Linked from

The 22 pages that link to Atomic spectrum, each with the reason it gives.

• Niels BohrRelated: Hydrogen’s spectral lines gave Bohr’s model its key empirical test.

• Pauli exclusion principleRelated: Unexplained spectral patterns motivated Pauli's proposal.

• Werner HeisenbergRelated: Measured spectral lines supplied the observable data that matrix mechanics was built to explain.

• Matrix mechanicsRelated: Spectral lines supplied the observable data Heisenberg used to build the theory.

• Doppler spectroscopyRelated: Stable atomic features provide identifiable reference lines for measuring shifts.

• Correspondence principleRelated: Bohr used spectral lines to connect quantized transitions with classical frequencies.

• Rydberg constantRelated: Hydrogen-like spectra reveal the regular spacing governed by the constant.

• Valence shellRelated: Transitions involving outer-shell electrons produce many visible spectral lines.

• Pieter ZeemanRelated: The regularity of atomic spectra made line splitting detectable.

• Kramers' theoremRelated: Atomic level structure provided the setting for Kramers' analysis.

• Theodor W. HänschRelated: Hänsch’s spectroscopy measured these signatures to test atomic theory.

• Atomic propertiesRelated: Spectral lines reveal discrete atomic energy levels and identify elements.

• QuantumRelated: Sharp spectral lines provided evidence that atomic energies take discrete values.