KnowraSolar spectrumLinked fromLinked fromThe 9 pages that link to Solar spectrum, each with the reason it gives.All 9Broader topic 2Related 7Gustav KirchhoffBroader topic: Kirchhoff explained the dark Fraunhofer lines as absorption by cooler gas in the Sun’s atmosphere.Spectral power distributionRelated: Absorption dips in the solar SPD motivated D-series illuminant definitions.Solar radiationBroader topic: It shows which wavelengths carry solar energy and how much each contributes.William Hyde WollastonRelated: Wollaston described dark lines in sunlight before Fraunhofer mapped them in detail.Joseph von FraunhoferRelated: Fraunhofer’s careful examination revealed the dark lines embedded in sunlight’s continuous spectrum.ChromosphereRelated: Chromospheric emission and absorption lines appear within the solar spectrum.SunlightRelated: Its wavelength bands distinguish ultraviolet, visible, and infrared sunlight.Diffuse sky radiationRelated: Wavelength-dependent scattering gives diffuse sky radiation its characteristic spectral composition.Sky blueRelated: The Sun supplies the visible wavelengths that the atmosphere scatters into the blue sky.