Radiative equilibrium is the condition where the total thermal radiation leaving an object is equal to the total thermal radiation entering it. It is...

The planetary equilibrium temperature is a theoretical temperature that a planet would be if it were in radiative equilibrium, typically under the assumption...

solely radiative connection, no matter how far apart, or what partially obstructive, reflective, or refractive, obstacles lie in their path of radiative exchange...

radiative-dynamical equilibrium." Instantaneous radiative forcing: "if no change in stratospheric temperature is accounted for". Effective radiative forcing:...

radiative-convective equilibrium (RCE) is a concept for the radiative balance of the atmosphere. It describes the balance between the net radiative longwave...

energy flows reduce radiative surface cooling (net upward radiative energy flow). Latent heat transport and thermals provide non-radiative surface cooling...

scattering processes. The equation of radiative transfer describes these interactions mathematically. Equations of radiative transfer have application in a wide...

example imagined by Planck. He was considering the internal thermal radiative equilibrium of a thermodynamic system in a cavity initially devoid of substance...

considers a grey stratosphere in radiative equilibrium. A grey stratosphere (or atmosphere) is an approach to modeling radiative transfer that does not take...

in radiative equilibrium in a cavity at the temperature of the matter of the 'cell'. Then it strictly obeys Kirchhoff's law of equality of radiative emissivity...

incoming and outgoing energy fluxes are in balance, Earth is in radiative equilibrium and the climate system will be relatively stable. Global warming...

colleague of Pictet, introduced the concept of radiative equilibrium, wherein all objects both radiate and absorb heat. When an object is cooler than...

thermodynamic equilibrium are simultaneously in mutual thermal, mechanical, chemical, and radiative equilibria. Systems can be in one kind of mutual equilibrium, while...

space", "empty room", or "cavity") is a cavity whose walls are in radiative equilibrium with the radiant energy within the cavity. First proposed by Gustav...

concept of radiative equilibrium between convection inside the Sun and thermal radiation at the surface. He developed an equation for radiative transfer...

{k_{f}}{k_{b}}}\right)_{2}\times \cdots } Equilibrium chemistry Mechanical equilibrium Chemical equilibrium Radiative equilibrium Atkins, P.W.; de Paula, J. (2006)...

Mechanical equilibrium, the state in which the sum of the forces, and torque, on each particle of the system is zero Radiative equilibrium, the state...

reaction within the core region. The overlying atmosphere is in radiative equilibrium. This is in contrast to the Sun, which has a radiation zone centered...

Milne, E. A. (1928). "The effect of collisions on monochromatic radiative equilibrium" (PDF). Monthly Notices of the Royal Astronomical Society. 88 (6):...

simplifications of the atmospheric radiative transfer on the basis of atmospheric radiative transfer codes, and cloud microphysics. Radiative parametrizations are important...

233, JSTOR 6491, PMID 17747682 Eddington, A. S. (1916). "On the radiative equilibrium of the stars". Monthly Notices of the Royal Astronomical Society...

temperature Earth's Energy Imbalance, a measurable change in the planet's radiative equilibrium which quantifies its heating (or cooling) rate Global Warming (Pitbull...

surface recombination. These decay channels can be separated into radiative and non-radiative. The latter occurs when the excess energy is converted into heat...

used in single-use reentry capsules. Passive daytime radiative cooling Daytime passive radiative coolers use the extremely cold temperature of outer space...

long-term, the planet's thermal inertia is surmounted and a new radiative equilibrium is reached when all energy arriving on the planet is leaving again...

measure of how much temperature change a given amount of radiative forcing will cause. Radiative forcings are generally quantified as Watts per square meter...

wavelength-specific radiative emission and absorption by a material body in thermodynamic equilibrium, including radiative exchange equilibrium. It is a special...

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...

A radiative zone is a layer of a star's interior where energy is primarily transported toward the exterior by means of radiative diffusion and thermal...

the 1950s showed that the pre-main-sequence star can remain in radiative equilibrium throughout some period of its contraction to the main sequence....