KnowraFraunhofer linesLinked fromLinked fromThe 19 pages that link to Fraunhofer lines, each with the reason it gives.All 19Broader topic 5Related 11Compared with 3Spectral lineBroader topic: Their pattern established that elements in the Sun imprint identifiable lines.Astronomical spectroscopyBroader topic: Their systematic study established that solar light contains a rich pattern of spectral features.Gustav KirchhoffRelated: Kirchhoff interpreted these previously mapped lines as absorption features caused by elements in the Sun.Atomic spectroscopyBroader topic: Their patterns helped connect atomic absorption to the spectrum of sunlight.Balmer seriesCompared with: They are absorption features, whereas Balmer lines can appear in either emission or absorption.Hydrogen spectral seriesCompared with: Their absorption pattern contrasts with the bright emission lines used to identify hydrogen series.Fraunhofer diffractionCompared with: The shared name can mislead: these spectral lines are not far-field diffraction patterns.Kirchhoff's laws of spectroscopyRelated: Kirchhoff explained these solar lines as absorption by cooler gas in the Sun's atmosphere.Solar spectrumBroader topic: They are the spectrum’s distinctive dark features, created when atoms absorb particular wavelengths.SpectroscopeRelated: Their precise positions showed that a spectrum contains more than a continuous spread of colors.Anders Jonas ÅngströmRelated: Ångström measured solar lines and compared them with laboratory spectra.Hydrogen-alphaRelated: The early cataloguing of solar lines provided a foundation for identifying spectral features.Joseph von FraunhoferBroader topic: These named lines are the best-known result of his systematic solar measurements.Norman LockyerRelated: Their established pattern provided the spectral background against which Lockyer recognized a new line.PhotosphereRelated: Many of these lines form in the photosphere and reveal its composition and motion.Abbe numberRelated: The standard Abbe number uses refractive indices at three designated Fraunhofer lines.William HugginsRelated: The comparison of stellar and solar lines connected Huggins’s observations to established spectroscopy.Heinrich KayserRelated: Comparing stellar and solar lines made spectroscopy a tool for studying celestial matter.Johann Wilhelm RitterRelated: Precise study of the spectrum formed the wider experimental setting for Ritter’s work.
KnowraFraunhofer linesLinked fromLinked fromThe 19 pages that link to Fraunhofer lines, each with the reason it gives.All 19Broader topic 5Related 11Compared with 3Spectral lineBroader topic: Their pattern established that elements in the Sun imprint identifiable lines.Astronomical spectroscopyBroader topic: Their systematic study established that solar light contains a rich pattern of spectral features.Gustav KirchhoffRelated: Kirchhoff interpreted these previously mapped lines as absorption features caused by elements in the Sun.Atomic spectroscopyBroader topic: Their patterns helped connect atomic absorption to the spectrum of sunlight.Balmer seriesCompared with: They are absorption features, whereas Balmer lines can appear in either emission or absorption.Hydrogen spectral seriesCompared with: Their absorption pattern contrasts with the bright emission lines used to identify hydrogen series.Fraunhofer diffractionCompared with: The shared name can mislead: these spectral lines are not far-field diffraction patterns.Kirchhoff's laws of spectroscopyRelated: Kirchhoff explained these solar lines as absorption by cooler gas in the Sun's atmosphere.Solar spectrumBroader topic: They are the spectrum’s distinctive dark features, created when atoms absorb particular wavelengths.SpectroscopeRelated: Their precise positions showed that a spectrum contains more than a continuous spread of colors.Anders Jonas ÅngströmRelated: Ångström measured solar lines and compared them with laboratory spectra.Hydrogen-alphaRelated: The early cataloguing of solar lines provided a foundation for identifying spectral features.Joseph von FraunhoferBroader topic: These named lines are the best-known result of his systematic solar measurements.Norman LockyerRelated: Their established pattern provided the spectral background against which Lockyer recognized a new line.PhotosphereRelated: Many of these lines form in the photosphere and reveal its composition and motion.Abbe numberRelated: The standard Abbe number uses refractive indices at three designated Fraunhofer lines.William HugginsRelated: The comparison of stellar and solar lines connected Huggins’s observations to established spectroscopy.Heinrich KayserRelated: Comparing stellar and solar lines made spectroscopy a tool for studying celestial matter.Johann Wilhelm RitterRelated: Precise study of the spectrum formed the wider experimental setting for Ritter’s work.