Difference between revisions of "Hemispherical Emittance"
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Latest revision as of 23:37, 19 December 2008
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Hemispherical Emittance
h</sub>, Eh)
</dt>
The ratio of the emissive power of a specimen to that of a black body at
the same temperature, considering radiation emitted in all possible
directions.
</dd>
References
This article is based on NASA's Dictionary of Technical Terms for Aerospace Use
