  Solar Coronal Heating is a Nonlinear Quantum Mechanical Phenomenon.
  Corona is a powerful source of X-rays and ionisations & emissions of such
radiations are quantum mechanical and levels are highly unstable to order of
femto-seconds. A linear method of energy transfer like collisional ionisation
to such levels is practically not feasible. We have proposed gire as the
mechanism of this problem and discussed the physics, found it as a nonlinear
process of multi photon absorption, similar to the multiple ionisation by ultra
fast laser. Here, we are discussing the energy budget for ionisations of all
the coronal elements and find gire is sufficient.
  Solar coronal heating balances the energy mass condition of the solar system,
is a classical thermodynamical problem, but done by a nonlinear quantum
mechanical process.
