Analytical lines for atomic spectroscopy

Resonance lines used in flame emission and atomic absorption: excitation energy, the excited fraction at 2500 K (air–acetylene flame) and 6000 K (ICP), and the Doppler width at 2500 K — all computed from the line wavelength.

9 rows
Na589.3003s ²S₁/₂ – 3p ²P (D₁ 589.592, D₂ 588.995)2.1041.72 × 10⁻⁴0.05134.40flame emission (flame photometer), AAS
K767.6004s ²S₁/₂ – 4p ²P (766.490, 769.896)1.6150.001660.1324.40flame emission, AAS
Li670.7802s ²S₁/₂ – 2p ²P (670.776, 670.791)1.8485.64 × 10⁻⁴0.08419.12flame emission (lithium therapy monitoring)
Ca422.6734s² ¹S₀ – 4s4p ¹P₁2.9333.66 × 10⁻⁶0.01032.39AAS (lanthanum added against phosphate)
Mg285.2133s² ¹S₀ – 3s3p ¹P₁4.3475.17 × 10⁻⁹6.69 × 10⁻⁴2.07AAS
Cu324.7544s ²S₁/₂ – 4p ²P₃/₂3.8184.02 × 10⁻⁸0.001241.46AAS
Zn213.8574s² ¹S₀ – 4s4p ¹P₁5.7986.16 × 10⁻¹²4.05 × 10⁻⁵0.95AAS (emission is hopeless)
Cd228.8025s² ¹S₀ – 5s5p ¹P₁5.4193.57 × 10⁻¹¹8.42 × 10⁻⁵0.77AAS, graphite furnace
Pb283.3056p² ³P₀ – 6p7s ³P₁4.3764.52 × 10⁻⁹6.33 × 10⁻⁴0.70AAS, graphite furnace

Excited fraction N₁/N₀ = (g₁/g₀)e^(−ΔE/kT); for the alkali doublets the whole ²P term (g = 6) is counted against the ²S ground state (g = 2). It assumes local thermal equilibrium and ignores ionisation.

Sources

  1. NIST Atomic Spectra Database, ver. 5.11 (A. Kramida, Yu. Ralchenko, J. Reader and NIST ASD Team), wavelengths and level assignments.
  2. D. A. Skoog, F. J. Holler, S. R. Crouch, Principles of Instrumental Analysis, 7th ed. (2018), ch. 8–10 (Boltzmann distribution, flames and plasmas).

Used in these lessons