The Model Atmospheric Principia Scientific （大气科学原理模型）.pdf

The Model Atmospheric Greenhouse Effect Joseph E. Postma, M.Sc. Astrophysics July 22, 2011 An Original Publication of Principia Scientific International Abstract: We develop and describe the standard model of the atmospheric radiative greenhouse effect. This is a model whose boundary conditions are widely accepted in creating the paradigm, and setting the starting point, for increasing model complexity, and is almost universally utilized amongst various research and educational institutions. It will be shown that the boundary conditions of the standard radiative atmospheric greenhouse are unjustified, unphysical, and fictional, and it will also be demonstrated that physically real boundary conditions cannot even truly be described by such a model. A new starting-point model is introduced with physically accurate boundary conditions, and this will be understood to physically negate the requirement for a postulation of a radiative atmospheric greenhouse effect. 1 The Standard Model Earth’s Radiative Equilibrium The standard, and generally only known approach, for determining Earth’s radiative equilibrium with the Sun, begins with the application of the principle of conservation of energy via several applications of the Stefan-Boltzmann law. The total solar energy absorbed by the Earth must be equal to the energy emitted by the Earth, over the long-term average assuming radiative thermal equilibrium, and assuming there are no significant terrestrial sources of energy. Additional output energy from geothermal sources and the addition of energy into the atmosphere via Coriolis forces due to the rotation of the Earth are assumed to be small compared to the solar energy.