| 11. | The effect of Rayleigh scattering on skyglow is very small.
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| 12. | Lastly, there is a clear wavelength dependence in Rayleigh scattering.
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| 13. | Averaging this over all angles gives the Rayleigh scattering cross-section
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| 14. | This type of scattering is known as Rayleigh scattering.
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| 15. | Thus, there is not enough light to undergo Rayleigh scattering and make the sky blue.
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| 16. | It has been interpreted as Rayleigh scattering from a cloud of fine particles around it.
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| 17. | Gratings lose power into the other orders while prisms lose power due to Rayleigh scattering.
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| 18. | Rayleigh scattering is a spectroscopic scattering phenomenon that accounts for the color of the sky.
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| 19. | See : Rayleigh scattering and diffuse sky radiation.
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| 20. | In 1910 Albert Einstein showed that the link between critical opalescence and Rayleigh scattering is quantitative.
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