This results in an intense outward energy flux that can not be sustained by radiative transfer.
His research interests are in cloud physics, atmospheric chemistry and radiative transfer.
He is an author of about 100 articles mostly on atmospheric optics, radiative transfer, and light scattering.
The equation of radiative transfer describes the way in which radiation is affected as it travels through a material medium.
The differential form of the equation for radiative transfer is:
Solutions to the equation of radiative transfer form an enormous body of work.
This makes radiative transfer of energy within the transition region very complicated.
It is often used to model radiative transfer, particularly in stellar atmospheres.
Such models are based on physical principles including fluid dynamics, thermodynamics and radiative transfer.
Instead the models predict how greenhouse gases will interact with radiative transfer and other physical processes.