Astrophysics – Exploring the Origin of Sunlight

astrophysicselectromagnetic-radiationstarssunthermal-radiation

The Sunlight is an electromagnetic radiation.

Is it known what is the origin of this radiation? Can it be adequately described by classical electrodynamics (Maxwell's equations) as a motion of electric charges in the Sun? Is it necessary to take into account quantum effects described by quantum electrodynamics? Or is it necessary to take into account other processes?

Best Answer

The light from the Sun comes from the photosphere; a relatively thin layer, a few hundred km thick.

The photosphere of the Sun is in radiative equilibrium, getting neither hotter or colder on average. What this means is that the emission processes that produce the radiation that escapes from the photosphere, are the inverse of the absorption processes that stop radiation from deeper, hotter layers reaching us.

The dominant continuum process is bound-free photoionisation of H$^{-}$ ions that form when hydrogen atoms capture electrons released from the ionisation of potassium and sodium atoms in the atmosphere. There are some other bound-free photoionisation processes of other species that contribute continuum opacity, and bound-bound transitions between energy levels in a variety of atoms and ions that contribute opacities at discrete wavelengths.

The principle of detailed balance means that these absorption processes are balanced by free-bound photorecombination of H$^-$ ions contributing light over a continuum of wavelengths and bound-bound downward transitions in atoms and ions at specific wavelengths.

The understanding of these processes certainly requires quantum physics and cannot be described by classical electromagnetism.