Physical properties of giant planets
The chemical identification and physical nature of giant planets are discussed. The phase equilibria of H2-He mixture is briefly described for these large planets.
Engineering topics
Publications and source records attributed to Wildt, R..
The chemical identification and physical nature of giant planets are discussed. The phase equilibria of H2-He mixture is briefly described for these large planets.
Investigations of deviations in local thermodynamic equilibrium in stellar atmospheres are summarized. Included are studies in gray and AO star atmospheres.
A theoretical discussion of the composition of the major planets is presented. A simplistic physical model of the giant planets is described. The conclusions of several theoretical explanations of the planetary structure are explained. Curves are developed to show the mass-radius relation for zero temperature spheres of various chemical compositions. The density of isothermal atmospheres of hydrogen as a function of the elevation above a surface of solid hydrogen.
Radiation equilibrium in atmosphere with constant Einstein absorption coefficient
Entropy defect and source function in gray atmosphere thermodynamics
Unattainability of detailed balancing in thermodynamic equilibrium of gray atmosphere
Hopf analytical solution for values of ratio of gray absorption coefficients for insolating and escaping radiation /greenhouse parameter/ assumed constant at all depths, presenting temperature distribution graphs
Hopf analytical solution for greenhouse parameter in gray planetary atmosphere
Radiative transfer inside gray atmosphere in strict equilibrium shows similarity transformation exists
Internal structure, composition, and conditions of planets