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File:24.05.2025 scattering psc.jpg

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    Captions

    Captions

    Sunset with sky colors due to the diffusion or scattering of light, radiation-matter interaction. High-frequency scattering for indigo (short wavelength), low-frequency scattering for orange (long wavelength).

    Summary

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    Description
    Italiano: I colori del cielo al tramonto originano dal fenomeno della diffusione o scattering di Rayleigh della luce solare, sorgente incoerente e naturale, da parte delle molecole dell’atmosfera terrestre (interazione radiazione-materia). Le lunghezze d’onda corte (violetto/blu) vengono diffuse più intensamente per scattering ad alta frequenza, rendendo il cielo azzurro durante il giorno. Al tramonto, la luce attraversa uno strato più spesso di atmosfera: le lunghezze d’onda corte vengono disperse e prevalgono le lunghezze d’onda lunghe (rosso/arancione) come scattering a bassa frequenza, che conferiscono al cielo i colori caldi tipici.
    English: The colors of the sky at sunset arise from the phenomenon of Rayleigh scattering of sunlight, an incoherent and natural source, by molecules in the Earth's atmosphere (radiation-matter interaction). Short wavelengths (violet/blue) are scattered more intensely by high-frequency scattering, making the sky blue during the day. At sunset, the light passes through a thicker layer of atmosphere: the short wavelengths are scattered, and long wavelengths (red/orange) prevail as low-frequency scattering, giving the sky its characteristic warm colors.
    Date
    Source Own work
    Author Pia Simona Cervello

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    Date/TimeThumbnailDimensionsUserComment
    current14:02, 24 November 2025Thumbnail for version as of 14:02, 24 November 20252,040 × 1,530 (140 KB)Pia Simona Cervello (talk | contribs)Uploaded own work with UploadWizard

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