Brightness Temperature -- from Eric Weisstein's World of Physics

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Brightness Temperature

The brightness temperature of a body is defined according to

(1)

where is the specific intensity and is given by the Planck Law. In radio astronomy, the Rayleigh-Jeans law can be used to approximate the Planck Law, so

(2)

where has MKS units of , is the frequency, k is Boltzmann's constant, T is the physical temperature, and c is the speed of light.

Antenna Temperature, Brightness, Planck Intensity Density, Planck Law, Specific Intensity




References

Janssen, M. A. "An Introduction to teh Passive Microwave Remote Sensing of Atmospheres." Ch. 1 in Atmospheric Remote Sensing by Microwave Radiometry (Ed. M. A. Janssen). New York: Wiley, pp. 1-35, 1993.

Rybicki, G. and Lightman, A. P. Radiative Processes in Astrophysics. New York: Wiley-Interscience, pp. 25-26, 1979.

Thompson, A. R.; Moran, J. M.; and Swenson, G. W. Jr. Interferometry and Synthesis in Radio Astronomy. New York: Wiley, p. 8, 1986.



© 1996-2007 Eric W. Weisstein

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