The classical, → non-relativistic scattering of photons by free
charged particles. When an electromagnetic wave is incident on a charged particle, the
electric and magnetic components of the wave exert a force on
the particle, setting it into motion. As it accelerates, it in turn radiates
in all directions. Such scattering is independent of wavelength
and equal numbers of photons are scattered forward and backward.
Thomson scattering occurs in stellar atmospheres and in any non-relativistic
→ plasma.
Thomson scattering is normally taken as the minimum → opacity.
See also: → Thomson; → scattering.