
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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
373.45	Cu	IIVIII	-	-	1s.2s	3S1	67035380	1s.2p	3P°0	67303150
374.4	Cu	IV	-	-
377.76	Cu	V	-	-
385.06	Cu	XXIX	-	-	2s	2S1/2	69902760	2p	2P°3/2	70162460
387.	Cu	XVII	-	-	3s2.3p	2P°3/2	33239	3s.3p2	4P3/2	291810
387.4	Cu	V	-	-
387.56	Cu	XVI	-	-	3s2.3p2	3P1	18596.7	3s.3p3	5S°2	276430
395.67	Cu	IVIII	-	-	3s.3p	1P°1	426987	3p2	1D2	679710
396.06	Cu	V	-	-
405.24	Cu	IV	-	-
406.45	Cu	IV	-	-
406.94	Cu	V	-	-
410.46	Cu	XVI	-	-	3s2.3p2	3P2	32730	3s.3p3	5S°2	276430
410.6	Cu	XVII	-	-	3s2.3p	2P°3/2	33239	3s.3p2	4P1/2	277231
413.45	Cu	IV	-	-
414.1	Cu	XXIV	-	-	2s2.2p2	3P1	132120	2s2.2p2	1D2	373620
420.	Cu	XXII	-	-	2s2.2p4	3P2	0	2s2.2p4	1D2	237950
430.44	Cu	IVIII	-	-	3s.3d	1D2	917020	3p.3d	1D°2	1149319
434.8	Cu	IIIII	-	-	2s2.2p3	4S°3/2	0	2s2.2p3	2D°5/2	230070
443.68	Cu	IV	-	-
451.16	Cu	IV	-	-
463.72	Cu	IV	-	-
484.142	Cu	XXVII	-	-	1s2.2p	2P°1/2	444861	1s2.2p	2P°3/2	651412
484.53	Cu	IV	-	-
497.	Cu	IV	-	-
504.6	Cu	IV	-	-
509.38	Cu	IV	-	-
519.51	Cu	IV	-	-
522.8	Cu	XXV	-	-	2s2.2p	2P°1/2	0	2s2.2p	2P°3/2	191280
540.	Cu	XXIV	-	-	2s2.2p2	3P2	188430	2s2.2p2	1D2	373620
540.65	Cu	IV	-	-
542.9	Cu	III	-	-
550.92	Cu	IV	-	-
584.85	Cu	IV	-	-
585.	Cu	IIIII	-	-	2s2.2p3	4S°3/2	0	2s2.2p3	2D°3/2	170860
592.3	Cu	XXI	-	-	2s2.2p5	2P°3/2	0	2s2.2p5	2P°1/2	168830
615.67	Cu	III	-	-
616.03	Cu	III	-	-
648.	Cu	XXVI	-	-	1s2.2s.2p	3P°1	438970	1s2.2s.2p	3P°2	593290
657.7	Cu	XXII	-	-	2s2.2p4	3P2	0	2s2.2p4	3P1	151990
675.5994	Cu	II	70	-	3d10	1S0	0	3d9.(2D3/2).5f	2[3/2]°1	148016.157
677.675	Cu	II	30	-	3d10	1S0	0	3d9.(2D5/2).7p	2[3/2]°1	147562.672
685.1377	Cu	II	210	-	3d10	1S0	0	3d9.(2D5/2).5f	2[3/2]°1	145955.447
685.3922	Cu	II	40	-	3d10	1S0	0	3d9.(2D5/2).5f	2[1/2]°1	145900.904
687.98	Cu	III	-	-
709.3098	Cu	II	195	-	3d10	1S0	0	3d9.(2D3/2).6p	2[1/2]°1	140981.51
715.53	Cu	III	-	-
718.1766	Cu	II	225	-	3d10	1S0	0	3d9.(2D5/2).6p	2[3/2]°1	139241.13
724.4881	Cu	II	330	-	3d10	1S0	0	3d9.(2D3/2).4f	2[3/2]°1	138028.384
725.	Cu	IIVIII	-	-	1s.3s	3S1	79453200	1s.3p	3P°2	79591200

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