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Strong spectral lines of the elements

The strongest emission lines of 99 elements, from hydrogen to einsteinium, as tabulated in NIST's Handbook of Basic Atomic Spectroscopic Data. One row per spectral line: element, ion stage, wavelength, relative intensity and whether it is a persistent line.

11,980 rows13 columns Updated 19 h ago Facts (not copyrightable) — source credited
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Columns

Stable keys — use them in the API, SQL and code

KeyNameTypeDescription
line_idIDstringSpectrum, medium and wavelength.
atomic_numberAtomic numberinteger—
elementElementstring—
symbolSymbolstring—
spectrumSpectrumstringElement and ion stage in spectroscopic notation: Fe I is neutral iron, Fe II singly ionized iron.
ion_stageIon stageinteger1 = neutral atom (I), 2 = singly ionized (II), and so on.
wavelength_angstromWavelength (Å)number · ÅWavelength as given by NIST, in ångströms.
wavelength_nmWavelengthnumber · nmWavelength in nanometres (Å ÷ 10).
mediumMediumstringWhether the wavelength is measured in vacuum or standard air.
intensityRelative intensitynumberRelative intensity on the element's own scale.
persistentPersistent linebooleanNIST marks this as a persistent line (P).
intensity_marksIntensity marksstringOther NIST intensity codes for the line, if any.
referenceReferencestringNIST Handbook bibliography code for the wavelength.

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