The spectral resolution can also be expressed in terms of physical quantities, such as velocity; then it describes the difference between velocities Δ v {\displaystyle \Delta v} that can be distinguished through the Doppler effect. Then, the resolution is Δ v {\displaystyle \Delta v} and the resolving power is R = c Δ v , {\displaystyle R={\frac {c}{\Delta v}},} where c {\displaystyle c} is the speed of light. The STIS example above then has a spectral resolution of 51 km/s.
IUPAC defines resolution in optical spectroscopy as the minimum wavenumber, wavelength or frequency difference between two lines in a spectrum that can be distinguished.2 Resolving power, R, is given by the transition wavenumber, wavelength or frequency, divided by the resolution.3
- CRIRES Instrument page at ESO http://www.eso.org/instruments/crires/ ↩
IUPAC, Compendium of Chemical Terminology, 2nd ed. (the "Gold Book") (1997). Online corrected version: (2006–) "resolution in optical spectroscopy". doi:10.1351/goldbook.R05319 /wiki/International_Union_of_Pure_and_Applied_Chemistry ↩
IUPAC, Compendium of Chemical Terminology, 2nd ed. (the "Gold Book") (1997). Online corrected version: (2006–) "resolving power, R, in optical spectroscopy". doi:10.1351/goldbook.R05322 /wiki/International_Union_of_Pure_and_Applied_Chemistry ↩