What is Scattering of Light and its Types?

SCATTERING OF LIGHT

  • When sunlight enters the Earth’s atmosphere, the atoms and molecules of different gases present in the atmosphere refract light in all possible directions.
  • This is called as ‘Scattering of light’.
  • In this phenomenon, the beam of light is redirected in all directions when it interacts with a particle of the medium.
  • The interacting particle of the medium is called as ‘scatterer’.

Types of scattering

  • When a beam of light, interacts with a constituent particle of the medium, it undergoes many kinds of scattering.
  • Based on the initial and final energy of the light beam, scattering can be classified as,
      1. Elastic scattering
      2. Inelastic scattering

Elastic scattering

  • If the energy of the incident beam of light and the scattered beam of light are the same, then it is called as ‘elastic scattering’.

Inelastic scattering

  • If the energy of the incident beam of light and the scattered beam of light are not the same, then it is called as ‘inelastic scattering.
  • The nature and size of the scatterer result in different types of scattering.

They are

      • Rayleigh scattering
      • Mie scattering
      • Tyndall scattering
      • Raman scattering

Rayleigh scattering

  • The scattering of sunlight by the atoms or molecules of the gases in the earth’s atmosphere is known as Rayleigh scattering.

Rayleigh’s scattering law

  • Rayleigh’s scattering law states that “The amount of scattering of light is inversely proportional to the fourth power of its wavelength”.
  • Amount of scattering ‘S’ According to this law, the shorter wavelength colours are scattered much more than the longer wavelength colours.
  • When sunlight passes through the atmosphere, the blue colour (shorter wavelength) is scattered to a greater extent than the red colour (longer wavelength). This scattering causes the sky to appear in blue colour.
  • At sunrise and sunset, the light rays from the Sun have to travel a larger distance in the atmosphere than at noon.
  • Hence, most of the blue lights are scattered away and only the red light which gets least scattered reaches us.
  • Therefore, the colour of the Sun is red at sunrise and sunset.

Mie scattering

  • Mie scattering takes place when the diameter of the scatterer is similar to or larger than the wavelength of the incident light.
  • It is also an elastic scattering. The amount of scattering is independent of wavelength.
  • Mie scattering is caused by pollen, dust, smoke, water droplets, and other particles in the lower portion of the atmosphere.
  • Mie scattering is responsible for the white appearance of the clouds.
  • When white light falls on the water drop, all the colours are equally scattered which together form the white light.

Tyndall Scattering

  • When a beam of sunlight, enters a dusty room through a window, then its path becomes visible to us.
  • This is because the tiny dust particles present in the air of the room scatter the beam of light. This is an example of Tyndall Scattering
  • The scattering of light rays by the colloidal particles in the colloidal solution is called Tyndall Scattering or Tyndall Effect.

Raman scattering

  • When a parallel beam of monochromatic (single coloured) light passes through a gas or liquid or transparent solid, a part of the light rays is scattered.
  • The scattered light contains some additional frequencies (or wavelengths) other than that of incident frequency (or wavelength).
  • This is known as Raman scattering or Raman Effect.
  • Raman Scattering is defined as “The interaction of light rays with the particles of pure liquids or transparent solids, which leads to a change in wavelength or frequency.”
  • The spectral lines having a frequency equal to the incident ray frequency are called ‘Rayleigh lines and the spectral lines which are having frequencies other than the incident ray frequency are called ‘Raman lines.
  • The lines having frequencies lower than the incident frequency are called stokes lines and the lines having frequencies higher than the incident frequency are called Antistokes lines.

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