Radiative equilibrium is the condition where the total thermal radiation leaving an object is equal to the total thermal radiation entering it. It is one of the several requirements for thermodynamic equilibrium, but it can occur in the absence of thermodynamic equilibrium. There are various types of radiative equilibrium, which is itself a kind of dynamic equilibrium.
and 25 Related for: Radiative equilibrium information
Radiativeequilibrium is the condition where the total thermal radiation leaving an object is equal to the total thermal radiation entering it. It is...
solely radiative connection, no matter how far apart, or what partially obstructive, reflective, or refractive, obstacles lie in their path of radiative exchange...
The planetary equilibrium temperature is a theoretical temperature that a planet would be if it were in radiativeequilibrium, typically under the assumption...
scattering processes. The equation of radiative transfer describes these interactions mathematically. Equations of radiative transfer have application in a wide...
radiative-dynamical equilibrium." Instantaneous radiative forcing: "if no change in stratospheric temperature is accounted for". Effective radiative forcing:...
monochromatic radiativeequilibrium, Monthly Notices of the Royal Astronomical Society, 88: 493–502. Gyarmati, I. (1970). Non-equilibrium Thermodynamics...
energy flows reduce radiative surface cooling (net upward radiative energy flow). Latent heat transport and thermals provide non-radiative surface cooling...
example imagined by Planck. He was considering the internal thermal radiativeequilibrium of a thermodynamic system in a cavity initially devoid of substance...
considers a grey stratosphere in radiativeequilibrium. A grey stratosphere (or atmosphere) is an approach to modeling radiative transfer that does not take...
{k_{f}}{k_{b}}}\right)_{2}\times \cdots } Equilibrium chemistry Mechanical equilibrium Chemical equilibriumRadiativeequilibrium Atkins, P.W.; de Paula, J. (2006)...
colleague of Pictet, introduced the concept of radiativeequilibrium, wherein all objects both radiates and absorb heat. When an object is cooler than...
Mechanical equilibrium, the state in which the sum of the forces, and torque, on each particle of the system is zero Radiativeequilibrium, the state...
simplifications of the atmospheric radiative transfer on the basis of atmospheric radiative transfer codes, and cloud microphysics. Radiative parameterizations are...
reaction within the core region. The overlying atmosphere is in radiativeequilibrium. This is in contrast to the Sun, which has a radiation zone centered...
This is the biggest non-radiative cooling effect at the surface. It compensates for roughly 70% of the average net radiative warming at the surface. Second...
radiative equilibria. Systems can be in one kind of mutual equilibrium, while not in others. In thermodynamic equilibrium, all kinds of equilibrium hold...
used in single-use reentry capsules. Passive daytime radiative cooling Daytime passive radiative coolers use the extremely cold temperature of outer space...
radiative forcing will cause. The conceptual framework is similar to that applied to evaluating the influences of economic externalities. Radiative forcings...
for a "hollow space" or "cavity") is a cavity whose walls are in radiativeequilibrium with the radiant energy within the cavity. This idealized cavity...
233, JSTOR 6491, PMID 17747682 Eddington, A. S. (1916). "On the radiativeequilibrium of the stars". Monthly Notices of the Royal Astronomical Society...
that Kirchhoff's law of equality of radiative absorptivity and emissivity holds. In strict thermodynamic equilibrium, the radiation field is said to be...
surface recombination. These decay channels can be separated into radiative and non-radiative. The latter occurs when the excess energy is converted into heat...
space, i.e., the only way the planet cools itself. Radiative heating from absorbed sunlight, and radiative cooling to space via OLR power the heat engine...
233. JSTOR 6491. PMID 17747682. Eddington, A. S. (1916). "On the radiativeequilibrium of the stars". Monthly Notices of the Royal Astronomical Society...