Linked from

The 23 pages that link to Absorption spectroscopy, each with the reason it gives.

• SpectroscopyRelated: It is one of the central ways spectra are collected and interpreted.

• FluorescenceRelated: It characterizes the excitation wavelengths that can initiate fluorescence.

• PhotochemistryRelated: Absorption spectra identify the wavelengths capable of exciting a molecule.

• Molecular spectroscopyRelated: It is one of the three principal radiation–molecule interactions encompassed here.

• DyeRelated: Absorption spectra help characterize a dye’s color and molecular transitions.

• Atomic spectroscopyRelated: Atoms absorb selected wavelengths when incident photons match energy gaps.

• PhotolysisRelated: Absorption spectra identify wavelengths capable of initiating photolysis.

• Excited stateRelated: Its spectral lines reveal energy gaps leading to excited states.

• Quantum yieldRelated: Absorbed-photon counts are needed to determine a yield rather than an incident-light ratio.

• Laser spectroscopyRelated: Laser absorption reveals transitions when a tunable beam passes through a sample.

• Doppler spectroscopyRelated: Many stellar Doppler measurements track absorption lines imprinted on a continuous spectrum.

• Galactic windRelated: Blueshifted absorption features can reveal gas flowing toward the observer.

• DichroismRelated: Polarization-resolved absorption measurements reveal dichroism.

• Bromothymol blueRelated: Spectral measurements can quantify bromothymol blue’s color and concentration.

• Optical spectrometerRelated: An optical spectrum can reveal absorption features imposed by a sample.

• Composition of astronomical objectsRelated: Starlight passing through a planet's atmosphere can acquire absorption features from its gases.