2.1: Absorptance, and the Definition of a Black Body

Stellar Atmospheres · LibreTexts

0%

Contents

    Text

    Size
    100%
    Theme
    Typeface
    Line length
    Spacing

    From LibreTexts, under CC BY-NC 4.0, as the source states it; its equations are written in TeX, which the PDF shows typeset. This page at LibreTexts.

    2.1: Absorptance, and the Definition of a Black Body

    If a body is irradiated with radiation of wavelength \(\lambda\), and a fraction \(a(\lambda)\) of that radiation is absorbed, the remainder being either reflected or transmitted, \(a(\lambda)\) is called the absorptance at wavelength \(\lambda\). Note that \(\lambda\) is written in parentheses, to mean "at wavelength \(\lambda\)", not as a subscript, which would mean "per unit wavelength interval". The fractions of the radiation reflected and transmitted are, respectively, the reflectance and the transmittance. The sum of the absorptance, reflectance and transmittance is unity, unless you can think of anything else that might happen to the radiation.

    A body for which \(a(\lambda) = 1\) for all wavelengths is a black body.

    A body for which a has the same value for all wavelengths, but less than unity, is a grey body.

    (Caution: We may meet the word "absorbance" later. It is not the same as absorptance.)


    This page titled 2.1: Absorptance, and the Definition of a Black Body was last modified on Sat, 05 Mar 2022 17:39:28 GMT and is shared under a CC BY-NC 4.0 license and was authored, remixed, and/or curated by Jeremy Tatum via source content that was edited to the style and standards of the LibreTexts platform.