Linked from

The 16 pages that link to Atomic emission spectrum, each with the reason it gives.

• AuroraRelated: Excited atmospheric gases emit the distinctive wavelengths seen in auroral colors.

• Electron shellRelated: Transitions between shell-associated states produce characteristic spectral lines.

• Flame testRelated: Each observed flame color corresponds to emitted wavelengths in an element's spectrum.

• Atomic theoryRelated: Distinct spectral lines reveal quantized energy changes within atoms.

• Rydberg formulaNarrower topic: The formula predicts positions of lines within this broader kind of spectrum.

• Balmer seriesNarrower topic: The Balmer series is one element-specific part of this broader phenomenon.

• Hydrogen spectral seriesNarrower topic: Hydrogen's series are organized parts of its broader emission spectrum.

• Rutherford modelRelated: The model could not explain why atoms emit discrete spectral lines rather than continuous radiation.

• FireworksRelated: Characteristic atomic emissions help explain why different elements produce different flame colors.

• Hydrogen spectrumCompared with: Emission lines are one half of the spectrum’s definition; absorption lines arise from upward transitions.

• XenonRelated: Xenon’s many emission lines produce the distinctive light from its discharge lamps.

• Franck–Hertz experimentCompared with: Spectral lines reveal energy differences through photons, unlike Franck–Hertz’s electron collisions.

• NeonRelated: Neon’s reddish-orange glow consists of discrete wavelengths from transitions between atomic energy levels.

• Paul Émile Lecoq de BoisbaudranBroader topic: The element’s characteristic emission pattern served as a distinct analytical fingerprint.

• Atomic emission spectroscopyBroader topic: Its element-specific lines are the direct signal used for identification.

• Heinrich KayserBroader topic: Kayser and Runge catalogued element-specific line patterns in these spectra.