Solar Coronal Heating by Gravity-Induced Resonant Emission

Abstract

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.