Given an atmospheric profile of temperature, variable gas concentrations, cloud and surface properties CRTM calculates radiances and brightness temperatures.
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The temperature derived from the Planck function is referred to as the brightness temperature ( which see, for derivation ).
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For objects in nature, often called Gray Bodies, the actual temperature is only a fraction of the brightness temperature.
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In 1965, Antony Hewish and Samuel Okoye discovered " an unusual source of high radio brightness temperature in the Crab Nebula ".
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The brightness temperature can be used to calculate the spectral index of a body, in the case of non-thermal radiation.
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Where T b is the brightness temperature, e is the emissivity, and T is the temperature of the surface sea water.
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Observations of the planet's brightness temperature with the Spitzer Space Telescope suggest a possible thermochemical disequilibrium in the atmosphere of this exoplanet.
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When looking at the polarized components of the brightness temperature, the spread of the brightness temperature curves will be different depending on the component.
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When looking at the polarized components of the brightness temperature, the spread of the brightness temperature curves will be different depending on the component.
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Thanks to the relatively well known vertical profile of oxygen concentration, the brightness temperature signals can be directly used to derive the unknown temperature profile.
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