College Physics I – Introduction

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Rayleigh Scattering

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College Physics I – Introduction

Definition

Rayleigh scattering is a physical phenomenon in which light is scattered by particles much smaller than the wavelength of the light. This type of scattering is responsible for the blue color of the sky and the reddish appearance of the sun during sunrises and sunsets.

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5 Must Know Facts For Your Next Test

  1. Rayleigh scattering is inversely proportional to the fourth power of the wavelength of the light, meaning that shorter wavelengths (such as blue) are scattered more strongly than longer wavelengths (such as red).
  2. The intensity of Rayleigh scattering is also proportional to the square of the size of the scattering particles, which is why it is most effective for particles much smaller than the wavelength of the light.
  3. Rayleigh scattering is the primary reason why the sky appears blue during the day, as the shorter wavelengths of visible light (blue) are scattered more strongly by the molecules in the atmosphere.
  4. The reddish appearance of the sun during sunrises and sunsets is also due to Rayleigh scattering, as the longer wavelengths of light (red) are less scattered and can pass through the atmosphere more easily.
  5. Polarization is an important aspect of Rayleigh scattering, as the scattered light is partially polarized perpendicular to the direction of the incident light.

Review Questions

  • Explain how Rayleigh scattering is responsible for the blue color of the sky.
    • Rayleigh scattering is the primary reason why the sky appears blue during the day. This phenomenon occurs because the shorter wavelengths of visible light (blue) are scattered more strongly by the molecules in the atmosphere than the longer wavelengths (red and yellow). As the sunlight passes through the atmosphere, the blue wavelengths are scattered in all directions, creating the blue hue we see in the sky. This scattering is inversely proportional to the fourth power of the wavelength, meaning that the shorter blue wavelengths are scattered much more than the longer red wavelengths.
  • Describe the relationship between Rayleigh scattering and the polarization of light.
    • Rayleigh scattering is closely related to the polarization of light. When light is scattered by particles much smaller than the wavelength, the scattered light becomes partially polarized perpendicular to the direction of the incident light. This is because the electric field of the incident light induces oscillations in the small particles, which then emit scattered light with a specific polarization. The degree of polarization of the scattered light depends on the angle of observation, with the maximum polarization occurring at angles perpendicular to the direction of the incident light. This relationship between Rayleigh scattering and polarization is an important concept in the study of the behavior of light in the atmosphere and other media.
  • Analyze the role of Rayleigh scattering in the reddish appearance of the sun during sunrises and sunsets.
    • The reddish appearance of the sun during sunrises and sunsets is also a consequence of Rayleigh scattering. As the sun's light passes through a greater thickness of the atmosphere near the horizon, the shorter wavelengths (blue and green) are scattered more strongly by the molecules in the air, leaving the longer wavelengths (red and orange) to predominate. This is because Rayleigh scattering is inversely proportional to the fourth power of the wavelength, meaning that the blue and green wavelengths are scattered much more than the red wavelengths. As a result, the sun appears reddish or orangish during these times of day, as the longer wavelengths of light are able to pass through the atmosphere more easily and reach our eyes. This phenomenon is a striking visual demonstration of the wavelength-dependent nature of Rayleigh scattering.
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