Definition of radiative equilibrium in English:

radiative equilibrium

noun

Astronomy Meteorology

A state of equilibrium (as in a star or the atmosphere) in which the total flux of emitted energy is equal to the flux of that absorbed; a state of equilibrium in which radiation is the predominant energy transport mechanism.

Early 20th century; earliest use found in Arthur Eddington (1882–1944), theoretical physicist and astrophysicist.

noun

Astronomy Meteorology

A state of equilibrium (as in a star or the atmosphere) in which the total flux of emitted energy is equal to the flux of that absorbed; a state of equilibrium in which radiation is the predominant energy transport mechanism.

Early 20th century; earliest use found in Arthur Eddington (1882–1944), theoretical physicist and astrophysicist.

单词	radiative equilibrium
释义	Definition of radiative equilibrium in English: radiative equilibrium noun Astronomy Meteorology A state of equilibrium (as in a star or the atmosphere) in which the total flux of emitted energy is equal to the flux of that absorbed; a state of equilibrium in which radiation is the predominant energy transport mechanism. Origin Early 20th century; earliest use found in Arthur Eddington (1882–1944), theoretical physicist and astrophysicist. Definition of radiative equilibrium in US English: radiative equilibrium noun Astronomy Meteorology A state of equilibrium (as in a star or the atmosphere) in which the total flux of emitted energy is equal to the flux of that absorbed; a state of equilibrium in which radiation is the predominant energy transport mechanism. Origin Early 20th century; earliest use found in Arthur Eddington (1882–1944), theoretical physicist and astrophysicist.
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