Fraunhofer lines

E556416

Fraunhofer lines are the dark absorption lines observed in the solar spectrum that reveal the presence and properties of elements in the Sun’s atmosphere and intervening gases.

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Statements (52)

Predicate Object
instanceOf absorption lines
solar spectral features
spectral lines
appearAs dark lines on a continuous spectrum
associatedElement calcium
helium
hydrogen
iron
magnesium
nitrogen
oxygen
sodium
causedBy absorption of light by atoms in the Earth’s atmosphere
absorption of light by atoms in the solar atmosphere
discoveredBy Joseph von Fraunhofer NERFINISHED
discoveryYear 1814
fieldOfStudy astrophysics
solar physics
spectroscopy
namedAfter Joseph von Fraunhofer NERFINISHED
notableExample Fraunhofer A line NERFINISHED
Fraunhofer B line NERFINISHED
Fraunhofer C line NERFINISHED
Fraunhofer D lines NERFINISHED
Fraunhofer E line NERFINISHED
Fraunhofer F line NERFINISHED
Fraunhofer G line NERFINISHED
Fraunhofer H line NERFINISHED
Fraunhofer K line NERFINISHED
numberOfIdentifiedLines hundreds
observedIn daylight spectrum
solar spectrum
stellar spectra
physicalOrigin atomic absorption of specific wavelengths
relatedConcept Kirchhoff’s laws of spectroscopy NERFINISHED
absorption spectrum
emission lines
spectralRegion near infrared
near ultraviolet
visible light
usedFor calibration of spectrographs
determination of solar atmospheric composition
determination of solar atmospheric pressure
determination of solar atmospheric temperature structure
determination of solar rotation
identification of chemical elements in stars
identification of chemical elements in the Sun
measurement of magnetic fields via Zeeman effect
measurement of radial velocities via Doppler shift
measurement of stellar surface gravities
measurement of stellar temperatures
study of interstellar medium absorption

Referenced by (2)

Full triples — surface form annotated when it differs from this entity's canonical label.

Joseph von Fraunhofer knownFor Fraunhofer lines
Joseph von Fraunhofer hasEponym Fraunhofer lines